| Name | 14660 |
| Title | Morphology and Orientation of QSO Absorber Host Galaxies at z<1.5 Detected with VLT/MUSE1/st |
| URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=14660;TAPCLIENT=DOI |
| DOI | https://doi.org/10.5270/esa-dw4j1qw |
| 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=14660&mission=hst |
| Publication | Characterizing circumgalactic gas around massive ellipticals at z ≈ 0.4 - III. The galactic environment of a chemically pristine Lyman limit absorber, Chen, Hsiao-Wen,Johnson, Sean D.,Straka, Lorrie A., Monthly Notices of the Royal Astronomical Society, 484, 2019-03-01 00:00:00, 2019MNRAS.484..431C||Directly Tracing Cool Filamentary Accretion over >100 kpc into the Interstellar Medium of a Quasar Host at z = 1, Johnson, Sean D.,Schaye, Joop,Walth, Gregory L., The Astrophysical Journal, 940, 2022-12-01 00:00:00, 2022ApJ...940L..40J||Signatures of extended discs and outflows in the circumgalactic medium using the Q0107 quasar triplet, Beckett, Alexander,Morris, Simon L.,Fumagalli, M., Monthly Notices of the Royal Astronomical Society, 517, 2022-11-01 00:00:00, 2022MNRAS.517.1020B |
| Instrument | ACS, ACS/WFC |
| Temporal Coverage | 2017-06-19T23:16:23Z/2017-12-01T21:11:53Z |
| 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 | 2018-12-03T07:10:30Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2018, Morphology And Orientation Of Qso Absorber Host Galaxies At Z<1.5 Detected With Vlt/Muse1/St, 1.0, European Space Agency, https://doi.org/10.5270/esa-dw4j1qw |