Results 51 to 60 of about 765,605 (153)
Charged Particles Moving around a Spherically Symmetric Dilatonic Black Hole
For the static spherically symmetric dilatonic black hole described by the Gibbons–Maeda–Garfinkle–Horowitz–Strominger geometry, we analyze the timelike trajectories for electrically charged test particles. Both cases of an electric black hole and a magnetic one are considered.
Vitalie Lungu +4 more
wiley +1 more source
A quasar-galaxy merger at [PDF]
We present JWST/NIRSpec integral field spectroscopy in the rest-frame optical bands of the system PJ308–21, a quasar at z = 6.2342 caught as its host galaxy interacts with companion galaxies.
Alessandro Lupi +179 more
core +3 more sources
Probing Dark Matter Halos of High-redshift Quasars via Wide-field Clustering
High-redshift quasars are powerful tracers of both astrophysical processes and large-scale structure in the early Universe. Using a sample of 1242 spectroscopically confirmed quasars and 827 highly reliable photometric quasar candidates selected with a ...
Hao Meng, Guangping Ye, Huanian Zhang
doaj +1 more source
Quasar and galaxy classification using Gaia EDR3 and CatWise2020 [PDF]
In this work, we assess the combined use of Gaia photometry and astrometry with infrared data from CatWISE in improving the identification of extragalactic sources compared to the classification obtained using Gaia data.
Bailer-Jones, Coryn A. L. +5 more
core +1 more source
UEG Week 2022 Oral Presentations
United European Gastroenterology Journal, Volume 10, Issue S8, Page 9-184, October 2022.
wiley +1 more source
Our understanding of large-scale radio jets in merger systems has been drastically improved in the era of the Very Large Array, Very Long Baseline Array/European VLBI Network, upgraded Giant Metrewave Radio Telescope, and MeerKAT.
Santanu Mondal +5 more
doaj +1 more source
We present the largest catalogue to date of Galaxies On Top Of Quasars (GOTOQs)—systems where the sight line to a background quasar passes directly through or very close to a foreground galaxy.
Labanya K. Guha +2 more
doaj +1 more source
Discovery of a bright quasar without a massive host galaxy
peer reviewedA quasar is thought to be powered by the infall of matter onto a supermassive black hole at the centre of a massive galaxy(1,2). Because the optical luminosity of quasars exceeds that of their host galaxy, disentangling the two components ...
Wisotzki, L. +13 more
core +1 more source
The VST ATLAS Quasar Survey II: Halo mass profiles of galaxies, LRGs and galaxy clusters via quasar and CMB lensing [PDF]
We cross-correlate a low-contamination subset of the VST ATLAS g < 22.5 quasar catalogue with g < 21.5 galaxy clusters, r < 21 galaxies and r < 19.5 Luminous Red Galaxies (LRGs) to probe their halo mass profiles via quasar magnification bias caused by ...
Murph, D. N. A. +6 more
core +4 more sources
Dual active galactic nuclei (AGNs), a phase in some galaxy mergers during which both central supermassive black holes (SMBHs) are active, are expected to be a key observable stage leading up to SMBH mergers.
Arran C. Gross +10 more
doaj +1 more source

