A dataset provided by the European Space Agency

Name 15179
Title Astrophysics Meets Atomic Physics: Fe I Line Identifications and Templates for Old Stellar Populations from Warm and Hot Stellar UV Spectra
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15179;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-o9xyv79
Author Peterson, Ruth C.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15179&mission=hst
Publication
  • High-resolution spectroscopy of the hot Am star HR 3383
  • New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra
Instrument STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage 2018-02-04T19:18:17Z/2019-05-27T16:38:08Z
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 2019-05-28T02:13:19Z
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, Peterson comma Ruth C., 2019, 'Astrophysics Meets Atomic Physics: Fe I Line Identifications and Templates for Old Stellar Populations from Warm and Hot Stellar UV Spectra', 1.0, European Space Agency, https://doi.org/10.5270/esa-o9xyv79