text:
KGN Industries appoints Deepak Soni as compliance officerKGN Industries Ltd has informed BSE that Mr. Deepak Raval has resigned from the Company from the position of CEO, Company Secretary Compliance Officer. Company hereby appointed Mr. Deepak Soni as Compliance Officer of the Company with effect from January 01, ... Money Control, 2 months ago
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Three patrol vessels join ENC fleet
Comment · print · T T T+· T- ENC Flag Officer Commanding-in-Chief Vice-Admiral Satish Soni at Naval Dockyard in Visakhapatnam on Tuesday. -Photo: K.R. Deepak The second batch of three immediate support vessels joined the fleet of the ...The Hindu, 5 days ago
3 vessels join Navy to protect offshore assets
Flag Officer Commanding-in-Chief Eastern Naval Command Vice Admiral Satish Soni unveiling the plaque of the Immediate Support Vessel IN ISV T 39 after he commissioned the vessel along with two other ISVs at Naval Dockyard in Visakhapatnam on ...The Hindu, 5 days ago
Parekh Suggests Large PSU Divestments, Wants Pro-Growth Budget
MUMBAI: Pitching for disinvestment in public sector behemoths like LIC, Air India and BSNL, top industry leader Deepak Parekh has said it can unlock huge funds worth lakhs of crores of rupees and shares should be given to retail investors without ...Silicon India, 1 month ago
Sony Music launches second YouTube channel for kids
MUMBAI: Sony Music has launched its second YouTube channel for kids called DArt of Science featuring Deepak Pathania, India's very own Steve Spangler. Known for his magical videos that artistically blend fun and innovation with science, Pathania, ...Indian Television, 1 month ago
Kundan Shah's P Se PM Tak to release on May 22
Written and directed by Kundan Shah, film 'P Se PM Tak' is now all set to release in theatres on May 22, 2015. The film is produced by Dhaval Jayantilal Gada and Kushal Kantilal Gada under their banner of PEN India production, who has produced the very ...Moviez Adda, 3 days ago
Dhanesh Dogra is Best Actor, Gurmeet Kour Best Actress
Excelsior Correspondent JAMMU, Mar 25: Dhanesh Dogra and Gurmeet Kour have been awarded as Best Actor and Best Actress, respectively as Jammu and Kashmir Academy of Art, Culture and Languages announced the results of the annual Drama Festival. ...Daily Excelsior.com, 4 days ago
Amateurs lit up Annual Theatre Festival
Lalit Gupta Despite non-existent training opportunities and apprenticeships, poor infrastructure, lack of economy around theatre topped with measly State re/awards, it surely goes to the credit of dedicated lot of the old and young amateur theatre ...Daily Excelsior.com, 1 week ago
Everyone Kanye West Has Ever Compared Himself To
Note: This is who Kanye has compared himself to in his music . 1. Cassius Clay (Muhammad Ali) Rogers / Grant Lamos IV / Stringer From: Primetime ( Watch the Throne ) Lyric: Primetime, basking in the lime / Cassius in ...BuzzFeed, 1 week ago
Bajaj Discover seeks to bring the spark back in married couples
Leo Burnett has conceptualised the campaign featuring three films that showcase how the two-wheeler brand fulfils its purpose of bringing romance back in the lives of married couples BestMediaInfo Bureau | Mumbai | March 19, 2015 Click on the ...Best Media Info, 1 week ago
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subset: commoncrawl


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Ashes: Fourth Test Day Four wrap
Grandstand's Jim Maxwell wraps up the final day of the fourth Ashes Test at Durham which England won by 74 runs.
Source: ABC News | Duration: 1min 49sec
In the lead-up to the New South Wales election both major parties have been making claims in key policy battlegrounds.
But how much of what the leaders claim checks out?
By Peta Yoshinaga
Australian comedian and satirist Barry Humphries says he draws inspiration from alter ego Dame Edna Everage.
The Coalition has closed gap on Labor in the latest Newspoll, but only once the NSW election and the May budget have passed will Tony Abbott's future be clear.
Leviathan is about a man who attempts to stop the demolition of his house by a corrupt politician, and in Russia it's been seen as a criticism of Vladimir Putin.


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Bed & Breakfasts South Africa - Baysands Lodge is situated in Bloubergstrand, a coastal village on the scenic west coast of Cape Town.
Bed & Breakfasts South Africa - Welcome to Dutch Manor in Cape Town.
Bed & Breakfasts South Africa - Over the years, this classic Cape Town bed & breakfast has earned an enviable reputation..
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Bed & Breakfasts South Africa - Affordable and smart rooms facing secluded garden. Mountain views all around. Quiet setting. Sparkling clean.
Bed & Breakfasts South Africa - The Rabbit Hole Guest House and Restaurant offers Award Winning Accommodation in Krugersdorp for Travelers to Chamdor, The Cradle of Humankind and West Rand Area.
Bed & Breakfasts South Africa - The Space Guest House is the most centrally located in the heart of trendy Melville, close to the SABC, Media 24, Wits and the University of Johannesburg.
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Health & Wellness
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A free 9-week program for parents and babies from birth to 12 months old. For more information, contact Public Health Nurse Cindy at 416-338-7054. Tuesday mornings from Feb 3rd- March 31st,10:30-12:30.
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Did you know that Tai Chi is the most popular and rapidly spreading form of exercise in the world? It helps millions of people of all ages to live a healthier and more active life....
Toronto Reference Library
Nutritionist Julie Daniluk shares science-based information that will shatter your need to count calories and conquer cravings. She will offer ideas on how to lose weight without dieting, using anti-inflammatory superfoods.
Toronto Reference Library
Depression is not a normal part of aging. Depression is a medical illness that can occur for the first time in late life. It is an illness that affects quality of life and is associated with many other medical conditions. ...
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The economic, political, and health systems in Ontario must be transformed in order to address the most powerful determinants of our health: income and income inequality. Gary Bloch is a family physician with St. Michael's Ho...
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Dr. Nasreen Khatri, Rotman Research Institute, discusses how the brain responds to information overload, technology and instant communication. Is there a change in ability to juggle or handle distractions as one ages? Presen...
