activity
20092022
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 1.7k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2022★ 20 cited

PASSAGES: The Large Millimeter Telescope and ALMA Observations of Extremely Luminous High Redshift Galaxies Identified by the Planck

Derek A. Berman, Min S. Yun, K. C. Harrington +20

The Planck All-Sky Survey to Analyze Gravitationally-lensed Extreme Starbursts (PASSAGES) project aims to identify a population of extremely luminous galaxies using the Planck All-…

astro-ph.IM2018★ 39 cited

Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond

J. E. Austermann, J. A. Beall, S. A. Bryan +10

Microwave Kinetic Inductance Detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for next-generation experi…

astro-ph.GA2017★ 101 cited

The unexpectedly large dust and gas content of quiescent galaxies at z>1.4

R. Gobat, E. Daddi, G. Magdis +13

Early type galaxies (ETG) contain most of the stars present in the local Universe and, above a stellar mass of ~5e10 Msun, vastly outnumber spiral galaxies like the Milky Way. Thes…

astro-ph.GA2016★ 11 cited

Continuum Observations of M51 and M83 at 1.1 mm with AzTEC

W. F. Wall, I. Puerari, R. Tilanus +9

We observed the spiral galaxies M51 and M83 at 20" spatial resolution with the bolometer array AzTEC on the JCMT in the 1.1mm continuum, recovering the extended emission out to…

astro-ph.CO2014★ 60 cited

AzTEC/ASTE 1.1 mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimeter galaxies

H. Umehata, Y. Tamura, K. Kohno +22

We present the results from a 1.1 mm imaging survey of the SSA22 field, known for having an overdensity of z=3.1 Lyman-alpha emitting galaxies (LAEs), taken with the AzTEC camera o…

astro-ph.IM2013★ 2 cited

An Efficient and Optimal Filter for Identifying Point Sources in Millimeter/Sub-Millimeter Wavelength Sky Maps

T. A. Perera, G. W. Wilson, K. S. Scott +3

A new technique for reliably identifying point sources in millimeter/sub-millimeter wavelength maps is presented. This method accounts for the frequency dependence of noise in the…

astro-ph.CO2012★ 90 cited

The source counts of submillimetre galaxies detected at 1.1 mm

K. S. Scott, G. W. Wilson, I. Aretxaga +21

The source counts of galaxies discovered at sub-millimetre and millimetre wavelengths provide important information on the evolution of infrared-bright galaxies. We combine the dat…

astro-ph.CO2011★ 1.1k cited

GOODS-Herschel: an infrared main sequence for star-forming galaxies

D. Elbaz, M. Dickinson, H. S. Hwang +52

We present the deepest far-IR observations obtained with Herschel and examine the 3-500um SEDs of galaxies at 0<z<2.5, supplemented by a local reference sample from IRAS, ISO, Spit…

astro-ph.CO2011★ 47 cited

The redshift and nature of AzTEC/COSMOS 1: A starburst galaxy at z=4.6

V. Smolcic, P. Capak, O. Ilbert +36

Based on broad/narrow-band photometry and Keck DEIMOS spectroscopy we report a redshift of z=4.64-0.08+0.06 for AzTEC/COSMOS 1, the brightest sub-mm galaxy in the AzTEC/COSMOS fiel…

astro-ph.CO2010★ 46 cited

Deep 1.1 mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts

K. S. Scott, M. S. Yun, G. W. Wilson +20

[Abridged] We present the first results from a 1.1 mm confusion-limited map of the GOODS-S field taken with AzTEC on the ASTE telescope. We imaged a 270 sq. arcmin field to a 1σdep…

astro-ph.CO2010★ 28 cited

Unveiling the Nature of Submillimeter Galaxy SXDF850.6

B. Hatsukade, D. Iono, T. Yoshikawa +22

We present an 880 micron Submillimeter Array (SMA) detection of the submillimeter galaxy SXDF850.6. SXDF850.6 is a bright source (S(850 micron) = 8 mJy) detected in the SCUBA Half…

astro-ph.CO2009★ 93 cited

The Atacama Cosmology Telescope (ACT): Beam Profiles and First SZ Cluster Maps

A. D. Hincks, V. Acquaviva, P. Ade +69

The Atacama Cosmology Telescope (ACT) is currently observing the cosmic microwave background with arcminute resolution at 148 GHz, 218 GHz, and 277 GHz. In this paper, we present A…