A dataset provided by the European Space Agency

Name 14072
Title The Evolution of Metal-rich Asymptotic Giant Branch Stars
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14072;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-w72kfdd
Author Boyer, Martha L.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14072&mission=hst
Publication
  • A Dramatic Decrease in Carbon Star Formation in M31
  • PHAT XX. AGB Stars and Other Cool Giants in M31 Star Clusters
  • The impact of satellite trails on Hubble Space Telescope observations
Instrument ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage 2016-07-11T22:21:23Z/2017-02-11T08:56:26Z
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 2018-02-11T13:53:36Z
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, Boyer et al., 2018, 'The Evolution of Metal-rich Asymptotic Giant Branch Stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-w72kfdd