Results 31 to 40 of about 10,764,000 (383)
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
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
Abstract Background Ultrasonography (US) and 99mTechnetium‐sestamibi scintigraphy (99mTc‐MIBI) are currently first‐line imaging modalities to localize parathyroid adenomas with sensitivities of 80% and 84%, respectively. Therefore, finding other modalities to further improve the diagnostic accuracy for preoperative localization is critically needed ...
Fangyi Liu+7 more
wiley +1 more source
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
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
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
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 +1 more source
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/
Michael J. Kurtz+4 more
openaire +3 more sources
The Faint End of the z = 5 Quasar Luminosity Function from the CFHTLS [PDF]
We present results from a spectroscopic survey of z ∼ 5 quasars in the CFHT Legacy Survey. Using both optical color selection and a likelihood method, we select 97 candidates over an area of 105 deg2 to a limit of iAB < 23.2, and 7 candidates in the ...
I. McGreer+3 more
semanticscholar +1 more source
The quasar luminosity function at redshift 4 with the Hyper Suprime-Cam Wide Survey [PDF]
We present the luminosity function of z=4 quasars based on the Hyper Suprime-Cam Subaru Strategic Program Wide layer imaging data in the g, r, i, z, and y bands covering 339.8 deg^2.
M. Akiyama+26 more
semanticscholar +1 more source