Chinese Family Services of Ontario (CFSO) is a non-profit, accredited professional counselling, family services and settlement agency. CFSO provides a wide range of services such as individual/marital/family counselling, sett...
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A basic overview of trusted websites and library databases to help you learn where to find the answers to your most common health questions. Please phone 416-393-7209 to register....


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1809 West Johannsen Road
Five Mile/Prairie, Spokane, 99208
Commute to Downtown Spokane
Almost all errands require a car.
It is possible to get on a bus.
Score Details
1809 West Johannsen Road has a Walk Score of 0 out of 100. This location is a Car-Dependent neighborhood so almost all errands require a car.
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124 North Express
0.8 mi
28 Nevada
0.8 mi
25 Division
1.3 mi
26 Lidgerwood
1.3 mi
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1809 West Johannsen Road is in the Five Mile/Prairie neighborhood. Five Mile/Prairie is the 25th most walkable neighborhood in Spokane with a neighborhood Walk Score of 8.


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My heart goes out to you with the huge difficulties you faced in "hauling" your class room from area to area. I am sure you were exhausted at times and felt devalued.
I do hope things got better for you and many of the ideas in this book have helped.
As hard as it was/is, I hope you developed a resiliency and methods taht have helped through the years.
How disgraceful to think many of our schools and classrooms are in such chaos.


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Andrew Robinson has found himself off the beaten trail more than most travellers.
From Afthanistan's high country to giving comfort to Syrian refugees, he has seen his fair share of the heartache suffered by the world's poor, but has also seen hope, kindness and beauty in some of the world's most remote places.
How often do you get away?
I've spent the past three years overseas. I was in Afghanistan for over two years, working on a variety of humanitarian projects. Most recently, as part of my work with Tear Fund, a New Zealand Christian action organisation which partners with Med-Air in Lebanon and Jordan, I was helping Syrian refugees.
Where was your first trip?
When I was 10, my family went to Thailand. I have fond memories of feeding peanuts to baby elephants.
Why do you travel – business or pleasure?
Work has given me the opportunity to travel to interesting places off the beaten path, but I've also enjoyed fun tourist destinations.
What is your favourite overseas destination?
The beaches of southern Sri Lanka. I didn't know what relaxation was until I visited Sri Lanka.
And here in New Zealand?
I've done a lot of tramping in New Zealand. Sunset on Lake Manapouri with a good group of mates and a roaring fire would be hard to beat.
Best trip ever?
Horse-trekking in the mountains of Afghanistan's Badakhshan province – the most stunning, unspoilt scenery I've ever seen and a real privilege to be in such a difficult-to-reach part of the world. Horse-trekking was the only way to reach some of the remote villages we were helping with clean-water projects and nutritional care for malnourished children.
A case of severe food-poisoning on the second day of a four-day hike in the Kaimanawa Ranges. I threw up in my buddy's small two-man tent.
If you could be anywhere but here, where would that be?
Back in Lebanon, continuing my work with Syrian refugees.
What is the wildest sight you've witnessed while travelling?
Watching Afghan horsemen competing in a buzkashi tournament. It's like rugby meets bullrush on horseback and, with over 200 riders involved, fearlessly charging about on their horses, it's frighteningly wild.
The most heartbreaking?
Meeting a young mother and her two small children who had just arrived in Lebanon as refugees from Syria. The father had been killed as he tried to cross the border with his family. The children were too young to understand what had happened, and their grieving, exhausted mother was doing her very best to find something for them to eat and a place for them to live in this new country.
Who or what is your favourite travelling companion?
I have a rather battered acoustic guitar that comes everywhere with me. It's great for sing-alongs or serenading, or for winding down by myself at the end of the day.
Where to next?
I've never been to Cape Reinga so, while I'm home, it's a trip I'd really like to make.
Anything you'd like to add?
I think travelling is incredibly rewarding and can be an eye-opening experience. I've seen and learnt so much during my travels, but sometimes this knowledge can be painful. Living in New Zealand, it's hard to imagine what Syrian refugees are going through. Displaced from their families, with no assurance of the next meal, it is a completely different life from what we are used to here.
I believe, though, that Kiwis are a kind and resourceful lot and we can do a bit to help these forgotten victims of the Syrian crisis.
To find out more about what you can do to help, visit the Tear fund
- The Dominion Post
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See Iron Man, Magneto, Gandalf, Superman, Spider-Man, Space Ghost, Mario, Hermione Granger, a Jedi Master and more geeky pop culture icons go for the goal.
A new trailer for the Marvel and Netflix original series shows just how formidable Daredevil's archnemesis Kingpin, played by Vincent D'Onofrio, is going to be.
Can the God of Mischief, Madness and Evil survive being locked in a cage with his most formidable opponent yet? Loki's chances of survival might just be a teenage dream.
Another bad guy is headed to "Gotham," causing trouble for the citizens of Bruce Wayne's hometown. The actor best known as Peter Petrelli in "Heroes" is slated to play the charming psychopath.
"Doctor Who" and "Broadchurch" actor David Tennant is set to play Kilgrave, but will he truly be shown as the Purple Man in the new series premiering on Netflix?
He's created an Iron Man wrist-mounted rocket launcher and a Spider-man web launcher. Now, laser enthusiast Patrick Priebe channels James Bond.
A "60 Minutes" report this Sunday will look at the lavish life of the Megaupload founder and why the entertainment industry considers him to be the world's No. 1 pirate. Here's a preview.
The evil creatures in Middle-earth may be paying for their dark ways with a vitamin D deficiency.
What makes DC Comics' bad guys even badder? Appearing on 3D covers, without the need for pesky glasses. Here's your chance to win the whole set of Villains Month comics. That's a lot of evil.
When the Joker gets out of jail, the impossible happens. Characters from DC and Marvel meet on the screen in a CGI extravaganza -- maybe.


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Kate Middleton, the Duchess of Cambridge, will soon give birth to a baby girl named Alexandra who will one day study at the University of St Andrews in Scotland and whose first boyfriend will be named Robert.
