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arXiv:astro-ph/9305025v1 19 May 1993
VESA T. JUNKKARINEN,3and ROSS D. COHEN3
To appear in the Astronomical Journal, August, 1993
1Based on observations obtained at Lick Observatory, University of California.
2Dept. Physics, University of California, San Diego (firstname.lastname@example.com).
3Center for Astrophysics and Space Sciences, 0111, University of California, San Diego, La Jolla, CA
4Department of Astronomy, Columbia University, New York.
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We present Lick Observatory slit spectra of 38 objects which were claimed to have pronounced ultraviolet
excess and emission lines. Zhan & Chen selected these objects by eye from a UK Schmidt telescope IIIaJ
objective prism plate of a field at 0h0.0◦(l ≃ 98◦, b ≃ −60◦). We concentrated on mJ ≃ 18 –19 objects
which Zhan & Chen thought were most likely to be QSOs at redshift zem≥ 2.8.
Most of our spectra have FWHM spectral resolutions of about 4˚ A, and relatively high S/N of about
10 – 50, although some have FWHM ≃ 15˚ A or lower S/N. We find eleven QSOs, four galaxies at z ≃ 0.1,
twenty-two stars and one unidentified object with a low S/N spectrum.
The ZC lists are found to contain many QSOs at low z but few at high z, as would be expected. Of
eleven objects which ZC suggested were QSOs with zprism≤ 2.8, eight (73%) are QSOs. But only three of
twenty-five candidates with zprism≥ 2.8 are QSOs, and only two (8%) of these are at z ≥ 2.8. Unfortunately
the ZC prism redshifts are often incorrect: only five of the eleven QSOs are at redshifts similar to zprism.
Six of the QSOs show absorption systems, including Q0000+027A with a relatively strong associated
C IV absorption system, and Q0008+008 (V≃ 18.9) with a damped Lyα system with an H I column density
of 1021cm−2.
The stars include a wide variety of spectral types. There is one new DA4 white dwarf at 170 pc, one
sdB at 14 kpc, and three M stars. The rest are of types F, G and K. We have measured the equivalent
widths of the Ca II K line, the G-band and the Balmer lines in ten stars with the best spectra, and we derive
metallicities. Seven of them are in the range −2.5 ≤ [Fe/H] ≤ −1.7, while the others are less metal poor. If
the stars are dwarfs, then they are at distances of 1 to 7 kpc, but if they are giants, typical distances will be
about 10 kpc.
Subject Headings: quasars: general – galaxies: distances and redshifts – stars: fundamental parameters –
white dwarfs – surveys
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Zhan & Chen (1987a,b, 1989a,b, hereafter ZC1, ZC2, ZC3 and ZC4) presented lists of several hundred
QSO candidates, which they selected by eye from a single UK Schmidt telescope IIIaJ objective prism plate.
The candidates were chosen because they had emission lines and UV excess in the range 3200–5400˚ A, and
each was assigned a reliability index, Q = Q1+Q2, where Q1was 1, 2 or 3 for increasing strength of emission
lines, and Q2was similarly valued for increasing strength of UV excess.
We have obtained slit spectra of 38 of these QSO candidates with the Lick Observatory 3 m telescope,
on three separate occasions, during unrelated projects. Two of the objects have Q = 6, thirty-four have
Q = 5 and the remaining two, with Q = 4, are the least likely to be QSOs. Since Q ≥ 4 for all thirty-eight
objects, all should have both emission lines and UV excess.
Table 1 is a journal of our observations, with the instrumental setup (§2 below), wavelength range and
integration time. We also give the reference to the Zhan & Chen paper which contains the object coordinates,
magnitude and finding chart. Note that these charts have East to the right, and that the English translation
of ZC3 lacks charts, while for the other papers the charts are often better in the translation.
Our spectra were taken in support of three different observing programs, at three different times, and
with three different instrumental setups, although in all cases we used a Cassegrain spectrograph with the
Shane 3-m telescope at Lick Observatory.
2.1 Setup A: Ten z ≃ 3 Objects
These targets were selected as bright QSO candidates with zprism≃ 3. They were selected and observed
by VTJ and RDC.
The UV Schmidt camera was used on the Cassegrain spectrograph (Miller & Stone 1987) with a 300
g/mm grating blazed at 4230˚ A in first order. A thinned TI 800×800 CCD with 15 µ pixels, and 7 e−
readout noise was used, giving 3.9˚ A per pixel across 3100˚ A. All observations were made on October 4,
1988, when the sky was clear and the seeing was about 1 arcsecond. For the ten program objects we used a
wide 2.88 arcsecond slit, giving a FWHM resolution of 3.5 pixels, which is 14˚ A, but for the flux standard
star we used a 7.9 arcsecond slit. The slit was not rotated to the parallactic angle, but it was rotated to
PA = 248◦to simultaneously record 0003+011A & B, and to PA = 92◦for 0011−002A & B. Hour angles
ranged from 2 hours 30 minutes East to 3 hours 10 min West. All exposures were 600 seconds, and the
spectra were reduced in the usual way.
2.2 Setup B: Eleven Intermediate z Objects with Close Neighbours
These eleven QSO candidates were observed on August 24 or 27, 1990 by DT and FXM to search for
Mg II absorption systems which might show large scale (≃ 100 h−1Mpc) correlations in three dimensions.
This program was motivated by the finding of Tytler et al. (1987) that a few QSOs each had more Mg II
systems than were expected if they were all intervening, a two sigma result which has since been refuted by
much larger samples which do not show any sign of such correlations (Sargent et al. 1988; Steidel & Sargent
1992, Tytler, Sandoval & Fan 1993 §2.4). The QSO candidates which we observed were chosen because
they had one or more neighbours within about 1◦. Here we present our observations of only the ZC QSO
candidates, two of which were also observed by VTJ and RDC with setup A. Other QSOs observed in this
program will be discussed elsewhere.
