MASS OF GALAXIES AT LOW AND HIGH REDSHIFT

By J. Dunlop, R. McLure. 2003

167 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/85c7c5f0a14a8a0d18bc7b76740df65606e047bf

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Citations in the corpus

The Chandra Deep Field North Survey. XIII. 2 Ms Point-Source Catalogs (2003, background): “…of the field (including almost all of the expected area of the IRAC observations for the Great Observatories Origins Deep Survey [GOODS; e.g., Dickinson & Giavalisco 2003]) has a full-band sensitivity limit of 3 10 16 ergs cm 2 s 1, and 360 arcmin2 (i.e., 1.3 times the size of a single…”
The Observed Properties of Dark Matter on Small Spatial Scales (2007, background): “Constant anisotropy models of this type favor rather shallow halo inner mass profiles with / r 0:5 (Magorrian 2003; Koch et al. 2007b).”
The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Deﬁnition and Goals (2012, background): “1 Infrared Processing and Analysis Center/Spitzer Science Center, California Institute of Technology, Mail Code 220-6, Pasadena, CA 91125, USA 2 National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA 3 Department of Physics and Astronomy, University of Sussex,…”
Optical Selection of Star-forming Galaxies at Redshifts 1 < z < 3 (2004, methodology): “In one field, the HDF-North, a publicly released z image from the GOODS survey (Dickinson & Giavalisco 2002) gave us photometric coverage of the entire optical window.”
Lyman break galaxies and the star formation rate of the Universe at z≈ 6 (2003, unknown): “…data from the Advanced Camera for Surveys (ACS, Ford et al. 2002) on HST, released as part of the Great Observatories Origins Deep Survey (GOODS – Dickinson & Giavalisco 2002⋆) programme, is of sufficient depth and volume to detect very high redshift galaxies, and that colour selection should…”
The Mass Discrepancy-Acceleration Relation: Disk Mass and the Dark Matter Distribution (2004, background): “It is straightforward to derive equivalent limits for other choices of halo models, but most other models resemble one of these two in their essential features.”
The Extended Chandra Deep Field-South Survey: Chandra Point-Source Catalogs (2005, background): “Subject headinggs: cosmology: observations — diffuse radiation — galaxies: active — surveys — X-rays Online material: color figure, machine-readable tables”
The Great Observatories Origins Deep Survey VLT/FORS2 Spectroscopy in the GOODS-South Field: Part II (2006, methodology): “For an overview of GOODS, see Dickinson et al. (2003), Renzini et al. (2003) and Giavalisco et al. (2004a). This is the second paper in a series presenting the results of the GOODS spectroscopic program carried out with the VLT/FORS2 spectrograph.”