A dataset provided by the European Space Agency

Name 13358
Title Trans-iron group elements in the hot white dwarf RE 0503-289
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13358;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-pwb70i6
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=13358&mission=hst
Publication Complete spectral energy distribution of the hot, helium-rich white dwarf <<>>RX J0503.9-2854>>, Hoyer, D.,Rauch, T.,Werner, K., Astronomy and Astrophysics, 598, 2017-02-01 00:00:00, 2017A&A...598A.135H||First detection of bromine and antimony in hot stars, Werner, K.,Rauch, T.,Knörzer, M., Astronomy and Astrophysics, 614, 2018-06-01 00:00:00, 2018A&A...614A..96W||Stellar laboratories. IV. New Ga iv, Ga v, and Ga vi oscillator strengths and the gallium abundance in the hot white dwarfs <<>>G191-B2B>> and RE 0503-289, Rauch, T.,Werner, K.,Quinet, P., Astronomy and Astrophysics, 577, 2015-05-01 00:00:00, 2015A&A...577A...6R||Stellar laboratories . IX. New Se v, Sr iv-vii, Te vi, and I vi oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191-B2B and RE 0503-289, Rauch, T.,Quinet, P.,Knörzer, M., Astronomy and Astrophysics, 606, 2017-10-01 00:00:00, 2017A&A...606A.105R||Stellar laboratories . VIII. New Zr iv-vii, Xe iv-v, and Xe vii oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs <<>>G191-B2B>> and <<>>RE 0503-289>>, Rauch, T.,Gamrath, S.,Quinet, P., Astronomy and Astrophysics, 599, 2017-03-01 00:00:00, 2017A&A...599A.142R||Stellar laboratories. VII. New Kr iv - vii oscillator strengths and an improved spectral analysis of the hot, hydrogen-deficient DO-type white dwarf <<>>RE 0503-289>>, Rauch, T.,Quinet, P.,Hoyer, D., Astronomy and Astrophysics, 590, 2016-05-01 00:00:00, 2016A&A...590A.128R||Stellar laboratories. VI. New Mo iv-vii oscillator strengths and the molybdenum abundance in the hot white dwarfs G191-B2B and RE 0503-289, Rauch, T.,Quinet, P.,Hoyer, D., Astronomy and Astrophysics, 587, 2016-03-01 00:00:00, 2016A&A...587A..39R||Stellar laboratories. V. The Xe vi ultraviolet spectrum and the xenon abundance in the hot DO-type white dwarf <<>>RE 0503-289...BJ>>, Rauch, T.,Hoyer, D.,Quinet, P., Astronomy and Astrophysics, 577, 2015-05-01 00:00:00, 2015A&A...577A..88R||Stellar laboratories. X. New Cu IV-VII oscillator strengths and the first detection of copper and indium in hot white dwarfs, Rauch, T.,Gamrath, S.,Quinet, P., Astronomy and Astrophysics, 637, 2020-05-01 00:00:00, 2020A&A...637A...4R||The prospective search for highly ionized technetium in hot (pre-) white dwarfs, Werner, K.,Rauch, T.,Kučas, S., Astronomy and Astrophysics, 574, 2015-02-01 00:00:00, 2015A&A...574A..29W
Instrument STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2014-08-14T08:56:11Z/2014-08-14T12:53:35Z
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 2015-08-14T19:45:13Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015, Trans-Iron Group Elements In The Hot White Dwarf Re 0503-289, 1.0, European Space Agency, https://doi.org/10.5270/esa-pwb70i6