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Publications (116)183.1 Total impact
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ABSTRACT: Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC telescopes, revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20% of the gravitational radius of its central black hole. We suggest that the emission is associated with pulsar-like particle acceleration by the electric field across a magnetospheric gap at the base of the radio jet.Science (New York, N.Y.). 11/2014;
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ABSTRACT: Mrk 501 is one of the brightest blazars at TeV energies and has been extensively studied since its first VHE detection in 1996. Our goal is to characterize in detail the source gamma-ray emission, together with the radio-to-X-ray emission, during the non-flaring (low) activity, which is less often studied than the occasional flaring (high) activity. We organized a multiwavelength (MW) campaign on Mrk 501 between March and May 2008. This multi-instrument effort included the most sensitive VHE gamma-ray instruments in the northern hemisphere, namely the imaging atmospheric Cherenkov telescopes MAGIC and VERITAS, as well as Swift, RXTE, the F-GAMMA, GASP-WEBT, and other collaborations and instruments. Mrk 501 was found to be in a low state of activity during the campaign, with a VHE flux in the range of 10%-20% of the Crab nebula flux. Nevertheless, significant flux variations were detected with various instruments, with a trend of increasing variability with energy. The broadband spectral energy distribution during the two different emission states of the campaign can be adequately described within the homogeneous one-zone synchrotron self-Compton model, with the (slightly) higher state described by an increase in the electron number density. This agrees with previous studies of the broadband emission of this source during flaring and non-flaring states. We report for the first time a tentative X-ray-to-VHE correlation during a low VHE activity. Although marginally significant, this positive correlation between X-ray and VHE, which has been reported many times during flaring activity, suggests that the mechanisms that dominate the X-ray/VHE emission during non-flaring-activity are not substantially different from those that are responsible for the emission during flaring activity.10/2014;
Article: The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system[Show abstract] [Hide abstract]
ABSTRACT: The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50 GeV to more than 50 TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011-2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, dead time of the system, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system.09/2014;
Article: The major upgrade of the MAGIC telescopes, Part II: The achieved physics performance using the Crab Nebula observations[Show abstract] [Hide abstract]
ABSTRACT: MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La Palma, Spain. During summer 2011 and 2012 it underwent a series of upgrades, involving the exchange of the MAGIC-I camera and its trigger system, as well as the upgrade of the readout system of both telescopes. We use observations of the Crab Nebula taken at low and medium zenith angles to assess the key performance parameters of the MAGIC stereo system. For low zenith observations the trigger threshold of the MAGIC telescopes is about 50GeV. The integral sensitivity for sources with Crab Nebula-like spectrum above 220GeV is (0.66+/-0.03)% of Crab Nebula flux in 50 h of observations. The angular resolution at those energies is < 0.07 degree, while the energy resolution is 16%. We also re-evaluate the effect of the systematic uncertainty on the data taken with the MAGIC telescopes after the upgrade. We estimate that the systematic uncertainties can be divided in following components: < 15% in energy scale, 11-18% in flux normalization and +/-0.15 for the energy spectrum power-law slope.09/2014;
Article: First broadband characterization and redshift determination of the VHE blazar MAGIC J2001+439[Show abstract] [Hide abstract]
ABSTRACT: We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associated with the unknown-redshift blazar MG4 J200112+4352. Based on its gamma-ray spectral properties, it was identified as a potential very high energy (VHE; E > 100 GeV) gamma-ray emitter. The source was observed with MAGIC first in 2009 and later in 2010 within a multi-instrument observation campaign. The MAGIC observations yielded 14.8 hours of good quality stereoscopic data. The object was monitored at radio, optical and gamma-ray energies during the years 2010 and 2011. The source, named MAGIC J2001+439, is detected for the first time at VHE with MAGIC at a statistical significance of 6.3 {\sigma} (E > 70 GeV) during a 1.3-hour long observation on 2010 July 16. The multi-instrument observations show variability in all energy bands with the highest amplitude of variability in the X-ray and VHE bands. We also organized deep imaging optical observations with the Nordic Optical Telescope in 2013 to determine the source redshift. We determine for the first time the redshift of this BL Lac object through the measurement of its host galaxy during low blazar activity. Using the observational evidence that the luminosities of BL Lac host galaxies are confined to a relatively narrow range, we obtain z = 0.18 +/- 0.04. Additionally, we use the Fermi-LAT and MAGIC gamma-ray spectra to provide an independent redshift estimation, z = 0.17 +/- 0.10. Using the former (more accurate) redshift value, we adequately describe the broadband emission with a one-zone SSC model for different activity states and interpret the few-day timescale variability as produced by changes in the high-energy component of the electron energy distribution.09/2014;
Article: Probing the very-high-energy gamma-ray spectral curvature in the blazar PG 1553+113 with the MAGIC telescopes[Show abstract] [Hide abstract]
ABSTRACT: PG 1553+113 is a very-high-energy (VHE, E>100 GeV) gamma-ray emitter classified as a BL Lac object. Its redshift is constrained by intergalactic absorption lines in the range 0.4<z<0.58. The MAGIC telescopes have monitored the source's activity since 2005. In early 2012, PG 1553+113 was found in a high-state, and later, in April of the same year, the source reached the highest VHE flux state detected so far. Simultaneous observations carried out in X-rays during 2012 April show similar flaring behaviour. In contrast, the gamma-ray flux at E<100 GeV observed by Fermi-LAT is compatible with steady emission. In this paper, a detailed study of the flaring state is presented. The VHE spectrum shows clear curvature, being well fitted either by a power-law with an exponential cut-off or by a log-parabola. A simple power-law fit hypothesis for the observed shape of the PG 1553+113 VHE gamma-ray spectrum is rejected with a high significance (fit probability P=2.6 x 10^{-6}). For the first time a VHE spectral shape compatible with an exponential decay has been found in a distant blazar (z>0.2). The observed curvature is compatible with the extragalactic background light (EBL) imprint predicted by the current generation of EBL models assuming a redshift z~0.4. New constraints on the redshift were derived from the VHE spectrum. These constraints are compatible with previous limits and suggest that the source is most likely located around the optical lower limit, z=0.4. Finally, we find that the synchrotron self-Compton (SSC) model gives a satisfactory description of the observed multi-wavelength spectral energy distribution during the flare.08/2014;
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ABSTRACT: It has been claimed that the nova-like cataclysmic variable (CV) AE Aquarii (AE Aqr) is a very-high-energy (VHE, $E>$100 GeV) source both on observational and theoretical grounds. We aim to search for VHE gamma-ray emission from AE Aqr during different states of the source at several wavelengths to confirm or rule out previous claims of detection of gamma-ray emission from this object. We report on observations of AE Aqr performed by MAGIC. The source was observed during 12 hours as part of a multiwavelength campaign carried out between May and June 2012 covering the optical, X-ray, and gamma-ray ranges. Besides MAGIC, the other facilities involved were the KVA, Skinakas, and Vidojevica telescopes in the optical and Swift in X-rays. We calculated integral upper limits coincident with different states of the source in the optical. We computed upper limits to the pulsed emission limiting the signal region to 30% of the phaseogram and we also searched for pulsed emission at different frequencies applying the Rayleigh test. AE Aqr was not detected at VHE energies during the multiwavelength campaign. We establish integral upper limits at the 95\% confidence level for the steady emission assuming the differential flux proportional to a power-law function d\phi/dE \propto E^{-Gamma}, with a Crab-like photon spectral index of Gamma=2.6. The upper limit above 200 GeV is 6.4\times10^{-12} cm^{-2}s^{-1} and above 1 TeV is 7.4\times10^{-13} cm^{-2}s^{-1}. We obtained an upper limit for the pulsed emission of 2.6\times10^{-12} cm^{-2}s^{-1} for energies above 200 GeV. Applying the Rayleigh test for pulsed emission at different frequencies we did not find any significant signal. Our results indicate that AE Aqr is not a VHE gamma-ray emitter at the level of emission previously claimed. We have established the most constraining upper limits for the VHE gamma-ray emission of AE Aqr.07/2014;
