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Extreme Emission Line Galaxies in the Ultra Deep Survey (UDS)

Extreme Emission Line Galaxies in the Ultra Deep Survey (UDS)

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    02h 17m 24s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -05° 12' 00"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Cetus

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 proposal 12064: S. Faber (University of California, Santa Cruz), et al. The science team for this release is led by A. van der Wel (Max Planck Institute for Astronomy, Heidelberg, Germany), and the images were produced by A. Koekemoer (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: F606W (V) and F814W (I) WFC3/IR: F125W (J) and F160W (H)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Distant galaxies in Ultra Deep Survey (UDS) field
  • Object Description
    Object DescriptionThe type of astronomical object.
    Distant galaxies
  • Release Date
    November 10, 2011
  • Science Release
    Hubble Uncovers Tiny Galaxies Bursting with Star Birth in Early Universe
    Read the release
  • Credit
    NASA, ESA, A. van der Wel (Max Planck Institute for Astronomy, Heidelberg, Germany), H. Ferguson and A. Koekemoer (STScI), and the CANDELS team

Downloads

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Extreme Emission Line Galaxies in the Ultra Deep Survey (UDS)
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images are composites of many separate exposures made by the ACS and WFC3 instruments on the Hubble Space Telescope using different filters that isolate broad wavelengths. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: F606W (V) Green: F814W (I) Red: F125W (J) + F160W (H)

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GOODS South Deep (GSD)

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Hubble Spies Tiny Galaxies Aglow with Star Birth in the UDS Field

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CANDELS Ultra Deep Survey (UDS)

CANDELS Ultra Deep Survey (UDS)

CANDELS Dwarf Galaxies

CANDELS Dwarf Galaxies

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Zoom to GOODS Field

Zoom to GOODS Field

Zoom into the Hubble GOODS South Deep (GSD) field. Candidate extreme emission line galaxies are identified. This object was observed as part of the Hubble CANDELS Legacy Project.

Zoom to UDS Field

Zoom to UDS Field

Zoom into the Hubble CANDELS Ultra Deep Survey (UDS) field. Candidate extreme emission line galaxies are identified. This object was observed as part of the Hubble CANDELS Legacy Project.

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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

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