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We present a systematic search for changing-look quasars based on repeat photometry from SDSS and Pan-STARRS1, along with repeat spectra from SDSS and SDSS-III BOSS. Objects with large, |\Delta g|>1 mag photometric variations in their light…

Despite extensive efforts, only two quasars have been found at $z>7$ to date due to a combination of low spatial density and high contamination from more ubiquitous Galactic cool dwarfs in quasar selection. This limits our current knowledge…

I present the discovery of Balmer-line absorption from H alpha to H9 in iron low-ionizaton broad absorption line (FeLoBAL) quasar, SDSS~J172341.10+555340.5 by near-infrared spectroscopy with the Cooled Infrared Spectrograph and Camera for…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Kentaro Aoki

We present the discovery of PSO J083.8371+11.8482, a weak emission line quasar with extreme star formation rate at $z=6.3401$. This quasar was selected from Pan-STARRS1, UHS, and unWISE photometric data. Gemini/GNIRS spectroscopy follow-up…

We report on the discovery of a peculiar Broad Absorption Line (BAL) quasar identified in our Gaia-assisted survey of red quasars. The systemic redshift of this quasar was difficult to establish due to the absence of conspicuous emission…

The study of high-redshift bright quasars is crucial to gather information about the history of galaxy assembly and evolution. Variability analyses can provide useful data on the physics of the quasar processes and their relation with the…

Astrophysics of Galaxies · Physics 2016-02-16 F. G. Saturni , D. Trevese , F. Vagnetti , M. Perna , M. Dadina

SDSS J083942.11+380526.3 is an Iron Low-ionization Broad Absorption Line (FeLoBAL) quasar at z = 2.3, and Aoki et al. (2006) recently found the presence of an H alpha absorption line in the broad H alpha emission line. Motivated by an idea…

We report a synchronized kinematic shift of CIV and SiIV broad absorption lines (BAL) in a high-ionization, radio-loud, and X-ray bright quasar SDSS-J092345+512710 (at $z_{em} \sim 2.1627$). This quasar shows two broad absorption components…

Astrophysics of Galaxies · Physics 2019-01-30 Ravi Joshi , Raghunathan Srianand , Hum Chand , Xue-Bing Wu , Pasquier Noterdaeme , Patrick Petitjean , Luis C. Ho

We present results on a survey to find extremely dust-reddened Type-1 Quasars. Combining the FIRST radio survey, the 2MASS Infrared Survey and the Sloan Digital Sky Survey, we have selected a candidate list of 122 potential red quasars.…

The radio-loud quasar SDSS J013127.34-032100.1at a redshift z=5.18 is one of the most distant radio-loud objects. The radio to optical flux ratio (i.e. the radio-loudness) of the source is large, making it a promising blazar candidate. Its…

High Energy Astrophysical Phenomena · Physics 2015-06-23 G. Ghisellini , G. Tagliaferri , T. Sbarrato , N. Gehrels

The broad absorption line (BAL) features seen in a small fraction of quasar optical/UV spectra are attributed to bulk outflows away from the quasar core. Observational evidence suggests that dust plays a key role in these systems, although…

Astrophysics · Physics 2009-11-10 Geraint F. Lewis , Scott C. Chapman , Zdenka Kuncic

We report the discovery of unusual broad absorption lines (BALs) in the bright quasar SDSS J075133.35+134548.3 at z~1, and present a detailed study of BAL and emission lines using the archived and newly obtained optical and NIR…

Astrophysics of Galaxies · Physics 2021-05-05 Bo Liu , Hongyan Zhou , Xinwen Shu , Shaohua Zhang , Tuo Ji , Xiang Pan , Peng Jiang

We report on three redshift $z>2$ quasars with dramatic changes in their C IV emission lines, the first sample of changing-look quasars (CLQs) at high redshift. This is also the first time the changing-look behaviour has been seen in a…

Astrophysics of Galaxies · Physics 2020-09-09 Nicholas P. Ross , Matthew J. Graham , Giorgio Calderone , K. E. Saavik Ford , Barry McKernan , Daniel Stern

Only very few z>5 quasars discovered to date are radio-loud, with a radio-to-optical flux ratio (radio-loudness parameter) higher than 10. Here we report the discovery of an optically luminous radio-loud quasar, SDSS J013127.34-032100.1…

We report the first discovery of the emergence of a high-velocity broad-line outflow in a luminous quasar, J105400.40+034801.2 at redshift z ~ 2.1. The outflow is evident in ultraviolet CIV and SiIV absorption lines with velocity shifts v ~…

Astrophysics · Physics 2009-11-13 F. Hamann , K. F. Kaplan , P. Rodriguez Hidalgo , J. X. Prochaska , S. Herbert-Fort

Quasar accretion-disk outflows might play an important role in galaxy evolution, but they are notoriously difficult to study due to line saturation and blending problems in the Ly-alpha forest. We circumvent these problems by constructing…

Astrophysics of Galaxies · Physics 2018-11-07 Fred Hamann , Hanna Herbst , Isabelle Paris , Daniel Capellupo

We present an analysis of the variability of broad absorption lines (BALs) in a quasar SDSS J141955.26+522741.1 at $z=2.145$ with 72 observations from the Sloan Digital Sky Survey Data Release 16 (SDSS DR16). The strong correlation between…

Astrophysics of Galaxies · Physics 2021-01-12 Qinyuan Zhao , Zhicheng He , Guilin Liu , Tinggui Wang , Hengxiao Guo , Lu Shen , Guobin Mou

We report a high-redshift ($z=1.404$) tidal disruption event (TDE) candidate in SDSS J000118.70+003314.0 (SDSS J0001), which is a quasar with apparent broad Mg~{\sc ii} emission line. The long-term variability in its nine-year photometric…

Astrophysics of Galaxies · Physics 2024-12-24 Ying Gu , Xue-Guang Zhang , Xing-Qian Chen , Xing Yang , En-Wei Liang

We report strong and rapid X-ray variability found from the super-Eddington accreting quasar SDSS J081456.10+532533.5 at $z=0.1197$. It has a black-hole mass of $2.7\times10^{7}{M_{\odot}}$ and a dimensionless accretion rate of $\approx4$…

High Energy Astrophysical Phenomena · Physics 2023-06-14 Jian Huang , Bin Luo , W. N. Brandt , Pu Du , Gordon P. Garmire , Chen Hu , Hezhen Liu , Qingling Ni , Jian-Min Wang

We report the discovery of extreme X-ray variability in a type 1 quasar: SDSS J$075101.42+291419.1$. It has a black hole mass of $1.6\times 10^7~\rm M_\odot$ measured from reverberation mapping (RM), and the black hole is accreting with a…

Astrophysics of Galaxies · Physics 2019-06-26 Hezhen Liu , B. Luo , W. N. Brandt , Michael S. Brotherton , Pu Du , S. C. Gallagher , Chen Hu , Ohad Shemmer , Jian-Min Wang