A dataset provided by the European Space Agency

Name 13312
Title The Evolution of C/O in Low Metallicity Dwarf Galaxies
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13312;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-sdo6h0y
Author Berg, Danielle
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=13312&mission=hst
Publication
  • A Comparison of UV and Optical Metallicities in Star-forming Galaxies
  • Carbon and Oxygen Abundances in Low Metallicity Dwarf Galaxies
  • Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies
  • High-mass X-ray binaries in nearby metal-poor galaxies: on the contribution to nebular He II emission
  • Modeling the High-energy Ionizing Output from Simple Stellar and X-Ray Binary Populations
Instrument COS, COS/FUV
Temporal Coverage 2013-10-16T00:43:24Z/2014-07-13T15:16:57Z
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 2015-07-13T21:41:26Z
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, Berg et al., 2015, 'The Evolution of C/O in Low Metallicity Dwarf Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-sdo6h0y