Name
13027
Title
Escape of Lyman photons from Tololo 1247-232
URL
https://hst.esac.esa.int/ehst/#/pages/search;proposal=13027;TAPCLIENT=DOI
DOI
https://doi.org/10.5270/esa-hwqcp4x
Author
Oestlin, Goeran
Description
This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=13027&mission=hst
Publication
Accurately predicting the escape fraction of ionizing photons using rest-frame ultraviolet absorption lines Lyman-I+- spectral properties of five newly discovered Lyman continuum emitters Lyman-a spectral properties of five newly discovered Lyman continuum emitters Mapping Lyman Continuum Escape in Tololo 1247-232 The impact of satellite trails on Hubble Space Telescope observations The Lyman Alpha Reference Sample. XII. Morphology of extended Lyman alpha emission in star-forming galaxies The Lyman continuum escape and ISM properties in Tololo 1247-232 - new insights from HST and VLA The Lya Reference Sample. XIV. Lya Imaging of 45 Low-redshift Star-forming Galaxies and Inferences on Global Emission Using Lyman-a to detect galaxies that leak Lyman continuum
Instrument
ACS, ACS/SBC, COS, COS/FUV, COS/NUV, WFC3, WFC3/UVIS
Temporal Coverage
2013-02-03T02:24:29Z/2013-07-18T13:11:03Z
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
2014-07-18T23:22:27Z
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, Oestlin et al., 2014, 'Escape of Lyman photons from Tololo 1247-232', 1.0, European Space Agency, https://doi.org/10.5270/esa-hwqcp4x Copy Example
