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相关论文: A QSO host galaxy and its Lyalpha emission at z=6.…

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We have taken a deep, moderate-resolution Keck/Deimos spectra of QSO, CFHQS2329, at z=6.4. At the wavelength of Lya, the spectrum shows a spatially-extended component, which is significantly more extended than a stellar spectrum, and also a…

宇宙学与河外天体物理 · 物理学 2015-06-03 Tomotsugu Goto , Yousuke Utsumi , Jeremy R. Walsh , Takashi Hattori , Satoshi Miyazaki , Chisato Yamauchi

We report the first unambiguous detection of the host galaxy of a normal radio-quiet QSO at high-redshift in K-band. The luminosity of the host comprises about 35% of the total K-band luminosity. Assuming the average colour of QSOs at z=2,…

天体物理学 · 物理学 2009-10-30 I. Aretxaga , D. Le Mignant , J. Melnick , R. J. Terlevich , B. J. Boyle

We first present new Subaru narrow-band observations of the Ly$\alpha$ halo around the quasi-stellar object (QSO) CFHQ J232908$-$030158 at $z=6.42$, which appears the most luminous and extended halo at $z>5$ ($L_{Ly\alpha}=9.8\times10^{43}$…

Based on an $R$-band imaging survey of high-redshift ($z \approx 2$) QSOs with the 4.2m WHT, we report the detection of extensions to the nuclear PSFs of two radio-quiet and one radio-loud QSO. The extensions are most likely host galaxies,…

天体物理学 · 物理学 2007-05-23 I. Aretxaga , B. J. Boyle , R. J. Terlevich

We have been conducting an imaging survey to detect host galaxies of radio-quiet QSOs at high redshift (z = 2), in order to compare them with those of radio-loud objects. Six QSOs were observed in the R passband with the auxiliary port of…

天体物理学 · 物理学 2007-05-23 I. Aretxaga , B. J. Boyle , R. J. Terlevich

We announce the discovery of an extended emission line region associated with a high redshift type-2 QSO. The halo, which was discovered in our new wide-field narrow-band survey, resides at z = 2.85 in the Spitzer First Look Survey region…

天体物理学 · 物理学 2009-11-13 Daniel J. B. Smith , Matt J. Jarvis , Chris Simpson , Alejo Martinez-Sansigre

We present results of the hosts of four high-redshift ($z \approx 2$) and high luminosity ($M_B \lsim -28$ mag) QSOs, three radio-quiet one radio-loud, imaged in R and K bands. The extensions to the nuclear unresolved source are most likely…

天体物理学 · 物理学 2007-05-23 Itziar Aretxaga , Brian J. Boyle , Roberto J. Terlevich

We have observed nine QSOs with redshifts 0.85 to 4.16 at near-IR wavelengths with the adaptive optics bonnette of the Canada-France-Hawaii telescope. Exposure times ranged from 1500 to 24000s (mostly near 7000s) in J, H, or K bands, with…

天体物理学 · 物理学 2009-10-31 J. B. Hutchings , D. Crampton , S. L. Morris , D. Durand , E. Steinbring

We have obtained deep J & Ks-band images centered on a bright radio quiet QSO UM402 (z_{em}=2.856) using IRCS camera and AO systems on Subaru Telescope, as well as retrieved WFC3/F140W archive images. A faint galaxy (m_{k}=23.32 +/- 0.05 in…

宇宙学与河外天体物理 · 物理学 2016-10-26 Yiping Wang , Wei He , Toru Yamada , Ichi Tanaka , Masanori Iye , Tuo Ji

We have discovered extended Lyman-$\alpha$ emission around a $z=4.5$ QSO in a deep long-slit spectrum with Keck/LRIS at moderate spectral resolution ($R\approx 1000$). The line emission extends 5\,arcsec beyond the continuum of the QSO and…

天体物理学 · 物理学 2009-11-07 Andrew Bunker , Joanna Smith , Hyron Spinrad , Daniel Stern , Stephen Warren

We report on deep imaging in 2 filters with the PC2 camera of HST, of five QSOs at redshift ~2, with a range of optical and radio luminosity. The observations included a suite of PSF observations which were used to construct new PSF models,…

天体物理学 · 物理学 2009-11-07 J. B. Hutchings , D. Frenette , R. Hanisch , J. Mo , P. J. Dumont , D. C. Redding , S. G. Neff

We present integral field spectrograph (IFS) with laser guide star adaptive optics (LGS-AO) observations of z=2 quasi-stellar objects (QSOs) designed to resolve extended nebular line emission from the host galaxy. Our data was obtained with…

星系天体物理 · 物理学 2016-05-31 Andrey Vayner , Shelley A. Wright , Tuan Do , James E. Larkin , Lee Armus , Sarah C. Gallagher

We report on ESO--VLT adaptive optics imaging of one radio-loud quasar at z $\sim$ 3. In spite of the large distance of the object we are able to detect its surrounding extended nebulosity the properties of which are consistent with an…

天体物理学 · 物理学 2009-11-13 R. Falomo , J. K. Kotilainen , R. Scarpa , A. Treves , M. Uslenghi

Three high-redshift (z=2) and high luminosity (M_B < -28 mag for Ho = 50, qo=0.5) QSOs, two radio-quiet one radio-loud, were imaged in R, I and K bands. The luminosities, colours and sizes of the hosts overlap with those of actively…

天体物理学 · 物理学 2007-05-23 I. Aretxaga , R. J. Terlevich , B. J. Boyle

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

Images are discussed of six QSOs at z=2.3, one QSO-like IRAS source at z=2.3, and one QSO at z=1.1, taken with resolution 0.6 to 0.9 arcsec. Five of the QSOs are radio-quiet. All QSOs except one are just resolved, while the IRAS source has…

天体物理学 · 物理学 2009-10-28 J. B. Hutchings

Based on an R-band imaging survey of 6 high redshift (z~2) and high luminosity (M<-28mag) QSOs, we report the detection of extensions in two radio-quiet and one radio-loud QSO. The extensions are most likely due to the host galaxies of…

天体物理学 · 物理学 2016-06-08 I. Aretxaga , B. J. Boyle , R. J. Terlevich

We present here the spectrum of the galaxy companion to the z=4.7 quasar BR1202-0725, in the optical range 6000-9000 A, corresponding to 1050-1580 A rest-frame. We detect a strong Lya emission line at z=4.702, with an integrated flux of…

天体物理学 · 物理学 2009-10-30 A. Fontana , S. D'Odorico , E. Giallongo , S. Cristiani , G. Monnet , P. Petitjean

We aim to illustrate the potentiality of the Advanced Large, Homogeneous Area, Medium-Band Redshift Astronomical (ALHAMBRA) survey to investigate the high redshift universe through the detection of quasi stellar objects (QSOs) at redshifts…

We present rest-frame UV and Ly-alpha images of spatially-resolved structures around five high-redshift radio-loud quasars obtained with the WFPC2 camera on the Hubble Space Telescope. We find that all five quasars are extended and this…

天体物理学 · 物理学 2009-10-31 Matthew D. Lehnert , Wil J. M. van Breugel , Timothy M. Heckman , George K. Miley
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