activity
20032009
most cited350 Micron Dust Emission from High Redshift Quasars

343 citations · 942 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2009

A complete view of galaxy evolution: panchromatic luminosity functions and the generation of metals

Andrew W. Blain, Lee Armus, Frank Bertoldi +13

When and how did galaxies form and their metals accumulate? Over the last decade, this has moved from an archeological question to a live investigation: there is now a broad pictur…

astro-ph200744 cited

SHARC-II 350 micron Observations of Thermal Emission from Warm Dust in z>=5 Quasars

Ran Wang, Jeff Wagg, Chris L. Carilli +10

We present observations of four z>= SDSS quasars at 350 micron with the SHARC-II bolometer camera on the Caltech Submillimeter Observatory. These are among the deepest observations…

astro-ph2007118 cited

Simultaneous Chandra, CSO and VLA Observations of Sgr A*: The Nature of Flaring Activity

F. Yusef-Zadeh, M. Wardle, C. Heinke +4

Sgr A*, the massive black hole at the center of the Galaxy, varies in radio through X-ray emission on hourly time scales. The flare activity is thought to arise from the innermost…

astro-ph20061 cited

Flaring Activity of Sgr A*: Expanding Hot Blobs

F. Yusef-Zadeh, M. Wardle, D. A. Roberts +5

Sgr A* is considered to be a massive black hole at the Galactic center and is known to be variable in radio, millimeter, near-IR and X-rays. Recent multi-wavelength observing campa…

astro-ph200631 cited

Images of Vega Dust Ring at 350 and 450 microns: New Clues to the Trapping of Multiple-Sized Dust Particles in Planetary Resonances

K. A. Marsh, C. D. Dowell, T. Velusamy +2

We have used the SHARC II camera at Caltech Submillimeter Observatory to make 350 and 450 micron images of the Vega dust disk at spatial resolutions (FWHM) of 9.7" and 11.1", respe…

astro-ph200668 cited

The Robinson Gravitational Wave Background Telescope (BICEP): a bolometric large angular scale CMB polarimeter

K. W. Yoon, P. A. R. Ade, D. Barkats +24

The Robinson Telescope (BICEP) is a ground-based millimeter-wave bolometric array designed to study the polarization of the cosmic microwave background radiation (CMB) and galactic…