Spectra were obtained with the Cassegrain spectrograph using a 600 g/mm grism, blazed at 4840˚ A in
first order (Miller and Stone 1987). We used a thinned TI 800×800 CCD with 15 µ pixels, and 7 e−readout
noise, giving 3.43˚ A per pixel from 4312 to 7059˚ A. The wavelength range was chosen to maximize the chance
of detecting redshifted Mg II absorption line systems, and it unfortunately misses blue wavelengths which
are most useful for stellar spectral classification. A 2.09 arcsec slit was used giving a FWHM resolution of
2.5 pixels, which is 8.6˚ A. The slit was not rotated to the parallactic angle, but the spectra were reduced in
the usual way.
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2.3 Setup C: Nineteen High z Objects
Nineteen QSOs were observed by DT in November 1992 with the superb new Kast double spectrograph,
which records blue and red spectra simultaneously. We used a dichroic with a nominal wavelength of 5500˚ A.
Light with wavelengths to the blue of this were dispersed with a 600 g/mm grism blazed at 4310˚ A, while
the red light was dispersed by a 600 g/mm reflection grating blazed at 7500˚ A. A thinned Reticon 1200×400
CCD was used in each of the blue and red cameras. In the blue we recorded from 3320 to 5485˚ A with
1.81˚ A per pixel, and a two pixel FWHM of 3.6˚ A, and in the red from 5530 to 8270˚ A with 2.34˚ A per pixel
and a two pixel FWHM of 4.7˚ A. A 1.5 arcsec slit was used, and was rotated to the appropriate parallactic
angle. The sky was clear, the seeing about 1.5 arcseconds, and the spectra were reduced in the usual manner.
We first discuss various problems with the spectra, then slit magnitude and color estimates.
3.1 The Spectra
The spectra shown in Figure 1 are grouped by setup (A, then B, then C) to make spectral features easier
to identify. The flux is fν, in units of micro-Jansky, and all wavelengths given in this paper are vacuum,
but they are not heliocentric. Wavelength scales should be accurate to about one pixel or better. A one
sigma error trace is shown beneath the spectra from setups B and C. Peaks in the error correspond to sky
emission lines. Note that poorly subtracted sky emission lines can appear as emission and/or absorption
in the spectra. In setup B there is frequently a bogus absorption at the extreme blue end of the spectrum
(4311˚ A), a bogus emission feature near 4325˚ A, and a second bogus absorption near 4370˚ A. The former
two arise from poor flux calibration, while the third is bad sky subtraction.
For setups A we did not attempt to correct for atmospheric absorption, hence the B band (6867˚ A) is
visible. For setups B and C we did use early type star spectra to attempt to remove the B band, the A band
(7600˚ A), and OH absorption at 7160–7340˚ A but with varying success.
The spectra have been corrected for atmospheric extinction, but not for interstellar extinction (b ≃
−60◦). Table 2 is a summary of our results.
3.2 Slit Magnitudes
Magnitudes listed by ZC were obtained from image sizes on a direct Schmidt plate, using the King et
al. (1981) calibration of the dependence of BJ magnitude on image size. ZC5 noted that these magnitudes
may be too bright by 0.5 – 1.0 mag. because they found most objects at ≃ 18.5, a whole magnitude brighter
than the peak of the otherwise similar survey by Savage et al. (1984). However H¨ ortnagl, Kimeswenger
& Weinberger (1992) have shown that King et al. measured larger image diameters at a given mj, which
suggests that the ZC magnitudes may actually be too faint, rather than too bright, for mj ≥ 18. We can
not determine which is correct because we do not know how ZC measured image sizes.
To try to reduce this uncertainty, we have estimated magnitudes from our slit spectra. These magnitudes
are highly uncertain because we used narrow slits. A broad band flux F is defined as
, (1)
where T(λ) is the band transmission (Kitchin, C.R. 1984), f(λ) is the flux per unit wavelength, and λmin
is ideally −∞, but in practice was the minimum wavelength of the spectrum.
an estimate of the flux in the dichroic filter gap, which was only 20˚ A. We obtained magnitudes from
U = −2.5log10FU+ KU, and similarly for B and V, where the constants KU, KB and KV were obtained
from the standard star spectra.
Our slit magnitudes are listed in Table 3. They have automatically been corrected for atmospheric
extinction by the usual flux calibration process, which converts from recorded photoelectrons to flux above
the atmosphere, as a function of wavelength. Galactic reddening E(B−V) values from Burstein & Heiles
For setup C we added
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(1982) are 0.01, 0.02, or 0.03 for the targets. The colors (B−V)0listed in Table 3 have been corrected for
these reddening values, but we have not corrected the individual magnitudes because their zero point errors
are much larger than the corrections of AV≃ 0.03 − 0.09.
We have checked our magnitudes in five ways. First, we calculated a magnitude from each of our thirteen
standard star spectra. We obtained standard deviations of s = 0.17 magnitudes for the V magnitudes and
s = 0.21 for the B magnitudes, which we regard as lower bounds on the external errors of our other magnitude
Second, two objects were observed twice, and in both cases the magnitudes were 0.7 – 1.0 fainter in
setup A, because a wider slit was used for the flux standard than for the program objects, although the
(B−V) colors differ by much less (0.02 and 0.14).
Third, when we compare our slit (B−V) colors with those estimated from the strength of the Balmer
lines in §3.4 below, we find excellent agreement which suggests that our slit (B−V) colors from setup C (the
only ones to have the silt aligned to the parallactic angle) have a 1σ error of under 0.04 mag.
Fourth, in Figure 2 we show the difference between our slit B magnitudes and the ZC image size BJ
magnitudes. Ours are on average 1.4 magnitudes fainter. ZC5 noted that their magnitudes were probably
too bright, but they guessed by only 0.5 – 1.0 magnitudes, which suggests that some of our magnitudes may
be too faint. We do not see any systematic differences between our three setups.
Fifth, four of the QSOs (0004-005B, 0006+020B, 0006+025 and 0010-002B) have been found indepen-
dently by Foltz et al. (1989). Their BJmagnitudes, which we list in §6, are brighter than ours by 0.3, 0.54,
1.19 and 1.57 magnitudes respectively, where the first three are from setup B, and the last one is from setup
These tests suggest that our colors, but not necessarily the individual magnitudes, from setup C are
good. Both the magnitudes and colors from setups A and B setups are also suspect because the slit was
narrow (1.5 to 2.88 arcsec), it was not rotated to the parallactic angle, and the TV camera guides on the
red, so we expect that the B and especially the U magnitudes will be systematically too faint, and the V
magnitudes should be the least bad. In addition there are several reasons why we expect our magnitudes
for the program objects to be systematically too faint. The standard stars were observed for much shorter
times than the faint targets, they should be better centered on the slit, and better focused, and for setup A
a wider slit was used for the standard stars than for the program objects.