Article: Measurement of the Crab Nebula spectrum over three decades in energy with the MAGIC telescopes[Show abstract] [Hide abstract]
ABSTRACT: The MAGIC stereoscopic system collected 69 hours of Crab Nebula data between October 2009 and April 2011. Analysis of this data sample using the latest improvements in the MAGIC stereoscopic software provided an unprecedented precision of spectral and night-by-night light curve determination at gamma rays. We derived a differential spectrum with a single instrument from 50 GeV up to almost 30 TeV with 5 bins per energy decade. In the low energies, MAGIC results, combined with the Fermi-LAT data, show a flat Inverse Compton peak. The Fermi-LAT and MAGIC spectral data were fit from 1 GeV to 30 TeV with a log-parabola, yielding a peak position at (53 $\pm$ 3) GeV with a $\chi^2_{red}$ = 82/27 (error probably underestimated due to the bad fit quality), showing that the log-parabola is not a good representation of the Inverse Compton peak of the Crab Nebula. There is no hint of the integral flux variability on daily scales at energies above 300 GeV if accounting for systematic uncertainties of the measurement. We consider two state-of-the-art theoretical models to describe the overall spectral energy distribution of the Crab Nebula. The constant B-field model cannot satisfactorily reproduce the VHE spectral measurements presented in this work, mostly troubled by the broadness of the observed IC peak. Most probably this implies that the assumption of the homogeneity of the magnetic field inside the nebula is incorrect. On the other hand, the time-dependent 1D spectral model provides a good fit of the new VHE results when considering a 80 {\mu}G magnetic field. However, it fails to match the data when including the morphology of the nebula at lower wavelengths.06/2014;
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ABSTRACT: The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-ray source candidates. It is energized by one of the highest spin-down power pulsars known (5% of Crab pulsar) and it has been compared to the Crab Nebula due to their morphological similarities. This object was previously observed by imaging atmospheric Cherenkov telescopes (Whipple, VERITAS and MAGIC), although not detected, with an upper limit of 2.4% Crab Unit (C.U.) at VHE. It was detected by Fermi-LAT with a spectrum extending beyond 100 GeV. We analyzed 81 hours of 3C 58 data taken with the MAGIC telescopes and we detected VHE gamma-ray emission with a significance of 5.7 sigma and an integral flux of 0.65% C.U. above 1 TeV. The differential energy spectrum between 400 GeV and 10 TeV is well described by a power-law function d\phi/dE=f_0(E/1TeV)^{-Gamma} with f_0=(2.0\pm0.4_{stat}\pm0.6_{sys})\times10^{-13}cm^{-2}s^{-1}TeV^{-1} and Gamma=2.4\pm0.2_{stat}\pm0.2_{sys}. The skymap is compatible with an unresolved source. We report the first significant detection of PWN 3C 58 at TeV energies. According to our results 3C 58 is the least luminous VHE gamma-ray PWN ever detected at VHE and the one with the lowest flux at VHE to date. We compare our results with the expectations of time-dependent models in which electrons up-scatter photon fields. The best representation favors a distance to the PWN of 2 kpc and Far Infrared (FIR) comparable to CMB photon fields. If we consider an unexpectedly high FIR density, the data can also be reproduced by models assuming a 3.2 kpc distance. A low magnetic field, far from equipartition, is required to explain the VHE data. Hadronic contribution from the hosting supernova remnant (SNR) requires unrealistic energy budget given the density of the medium, disfavoring cosmic ray acceleration in the SNR as origin of the VHE gamma-ray emission.05/2014;
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ABSTRACT: The discovery of rapidly variable Very High Energy (VHE; E > 100 GeV) γ-ray emission from 4C +21.35 (PKS 1222+216) by MAGIC on 2010 June 17, triggered by the high activity detected by the Fermi Large Area Telescope (LAT) in high energy (HE; E > 100 MeV) γ-rays, poses intriguing questions on the location of the γ-ray emitting region in this flat spectrum radio quasar (FSRQ). We present multifrequency data of 4C +21.35 collected from centimeter to VHE during 2010 to investigate the properties of this source and discuss a possible emission model. The first hint of detection at VHE was observed by MAGIC on 2010 May 3, soon after a γ-ray flare detected by Fermi-LAT that peaked on April 29. The same emission mechanism may therefore be responsible for both the HE and VHE emission during the 2010 flaring episodes. Two optical peaks were detected on 2010 April 20 and June 30, close in time but not simultaneous with the two γ-ray peaks, while no clear connection was observed between the X-ray and γ-ray emission. An increasing flux density was observed in radio and mm bands from the beginning of 2009, in accordance with the increasing γ-ray activity observed by Fermi-LAT, and peaking on 2011 January 27 in the mm regime (230 GHz). We model the spectral energy distributions (SEDs) of 4C +21.35 for the two periods of the VHE detection and a quiescent state, using a one-zone model with the emission coming from a very compact region outside the broad line region. The three SEDs can be fit with a combination of synchrotron self-Compton and external Compton emission of seed photons from a dust torus, changing only the electron distribution parameters between the epochs. The fit of the optical/UV part of the spectrum for 2010 April 29 seems to favor an inner disk radius of <6 gravitational radii, as one would expect from a prograde-rotating Kerr black hole.The Astrophysical Journal 04/2014; · 6.73 Impact Factor
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ABSTRACT: The Crab pulsar is the only astronomical pulsed source detected at very high energy (VHE, E>100GeV) gamma-rays. The emission mechanism of VHE pulsation is not yet fully understood, although several theoretical models have been proposed. In order to test the new models, we measured the light curve and the spectra of the Crab pulsar with high precision by means of deep observations. We analyzed 135 hours of selected MAGIC data taken between 2009 and 2013 in stereoscopic mode. In order to discuss the spectral shape in connection with lower energies, 4.6 years of {\it Fermi}-LAT data were also analyzed. The known two pulses per period were detected with a significance of $8.0~\sigma$ and $12.6~\sigma$. In addition, significant emission was found between the two pulses with $6.2~\sigma$. We discovered the bridge emission above 50 GeV between the two main pulses. This emission can not be explained with the existing theories. These data can be used for testing new theoretical models.02/2014;
Article: Search for Very-High-Energy Gamma Rays from the z = 0.896 Quasar 4C +55.17 with the MAGIC telescopes[Show abstract] [Hide abstract]
ABSTRACT: The bright gamma-ray quasar 4C +55.17 is a distant source ($z = 0.896$) with a hard spectrum at GeV energies as observed by the Large Area Telescope (LAT) on board the {{\it Fermi}} satellite. This source is identified as a good source candidate for very-high-energy (VHE; $> 30$ GeV) gamma rays. In general VHE gamma rays from distant sources provide an unique opportunity to study the extragalactic background light (EBL) and underlying astrophysics. The flux intensity of this source in the VHE range is investigated. Then, constraints on the EBL are derived from the attenuation of gamma-ray photons coming from the distant blazar. We searched for a gamma-ray signal from this object using the 35-hour observations taken by the MAGIC telescopes between November 2010 and January 2011. No significant VHE gamma-ray signal was detected. We computed the upper limits of the integrated gamma-ray flux at $95\%$ confidence level of $9.4 \times 10^{-12}$ cm$^{-2}$ s$^{-1}$ and $2.5 \times 10^{-12}$ cm$^{-2}$ s$^{-1}$ above $100$ GeV and $200$ GeV, respectively. The differential upper limits in four energy bins in the range from $80$ GeV to $500$ GeV are also derived. The upper limits are consistent with the attenuation predicted by low-flux EBL models on the assumption of a simple power-law spectrum extrapolated from LAT data.02/2014;
