A dataset provided by the European Space Agency

Name 9491
Title The Oxygen Abundance in the Metal-Poor Halo Star HD 140283 from UV-OH lines
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9491;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-0m8fzse
Author Balachandran, Suchitra
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9491&mission=hst
Publication
  • New Fe I Level Energies and Line Identifications from Stellar Spectra
  • New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra
  • The Extreme Overabundance of Molybdenum in Two Metal-poor Stars
  • Trans-iron Ge, As, Se, and heavier elements in the dwarf metal-poor stars HD 19445, HD 84937, HD 94028, HD 140283, and HD 160617
Instrument STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage 2003-07-11T02:27:08Z/2003-07-24T17:48:31Z
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 2007-01-23T00:07:11Z
Last Update 2025-01-25
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, Balachandran et al., 2007, 'The Oxygen Abundance in the Metal-Poor Halo Star HD 140283 from UV-OH lines', 1.0, European Space Agency, https://doi.org/10.5270/esa-0m8fzse