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Four Galaxies from HUDF WFC3/G141 Emission-Line Galaxies Sample

Four Galaxies from HUDF WFC3/G141 Emission-Line Galaxies Sample

This is a montage of four small, young galaxies taken from a Hubble Space Telescope Wide Field Camera 3 slitless grism sample of 28 low-mass galaxies located 10 billion light-years away in the Hubble Ultra Deep Field region of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). These color images were generated from exposures in six different Hubble filters and provide detailed information about the different wavelengths of light coming from the galaxies. Astronomers say this new study gives them a view of galaxies as they appeared when the universe was less than a quarter of its current age and shows that central black holes formed at an early stage in galaxy evolution.

The authors of this study to be published in the Astrophysical Journal are Jonathan Trump, Dale Kocevski, Elizabeth McGrath, David Koo, Sandra Faber, Mark Mozena, and Hassen Yesuf (University of California, Santa Cruz); Benjamin Weiner and Stephanie Juneau (Steward Observatory); Claudia Scarlata (University of Minnesota); Eric Bell (University of Michigan); Elise Laird and Cyprian Rangel (Imperial College of London); Renbin Yan (New York University); Hakim Atek and Harry Teplitz (Spitzer Science Center, Caltech); Mark Dickinson and Jeyhan Kartaltepe (National Optical Astronomical Observatories); Jennifer Donley, Henry Ferguson, Norman Grogin, and Anton Koekemoer (Space Telescope Science Institute); James Dunlop (University of Edinburgh); Steven Finkelstein (Texas A&M University); Nimish Hathi (Carnegie Observatories); Kirpal Nandra (Max Planck Institute for Extraterrestrial Physics); Jeffrey Newman (University of Pittsburgh); Steven Rodney (Johns Hopkins University); and Amber Straughn (Goddard Space Flight Center).

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    03h 32m 39.99s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -27° 48' 0.0"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Fornax

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    This image was created from HST data from proposals 12060: S. Faber (University of California, Santa Cruz) et al. and 9425: M. Giavalisco (University of Massachusettes) et al. The science team for this release is led by J. Trump (University of California, Santa Cruz) and the images were produced by A. Koekemoer (STScI). The CANDELS Team is led by S. Faber (University of California, Santa Cruz) and H. Ferguson (STScI).
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/WFC and HST>WFC3/IR
  • Filters
    FiltersThe camera filters that were used in the science observations.
    ACS/WFC: F435W (B) F606W (V), F775W (i), and F850LP (z) WFC3/IR: F125W (J) and F160W (H)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    CANDELS Galaxies in the GOODS/HUDF Region
  • Object Description
    Object DescriptionThe type of astronomical object.
    Young galaxies
  • Release Date
    September 15, 2011
  • Science Release
    Even Low-Mass Galaxies Can Harbor Supermassive Black Holes
  • Credit
    NASA, ESA, A. Koekemoer (STScI), J. Trump, S. Faber (University of California, Santa Cruz), H. Ferguson (STScI), and the CANDELS Team

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Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov