A dataset provided by the European Space Agency

Name 14608
Title Host galaxies of high-redshift quasars with extreme outflows
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14608;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-qesblid
Author Zakamska, Nadia L
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14608&mission=hst
Publication
  • Evidence of extended cold molecular gas and dust haloes around z 2.3 extremely red quasars with ALMA
  • First Results from the JWST Early Release Science Program Q3D: Ionization Cone, Clumpy Star Formation, and Shocks in a z = 3 Extremely Red Quasar Host
  • First Results from the JWST Early Release Science Program Q3D: Powerful Quasar-driven Galactic Scale Outflow at z = 3
  • First Results from the JWST Early Release Science Program Q3D: Turbulent Times in the Life of a z 3 Extremely Red Quasar Revealed by NIRSpec IFU
  • Host galaxies of high-redshift extremely red and obscured quasars
  • Powerful winds in high-redshift obscured and red quasars
  • The impact of satellite trails on Hubble Space Telescope observations
Instrument ACS/WFC, WFC3/IR
Temporal Coverage 2016-12-23T18:29:57Z/2017-12-20T17:32:01Z
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 2018-12-21T01:02:58Z
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, Zakamska et al., 2018, 'Host galaxies of high-redshift quasars with extreme outflows', 1.0, European Space Agency, https://doi.org/10.5270/esa-qesblid