Or at least that's what the crystal-ball gazing British public are telling bookmakers, who are relishing the frenzy of betting related to the royal baby, the heir to the heir to the heir of the British throne.
Britons can - and do - bet on anything, with some 9,000-plus betting parlours dotted around the country. And with the birth of Britain's most anticipated baby since Prince William expected this month - or July 17, odds-on favorite - wager-happy Britons are queuing up to try and make a royal buck.
"There's a royal bump of excitement across the country," said Rory Scott, a spokesman for Paddy Power, a bookmaker.
"Betting and the royal family are two of our favorite pastimes in the UK, along with talking about the miserable weather, and people are really into it," he said.
Bookies here are taking bets on everything from the baby's weight to its hair color to whether Kate will be "too posh to push."
Bookmakers say that more than £1 million has already been wagered and that the biggest flurry of bets will flood in once Buckingham Palace announces that Kate has gone in to labor.
"We expect it will go through the roof then," said James Dirs, a spokesman at bookmaker Coral.
The big money is on the baby's name, with Alexandra, the queen's middle name, and Charlotte, Pippa Middleton's middle name and the name of King George III's wife, leading the pack. Other favorites include Victoria, Elizabeth and Diana.
"The name is a massive talking point, and there's a long list, all with attractive odds. It's like the Grand National," said Ladbrokes' spokesman Alex Donohue, referring to Britain's most famous horse race and the granddaddy of all betting events in the UK.
Ladbrokes started taking bets on the royal baby the day William and Kate got hitched and have so far handled about £100,000, or double the amount they took on the royal wedding.
The betting public is convinced the baby is a girl. Palace officials have said that the couple themselves don't know the gender, but the thinking here is: Yeah, right.
Punters like to point to an incident in March when Kate accepted a teddy bear from a well-wisher and reportedly said "thank you - I will take that for my d. . .," the wide assumption being she stopped short of saying daughter.
Paddy Power was so certain she meant daughter - and not, say, "dog" - that it paid out winnings of about £6,711 to the 700 people who had already bet on girl. If it is a boy, gamblers are backing the names George and James.
Reflecting the global fascination with the baby, William Hill, Britain's largest bookmaker, said that it has taken around £100,000 in bets from people in 103 countries - although not from the United States, where betting on such events is illegal.
Tony Kenny, a spokesman, said that many of the Britons who are betting are placing small sums on their own name or friends' names and "giving it as a little present, or using it as a joke to share down at the pub." He added that this helped to explain bets placed on non-regal names like Madonna and Waynetta.
While betting is largely done online, Kenny said about 500 people a day are walking in to their shops and dropping a pound or two to fill out a "royal baby" form with six questions including "Will William be holding the baby when they first emerge from the hospital?" (Most people check yes). Bookies also encourage people to dream up their own bets, even long-term ones like the name of the baby's first boyfriend (Robert, 33-1 odds) or girlfriend (Camilla, 50-1).
And one need not wander into a parlour to catch some of the betting buzz: it's enough just to tootle around London. To publicise its offerings, Paddy Power this week sent four plump men dressed as giant babies wearing only diapers and crowns on the subway en route to Buckingham Palace.
Like the thousands of people who have placed a wager, Scott Moorhead, a 34-year-old Londoner who works in advertising, is eagerly awaiting the official announcement of the baby. By tradition, the announcement will be placed on an easel outside of the gates of Buckingham Palace.
He recently bet £40 on Victoria - "a royal name of good pedigree," he said - and is considering placing another on the baby's hair being red (9-to-4), like its Uncle Harry.
Betting on current events like the royal baby "makes reading the news a little more interesting," he said.
-Washington Post
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The investment, which will include
Olaf Wiertz, Sales Director at Schmiedag GmbH (SDG) and Wildauer Schmiedewerke GmbH & Co. KG (WSW) said: "We are more than just a supplier to our customers – we are their partner.
Located on the periphery of two great continents, Turkey has benefitted from being in a favored position right at the center of an assertive and fast growing economic area.
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The Maritime Training Academy announced the launch of its new diploma in maritime security today.
The Surrey, UK-based distance learning center said the


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Today I took a bit of a "mental health" day, I hoped to be well for this whole trip but that's not reality. I'm thankful for meditation and cannabis and love.
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I found this small hand pipe in Smoking Aces on Polk Street, in San Francisco. The glass is really thick, the dichroic sparkle is awesome, and the bowl is deep enough to make it worthy. The pipe along with my mini lighter wrapper in Humboldt Wick accompanied me on an afternoon bike ride today.
Packed up some Platinum Pink Cream Soda before heading into work today.
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Packed the glass blunt with Lemon Skunk Haze this afternoon in Golden Gate Park with some friends from the interwebz.
My glass blunt was sent by Humboldt Traders, I love it!
Milking my Fish Bong.
Don't forget your extra lighters and Humboldt wick this 4/20!!
Rose's PHX added to the Glass Gallery, though I'm sure it's not the first time.
Packing up goodies bags tonight and taking dabs. My FAQ page at coralreefer420.com has some info about where and when I give away bags.


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Are you Toru Yamada?Claim your profile
Publications (133)488.57 Total impact
Article: The environments of Ly blobs - I. Wide-field Ly imaging of TN J1338-1942, a powerful radio galaxy at z = 4.1 associated with a giant Ly nebula[Show abstract] [Hide abstract]
ABSTRACT: We exploit wide-field Ly α imaging with Subaru to probe the environment around TN J1338-1942, a powerful radio galaxy with a 〉 100 kpc Ly α halo at z = 4.11. We used a sample of Ly α emitters (LAEs) down to log (LLyα[ erg s-1]) ̃ 42.8 to measure the galaxy density around TN J1338-1942, compared to a control sample from a blank field taken with the same instrument. We found that TN J1338-1942 resides in a region with a peak overdensity of δLAE = 2.8 ± 0.5 on scales of 8 h- 1 Mpc (on the sky) and 112 h- 1 Mpc (line of sight) in comoving coordinates. Adjacent to this overdensity, we found a strong underdensity where virtually no LAEs are detected. We used a semi-analytical model of LAEs derived from the Millennium Simulation to compare our results with theoretical predictions. While the theoretical density distribution is consistent with the blank field, overdense regions such as that around TN J1338-1942 are very rare, with a number density of 6.4 × 10- 8 Mpc- 3 (comoving), corresponding to the densest 〈0.4 percentile at z ≃ 4.1. We also found that the Ly α luminosity function in the TN J1338-1942 field differs from that in the blank field: the number of bright LAEs (log (LLyα[ erg s- 1]) ≳ 43.3) is enhanced, while the number of fainter LAEs is relatively suppressed. These results suggest that some powerful radio galaxies associated with Ly α nebulae reside in extreme overdensities on ̃3-6 Mpc scales, where star formation and AGN activity may be enhanced via frequent galaxy mergers or high rates of gas accretion from the surroundings.Monthly Notices of the Royal Astronomical Society 02/2015; 447(4). DOI:10.1093/mnras/stu2538 · 5.23 Impact Factor
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ABSTRACT: We present the results of near-infrared spectroscopic observations of the $K$-band selected candidate galaxies in the protocluster at $z=3.09$ in the SSA22 field. We observed 67 candidates with $K_{\rm AB}<24$ and confirmed redshifts of the 39 galaxies at $2.0< z_{\rm spec}< 3.4$. Of the 67 candidates, 24 are certainly protocluster members with $3.04\leq z_{\rm spec}\leq 3.12$, which are massive red galaxies those have been unidentified in previous optical observations of the SSA22 protocluster. Many distant red galaxies (DRGs; $J-K_{\rm AB}>1.4$), hyper extremely red objects (HEROs; $J-K_{\rm AB}>2.1$), {\it Spitzer} MIPS 24 $\mu$m sources, active galactic nuclei (AGNs) as well as the counterparts of Ly$\alpha$ blobs and the AzTEC/ASTE 1.1-mm sources in the SSA22 field are also found to be the protocluster members. The mass of the SSA22 protocluster is estimated to be $\sim2-5\times10^{14}~M_{\odot}$ and this system is plausibly a progenitor of the most massive clusters of galaxies in the current Universe. The reddest ($J-K_{\rm AB}\geq 2.4$) protocluster galaxies are massive galaxies with $M_{\rm star}\sim10^{11}~M_{\odot}$ showing quiescent star formation activities and plausibly dominated by old stellar populations. Most of these massive quiescent galaxies host moderately luminous AGNs detected by X-ray. There are no significant differences in the [O{\footnotesize III}] $\lambda$5007/H$\beta$ emission line ratios, and [O{\footnotesize III}] $\lambda$5007 line widths and spatial extents of the protocluster galaxies from those of massive galaxies at $z\sim2-3$ in the general field.The Astrophysical Journal 11/2014; 799(1). DOI:10.1088/0004-637X/799/1/38 · 6.28 Impact Factor
Article: SEEDS Adaptive Optics Imaging of the Asymmetric Transition Disk Oph IRS 48 in Scattered Light[Show abstract] [Hide abstract]
ABSTRACT: We present the first resolved near infrared imagery of the transition disk Oph IRS 48 (WLY 2-48), which was recently observed with ALMA to have a strongly asymmetric sub-millimeter flux distribution. H-band polarized intensity images show a $\sim$60AU radius scattered light cavity with two pronounced arcs of emission, one from Northeast to Southeast and one smaller, fainter and more distant arc in the Northwest. K-band scattered light imagery reveals a similar morphology, but with a clear third arc along the Southwestern rim of the disk cavity. This arc meets the Northwestern arc at nearly a right angle, revealing the presence of a spiral arm or local surface brightness deficit in the disk, and explaining the East-West brightness asymmetry in the H-band data. We also present 0.8-5.4$\mu$m IRTF SpeX spectra of this object, which allow us to constrain the spectral class to A0$\pm$1 and measure a low mass accretion rate of 10$^{-8.5}$M$_{\odot}$/yr, both consistent with previous estimates. We investigate a variety of reddening laws in order to fit the mutliwavelength SED of Oph IRS 48 and find a best fit consistent with a younger, higher luminosity star than previous estimates.
[Show abstract] [Hide abstract]
ABSTRACT: We compared the number of faint stars detected in deep survey fields with the current stellar distribution model of the Galaxy and found that the detected number in the H band is significantly smaller than the predicted number. This indicates that M-dwarfs, the major component, are fewer in the halo and the thick disk. We used archived data of several surveys in both the north and south field of GOODS (Great Observatories Origins Deep Survey), MODS in GOODS-N, and ERS and CANDELS in GOODS-S. The number density of M-dwarfs in the halo has to be 20+/-13% relative to that in the solar vicinity, in order for the detected number of stars fainter than 20.5 mag in the H band to match with the predicted value from the model. In the thick disk, the number density of M-dwarfs must be reduced (52+/-13%) or the scale height must be decreased (~600 pc). Alternatively, overall fractions of the halo and thick disks can be significantly reduced to achieve the same effect, because our sample mainly consists of faint M-dwarfs. Our results imply that the M-dwarf population in regions distant from the Galactic plane is significantly smaller than previously thought. We then discussed the implications this has on the suitability of the model predictions for the prediction of non-companion faint stars in direct imaging extrasolar planet surveys by using the best-fit number densities.
[Show abstract] [Hide abstract]
ABSTRACT: We present a new method of analysis for determining the surface geometry of five protoplanetary disks observed with near-infrared imaging polarimetry using Subaru-HiCIAO. Using as inputs the observed distribution of polarized intensity (PI), disk inclination, assumed properties for dust scattering, and other reasonable approximations, we calculate a differential equation to derive the surface geometry. This equation is numerically integrated along the distance from the star at a given position angle. We show that, using these approximations, the local maxima in the PI distribution of spiral arms (SAO 206462, MWC 758) and rings (2MASS J16042165-2130284, PDS 70) is associated with local concave-up structures on the disk surface. We also show that the observed presence of an inner gap in scattered light still allows the possibility of a disk surface that is parallel to the light path from the star, or a disk that is shadowed by structures in the inner radii. Our analysis for rings does not show the presence of a vertical inner wall as often assumed in studies of disks with an inner gap. Finally, we summarize the implications of spiral and ring structures as potential signatures of ongoing planet formation.
[Show abstract] [Hide abstract]
ABSTRACT: We conduct a deep narrow-band imaging survey of 13 Ly$\alpha$ blobs (LABs) located in the SSA22 proto-cluster at z~3.1 in the CIV and HeII emission lines in an effort to constrain the physical process powering the Ly$\alpha$ emission in LABs. Our observations probe down to unprecedented surface brightness limits of 2.1 $-$ 3.4 $\times$ 10$^{-18}$ erg s$^{-1}$ cm$^{-2}$ arcsec$^{-2}$ per 1 arcsec$^2$ aperture (5$\sigma$) for the HeII$\lambda$1640 and CIV$\lambda$1549 lines, respectively. We do not detect extended HeII and CIV emission in any of the LABs, placing strong upper limits on the HeII/Ly$\alpha$ and CIV/Ly$\alpha$ line ratios, of 0.11 and 0.16, for the brightest two LABs in the field. We conduct detailed photoionization modeling of the expected line ratios and find that, although our data constitute the deepest ever observations of these lines, they are still not deep enough to rule out a scenario where the Ly$\alpha$ emission is powered by the ionizing luminosity of an obscured AGN. Our models can accommodate HeII/Ly$\alpha$ and CIV/Ly$\alpha$ ratios as low as $\simeq$0.05 and $\simeq$0.07 respectively, implying that one needs to reach surface brightness as low as 1 $-$ 1.5 $\times$ 10$^{-18}$ erg s$^{-1}$ cm$^{-2}$ arcsec$^{-2}$ (at 5$\sigma$) in order to rule out a photoionization scenario. These depths will be achievable with the new generation of image-slicing integral field units such as VLT/MUSE or Keck/KCWI. We also model the expected HeII/Ly$\alpha$ and CIV/Ly$\alpha$ in a different scenario, where Ly$\alpha$ emission is powered by shocks generated in a large-scale superwind, but find that our observational constraints can only be met for shock velocities $v_{\rm s} \gtrsim$ 250 km s$^{-1}$, which appear to be in conflict with recent observations of quiescent kinematics in LABs.
Article: The environments of Ly$\alpha$ blobs I: Wide-field Ly$\alpha$ imaging of TN J1338-1942, a powerful radio galaxy at $z\simeq 4.1$ associated with a giant Ly$\alpha$ nebula[Show abstract] [Hide abstract]
ABSTRACT: We present wide-field Lya imaging observations of the field around TN J1338-1942, a powerful radio galaxy associated with an extended Lya nebula (>100 kpc) at z=4.11, with Subaru Prime-focus Camera to probe the environment of the radio galaxy. We used a sample of Lya emitters (LAEs) down to the Lya luminosity of $\log(L_{\rm Lya}\rm [erg\, s^{-1}])\sim 42.8$ to measure the galaxy density of this field, calibrating by direct comparison with a control sample in a blank field taken with the same instrument. We found that the radio galaxy resides in a region with a peak overdensity of $\delta_{\rm LAE}=3.1\pm 0.5$, after being smoothed on $8\, h^{-1}$ Mpc scales on the sky and $160\, h^{-1}$ Mpc along the line of sight (both in comoving coordinates). Adjacent to this overdense region, we found a highly underdense region where virtually no LAEs are detected. We used a semi-analytical model of LAEs derived from the Millennium Simulation to compare our results with theoretical predictions. This comparison suggests that, while the density distribution of the simulation is consistent with that of the blank field, overdense regions such as the one found in the radio galaxy field are very rare, with the number density of $2\times 10^{-7}h^{3}$ Mpc$^{-3}$ (comoving), corresponding to the densest <0.1 percentile at these redshifts. We also found a difference in the Lya luminosity function in the radio galaxy field compared with the blank field: the number of bright LAEs ($\log(L_{\rm Lya}\rm [erg\, s^{-1}])<43.3$) is enhanced, while the number of fainter LAEs is relatively suppressed. These results suggest that some powerful radio galaxies associated with Lya nebulae reside in extreme overdensities on $\sim 10-20\, h^{-1}$ Mpc scales, where star-formation and AGN activities may be enhanced via more frequent galaxy mergers or higher rates of gas accretion from the surroundings.