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ABSTRACT: HESS J1857+026 is an extended TeV gamma-ray source that was discovered by H.E.S.S. as part of its Galactic plane survey. Given its broadband spectral energy distribution and its spatial coincidence with the young energetic pulsar PSR J1856+024, the source has been put forward as a pulsar wind nebula (PWN) candidate. MAGIC has performed follow-up observations aimed at mapping the source down to energies approaching 100 GeV in order to better understand its complex morphology. HESS J1857+026 was observed by MAGIC in 2010, yielding 29 hours of good quality stereoscopic data that allowed us to map the source region in two separate ranges of energy. We present an energy spectrum of the region, which bridges the gap between the GeV emission measured by Fermi-LAT and the multi-TeV emission measured by H.E.S.S., together with a detailed analysis of its energy-dependent morphology. We couple these results with archival multi-wavelength data and outline evidence in favor of a two-source scenario, whereby one source is associated with a PWN while the other could be linked with a molecular cloud complex containing a HII region and a possible gas cavity.01/2014;
Article: MAGIC gamma-ray and multifrequency observations of flat spectrum radio quasar PKS 1510-089 in early 2012[Show abstract] [Hide abstract]
ABSTRACT: Among more than fifty blazars detected in very high energy (VHE, E>100GeV) gamma-rays, only three belong to the subclass of Flat Spectrum Radio Quasars (FSRQs). MAGIC observed FSRQ PKS 1510-089 in February-April 2012 during a high activity state in the high energy (HE, E>100 MeV) gamma-ray band observed by AGILE and Fermi. MAGIC observations result in the detection of a source with significance of 6.0 sigma. In agreement with the previous VHE observations of the source, we find no statistically significant variability during the MAGIC observations in daily, weekly or monthly time scales. The other two known VHE FSRQs have shown daily scale to sub-hour variability. We study the multifrequency behaviour of the source at the epoch of MAGIC observation, collecting quasi-simultaneous data at radio and optical (GASP-WEBT and F-Gamma collaborations, REM, Steward, Perkins, Liverpool, OVRO and VLBA telescopes), X-ray (Swift satellite) and HE gamma-ray frequencies. The gamma-ray SED combining AGILE, Fermi and MAGIC data joins smoothly and shows no hint of a break. The multifrequency light curves suggest a common origin for the millimeter radio and HE gamma-ray emission and the HE gamma-ray flaring starts when the new component is ejected from the 43GHz VLBA core. The quasi-simultaneous multifrequency SED is modelled with a one-zone inverse Compton model. We study two different origins of the seed photons for the inverse Compton scattering, namely the infra-red torus and a slow sheath surrounding the jet around the VLBA core. Both models fit the data well. However, the fast HE gamma-ray variability requires that within the modelled large emitting region, there must exist more compact regions. We suggest that these observed signatures would be most naturally explained by a turbulent plasma flowing at a relativistic speed down the jet and crossing a standing conical shock.01/2014;
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ABSTRACT: Aims. We present a study of the very high energy (VHE; E>100 GeV) gamma-ray emission of the blazar PKS 1424+240 observed with the MAGIC telescopes. The primary aim of this paper is the multiwavelength spectral characterization and modeling of this blazar, made particularly interesting by the recent discovery of a lower limit of its redshift of z>0.6, which makes it a promising candidate to be the most distant VHE source. Methods. The source has been observed with the MAGIC telescopes in VHE gamma rays for a total observation time of 33.6 h from 2009 to 2011. Results. The source was marginally detected in VHE gamma rays during 2009 and 2010 and later the detection was confirmed during an optical outburst in 2011. The combined significance of the stacked sample is 7.2 sigma. The differential spectra measured during the different campaigns can be described by steep power laws, with the indices ranging from 3.5+/-1.2 to 5.0+/-1.7. The MAGIC spectra corrected for the absorption due to the extragalactic background light connect rather smoothly, within systematic errors, with the mean spectrum in 2009-2011 observed at lower energies by the Fermi-LAT. A recent study including the combined VERITAS and Fermi-LAT contemporaneous observations from 2009 provided different results. In addition the absorption-corrected MAGIC spectrum is flat with no apparent turn down up to 400 GeV. The multiwavelength light curve shows increasing flux in radio and optical bands that could point to a common origin from the same region of the jet. Also the large separation between the two peaks of the constructed non-simultaneous spectral energy distribution requires an extremely high Doppler factor if a one zone synchrotron self-Compton model is applied. We find that a two-component synchrotron self-Compton model describes the spectral energy distribution of the source well, if the source is located at z~0.6.01/2014;
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ABSTRACT: We present the results of stereoscopic observations of the satellite galaxy Segue 1 with the MAGIC Telescopes, carried out between 2011 and 2013. With almost 160 hours of good-quality data, this is the deepest observational campaign on any dwarf galaxy performed so far in the very high energy range of the electromagnetic spectrum. We search this large data sample for signals of dark matter particles in the mass range between 100 GeV and 20 TeV. For this we use the full likelihood analysis method, which provides optimal sensitivity to characteristic gamma-ray spectral features, like those expected from dark matter annihilation or decay. In particular, we focus our search on gamma-rays produced from different final state Standard Model particles, annihilation with internal bremsstrahlung, monochromatic lines and box-shaped signals. Our results represent the most stringent constraints to the annihilation cross-section or decay lifetime obtained from observations of satellite galaxies, for masses above few hundred GeV. In particular, our strongest limit (95% confidence level) corresponds to a ~500 GeV dark matter particle annihilating into tau+tau-, and is of order ~ 1.2x10^{-24} cm^3 s^{-1} - a factor ~40 above the thermal value.Journal of Cosmology and Astroparticle Physics 12/2013; 2014(02):008. · 6.04 Impact Factor
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ABSTRACT: Indications of a GeV component in the emission from GRBs are known since the EGRET observations during the 1990's and they have been confirmed by the data of the Fermi satellite. These results have, however, shown that our understanding of GRB physics is still unsatisfactory. The new generation of Cherenkov observatories and in particular the MAGIC telescope, allow for the first time the possibility to extend the measurement of GRBs from several tens up to hundreds of GeV energy range. Both leptonic and hadronic processes have been suggested to explain the possible GeV/TeV counterpart of GRBs. Observations with ground-based telescopes of very high energy photons (E>30 GeV) from these sources are going to play a key role in discriminating among the different proposed emission mechanisms, which are barely distinguishable at lower energies. MAGIC telescope observations of the GRB 090102 (z=1.547) field and Fermi Large Area Telescope (LAT) data in the same time interval are analysed to derive upper limits of the GeV/TeV emission. We compare these results to the expected emissions evaluated for different processes in the framework of a relativistic blast wave model for the afterglow. Simultaneous upper limits with Fermi and a Cherenkov telescope have been derived for this GRB observation. The results we obtained are compatible with the expected emission although the difficulties in predicting the HE and VHE emission for the afterglow of this event makes it difficult to draw firmer conclusions. Nonetheless, MAGIC sensitivity in the energy range of overlap with space-based instruments (above about 40 GeV) is about one order of magnitude better with respect to Fermi. This makes evident the constraining power of ground-based observations and shows that the MAGIC telescope has reached the required performance to make possible GRB multiwavelength studies in the very high energy range.Monthly Notices of the Royal Astronomical Society 11/2013; 437(4). · 5.52 Impact Factor
