A dataset provided by the European Space Agency

Name 14177
Title Identifying Ionization Mechanisms through Spatially-Resolved Neon Emission in the Jets of Sz 102
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14177;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-w7phdk5
Author Liu, Chun-Fan
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14177&mission=hst
Publication
  • Compositions of Planetary Debris around Dusty White Dwarfs
  • Revealing Ionization Conditions of Sz 102 with Spatially Resolved Ne III Microjets
Instrument STIS, STIS/CCD
Temporal Coverage 2016-05-06T12:41:05Z/2016-05-06T15:04:29Z
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 2017-05-06T17:51:21Z
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, Liu comma Chun-Fan, 2017, 'Identifying Ionization Mechanisms through Spatially-Resolved Neon Emission in the Jets of Sz 102', 1.0, European Space Agency, https://doi.org/10.5270/esa-w7phdk5