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Since no spectroscopic redshift is available for the remarkable BL Lac object 1ES 0647+250, we aim to derive an estimate of its distance from the properties of its host galaxy.We obtained a deep, high-resolution near-infrared H-band image…

宇宙学与河外天体物理 · 物理学 2015-05-30 J. K. Kotilainen , T. Hyvönen , R. Falomo , A. Treves , M. Uslenghi

We have acquired a deep i-band image of the BL Lacertae object S5 0716+714 while the target was in an low optical state. Due to the faintness of the nucleus, we were able to detect the underlying host galaxy. The host galaxy is measured to…

天体物理学 · 物理学 2015-05-13 K. Nilsson , T. Pursimo , A. Sillanpää , L. O. Takalo , E. Lindfors

We have obtained high dynamic range, good natural seeing i' images of BL Lacertae objects (BL Lacs) to search for the AGN host and thus constrain the source redshift. These objects are drawn from a sample of bright flat-spectrum radio…

宇宙学与河外天体物理 · 物理学 2015-05-18 Aaron M. Meisner , Roger W. Romani

We present the discovery and a detailed multi-wavelength study of a strongly-lensed luminous infrared galaxy at z=0.816. Unlike most known lensed galaxies discovered at optical or near-infrared wavelengths this lensed source is red, r-Ks =…

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

Aims: The determination of elusive redshifts of bright BL Lac objects Methods: We use the capabilities of newly available spectrograph X-Shooter at European Southern Observatory (ESO) Very Large Telescope, that combines high resolution and…

宇宙学与河外天体物理 · 物理学 2015-06-05 Marco Landoni , Renato Falomo , Aldo Treves , Boris Sbarufatti , Roberto Decarli , Fabrizio Tavecchio , Jari Kotilainen

We have obtained WIYN and SOAR i' images of BL Lacertae objects (BL Lacs) and used these to detect or constrain the flux of the host galaxy. Under common standard candle assumptions these data provide estimates of, or lower bounds on, the…

星系天体物理 · 物理学 2015-06-18 Matt Stadnik , Roger W. Romani

We report the detection of a third HI 21-cm absorber in the sight-line towards the z=2.64 quasar MG J0414+0534 (4C +05.19). In addition to the absorption at the host redshift and in the z=0.96 gravitational lens, we find, through a…

宇宙学与河外天体物理 · 物理学 2015-05-27 S. J. Curran , M. T. Whiting , A. Tanna , C. Bignell , J. K. Webb

We present the results of a near-infrared imaging study of high redshift (z~3) quasars using the ESO-VLT. Our targets were selected to have luminosities among the highest known (absolute magnitude M_B <~ -28. We searched for resolved…

天体物理学 · 物理学 2009-11-13 M. Schramm , L. Wisotzki , K. Jahnke

We present the results of near-infrared H band (1.65 microns) imaging of 11 BL Lac objects with redshifts ranging from z = 0.05 to 0.9. We are able to clearly detect the host galaxy in seven low redshift (z<=0.24) BL Lacs, while the four…

天体物理学 · 物理学 2007-05-23 J. K. Kotilainen , R. Falomo , R. Scarpa

We identify a strong lensing galaxy in the cluster IRC 0218 (also known as XMM-LSS J02182$-$05102) that is spectroscopically confirmed to be at $z=1.62$, making it the highest-redshift strong lens galaxy known. The lens is one of the two…

Hubble Space Telescope WFPC-2 I-band (F814W) images of the BL Lacertae object OJ 287 and the surrounding field are presented. We find evidence of associated extended nebulosity near OJ 287, as well as a small nebulosity to the West, which…

天体物理学 · 物理学 2011-04-04 Brian Yanny , Buell T. Jannuzi , Chris Impey

The BL Lac object 4FGLJ0955.1+3551 has been suggested as a possible source of ultra energetic neutrinos detected by the Icecube observatory. The target was observed in January 2020 at the Large Binocular Telescope. Our spectroscopy…

高能天体物理现象 · 物理学 2020-04-22 Simona Paiano , Renato Falomo , Paolo Padovani , Paolo Giommi , Adriana Gargiulo , Michela Uslenghi , Andrea Rossi , Aldo Treves

We present the results from an ESO/VLT campaign aimed at studying the afterglow properties of the short/hard gamma ray burst GRB 070707. Observations were carried out at ten different epochs from ~0.5 to ~80 days after the event. The…

We have used the HST WFPC2 camera to survey 132 BL Lac objects comprising seven complete radio-, X-ray-, and optically-selected samples. We obtained useful images for 110 targets spanning the redshift range 0 < z < 1.3. In two thirds of the…

天体物理学 · 物理学 2009-10-31 C. Megan Urry , Riccardo Scarpa , Matthew O'Dowd , Renato Falomo , Joseph E. Pesce , Aldo Treves

We demonstrate that deep good-seeing VLT/HAWK-I $K_\mathrm{s}$ images complemented with $g$+$z$-band photometry can yield a sensitivity for weak lensing studies of massive galaxy clusters at redshifts \mbox{$0.7\lesssim z \lesssim 1.1$},…

Direct redshift determination of BL Lac objects is highly challenging as the emission in the optical and near-infrared (NIR) bands is largely dominated by the non-thermal emission from the relativistic jet that points very close to our line…

BL Lac objects emitting in the Very High Energy (VHE) regime are unique tools to peer into the properties of the Extragalactic Background Light (EBL). However, due to the typical absence of features in their spectra, the determination of…

PKS0447-439 is one of the BL Lacertae objects that have been detected at very high energy. There has been a recent report of a lower limit of z>1.246 for the redshift of this blazar, challenging the current paradigm in which very…

宇宙学与河外天体物理 · 物理学 2012-08-16 Michele Fumagalli , Amy Furniss , John M. O'Meara , J. Xavier Prochaska , David A. Williams , Emanuele P. Farina

We present {\it Hubble Space Telescope} and ground--based data on the $z_{abs}=0.8596$ metal line absorption system along the line of sight to PKS 0454+0356. The system is a moderate redshift damped Lyman alpha system, with ${\rm…

天体物理学 · 物理学 2009-10-22 C. Steidel , D. Bowen , J. C. Blades , M. Dickinson
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