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The ALPINE-ALMA [C II] Survey: [C II] 158micron Emission Line Luminosity Functions at z∼4−6
(American Astronomical Society, 2020)
We present the [C II] 158 μm line luminosity functions (LFs) at z ~ 4–6 using the ALMA observations of 118 sources, which are selected to have UV luminosity M1500Å < −20.2 and optical spectroscopic redshifts in COSMOS and ...
Star formation in AGN hosts in GOODS-N
(2010)
Sensitive Herschel far-infrared observations can break degeneracies that were inherent to previous studies of star formation in high-z AGN hosts. Combining PACS 100 and 160um observations of the GOODS-N field with 2Msec ...
Future virialized structures: an analysis of superstructures in the SDSS-DR7
(2011)
We construct catalogues of present superstructures that, according to a LCDM scenario, will evolve into isolated, virialized structures in the future. We use a smoothed luminosity density map derived from galaxies in ...
Low X-ray luminosity galaxy clusters – II. Optical properties and morphological content at 0.18 < z < 0.70
(Oxford University Press, 2013-12)
This is the second of a series of papers on low X-ray luminosity galaxy clusters, in which we present the r′, g′ and i′ photometry obtained with Gemini Multi-Object Spectrograph IMAGE at Gemini North and South telescopes ...
White dwarf luminosity and mass functions from sloan digital sky survey spectra
(IOP Publishing, 2008-01)
We present the first phase in our ongoing work to use Sloan Digital Sky Survey (SDSS) data to create separate white dwarf (WD) luminosity functions (LFs) for two or more different mass ranges. In this paper, we determine ...
C-GOALS II. Chandra observations of the lower luminosity sample of nearby luminous infrared galaxies in GOALS
(2018)
We analyze Chandra X-ray observatory data for a sample of 63 luminous infrared galaxies (LIRGs), sampling the lower-infrared luminosity range of the Great Observatories All-Sky LIRG survey (GOALS), which includes the most ...