385 citations · 789 across the 13 of their papers we have counts for
8 papers · 1 filter
UV-FIR SED modeling of AGN in IR-luminous galaxies up to z~2.5: Understanding the effects of torus models
Alyssa D. Sokol, M. Yun, A. Pope +2
UV-FIR SED modeling is an effective way to disentangle emission between star formation (SF) and active galactic nuclei (AGN) in galaxies; however, this approach becomes uncertain f…
Disturbed, diffuse, or just missing? A global study of the HI content of Hickson Compact Groups
M. G. Jones, L. Verdes-Montenegro, J. Moldon +11
Hickson Compact Groups (HCGs) are dense configurations of 4 to 10 galaxies, whose HI (neutral gas) morphology appears to follow an evolutionary sequence of three phases, with gas i…
A 0.6 Mpc HI Structure Associated with Stephan's Quintet
C. K. Xu, C. Cheng, P. N. Appleton +8
Stephan's Quintet (SQ, distance=856 Mpc) is unique among compact groups of galaxies. Observations have previously shown that interactions between multiple members, including a…
Early Science with the Large Millimeter Telescope: a 1.1 mm AzTEC Survey of Red- dusty star-forming galaxies
A. Montaña, J. A. Zavala, I. Aretxaga +32
We present LMT/AzTEC 1.1mm observations of luminous high-redshift dusty star-forming galaxy candidates from the sq.deg -ATLAS survey, selected on the…
Evolution of compact groups from intermediate to final stages: A case study of the HI content of HCG 16
Michael G. Jones, Lourdes Verdes-Montenegro, Ancor Damas-Segovia +13
Hickson Compact Group (HCG) 16 is a prototypical compact group of galaxies, apparently in an intermediate stage of evolution, where its galaxies are losing gas to the intra-group m…
A deep ALMA image of the Hubble Ultra Deep Field
J. S. Dunlop, R. J. McLure, A. D. Biggs +33
We present the results of the first, deep ALMA imaging covering the full 4.5 sq arcmin of the Hubble Ultra Deep Field (HUDF) as previously imaged with WFC3/IR on HST. Using a mosai…
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…
ALMA Deep Field in SSA22: A concentration of dusty starbursts in a z=3.09 protocluster core
H. Umehata, Y. Tamura, K. Kohno +20
We report the results of mapping at 1.1~mm with the Atacama Large Millimeter/submillimeter Array (ALMA) toward the central region of the SS…