American Astronomical Society Meeting Abstracts

By T. D. Boer, E. Tolstoy, V. Hill, A. Saha, Kirsty Olsen, E. Starkenburg, M. Irwin, G. Battaglia. 2012

192 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/31e68f1e0c5ab9a8732eef6377bc25a8828d0b60

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Citations in the corpus

LOFAR 150-MHz observations of the Boötes field: catalogue and source counts (2016, methodology): “Radio observations have been carried out at 153 MHz with the GMRT, both as a single deep 10 deg2 pointing (Intema et al. 2011) and as a seven-pointing 30 deg2 mosaic (Williams, Intema & Röttgering 2013).”
J-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey (2014, background): “Such a post-tidal disruption event by a GC black hole is believed to have been observed in a GC near the Fornax Cluster elliptical galaxy NGC 1399 that harbors the luminous X-ray source CXO J033831.8–352604. Irwin et al. (2010) detected strong [N II] and [O III] emission lines in the optical spectru”
Reionization and the Cosmic Dawn with the Square Kilometre Array (2012, methodology): “…the Long Wavelength Array (LWA) in beam forming mode (Bowman priv. comm.), observations with the Large-aperture Experiment to detect the Dark Ages (LEDA, Greenhill & Bernardi 2012) and Dark Ages Radio Explorer (DARE, Burns et al. 2012; Harker et al. 2012) - a proposed single dipole space mission.”
SUBMILLIMETER GALAXIES AS PROGENITORS OF COMPACT QUIESCENT GALAXIES (2014, background): “This is a factor of > 3 larger than the observed average SFR in star-forming Lyman break galaxies (LBGs) at z > 3 (Carilli et al. 2008). Furthermore, the space density of z ∼ 2 quiescent galaxies with logM∗/M > 11, is 5, 10 and > 100 times larger than that of similar mass LBGs at z=4,5 and 6 respect”