| Name | 12010 |
| Title | COS FUV Line Spread Function Characterization |
| URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=12010;TAPCLIENT=DOI |
| DOI | https://doi.org/10.5270/esa-xwbhyjx |
| 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=12010&mission=hst |
| Publication | Optical Emission of the Ultraluminous X-Ray Source NGC 5408 X-1: Donor Star or Irradiated Accretion Disk?, Grisé, F.,Kaaret, P.,Corbel, S., The Astrophysical Journal, 745, 2012-02-01 00:00:00, 2012ApJ...745..123G||Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs, Pinto, C.,Mehdipour, M.,Walton, Dominic J., Monthly Notices of the Royal Astronomical Society, 491, 2020-02-01 00:00:00, 2020MNRAS.491.5702P |
| Instrument | STIS/CCD, STIS/FUV-MAMA |
| Temporal Coverage | 2009-09-23T21:25:05Z/2009-09-23T23:50:39Z |
| 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 | 2009-09-24T03:45:34Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2009, Cos Fuv Line Spread Function Characterization, 1.0, European Space Agency, https://doi.org/10.5270/esa-xwbhyjx |