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相关论文: NICMOS Observations of Low-Redshift Quasar Host Ga…

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We present deep Near-infrared (NIR) images of a sample of 19 intermediate-redshift ($0.3<z<1.0$) radio-loud active galactic nuclei (AGN) with powerful relativistic jets ($L_{1.4GHz} >10^{27}$ WHz$^{-1}$), previously classified as…

We use photometric data, from the optical to the mm for a large sample of optically selected radio-quiet quasars, at low and high redshifts, to test emission models from circum-nuclear dusty torii around them. Model parameters, such as dust…

天体物理学 · 物理学 2007-05-23 P. Andreani , A. Franceschini , G. L. Granato

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 present detailed clustering measurements for a flux limited sample of 14,000 quasars extracted from the 2dF QSO Redshift Survey (2QZ) in the redshift range 0.8<z<2.1. After splitting the sample into three redshift bins and each of them…

天体物理学 · 物理学 2009-11-11 Cristiano Porciani , Peder Norberg

Observations with the Wide-Field/Planetary Camera-2 of the Hubble Space Telescope (HST) are presented for three radio-loud quasars: 3C 48 (z=0.367), B2 1425+267 (z=0.366), and 3C 345 (z=0.594). All three quasars have luminous (~4 L^*)…

天体物理学 · 物理学 2009-10-31 Sofia Kirhakos , John N. Bahcall , Donald P. Schneider , Jerome Kristian

We report the serendipitous discovery of an "Einstein Ring" in the optical band from the Sloan Digital Sky Survey (SDSS) data and associated four images of a background source. The lens galaxy appears to be a nearby dwarf spheroid at a…

天体物理学 · 物理学 2011-02-11 Kajal K Ghosh , D. Narasimha

We study the dependence of the number density and properties of quasars on the background galaxy density using the currently largest spectroscopic datasets of quasars and galaxies. We construct a galaxy number density field smoothed over…

宇宙学与河外天体物理 · 物理学 2016-08-17 Hyunmi Song , Changbom Park , Heidi Lietzen , Maret Einasto

Galaxies hosting z~2 quasars are the high-$z$ progenitors of today's massive `red-and-dead' galaxies. With close pairs of quasars at different redshifts, a background quasar can be used to study a foreground quasar's halo gas in absorption,…

天体物理学 · 物理学 2011-02-11 J. Xavier Prochaska , Joseph F. Hennawi

We present X-ray imaging and spectroscopy of the redshift z=7.084 radio-quiet quasar ULAS J112001.48+064124.3 obtained with Chandra and XMM-Newton. The quasar is detected as a point source with both observatories. The Chandra observation…

宇宙学与河外天体物理 · 物理学 2015-06-17 M. J. Page , C. Simpson , D. J. Mortlock , S. J. Warren , P. C. Hewett , B. P. Venemans , R. G. McMahon

We present the results of XMM-Newton observations of four high-z quasars, two radio-loud and two radio-quiet. One of the radio-loud objects, PKS 2126-158, clearly shows absorption in excess of the galactic value as claimed before from ASCA…

天体物理学 · 物理学 2011-05-23 E. Ferrero , W. Brinkmann

Although absorbed quasars are extremely important for our understanding of the energetics of the Universe, the main physical parameters of their central engines are still poorly known. In this work we present and study a complete sample of…

星系天体物理 · 物理学 2015-06-22 L. Ballo , P. Severgnini , R. Della Ceca , A. Caccianiga , C. Vignali , F. J. Carrera , A. Corral , S. Mateos

We investigate the properties of the environment around 20 powerful radio galaxies and quasars at redshifts between 0.45 and 1. Using XMM-Newton and Chandra observations we probe the spatial distribution and the temperature of the cluster…

天体物理学 · 物理学 2009-11-13 Elena Belsole , Diana M. Worrall , Martin J. Hardcastle , Judith H. Croston

We test emission models of circum-nuclear dust torii around quasars, at low and high redshifts, by using a large collection of photometric data for an unbiased sample of 120 optically-selected objects with millimetric and sub-millimetric…

天体物理学 · 物理学 2009-10-31 Paola Andreani , Alberto Franceschini , Gianluigi Granato

Quasars at redshifts $z>6$ are an excellent probe of the formation and evolution of supermassive black holes in the early Universe. The population of radio-luminous quasars is of particular interest, as such quasars could potentially be…

星系天体物理 · 物理学 2024-02-15 Pascal M. Keller , Nithyanandan Thyagarajan , Ajay Kumar , Nissim Kanekar , Gianni Bernardi

We use the ROSAT All Sky Survey (RASS) to study the soft X-ray properties of a homogeneous sample of 46,420 quasars selected from the third data release of the Sloan Digital Sky Survey (SDSS). Optical luminosities, both at rest-frame…

We present new radio and X-ray observations of two nearby ($< 4$ Mpc) low-mass early-type galaxies with dynamically-confirmed central black holes: NGC 5102 and NGC 205. NGC 5102 shows a weak nuclear X-ray source and has no core radio…

星系天体物理 · 物理学 2022-12-07 R. Urquhart , L. I. McDermott , J. Strader , A. C. Seth , L. Chomiuk , N. Neumayer , D. D. Nguyen , E. Tremou

Although radio-quiet quasars (RQQs) constitute >90% of optically-identified quasar samples their radio properties are only poorly understood. In this paper we present the results of a multi-frequency VLA study of 27 low-redshift RQQs. We…

天体物理学 · 物理学 2015-06-24 M. J. Kukula , J. S. Dunlop , D. H. Hughes , S. Rawlings

Hubble Space Telescope (HST) WFPC-2 I-band (F814W) images of three X-ray selected BL Lacertae objects (MS1221.8+2452, MS1407.9+5954, & MS2143.4+0704) reveal that each of these BL Lac objects is well-centered in an extended nebulosity that…

天体物理学 · 物理学 2011-03-03 Buell T. Jannuzi , Brian Yanny , Chris Impey

We study the galaxy environment of active galaxies, radio-loud and radio-quiet quasars in the redshift range $0.1\leq z\leq0.25$. We use APM galaxies in order to explore the local galaxy overdensity and the $b_J-R$ colour distribution of…

天体物理学 · 物理学 2009-11-07 Georgina V. Coldwell , Hector J. Martinez , Diego G. Lambas

We use 62,185 quasars from the Sloan Digital Sky Survey DR5 sample and standard virial mass scaling laws based on the widths of H beta, Mg II, and C IV lines and adjacent continuum luminosities to explore the maximum mass of quasars as a…

高能天体物理现象 · 物理学 2015-05-14 Charles L. Steinhardt , Martin Elvis
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