Papers by Gunn & Stryker (1983) and Jacoby, Hunter & Christian (1984) were consulted to obtain
rough stellar classifications. Berg et al. (1992) present a simple classification scheme which they used on
their 6˚ A FWHM optical spectra of QSO candidates. Beers et al. (1992a) present digital spectra covering
3700 – 4500˚ A at 0.7 to 1.2˚ A FWHM for various hot halo stars (A, DA, sdO, sdB, Horizontal Branch =
HB), together with classification criteria, while Beers, Preston & Shectman (1992b, hereafter BPS2) present
spectra of cooler halo F and G stars of various metallicities.
Greenstein (1980) discusses the difficulty of distinguishing white dwarfs (WDs) from hot halo (subdwarfs
sdO or sdB, hot HB) stars. The separation is hardest for the hottest stars because the physical differences
in temperature and gravity are also small, so that DAwk (weak Balmer lines) and sharp lined DAs can be
confused with sdBs. But the distinction is easy below 12,000 K because the WDs then have stronger Balmer
lines. Greenstein (1980) shows that any star with W(Hγ) ≥ 15˚ A must be a DA, but as W(Hγ) drops from
15 to 5˚ A, one has either DA stars of increasing T, or stars from the sequence HBA (HB type A), HBB, sdB
and sdO, which is one of both increasing T and gravity. For the hot stars we searched for but did not find
any He I 4026, 4388, and 4471, or He II 4686.
Our spectral classifications are given in Table 2. For the stars we list the spectral type implied by the
spectral features, and then, in parentheses, that which would correspond to the (B−V) if the star had solar
metallicity. Most of the stars actually have significantly lower metallicities, so their (B−V) colors are from
0.1 to 0.3 magnitudes bluer (e.g. Beers et al. 1990; hereafter BPSK) than those of solar abundance stars
with the same MV. This deblanketing effect accounts for why the spectra type deduced from the colors are
hotter than those from the spectral features. Notes on the classification of individual objects are given in §6

subset: commoncrawl


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KAFC is providing Free Friday soccer!
Posted: Wednesday October 7th, 2015 Expires: 12/1/2015
It's BACK!
KAFC is providing Free Friday soccer.
Take advantage of this great offering of a supervised soccer pick up session for all local players on the Kitsap & Olympic Peninsulas.
It's not that structured. (But it is FUN!)
They run a quick warm up then get into games and play.
Players can NEVER get enough touches, and this kind of organized pick up soccer can only benefit all the clubs in our community.
Contact KAFC, http://www.kitsapalliancefc.com or for more details follow this link
Say it carefully, quickly and clearly: Getting your players' attention
Posted: Tuesday October 6th, 2015 Expires: 12/15/2015
It can be a challenge to get a rambunctious group of young players to pay attention for even a brief time. And with the fall season underway, we thought it'd be a good time to revisit advice from teacher and coach trainer Doug Lemov that first appeared in the Youth Soccer Insider in January of 2014.
These excellent classroom management tips work on the soccer field as well as the corporate board room!
Enjoy reading this full article.
Tournament Time!
Posted: Tuesday October 6th, 2015 Expires: 12/1/2015
2015 - 10/17/2015 - Soccer To The Maxx Jamboree 2015 (Local Jamboree) - BUT HURRY! Registration Closes SOON!
2015-2016 - State Recreational Cup Tournament (IS STILL OPEN!), but HURRY!
Click Here for complete and updated tournament details
Equipment check: What refs allow and don't
Posted: Saturday October 3rd, 2015 Expires: 12/15/2015
A soccer player's basic uniform consists of a shirt, shorts, socks, shinguards and footwear.
"Regarding arm and/or hand casts, they must be properly covered in sponge and not be dangerous to others for that player to participate.
"For complete knee braces, manufacturer's padding comes with each brace and should be worn over it so that there are no sharp edges, which can be dangerous. Some players do not like to wear the padding as they believe it limits their mobility. Have them wear the manufacturer's padding over the brace so they can play."
Please take a few minutes to read the rest of the Soccer America post so players, coaches and parents will be on the same page as referees.
NSYSA BOD Meeting
Posted: Saturday October 3rd, 2015 Expires: 12/1/2015
The NSYSA BOD Meeting is typically scheduled for the 1st Monday of each month.
The meeting will be held at:
Poulsbo Fire Station
911 Liberty Rd
Poulsbo, WA 98370
Time: 7:30PM-10:00PM
Please note that the NSYSA Board Meeting is a public meeting - open to all who wish to attend. However, should any attendee wish to speak to the board on any particular matter, they should first contact the NSYSA Secretary (email@example.com) in sufficient time to be placed on the Meeting Agenda.
To view the current Meeting Package, please click here:
Washington Youth Soccer Sideline Development Video
Dear Parents, Club and Association Presidents,
Washington Youth Soccer recently produced a video that focuses on Sideline Development – How parents can improve the game. Experts in coaching and child development have identified three key areas where parents can contribute to a better experience for players.
These 3 areas discussed are:
> Referee Abuse
> Coaching from the sidelines
> The Car Ride Home
"Sideline Development" addresses these circumstances where parents often have the right intentions, but can instead be detrimental to the development of the players and the sport.
NSYSA has posted a supporting paper which when combined with the WYS "Sideline Development" video provide important educational reminders we hope every sideline demonstrates. Download the "Parents are Important Too" document here: https://www.nsysasoccer.org/files/Parents%20are%20Important%20Too.pdf
Please take a few minutes to watch the video and help improve soccer for all.