Article: High-Resolution Submillimeter and Near-Infrared Studies of the Transition Disk around Sz 91[Show abstract] [Hide abstract]
ABSTRACT: To reveal the structures of a transition disk around a young stellar object in Lupus, Sz 91, we have performed aperture synthesis 345 GHz continuum and CO(3--2) observations with the Submillimeter Array ($\sim1\arcsec$--3$\arcsec$ resolution), and high-resolution imaging of polarized intensity at the $K_s$-band by using the HiCIAO instrument on the Subaru Telescope ($0\farcs25$ resolution). Our observations successfully resolved the inner and outer radii of the dust disk to be 65 AU and 170 AU, respectively, which indicates that Sz 91 is a transition disk source with one of the largest known inner holes. The model fitting analysis of the spectral energy distribution reveals an H$_2$ mass of $2.4\times10^{-3}$ $M_\sun$ in the cold ($T<$30 K) outer part at $65<r<170$ AU by assuming a canonical gas-to-dust mass ratio of 100, although a small amount ($>3\times10^{-9}$ $M_\sun$) of hot ($T\sim$180 K) dust possibly remains inside the inner hole of the disk. The structure of the hot component could be interpreted as either an unresolved self-luminous companion body (not directly detected in our observations) or a narrow ring inside the inner hole. Significant CO(3--2) emission with a velocity gradient along the major axis of the dust disk is concentrated on the Sz 91 position, suggesting a rotating gas disk with a radius of 420 AU. The Sz 91 disk is possibly a rare disk in an evolutionary stage immediately after the formation of protoplanets because of the large inner hole and the lower disk mass than other transition disks studied thus far.The Astrophysical Journal 02/2014; 783(2). DOI:10.1088/0004-637X/783/2/90 · 6.28 Impact Factor
Article: Clustering of extremely red objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS 1 and Subaru[Show abstract] [Hide abstract]
ABSTRACT: We measure the angular clustering of 33 415 extremely red objects (EROs) in the Elais-N1 field covering 5.33 deg2, which cover the redshift range z = 0.8 to 2. This sample was made by merging the UKIDSS Deep eXtragalactic Survey (DXS) with the optical Subaru and Pan-STARRS PS1 data sets. We confirm the existence of a clear break in the angular correlation function at ̃0.02° corresponding to 1 h-1 Mpc at z ̃ 1. We find that redder or brighter EROs are more clustered than bluer or fainter ones. Halo occupation distribution (HOD) model fits imply that the average mass of dark matter haloes which host EROs is over 1013 h-1 M☉ and that EROs have a bias ranging from 2.7 to 3.5. Compared to EROs at z ̃ 1.1, at z ̃ 1.5 EROs have a higher bias and fewer are expected to be satellite galaxies. Furthermore, EROs reside in similar dark matter haloes to those that host 1011.0 M☉ < M* < 1011.5 M☉ galaxies. We compare our new measurement and HOD fits with the predictions of the GALFORM semi-analytical galaxy formation model. Overall, the clustering predicted by GALFORM gives an encouraging match to our results. However, compared to our deductions from the measurements, GALFORM puts EROs into lower mass haloes and predicts that a larger fraction of EROs are satellite galaxies. This suggests that the treatment of gas cooling may need to be revised in the model. Our analysis illustrates the potential of clustering analyses to provide observational constraints on theoretical models of galaxy formation.Monthly Notices of the Royal Astronomical Society 01/2014; 438(1). DOI:10.1093/mnras/stt2245 · 5.23 Impact Factor
Article: Probing Intergalactic Neutral Hydrogen by High Precision Analysis of the Red Damping Wing of Gamma-Ray Burst 130606A Afterglow Spectrum at z = 5.913[Show abstract] [Hide abstract]
ABSTRACT: The unprecedentedly bright optical afterglow of GRB 130606A at a redshift close to the reionization era (z = 5.913) provides a new opportunity to probe the ionization status of intergalactic medium (IGM). Here we present a high-precision analysis of the red Ly alpha damping wing of the afterglow spectrum taken by Subaru/FOCAS during 10.4-13.2 hr after the burst. We find that the minimal model including only the baseline power-law and HI absorption in the host galaxy does not give a good fit, leaving residuals showing concave curvature in 8400-8900 A with an amplitude of about 0.6% of the flux. Such a curvature in the short wavelength range cannot be explained either by extinction at the host with standard extinction curves or by the known systematic uncertainties in the observed spectrum. The red damping wing by intervening HI gas outside the host can reduce the residual by about 3 sigma statistical significance. We find that a damped Ly alpha system is not favored as the origin of this intervening HI absorption, from the observed Ly beta and metal absorption features. Therefore absorption by diffuse IGM remains as a plausible explanation. A fit by a simple uniform IGM model requires HI neutral fraction of f_{HI} ~ 0.1-0.5 depending on the distance to the GRB host, implying high f_{HI} IGM associated with the observed dark Gunn-Peterson (GP) troughs. This gives a new evidence that the reionization is not yet complete at z ~ 6. Further investigations using more GRB afterglows to various sightlines, in comparison with realistic theoretical simulations, are desirable.Publications- Astronomical Society of Japan 12/2013; 66(3). DOI:10.1093/pasj/psu032 · 2.01 Impact Factor
Article: Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru[Show abstract] [Hide abstract]
ABSTRACT: We measure the angular clustering of 33 415 extremely red objects (EROs) in the Elais-N1 field covering 5.33 deg$^{2}$, which cover the redshift range $z=0.8$ to $2$. This sample was made by merging the UKIDSS Deep eXtragalactic Survey (DXS) with the optical Subaru and Pan-STARRS PS1 datasets. We confirm the existence of a clear break in the angular correlation function at $\sim 0.02^{\circ}$ corresponding to $1 h^{-1}$ Mpc at $z\sim1$. We find that redder or brighter EROs are more clustered than bluer or fainter ones. Halo Occupation Distribution (HOD) model fits imply that the average mass of dark matter haloes which host EROs is over $10^{13} h^{-1} M_{\odot}$ and that EROs have a bias ranging from 2.7 to 3.5. Compared to EROs at $z\sim1.1$, at $z\sim1.5$ EROs have a higher bias and fewer are expected to be satellite galaxies. Furthermore, EROs reside in similar dark matter haloes to those that host $10^{11.0} M_{\odot}<M_{*}<10^{11.5} M_{\odot}$ galaxies. We compare our new measurement and HOD fits with the predictions of the GALFORM semi-analytical galaxy formation model. Overall, the clustering predicted by GALFORM gives an encouraging match to our results. However, compared to our deductions from the measurements, GALFORM puts EROs into lower mass haloes and predicts that a larger fraction of EROs are satellite galaxies. This suggests that the treatment of gas cooling may need to be revised in the model. Our analysis illustrates the potential of clustering analyses to provide observational constraints on theoretical models of galaxy formation.
