activity
20062026
most citedThe Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey

293 citations · 1.1k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

Effects of low resolution on the column density PDF of molecular clouds

Yuping Tang, Q. Daniel Wang, Grant W. Wilson +2

Observational resolution significantly impacts the interpretation of column density probability distribution functions (N-PDFs) in molecular clouds, which are essential for underst…

astro-ph.GA2018★ 103 cited

A gravitationally unstable gas disk of a starburst galaxy 12 billion years ago

Ken-ichi Tadaki, Daisuke Iono, Min S. Yun +18

Submillimeter bright galaxies in the early Universe are vigorously forming stars at ~1000 times higher rate than the Milky Way. A large fraction of stars is formed in the central 1…

astro-ph.GA2017★ 7 cited

Early Science with the Large Millimetre Telescope: Fragmentation of molecular clumps in the Galaxy

M. Heyer, G. W. Wilson, R. Gutermuth +6

Sensitive, imaging observations of the 1.1 mm dust continuum emission from a 1 deg^2 area collected with the AzTEC bolometer camera on the Large Millimeter Telescope are presented.…

astro-ph.GA2017★ 109 cited

A dusty star-forming galaxy at z=6 revealed by strong gravitational lensing

Jorge A. Zavala, Alfredo Montaña, David H. Hughes +28

Since their discovery, submillimetre-selected galaxies (SMGs) have revolutionized the field of galaxy formation and evolution. From the hundreds of square degrees mapped at submill…

astro-ph.GA2016★ 29 cited

Asymmetric structure in Sgr A* at 3mm from closure phase measurements with VLBA, GBT and LMT

Christiaan D. Brinkerink, Cornelia Müller, Heino Falcke +19

We present the results of a closure phase analysis of 3 mm very long baseline interferometry (VLBI) measurements performed on Sagittarius A* (Sgr A*). We have analyzed observations…

astro-ph.GA2016★ 16 cited

SXDF-ALMA 2 Arcmin^2 Deep Survey: Resolving and Characterizing the Infrared Extragalactic Background Light Down to 0.5 mJy

Yuki Yamaguchi, Yoichi Tamura, Kotaro Kohno +22

We present a multi-wavelength analysis of five submillimeter sources (S_1.1mm = 0.54-2.02 mJy) that were detected during our 1.1-mm-deep continuum survey in the SXDF-UDS-CANDELS fi…

astro-ph.GA2016★ 1 cited

SXDF-UDS-CANDELS-ALMA 1.5 arcmin deep survey

K. Kohno, Y. Yamaguchi, Y. Tamura +26

We have conducted 1.1 mm ALMA observations of a contiguous or 1.5 arcmin window in the SXDF-UDS-CANDELS. We achieved a 5 sensitivity of 0.28 mJy, providi…

astro-ph.GA2015★ 46 cited

The Red Radio Ring: a gravitationally lensed hyperluminous infrared radio galaxy at z=2.553 discovered through citizen science

J. E. Geach, A. More, A. Verma +49

We report the discovery of a gravitationally lensed hyperluminous infrared galaxy (L_IR~10^13 L_sun) with strong radio emission (L_1.4GHz~10^25 W/Hz) at z=2.553. The source was ide…

astro-ph.CO2012★ 39 cited

AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts, and evidence for large-scale structure

M. J. Michałowski, J. S. Dunlop, R. J. Ivison +20

The AzTEC 1.1 mm survey of the SCUBA HAlf Degree Extragalactic Survey (SHADES) fields is the largest (0.7 deg2) blank-field millimetre-wavelength survey undertaken to date at a res…

astro-ph.CO2011★ 5 cited

AzTEC 1.1 mm Observations of the MBM12 Molecular Cloud

M. J. Kim, S. Kim, S. Youn +11

We present 1.1 mm observations of the dust continuum emission from the MBM12 high-latitude molecular cloud observed with the Astronomical Thermal Emission Camera (AzTEC) mounted on…

astro-ph.GA2011★ 13 cited

IRAS 15099-5856: Remarkable Mid-Infrared Source with Prominent Crystalline Silicate Emission Embedded in the Supernova Remnant MSH15-52

Bon-Chul Koo, Christopher F. McKee, Kyung-Won Suh +18

We report new mid-infrared observations of the remarkable object IRAS 15099-5856 using the space telescopes AKARI and Spitzer, which demonstrate the presence of prominent crystalli…

astro-ph.GA2010★ 54 cited

New Panoramic View of CO and 1.1 mm Continuum Emission in the Orion A Molecular Cloud. I. Survey Overview and Possible External Triggers of Star Formation

Yoshito Shimajiri, Ryohei Kawabe, Shigehisa Takakuwa +17

We present new, wide and deep images in the 1.1 mm continuum and the CO (=1-0) emission toward the northern part of the Orion A Giant Molecular Cloud (Orion-A GMC). The 1…

astro-ph.CO2010★ 293 cited

The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey

T. A. Marriage, V. Acquaviva, P. A. R. Ade +68

We report on twenty-three clusters detected blindly as Sunyaev-Zel'dovich (SZ) decrements in a 148 GHz, 455 square-degree map of the southern sky made with data from the Atacama Co…

astro-ph.CO2010★ 94 cited

The Atacama Cosmology Telescope: Extragalactic Sources at 148 GHz in the 2008 Survey

T. A. Marriage, J. B. Juin, Y. -T. Lin +66

We report on extragalactic sources detected in a 455 square-degree map of the southern sky made with data at a frequency of 148 GHz from the Atacama Cosmology Telescope 2008 observ…

astro-ph.CO2010★ 40 cited

The physical scale of the far-infrared emission in the most luminous submillimetre galaxies II: evidence for merger-driven star formation

J. D. Younger, G. G. Fazio, M. L. N. Ashby +11

We present high-resolution 345 GHz interferometric observations of two extreme luminous (L_{IR}>10^{13} L_sun), submillimetre-selected galaxies (SMGs) in the COSMOS field with the…

astro-ph2008★ 58 cited

Spitzer IRAC Infrared Colours of Submillimetre-bright Galaxies

Min S. Yun, I. Aretxaga, M. L. N. Ashby +11

High-redshift submillimetre-bright galaxies identified by blank field surveys at millimetre and submillimetre wavelengths appear in the region of the IRAC colour-colour diagrams pr…

astro-ph2008★ 131 cited

Spectroscopic Confirmation Of An Extreme Starburst At Redshift 4.547

Peter Capak, C. L. Carilli, N. Lee +22

We report the spectroscopic confirmation of a sub-mm galaxy (SMG) at z=4.547 with an estimated L_IR=0.5-2.0x10^13 L_sun. The spectra, mid-IR, and X-ray properties indicate the bolo…

astro-ph2006★ 12 cited

The optical performance of frequency selective bolometers

T. A. Perera, T. C. Chen, E. S. Cheng +10

Frequency Selective Bolometers (FSBs) are a new type of detector for millimeter and sub-millimeter wavelengths that are transparent to all but a narrow range of frequencies as set…