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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…

Astrophysics · Physics 2007-05-23 O. Almaini , B. J. Boyle , R. E. Griffiths , T. Shanks , G. C. Stewart , I. Georgantopoulos

We report the first detection of emission line gas within the host galaxies of high redshift QSOs. This was done using narrow-band imaging at the redshifted wavelengths of [O III] and H alpha, using the PUEO adaptive optics camera of the…

Astrophysics · Physics 2009-10-31 J. B. Hutchings , S. L. Morris , D. Crampton

I propose that broad narrow-topped emission lines with full width at zero intensity >20000 km/s, seen in early-time spectra of SN 1998S, originate from a dense circumstellar gas and not from the supernova ejecta. The tremendous line width…

Astrophysics · Physics 2016-01-13 N. N. Chugai

We present near-IR spectroscopy of a sample of luminous (Lbol >10^14 Lsun), sub-millimeter-detected, dusty (M_dust~10^9 Msun), radio-quiet QSOs at z~2. We measure the redshift, width, and luminosity of the Halpha line, and the continuum…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Gustavo Orellana , Neil M. Nagar , Kate G. Isaac , Robert Priddey , Roberto Maiolino , Richard McMahon , Alessandro Marconi , Ernesto Oliva

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…

Astrophysics · Physics 2009-11-07 Andrew Bunker , Joanna Smith , Hyron Spinrad , Daniel Stern , Stephen Warren

Optical spectropolarimetry of the nucleus of the LINER NGC 1052, obtained at the Keck Observatory, reveals a rise in polarization in the wings of the H-alpha line profile. The polarization vector of H-alpha is offset by 67 degrees from the…

Astrophysics · Physics 2009-10-31 A. J. Barth , A. V. Filippenko , E. C. Moran

Highly polarized QSOs discovered in the Two-Micron All Sky Survey (2MASS) have been observed to determine the source(s) of optical polarization in this near-infrared color-selected sample. Broad emission lines are observed in the polarized…

Astrophysics · Physics 2009-11-07 Paul S. Smith , Gary D. Schmidt , Dean C. Hines , Craig B. Foltz

We present in this paper optical and X-ray follow up observations for three X-ray selected objects extracted from the ROSAT North Ecliptic Pole survey which is a flux-limited, completely identified survey. All three objects have X-ray…

Astrophysics · Physics 2016-08-30 A. Wolter , I. M. Gioia , J. P. Henry , C. R. Mullis

We performed a search for the HeH+ J=1-0 line (\nu_{rest} = 2010.183873 GHz) and simultaneously for the CH ^2\Pi_{3/2}(F_2)J=3/2 - ^2\Pi_{1/2}(F_2)J=1/2 lines (\nu_{rest}\approx 2006.8 and 2010.8 GHz) toward one of the highest-redshift…

Cosmology and Nongalactic Astrophysics · Physics 2011-05-25 I. Zinchenko , V. Dubrovich , C. Henkel

High quality 4500-6800 A spectropolarimetric observations of the Circinus galaxy are reported. These show polarized and relatively broad (FWHM~3300 km/s) Halpha (as well as marginal Hbeta) arising from a <3" (<60 pc) region centered on the…

Astrophysics · Physics 2007-05-23 E. Oliva , A. Marconi , A. Cimatti , S. di Serego Alighieri

Ground based long slit spectroscopic observations of the nuclear region of NGC 5252, and Hubble Space Telescope (HST) Faint Object Spectrograph (FOS) spectra of the nucleus and two bright knots located 0.36" NE and 0.31" SW from it, show…

Astrophysics · Physics 2007-05-23 A. C. Goncalves , P. Veron , M. -P. Veron-Cetty

In this Letter, the broad emission line (BEL) profiles of superluminal quasars with apparent jet velocities, $\beta_{a}>10$, (ultraluminal QSOs, or ULQSOs hereafter) are studied as a diagnostic of the velocity field of the BEL emitting gas…

Astrophysics · Physics 2009-11-13 Brian Punsly

We present the detection of extremely broad, double-peaked, highly polarized Halpha emission lines in the nuclei of the well-known Seyfert 2 galaxies NGC 2110 and NGC 5252. These hidden broad Halpha emission lines, visible only in scattered…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-23 Hien D. Tran

We present a spectropolarimetric survey of 36 broad absorption line quasi-stellar objects (BAL QSOs). The continuum, absorption trough, and emission line polarization of BAL QSOs yield clues about their structure. We confirm that BAL QSOs…

Astrophysics · Physics 2009-10-31 P. M. Ogle , M. H. Cohen , J. S. Miller , H. D. Tran , R. W. Goodrich , A. R. Martel

We report the results of a spectropolarimetric survey of a complete far infrared selected sample of Seyfert 2 galaxies. We have found polarized broad Halpha emission in one new source, NGC5995. In the sample as a whole, there is a clear…

Astrophysics · Physics 2009-11-06 S. L. Lumsden , C. A. Heisler , J. A. Bailey , J. H. Hough , S. Young

An object discovered during an infrared survey of the field near the quasar B2 0149+33 has an emission line at 2.25$\mu$m that we interpret as H$\alpha$ at a redshift of 2.43. The K-band image shows two compact components 10 kpc apart…

Astrophysics · Physics 2009-10-30 S. V. W. Beckwith , D. Thompson , F. Mannucci , S. G. Djorgovski

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…

Astrophysics · Physics 2009-11-13 Daniel J. B. Smith , Matt J. Jarvis , Chris Simpson , Alejo Martinez-Sansigre

Optical broad-band polarimetry is presented for near-infrared color-selected AGN classified QSOs based on their K-band luminosity. More than 10% of a sample of 70 QSOs discovered in the Two Micron All Sky Survey (2MASS) with J-K > 2 and M_K…

Astrophysics · Physics 2009-11-07 P. S. Smith , G. D. Schmidt , D. C. Hines , R. M. Cutri , B. O. Nelson

Extremely high velocity (EHV) wings, with full widths of 72 to 140 km/s, are seen on the CO J=3-2 lines toward W3 IRS 5, GL 490, NGC 2071, W28 A2, GL 2591, S140, and Cepheus A. The results of our survey suggest that EHV wings are common…

Astrophysics · Physics 2009-10-22 Minho Choi , Neal J. Evans , Daniel T. Jaffe
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