385 citations · 789 across the 13 of their papers we have counts for
13 papers
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…
CHILES VII: Deep Imaging for the CHILES project, a SKA prototype
R. Dodson, E. Momjian, D. J. Pisano +16
Radio Astronomy is undergoing a renaissance, as the next-generation of instruments provides a massive leap forward in collecting area and therefore raw sensitivity. However, to ach…
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…
The Pulsar Search Collaboratory: Discovery and Timing of Five New Pulsars
R. Rosen, J. Swiggum, M. A. McLaughlin +68
We present the discovery and timing solutions of five new pulsars by students involved in the Pulsar Search Collaboratory (PSC), a NSF-funded joint program between the National Rad…
Submillimeter Array Identification of the Millimeter-Selected Galaxy SSA22-AzTEC1: A Protoquasar in a Protocluster?
Y. Tamura, D. Iono, D. J. Wilner +19
We present results from Submillimeter Array (SMA) 860-micron sub-arcsec astrometry and multiwavelength observations of the brightest millimeter (S_1.1mm = 8.4 mJy) source, SSA22-Az…
The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light
S. Serjeant, M. Negrello, C. Pearson +22
We present a comparison of the SCUBA Half Degree Extragalactic Survey (SHADES) at 450, 850 and 1100 microns with deep guaranteed time 15 microns AKARI FU-HYU survey data and Spitze…
The Canada-UK Deep Submillimeter Survey VI: The 3-Hour Field
T. M. A. Webb, S. A. Eales, S. J. Lilly +5
We present the complete submillimeter data for the Canada-UK Deep Submillimeter Survey (CUDSS) 3-hour field. The obeservations were taken with the Submillimeter Common-User Bolomet…