Results 71 to 80 of about 10,586,291 (388)
The Luminosity Function of ω Centauri [PDF]
Deep HST-WFPC2 observations of the stellar population in the globular cluster Omega Cen (NGC 5139) have been used to measure the luminosity function of main sequence stars at the low-mass end. Two fields have been investigated, located respectively ~4.6' and ~7' away from the cluster center, or near the half-light radius of this cluster (~4.8').
openaire +3 more sources
THE LOCAL [C ii] 158 μm EMISSION LINE LUMINOSITY FUNCTION [PDF]
We present, for the first time, the local [C ii] 158 μm emission line luminosity function measured using a sample of more than 500 galaxies from the Revised Bright Galaxy Sample. [C ii] luminosities are measured from the Herschel PACS observations of the
S. Hemmati+6 more
semanticscholar +1 more source
Modeling the Near-Infrared Luminosity Functions of Young Stellar Clusters [PDF]
We present the results of numerical experiments designed to evaluate the usefulness of near-infrared luminosity functions for constraining the Initial Mass Function (IMF) of young stellar populations.
August A. Muench+16 more
core +3 more sources
The galaxy UV luminosity function at z≃ 2–4; new results on faint-end slope and the evolution of luminosity density [PDF]
We present a new, robust measurement of the evolving rest-frame ultraviolet (UV) galaxy luminosity function (LF) over the key redshift range from z ≃ 2 to z ≃ 4.
S. Parsa+3 more
semanticscholar +1 more source
The overdensities of galaxy environments as a function of luminosity and color [PDF]
We study the mean environments of galaxies in the Sloan Digital Sky Survey as a function of rest-frame luminosity and color. Overdensities in galaxy number are estimated in $8 h^{-1} \mathrm{Mpc}$ and $1 h^{-1} \mathrm{Mpc}$ spheres centered on $125,000$
Daniel J. Eisenstein+16 more
core +2 more sources
General Physical Properties of Gamma-Ray-emitting Radio Galaxies
We study the radio galaxies with known redshifts detected by the Fermi satellite after 10 yr of data (4FGL-DR2). We use a one-zone leptonic model to fit the quasi-simultaneous multiwavelength data of these radio galaxies and study the distributions of ...
Yongyun Chen+6 more
doaj +1 more source
Estimating galaxy luminosity functions. [PDF]
29 pages, uses AASTeX 4.0 macros. Includes 6 tables and 8 Postscript figures.
openaire +4 more sources
Galaxy Luminosity Function in Groups [PDF]
Accepted for publication in ApJ, 5 pages including 3 ...
Carlos Valotto+2 more
openaire +3 more sources
Constraining the AGN Luminosity Function from JWST with the X-Ray Background
We predict the X-ray background (XRB) expected from the population of quasars detected by the James Webb Space Telescope spectroscopic surveys over the redshift range z ∼ 4–7.
Hamsa Padmanabhan, Abraham Loeb
doaj +1 more source
The Planetary Nebula Luminosity Function in the Era of Precision Cosmology
One of the great surprises of the late 1980s was the discovery that the [O III] λ5007 planetary nebula luminosity function (PNLF) could be used as a precision extragalactic standard candle.
Robin Ciardullo, Robin Ciardullo
doaj +1 more source