Article: MAGIC observations and multifrequency properties of the Flat Spectrum Radio Quasar 3C 279 in 2011[Show abstract] [Hide abstract]
ABSTRACT: We study the multifrequency emission and spectral properties of the quasar 3C 279. We observed 3C 279 in very high energy (VHE, E>100GeV) gamma rays, with the MAGIC telescopes during 2011, for the first time in stereoscopic mode. We combine these measurements with observations at other energy bands: in high energy (HE, E>100MeV) gamma rays from Fermi-LAT, in X-rays from RXTE, in the optical from the KVA telescope and in the radio at 43GHz, 37GHz and 15GHz from the VLBA, Mets\"ahovi and OVRO radio telescopes and optical polarisation measurements from the KVA and Liverpool telescopes. During the MAGIC observations (February to April 2011) 3C 279 was in a low state in optical, X-ray and gamma rays. The MAGIC observations did not yield a significant detection. These upper limits are in agreement with the extrapolation of the HE gamma-ray spectrum, corrected for extragalactic background light absorption, from Fermi-LAT. The second part of the MAGIC observations in 2011 was triggered by a high activity state in the optical and gamma-ray bands. During the optical outburst the optical electric vector position angle rotatated of about 180 degrees. There was no simultaneous rotation of the 43GHz radio polarisation angle. No VHE gamma rays were detected by MAGIC, and the derived upper limits suggest the presence of a spectral break or curvature between the Fermi-LAT and MAGIC bands. The combined upper limits are the strongest derived to date for the source at VHE and below the level of the previously detected flux by a factor 2. Radiation models that include synchrotron and inverse Compton emissions match the optical to gamma-ray data, assuming an emission component inside the broad line region (BLR) responsible for the high-energy emission and one outside the BLR and the infrared torus causing optical and low-energy emission. We interpreted the optical polarisation with a bent trajectory model.11/2013;
Article: Contemporaneous observations of the radio galaxy NGC 1275 from radio to very high energy gamma-rays[Show abstract] [Hide abstract]
ABSTRACT: The radio galaxy NGC 1275, recently identified as a very high energy (VHE, >100 GeV) gamma-ray emitter by MAGIC, is one of the few non-blazar AGN detected in the VHE regime. In order to better understand the origin of the gamma-ray emission and locate it within the galaxy, we study contemporaneous multi-frequency observations of NGC 1275 and model the overall spectral energy distribution (SED). We analyze unpublished MAGIC observations carried out between Oct. 2009 and Feb. 2010, and the already published ones taken between Aug. 2010 and Feb. 2011. We study the multi-band variability and correlations analyzing data of Fermi-LAT (0.1 - 100 GeV), Chandra (X-ray), KVA (optical) and MOJAVE (radio) taken during the same period. Using custom Monte Carlo simulations corresponding to early MAGIC stereo data, we detect NGC 1275 also in the earlier MAGIC campaign. The flux level and energy spectra are similar to the results of the second campaign. The monthly light curve above 100 GeV shows a hint of variability at the 3.6 sigma level. In the Fermi-LAT band, both flux and spectral shape variabilities are reported. The optical light curve is also variable and shows a clear correlation with the gamma-ray flux above 100 MeV. In radio, three compact components are resolved in the innermost part of the jet. One of them shows a similar trend as the LAT and KVA light curves. The 0.1 - 650 GeV gamma-ray spectra measured simultaneously with MAGIC and LAT are well fit either by a log-parabola or by a power-law with a sub-exponential cutoff for both campaigns. A single-zone synchrotron-self-Compton model, with an electron spectrum following a power-law with an exponential cutoff, can explain the broadband SED and the multi-frequency behavior of the source. However, this model suggests an untypical low bulk Lorentz factor or a velocity alignment closer to the line of sight than the pc-scale radio jet.10/2013;
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ABSTRACT: Context. The galaxy IC 310 has recently been identified as a $\gamma$-ray emitter by the Fermi-LAT and at very high energies by the MAGIC telescopes. Originally classified as a head-tail radio galaxy, the nature of this object is subject of controversy because its nucleus shows blazar-like behavior. Aims. In order to understand the nature of IC 310 and the origin of the VHE emission we studied the spectral and flux variability of IC 310 from the X-ray band to the VHE regime. Methods. The daily light curve of IC 310 above 300 GeV has been measured with MAGIC from 2009 October to 2010 February. Contemporaneous Fermi-LAT data (2008-2011) in the 10-500 GeV energy range were also analyzed. In X-ray, archival observations from 2003 to 2007 with XMM-Newton, Chandra, and Swift-XRT in the 0.5-10 keV band were studied. Results. Several flares with similar amplitude can be seen in the MAGIC light curve. Day to day flux variability is clearly present. The photon index between 120 GeV and 8 TeV is measured to be $\Gamma=2.0$ during both low and high flux states. It does not show variability, whereas the flux at 1 TeV changes by a factor of 7. Fermi-LAT detected only eight $\gamma$ rays in the energy range 10 GeV-500 GeV in three years of observation. The measured photon index of $\Gamma=1.3\pm0.5$ in the Fermi-LAT range is very hard. The X-ray measurements show strong variability in both flux and photon index. The latter varied from 1.76 to 2.55. Conclusion. The rapid variability measured in $\gamma$ rays and X-rays confirms the blazar-like behavior of the source. The spectral behavior measured in both energy bands suggest IC 310 could be linked to extreme HBL objects. The apparent luminosity of IC 310 is a few orders of magnitude lower than other extreme HBLs however and, atypical for an HBL, it harbors a kiloparsec-scale radio structure. Thus, IC 310 could be a peculiar type of a HBL.05/2013;
Top Journals
Ciemat-Centro Investigaciones Energéticas, Medioambientales Y TecnológicasMadrid, Madrid, Spain
Max Planck Institute of PhysicsMünchen, Bavaria, Germany
National University of TechnologyCórdoba, Córdoba, Argentina
University of Wuerzburg
Würzburg, Bavaria, Germany
- Faculty of Physics and Astronomy
Iowa State University
Ames, IA, United States
- Department of Physics and Astronomy
St Patrick's CollegeLondinium, England, United Kingdom


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Statewide News Briefs - Jan. 2008
» A run on a state-managed investment pool for local governments caused the State Board of Administration to freeze the fund temporarily last month. Local governments had withdrawn close to $14 billion, about half of the funds from the pool, in two months. Investors became concerned over the fallout from mortgage-backed securities. About 6% of the state-run fund is invested in securities that have defaulted. Four days after closing, the state reopened the fund with limits on withdrawals. Pool manager Coleman Stipanovich resigned, and the state shifted management of the fund to BlackRock Inc.
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5 reasons we're thankful for Bella Thorne
My BF broke up with me and has ignored me ever since. Why?
Be a pro pet sitter!
7 (other) awesome dystopian books to read right now
Christmas crafts for the entire fam under $10
GL's Friends Gift Guide: Exactly what to get your besties for under $20
Mani roundup: Too-cute Thanksgiving nail ideas
Flu shots: myths uncovered
Which celeb should be at your dinner table this Thanksgiving?
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Everything to be an "It Girl"
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Teenage girl...and assassin nun? Meet Annith in Mortal Heart
Mortal Heart—the third and final chapter in the His Fair Assassin trilogy—follows a trio of teen girls trained in the dark arts of spying and murder. CLICK HERE to catch up on the first two books...and get a sneak peek at the gripping conclusion in Mortal Heart.
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Crowcon Detection Instruments Ltd
based in Milton Park, UNITED KINGDOM
Crowcon Detection Instruments develop, manufacture and market a complete range of portable and fixed gas detection products you can trust to protect people and plant against gas hazards. Established over 40 years the company has strong regional centres in North America, Singapore, The Netherlands and India, with a mature network of trained distributors covering almost ...
Telegan Gas Detection
based in Oxfordshire, UNITED KINGDOM
Telegan Gas Detection is a specialist in flue gas analysers and gas leak detection. Telegan gas monitoring leads the world in the development of portable emission monitoring, flue gas analysers and gas leak detection.
