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Compass and Scale Image for GOODS-N and GN-z11

About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.12h 36m 54.99s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.62° 14' 15.0"
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Ursa Major
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.Recent data were obtained from the HST proposal 13871, PI: P. Oesch (Yale University), G. Illingworth (University of California, Santa Cruz), I. Labbé (Leiden University), G. Brammer (STScI), R. Bouwens and M. Franx (Leiden University), P. van Dokkum (Yale University), D. Magee (UCO/Lick Observatory/University of California, Santa Cruz), I. Momcheva (Harvard-Smithsonian Center for Astrophysics), R. Smit (Durham University), M. Ashby, G. Fazio, J. Huang, and S. Willner (Harvard-Smithsonian Center for Astrophysics), V. Gonzalez (University of California, Riverside), R. Skelton (South African Astronomical Observatory), M. Trenti (University of Melbourne), and L. Spitler (Macquarie University/Australian Astronomical Observatory). The science team includes: P. Oesch (Yale University), G. Brammer (STScI), P. van Dokkum (Yale University), G. Illingworth (University of California, Santa Cruz), R. Bouwens, I. Labbé, and M. Franx (Leiden University), I. Momcheva, M. Ashby, and G. Fazio (Harvard-Smithsonian Center for Astrophysics), V. Gonzalez (University of California, Riverside), B. Holden and D. Magee (UCO/Lick Observatory/University of California, Santa Cruz), R. Skelton (South African Astronomical Observatory), R. Smit (Durham University), L. Spitler (Macquarie University/Australian Astronomical Observatory), M. Trenti (University of Melbourne), and S. Willner (Harvard-Smithsonian Center for Astrophysics). - InstrumentInstrumentThe science instrument used to produce the data.HST>ACS/WFC, and HST>WFC3/IR
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.February 11, 2015, and April 3, 2015
- FiltersFiltersThe camera filters that were used in the science observations.Main CANDELS/GOODS-N Field: HST>ACS/WFC: F435W (B), F606W (V), F814W (I), and F850LP (z), and HST> WFC3/IR: F105W (Y), F125W (J), and F160W (H) Grism Data (February 11, 2015, and April 3, 2015): HST>WFC3/IR: G141
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.GOODS North Survey, and GN-z11 (inset image)
- Object DescriptionObject DescriptionThe type of astronomical object.Farthest Galaxy Candidate from CANDELS/GOODS-N Field
- Release DateMarch 3, 2016
- Science ReleaseHubble Team Breaks Cosmic Distance Record
- Credits

The main GOODS-N composite includes exposures acquired by the ACS and WFC3 instruments on the Hubble Space Telescope. 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: F814W (I) + F850LP (z) Red: F125W (J) + F160W (H)

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