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High resolution imaging of molecular line emission from high redshift QSOs
C. L. Carilli, K. Kohno, R. Kawabe +6
We present moderate (1'') and high resolution (0.2'') observations of the CO(2-1) emission at 43 GHz, and radio continuum emission at 1.47 GHz, from the z=4.7 QSO BRI 1202-0725 and…
Radio-to-FIR Spectral Energy Distribution and Photometric Redshifts for Dusty Starburst Galaxies
Min S. Yun, C. L. Carilli
As a logical next step in improving the radio-to-submm spectral index as a redshift indicator (Carilli & Yun 1999), we have investigated a technique of using the entire radio-to-FI…
Discovery of Molecular Gas in the Outflow and Tidal Arms around M82
Christopher L. Taylor, Fabian Walter, Min S. Yun
We present the first fully sampled map of 12CO (1-0) emission from M82 covering the entire galaxy. Our map contains a 12 x 15 kpc^2 area. We find that extraplanar CO emission, prev…
Where is the Neutral Atomic Gas in Hickson Groups?
L. Verdes-Montenegro, M. S. Yun, B. A. Williams +3
We have analyzed the total HI contents of 72 Hickson compact groups of galaxies (HCGs) and the detailed spatial distributions and kinematics of HI within a subset of 16 groups usin…
A 250 GHz Survey of High Redshift QSOs from the Sloan Digital Sky Survey
C. L. Carilli, F. Bertoldi, M. Rupen +8
We present observations at 250 GHz (1.2 mm), 43 GHz, and 1.4 GHz of a sample of 41 QSOs at z > 3.7 found in the Sloan Digital Sky Survey. We detect 16 sources with a 250 GHz flux d…