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相关论文: A low-luminosity type-1 QSO sample; III. Optical s…

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The faint radio-source population includes sources dominated both by star formation and active galactic nuclei (AGN), encoding the evolution of activity in the Universe. To investigate its nature, we probabilistically classified 4,471 radio…

We present the results of a systematic analysis of the XMM-Newton spectra of nearby optically bright QSOs. The objects have been selected from X-ray Galaxy Catalog Xgal20. It is a catalog of 1172 manually identified and classified galaxies,…

宇宙学与河外天体物理 · 物理学 2021-10-15 Lidiia Zadorozhna , Anatolii Tugay , Nadiia Pulatova , Oleh Maluy

We have searched the Faint Images of the Radio Sky at Twenty centimeters (FIRST) and the NRAO VLA Sky Survey (NVSS) 1.4 GHz radio surveys for sources that are coincident with emission-line galaxy (ELG) candidates from the KPNO International…

天体物理学 · 物理学 2009-11-10 J. Van Duyne , E. Beckerman , J. Salzer , C. Gronwall , T. Thuan , J. Condon , L. Frattare

We present quasi-simultaneous multi-colour optical/near-IR photometry for 157 radio selected quasars, forming an unbiassed sub-sample of the Parkes Flat-Spectrum Sample. Data are also presented for 12 optically selected QSOs, drawn from the…

天体物理学 · 物理学 2015-06-24 Paul J. Francis , Matthew T. Whiting , Rachel L. Webster

We report on the analysis of B band imaging data of 57 low-redshift QSOs and Seyfert 1 galaxies selected from the Hamburg/ESO-Survey, for which host galaxy dependent selection biases are greatly reduced compared to other optical surveys.…

天体物理学 · 物理学 2009-11-10 K. Jahnke , L. Wisotzki

We study the Distant Red Galaxy (DRG, J-K_s > 2.3) neighbour population of Quasi Stellar Objects (QSOs) selected from the Sloan Digital Sky Survey (SDSS) in the redshift range 1 < z < 2. We perform a similar analysis for optically obscured…

天体物理学 · 物理学 2008-11-26 Carlos G. Bornancini , Diego Garcia Lambas

We report the first results of quasi-simultaneous two passband optical monitoring of six quasi-stellar objects to search for micro-variability. We carried out photometric monitoring of these sources in an alternating sequence of R and V…

天体物理学 · 物理学 2008-09-14 Alok C. Gupta , Weimin Yuan

We present a detailed analysis of a sample of radio-detected quasars, obtained by matching together objects from the FIRST and 2dF Quasar Redshift Surveys. The dataset consists of 113 sources, spanning a redshift range 0.3 < z < 2.2, with…

天体物理学 · 物理学 2009-11-07 M. Cirasuolo , M. Magliocchetti , A. Celotti , L. Danese

We present results from uGMRT 685 MHz observations of 87 QSOs belonging to the Palomar Green (PG) quasar sample with $z<0.5$. Radio emission is detected in all sources except for 3 radio-quiet (RQ) sources, viz., PG 0043+039, PG 1121+422,…

星系天体物理 · 物理学 2025-10-06 Sanna Gulati , Silpa Sasikumar , Preeti Kharb , Luis C. Ho , Salmoli Ghosh , Janhavi Baghel

We combine emission line and X-ray luminosities for 45 sources from the Chandra Deep Field South (CDF-S), and seven HELLAS sources, to obtain a new sample of 52 X-ray selected type-II active galactic nuclei (AGNs). Eighteen of our sources…

天体物理学 · 物理学 2009-11-11 Hagai Netzer , V. Mainieri , P. Rosati , Benny Trakhtenbrot

We present the result of 27 ASCA observations of 26 radio-quiet quasars (RQQs) from the PG survey. All the RQQs were detected except 2 BALQSOs. We find the variability characteristics of the sources to be consistent with Seyf-1s. A powerlaw…

天体物理学 · 物理学 2009-10-31 I. M. George , T. J. Turner , T. Yaqoob , H. Netzer , A. Laor , R. F. Mushotzky , K. Nandra , T. Takahashi

We present a spectroscopically complete sample of 147 infrared-color-selected AGN down to a 22 $\mu$m flux limit of 20 mJy over the $\sim$270 deg$^2$ of the SDSS Stripe 82 region. Most of these sources are in the QSO luminosity regime…

The growth of active galactic nuclei (AGN) occurs under some form of obscuration in a large fraction of the population. The difficulty in constraining this population leads to high uncertainties in cosmic X-ray background and galaxy…

We present some results from our HST archival image study of 71 QSO host galaxies. The objects are selected to have z < 0.46 and total absolute magnitude M_V < -23 (H_0=50 km/s/Mpc). This initial study investigates host morphology and radio…

天体物理学 · 物理学 2009-10-31 Timothy S. Hamilton , Stefano Casertano , David A. Turnshek

We present spectral energy distributions (SEDs) of 69 QSOs at z>5, covering a rest frame wavelength range of 0.1mu to ~80mu, and centered on new Spitzer and Herschel observations. The detection rate of the QSOs with Spitzer is very high…

星系天体物理 · 物理学 2015-06-18 C. Leipski , K. Meisenheimer , F. Walter , U. Klaas , H. Dannerbauer , G. De Rosa , X. Fan , M. Haas , O. Krause , H. -W. Rix

We use the Hubble Space Telescope to analyse the extended [O III] 5007A emission in seven bright radio-quiet type 1 quasars (QSO1s), focusing on the morphology and physical conditions of their extended Narrow-Line Regions (NLRs). We find…

There is growing evidence of a higher intrinsic fraction of broad absorption line quasars (BALQSOs) than that obtained in optical surveys, on which most previous X-ray studies of BALQSOs have focused. Here we present Chandra observations of…

高能天体物理现象 · 物理学 2014-04-21 Leah K. Morabito , Xinyu Dai , Karen M. Leighly , Gregory R. Sivakoff , Francesco Shankar

Type II quasars are the long-sought luminous analogs of type II (narrow emission line) Seyfert galaxies, suggested by unification models of active galactic nuclei (AGN) and postulated to account for an appreciable fraction of the cosmic…

We present results of near-infrared photometry (J, H, K_S) for a sample of active galactic nuclei (AGNs) obtained from hard X-ray surveys with ASCA. The sample covers the AGNs at z=0.1-1 with L(2-10keV)=10^42-10^46 erg/s with very high…

天体物理学 · 物理学 2009-11-10 Chisato Watanabe , Kouji Ohta , Masayuki Akiyama , Yoshihiro Ueda

We present the first multi-parameter analysis of the narrow line AGN clustering properties. Estimates of the two-point correlation function (CF) based on SDSS DR2 data reveal that Seyferts are clearly less clustered than normal galaxies,…

天体物理学 · 物理学 2011-02-11 Anca Constantin , Michael S. Vogeley