[Show abstract] [Hide abstract]
ABSTRACT: The properties of K-band selected galaxies (K_AB<24) in the z = 3.09 SSA22 protocluster field are studied. 430 galaxies at 2.6 < z_phot < 3.6 are selected as potential protocluster members in a 112 arcmin^2 area based on their photometric redshifts. We find that \approx 20% of the massive galaxies with stellar masses >10^11 M_sun at z_phot \sim 3.1 have colors consistent with those of quiescent galaxies with ages > 0.5 Gyr. This fraction increases to \approx 50% after correcting for unrelated foreground/background objects. We also find that 30% of the massive galaxies are heavily reddened dusty star-forming galaxies. Few such quiescent galaxies at similar redshifts are seen in typical survey fields. An excess surface density of 24\mu m sources at z_phot \sim 3.1 is also observed, implying the presence of dusty star-formation activity in the protocluster. Cross-correlation with the X-ray data indicates that the fraction of K-band selected protocluster galaxies hosting active galactic nuclei (AGN) is also high compared with the field. The sky distribution of the quiescent galaxies, the 24\mu m sources, and the X-ray AGNs show clustering around a density peak of z=3.1 Ly\alpha emitters (LAEs). A significant fraction of the massive galaxies have already become quiescent, while the dusty star-formation is still active in the SSA22 protocluster. These findings indicate that we are witnessing the formation epoch of massive early-type galaxies at the center of predecessors to present-day rich galaxy clusters.The Astrophysical Journal 10/2013; 778(2). DOI:10.1088/0004-637X/778/2/170 · 6.28 Impact Factor
Article: A Discovery of a Candidate Companion to a Transiting System KOI-94: A Direct Imaging Study for a Possibility of a False Positive[Show abstract] [Hide abstract]
ABSTRACT: We report a discovery of a companion candidate around one of {\it Kepler} Objects of Interest (KOIs), KOI-94, and results of our quantitative investigation of the possibility that planetary candidates around KOI-94 are false positives. KOI-94 has a planetary system in which four planetary detections have been reported by {\it Kepler}, suggesting that this system is intriguing to study the dynamical evolutions of planets. However, while two of those detections (KOI-94.01 and 03) have been made robust by previous observations, the others (KOI-94.02 and 04) are marginal detections, for which future confirmations with various techniques are required. We have conducted high-contrast direct imaging observations with Subaru/HiCIAO in $H$ band and detected a faint object located at a separation of $\sim0.6''$ from KOI-94. The object has a contrast of $\sim 1\times 10^{-3}$ in $H$ band, and corresponds to an M type star on the assumption that the object is at the same distance of KOI-94. Based on our analysis, KOI-94.02 is likely to be a real planet because of its transit depth, while KOI-94.04 can be a false positive due to the companion candidate. The success in detecting the companion candidate suggests that high-contrast direct imaging observations are important keys to examine false positives of KOIs. On the other hand, our transit light curve reanalyses lead to a better period estimate of KOI-94.04 than that on the KOI catalogue and show that the planetary candidate has the same limb darkening parameter value as the other planetary candidates in the KOI-94 system, suggesting that KOI-94.04 is also a real planet in the system.
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ABSTRACT: We carried out an imaging survey for extrasolar planets around stars in the Pleiades (125 Myr, 135 pc) in the $H$ and $K_{S}$ bands using HiCIAO combined with the adaptive optics, AO188, on the Subaru telescope. We found 13 companion candidates fainter than 14.5 mag in the $H$ band around 9 stars. Five of these 13 were confirmed to be background stars by measurement of their proper motion. One was not found in the second epoch observation, and thus was not a background or companion object. One had multi-epoch image, but the precision of its proper motion was not sufficient to conclude whether it was background object. Four other candidates are waiting for second epoch observations to determine their proper motion. Finally, the remaining 2 were confirmed to be 60 $M_{J}$ brown dwarf companions orbiting around HD 23514 (G0) and HII 1348 (K5) respectively, as had been reported in previous studies. In our observations, the average detection limit for a point source was 20.3 mag in the $H$ band beyond 1''.5 from the central star. On the basis of this detection limit, we calculated the detection efficiency to be 90% for a planet with 6 to 12 Jovian masses and a semi-major axis of 50--1000 AU. For this we extrapolated the distribution of planet mass and semi-major axis derived from RV observations and adopted the planet evolution model of Baraffe et al. (2003). As there was no detection of a planet, we estimated the frequency of such planets to be less than 17.9% ($2\sigma$) around one star of the Pleiades cluster.Publications- Astronomical Society of Japan 06/2013; 65(4). DOI:10.1093/pasj/65.4.90 · 2.01 Impact Factor
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ABSTRACT: We present near-infrared coronagraphic imaging polarimetry of RY Tau. The scattered light in the circumstellar environment was imaged at H-band at a high resolution (~0".05) for the first time, using Subaru-HiCIAO. The observed polarized intensity (PI) distribution shows a butterfly-like distribution of bright emission with an angular scale similar to the disk observed at millimeter wavelengths. This distribution is offset toward the blueshifted jet, indicating the presence of a geometrically thick disk or a remnant envelope, and therefore the earliest stage of the Class II evolutionary phase. We perform comparisons between the observed PI distribution and disk models with: (1) full radiative transfer code, using the spectral energy distribution (SED) to constrain the disk parameters; and (2) monochromatic simulations of scattered light which explore a wide range of parameters space to constrain the disk and dust parameters. We show that these models cannot consistently explain the observed PI distribution, SED, and the viewing angle inferred by millimeter interferometry. We suggest that the scattered light in the near-infrared is associated with an optically thin and geometrically thick layer above the disk surface, with the surface responsible for the infrared SED. Half of the scattered light and thermal radiation in this layer illuminates the disk surface, and this process may significantly affect the thermal structure of the disk.The Astrophysical Journal 06/2013; 772(2). DOI:10.1088/0004-637X/772/2/145 · 6.28 Impact Factor
Article: The SEEDS Direct Imaging Survey for Planets and Scattered Dust Emission in Debris Disk Systems[Show abstract] [Hide abstract]