Referee - New (Grade 8) - clinic training dates and details
Posted: Monday September 28th, 2015 Expires: 10/30/2015
Full Sided Referee Clinic offered by KPSRA
Location: Central Kitsap Fire Station #41,
7600 Old Military Road NE,
Bremerton WA 98311
Date: Sunday 10/4/2015
Time: 8:30-5:00
Pre-registration and completion of online material is REQUIRED.
VERY, VERY IMPORTANT: This class has online material that MUST be completed (and this system MUST say ONLINE COMPLETE in green highlight) prior to class. You WILL NOT be admitted to the class if you have not completed the education and the system does not indicate ONLINE COMPLETE. Paper or email proof of completion is not accepted. There are no exceptions.
If you have questions please feel free to contact Brad Wiggins, firstname.lastname@example.com, 360-271-9633
WA Referees registration link here:
The fall season's underway. Is your first-aid kit in order?
Posted: Friday September 18th, 2015 Expires: 12/1/2015
With the fall season underway, you've made sure your team's first-aid kit is in order, right?
Every youth coach should have a very basic sideline first-aid kit. You should have this at each training session and game.
Read the rest of this Youth Soccer Insider article by following this link
NSYSA security cert recently renewed
Posted: Saturday September 12th, 2015 Expires: 12/1/2015
The NSYSA site uses a thawte SSL123 Certificate to offer secure communications by encrypting all data to and from the site. thawte has checked and verified the site's registered domain name.
Users encountering a "caution" warning if visiting the site for the first time since Sept. 8, are encouraged to refresh their browser and proceed.
(Refreshing browser will pull in updated SSL123 credentials.)
Should you continue to encounter "caution" warnings, please send an email to Northwest Sound Youth Soccer Association's firstname.lastname@example.com with:
a) date and time
b) devise (e.g. Android XYZ phone or Dell laptop)
c) version of web browser, i.e. Chrome, Firefox, (and if possible version/edition)
d) optional - screen shot of "caution" warning screen.
This information will be used for building a support case with Thawte and NSYSA software company.
More details on the current and valid NSYSA Thawte SSL certificate can be found by following this link
Posted: Saturday September 5th, 2015 Expires: 11/1/2015
The September 7 meeting will be held at:
Fire Station on Old Military Rd, Station 41
7600 Old Military Rd NE
Bremerton, WA 98311
To view the current Meeting Package, (when available), please click here:
International Clearance Options for foreign exchange students
Posted: Thursday September 3rd, 2015 Expires: 12/15/2015
With school back in season, here is a useful link for clubs welcoming foreign exchange students/non US citizen players that are interested in playing.
The process required to follow in order to play and the steps to obtain clearance from the federation.
For children born in military families, please fill out an FR-11 form and use their Consular Certificate of Foreign Birth to clear the players as U.S. citizens.
Contact the NSYSA VP of Admin firstname.lastname@example.com if your Club has further questions after reading this article.
Tips Video to help take some of the mystery out of RMA's
Posted: Thursday June 25th, 2015 Expires: 12/31/2015
This brief NSYSA Tips Video attempts to answer the question:
"Why doesn't isn't my approved RMA recognized when I log into NSYSA?"
RMA (Risk Management Authorization), is essential for all:
Without current RMA synced to your NSYSA user profile you are limited in what you can access on this site.
Watch the brief video here
Posted: Monday December 29th, 2014 Expires: 2/1/2016
The NSYSA BOD Meeting is typically scheduled for the 1st Monday of each month.
To view the current Meeting Package, (when available), please click here:
Posted: Monday December 29th, 2014 Expires: 1/1/2016
Welcome to the Northwest Sound Youth Soccer Association Site on Tuesday, October 13th, 2015 at 3:59pm PDT. We provide organization to the Youth Soccer program in Washington State in and around the Kitsap and Olympic Peninsulas.
Navigation around and about our website is done by clicking on any of the active hyperlinks that look like this, the active graphical elements you'll find distributed throughout the site, or via the Table of Contents which appears at the left edge of virtually all the website pages. It is also possible to return to this home page at any time by clicking on our Logo in the upper left corner of any of the site's pages.
If you are a current NSYSA participant, you can logon to the site by identifying yourself on our Logon page. Once successfully logged on, you'll be able to interact with NSYSASoccer.org and obtain access to the information that is appropriate for your involvement with our efforts.
We hope that you are successful at locating the information you are seeking here on our site or wherever your travels through the World Wide Web may take you.
See you on the pitch!


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+myConnections: Engage your community - connect to news, events and information you care about. View more information...
View your community's facilities and features online with the new Facilities Module.
Personalize your online experience to stay up-to-date on news, events and other information.
64th Street (Mission Road to Indian Lane):
The stormwater system will be upgraded and replaced, as well as all of the curbs, drive approaches, and asphalt. The construction is currently planned for the summer.
Street work on the four streets listed below will include new curbs, undercurb drains and driveway approaches, as well as new asphalt:
• Verona Terrace
• Sagamore (Tomahawk to 65th Street)
• Intersection of Verona Road and
Norwood (south of 63rd Street)
• 64th Street (Belinder to Ensley Lane) - mill and pave only
Spot Curb Replacement Program:
The City will also conduct its annual assessment of the all curbs and gutters in the City to determine a list of areas for priority replacement in 2015.
Looking Ahead to 2016:
Built in 1951, the 63rd Street bridge is in need of replacement. While it is still safe to drive on, the state of Kansas has rated the bridge as structurally deficient. The surface of the bridge was rebuilt in 1991, but there has not been any significant projects that have addressed the bridge's substructure. The entire structure of the bridge will be completely replaced. Additionally, 63rd Street from Mission Road to State Line Road will be rebuilt including new curbs and drive approaches. Engineering for this project is underway. It is estimated that 63rd Street will be closed about 4 months while this project is completed.


text:
Hotel Baba Haveli - Jaipur
- Free WiFi and free parking
Your hotel has a restaurant where you'll find good menu choices for breakfast, lunch and dinner. The on-site spa is the place to be for rest and relaxation, offering facials and body treatments.
Massage/treatment rooms and spa services are among the leisure facilities on offer. Free high-speed (wired) Internet access is available.