Gas Data Ltd
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Gas Data have 20 years of experience in designing and manufacturing an extensive range of portable and fixed instrumentation for a wide range of applications including Anaerobic Digestion and many others. The instruments are used in the control of landfill gas, biogas, contaminated land remediation, food storage, security, odour control, biofuel and many more. Our GFM ...
Matheson Tri-Gas, Inc.
based in Parsippany, NEW JERSEY (USA)
Matheson Gas Products and Tri-Gas, Inc merged to form Matheson Tri-Gas, Inc. on July 1, 1999. Our mission is to provide the best service and quality of products in the specialty gases and related equipment industry which will meet or exceed the requirements of both customers and future markets.
Gas Measurement Instruments Ltd - an Industrial Scientific Corporation Company
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GMI design and manufacture a wide range of gas detection products. Portable gas detectors, handheld personal monitors, and fixed systems for permanent installation. Gas detection for all industries.
Analytical Pixels Technology (APIX)
based in Grenoble, FRANCE
Analytical Pixels Technology (APIX) manufactures portable, powerful Gas Chromatographs for sample analysis in the field. Using the latest, cutting edge Nano technology, we are able to miniturize an entire gas analysis lab onto a chip, making Gas Analysis much more portable, less expensive, and easier to use. Analytical Pixels Technology (APIX) leads in manufacture and ...
Cerex Monitoring Solutions, LLC.
based in Atlanta, GEORGIA (US) (USA)
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Advance Field Systems, Inc.
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Advance Field Systems, Inc. is a y created by experts in physics, analytical chemistry and materials science to develop fast portable chromatograph instrumentation with speed and sensitivity previously unmatched in the marketplace. By leveraging proprietary innovations by incorporating a novel new detector and unique sampling system, the company was able to engineer a ...
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Price GIANT DOME THEATER ADMISSION (1 film + access to all eight exhibit galleries): Adults $15.75; Children/Seniors $12.75
Age Suitability All Ages
Rocky Mountain Express
Saturday, Jun 29, 2013 10:00a
IMAX® film Rocky Mountain Express propels audiences on a steam train journey through the breathtaking vistas of the Canadian Rockies and highlights the adventure of building a nearly impossible transcontinental railway. Spectacular IMAX aerial cinematography, archival photographs and maps, and the potent energy and rhythms of a live steam locomotive immerse audiences in this remarkable story form the age of steam. Visit www.rhfleet.org for showtimes.
Created by rhfleet
Location & Nearby Info
IMAX at the Reuben H. Fleet Science Center
1875 El Prado
Carmel Valley, CA 92101
1875 El Prado
Carmel Valley, CA 92101
Show nearby:
1.2 mi 2 Mamá Testa Taqueria
1.2 mi 3 Tre Porcellini Restaurant
1.4 mi 4 Cowboy Star
1.5 mi 6 California Crepes
1.6 mi 7 Cafe Sevilla
1.6 mi 8 Tabule Restaurant and Bar
2.0 mi 9 Parkhouse Eatery
2.2 mi 10 Savory Deli & Market
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Thu 2/26 7:30p
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Kukla's Korner Hockey
Look Around- Groin Pulls Everywhere
by Paul on 12/14/05 at 09:24 AM ET
Comments (0)
So what's the cause? Are players really not prepared to play this type of game? The answer is yes. After being off for an entire season and then coming back to a different game, players and coaches are finding that they are going to have to change. For the players, how they prepare, and for the coaches, how they train their players. "There's definitely a lot more skating," Forsberg said. "People are used to holding and grabbing and all that stuff where you couldn't skate before. "But it's probably a combination of that and guys being out that long. But there is definitely more skating up and down the ice and back and forth and the way the game is now you have to be ready to skate every time you're out there."read on
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Check out our Pie of the Day Pinterest board.
Learn new tips, tricks and techniques from the Test Kitchen experts. Save $5 with code ONLINE at checkout.
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Cut light-green strips of ribbon just long enough to wrap around and slightly inside the lid of a gift box. Secure the ends of the ribbon to the inside of he lid with a hot glue gun. Cover lid completely with light-green ribbons, then weave deeper green ribbons between the light-green ribbons to achieve a lattice effect. Glue ends in place.
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Jagmohan Dalmiya playing it safe on elections
As the IPL betting and spot fixing case inches closer to judgment day, the powers that be in the BCCI have turned their focus on East Zone that has the right to nominate the presidential candidate at
Rory McIlroy, Scott reignite duel ahead of Australian Open
World no. 1 Rory McIlroy returns to defend his Australian Open title this week with Adam Scott itching for revenge after last year's final hole anguish.
Liverpool, City's fate is uncertain in Champions League
In case both Manchester City and Liverpool succumb in their last league matches, questions will again be raised about the usefulness of the EPL
Chinese teen sends Advani packing at World snooker
On a day Chinese prodigy Yan Bingtao broke Indian hearts by sending out home hero Pankaj Advani 6-4 in the quarter-finals of the Seaways IBSF World Snooker Championships, Pakist-an's giant-killer Muha
Lewis Hamilton on top of world
Mercedes man clinches Abu Dhabi GP to become 4th British driver to win crown twice


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Bellator 101
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Bellator 101 Weigh-In Results: Warren-Kirk, Lightweight Competitors Cleared For Bouts
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Latest Full Contact Fighter Radio Features Bellator Lightweights Saad Awad and Will Brooks
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Bellator 101: Rob Sinclair Injured, Ricardo Tirloni to Compete in Lightweight Tourney
Cheick Kongo Booked to Fight Mark Godbeer in Bellator Debut
New Full Contact Fighter Radio Features Bellator's Nate Coy, WSOF'S Rick Glenn
Bellator 101 Card Finalized, Prelims Include Nate Moore and Marcin Held
Alessio, Davis and Clementi Among Bellator Season 9 Lightweight Tourney Competitors
UFC FN 57: Alexey Oliynyk and Matt Wiman Backstage Interviews
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Lion Fight 19 Highlights: Late Replacement Jo Nattawut Decisions Sean Kearney
GLORY 18 – Zack Mwekassa vs. Brian Collette (Full Video)
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Select () or exclude () categories to narrow your recipe search.
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1/6 Photos of Kabab (Kebabs or Middle Eastern Skewers)
Prep Time:
Cook Time:
10 mins
15 mins
Kababs are popular in the Middle East. These are often prepared during barbecues and eaten with pita bread and salads. Yield is approximate.
Serves: 6
Units: US | Metric
Serving Size: 1 (169 g)
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3 piece modular office furniture, ideal for reception area. Includes: 1 x Soft Chair with right arm rest 1 x Soft Chair with left arm rest 1 x square table with glass top, finished in the same material as the chairs. All in good
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Used school photocopier with manual
Work cabinet in excellent condition. Has a lot of space to put you equipment in and also space on the top to work on. Great for commercial and domestic use. Here are some more details of the product: • Ideal working height • Extremely high ca
Falcon G2112/2 Dominator Convection Oven NAT GAS In a good working condition Just came out of Sainsbury little usage Approximately 2years old COST BRAND NEW £8,484.00 2YEAS AGO CASH ON COLLECTION OR BANK TRANSFER ONLY NO PAYPAL IN THIS I
Piranha Corner Computer Desk with Lockable Filing Cabinet Brand new, still in original wrapping. Gutted as it is a great product but just too big for our room. Large sturdy corner computer desk with a generous working surface of Width 143.5cm
For sale is out 6 drawer plan chest we have located in our office at work in Harlow. It is a used unit but all drawers are working and it is in good condition. Can be split in to two sections so 3 drawers per section. Dimensions (w x d x h): 1345mm x
MINIMUM ORDER 100kg of a cream NOT AA QUALITY (DONT BE CONFUSED) In a Cream quality clothing you will NOT find ANY soiled, too worn, stained, ripped items, and also those with a strong smell. All is left is only item in good and new condition. L
FOR SALE: SHARP XE-A203 electronic till. Hardly used and in excellent, full working order. Comes complete with cash draw lock key, 2 x operator key & 2 x management keys, instruction manual and 6 till rolls. Buyer collects. Cash payment on
I have some office chairs. They are black, in leather, big and quite comfortable. They are modern. They provide generous backrest and great armrests. They cost 30 pounds each. If you are interested, please call on: 07448 718696 or on: 075 211 60 712.
