GOODS-S/ERS2 Field (Hubble)

 GOODS-S/ERS2 Field (Hubble)

This is a Hubble Space Telescope view of a portion of GOODS-South, the southern field of a large deep-sky study by several observatories to trace the formation and evolution of galaxies. The image shows a rich tapestry of 7,500 galaxies stretching back through most of the universe's history. The farthest galaxies, a few of the very faint red specks, are seen as they appeared more than 13 billion years ago, or roughly 650 million years after the Big Bang. Soon, the James Webb Space Telescope will peer back even farther into this field to trace the formation and evolution of the very first galaxies.

Credits

Image

NASA, ESA, Rogier Windhorst (ASU), S. Cohen (ASU), M. Mechtley (ASU), M. Rutkowski (ASU), Robert O'Connell (UVA), P. McCarthy (OCIW), N. Hathi (UC Riverside), R. Ryan (UC Davis), Haojing Yan (OSU), Anton M. Koekemoer (STScI)

About The Object
Object Name GOODS-S/ERS, GOODS South Field WFC3 Early Release Science Data (GOODS-S WFC3 ERS), Chandra Deep Field South (CDF-S)
Object Description Cosmological Survey
R.A. Position 03h 32m 40.23s
Dec. Position -27° 43' 9.86"
Constellation Fornax
Dimensions This image is approximately 9.68 arcminutes wide by 4.27 arcminutes high.
About The Data
Data Description The image was created from Hubble WFC3 data from proposal , R. O'Connell (University of Virginia) and collaborators, combined with the HST/ACS , which includes data from proposals and , P.I. M. Giavalisco; , P.I. Saul Perlmutter; , , and , P.I. A. Riess.
Instrument HST>ACS/WFC, HST>WFC3/UVIS, and HST>WFC3/IR
Exposure Dates Sept. 2002 - Dec. 2004, Exposure Time: 96 orbits (ACS) and Sept. 6, 2009 - Oct. 11, 2009, Exposure Time: 104 orbits (WFC3)
Filters WFC3/IR: F098M, F125W, and F160W ACS/WFC: F435W, F606W, F775W, and F850LP WFC3/UVIS: F225W, F275W, and F336W
About The Image
Color Info The image is a composite of separate exposures made by the WFC3 and ACS instruments on the Hubble Space Telescope. In total, 10 filters were used to sample a very wide wavelength range. The color results from assigning different hues (colors) to combinations of the monochromatic images. In this case, the assigned colors are:  Red: WFC3/IR F125W + F160W Green: ACS/WFC F606W + F775W + F850LP + WFC3/IR F098M Blue: WFC3/UVIS F225W + F275W + F336W + ACS/WFC F435W
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: 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.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.