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HST HUDF ACS/WFC3 Image

HST HUDF ACS/WFC3 Image

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    03h 32m 38.01s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -27° 46' 39.08"
  • 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.
    These images were created from Hubble data from proposals 12060 (PI: S. Faber, University of California, Santa Cruz) and 12099 (PI: A. Riess (STScI/JHU). The lead author on the paper is S. Rodney (JHU).
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/WFC and HST>WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    2010 and 2011
  • Filters
    FiltersThe camera filters that were used in the science observations.
    ACS/WFC: F435W (B), F606W (V), F775W (i), and F850LPW (z); WFC3/IR: F105W (Y), F125W (J), and F160W (H)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Hubble Ultra Deep Field, HUDF
  • Object Description
    Object DescriptionThe type of astronomical object.
    Deep survey
  • Release Date
    January 11, 2012
  • Science Release
    NASA’s Hubble Breaks New Ground with Distant Supernova Discovery
  • Credits
    NASA, ESA, A. Riess (STScI and JHU), and S. Rodney (JHU)

Downloads

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  • 1000 × 746
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  • 200 × 200
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  • 400 × 298
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  • 1280 × 955
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HST HUDF ACS/WFC3 Image
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

This image is a composite of separate exposures acquired by the WFC3 and ACS instruments on HST. Several filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F435W (B) + F606W (V) Green: F775W (i) + F850LPW (z) Red: F105W (Y) + F125W (J) + F160W (H)

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Details

Last Updated
Feb 17, 2025
Contact
Media

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