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相关论文: Bright X-ray galaxies in SDSS filaments

200 篇论文

The optical properties of a number of supercompact ultraviolet luminous galaxies (UVLG), recently discovered in the local Universe matching GALEX and Sloan Digital Sky Survey (SDSS) data, are discussed. Detailed re-analysis of the SDSS data…

天体物理学 · 物理学 2009-11-13 Riccardo Scarpa , Renato Falomo , Eric Lerner

We review recent results on populations of compact X-ray sources in normal galaxies. The luminosity distributions of low and high mass X-ray binaries in nearby galaxies appear to be described by the respective ``universal'' luminosity…

天体物理学 · 物理学 2008-11-26 M. Gilfanov

We present a sample of 383 X-ray selected galaxy groups and clusters with spectroscopic redshift measurements (up to z ~ 0.79) from the 2XMMi/SDSS Galaxy Cluster Survey. The X-ray cluster candidates were selected as serendipitously detected…

宇宙学与河外天体物理 · 物理学 2014-03-05 A. Takey , A. Schwope , G. Lamer

Eighteen candidates for emission line galaxies were discovered in a narrow-band infrared survey that targeted the redshifts of damped Lyman-alpha or metal lines in the spectra of quasars. The presence of emission lines is inferred from the…

天体物理学 · 物理学 2009-10-30 F. Mannucci , D. Thompson , S. V. W. Beckwith , G. M. Williger

We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey (SDSS) data within the GAMA equatorial fields. The search method consisted of masking objects detected with SDSS photo, combining gri…

We present a new catalog of merging galaxies obtained through an automated systematic search routine. The 1479 new pairs of merging galaxies were found in approximately 462 sq deg of the Sloan Digital Sky Survey Early Data Release (SDSS…

天体物理学 · 物理学 2009-11-10 S. S. Allam , D. L. Tucker , J. A. Smith , B. C. Lee , J. Annis , H. Lin , I. Karachentsev , B. E. Laubscher

Using the Herschel ATLAS science demonstration phase data crossidentified with SDSS DR7 spectra, we select 297 galaxies with F250{\mu}m > 5{\sigma}. The sample galaxies are classified into five morphological types, and more than 40% of the…

宇宙学与河外天体物理 · 物理学 2015-06-12 M. I. Lam , H. Wu , Y. -N. Zhu , Z. -M. Zhou

Using imaging data from the SDSS survey, we present the g' and r' radial stellar light distribution of a complete sample of ~90 face-on to intermediate inclined, nearby, late-type (Sb-Sdm) spiral galaxies. The surface brightness profiles…

天体物理学 · 物理学 2009-11-11 M. Pohlen , I. Trujillo

X-ray luminosities and spectral indices of 97 bright Seyfert 1 galaxies from XMM archive are analyzed in this article. Distribution of these values is random so we conclude that the model of emission should be at least two-parametric.…

星系天体物理 · 物理学 2018-12-12 V. A. Sadova , A. V. Tugay

We present a multi-wavelength study of the nature of the SDSS galaxies divided into fine classes based on their morphology, colour and spectral features. The SDSS galaxies are classified into early-type and late-type; red and blue; passive,…

宇宙学与河外天体物理 · 物理学 2015-05-14 Joon Hyeop Lee , Myung Gyoon Lee , Changbom Park , Yun-Young Choi

We present the results of a search for X--ray luminous distant clusters of galaxies. We found extended X--ray emission characteristic of a cluster towards two of our candidate clusters of galaxies. They both have a luminosity in the ROSAT…

天体物理学 · 物理学 2009-10-22 R. C. Nichol , M. P. Ulmer , R. G. Kron , G. D. Wirth , D. C. Koo

We report the detection of 10 new X-ray filaments using the data from the {\sl Chandra} X-ray satellite for the inner $6^{\prime}$ ($\sim 15$ parsec) around the Galactic center (GC). All these X-ray filaments are characterized by…

天体物理学 · 物理学 2009-11-13 F. J. Lu , T. T. Yuan , Y. -Q. Lou

We present results from a near/mid IR search for submillimetre galaxies over a region of 6230 sq deg. of the southern sky. We used a cross-correlation of the VISTA Hemispheric Survey (VHS) and the WISE database to identify bright galaxies…

星系天体物理 · 物理学 2017-02-15 S. Iglesias-Groth , A. Diaz-Sanchez , R. Rebolo , H. Dannerbauer

We present photometric and spectroscopic measurements of 53 QSO-galaxy pairs from the Sloan Digital Sky Survey, where nebular emission lines from a 0<z<0.84 foreground galaxy are detected in the fiber spectra of a background QSO, bringing…

We use archival Chandra X-ray Observatory data to investigate X-ray emission from early-type galaxies in the rich z=0.06 cluster Abell 3128. By combining the X-ray count-rates from an input list of optically-selected galaxies, we obtain a…

天体物理学 · 物理学 2009-11-10 Russell J. Smith

We performed five pointing observations with Suzaku to search for hot gases associated with the junctions of galaxy filaments where no significant diffuse X-ray sources were detected so far. We discovered X-ray sources successfully in all…

宇宙学与河外天体物理 · 物理学 2014-03-05 Ikuyuki Mitsuishi , Hajime Kawahara , Norio Sekiya , Shin Sasaki , Thierry Sousbie , Noriko Y. Yamasaki

We have used the Parkes Multibeam system and the Sloan Digital Sky Survey (SDSS) to assemble a sample of 195 galaxies selected originally from their HI signature to avoid biases against unevolved or low surface brightness objects. For each…

We search for the lensing signal of massive filaments between 135,000 pairs of Luminous Red Galaxies (LRGs) from the Sloan Digital Sky Survey. We develop a new estimator that cleanly removes the much larger shear signal of the neighboring…

宇宙学与河外天体物理 · 物理学 2016-03-02 Joseph Clampitt , Hironao Miyatake , Bhuvnesh Jain , Masahiro Takada

Six Narrow-Line Seyfert 1 galaxies have been discovered in optical follow-up spectroscopy of nuclei of galaxies selected for their high X-ray flux in the ROSAT All Sky Survey. We give X-ray and optical parameters of the sources and show…

天体物理学 · 物理学 2007-05-23 W. Pietsch , K. Bischoff , Th. Boller

We present an analysis of 39 X-ray luminous early-type galaxies observed with the ROSAT PSPC. Using multi-component spectral and spatial fits to these data we have measured halo abundance, temperature, luminosity and surface brightness…

天体物理学 · 物理学 2009-11-07 Ewan O'Sullivan , Trevor J. Ponman , Ross S. Collins