A dataset provided by the European Space Agency

Name 14232
Title STIS Observations of Metal-Poor Stars: Direct Confrontation with Nucleosynthetic Predictions
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14232;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-mcw655y
Author Roederer, Ian U.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14232&mission=hst
Publication
  • Atomic Transition Probabilities for Transitions of Si I and Si II and the Silicon Abundances of Several Very Metal-poor Stars
  • Consistent Iron Abundances Derived from Neutral and Singly Ionized Iron Lines in Ultraviolet and Optical Spectra of Six Warm Metal-poor Stars
  • Detailed Iron-peak Element Abundances in Three Very Metal-poor Stars
  • Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
  • In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Instrument STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage 2016-02-16T22:30:57Z/2017-01-08T00:13:47Z
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 2018-01-09T00:20:52Z
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, Roederer et al., 2018, 'STIS Observations of Metal-Poor Stars: Direct Confrontation with Nucleosynthetic Predictions', 1.0, European Space Agency, https://doi.org/10.5270/esa-mcw655y