Name | 13732 |
Title | Detecting dark matter substructure with narrow line lensing |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=13732;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-nlmlq6w |
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=13732&mission=hst |
Publication | Double dark matter vision: twice the number of compact-source lenses with narrow-line lensing and the WFC3 grism, Nierenberg, A. M.,Gilman, D.,Treu, T., Monthly Notices of the Royal Astronomical Society, 492, 2020-03-01 00:00:00, 2020MNRAS.492.5314N||Probing dark matter substructure in the gravitational lens HE 0435-1223 with the WFC3 grism, Nierenberg, A. M.,Treu, T.,Brammer, G., Monthly Notices of the Royal Astronomical Society, 471, 2017-10-01 00:00:00, 2017MNRAS.471.2224N||The missing satellite problem in 3D, Nierenberg, A. M.,Treu, T.,Menci, N., Monthly Notices of the Royal Astronomical Society, 462, 2016-11-01 00:00:00, 2016MNRAS.462.4473N||The primordial matter power spectrum on sub-galactic scales, Gilman, Daniel,Benson, Andrew J.,Bovy, Jo, Monthly Notices of the Royal Astronomical Society, 512, 2022-05-01 00:00:00, 2022MNRAS.512.3163G |
Instrument | WFC3, WFC3/IR |
Temporal Coverage | 2015-02-23T01:40:04Z/2015-09-15T13:02:27Z |
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 | 2016-09-15T15:48:53Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2016, Detecting Dark Matter Substructure With Narrow Line Lensing, 1.0, European Space Agency, https://doi.org/10.5270/esa-nlmlq6w |