A dataset provided by the European Space Agency

Name 9875
Title The Fundamental Plane of Massive Gas-Rich Mergers
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9875;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-o0nvs5i
Author Veilleux, Sylvain
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9875&mission=hst
Publication
  • A Deep Hubble Space Telescope H-Band Imaging Survey of Massive Gas-rich Mergers
  • A Deep Hubble Space Telescope H-Band Imaging Survey of Massive Gas-Rich Mergers. II. The QUEST QSOs
  • Characterization of Optically Selected Star-Forming Knots in (U)LIRGs
  • Compact Molecular Gas Distribution in Quasar Host Galaxies
  • Distributions of Quasar Hosts on the Galaxy Main Sequence Plane
  • Dynamical Properties of Ultraluminous Infrared Galaxies. I. Mass Ratio Conditions for ULIRG Activity in Interacting Pairs
  • GEMINI 3D spectroscopy of BAL + IR + FeII QSOs - I. Decoupling the BAL, QSO, starburst, NLR, supergiant bubbles and galactic wind in Mrk 231
  • Host Dynamics and Origin of Palomar-Green QSOs
  • Infrared mergers and infrared quasi-stellar objects with galactic winds - III. Mrk 231: an exploding young quasi-stellar object with composite outflow/broad absorption lines (and multiple expanding superbubbles)
  • Ionization Mechanisms in Quasar Outflows
  • Modeling the Unresolved NIR-MIR SEDs of Local (z < 0.1) QSOs
  • Physics of ULIRGs with MUSE and ALMA: The PUMA project. II. Are local ULIRGs powered by AGN? The subkiloparsec view of the 220 GHz continuum
  • Physics of ULIRGs with MUSE and ALMA: The PUMA project. III. Incidence and properties of ionised gas disks in ULIRGs, associated velocity dispersion, and its dependence on starburstiness
  • Physics of ULIRGs with MUSE and ALMA: The PUMA project. I. Properties of the survey and first MUSE data results
  • Searching for molecular outflows in hyperluminous infrared galaxies
  • The hosts and environments of local ULIRGs and QSOs
  • The Infrared Emission and Vigorous Star Formation of Low-redshift Quasars
  • The properties of the stellar populations in ULIRGs - I. Sample, data and spectral synthesis modelling
Instrument NICMOS, NICMOS/NIC2
Temporal Coverage 2003-08-26T19:29:28Z/2004-09-24T01:52:36Z
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 2005-09-24T12:21:53Z
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, Veilleux comma Sylvain, 2005, 'The Fundamental Plane of Massive Gas-Rich Mergers', 1.0, European Space Agency, https://doi.org/10.5270/esa-o0nvs5i