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GN-z10-2 Detail
About the Data
- Data DescriptionData 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 science team members are G. Illingworth (University of California, Santa Cruz), P. Oesch (University of California, Santa Cruz; Yale University), R. Bouwens, I. Labbé, R. Smit, and M. Franx (Leiden University), P. van Dokkum and I. Momcheva (Yale University), M. Ashby, G. Fazio, J.-S. Huang, and S. Willner (Harvard-Smithsonian Center for Astrophysics), V. Gonzalez (University of California, Riverside), D. Magee (University of California, Santa Cruz), M. Trenti (University of Cambridge), G. Brammer (STScI), R. Skelton (South African Astronomical Observatory), and L. Spitler (Macquarie University/AAO). - InstrumentInstrumentThe science instrument used to produce the data.HST>WFC3/IR
- FiltersFiltersThe camera filters that were used in the science observations.F105W (Y), F125W (J) and F160W (H)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.GN-z10-2
- Object DescriptionObject DescriptionThe type of astronomical object.Distant galaxy
- Release DateJanuary 7, 2014
- Science ReleaseNASA Great Observatories Team Up to Discover Ultra-Bright Young Galaxies
- Credit
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.
Blue: F105W Green: F125W Red: F160W

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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Last Updated
Mar 28, 2025
Contact
Media
Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov