Artist's Illustration of the Early Milky Way

 Artist's Illustration of the Early Milky Way

Credits

NASA, ESA, and Z. Levay (STScI/AURA)

About The Data
Data Description This release is based on Hubble data from proposals and : P. van Dokkum (Yale University), C. Steidel (Caltech), H.-W. Rix (Max Planck Institute for Astronomy), M. Kriek (University of California, Berkeley), G. Kauffmann (Max Planck Institute for Astronomy), G. Brammer (European Southern Observatory), D. Erb (University of Wisconsin, Milwaukee), M. Franx (Leiden University), N. Schreiber (Max Planck Institute for Extraterrestrial Physics), X. Fan (University of Arizona), R. Quadri, I. Labbe, and P. McCarthy (Observatories of the Carnegie Institution of Washington), D. Marchesini (Tufts University), A. Pasquali (Max Planck Institute for Astronomy), G. Illingworth (University of California, Santa Cruz), K. Whitaker (NASA Goddard Space Flight Center), J. Hennawi (Max Planck Institute for Astronomy), D. Wake (Yale University), and S. Patel (Leiden University). The science teams comprise the following: Patel et al. Paper: S. Patel, M. Fumagalli, and M. Franx (Leiden University), P. van Dokkum (Yale University), A. van der Wel (Max Planck Institute for Extraterrestrial Physics.), J. Leja (Yale University), I. Labbe (Leiden University), G. Brammer (European Southern Observatory), R. Skelton and I. Momcheva (Yale University), K. Whitaker (NASA Goddard Space Flight Center), B. Lundgren (University of Wisconsin, Madison), A. Muzzin (Leiden University), R. Quadri (Observatories of the Carnegie Institution of Washington), E. Nelson (Yale University), D. Wake (University of Wisconsin, Madison), and H.-W. Rix (Max Planck Institute for Extraterrestrial Physics). van Dokkum et al. Paper: P. van Dokkum, J. Leja, and E. Nelson (Yale University), S. Patel (Leiden University), R. Skelton and I. Momcheva (Yale University), G. Brammer (European Southern Observatory), K. Whitaker (NASA Goddard Space Flight Center), B. Lundgren (University of Wisconsin, Madison), M. Fumagalli (Leiden University), C. Conroy (University of California, Santa Cruz), N. Schreiber (Max Planck Institute for Extraterrestrial Physics), M. Fumagalli (Leiden University), M. Kriek (University of California, Berkeley), I. Labbe (Leiden University), D. Marchesini (Tufts University), H.-W. Rix and A. van der Wel (Max Planck Institute for Astronomy), and S. Wuyts (Max Planck Institute for Extraterrestrial Physics).
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.