753 datasets found

Keywords: magellanic clouds

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  • OGLE II SMC eclipsing binaries

    We present new version of the OGLE-II catalog of eclipsing binary stars detected in the Small Magellanic Cloud, based on Difference Image Analysis catalog of variable stars in...
  • OGLE RR Lyrae in LMC

    We present the catalog of RR Lyr stars discovered in a 4.5 square degrees area in the central parts of the Large Magellanic Cloud (LMC). Presented sample contains 7612 objects,...
  • OGLE eclipsing binaries in LMC

    We present the catalog of 2580 eclipsing binary stars detected in 4.6 square degree area of the central parts of the Large Magellanic Cloud. The photometric data were collected...
  • OGLE II SMC RR Lyrae stars

    We present the catalog of RR Lyrae stars from 2.4 square degrees of central parts of the Small Magellanic Cloud (SMC). The photometric data were collected during four years of...
  • QSO candidates in OGLE-II data

    A search for faint slowly variable objects was undertaken in the hope of finding QSO candidates behind the Small and Large Magellanic Clouds (SMC and LMC). This search used the...
  • OGLE high proper motion stars towards MC

    We present a catalog of high proper motion (HPM) stars detected in the foreground of central parts of the Magellanic Clouds. The Catalog contains 2161 objects in the 4.5 square...
  • OGLE DIA. Catalog of LMC and SMC images

    We present the first edition of a catalog of variable stars found in the Magellanic Clouds using OGLE-II data obtained during four years: 1997-2000. The catalog covers about 7...
  • OGLE Multiple Cluster Candidates in LMC

    We present 100 multiple cluster candidates selected from the OGLE catalog of star clusters in the Large Magellanic Cloud. Statistical analysis shows that the significant...
  • OGLE LMC star clusters

    We present results of age determination based on the standard procedure of isochrone fitting for about 600 star clusters younger than about 1.2Gyr from the central parts of the...
  • OGLE LMC BVI photometry

    We present the BVI photometric maps of the Large Magellanic Cloud. They contain BVI photometry and astrometry of more than 7 million stars from the central parts of the LMC. The...
  • OGLE LMC & SMC Cepheids VI photometry

    We present Cepheids located in the close neighborhood of star clusters from the Magellanic Clouds. 204 and 132 such stars were found in the LMC and SMC, respectively. The lists...
  • OGLE LMC star clusters BVI photometry

    We present the catalog of star clusters found in the area of about 5.8 square degree in the central regions of the Large Magellanic Cloud. It contains data for 745 clusters. 126...
  • BVI photometry of OGLE SMC Cepheids

    We present the Catalog of Cepheids from the SMC which contains data for 2049 objects detected in the 2.4 square degree area of central parts of the SMC. For each object period,...
  • Radio continuum study of the MC

    By comparing Parkes telescope radio surveys with the X-ray ROSAT All-Sky Survey (RASS) we have found 71 discrete sources of both radio and X-ray emission in the Large Magellanic...
  • Compact Radio Sources in & behind LMC catalogue

    We present the results of a continuum snapshot survey of a 3x4{deg}^2^ region of the Large Magellanic Cloud including the area of the giant molecular cloud and the 30 Doradus...
  • X-Shooting ULLYSES II. Data Release 1

    The XShootU project aims to obtain ground-based optical to near-infrared spectroscopy of all targets observed by the Hubble Space Telescope (HST) under the Director's...
  • NGC 1835 F300X, F606W and F814W photometry

    In the context of the study of the size-age relationship observed in star clusters in the Large Magellanic Cloud and the investigation of its origin, here we present the...
  • SuperCAM CO(3-2) APEX survey in SMC

    The Small Magellanic Cloud (SMC) is an ideal laboratory for studying the properties of star-forming regions thanks to its low metallicity, which has an impact on the molecular...
  • New QSOs behind the Magellanic Clouds. II.

    Quasi-stellar objects (QSOs) are a basis for an absolute reference system for astrometric studies. There is a need for creating such system behind nearby galaxies, to facilitate...
  • SMC AGN in XMM-Newton

    Finding active galactic nuclei (AGN) behind the Magellanic Clouds (MCs) is difficult because of the high stellar density in these fields. Although the first AGN behind the Small...
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