Main amenities
- 14 guestrooms
- Restaurant
- Full-service spa
- Breakfast available
- Free train station pick-up
- Airport shuttle
- 24-hour front desk
- Coffee/tea in the lobby
- Air conditioning
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- Front desk safe
- Laundry service
What's around
- Triton Mall (1.6 mi / 2.6 km)
- Bhawani Niketan Girls College (1.7 mi / 2.8 km)
- Heaven-Piercing Minaret (2.8 mi / 4.5 km)
- Nahargarh Fort (3 mi / 4.8 km)
- City Palace (3 mi / 4.9 km)
This place is perfect. The food is great, the owner Vijay is the most welcoming I've ever…
I would like to thank Mr Gautam and his kids for a pleasurable experience in Jaipur . He…
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Hotel Info: 1-877-214-4288from $15
- Standard Room (NON AC)
- Standard Room
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- This hotel has 14 rooms
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- Check-in time starts at noon
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- Credit card or cash deposit required
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- Children (4 years old and younger) stay free when occupying the parent or guardian's room, using existing bedding
- Free wired Internet access in public areas
- Free WiFi and wired Internet access in rooms
- Airport shuttle (available 24 hours) *
- Free train station pickup
- Free self parking
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- Breakfast (surcharge)
- Restaurant
- Room service (during limited hours)
- Coffee/tea in the lobby
- Full-service spa
- Spa treatment room(s)
- Scooter/moped rentals on site
- 24-hour front desk
- Tours/ticket assistance
- Dry cleaning/laundry service
- Wedding services
- Number of buildings/towers - 1
- Year Built 2008
- Safe-deposit box at front desk
- Accessible path of travel
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In the room
- Air conditioning
- Ceiling fan
- Individually decorated
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- Separate dining area
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- Private bathroom
- Shower only
- Free toiletries
- Cable TV channels
- Desk
- Free newspaper
- Free WiFi
- Phone
- Daily housekeeping
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The onsite spa has massage/treatment rooms. Services include facials and body treatments.
DiningRoof Top - This restaurant serves breakfast, lunch, and dinner.
Hotel Baba Haveli - Jaipur's small print
Only registered guests are allowed in the guestrooms.
Optional extras
Airport shuttle service is offered for an extra charge of INR 450 per vehicle (one way)
High-speed Internet access (wired) is available in guestrooms for INR 60 for 2 hours (rates may vary)
We have included all charges provided to us by this hotel. However, charges can vary, for example, based on length of stay or the room you book.


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Elizabeth Arden, Inc. has entered into an exclusive long-term global licensing agreement with AEFFE S.p.A. for the development, marketing and distribution of fragrance, cosmetics and skin care products with fashion designer Alberta Ferretti. A debut fragrance is planned to launch in the spring of 2009. Elizabeth Arden will produce and market the fragrance collections with creative direction for the scents to come from Alberta Ferretti herself.
"Alberta Ferretti is an icon in the world of fashion design, and we are thrilled to be working with her to create a fragrance line that reflects the sensibilities of her style," said E. Scott Beattie, chairman and CEO, Elizabeth Arden. "Adding the Alberta Ferretti name to our designer fragrance brands allows us to diversify our fragrance brand portfolio and strategically expand our reach of prestige fragrance distribution, particularly in the European fragrance market."
"I'm extremely proud to embark on the adventure of creating my fragrance with Elizabeth Arden," said Ferretti. "The history of Elizabeth Arden in the world of beauty is characterized by a distinct definition of femininity that is quite close to my own world, in which beauty, femininity and sensuality emanate from the personality. I am convinced that this collaboration will result in a remarkable fragrance that will express the contemporary nature of a woman who lives in the present yet looks to the future," she added.
"The signing of the agreement for Alberta Ferretti fragrances with Elizabeth Arden guarantees the same standards of quality and excellence which are synonymous with those of our brand," said Ferretti, chairman, AEFFE S.p.A. "Moreover, the leadership held by this American company in the fragrance sector enables us to realize a commercial development focused also on prestige and quality factors."
Financial terms of the agreement were not disclosed.
Elizabeth Arden; AEFFE S.p.A. Sign Licensing Agreement
January 28, 2008
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|The Lounge | Champions | The Wire | Schedule | Audio | Arcade | The Top Ten | Historical | Email | Video
Choosing Fitness Equipment
Finding the perfect piece of fitness equipment can be a little confusing with so many different types on the market these days. Every other infomercial on television is advertising some sort of fitness equipment. You need to have a good idea of your target area, or areas, the space you have available to use and to store your equipment, and how much money you are willing to spend to get yourself in shape. Once you have the basics in mind then you can narrow it down a little.
One consideration if you are on a budget with limited space is Tony Little's Gazelle. You can get the basic model for less than $100 and it folds down to store in a tight space. The workout is a total body workout and you can do a variety of exercises to target specific parts of the body.
Treadmills are a very popular option for cardio and they are simple to use as well. You will be looking at a heftier price tag but you are more likely to stick with a piece of fitness equipment like a treadmill that mimics your natural movements of walking and running.
Of course there are plenty of other options but you might want to start small before you invest in a total home gym or something of the like. As with any new fitness program, you will need to check with your doctor to make sure that the fitness equipment that you decide on is going to be a healthy choice for you.
James is a published author at Fitness Freaks, a site dedicted to bringing you up to date information on Health and Fitness related topics. For more great articles, visit our Fitness Articles page.
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Business Directory » Health & Beauty » Psychiatrists
Long Island Psychiatrists
For many, the path to mental wellness can be made significantly easier with the assistance of a trained, professional Psychiatrist. A psychiatrist has the medical knowledge to properly treat and medicate patients for mental illness and issues such as depression and anxiety. Unlike a psychologist, a psychiatrist can prescribe patients medication that will help them on their journey to health, and aid in their treatment and recovery. There are many psychiatrists on Long Island, with countless specialties, that can help you get through a difficult time you may be facing, and begin your journey back to a happy and fulfilling life.
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Dr. Jeffrey R. DeSarbo, DO
(516) 414-2545
Jennifer Serrentino
Long Island Psychiatric
Mental Health Services
Stony Brook Medicine - Psychiatry
Leg. Lindsay III Tours Updated Facility for Mental Health Program
Recently, Skills Unlimited, an affiliate of Family Residences and Essential Enterprises, Inc. ...
Kaminsky Calls For Investigation of Deficient Mental Health Coverage For Children
Assemblyman Todd Kaminsky authored a letter to the New York State Department ...
Governor Cuomo Holds First New York Veterans and Military Families Summit
Governor Announces Initiatives to Provide Veteran and Military Families with Affordable Housing, ...
Crime Update: Three Suspects Start Off the New Year By Robbing a Duane Reade, Multiple Cars Stolen in West Hempstead on the Same Morning
Three suspects rob a Duane Reade in Hewlett, while in West Hempstead ...


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Read the original here:
SEOLOGIST – SEO Company Toronto – Content Marketing Canada …


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Latest Articles
Peter Asher to Join Denny Laine at Capitol Center for the Arts, 10/25
by BWW News Desk - September 18, 2015
Denny Laine, formerly of the Moody Blues and Wings, returns to Concord with special guest emcee Peter Asher for the Complete Band on the Run, a live on-stage performance of the classic album at Capitol Center for the Arts in Concord -- complete and unabridged on Sunday, October 25, at 7:30pm... (more...)
Symphonic Rock Icons Renaissance to Tour The US Fall 2015
by BWW News Desk - August 31, 2015
Symphonic rock icons Renaissance featuring legendary singer Annie Haslam will be performing in the US in the Fall 2015!... (more...)
NJPAC & Concord Music Group Accepting Entries for 4th Annual Sarah Vaughan Competition Through 9/14
by BWW News Desk - August 19, 2015
The Sarah Vaughan International Jazz Vocal Competition is the world's most visible jazz vocal competition of its kind and provides a platform for one outstanding female singer to launch a career in the music industry. The competition started in 2012 and was co-produced by NJPAC and JAZZ ROOTS, a Lar... (more...)
The Moody Blues Vocalist Justin Hayward to Perform in Nashville, 9/10
by BWW News Desk - August 17, 2015
Justin Hayward, the esteemed vocalist, lead guitarist, and composer of The Moody Blues, will visit Nashville with a one-night-only performance at the Tennessee Performing Arts Center's James K. Polk Theater on September 10. English virtuoso guitar player Mike Dawes will open the show.... (more...)
Faith Prince, Joshua Bell & More Set for Arizona Musicfest 2016
by BWW News Desk - July 31, 2015
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Justin Hayward to Perform at MPAC, 8/30
by BWW News Desk - July 29, 2015
Justin Hayward, esteemed vocalist, lead guitarist, and composer of the Moody Blues, brings his acoustic tour to Mayo Performing Arts Center on Sunday, August 30, 2015 at 8 pm. Tickets are $39-69.... (more...)
Ken Greves to Play Cafe Noctambulo on July 2
by BWW News Desk - July 01, 2015
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Lexus Pop-Up Concert Series Powered By Pandora Live In Miami
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The Toyota Summer Concert Series at the Pacific Amphitheatre at the 2015 OC Fair features 24 nights of country, pop, reggae, classic rock and comedy offering concertgoers a variety of entertainment options to select from this summer.... (more...)
5th Annual Pittsburgh JazzLive International Festival Welcomes Rachelle Ferrell, 6/19-21
by BWW News Desk - June 05, 2015
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The Nash Sets June Lineup
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June is getting Jazzy as The Nash's calendar heats up for the summer. The jazz club brings some new groups to the venue including Rachel Eckroth performing with Holly Pyle, Sloth Moth for First Friday and the fascinating Nautabot. ... (more...)
Justin Hayward to Bring 'Watching and Waiting Tour' to Boulder Theater, 9/16
by BWW News Desk - May 15, 2015
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Count Basie Orchestra, Diane Schuur and More Among Birdland's May 2015 Lineup
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Emily West's New Single 'Bitter' Available Now; Album Due in August
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The Moody Blues & ZZ Top Join Spring 2015 Line-Up at Wells Fargo Center for the Arts
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by TV News Desk - December 03, 2014
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Concert Data Provided by Pollstar
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Watch Video: Fantasy Football: Week 6 advice
Tampa Bay coach Jon Gruden said he had to walk away after watching film of the Carolina Panthers' defense.
On Sunday, the Buccaneers coach will see why the Panthers' have frustrated so many opponents this season when Carolina looks to create further separation atop the NFC South.
The Panthers (4-1) lead the division thanks to one of the NFL's best defenses, which has held opponents to five touchdowns the last four games and 268.6 yards per game overall—fourth-best in the NFL.
Carolina hasn't allowed a touchdown in its last nine quarters, shutting out the Kansas City Chiefs 34-0 last Sunday after limiting the Atlanta Falcons to three field goals in a 24-9 victory on Sept. 28. Still, defensive end Julius Peppers doesn't think the team's done anything special yet.
"We're taking care of the things we should be taking care of going into the sixth week of the season," said Peppers, who got his third sack of the year Sunday to surpass the 2 1/2 he had in his abysmal 2007. "I only see us getting better from here."
While Peppers might not be impressed, Gruden said he was after watching film.
"I had to turn the film off and go for a walk," he said. "I got a little nervous, you know what I mean?"
Gruden has good reason to be. Last Sunday, the Chiefs were held to 127 yards of total offense—35 on the ground. Larry Johnson joined Michael Turner, Adrian Peterson, Matt Forte and LaDainian Tomlinson as leading rushers who have failed to gain 100 yards against the Panthers.
It helps that they were backed by a solid offensive effort by DeAngelo Williams, who rushed for a season-high 123 yards and two touchdowns, and Jake Delhomme was 14-of-22 for 236 yards, two touchdowns and one interception.
The 4-1 start is Carolina's best since going 5-0 in 2003, when the Panthers lost to the New England Patriots in the Super Bowl. The Panthers returned to the playoffs in 2005, losing in the NFC title game, but went 15-17 the last two years and failed to make the postseason.
While the defense has received much of the attention, coach John Fox also credits a big part of the turnaround to Delhomme.
