494 datasets found

Keywords: astronomical object identification

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  • XMM-Newton survey of the ELAIS-S1 field. II.

    We present the optical identifications and a multi-band catalogue of a sample of 478 X-ray sources detected in the XMM-Newton and Chandra surveys of the central 0.6deg^2^ of the...
  • XMM-LSS field optical identifications

    The XMM-Large Scale Structure survey field (XMM-LSS) is an extragalactic window surveyed in the X-ray with the XMM-Newton satellite. It has also been observed in the optical...
  • SEDs in ADFS (AKARI Deep Field South)

    We investigate the nature and properties of far-infrared (FIR) sources in the AKARI Deep Field South (ADF-S). We performed an extensive search for the counterparts to 1000 ADF-S...
  • 2XMMi/SDSS DR7 cross-correlation

    The Survey Science Centre of the XMM-Newton satellite released the first incremental version of the 2XMM catalogue in August 2008. Containing more than 220000 X-ray sources, the...
  • Coordinates for Arp's Baade's Window stars

    Identifications and coordinates for all stars in Arp's (1965ApJ...141...43A) finding chart for Baade's Window. For each star Arp's ID is presented, as are 2MASS and OGLE IDs...
  • MCXC Meta-Catalogue X-ray galaxy Clusters

    We present the compilation and properties of a meta-catalogue of X-ray detected clusters of galaxies, the MCXC. This very large catalogue is based on publicly available ROSAT...
  • YSOs in 9 LMC star forming regions

    We introduce a new set of selection criteria for the identification of infrared bright young stellar object (YSO) candidates and apply them to nine HII regions in the Large...
  • Improved astrometry bor BE74 stars

    Accurate astrometry is required to reliably cross-match 20th-century catalogues against 21st-century surveys. The present work aims to provide such astrometry for the 625...
  • XMM-Newton SSC survey of Galactic Plane

    Many different classes of X-ray sources contribute to the Galactic landscape at high energies. Although the nature of the most luminous X-ray emitters is now fairly well...
  • XMM sources in M83 (NGC5236)

    We present the results obtained from the analysis of three XMM-Newton observations of M83. The aims of the paper are studying the X-ray source populations in M83 and calculating...
  • On the metallicity of open clusters. II.

    The literature was searched for [Fe/H] estimates of individual member stars of open clusters (OCs) based on the analysis of high-resolution spectra. The lower limit for spectral...
  • XMM sources in NGC1512/1510

    The galaxy NGC1512 is interacting with the smaller galaxy NGC1510 and shows a peculiar morphology, characterised by two extended arms immersed in an HI disc whose size is about...
  • Optical counterparts of ROSAT X-ray in 2 fields

    The optical identification of large number of X-ray sources such as those from the ROSAT All-Sky Survey is challenging with conventional spectroscopic follow-up observations. We...
  • ASTRODEEP Frontier Fields Catalogues

    We present multiwavelength photometric catalogues (HST, Spitzer and Hawk-I K band) for the first two of the Frontier Fields, Abell2744 and MACSJ0416 (plus their parallel...
  • Large Quasar Astrometric Catalogue 4, LQAC-4

    From an astrometric point of view, quasars constitute the best and almost ideal reference objects in the celestial sphere, with a priori no significant proper motion. Since the...
  • Stellar content of the XMM-Newton slew survey

    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...
  • Membership probabilities of Pleiades objects

    The photometric and astrometric measurements of the Pleiades DANCe DR2 survey provide an excellent test case for the benchmarking of statistical tools aiming at the...
  • Classification-aided zph estimation

    Broadband photometry offers a time and cost effective method to reconstruct the continuum emission of celestial objects. Thus, photometric redshift estimation has supported the...
  • Census of Rho Oph candidate members from Gaia DR2

    The Ophiuchus cloud complex is one of the best laboratories to study the earlier stages of the stellar and protoplanetary disc evolution. We constructed a control sample...
  • SDSS-IV/SPIDERS X-ray PS Spectroscopic Catalog

    We look to provide a detailed description of the SPectroscopic IDentification of ERosita Sources (SPIDERS) survey, an SDSS-IV programme aimed at obtaining spectroscopic...
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