Results 21 to 30 of about 10,586,291 (388)

The subdwarf luminosity function [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2003
Using data from the Sloan Digital Sky Survey Early Data Release and SuperCOSMOS Sky Survey scans of POSS-I plates we identify a sample of 2600 subdwarfs using reduced proper motion methods and strict selection criteria. This forms one of the largest and most reliable samples of candidate subdwarfs known, and enables us to determine accurate luminosity ...
Andrew Digby   +4 more
openaire   +4 more sources

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6 [PDF]

open access: yesAstrophysical Journal, 2018
We present new measurements of the quasar luminosity function (LF) at z ∼ 6 over an unprecedentedly wide range of the rest-frame ultraviolet luminosity M1450 from −30 to −22 mag.
Y. Matsuoka   +46 more
semanticscholar   +1 more source

Luminosity function of clusters of galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2001
15 pages, 14 figures, 4 tables; uses subfigure.sty; accepted for publication in Astronomy and ...
PAOLILLO, MAURIZIO   +7 more
openaire   +7 more sources

Evolution of the AGN UV luminosity function from redshift 7.5 [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
Determinations of the ultraviolet (UV) luminosity function of active galactic nuclei (AGN) at high redshifts are important for constraining the AGN contribution to reionization and understanding the growth of supermassive black holes.
Girish Kulkarni, G. Worseck, J. Hennawi
semanticscholar   +1 more source

COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe [PDF]

open access: yesAstrophysical Journal, 2018
We report the first detailed measurement of the shape of the CO luminosity function at high redshift, based on >320 hr of the NSF’s Karl G. Jansky Very Large Array (VLA) observations over an area of ∼60 arcmin2 taken as part of the CO Luminosity Density ...
D. Riechers   +34 more
semanticscholar   +1 more source

The Hα Luminosity Function of Galaxies at z ∼ 4.5

open access: yesThe Astrophysical Journal, 2023
We present the H α luminosity function (LF) derived from a large sample of Lyman break galaxies at z ∼ 4.5 over the GOODS-South and North fields.
Victoria Bollo   +7 more
doaj   +1 more source

Correlation function of the luminosity distances [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2017
We present the correlation function of the luminosity distances in a flat $ $CDM universe. Decomposing the luminosity distance fluctuation into the velocity, the gravitational potential, and the lensing contributions, we study their individual contributions to the correlation function. The lensing contribution is important at large redshift ($z\gtrsim
Biern, Sang Gyu, Yoo, Jaiyul
openaire   +4 more sources

Joint Power Spectrum and Voxel Intensity Distribution Forecast on the CO Luminosity Function with COMAP [PDF]

open access: yesAstrophysical Journal, 2018
We develop a framework for joint constraints on the CO luminosity function based on power spectra (PS) and voxel intensity distributions (VID) and apply this to simulations of CO Mapping Array Pathfinder (COMAP), a CO intensity mapping experiment.
H. Ihle   +14 more
semanticscholar   +1 more source

The Imprint of Cosmic Reionization on the Luminosity Function of Galaxies [PDF]

open access: yesAstrophysical Journal, 2018
The (re)ionization of hydrogen in the early universe has a profound effect on the formation of the first galaxies: by raising the gas temperature and pressure, it prevents gas from cooling into small halos, thus affecting the abundance of present-day ...
S. Bose, A. Deason, C. Frenk
semanticscholar   +1 more source

Galactic Model Parameters and Spatial Density of Cataclysmic Variables in the Gaia Era: New Constraints on Population Models

open access: yesThe Astronomical Journal, 2023
The spatial distribution, Galactic model parameters, and luminosity function of cataclysmic variables (CVs) are established using reestimated trigonometric parallaxes from Gaia DR3.
Remziye Canbay   +3 more
doaj   +1 more source

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