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This paper reports X-ray spectral observations of a relatively nearby z = 0.048 BL Lacertae (BL Lac) object 1ES1959+650, which is a potential TeV emitter. The observations include 31 short pointings made by the Unconventional Stellar Aspect…

We report a deep optical imaging observation by the Subaru telescope for a very soft X-ray source RX J1836.2+5925, which has been suspected to be an isolated neutron star associated with the brightest as-yet unidentified EGRET source…

Astrophysics · Physics 2015-06-24 T. Totani , W. Kawasaki , N. Kawai

One of the major challenges in studying the cosmic evolution of relativistic jets is the identification of the high-redshift ($z>3$) BL Lacertae objects, a class of jetted active galactic nuclei characterized by their quasi-featureless…

High Energy Astrophysical Phenomena · Physics 2020-11-11 Vaidehi S. Paliya , A. Domínguez , C. Cabello , N. Cardiel , J. Gallego , B. Siana , M. Ajello , D. Hartmann , A. Gil de Paz , C. S. Stalin

We report discovery of a compact object at high Galactic latitude. The object was initially identified as a ROSAT All-Sky Survey Bright Source Catalog X-ray source, 1RXS J141256.0+792204, statistically likely to possess a high X-ray to…

Astrophysics · Physics 2009-11-13 R. E. Rutledge , D. B. Fox , A. H. Shevchuk

We report the discovery of a very bright (r = 20.16), highly magnified, and yet intrinsically very luminous Ly{\alpha} emitter (LAE) at z = 2.82. This system comprises four images in the observer plane with a maximum separation of ~ 6" and…

The optical Einstein ring 0047-2808 was imaged by the VLT UT1 during the science verification programme. The ring is the image of a high-redshift z=3.595 star-forming galaxy, with strong Ly-alpha emission at 5589A, gravitationally lensed by…

Astrophysics · Physics 2007-05-23 S. J. Warren , G. F. Lewis , P. C. Hewett , P. Moller , P. Shaver , A. Iovino

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Marco Landoni , Renato Falomo , Aldo Treves , Boris Sbarufatti , Roberto Decarli , Fabrizio Tavecchio , Jari Kotilainen

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

High-resolution images of 7 newly identified BL Lac objects (among them one BL Lac candidate) at z < 0.2 from the Einstein Slew Survey are presented for the first time. In all cases we were able to resolve the host galaxy. Our 2-dimensional…

Astrophysics · Physics 2007-05-23 J. Heidt , K. Nilsson , A. Sillanpaeae , L. O. Takalo , T. Pursimo

We present the results of an intermediate-resolution (1.5\AA) spectroscopic study of 17 X-ray luminous narrow emission-line galaxies previously identified in the Cambridge-Cambridge {\it ROSAT} Serendipity Survey and the {\it Einstein}…

Astrophysics · Physics 2015-06-24 B. J. Boyle , R. G. McMahon , B. J. Wiles , M. Elvis

We report the serendipitous discovery of transient, point-like high energy gamma-ray emission coincident with the position of the suspected BL Lac object 5C 3.178. The source was detected using the Fermi Large Area Telescope (LAT) at a…

High Energy Astrophysical Phenomena · Physics 2013-04-18 Hugh Dickinson , Christian Farnier

Models that seek to unify BL Lacs and low-power radio galaxies predict that the two types of object should show similar isotropically emitted X-ray emission. Testing this is usually limited by difficulties in separating strong X-ray…

Astrophysics · Physics 2009-10-31 M. J. Hardcastle , D. M. Worrall , M. Birkinshaw

We report the discovery of an almost complete Einstein ring of diameter 10" in Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5). Spectroscopic data from the 6m telescope of the Special Astrophysical Observatory reveals that the…

We present evidence that the optically unidentified radio source, FIRST J121839.7+295325, may be strongly lensing a background galaxy. We estimate the redshift of the assumed gravitational arc, discovered in parallel imaging with HST, from…

Astrophysics · Physics 2009-11-13 R. E. Ryan , S. H. Cohen , R. A. Windhorst , C. R. Keeton , T. J. Veach

We report on the 1.6 GHz (18 cm) VLBI observations of the unresolved, steady TeV source HESS J1943+213 located in the Galactic plane, performed with the European VLBI Network (EVN) in 2014. Our new observations with a nearly full EVN array…

High Energy Astrophysical Phenomena · Physics 2016-06-01 Kazunori Akiyama , Łukasz Stawarz , Yasuyuki T. Tanaka , Hiroshi Nagai , Marcello Giroletti , Mareki Honma

GN-108036 is a star-forming galaxy at $z=7.21$, and one of the most distant known sources in the Northern hemisphere. Based on observations from the NOrthern Extended Millimeter Array (NOEMA), here we report the tentative detection of the…

Astrophysics of Galaxies · Physics 2022-08-10 R. Baier-Soto , R. Herrera-Camus , N. M. Förster Schreiber , A. Contursi , R. Genzel , D. Lutz , L. Tacconi

The bright BL Lac object TXS 0506+056 is a most likely counterpart of the IceCube neutrino event EHE 170922A. The lack of this redshift prevents a comprehensive understanding of the modeling of the source. We present high signal-to-noise…

Astrophysics of Galaxies · Physics 2018-03-14 Simona Paiano , Renato Falomo , Aldo Treves , Riccardo Scarpa

The X-ray transient source EP240309a/EP\,J115415.8$-$501810 was first detected by the Wide-Field X-ray Telescope (WXT) on board Einstein Probe (EP) during the commissioning phase. Subsequent optical observations confirmed it as a…

We present optical spectroscopy data that allowed a measurement of the redshift for the X-ray selected BL Lacertae object 1517+656. With a redshift of z = 0.702 this object has an absolute magnitude of B = -26.4 and is also an extremely…

Astrophysics · Physics 2007-05-23 Volker Beckmann , Norbert Bade , Olaf Wucknitz