activity
19992021
most citedThe Evolution of Dust in the Early Universe with Applications to the Galaxy SDSS J1148+5251

256 citations · 1.6k across the 32 of their papers we have counts for

collaborators
Showing 2019Show all

7 papers · 1 filter

astro-ph.SR201925 cited

Final Spitzer IRAC Observations of the Rise and Fall of SN 1987A

Richard G. Arendt, Eli Dwek, Patrice Bouchet +4

Spitzer's final Infrared Array Camera (IRAC) observations of SN 1987A show the 3.6 and 4.5 m emission from the equatorial ring (ER) continues a period of steady decline. Deconvo…

astro-ph.HE2019100 cited

High angular resolution ALMA images of dust and molecules in the SN 1987A ejecta

Phil Cigan, Mikako Matsuura, Haley L. Gomez +23

We present high angular resolution (~80 mas) ALMA continuum images of the SN 1987A system, together with CO =2 1, =6 5, and SiO =5 $\!\…

astro-ph.GA201921 cited

Dust formation in AGN winds

Arkaprabha Sarangi, Eli Dwek, Demos Kazanas

Infrared observations of active galactic nucleus (AGN) reveal emission from the putative dusty circumnuclear 'torus' invoked by AGN unification, that is heated up by radiation from…

astro-ph.GA2019

2 mm GISMO Observations of the Galactic Center. II. A Nonthermal Filament in the Radio Arc and Compact Sources

Johannes Staguhn, Richard G. Arendt, Eli Dwek +5

We have used the Goddard IRAM 2-Millimeter Observer (GISMO) with the 30 m IRAM telescope to carry out a 2 mm survey of the Galaxy's central molecular zone (CMZ). These observations…

astro-ph.GA2019

2 mm GISMO Observations of the Galactic Center. I. Dust Emission

Richard G. Arendt, Johannes Staguhn, Eli Dwek +5

The Central Molecular Zone (CMZ), covering the inner ~1 of the Galactic plane has been mapped at 2 mm using the GISMO bolometric camera on the 30 m IRAM telescope. The $21'…

astro-ph.CO201928 cited

Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations

N. Odegard, J. L. Weiland, D. J. Fixsen +4

New determinations are presented of the cosmic infrared background monopole brightness in the Planck HFI bands from 100 GHz to 857 GHz. Planck was not designed to measure the monop…