Results 11 to 20 of about 5,279,442 (297)
Luminosity function of GRBs [PDF]
11 pages, 4 postscript figures; uses aa.cls. Accepted for publication in A & A (29 June 2001)
Sethi, Shiv, Bhargavi, S. G.
openaire +3 more sources
On the normalized FRB luminosity function [PDF]
Thirty-three fast radio bursts (FRBs) had been detected by March 2018. Although the sample size is still limited, meaningful statistical studies can already be carried out. The normalised luminosity function places important constraints on the intrinsic power output, sheds light on the origin(s) of FRBs, and can guide future observations. In this paper,
Rui Luo, Bing Zhang
exaly +4 more sources
Luminosity function of clusters of galaxies [PDF]
15 pages, 14 figures, 4 tables; uses subfigure.sty; accepted for publication in Astronomy and ...
Reinaldo de Carvalho +2 more
exaly +6 more sources
A Left and Right Truncated Schechter Luminosity Function for Quasars
The luminosity function for quasars (QSOs) is usually fitted by a Schechter function. The dependence of the number of quasars on the redshift, both in the low and high luminosity regions, requires the inclusion of a lower and upper boundary in the ...
Lorenzo Zaninetti
doaj +2 more sources
We present an analysis of 123 gamma-ray bursts (GRBs) with known redshifts possessing an afterglow plateau phase. We reveal that La-T∗a correlation between the X-ray luminosity La at the end of the plateau phase and the plateau duration, T∗a, in the GRB ...
Paul Thomas O'Brien (7629023) +5 more
core +8 more sources
The Ultraviolet Luminosity Function at 0.6 < z < 1 from UVCANDELS [PDF]
UVCANDELS is a Hubble Space Telescope Cycle-26 Treasury Program awarded 164 orbits of primary ultraviolet (UV) F275W imaging and coordinated parallel optical F435W imaging in four CANDELS fields—GOODS-N, GOODS-S, EGS, and COSMOS—covering a total area of ∼
Lei Sun +77 more
doaj +2 more sources
The Galaxy Luminosity Function and Luminosity Density at Redshiftz= 0.1 [PDF]
submitted to ...
Blanton, M R +19 more
openaire +5 more sources
The Luminosity Function of Galaxies in Some Nearby Clusters
In the present work, the galaxy luminosity function (LF) has been studied for a sample of seven clusters in the redshift range (0.0 ≲ z ≲ 0.1), within Abell radius (1.5 h−1 Mpc), in the five SDSS passbands ugriz.
Mariwan Ahmed Rasheed +1 more
doaj +1 more source
THE PROTOSTELLAR LUMINOSITY FUNCTION [PDF]
The protostellar luminosity function (PLF) is the present-day luminosity function of the protostars in a region of star formation. It is determined using the protostellar mass function (PMF) in combination with a stellar evolutionary model that provides the luminosity as a function of instantaneous and final stellar mass. As in McKee & Offner (2010)
Offner, Stella S. R. +1 more
openaire +2 more sources
On the mass distribution of stars in the solar neighborhood [PDF]
The present authors analyze samples consisting of Hipparcos stars. Based on the corresponding HR diagrams they estimate masses of Main-Sequence stars from their visual magnitudes. They find that already beyond the heliocentric radius of 10 pc the effects
Ninković S., Trajkovska V.
doaj +1 more source

