activity
20042008
most citedThe AzTEC mm-Wavelength Camera

161 citations · 181 across the 3 of their papers we have counts for

collaborators
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7 papers · 1 filter

astro-ph20082 cited

Tracing star formation in galaxies with molecular line and continuum observations

K. Kohno, K. Muraoka, B. Hatsukade +14

We report our recent progress on extragalactic spectroscopic and continuum observations, including HCN(J=1-0), HCO(J=1-0), and CN(N=1-0) imaging surveys of local Seyfert and st…

astro-ph2008161 cited

The AzTEC mm-Wavelength Camera

G. W. Wilson, J. E. Austermann, T. A. Perera +13

AzTEC is a mm-wavelength bolometric camera utilizing 144 silicon nitride micromesh detectors. Herein we describe the AzTEC instrument architecture and its use as an astronomical in…

astro-ph200618 cited

AEGIS: A Panchromatic Study of IRAC-selected Extremely Red Objects with Confirmed Spectroscopic Redshifts

G. Wilson, J. S. Huang, G. G. Fazio +17

We study 87 Extremely Red Objects (EROs), selected both to have color redder than R-[3.6] = 4.0, and to have confirmed spectroscopic redshifts. Together, these two constraints resu…

astro-ph2004

In-flight performance and calibration of the Infrared Array Camera (IRAC) for the Spitzer Space Telescope

J. L. Hora, the IRAC team

The Infrared Array Camera (IRAC) is one of three focal plane instruments on board the Spitzer Space Telescope. IRAC is a four-channel camera that obtains simultaneous broad-band im…

astro-ph2004

The nature of luminous X-ray sources with mid-infrared counterparts

A. Alonso-Herrero, P. G. Perez-Gonzalez, J. Rigby +28

We investigate the luminous X-ray sources in the Lockman Hole (LH) and the Extended Groth Strip (EGS) detected at 24microns using MIPS and also with IRAC on board Spitzer. We assem…

astro-ph2004

Identification of luminous infrared galaxies at 1<z<2.5

E. Le Floc'h, P. G. Perez-Gonzalez, G. H. Rieke +24

We present preliminary results on 24micron detections of luminous infrared galaxies at z>1 with the Multiband Imaging Photometer for Spitzer (MIPS). Observations were performed in…