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相关论文: A hyperluminous obscured quasar at a redshift of z…

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We have conducted ultra-deep optical and deep near-infrared observations of a field around the z=1.226 radio-quiet quasar 104420.8+055739 from the Clowes-Campusano LQG of 18 quasars at z~1.3 in search of associated galaxy clustering.…

天体物理学 · 物理学 2015-06-24 C. P. Haines , R. G. Clowes , L. E. Campusano , A. J. Adamson

JWST observations of quasars in the Epoch of Reionization have revealed that many lie in host galaxies that are severely undermassive relative to the supermassive black holes. It is unclear how these systems will evolve to the tight local…

The intergalactic medium was not completely reionized until approximately a billion years after the Big Bang, as revealed by observations of quasars with redshifts of less than 6.5. It has been difficult to probe to higher redshifts,…

We report the discovery of an unambiguous, substantial low-energy cutoff in the broad band X-ray spectrum of the radio quasar RXJ1028.6-0844 at a redshift of 4.276 obtained with the ASCA satellite, which we preferably explained as…

天体物理学 · 物理学 2009-10-31 W. Yuan , M. Matsuoka , T. Wang , S. Ueno , H. Kubo , T. Mihara

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…

We aim at probing the emission mechanism of the accreting super massive black holes in the high redshift Universe. We study the X-ray spectrum of ULAS1120+0641, the highest redshift quasar detected so far at z=7.085, which has been deeply…

星系天体物理 · 物理学 2015-06-18 A. Moretti , L. Ballo , V. Braito , A. Caccianiga , R. Della Ceca , R. Gilli , R. Salvaterra , P. Severgnini , C. Vignali

We present an imaging study of the black hole binary candidate SDSS J1536+0441 (z=0.3893), based on deep, high resolution VzK images collected at the ESO/VLT. The images clearly show an asymmetric elongation, indicating the presence of a…

宇宙学与河外天体物理 · 物理学 2015-05-13 R. Decarli , M. Dotti , R. Falomo , A. Treves , M. Colpi , J. K. Kotilainen , C. Montuori , M. Uslenghi

We present the 0.85-2.5-micron discovery spectrum and multi-epoch photometry of the new high-redshift quasar ULAS J081621.47+213442.6 obtained using the GNIRS spectrograph of the Gemini North and near-infrared wide-field camera of the 4-m…

星系天体物理 · 物理学 2022-12-13 Ekaterina Koptelova , Chorng-Yuan Hwang

We report the discovery of the hyperluminous, highly obscured AGN WISE J190445.04+485308.9 (W1904+4853 hereafter, $L_{bol} = 1.1 \times 10^{13} \ L_{\odot}$) at z=0.415. Its well-sampled spectral energy distribution (SED) is dominated by…

2MASX J04035024-0239275 is a bright red elliptical galaxy at redshift 0.0661 that presents two extended sources at 2\arcsec~to the north-east and 1\arcsec~to the south-west. The sizes and surface brightnesses of the two blue sources are…

We present the initial results from our search for high redshift, z > 6, quasars using near infrared data from the UKIRT Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS). Our analysis of 106 deg^2 of sky from Data Release 1 (DR1)…

A five square arcminute region around the luminous radio-loud quasar SDSS J0836+0054 (z=5.8) hosts a wealth of associated galaxies, characterized by very red (1.3 < i_775 - z_{850} < 2.0) color. The surface density of these z~5.8 candidates…

In this paper we explore the properties of the z=6.853 obscured hyperluminous quasar COS-87259, discovered in the Cosmological Evolution Survey (COSMOS) field, with our recently developed Bayesian spectral energy distribution (SED) fitting…

星系天体物理 · 物理学 2024-10-14 Charalambia Varnava , Andreas Efstathiou , Duncan Farrah

We report the discovery of an X-ray luminous galaxy cluster at z=1.26. RXJ0848.9+4452 was selected as an X-ray cluster candidate in the ROSAT Deep Cluster Survey, on the basis of its spatial extent. Deep optical and near-IR imaging have…

High-redshift quasars are believed to reside in massive halos in the early universe and should therefore be located in fields with overdensities of galaxies, which are thought to evolve into galaxy clusters seen in the local universe.…

宇宙学与河外天体物理 · 物理学 2013-08-20 Eduardo Bañados , Bram Venemans , Fabian Walter , Jaron Kurk , Roderik Overzier , Masami Ouchi

We present the first rest-frame optical spectrum of a high-redshift quasar observed with JWST/NIRCam in Wide Field Slitless (WFSS) mode. The observed quasar, J0100+2802, is the most luminous quasar known at $z>6$. We measure the mass of the…

We present ALMA observations of rest-frame far-infrared continuum and [CII] line emission in two z=6.4 quasars with black hole masses of ~10^8 M_sun. CFHQS J0210-0456 is detected in the continuum with a 1.2 mm flux of 120+/-35 microJy,…

宇宙学与河外天体物理 · 物理学 2015-06-12 Chris J. Willott , Alain Omont , Jacqueline Bergeron