A dataset provided by the European Space Agency

Name 17190
Title Will the Recurrent Nova T Pyxidis Become a Type Ia Supernova?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=17190;TAPCLIENT=DOI
DOI https://doi.org/10.57780/esa-w0wue3j
Author Godon, Patrick
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=17190&mission=hst
Publication No publications found
Instrument COS, COS/FUV, COS-STIS, STIS, STIS/CCD
Temporal Coverage 2023-03-24T00:13:08Z/2023-03-24T10:30:17Z
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 2023-09-24T14:41:05Z
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, Godon comma Patrick, 2023, 'Will the Recurrent Nova T Pyxidis Become a Type Ia Supernova?', 1.0, European Space Agency, https://doi.org/10.57780/esa-w0wue3j