Name | 15179 |
Title | Astrophysics Meets Atomic Physics: Fe I Line Identifications and Templates for Old Stellar Populations from Warm and Hot Stellar UV Spectra |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=15179;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-o9xyv79 |
Author | European Space Agency |
Description | This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=15179&mission=hst |
Publication | High-resolution spectroscopy of the hot Am star HR 3383, Wahlgren, G. M.,Nielsen, Krister,Leckrone, D. S., Monthly Notices of the Royal Astronomical Society, 500, 2021-01-01 00:00:00, 2021MNRAS.500.2451W||New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra, Peterson, Ruth C.,Kurucz, Robert L., The Astrophysical Journal Supplement Series, 260, 2022-06-01 00:00:00, 2022ApJS..260...28P |
Instrument | STIS/CCD, STIS/NUV-MAMA |
Temporal Coverage | 2018-02-04T19:18:17Z/2019-05-27T16:38:08Z |
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 | 2019-05-28T02:13:19Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2019, Astrophysics Meets Atomic Physics: Fe I Line Identifications And Templates For Old Stellar Populations From Warm And Hot Stellar Uv Spectra, 1.0, European Space Agency, https://doi.org/10.5270/esa-o9xyv79 |