ABSTRACT: Debris disks around young main-sequence stars often have gaps and cavities which for a long time have been interpreted as possibly being caused by planets. In recent years, several giant planet discoveries have been made in systems hosting disks of precisely this nature, further implying that interactions with planets could be a common cause of such disk structures. As part of the SEEDS high-contrast imaging survey, we are surveying a population of debris disk-hosting stars with gaps and cavities implied by their spectral energy distributions, in order to attempt to spatially resolve the disk as well as to detect any planets that may be responsible for the disk structure. Here we report on intermediate results from this survey. Five debris disks have been spatially resolved, and a number of faint point sources have been discovered, most of which have been tested for common proper motion, which in each case has excluded physical companionship with the target stars. From the detection limits of the 50 targets that have been observed, we find that beta Pic b-like planets (~10 Mjup planets around G--A-type stars) near the gap edges are less frequent than 15--30%, implying that if giant planets are the dominant cause of these wide (27 AU on average) gaps, they are generally less massive than beta Pic b.The Astrophysical Journal 06/2013; 773(1). DOI:10.1088/0004-637X/773/1/73 · 6.28 Impact Factor
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ABSTRACT: We present the first near infrared (NIR) spatially resolved images of the circumstellar transitional disk around SR21. These images were obtained with the Subaru HiCIAO camera, adaptive optics and the polarized differential imaging (PDI) technique. We resolve the disk in scattered light at H-band for stellocentric 0.1"<r<0.6" (12<r<75AU). We compare our results with previously published spatially-resolved 880 micron continuum Submillimeter Array (SMA) images that show an inner r<36AU cavity in SR21. Radiative transfer models reveal that the large disk depletion factor invoked to explain SR21's sub-mm cavity cannot be "universal" for all grain sizes. Even significantly more moderate depletions (delta=0.1, 0.01 relative to an undepleted disk) than those that reproduce the sub-mm cavity (delta~10^-6) are inconsistent with our H-band images when they are assumed to carry over to small grains, suggesting that surface grains scattering in the NIR either survive or are generated by whatever mechanism is clearing the disk midplane. In fact, the radial polarized intensity profile of our H-band observations is smooth and steeply inwardly-increasing (r^-3), with no evidence of a break at the 36AU sub-mm cavity wall. We hypothesize that this profile is dominated by an optically thin disk envelope or atmosphere component. We also discuss the compatibility of our data with the previously postulated existence of a sub-stellar companion to SR21 at r~10-20AU, and find that we can neither exclude nor verify this scenario. This study demonstrates the power of multiwavelength imaging of transitional disks to inform modeling efforts, including the debate over precisely what physical mechanism is responsible for clearing these disks of their large midplane grains.The Astrophysical Journal 02/2013; 767(1). DOI:10.1088/0004-637X/767/1/10 · 6.28 Impact Factor
Article: Polarimetric Imaging of Large Cavity Structures in the Pre-transitional Protoplanetary Disk around PDS 70: Observations of the Disk[Show abstract] [Hide abstract]
ABSTRACT: We present high-resolution H-band polarized intensity (FWHM = 0farcs1: 14 AU) and L'-band imaging data (FWHM = 0farcs11: 15 AU) of the circumstellar disk around the weak-lined T Tauri star PDS 70 in Centaurus at a radial distance of 28 AU (0farcs2) up to 210 AU (1farcs5). In both images, a giant inner gap is clearly resolved for the first time, and the radius of the gap is ~70 AU. Our data show that the geometric center of the disk shifts by ~6 AU toward the minor axis. We confirm that the brown dwarf companion candidate to the north of PDS 70 is a background star based on its proper motion. As a result of spectral energy distribution fitting by Monte Carlo radiative transfer modeling, we infer the existence of an optically thick inner disk at a few AU. Combining our observations and modeling, we classify the disk of PDS 70 as a pre-transitional disk. Furthermore, based on the analysis of L'-band imaging data, we put an upper limit of ~30 to ~50 M J on the mass of companions within the gap. Taking into account the presence of the large and sharp gap, we suggest that the gap could be formed by dynamical interactions of sub-stellar companions or multiple unseen giant planets in the gap.The Astrophysical Journal 10/2012; 775(1). DOI:10.1088/2041-8205/758/1/L19 · 6.28 Impact Factor
Article: Characterization of the distribution of the Lly\alpha emitters in the 53W002 field at z = 2.4[Show abstract] [Hide abstract]
ABSTRACT: We present the results of our wide-field narrow band imaging of the field around the radio galaxy 53W002 at z = 2.390 with Subaru/Suprime-Cam. A custom made filter NB413 centered at 4140 \AA\ with the width of 83 \AA\ is used to observe the 31' x 24' area around the radio galaxy. We detected 204 Ly\alpha emitters (LAEs) at z = 2.4 with a rest frame equivalent width larger than 25 \AA\ to the depth of 26 AB mag (in NB413). The entire LAE population in the 53W002 field has an average number density and distributions of equivalent width and size that are similar to those of other fields at z ~ 2. We identify a significant high density region (53W002F-HDR) that spreads over ~ 5' x 4' near 53W002 where the LAE number density is nearly four times as large as the average of the entire field. Using the probability distribution function of density fluctuation, we evaluate the rareness probability of the 53W002F-HDR to be 0.9^{+2.4}_{-0.62}%, which corresponds to a moderately rich structure. No notable environmental dependency at the comoving scale of 10 Mpc is found for the distributions of the Ly\alpha equivalent width and luminosity in the field. We also detected 4 Ly\alpha blobs (LABs), one of which is newly discovered. They are all found to be located in the rims of high density regions. The biased location and unique morphologies in Ly\alpha suggest that galaxy interaction play a key role in their formation.The Astrophysical Journal 09/2012; 759(2). DOI:10.1088/0004-637X/759/2/133 · 6.28 Impact Factor
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ABSTRACT: We report that HAT-P-7 has a common proper motion stellar companion. The companion is located at ∼ 3.9 arcsec to the east and estimated as an M5.5V dwarf based on its colors. We also confirm the presence of the third companion, which was first reported by Winn et al. (2009), based on long-term radial velocity measurements. We revisit the migration mechanism of HAT-P-7b given the presence of those com- panions, and propose sequential Kozai migration as a likely scenario in this system. This scenario may explain the reason for an outlier in the discussion of the spin-orbit alignment timescale for HAT-P-7b by Albrecht et al. (2012).Publications- Astronomical Society of Japan 09/2012; DOI:10.1093/pasj/64.6.L7 · 2.01 Impact Factor
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Edo, Tōkyō, Japan
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National Astronomical Observatory of Japan
Edo, Tōkyō, Japan
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RIKENВако, Saitama, Japan
Kyoto University
Kioto, Kyōto, Japan
- Department of Astronomy


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Top 5 Whitney Houston Songs
February 11, 2012 8:52 PM
Whitney Houston will always be remembered for her musical talents. Houston's career spanned decades, launching her to the top of the music world in the 80s and 90s. We look back on Whitney's life through her songs.
5. I Wanna Dance With Somebody
4. One Moment in Time
3. How Will I Know
2. Greatest Love of All
1. I Will Always Love You
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