Results 31 to 40 of about 10,786,884 (386)
The Faint End of the Centaurus A Satellite Luminosity Function [PDF]
The Panoramic Imaging Survey of Centaurus and Sculptor (PISCeS) is constructing a wide-field map of the resolved stellar populations in the extended halos of these two nearby, prominent galaxies.
D. Crnojevi'c +46 more
semanticscholar +1 more source
Luminosity Function of the Perigalactocentric Region [PDF]
We present H and K photometry of 42,000 stars in an area of 250 arcmin$^{2}$ centered on the Galactic center. We use the photometry to construct a dereddened K band luminosity function (LF) for this region, excluding the excessively crowded inner 2' of ...
DePoy, D. L. +2 more
core +2 more sources
EVOLUTION OF THE Hα LUMINOSITY FUNCTION [PDF]
26 pages, 23 figures, submitted to ApJ; version with high resolution figures available at http://www.cfa.harvard.edu/~ewestra/publications/
Westra, Eduard +4 more
openaire +2 more sources
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
Luminosity function of clusters of galaxies [PDF]
15 pages, 14 figures, 4 tables; uses subfigure.sty; accepted for publication in Astronomy and ...
PAOLILLO, MAURIZIO +7 more
openaire +5 more sources
We present a novel fully Bayesian analysis to constrain short gamma-ray burst (sGRB) jet structures associated with cocoon, wide-angle, and simple top-hat jet models, as well as the binary neutron star (BNS) merger rate.
Fergus Hayes +5 more
doaj +1 more source
Axions and the luminosity function of white dwarfs: the thin and thick discs, and the halo [PDF]
The evolution of white dwarfs is a simple gravothermal process of cooling. Since the shape of their luminosity function is sensitive to the characteristic cooling time, it is possible to use its slope to test the existence of additional sources or sinks ...
J. Isern +4 more
semanticscholar +1 more source
Pure Spectroscopic Constraints on UV Luminosity Functions and Cosmic Star Formation History from 25 Galaxies at z spec = 8.61–13.20 Confirmed with JWST/NIRSpec [PDF]
We present pure spectroscopic constraints on the UV luminosity functions and cosmic star formation rate (SFR) densities from 25 galaxies at z spec = 8.61–13.20. By reducing the JWST/NIRSpec spectra taken in multiple programs of Early Release Observation,
Y. Harikane +7 more
semanticscholar +1 more source
Padé Approximant and Minimax Rational Approximation in Standard Cosmology
The luminosity distance in the standard cosmology as given by ΛCDM and, consequently, the distance modulus for supernovae can be defined by the Padé approximant.
Lorenzo Zaninetti
doaj +1 more source
Tidal disruption events (TDEs), in which a star is destroyed by the gravitational field of a supermassive black hole (SMBH), are being observed at a high rate owing to the advanced state of survey science.
Eric R. Coughlin, Matt Nicholl
doaj +1 more source

