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Related papers: Extended CIII]lambda1909 emission in Q0957+561

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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

Blueshifts - or, more accurately, blue asymmetries - in broad emission lines such as CIV $\lambda$1550 are common in luminous quasars and correlate with fundamental properties such as Eddington ratio and broad absorption line (BAL)…

The peculiar QSO J0927+2943 shows multiple sets of emission lines in its optical spectrum. This signature has been interpreted as the relative motion between a black hole, either recoiling or bound in a binary system, and its host galaxy,…

Astrophysics of Galaxies · Physics 2015-06-22 Roberto Decarli , Massimo Dotti , Chiara Mazzucchelli , Carmen Montuori , Marta Volonteri

We present a new SCUBA image of the cluster MS0451.6-0305, which exhibits strong, extended sub-mm flux at 850 microns. The most striking feature in the map is an elongated region of bright sub-mm emission, with a flux density of >10 mJy…

(ABRIDGED) Aims: We discuss and characterize micro-lensing among the 3 brightest lensed images (A-B-C) of the gravitational lens system RXS J1131-1231 (a quadruply imaged AGN) by means of long slit optical and NIR spectroscopy. Qualitative…

Astrophysics · Physics 2009-11-13 D. Sluse , J. -F. Claeskens , D. Hutsemékers , J. Surdej

We studied the spectra of six $z \sim 2.2$ quasars obtained with the X-shooter spectrograph at the Very Large Telescope. The redshift of these sources and X-shooter's spectral coverage allow us to cover the rest spectral range $\sim1200 -…

We utilize the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope (VLT) to search for extended Lyman-Alpha emission around the z~6.6 QSO J0305-3150. After carefully subtracting the point-spread-function, we reach a nominal…

We have obtained quasi-simultaneous ultraviolet-optical spectra for 22 out of 23 quasars in the complete PG-X-ray sample with redshift, z<0.4, and M_B<-23. The spectra cover rest-frame wavelengths from at least Lyman-alpha to H-alpha. Here…

Astrophysics · Physics 2008-11-26 Zhaohui Shang , Beverley J. Wills , D. Wills , Michael S. Brotherton

We present the analysis of single epoch long slit spectra of the three brightest images of the gravitationally lensed system J1131-1231. These spectra provide one of the clearest observational evidence for differential micro-lensing of…

Astrophysics · Physics 2008-01-18 D. Sluse , J. -F. Claeskens , D. Hutsemékers , J. Surdej

The quasar SDSS 0956+5128 exhibits three distinct velocity components with large offsets in emission: the systemic velocity of [O II], [O III] and [Ne III] narrow lines have redshift $z=0.7142$; broad Mg II line is shifted by $-1200$ km…

High Energy Astrophysical Phenomena · Physics 2023-03-06 V. Rusakov , C. L. Steinhardt , M. Schramm , A. L. Faisst , D. Masters , B. Mobasher , P. Pattarakijwanich

We present Gemini Multiobject Spectrograph integral field spectroscopy of the extended emission-line region associated with quasar 3C 249.1. The kinematics of the ionized gas measured from the [O III] $\lambda$5007 line is rather complex…

Astrophysics · Physics 2011-02-11 Hai Fu , Alan Stockton

We report the discovery of extended gamma-ray emission measured by the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope in the region of the supernova remnant (SNR) HB3 (G132.7+1.3) and the W3 HII complex adjacent to…

High Energy Astrophysical Phenomena · Physics 2016-02-17 H. Katagiri , K. Yoshida , J. Ballet , M. H. Grondin , Y. Hanabata , J. W. Hewitt , H. Kubo , M. Lemoine-Goumard

We present a high S/N spectrum for the quasar PG 1138+222. We detect a very broad HeII$\lambda$4686 emission line component with twice the FWHM of the conventional broad line region (BLR) as evidenced by the Balmer lines. The profile shape…

Astrophysics · Physics 2009-10-22 Paolo Marziani , Jack W. Sulentic

We present optical spectra of SN 2007gr, SN 2007rz, SN 2007uy, SN 2008ax, and SN 2008bo obtained in the nebular phase when line profiles can lead to information about the velocity distribution of the exploded cores. We compare these to 13…

Cosmology and Nongalactic Astrophysics · Physics 2010-01-21 D. Milisavljevic , R. Fesen , C. Gerardy , R. Kirshner , P. Challis

We present new results from extremely deep, high-resolution images of the field around the double quasar QSO 0957+561. A possible gravitational arc system near the double quasar has recently been reported, which, if real, would set strong…

Astrophysics · Physics 2009-10-22 H. Dahle , S. J. Maddox , Per B. Lilje

We investigate the spatial extent and structure of the [CII] line emission in a sample of 34 galaxies at $z=4-6$ from the ALMA-CRISTAL Survey. By modeling the [CII] line emission in the interferometric visibility, we derive the effective…

We report the detection of a nearby emission-line companion to the z=4.695 quasar BR1202-0725. Deep narrow-band exposures on this field from the UH 2.2 m show a Ly alpha flux of 1.5\times\ten{-16} ergs cm^{-2} s^{-1}. High-resolution HST…

Astrophysics · Physics 2009-10-28 Esther M. Hu , Richard G. McMahon , Eiichi Egami

We aim to unveil the structure of the continuum and broad-emission line (BEL) emitting regions in the gravitationally lensed quasar SDSS J1339+1310 by examining the distinct signatures of microlensing present in this system. Our study…

Astrophysics of Galaxies · Physics 2024-07-09 C. Fian , J. A. Muñoz , J. Jiménez-Vicente , E. Mediavilla , D. Chelouche , S. Kaspi , R. Forés-Toribio

We use Hubble Space Telescope (HST)/ Space Telescope Imaging Spectrograph (STIS) long-slit G430M and G750M spectra to analyse the extended [O~III] 5007A emission in a sample of twelve nearby (z < 0.12) luminous (L_bol > 1.6 x 10^45 erg…

The extended supernova remnant G 116.5+1.1 was observed in the optical emission lines of Halpha+[N II], [S II] and [O III]; deep long-slit spectra were also obtained. The morphology of the remnant's observed emission is mainly diffuse and…

Astrophysics · Physics 2009-11-10 F. Mavromatakis , P. Boumis , E. M. Xilouris , J. Papamastorakis , J. Alikakos
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