A dataset provided by the European Space Agency

Name	12189
Title	Do stars ionise the filaments in NGC 1275 ?
URL	https://hst.esac.esa.int/ehst/#/pages/search;proposal=12189;TAPCLIENT=DOI
DOI	https://doi.org/10.5270/esa-0qrztml
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=12189&mission=hst
Publication	Revealing the Broad Line Region of NGC 1275: The Relationship to Jet Power, Punsly, Brian,Marziani, Paola,Bennert, Vardha N., The Astrophysical Journal, 869, 2018-12-01 00:00:00, 2018ApJ...869..143P
Instrument	COS/FUV, COS/NUV
Temporal Coverage	2011-07-18T23:33:48Z/2012-02-16T08:10:30Z
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	2013-02-16T10:14:30Z
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, 2013, Do Stars Ionise The Filaments In Ngc 1275 ?, 1.0, European Space Agency, https://doi.org/10.5270/esa-0qrztml