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相关论文: Emission line imaging of QSOs with high resolution

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2 micron broad- and narrow-band imaging with the Gemini-N telescope of five z~4.7 QSOs, has resolved both the host galaxies and [O II] emission-line gas. The resolved fluxes of the host galaxies fall within the extrapolated spread of the…

天体物理学 · 物理学 2009-11-07 J. B. Hutchings

We discuss broad- and narrow-band imaging of 7 arcmin fields of 14 QSOs with redshift ~1.1. The narrow-band filters were chosen to detect redshifted [O II] 3727A, and the broad bands are R and I, which correspond to rest wavelengths…

天体物理学 · 物理学 2009-10-22 J. B. Hutchings , D. Crampton , Andrea Johnson

We present the results of an infrared survey of QSO fields at z=0.95, 0.995 and 1.5. Each z<1 field was imaged to typical continuum limits of J=20.5, Kprime=19 (5 sigma), and line fluxes of 1.3E10{-16}ergs/cm^2/s (1 sigma)in a 1%…

天体物理学 · 物理学 2009-10-31 Harry I. Teplitz , Ian S. McLean , Matthew A. Malkan

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 present off-nuclear spectra of 3 radio loud QSO's, 3C249.1, 3C273 and 3C323.1., taken with the echellette spectrograph and imager (ESI) at Keck observatory. From these spectra we have extracted the spatial profile along the slit of the…

天体物理学 · 物理学 2007-05-23 Andrew Sheinis

We report the discovery of a high redshift, narrow emission-line galaxy identified in the optical follow-up of deep ROSAT fields. The object has a redshift of z=2.35 and its narrow emission lines together with its high optical and X-ray…

天体物理学 · 物理学 2007-05-23 O. Almaini , B. J. Boyle , R. E. Griffiths , T. Shanks , G. C. Stewart , I. Georgantopoulos

We present Very Large Array (VLA) observations at 1.4 GHz and 5 GHz of a sample of 12 Quasi-stellar Objects (QSOs) at z = 3.99 to 4.46. The sources were selected as the brightest sources at 250 GHz from the recent survey of Omont et al.…

天体物理学 · 物理学 2009-11-06 C. L. Carilli , F. Bertoldi , A. Omont , P. Cox , R. G. McMahon , K. G. Isaak

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 present moderate (1'') and high resolution (0.2'') observations of the CO(2-1) emission at 43 GHz, and radio continuum emission at 1.47 GHz, from the z=4.7 QSO BRI 1202-0725 and the z=4.4 QSO BRI 1335--0417 using the Very Large Array.…

天体物理学 · 物理学 2009-11-07 C. L. Carilli , K. Kohno , R. Kawabe , K. Ohta , C. Henkel , K. Menten , M. Yun , A. Petric , Y. Tutui

In a pilot search for high-redshift radio QSOs, we have obtained spectra of 55 FIRST sources (S(1.4GHz) > 1 mJy) with very red (O-E > 3) starlike optical identifications. 10 of the candidates are QSOs with redshifts 3.6 < z < 4.4 (4…

天体物理学 · 物理学 2009-11-07 C. R. Benn , M. Vigotti , M. Pedani , J. Holt , K. -H. Mack , R. Curran , S. F. Sanchez

A narrowband imaging survey of 276 square minutes of arc was carried out at near infrared wavelengths to search for emission line objects at high redshifts. Most of the fields contained a known quasar or radio galaxy at a redshift that…

天体物理学 · 物理学 2009-10-28 D. Thompson , F. Mannucci , S. V. W. Beckwith

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

An infrared-selected, narrow-line QSO has been found to exhibit an extraordinarily broad Halpha emission line in polarized light. Both the extreme width (35,000 km/sec full-width at zero intensity) and 3,000 km/sec redshift of the line…

天体物理学 · 物理学 2009-11-07 G. D. Schmidt , P. S. Smith , C. B. Foltz , D. C. Hines

We present the first results from a near-infrared narrow-band search for primeval galaxies (PGs) using the Keck 10~m telescope. We have targeted our fields for three QSOs and one radio galaxy at redshifts $z = 2.28$ to $4.70$. We selected…

天体物理学 · 物理学 2009-10-28 M. A. Pahre , S. G. Djorgovski

We present K-band imaging and photometry of a sample of 52 radio loud quasars (RQs) selected from the B3 survey with flux densities above 0.5 Jy at 408 MHz. The optical completeness of the sample is 90% and the quasars cover the redshift…

天体物理学 · 物理学 2009-10-30 R. Carballo , S. F. Sanchez , J. I. Gonzalez-Serrano , C. R. Benn , M. Vigotti

We present the results of a narrow-band survey of QSO fields at redshifts that place the [OIII](5007) emission line in the 1% 2.16micron filter. We have observed 3 square arcminutes and detected one emission line candidate object in the…

天体物理学 · 物理学 2009-10-31 Harry I. Teplitz , Matthew A. Malkan , Ian S. McLean

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 present the results of a survey for CO line emission from a sample of nearby QSO hosts taken from the Hamburg/ESO survey (HES) and the Veron-Cetty and Veron quasar catalogue. From a total of 39 observed sources we clearly detected 5…

天体物理学 · 物理学 2009-11-13 T. Bertram , A. Eckart , M. Krips , C. Straubmeier , S. Fischer , J. G. Staguhn

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 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…

天体物理学 · 物理学 2009-10-31 R. J. Wilman , R. M. Johnstone , C. S. Crawford
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