Delhomme, who missed the final 13 games last season to undergo ligament-replacement surgery in his elbow, has thrown five touchdowns against only two interceptions, and is ninth in the NFL with 1,096 passing yards
"I don't think we wanted to be 8-8 two years ago or 7-9 last year. The reality is we didn't have a quarterback a year ago," Fox said. "Those things happen. … When you can't throw the ball it's rough."
While the revival of Delhomme and the work of the defense gives the Panthers reason to be optimistic about the future, the Buccaneers (3-2) aren't even sure who will be starting at quarterback on Sunday when they try to bounce back after having their three-game winning streak snapped.
Brian Griese was knocked out of Tampa Bay's 16-13 loss to Denver in the third quarter last Sunday with a swollen right elbow. Griese was 13-of-19 for 88 yards before he was replaced by Jeff Garcia, who went 13-of-17 for 93 yards and a touchdown.
Griese had started all three of Tampa Bay's wins, throwing four touchdowns and six interceptions after taking over in Week 2 for Garcia, who was struggling with injuries suffered in the preseason.
Gruden wouldn't commit to a starter and said it will be a day-to-day situation.
"We're going to address the quarterback situation once we get all the facts," he told the Buccaneers' official Web site. "Obviously, health is going to be an issue. I thought Jeff did do some good things (Sunday). His health has been an issue, and his return to health is also something that we're excited about."
Garcia started 13 games for Tampa Bay in 2007, throwing 13 touchdowns, four interceptions and averaging 187.7 passing yards. The Buccaneers went 9-7 last season, losing to the eventual Super Bowl champion New York Giants in the playoffs.
Tampa Bay and Carolina split their two meetings last season with each winning on the road. The Panthers have won five straight at Raymond James Stadium.
Team Comparison
Blog Coverage from SB Nation
Tyronne Green G, Stephen Hill WR, Kelvin Benjamin WR, Frank Alexander DE, Davonte Wallace T, Arthur Miley DE, Nate Chandler T, Charles Johnson DE
Leonard Johnson CB, Kenny Bell WR, Larry English DE, Garrett Gilkey G, Patrick Murray K, Demar Dotson T, T.J. Fatinikun DE


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February 2013, TruckingInfo.com - Feature
By Contributed by Pam Whitfield & Don Jacobson
February is American Heart Month for one really good reason. Heart disease is the number one killer in this country, accounting for about a quarter of all deaths every year. That means the odds are nearly six to one that you will die of a heart problem rather than in an accident.
Tags: Fit to Drive, Health, Diet & Nutrition, Drivers
November 2012, TruckingInfo.com - Feature
By Deborah Lockridge, Editor in Chief
Bob Perry has been trying to help drivers be healthier for about 25 years, but he was way ahead of the curve. It's only in the past couple of years that the industry has embraced the notion that healthier drivers are safer, happier and more productive
Tags: Diet & Nutrition, Drivers, Health
September 2012, TruckingInfo.com - Feature
By Genevieve Conti, Assistant Editor
Carl Bailey's before and after weight-loss pictures make dropping 58 pounds look like magic
Tags: Diet & Nutrition
We offer e-newsletters that deliver targeted news and information for the entire fleet industry.
The expert, Mark Betner from CITGO, will answer your questions
The expert, Rence Oliphant from Hendrickson, will answer your questions
LockLight Indicates When a Lift is Safe
Diesel Fuel Test Takes 20 Minutes
CT50 Mobile Computer Offers Flexible Features
Accuride App Displays Products and Information


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Photos: Rally for Immigration Reform -- Change Takes Courage and Faith
We All Share Responsibility for Going to War -- and for Stopping It
A comment on my recent blog about The Hurt Locker really got my blood boiling.
Pray Immigration Reform Into Passage
On Sunday, a major march for immigration reform will take place in Washington, D.C. Tens of thousands of people will gather to call on the White House to lead, and put forward an immigration reform bill whose time has come.
Standing (Online) With Immigrants
This Sunday, March 21, we invite you to join with us and thousands of other people of faith from around the country, and with tens of thousands of other Americans, at March for America: Change Takes Courage and Faith.
Glenn Beck Responds: Social Justice 'Is a Perversion of the Gospel'
International Women's Day: 'Whom God Hath Made Equal'
Immigration Reform: Change Takes Courage and Faith
The window is closing on comprehensive immigration reform. At least that's what the politicians in Washington are saying. They're afraid of more demagoguery. They're afraid of upcoming elections. They're afraid of the politics of fear.


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Los Angeles Lakers v Oklahoma City Thunder
Jordan Hill of the Los Angeles Lakers goes to the basket against the... News PhotoBasketball - Sport,Horizontal,Jordan Hill - Basketball Player,Los Angeles Lakers,NBA,NBA Pro Basketball,Oklahoma City,Oklahoma City Arena,Oklahoma City Thunder - Basketball Team,Sport,USAPhotographer Layne MurdochCollection: National Basketball Association 2012 NBAEOKLAHOMA CITY, OK - December 7 : Jordan Hill #27 of the Los Angeles Lakers goes to the basket against the Oklahoma City Thunder during an NBA game on December 7, 2012 at the Chesapeake Energy Arena in Oklahoma City, Oklahoma. NOTE TO USER: User expressly acknowledges and agrees that, by downloading and or using this Photograph, user is consenting to the terms and conditions of the Getty Images License Agreement. Mandatory Copyright Notice: Copyright 2012 NBAE (Photo by Layne Murdoch/NBAE via Getty Images)


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Even though gas prices have recently dropped to nearly record low levels for the past few years, there is still a movement of folks vying for alternative fuel and electric vehicles. During Full Article »
I know you have seen it and maybe even participated in it. During one of those awful rain storms or frequent downpours about 50% of the driving public here in Full Article »
I have always been a fan of science fiction. The original Star Wars trilogy sits atop my favorites, but movies set in the not-so-distant future, like the second film in Full Article »
A demonstration for a self-parking Volvo XC60 did not go as planned last week when the driver decided to perform a quick demo of the Pedestrian Detection with Full Auto Full Article »
Drought conditions do not necessarily have to equate to dirty dusty cars. This Silicon Valley car wash uses a "secret" spray bottle solution to get dirty vehicles looking Full Article »
Oil companies have always pimped the idea of their brand giving cars additional performance but never really showing us the numbers, at least numbers that most of us understand. Though, Full Article »
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WholeFoods Magazine SourceBook: The Natural Products Directory
Hodgson Mill added 18 products to its line of whole grain foods using ancient grains and gluten-free ingredients. Products include: Non-GMO Cornstarch; Potato Starch; Pearled Sorghum; Buckwheat Groats/Hearts; Quinoa; Quinoa Flour; five flavors of Sorghum, Brown Rice & Quinoa Side Dishes; and Steel Cut Oat, Sorghum & Quinoa Hot Cereal.
