56 citations · 280 across the 8 of their papers we have counts for
8 papers
A Diverse Population of z ~ 2 ULIRGs Revealed by JWST Imaging
J. -S. Huang, Zi-Jian Li, Cheng Cheng +12
Four ultra-luminous infrared galaxies (ULIRGs) observed with JWST/NIRcam in the Cosmos Evolution Early Release Science program offer an unbiased preview of the ULIRG po…
A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
X. W. Shu, Y. Q. Xue, D. Z. Liu +10
We present a multiwavelength study of an atypical submillimeter galaxy in the GOODS-North field, with the aim to understand its physical properties of stellar and dust emission, as…
An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115
J. M. Simpson, Ian Smail, Wei-Hao Wang +28
The identification of high-redshift massive galaxies with old stellar populations may pose challenges to some models of galaxy formation. However, to securely classify a galaxy as…
AGN-Host Connection at 0.5 < z < 2.5: A rapid evolution of AGN fraction in red galaxies during the last 10 Gyr
Tao Wang, D. Elbaz, D. M. Alexander +13
We explore the dependence of the incidence of moderate-luminosity ( erg s) AGNs and the distribution of their accretion rates on host color at 0.5 <…
Multi-Wavelength Study of a Complete IRAC 3.6micron-Selected Galaxy Sample: a Fair Census of Red and Blue Populations at Redshifts 0.4-1
J. -S. Huang, S. M. Faber, C. N. A. Willmer +14
We present a multi-wavelength study of a 3.6 m-selected galaxy sample in the Extended Groth strip. The sample is complete for galaxies with stellar mass \Msun and re…
Four IRAC Sources with an Extremely Red H-[3.6] Color: Passive or Dusty Galaxies at z>4.5?
J. -S. Huang, X. Z. Zheng, D. Rigopoulou +3
We report detection of four IRAC sources in the GOODS-South field with an extremely red color of H[3.6]4.5. The four sources are not detected in the deep HST WFC3 H-band imag…
Observational constraints on the co-evolution of supermassive black holes and galaxies
X. Z. Zheng, E. F. Bell, R. S. Somerville +6
The star formation rate (SFR) and black hole accretion rate (BHAR) functions are measured to be proportional to each other at z < ~3. This close correspondence between SF and BHA w…
A LABOCA survey of the Extended Chandra Deep Field South - submillimeter properties of near-IR selected galaxies
T. R. Greve, A. Weiss, F. Walter +25
Using the 330hr ESO-MPG 870-micron survey of the Extended Chandra Deep Field South (ECDF-S) obtained with the Large Apex BOlometer CAmera (LABOCA) on the Atacama Pathfinder EXperim…