A dataset provided by the European Space Agency

Name	14111
Title	The SN Ia Candidate T Pyxidis: The Mystery of its High Accretion Rate
URL	https://hst.esac.esa.int/ehst/#/pages/search;proposal=14111;TAPCLIENT=DOI
DOI	https://doi.org/10.5270/esa-n0m561o
Author	European Space Agency
Description	This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=14111&mission=hst
Publication	The Long-term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis, Godon, Patrick,Sion, Edward M.,Williams, Robert, The Astrophysical Journal, 862, 2018-07-01 00:00:00, 2018ApJ...862...89G
Instrument	COS/FUV
Temporal Coverage	2015-10-12T23:49:19Z/2016-06-01T05:49:36Z
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	2017-06-01T08:39:22Z
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, 2017, The Sn Ia Candidate T Pyxidis: The Mystery Of Its High Accretion Rate, 1.0, European Space Agency, https://doi.org/10.5270/esa-n0m561o