Results 141 to 150 of about 110,927 (295)
Quasar Microlensing Variability Studies Favor Shallow Accretion Disk Temperature Profiles [PDF]
Matthew A. Cornachione +3 more
openalex +1 more source
Abstract Purpose In electron beam therapy targeting superficial thoracic and abdominal lesions, the source‐to‐surface distance (SSD) varies due to patient respiration. This study aimed to investigate the percentage depth dose (PDD) and off‐center ratio (OCR) of 6, 9, and 12 MeV electron beams at extended SSDs; and to assess the variations in dose ...
Takaaki Ito +4 more
wiley +1 more source
Quasar candidate selection and photometric redshift estimation based on SDSS and UKIDSS data
We present a sample of 8498 quasars with both SDSS $ugriz$ optical and UKIDSS $YJHK$ near-IR photometric data. With this sample, we obtain the median colour-z relations based on 7400 quasars with magnitude uncertainties less than 0.1mag in all bands.
Abazajian +36 more
core +1 more source
Quest for a Coherent Definition of Weak-line Quasars and Its Physical Implications
Weak-line quasars (WLQs) represent a subset of type 1 quasars distinguished by remarkably weak high-ionization broad emission lines, yet exhibiting normal optical/UV continua. This study establishes a physically motivated definition of WLQs using 371,091
Xiaoqiang Cheng, Jianfeng Wu, Qiaoya Wu
doaj +1 more source
We have selected quasars with X-ray colors suggestive of a low energy cut-off, from the ROSAT PSPC pointed archive. We examine the radio and optical properties of these 13 quasars.
Allen S. W. +43 more
core +1 more source
The host galaxies of low luminosity quasars at high redshift
We present VLT/ISAAC near-infrared imaging of the host galaxies of 15 low luminosity quasars at 1 < z < 2. This work complements our studies to trace the cosmological evolution of the host galaxies of high luminosity quasars.
A. Treves +24 more
core +1 more source
Winds accelerated by active galactic nuclei (AGNs) are invoked in the most successful models of galaxy evolution to explain the observed physical and evolutionary properties of massive galaxies.
G. Vietri +23 more
semanticscholar +1 more source
The Jets in Micro-Quasars and Quasars: A Comparison [PDF]
AbstractThe discovery of relativistic jets in radio emitting X-ray binaries in our own galaxy has led to the term ‘microquasar’ being coined for these objects. In this paper the properties of microquasars are compared with those of quasars and radio galaxies, with the aim of trying to see how the similarities and differences can inform us about the ...
openaire +1 more source
RESOLVING THE OPTICAL EMISSION LINES OF Lyα BLOB “B1” ATz= 2.38: ANOTHER HIDDEN QUASAR [PDF]
Roderik Overzier +7 more
openalex +1 more source
We previously built a sample of 14,012 extremely variable quasars (EVQs) based on Sloan Digital Sky Survey (SDSS) and Pan-STARRS1 photometric observations.
Wenke Ren +3 more
doaj +1 more source

