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IRC 0218 Lensing Feature Without Foreground Cluster

IRC 0218 Lensing Feature Without Foreground Cluster

About the Object

  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Eridanus

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.
    The image was created from Hubble data from the following proposal: 12590, PI: C. Popovich (Texas A & M University) et al. The science team comprises: K. Wong (Academia Sinica Institute of Astronomy & Astrophysics, Taiwan), K.-V. Tran (Texas A&M University), S. Suyu (Academia Sinica Institute of Astronomy & Astrophysics, Taiwan), I. Momcheva (Yale University), G. Brammer (STScI), M. Brodwin (University of Missouri), A. Gonzalez (University of Florida), A. Halkola and G. Kacprzak (Swinburne University), A. Koekemoer (STScI), and C. Papovich (Texas A&M University).
  • 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.
    November and December 2011, Exposure Time: 3.3 hours
  • Filters
    FiltersThe camera filters that were used in the science observations.
    ACS/WFC: F475W (g) and F814W (I) WFC3/IR: F105W (Y), F125W (J), and F160W (H)
  • Object Description
    Object DescriptionThe type of astronomical object.
    Lensing feature
  • Release Date
    July 31, 2014
  • Science Release
    Hubble Shows Farthest Lensing Galaxy Yields Clues to Early Universe
  • Credit
    NASA, ESA, K.-V. Tran (Texas A&M University), and K. Wong (Academia Sinica Institute of Astronomy & Astrophysics)

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IRC 0218 Lensing Feature Without Foreground Cluster
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 ACS/WFC and WFC3/IR instruments. Several filters were used to sample various wavelengths. The color results from assigning different hues (colors) to each monochromatic (grayscale) image as follows: Blue: F475W (g) Green: F814W (I) Red: F105W (Y) + F125W (J) + F160W (H)

Compass and Scale
Compass and ScaleAn astronomical image with a scale that shows how large an object is on the sky, a compass that shows how the object is oriented on the sky, and the filters with which the image was made.

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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