A dataset provided by the European Space Agency

Name 12265
Title Determining the Physical Nature of a Unique Giant Lya Emitter at z=6.595
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12265;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-yfbgx9p
Author Ouchi, Masami
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12265&mission=hst
Publication
  • ALMA Detection of Extended C II Emission in Himiko at z = 6.6
  • An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
  • An Intensely Star-forming Galaxy at z ~ 7 with Low Dust and Metal Content Revealed by Deep ALMA and HST Observations
  • Deep rest-frame far-UV spectroscopy of the giant Lyman a emitter `Himiko
  • Faint Submillimeter Galaxies Revealed by Multifield Deep ALMA Observations: Number Counts, Spatial Clustering, and a Dark Submillimeter Line Emitter
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
  • The missing light of the Hubble Ultra Deep Field
Instrument WFC3, WFC3/IR
Temporal Coverage 2010-09-09T17:55:44Z/2010-09-30T15:46:30Z
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 2011-09-30T21:15:59Z
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, Ouchi comma Masami, 2011, 'Determining the Physical Nature of a Unique Giant Lya Emitter at z=6.595', 1.0, European Space Agency, https://doi.org/10.5270/esa-yfbgx9p