A dataset provided by the European Space Agency

Name 12010
Title COS FUV Line Spread Function Characterization
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12010;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-xwbhyjx
Author Ghavamian, Parviz
Description This is a scientific proposal for HST mission. For specific information please visit https:archive.stsci.eduproposal_search.php?id=12010&mission=hst
Publication Optical Emission of the Ultraluminous X-Ray Source NGC 5408 X-1: Donor Star or Irradiated Accretion Disk?, Grisé, F.,Kaaret, P.,Corbel, S., The Astrophysical Journal, 745, 2012-02-01 00:00:00, 2012ApJ...745..123G||Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs, Pinto, C.,Mehdipour, M.,Walton, Dominic J., Monthly Notices of the Royal Astronomical Society, 491, 2020-02-01 00:00:00, 2020MNRAS.491.5702P
Temporal Coverage 2009-09-23T21:25:05Z/2009-09-23T23:50:39Z
Version V1.0
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 2009-09-24 03:45:34
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009, 12010, V1.0. https://doi.org/10.5270/esa-xwbhyjx