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相关论文: The XMM-LSS catalogue: X-ray sources and associate…

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We present the XMM-LSS cluster catalogue corresponding to the CFHTLS D1 area. The list contains 13 spectroscopically confirmed, X-ray selected galaxy clusters over 0.8 deg2 to a redshift of unity and so constitutes the highest density…

We present the first data release from the second epoch Molonglo Galactic Plane Survey (MGPS-2). MGPS-2 was carried out with the Molonglo Observatory Synthesis Telescope at a frequency of 843 MHz and with a restoring beam of 45 arcsec x 45…

天体物理学 · 物理学 2009-11-13 T. Murphy , T. Mauch , A. Green , R. W. Hunstead , B. Piestrzynska , A. P. Kels , P. Sztajer

We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extragalactic areas of 25 deg2 each at a point-source sensitivity…

We present an enhanced version of the publicly-available Stripe 82X catalog (S82-XL), featuring a comprehensive set of 22,737 unique X-ray point sources identified with a significance $\gtrsim 4\sigma$. This catalog is four times larger…

We present point-source catalogs for the ~2 Ms exposure of the Chandra Deep Field-South (CDF-S); this is one of the two most-sensitive X-ray surveys ever performed. The survey covers an area of ~436 arcmin^2 and reaches on-axis sensitivity…

The XMM-Newton Slew Survey (XSS) covers a significant fraction of the sky in a broad X-ray bandpass. Although shallow by contemporary standards, in the `classical' 2-10 keV band of X-ray astronomy, the XSS provides significantly better…

宇宙学与河外天体物理 · 物理学 2015-06-11 R. S. Warwick , R. D. Saxton , A. M. Read

We present a new edition of the catalogue of high-mass X-ray binaries in the Galaxy. The catalogue contains source name(s), coordinates, finding chart, X-ray luminosity, system parameters, and stellar parameters of the components and other…

天体物理学 · 物理学 2008-11-26 Q. Z. Liu , J. van Paradijs , E. P. J. van den Heuvel

We present multi-waveband optical imaging data obtained from observations of the Subaru/XMM-Newton Deep Survey (SXDS). The survey field, centered at R.A.=02:18:00, decl.=-05:00:00, has been the focus of a wide range of multi-wavelength…

We present a sample of eight extended X-ray sources detected in the wide-field (~2.3 deg^2), bright (2-10 ksec) XMM-Newton/2dF survey, reaching a flux limit of ~2 X 10^{-14} erg/s/cm^2. Of these, seven are identified as secure X-ray…

天体物理学 · 物理学 2010-03-19 T. Gaga , M. Plionis , S. Basilakos , I. Georgantopoulos , A. Georgakakis

We present a detailed analysis of the stellar content of the current version of the XMM-Newton slew survey (XMMSL2). Since stars emit only a small fraction of their total luminosity in the X-ray band, the stellar XMMSL2 sources ought to…

太阳与恒星天体物理 · 物理学 2018-07-04 S. Freund , J. Robrade , C. Schneider , J. H. M. M. Schmitt

XMM and Chandra opened a new area for the study of clusters of galaxies. Not only for cluster physics but also, for the detection of faint and distant clusters that were inaccessible with previous missions. This article presents 66…

(Abridged) This paper presents the data recently released for the XMM-Newton/WFI survey carried out as part of the ESO Imaging Survey (EIS) project. The aim of this survey is to provide optical imaging follow-up data in BVRI for…

We present X-ray and optical spectroscopic observations of twelve galaxy groups and clusters identified within the XMM Large-Scale Structure (LSS) survey. Groups and clusters are selected as extended X-ray sources from a 3.5 deg2 XMM image…

[ABRIGED] We present the optical identification of a sample of 695 X-ray sources detected in the first 1.3 deg^2 of the XMM-COSMOS survey, down to a 0.5-2 keV (2-10 keV) limiting flux of ~10^-15 erg cm-2 s-1 (~5x10^-15 erg cm^-2 s-1). We…

The XXL survey currently covers two 25 sq. deg. patches with XMM observations of ~10ks. We summarise the scientific results associated with the first release of the XXL data set, that occurred mid 2016. We review several arguments for…

星系天体物理 · 物理学 2017-07-12 M. Pierre , C. Adami , M. Birkinshaw , L. Chiappetti , S. Ettori , A. Evrard , L. Faccioli , F. Gastaldello , P. Giles , C. Horellou , A. Iovino , E. Koulouridis , C. Lidman , A. Le Brun , B. Maughan , S. Maurogordato , I. McCarthy , S. Miyazaki , F. Pacaud , S. Paltani , M. Plionis , T. Reiprich , T. Sadibekova , V. Smolcic , S. Snowden , J. Surdej , M. Tsirou , C. Vignali , J. Willis , S. Alis , B. Altieri , N. Baran , C. Benoist , A. Bongiorno , M. Bremer , A. Butler , A. Cappi , C. Caretta , P. Ciliegi , N. Clerc , P. S. Corasaniti , J. Coupon , J. Delhaize , I. Delvecchio , J. Democles , Sh. Desai , J. Devriendt , Y. Dubois , D. Eckert , A. Elyiv , A. Farahi , C. Ferrari , S. Fotopoulou , W. Forman , I. Georgantopoulos , V. Guglielmo , M. Huynh , N. Jerlin , Ch. Jones , S. Lavoie , J. -P. Le Fevre , M. Lieu , M. Kilbinger , F. Marulli , A. Mantz , S. McGee , J. -B. Melin , O. Melnyk , L. Moscardini , M. Novak , E. Piconcelli , B. Poggianti , D. Pomarede , E. Pompei , T. Ponman , M. E. Ramos Ceja , P. Ranalli , D. Rapetti , S. Raychaudhury , M. Ricci , H. Rottgering , M. Sahlén , J. -L. Sauvageot , C. Schimd , M. Sereno , G. P. Smith , K. Umetsu , P. Valageas , A. Valotti , I. Valtchanov , A. Veropalumbo , B. Ascaso , D. Barnes , M. De Petris , F. Durret , M. Donahue , M. Ithana , M. Jarvis , M. Johnston-Hollitt , E. Kalfountzou , S. Kay , F. La Franca , N. Okabe , A. Muzzin , A. Rettura , F. Ricci , J. Ridl , G. Risaliti , M. Takizawa , P. Thomas , N. Truong

We present the 1SXPS (Swift-XRT Point Source) catalog of 151,524 X-ray point-sources detected by the Swift-XRT in 8 years of operation. The catalog covers 1905 square degrees distributed approximately uniformly on the sky. We analyze the…

We present the 2SXPS (Swift-XRT Point Source) catalog, containing 206,335 point sources detected by the Swift X-ray Telescope (XRT) in the 0.3--10 keV energy range. This catalog represents a significant improvement over 1SXPS, with double…

We present preliminary results on the optical identifications of sources from the High Energy Large Area Survey performed with XMM-Newton (HELLAS2XMM). This survey covers about 3 square degrees of sky down to a 2-10 keV flux of 7 x 10^-15…

We present the X-ray point-source catalogs in two of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) fields, W-CDF-S (4.6 deg$^2$) and ELAIS-S1 (3.2 deg$^2$), aiming to fill the gap between deep pencil-beam X-ray…

(abridged) The XMM-Newton survey in the Chandra Deep Field South (XMM-CDFS) aims at detecting and studying the spectral properties of a significant number of obscured and Compton-thick AGN. The large effective area of XMMin the 2--10 and…