Herman Miller Aeron chairs for Sale, Black with green mesh. please get in touch for details city used office furniture city office furniture
I have many big office desks. They are rectangular, wooden, brown, in a good condition. They are modern and practical with all the features you need. If you are interested, please call on: 07448 718696 or on: 075 211 60 712. Thank you.
Next "Roma" corner desk,plus this model has a free standing shelf unit that can be placed alongside or under desk.Price reduced for quick sale. Only 6 months old was £150 new.Buyer to collect
I have 10 of these office desks. They are nice wooden office desks in good condition. They are big, light browned. Each of them is supplied with 2 fixed drawer pedestals. If you are interested, please call me on: 07448 718696 or on: 075 211 60 712.
we have 4 filing cabinets for sale 2 are 3 drawer 2 are 4 drawer they are priced at £20 each though i will accept reasonable offers for them they are not currently used and are in storage collection from our business address


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I just bought this 7" on the Well charge label. It's not on Roots knotty roots database.
Is it a bootleg or a missprint label?
The Matrix # is Channel One 011 A and 011 B.
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How to make a stand-up deskBecause staring into a computer screen for too long has a certain effect on me—Think: Tranquilizer dart and clinical depressant—I'm what you'd call a stand-up desk fan. A stand-up desk truly does help me fight off the urge to go nighty-night at midday. And I also feel it's helping me do my part to keep [...]
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Obama's online townhall: What's really going on? Updated: Megalomania-palooza!
Scroll down for updates…
At 11:30am Eastern, President Obama will conduct an "online townhall" on the economy.
At this moment, the White House website reports that "92,889 people have submitted 104,079 questions and cast 3,608,538 votes."
In order to ask a question, you must register your name, e-mail, and zip code.
The DNC, fresh off its failed attempt to muster grass-roots support for the president's budget, has been aggressively advertising the townhall:
Friend –
I wanted to tell you about an exciting new feature just launched on the White House website called "Open for Questions."
Here's how it works — President Obama is inviting everyone to ask a question about the economy and to rate other questions up or down.
On Thursday morning, the President will conduct an online town hall on the economy and answer some of the most popular questions live.
Watch a video of the President explaining this new feature and be a part of it now.
"Open for Questions" is an opportunity to open up the White House to all Americans.
It's an experiment designed to encourage transparency and accountability by giving you a direct line to the White House.
This first round will deal with the economy. Americans deserve to know what their government is doing to get our economy back on track. But it's up to you to participate and make this experiment a success.
Join the discussion now:
Thanks, and remember to check back Thursday to watch the President answer some of your questions live.
Mitch Stewart
Organizing for America
Question: Who will have access to the e-mail registrant list?
The White House privacy policy does not bar sharing of the info with other parties:
Collection and disclosure of information: To ensure we are able to communicate effectively with visitors to our web site, we collect some information that can be directly associated with a specific person. We call this "Personal Information," and it includes, by way of illustration, names, addresses, telephone numbers and e-mail addresses.
We collect Personal Information from eligible individuals who affirmatively request to receive e-mail or other services from us. We collect this Personal Information in order to provide these eligible individuals with timely information via e-mail regarding events, resources and issues.
It is our general policy not to make Personal Information available to anyone other than our employees, staff, and agents.
Online Comments and Personal Information: We treat your name, city, state, and any comments you provide as public information. We may, for example, provide compilations of your comments to national leaders and other individuals participating in our efforts, without disclosing email addresses. We may also make comments along with your city and state available to the press and public online.
If it is the "general policy" not to share data gathered through the White House website, when and with whom do they make exceptions to the policy? And will the White House notify e-mail registrants when the "general policy" is breached? We saw Team Obama's rule-bending over Change.gov before.
If this online townhall looks like another permanent campaign registration tool to you, you're not alone.
11:45am Eastern. Obama wasted the first 15 minutes of the "townhall" re-reading his prompter script from the press briefing on Tuesday. The first "hardball" question? How will Obama restore education as a "right?"
12:13pm Eastern. Obama just asked if he could interrupt to make a point. He's the only one talking.
Obama's executive amnesty helps draw thousands of Lois Lerner's emails out of the shadows
November 21, 2014 07:04 PM by Doug Powers
With a rebuttal to President Obama's amnesty announcement, here's President Obama
November 20, 2014 08:25 PM by Doug Powers
Good luck with that: St. Louis mayor agrees to protest group's demands
November 19, 2014 07:59 AM by Doug Powers
White House: Do something about 'climate change' or prepare for a fiery death — or worse
November 18, 2014 07:24 PM by Doug Powers
Jonathan Gruber cashed in even more than previously thought; Update: And Obama JUST found out about all this
November 16, 2014 09:23 AM by Doug Powers
Categories: Barack Obama, Corruption, Democrats, Health care, Nancy Pelosi


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Post Election Reflections
Post Election Reflection: The Virginia Governors Race and the Coming Midterm and Presidential Elections
Keith A. Fournier
� Third Millennium, LLC
Catholic Online
Five qualifiers before I share my personal thoughts on the recent Virginia Gubernatorial race:
First, I write as a private citizen. I am not speaking for any organization or for my Church. Second, I write as a Virginian who lives in the Hampton Roads section of Southeastern Virginia. Third, I write as a �Reluctant Republican�, having never formally registered as a Republican when I moved to Virginia from Steubenville, Ohio in 1991 where I was still a registered Democrat. I do not fit the tired labels of �liberal�, �conservative� or any of their hybrids and have openly and repeatedly rejected them. Fourth, I write as one who is convinced that the current language of, and charged debate in, the political arena is one of many indications that a major change is needed. Fifth, I write as one who has been involved in policy and political action for thirty years, seeking always to inform my social, cultural, economic and political participation by the values I derive from my orthodox, Catholic Christian faith. I propose the principles and guidance found in Catholic Social teaching as the path to building a more just society. As one committed to building a culture of life and a civilization of love, I am pro-life (from conception till natural death), pro-marriage and family, pro-freedom (rightly understood as a �freedom from� as well as a �freedom for�), pro-poor and pro-peace.
Having said all that, I have waited to write these few thoughts in order to let the spin unfold concerning the reasons and the implications of this gubernatorial race in Virginia. It went exactly as I had expected. The �conservative� pundits on talk radio insisted it said nothing about the National climate or the implications for the upcoming mid-term and Presidential elections. Utter Nonsense! They had their talking points so aligned that you could actually turn from one of their radio programs to another throughout the course of the day and hear the same things being said, with a different vocal cadence! Similarly, the �liberal� pundits insisted it portended a major shift away from the Republican Party and to the Democratic Party. More Nonsense! Their talking points were also aligned like clockwork and their minions were out in legion, on their radio programs, and in particular, in their fifth column, the printed media. The spin, right and left, was so rehearsed it was almost comedic.
So, what, if anything, did this election actually tell us about where the voters of America are looking concerning the critical decisions that lie ahead? I say, it told us a lot�and that any candidate serious about being elected in either 2006 or 2008 need to study this race in order to learn about the changing landscape in the political arena. Here are just a few of my own thoughts.
