301 citations · 940 across the 15 of their papers we have counts for
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Simultaneous Measurements of Star Formation and Supermassive Black Hole Growth in Galaxies
Alexandra Pope, Lee Armus, Eric Murphy +29
Galaxies grow their supermassive black holes in concert with their stars, although the relationship between these major galactic components is poorly understood. Observations of th…
Cosmic Dawn and Reionization: Astrophysics in the Final Frontier
Asantha Cooray, James Aguirre, Yacine Ali-Haimoud +71
The cosmic dawn and epoch of reionization mark the time period in the universe when stars, galaxies, and blackhole seeds first formed and the intergalactic medium changed from neut…
Probing the High-Redshift Universe with SPICA: Toward the Epoch of Reionization and Beyond
E. Egami, S. Gallerani, R. Schneider +36
With the recent discovery of a dozen dusty star-forming galaxies and around 30 quasars at z>5 that are hyper-luminous in the infrared ( L, where $μ…
Investigating overdensities around z>6 galaxies through ALMA observations of [CII]
Tim B. Miller, Scott C. Chapman, Christopher C. Hayward +4
We present a search for companion [CII] emitters to known luminous sources at z in deep, archival ALMA observations. The observations are deep enough to detect sources…
Shock Excited Molecules in NGC 1266: ULIRG conditions at the center of a Bulge Dominated Galaxy
E. W. Pellegrini, J. D. Smith, M. G. Wolfire +28
We investigate the far infrared spectrum of NGC 1266, a S0 galaxy that contains a massive reservoir of highly excited molecular gas. Using the SPIRE-FTS, we detect the CO la…
Herschel-SPIRE Imaging Spectroscopy of Molecular Gas in M82
J. Kamenetzky, J. Glenn, N. Rangwala +14
We present new Herschel-SPIRE imaging spectroscopy (194-671 microns) of the bright starburst galaxy M82. Covering the CO ladder from J=4-3 to J=13-12, spectra were obtained at mult…
The central region of spiral galaxies as seen by Herschel. M81, M99 and M100
M. Sauvage, N. Sacchi, G. J. Bendo +57
With appropriate spatial resolution, images of spiral galaxies in thermal infrared (~10 micron and beyond) often reveal a bright central component, distinct from the stellar bulge,…