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  2. Hubble Deep Field - Wikipedia

    en.wikipedia.org/wiki/Hubble_Deep_Field

    The Hubble Deep Field (HDF) is an image of a small region in the constellation Ursa Major, constructed from a series of observations by the Hubble Space Telescope. It covers an area about 2.6 arcminutes on a side, about one 24-millionth of the whole sky, which is equivalent in angular size to a tennis ball at a distance of 100 metres. [ 1 ]

  3. List of deep fields - Wikipedia

    en.wikipedia.org/wiki/List_of_Deep_Fields

    Hubble eXtreme Deep Field: 2012: 2.3′x3′ Hubble Ultra-Deep Field (UV/VIS/NIR) 2014: Hubble Frontier Fields MACS J0416.1-2403 [10] 2015: Hubble Frontier Fields Abell 2744 [11] 2015: Hubble Frontier Fields MACS J0717.5+3745: 2015: Hubble Frontier Fields MACS J1149.5+2223 [12] 2015: Hubble Frontier Fields Abell S1063 [13] 2016: Hubble Frontier ...

  4. Near Infrared Camera and Multi-Object Spectrometer - Wikipedia

    en.wikipedia.org/wiki/Near_Infrared_Camera_and...

    NICMOS was installed on Hubble during its second servicing mission in 1997 along with the Space Telescope Imaging Spectrograph, replacing two earlier instruments.. NICMOS in turn has been largely superseded by the Wide Field Camera 3, which has a much larger field of view (135 by 127 arcsec, or 2.3 by 2.1 arcminutes), and reaches almost as far into the in

  5. Great Observatories Origins Deep Survey - Wikipedia

    en.wikipedia.org/wiki/Great_Observatories...

    The Great Observatories Origins Deep Survey, or GOODS, is an astronomical survey combining deep observations from three of NASA's Great Observatories: the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory, along with data from other space-based telescopes, such as XMM Newton, and some of the world's most powerful ground-based telescopes.

  6. Photometric system - Wikipedia

    en.wikipedia.org/wiki/Photometric_system

    GOODS (Hubble ACS) B = 435 nm V = 606 nm i = 775 nm z = 850 nm Advanced Camera for Surveys on the Hubble Space Telescope HAWC+ Band 1 = 53 μm Band 2 = 89 μm Band 3 = 154 μm Band 4 = 214 μm High-resolution Airborne Wideband Camera+ for SOFIA [15] HDF 450 nm 606 nm 814 nm Hubble Deep Field from the Hubble Space Telescope: IRTF NSFCAM

  7. Cosmic Assembly Near-infrared Deep Extragalactic Legacy ...

    en.wikipedia.org/wiki/Cosmic_Assembly_Near...

    Hubble image of a field of galaxies with high redshift (z = 7.7). [1]The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) is the largest project in the history of the Hubble Space Telescope, with 902 assigned orbits (about 60 continuous days [2]) of observing time.

  8. Robert Williams (astronomer) - Wikipedia

    en.wikipedia.org/wiki/Robert_Williams_(astronomer)

    This historic project resulted in the Hubble Deep Field, a landmark image showing in remarkable detail the structure of galaxies in the early universe. For his leadership of this project, he was awarded the 1998 Beatrice M. Tinsley Prize , [ 6 ] the NASA Distinguished Public Service Medal in 1999, [ 7 ] and the 2016 Karl Schwarzschild Medal .

  9. Drizzle (image processing) - Wikipedia

    en.wikipedia.org/wiki/Drizzle_(image_processing)

    Drizzle (or DRIZZLE) is a digital image processing method for the linear reconstruction of undersampled images. The method is normally used for the combination of astronomical images and was originally developed for the Hubble Deep Field observations made by the Hubble Space Telescope.

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