It told us that Americans are neither �liberal� nor �conservative�, or any variation of these tired old labels, such as �neo- conservative�, �progressive��. Americans are tired of the charged rhetoric that has come to characterize recent political campaigns. In fact, the loser in this race ran, in my opinion, one of the worst political campaigns in modern history. He was not only negative but downright nasty. In his efforts to paint himself as a �conservative�, and his opponent as a �liberal�, he failed miserably in winning the hearts and minds of Virginians. He also ended up alienating many groups, including Catholics. His efforts to deride his Catholic opponents stand on capital punishment backfired. This is ironic, since his own stand against the �capital punishment� of children in the womb was more in keeping with the Catholic Church�s position on the unalienable right to life than his Catholic opponents unfaithful efforts to espouse the �I�m personally opposed but�� position that has been the errant siren song of some deluded Catholics concerning this fundamental human rights issue. The Catholic Church is absolutely and unequivocally clear about the right to life and this Democratic Catholic candidate was wrong in trying to hide behind a �personal v public� curtain.
So, we Virginians got our first Catholic Governor. As a Catholic, this is a source of pride and hope. However, we need to pray that our Governor- elect grows in his understanding of the teaching of the Catholic Church concerning the intrinsic evil of every procured abortion. It is the taking of innocent human life. We need to help him to understand the unity of life that the Christian faith demands. We need to help him come to recognize that children in the womb are, in the words of Mother Teresa, the �poorest of the poor�. As a former lay missionary, he has proven himself capable of not only hearing their cry but standing with the poor. Now, as ...
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accountant billing/systems jobs near Golden Valley, MN
Retirement Accountant
Alerus Financial- Arden Hills, MN
of retirement and recordkeeping systems and recordkeeping operational functions. ... Retirement Accountant https://rn22.ultipro.com..5 days ago from Alerus Financial
Hedge Fund Accountant
Wells Fargo US- Edina, MN
of related derivatives, and more. The Fund Accountant is responsible for managing the ... trade settlement operations, the role of systems supporting these functions, and the...13 days ago from eFinancial Careers
Cost Accountant, Job#COST102414
Nuaire- Plymouth, MN
and variety of complementary products and systems to serve the needs of the world's ... NuAire is currently seeking a Cost Accountant to perform all tasks necessary to...5 days ago from ZipRecruiter
Sr AccountantNEW
Hamon Deltak- Plymouth, MN
Accountant is the driver/owner of the monthly P&L close ... Accountant will be required to participate in/or complete various projects (i.e...3 days ago from ZipRecruiter
Accountant – I
Horizontal Integration- Minneapolis, MN
efficient for our clients. Job Description: Accountant – I Duration: 6 months 250 ... Preparation of monthly journals for billing, general ledger oversight and audit...9 days ago from ZipRecruiter
Accounts Receivable ClerkNEW
Robert Half International- Shoreview, MN
We are currently sourcing for a long term A/R accountant for a well known corporation in t ... Duties will include detailed customer billing, A/R aging report monitoring, back up to A/R...3 days ago from Global Compliance Jobs
Accounts Receivable Clerk
Accountemps- Saint Paul, MN
We are currently sourcing for a long term A/R accountant for a well known corporation in t ... Duties will include detailed customer billing, A/R aging report monitoring, back up to A/R...4 days ago from Accountemps
Accounts Receivable Associate
Integrated Healthcare Strategies- Minneapolis, MN
system, and mailing to clients. Perform pre-billing integrity checks and procedures to ... timesheet approval and data gathering for billing purposes. Provide client invoice...13 days ago from ZipRecruiter
Entry Level AccountantNEW
Accountemps- Minneapolis, MN
eivable account analysis journal entry preparation bank account reconciliation data entry project work reporting If you are an entry level accountant and looking to get your...2 days ago from Accountemps
Staff AccountantNEW
Cliftonlarsonallen- Minneapolis, MN
and accounting solutions. The staff accountant will process transactions, complete ... *Requisition Number:* 14-0384 *Title:* Staff Accountant *City:* Minneapolis *State:*...2 days ago from CliftonLarsonAllen, LLP
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Renaissance Learning
Renaissance Learning Jobs & Careers in Madison, WI
Inside Account Executive
Renaissance Learning, Inc. – Madison, WI
We are seeking inside sales professionals who are passionate about ensuring that their customers have the right solutions, dedicated to our mission… CareerBuilder
Sr. Business (Marketing) Analyst
Renaissance Learning, Inc. – Madison, WI
with supporting analysis. • Support Budget process by providing summary and… CareerBuilder
Programmer Analyst (VB.NET, SQL)
Renaissance Learning, Inc. – Madison, WI
Analysis, design and programming of solutions to meet end-user needs. Delivers quality systems and support to various business units using RLI… CareerBuilder
Renaissance Learning Reviews
"Great Company "
- Comp & Benefits
- Work/Life Balance
- Senior Management
- Culture & Values
- Career Opportunities
I worked at Renaissance Learning full-time (less than an year)Pros
Great market, great products for K-12 market.Cons
Could be a little more forward-thinking on mobile.RecommendsNeutral Outlook


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Botres Global
based in ITALY
Experts with unique technology in field of residue biorefinery, biogas and waste water treatment. Coverage of all fields, like waste pre-treatment, anaerobic digestion, waste water treatment, fertilizer production/composting, green chemistry, and bio-materials.
LimnoTec Abwasseranlagen GmbH
based in Hille, GERMANY
Waste water treatment; Waste water treatment plants; DIC-SBR-process; Dynamic simulation; Shuttering; Activated sludge tanks/settling tanks; Anaerobic tanks; Rainwater reservoirs.
DVO, Inc.
based in Chilton, WISCONSIN (USA)
DVO, Inc. as the U.S. leader in anaerobic digestion, DVO`s patented two-stage mixed plug-flow digesters process more farm waste than any other - with unparalled performance. Our systems greatly reduce the odor on farms, are cost-effective, operate automatically and require low maintenance. DVO. Inc. has been a leader in environmental engineering for over 22 years, ...
GEA Filtration
based in Hudson, WISCONSIN (USA)
GEA Filtration custom designs membrane filtration systems that best utilize the technologies of microfiltration, ultrafiltration, nanofiltration, or reverse osmosis for each customer`s specific application. GEA Filtration is a world leader in the design, engineering, production, installation, support, and testing of large filtration systems for the dairy, food and ...
Global Bioenergies SA
based in Evry Cedex, FRANCE
Global Bioenergies is one of the few companies worldwide, and the only one in Europe, that is developing a process to convert renewable resources into hydrocarbons through fermentation. The Company initially focused its efforts on the production of isobutene, one of the most important petrochemical building blocks that can be converted into fuels, plastics, organic glass ...
Stichting Platform Bio-Energie
based in Arnhem, NETHERLANDS
Stichting Platform Bio-Energie is the Netherlands Bio-energy Association, NL-BEA in short. It is the Dutch association that promotes the interests of all Dutch companies involved in the biomass for energy chain. Members of the association represent the entire chain.
Kent BioEnergy Corporation
based in Temecula, CALIFORNIA (USA)
Kent BioEnergy employs commercially viable microalgae-based technologies for water pollution remediation, CO2 capture, landfill management, and the production of livestock feed additives, fertilizer, and biomass derived energy. Today, Kent BioEnergy has emerged as an industry leader in the development of advanced concepts for culturing and harvesting microalgae - ...
Lipten Company
based in Wixom, MICHIGAN (USA)
The Lipten Company is an Engineering, Procurement and Construction firm (EPC) that specializes in Central Energy Plant (CEP) General Contracting. We provide Steam generation, Power generation, Control Systems, Chilled Water Systems, and Water treatment systems. Lipten systems are custom designed to match the unique requirements of each of our clients for both new ...
Ennix Incorporated
based in Paso Robles, CALIFORNIA (USA)
Ennix has provided biosolids reduction and energy management with turnkey service programs to wastewater treatment industries since 1995. Wastewater treatment plants lower digester aeration requirements and improve sludge reduction using Ennix. Ennix is the first company to combine proprietary biochemical products and patented application systems with a `hands on` service ...
