Results 61 to 70 of about 771 (176)
The relationship between the emission line, continuum luminosity, and Baldwin effect in blazars
Aims. This study investigates the relationship between the Mg II λ2798 Å emission line and the 3000 Å continuum luminosity, as well as the Baldwin effect, in a sample of 40’,685 radio-quiet (RQ) quasars and 441 flat spectrum radio quasars (FSRQs ...
Patiño-Álvarez Víctor M. +5 more
doaj +1 more source
UEG Week 2023 Moderated Posters
United European Gastroenterology Journal, Volume 11, Issue S8, Page 201-534, October 2023.
wiley +1 more source
Optical Microvariability in Radio-quiet Quasars
We report the results of a study of optical microvariability in radio-quiet and radio-intermediate quasars. Observations were obtained on a total of seven objects: five radio-quiet quasars and two radio-intermediate quasars. No microvariability was detected in either the radio-quiet or radio-intermediate objects in our sample, despite intensive ...
M. T. Carini +3 more
openaire +1 more source
Cosmic Supernova Neutrino and Gamma-Ray Backgrounds in the MeV Regime
Cosmic multimessenger backgrounds include relic diffuse components created in the early universe and contributions from individual sources. Here, we study both type Ia supernovae (SNe Ia) and core-collapse supernovae (CCSNe) contributions to the diffuse ...
Samalka Anandagoda +6 more
doaj +1 more source
UEG Week 2023 Poster Presentations
United European Gastroenterology Journal, Volume 11, Issue S8, Page 535-1498, October 2023.
wiley +1 more source
LoTSS/HETDEX:Disentangling star formation and AGN activity in gravitationally-lensed radio-quiet quasars [PDF]
Determining the star-forming properties of radio-quiet quasars is important for understanding the co-evolution of star formation and black hole accretion.
L. K. Morabito +81 more
core +1 more source
Quasar Winds Caught on Acceleration and Deceleration
We present an observational study of wind acceleration based on four low-ionization broad absorption line (BAL) quasars (J0136, J1238, J1259, and J1344).
Weimin Yi +7 more
doaj +1 more source
A unique UV flare in the optical light curve of the quasar J004457.9+412344
We found that the nova candidate J004457.9+412344 is a radio-quiet quasar at z ∼ 2. Its optical long-term light curve, covering more than half a century, shows quasar typical flux variations superimposed by a spectacular single flare lasting more than ...
Hatzidimitriou D. +10 more
doaj +1 more source
Deep Space Network Radio Science and Ground‐Based Planetary Radar in the Next Decade
Abstract The Deep Space Network (DSN) has been a core operational element of NASA's crewed and robotic exploration of the Solar System since the early 1960s. The primary role of the DSN has been to acquire telemetry and navigation data, but over the years, its radiometric and radar capabilities have expanded to form a system for obtaining unique ...
R. S. Park +13 more
wiley +1 more source
Fundamental differences in the radio properties of red and blue quasars: enhanced compact AGN emission in red quasars [PDF]
We have recently used the Faint Images of the Radio Sky at Twenty-centimeters (FIRST) survey to show that red quasars have fundamentally different radio properties to typical blue quasars: a significant (factor ≈3) enhancement in the radio-detection ...
Rosario, D.J. +15 more
core +1 more source

