A dataset provided by the European Space Agency

Name 12200
Title STIS UV spectroscopy of a bright classical nova during its super soft X-ray phase
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12200;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-kdvirg5
Author Schwarz, Greg James
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12200&mission=hst
Publication
  • The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst. III. The ultraviolet development from iron curtain through the post-X-ray turnoff
  • The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst. II. The optically thin phase and the structure of the ejecta in recurrent novae
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2011-05-07T07:55:03Z/2011-10-04T13:38:44Z
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 2012-10-04T19:51:33Z
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, Schwarz comma Greg James, 2012, 'STIS UV spectroscopy of a bright classical nova during its super soft X-ray phase', 1.0, European Space Agency, https://doi.org/10.5270/esa-kdvirg5