A dataset provided by the European Space Agency

Name 10768
Title Locating the Ultraluminous X-Ray Source in IC 342
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10768;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-6sthpyx
Author Kaaret, Philip
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=10768&mission=hst
Publication
  • Black Hole Powered Nebulae and a Case Study of the Ultraluminous X-Ray Source IC 342 X-1
  • Compact Optical Counterparts of Ultraluminous X-Ray Sources
  • Distance to the galaxy IC 342
  • Optical Counterpart of the Ultraluminous X-Ray Source IC 342 X-1
  • Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
  • Roche-lobe Overflow Systems Powered by Black Holes in Young Star Clusters: The Importance of Dynamical Exchanges
  • The impact of satellite trails on Hubble Space Telescope observations
Instrument ACS, ACS/WFC
Temporal Coverage 2005-12-16T01:32:21Z/2005-12-18T22:27:48Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2007-06-29T19:27:36Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Kaaret comma Philip, 2007, 'Locating the Ultraluminous X-Ray Source in IC 342', 1.0, European Space Agency, https://doi.org/10.5270/esa-6sthpyx