Bakery On Main has launched a new snack line: the Nut Crunch Snack. Made from nuts, gluten-free oats and dried fruit or chocolate, the product is available in Original, Blueberry Cobbler, Chocolate, Maple Vanilla, Chocolate Peppermint and Chocolate Orange. The snack is certified gluten free (GFCO), Non-GMO Project Verified and dairy and casein free.
Dave's Killer Bread has released three new organic and Non-GMO Project Verified products. White Bread Done Right is organic white bread with 10 g of whole grains in each slice. Sprouted Whole Grains features four sprouted grains: wheat, barley, oats and rye. The Million Dollar Bun is a bun filled with 18 g of whole grains, 8 g of protein and over 1,000 mg of omega-3s.
News from industry food companies.
Montpelier, VT—Vermont attorney general Bill Sorrell has formally adopted regulations implementing a state law requiring labels for genetically modified foods, following the passing of the bill by state lawmakers in 2014 after months of outreach and grassroots support.
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Ancient grains have achieved strong recognition from mainstream and natural shoppers alike. Here's what you need to know about some of the hottest grains on the market.
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Soooo the last bit of the journey.... combining Primal/crossfit/walking/running to try and get in those size 14 jeans!!!
Soooo the last bit of the journey.... combining Primal/crossfit/walking/running to try and get in those size 14 jeans!!!
Hi and welcome! Your loss so far is truly inspirational, I'm looking forward to reading about your progress here.
Awwww thanks hun! This last 2 stone is a right bugger lol!
Sooooo yesterday was my treat day.... Tapas/wine and cheese..... lovely.... so back at it today!!!
Its the days I do crossfit that I struggle to get all my calories in.... very aware of eating too little as i know this causes me to stall....
What makes you struggle? Is it sheer volume of food? Healthy fats are a good way to overcome this problem.
I just feel like I'm eating all the time lol.... I have nuts generally to snack on but am always a bit wary of too much fat... Isn't it a hard habit to break not reaching for low fat stuff.... I'm going to try to have some mackeral this week.... also maybe roast some veg in a bit of oil to take to work.... I usually just take raw veg!!!
Is there anything else i could up my cals with???
Fat has 9 calories per gram whereas protein and carbs have 4 calories per gram, so fat is the most efficient way to increase calories without adding too much bulk. There are a lot of web resources on eating fat in the paleo diet, I know it seems strange to go from 'traditional' thinking about diet (high wholegrain carbs, low fat) to paleo thinking (high fat, moderate protein, lower carbs and none from grains) but if you stick with it then you'll get there. If it helps put it into perspective, with higher fat foods I eat around 1750 calories/day easily in 3 meals and a snack (plus a small treat after dinner) without having enormous heaped platefuls.
Good fat sources that I use when I haven't had enough fat in a day are macadamia nuts, a bit of cheese, full fat yoghurt or cream (which I allow as I'm more primal than paleo), good quality mayonnaise and avocados. I also cook with more fat now (coconut oil or ghee usually) and add more oil to salads. Nuts aren't the only source and you want to be a little careful with them if you are worried about your omega 3/6 balance (again loads on the web so I won't bore you here).
Without seeing what types of meal you are tending to have it's difficult to make other suggestions.
I'm thinking yoghurts are going to be a good way forward... I am convinced I dont like avacado... but I dont remember actually tasting them... lol... sounds daft! So i think I'm gonna give them another go!!
You have done amazingly well..... Have you lost all your weight paleo???
Make sure you get a ripe avocado, if they're still hard they're a bit gack! LOL! Even the 'ripe and ready' ones you get in the supermarket can usually do with a day or two of further ripening at home. Ripe ones are really nice chopped up or mashed into quacamole. In Cyprus I had an amazing avocado salad that was two halves of an avocado filled with small prawns and smothered in olive oil and lemon dressing - thought I'd died and gone to heaven!
And thank you! My first 6 months were with Slimming World, I then switched to low GI as I was eating a lot of junk within the SW rules. Ate low GI/South Beach Diet for just over a year, until the end of the summer this year when I gravitated towards primal naturally after cutting out wheat and finding that a lot of gluten-free foods were high GI.
Thought I'd stop by on ur new diary honey xxx
Hey chick.... How you feeling??? X
I'm checking in too miss amazon )
How's the crossfit going??
Must say primal is my idea of heaven... Mmm fats ahoy .. love coconut oil yums and avacado ... Try it really ripe with crayfish mmm
Hey ladies....
Last nights crossfit was...
400m run
3 rounds 5*pull ups 5*press ups 5*sit ups 5*squats
3-3-3-3-3 Bench press (3 rep max 30kg, 1 rep max 32.5kg) Both personal bests.... but thats as I've never done it before lol....
Workout- 25-20-15-10-5 reps of press ups and then kettle bell swings.....
Got a feeling tonight will be legs!!!! Cant wait.... Although I am feeling a bit groggy!!! Sore throat!! Noooooo!!!!!
Your doing grand hun
I adore benching your strength will increase so fast too :-)
Well done Xx
Oooooh Crossfit was a toughey tonight!!!!
Warm up...
Then 3 rounds of each (One minute)
Medicine ball slams
Box jumps (I do step ups)
Pull ups (On the rings)
Dumbell thrusters (5kg)
Afterwards some stretches and working on my press ups!!!!
Gonna feel that in the morning!!!!
Loved it though!!! Feel a million dollars after!!!!


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