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200 papers

The ROSAT ALL Sky Survey Bright Source Catalogue (RASS-BSC) has been correlated with the Catalogue of Principal Galaxies (PGC) to identify new extragalactic counterparts. 550 reliable optical counterparts have been detected. We took optical…

Astrophysics · Physics 2009-11-13 W. Kollatschny , R. Kotulla , W. Pietsch , K. Bischoff , M. Zetzl

Sloan Digital Sky Survey (SDSS) DR5 photometric data with $120^{\circ} < \alpha < 270^{\circ}$, $25^{\circ} < \delta < 70^{\circ}$ are searched for new Milky Way companions or substructures in the Galactic halo. Five candidates are…

Astrophysics · Physics 2011-11-09 C. Liu , J. Hu , H. Newberg , Y. Zhao

We present a sample of 12 Quasi-Stellar Objects (QSOs) potentially acting as strong gravitational lenses on background Emission Line Galaxies (ELG) or Lyman-$\alpha$ Emitters (LAEs) selected selected through a systematic search of the…

Astrophysics of Galaxies · Physics 2019-05-13 Romain A. Meyer , Timothée Delubac , Jean-Paul Kneib , Frédéric Courbin

Type II quasars are suggested by unification models of Active Galactic Nuclei as luminous analogs of Seyfert 2 galaxies. A number of different methods have been used hitherto to discover type II quasars, but only a handful have been found.…

Astrophysics · Physics 2007-05-23 Nadia L. Zakamska , Michael A. Strauss , Julian H. Krolik , Timothy M. Heckman

We report on a new method to identify Active Galactic Nuclei (AGN) among unidentified INTEGRAL sources. This method consists of cross-correlating unidentified sources listed in the fourth IBIS Survey Catalogue first with infrared and then…

Gravitationally-lensed quasars should be discovered as a by-product of large galaxy redshift surveys, being discovered spectroscopically when a low-redshift galaxy exhibits high-redshift quasar emission lines. The number of lenses expected…

Astrophysics · Physics 2007-05-23 Daniel J. Mortlock , Rachel L. Webster

We report on optical searches in the error circles of 93 ROSAT survey sources located at low galactic latitudes (|b| < 20 deg). These sources were extracted from the ROSAT Galactic Plane Survey using various selection criteria on hardness…

We analyse a Chandra observation of the rich globular cluster NGC 362, finding 33 X-ray sources within 1' (1.2 half-mass radii) of the cluster center. Spectral analysis of the brightest source (X1) shows blackbody-like emission, indicating…

High Energy Astrophysical Phenomena · Physics 2024-03-26 Gourav Kumawat , Craig O. Heinke , Haldan N. Cohn , Phyllis M. Lugger

We study the link between galaxies and HI-selected absorption systems at z~3-4 in the MUSE Analysis of Gas around Galaxies (MAGG) survey, an ESO large programme consisting of integral field pectroscopic observations of 28 quasar fields…

The Magellanic System (MS), consisting of the Large Magellanic Cloud (LMC), the Small Magellanic Cloud (SMC) and the Magellanic Bridge (MBR), contains diverse sample of star clusters. Their spatial distribution, ages and chemical abundances…

The multi-epoch YJKs sub-arcsecond photometry of the VMC survey provides a long anticipated deep near-infrared (NIR) window into further understanding the stellar populations of the Magellanic Clouds. The first year of observations…

Solar and Stellar Astrophysics · Physics 2015-05-30 B. Miszalski , R. Napiwotzki , M. -R. L. Cioni , M. A. T. Groenewegen , J. M. Oliveira , A. Udalski , J. Nie

We present initial results of an ongoing study of the supernova remnants (SNRs) and candidates in the Magellanic Clouds. Some 108 objects in both Clouds are considered to be either an SNR or a reliable candidate. This represents the most…

Astrophysics of Galaxies · Physics 2016-04-07 Miroslav D. Filipović , Luke M. Bozzetto

We present X-ray data for a complete sample of 44 luminous infrared galaxies (LIRGs), obtained with the Chandra X-ray Observatory. These are the X-ray observations of the high luminosity portion of the Great Observatory All-sky LIRG Survey…

We present an analysis of archival Spitzer images and new ground-based and Hubble Space Telescope (HST) near-infrared (IR) and optical images of the field of M83 with the goal of identifying rare, dusty, evolved massive stars. We present…

Solar and Stellar Astrophysics · Physics 2015-06-11 S. J. Williams , A. Z. Bonanos , B. C. Whitmore , J. L. Prieto , W. P. Blair

AGB stars are ideal IR targets because they are cool and bright. Most of them escaped detection in optical or shallow IR surveys in the eighties contributing to the puzzling missing number of AGB stars with respect to theoretical…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 Maria-Rosa L. Cioni

We present a new optical imaging survey of supernova remnants in M83, using data obtained with the Magellan I 6.5m telescope and IMACS instrument under conditions of excellent seeing. Using the criterion of strong [S II] emission relative…

Astrophysics of Galaxies · Physics 2015-06-11 William P. Blair , P. Frank Winkler , K. S. Long

We have observed two low concentration Galactic globular clusters with the X-ray observatory XMM-Newton. We detect 47 faint X-ray sources in the direction of M 55 and 62 in the field of view of NGC 3201. Using the statistical Log N-Log S…

Astrophysics · Physics 2009-11-11 N. A. Webb , P. J. Wheatley , D. Barret

This paper is the second in a series devoted to the hard X-ray (17-60 keV) whole sky survey performed by the INTEGRAL observatory over seven years. Here we present a catalog of detected sources which includes 521 objects, 449 of which…

High Energy Astrophysical Phenomena · Physics 2015-05-19 R. Krivonos , S. Tsygankov , M. Revnivtsev , S. Grebenev , E. Churazov , R. Sunyaev

The third Fermi source catalog lists 3033 gamma-ray sources above $4\sigma$ significance. More than 30% are classified as either unidentified/unassociated Gamma-ray sources (UGSs), with about 20% classified as Blazar candidates of uncertain…

Astrophysics of Galaxies · Physics 2019-03-26 Marchesini , E. J. , Peña-Herazo , H. A. , Álvarez Crespo , N. , Ricci , F. , M. Negro , Milisavljevic , D. , Massaro , F. , Masetti , N. , Landoni , M. , Chavushyan , V. , D'Abrusco , R. , Jiménez-Bailón , E. , La Franca , F. , Paggi , A. , Smith , H. A. , Tosti , G.

At least 50% of the baryons in the local universe are undetected and predicted to be in a hot dilute phase (1E5-1E7 K) in low and moderate overdensity environments. We searched for the predicted diffuse faint emission through shadowing…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-30 Joel N. Bregman , Birgit Otte , Jimmy A. Irwin , Mary E. Putman , Edward J. Lloyd-Davies , Christian Brüns