Zhengzhou Allance Machinry
based in Zhengzhou, CHINA
We have always been improving the design of our machinery to be and keep the leading position of the world market. High quality, reliability and speciality are our strong points.Your satisfaction is our permanent pursue! All the successful cases have witnessed a competitive and reliable manufacturer!


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Singular focus: Beat IUTalk about it in Knucklehead CentralSean RobinsonDavid HedelinJ.J. It was lingering for Coach Darrell Hazell - he didn't sleep much Saturday night - and so he assumed it was weighing on his players and coaches as well.So Hazell made sure to ... Austin American Statesman, 3 hours ago
187 images for singularity
Ferguson joins the sad battlefields of U.S. race tension
Special to The Globe and Mail David Shribman The singular tragedy of Ferguson, Missouri, in 2014, is that it is a story of plural tragedies. The tragedy that Michael Brown, an unarmed black teenager, was shot at all. The tragedy that his body, ...Globe and Mail, 4 hours ago
Bookmarked: Marianne Faithful's Friends Documented in 'A Life on Record'
For the past 50 years, Marianne Faithfull has been one of the music world's most singular characters: a Swinging London teen icon and mid-'60s girlfriend of Mick Jagger, a notorious heroin addict who revived her career in 1979 with the landmark ...Billboard, 2 days ago
Ariel Pink plugs into 'Pom Pom' buzz in his own singular style
Ariel Pink was craving a cigarette. It was the first thing he asked for one recent morning when he arrived at my place to talk about his new album, "Pom Pom." I didn't have one, so a representative from his record label, 4AD, was dispatched to ...Los Angeles Times, 4 days ago
This Week: A Singular Look at Stephen Hawking
In Theaters: A heartfelt look at the burden of genius. At Home: Rob Reiner's latest. Plus: The first true horror movie looks better than ever. Click here to view the embedded video. The Theory of Everything The life of a monumental ...AARP Bulletin Today, 5 days ago
The Rate of Innovation - Singularity Breakthroughs
He said, the ever accelerating progress of technology … gives the appearance of approaching some essential singularity in the history of the race beyond which human affairs, as we know them, could not continue. He called the Singularity the moment ...Austin American Statesman, 1 week ago
Fireflies review Spare yourself the stereotypes and cliches this week
The wellmeaning plot of Fireflies is totally wasted for a singular lack of imagination and the overdependence on stereotypes Skip this one unless you are looking for a depressing movie that only confirms to all norms of cliches in the name of an Indie film ...Hindustan Times, 3 weeks ago
Like! Stephen Hawking joins Facebook
Famed physicist Stephen Hawking, best known for his work on gravitational singularities and black hole radiation, has joined the popular social networking website Facebook. "I have always wondered what makes the universe exist. Time and space may forever be a mystery, but that has not stopped my pursuit," the 72-year-old astrophysicist wrote in his first post on Facebook. "Our connections to one another have grown infinitely and now that I have the chance, I'm eager to share this journey ...Rediff.com, 1 month ago Stephen Hawking Finally on Facebook Outlook, 1 month ago You can now follow Stephen Hawking on Facebook! Business Standard, 1 month ago
Singular horsepower
Apple's new, new things overshadowed by old thing Robert Cyran October 21, 2014 Last Updated at 21:32 IST Apple's new, new things have been overshadowed by an old thing. The drumbeat for innovation banged on for years till watch and payments technology ...Business Standard, 1 month ago
Birthday Special: Bollywood's Queen of Glamour, Rekha
Celebrating the glamorous Rekha. If there is one actress who singularly embodies Bollywood's charisma, enigma, glamour and giddy stardom, it is Rekha. Ever so sparkling, stunning and sophisticated, the actress didn't start out on an impressive note. Far from it, she was ridiculed for her chubby, gawky demeanour even though her debut Saawan Bhadon was a box office success. The teenager took the criticism in her stride and began to work on her appearance and style till the camera ...Rediff.com, 1 month ago
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on your WebpageAdd Widget >Get your members hooked!


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Mix of jill-off and jack-off, when a she male masturbates.
hey look it wants to jilack-off! EWWWW
by jjoff November 13, 2007
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Do you love Animal Crossing but hate all the communicating, working, running errands, and maintaining the town bits? Also, is it too much of a game for you? Deco Tendances (Deco Trends) is perfect for you: it focuses entirely on home decoration.
The program is designed to help with principles of interior design, featuring 24 tips in six major categories, including painting and wallpapering, window decoration, and complementing colors. Each tip is accompanied by multiple photos, and a color wheel is included as well. In addition, just because, there are four minigames.
The immediate reaction to something like this is to dismiss it as shovelware and get angry about how it's destroying the industry, and maybe that's accurate (the first part). But we also see somebody doing something new on the DS, that may be helpful to someone. And you still don't have to buy it. Besides, as we suggested above, interior decoration is the heart of one of Nintendo's most beloved franchises.
Featured Stories
Happy birthday, Nintendo DS
Posted on Nov 28th 2014 5:00PM
Super Joystiq Podcast 123: Persona Q, Tales from the Borderlands, Escape Dead Island
Posted on Nov 28th 2014 1:00PM
Joystiq Presents: A Zelda Story
Posted on Nov 28th 2014 9:00AM


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Milk production is on the rise and that trend is expected to continue into 2015. And milk prices have started to falter and that trend also looks to continue in 2015. So what are producer to do to protect their margins? A market analyst with Stewart Peterson shares his thoughts.
Some 40 students from Edison Middle School spent a day visiting all the stops that are necessary to building a pizza. The students visited an operation where wheat is produced, then visited a dairy farm before learning how to plant tomato seeds and ultimately preparing their own personal pizza.
With agriculture being such a capital intensive industry interest rates are always a focal point and at this years version of trade talk in Kansas City. Farm Credit shared the results of a poll of their CFO's on what they though may happen to interest rates in 2015.
With the Republicans now having control of both the senate and the house there will be changes in committee leadership including the two Ag committees. Who is expected to hold those positions and what issues may they be addressing in 2015. A lobbyist from AFBF shared his insights.
DMI and the National Dairy Board have had quite a bit of success forming partnerships with companies to increase dairy product consumption, especially in the cheese category. Now they are hoping to accomplish more positive results in the fluid milk sales through new partnerships formed with 7 companies.
With planting starting late, and now the harvest being challenged by far from ideal weather, No one was really expecting any exceptional yields this year. That is why it's been a pleasant surprise to hear of some 200 bushel plus yields and the news that a Seymour area farmers has set a new yield record for Outagamie County.
Despite efforts by area growers to take advantage of every weather window they get, the harvest pace is still lagging behind the norm. And while harvesting corn for silage went past Halloween, the grain harvest is projected to go past Thanksgiving as well.
With more and more agronomists and soil specialist encouraging producers to use more cover crops. the agronomists from the Marshfield experimental farm was asked to share some of his field results on various cover crop options during the NWTC Fall Field Days.
With farmers playing catch-up all year and concerns over compaction rising some producers are thinking twice about their fall tillage. Also during NWTC's fall field day a big focus was on the benefits on good surface and core soil treatment, and the impact tillage has.
During the annual convention of the National Milk Producers Federation CEO Jim Mulhern stressed priorities that the industry needs to address now. Right near the top of the list was the F.A.R.M Program, an effort that National Milk has made mandatory for its members to be a part of to show that animal care is a priority in producing milk and dairy products.


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20 December, 2011@9:11 pm
1 comments
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Asher Roth – "Pabst & Jazz" (Mixtape)
Nice! I'll definitely be downloading when I get home tonight and bumpin' this!
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