A dataset provided by the European Space Agency

Name 9455
Title Mid-Ultraviolet Spectral Templates for Old Stellar Systems
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9455;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-548s7xj
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=9455&mission=hst
Publication
  • Boron Abundances Across the Li-Be Dip in the Hyades Cluster
  • Chemical diversity among A-B stars with low rotational velocities: non-LTE abundance analysis
  • CoolCAT
  • 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 Neutral Phosphorus in the Near-ultraviolet Spectra of Late-type Stars
  • Detection of the Second r-process Peak Element Tellurium in Metal-poor Stars
  • Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
  • Germanium, Arsenic, and Selenium Abundances in Metal-poor Stars
  • High-resolution spectroscopy of the hot Am star HR 3383
  • Hot Populations in M87 Globular Clusters
  • Improved oscillator strengths and wavelengths in Hf II, with applications to stellar elemental abundances
  • In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
  • Mg II h + k Flux--Rotational Period Correlation for G-type Stars
  • 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 Chemical Evolution of Phosphorus
  • The Extreme Overabundance of Molybdenum in Two Metal-poor Stars
  • The Radiation Environments of Middle-aged F-type Stars
  • The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
  • 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
  • Ultraviolet spectral synthesis of HD 72660
  • UV bright globular clusters in M87: more evidence for super-He-rich stellar populations?
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2002-08-21T16:54:51Z/2003-09-19T20:39:29Z
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 2003-09-20T01:04:51Z
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., 2003, 'Mid-Ultraviolet Spectral Templates for Old Stellar Systems', 1.0, European Space Agency, https://doi.org/10.5270/esa-548s7xj