A dataset provided by the European Space Agency

Name 14161
Title The Intersection of Atomic Physics and Astrophysics: Identifying UV Fe I Lines from Metal-Poor Turnoff Stars
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14161;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-o19o4r5
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=14161&mission=hst
Publication
  • Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937
  • A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu II and Zn II Lines
  • Atomic Transition Probabilities for Transitions of Si I and Si II and the Silicon Abundances of Several Very Metal-poor Stars
  • Atomic Transition Probabilities of Neutral Calcium
  • Consistent Iron Abundances Derived from Neutral and Singly Ionized Iron Lines in Ultraviolet and Optical Spectra of Six Warm Metal-poor Stars
  • Copper abundance from Cu I and Cu II lines in metal-poor star spectra: NLTE versus LTE
  • Correlating Intrinsic Stellar Parameters with Mg II Self-reversal Depths
  • Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
  • Detection of Pb II in the Ultraviolet Spectra of Three Metal-poor Stars
  • Galactic evolution of copper in the light of NLTE computations
  • Influence of Collisions with Hydrogen on Titanium Abundance Determinations in Cool Stars
  • In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
  • New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra
  • New Fe I Level Energies and Line Identifications from Stellar Spectra. II. Initial Results from New Ultraviolet Spectra of Metal-poor Stars
  • Non-LTE aluminium abundances in late-type stars
  • The Abundance of Lead in Four Metal-poor Stars
  • The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
  • The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925
  • 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 2016-03-09T11:09:22Z/2016-07-16T20:20:15Z
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 2016-07-17T02:31:18Z
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., 2016, 'The Intersection of Atomic Physics and Astrophysics: Identifying UV Fe I Lines from Metal-Poor Turnoff Stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-o19o4r5