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The interactions between radio jets and the interstellar medium play a defining role for the co-evolution of central supermassive black holes and their host galaxies, but observational constraints on these feedback processes are still very…

We report the serendipitous discoveries of companion galaxies to two high-redshift quasars. SDSS J025617.7+001904 is a z=4.79 quasar included in our recent survey of faint quasars in the SDSS Stripe 82 region. The initial MMT slit…

[Abridged] We compare broad emission line profiles and estimate line ratios for all major emission lines between Ly-alpha and H-beta in a sample of six quasars. The sources were chosen with two criteria in mind: the existence of high…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 P. Marziani , J. W. Sulentic , C. A. Negrete , D. Dultzin , S. Zamfir , R. Bachev

We present integral field spectroscopy of a small sample of radio-loud quasars at intermediate redshift (0.26<z<0.60), most of which are associated with large radio sources. All have oxygen line emission extended over tens of kiloparcsecs,…

Astrophysics · Physics 2009-10-31 C. S. Crawford , C. Vanderriest

We present near-infrared spectra of seven radio-loud quasars with a median redshift of 2.1, five of which were previously known to have Ly alpha nebulae. Extended [OIII]5007 and H alpha emission are evident around six objects, at the level…

Astrophysics · Physics 2009-10-31 R. J. Wilman , R. M. Johnstone , C. S. Crawford

The study of ionized gas kinematics in high-z active galaxies plays a key part in our understanding of galactic evolution, in an age where nuclear activity was widespread and star formation close to its peak. We present a study of TXS…

We present high S/N UV spectra for eight quasars at $z\sim3$\ obtained with VLT/FORS. The spectra enable us to analyze in detail the strongest emission features in the rest-frame range 1400-2000 \AA\ of each source (\ciii, \siiii, \aliii,…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 C. Alenka Negrete , Deborah Dultzin , Paola Marziani , Jack Sulentic

We report on the discovery of a rare case of spatially and kinematically resolved galactic scale outflow at intermediate redshift, based on VLT/MUSE optical integral field spectroscopic observation of the quasar HE 0238$-$1904. This…

Astrophysics of Galaxies · Physics 2023-02-08 Qinyuan Zhao , Junfeng Wang

We use near-infrared (NIR) spectroscopy covering simultaneously the $zJHK$ bands to look for outflowing gas from the nuclear environment of 1H0707-495 taking advantage that this region is dominated by low-ionization broad line region (BLR)…

In the last few years, prominent high-ionization nebular emission lines (i.e., OIII], CIII], CIV, HeII) have been observed in the deep UV spectra of z~5-7 galaxies, indicating that extreme radiation fields characterize reionization-era…

Astrophysics of Galaxies · Physics 2019-06-12 Danielle A. Berg , John Chisholm , Dawn K. Erb , Richard Pogge , Alaina Henry , Grace M. Olivier

We have obtained optical intermediate resolution spectra (R = 3000) of the narrow-line quasars DMS 0059-0055 and PG 1543+489. The [O III] emission line in DMS 0059-0055 is blueshifted by 880 km/s relative to Hbeta. We also confirm that the…

Astrophysics · Physics 2009-11-10 Kentaro Aoki , Toshihiro Kawaguchi , Kouji Ohta

The quasar SDSS J105041.35+345631.3 (z = 0.272) has broad emission lines blueshifted by 3500 km/s relative to the narrow lines and the host galaxy. Such an object may be a candidate for a recoiling supermassive black hole, binary black…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 G. A. Shields , D. J. Rosario , K. L. Smith , E. W. Bonning , S. Salviander , J. S. Kalirai , R. Strickler , E. Ramirez-Ruiz , A. A. Dutton , T. Treu , P. J. Marshall

Extremely red quasars, with bolometric luminosities exceeding $10^{47}$ erg s$^{-1}$, are a fascinating high-redshift population that is absent in the local universe. They are the best candidates for supermassive black holes accreting at…

We report the results from an ASCA observation of the high-luminosity, radio-loud quasar PKS 0637-752 (redshift 0.654), covering the 0.8-15 keV band in the quasar-frame. We find the source to have a luminosity ~10^46 erg/s in the 2-10 keV…

Astrophysics · Physics 2009-10-30 T. Yaqoob , I. M. George , T. J. Turner , K. Nandra , A. Ptak , P. J. Serlemitsos

In order to investigate where and how low ionization lines are emitted in quasars we are studying a new collection of spectra of the CaII triplet at $\lambda$8498, $\lambda$8542, $\lambda$8662 observed with the Very Large Telescope (VLT)…

We present a high spectral resolution optical spectrum of the bright quasar Q~1037-2704. The large number of absorption systems suggests the presence of an intervening supercluster, but the issue remains controversial.\par We demonstrate…

Astrophysics · Physics 2007-05-23 Yannick Lespine , Patrick Petitjean

4C 71.07 is a high-redshift blazar whose optical radiation is dominated by quasar-like nuclear emission. We here present the results of a spectroscopic monitoring of the source to study its unbeamed properties. We obtained 24 optical…

Astrophysics of Galaxies · Physics 2020-03-11 C. M. Raiteri , J. A. Acosta Pulido , M. Villata , M. I. Carnerero , P. Romano , S. Vercellone

We present an investigation of the low-frequency radio and ultraviolet properties of a sample of $\simeq$10,500 quasars from the Sloan Digital Sky Survey Data Release 14, observed as part of the first data release of the Low-Frequency-Array…

Astrophysics of Galaxies · Physics 2021-03-03 Amy L. Rankine , James H. Matthews , Paul C. Hewett , Manda Banerji , Leah K. Morabito , Gordon T. Richards

We investigate the radial velocity difference between the [OIII]5007,4959 and H-beta lines for a sample of 200 low redshift AGN. We identify seven objects showing an [OIII]5007 blueshift relative to H-beta with amplitude larger than 250…

Astrophysics · Physics 2009-11-07 R. Zamanov , P. Marziani , J. W. Sulentic , M. Calvani , D. Dultzin-Hacyan , R. Bachev

We report a new changing-look quasar, WISE~J105203.55+151929.5 at $z=0.303$, found by identifying highly mid-IR variable quasars in the WISE/NEOWISE data stream. Compared to multi-epoch mid-IR photometry of a large sample of SDSS-confirmed…