Catalogs of distant, faint sources dark fields [rejected]

August 21, 2013 in Astronomy & Space / Astronomy
This image of a "dark field" was taken by the Great Observatories Origins Deep Survey project using NASA's Hubble Space Telescope. The full program has just released a multi-wavelength catalog of 34,930 galaxies, enabling astronomers to study the evolution of galaxies in the early universe. Credit: NASA, HST, and the CANDELS team

Over the past decade, the Hubble Space Telescope (HST) and other modern, giant telescopes have opened a new era in observational cosmology. By staring for long times at so-called "dark fields"—regions of the sky without much background emission from the solar system or the galaxy—astronomers have been able to detect very faint galaxies in the early universe, and to study their evolution from early stages to the present. More recently, deep multi-wavelength imaging surveys have been undertaken, and have revealed a complex interplay between galaxy mergers, star formation, and black holes over cosmic time, leading to new insights into the physical processes that drive galaxy formation and evolution.

From the entire span of cosmic time, two epochs are particularly of great interest: "cosmic high noon," from which period light has been traveling for about ten billion years, and "" with much older galaxies whose light has been en route to us for about thirteen billion years. During the former period, cosmic star formation activity reached its peak; the latter period is when in the cosmos became ionized.

CfA astronomers Giovanni Fazio, Steve Willner, and Matt Ashby are the PI and key team leaders, respectively, of the Spitzer Infrared Array Camera (IRAC). Along with a large team of colleagues, they have just published a multi-wavelength catalog—from the ultraviolet to the infrared—of 34,930 galaxies spanning the cosmic high noon and cosmic dawn taken with IRAC, HST, and other telescopes in the direction of five popular "dark fields."

The large sample of remote systems is called CANDELS (The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey). It is able to detect star forming galaxies smaller than our Milky Way at these huge distances with a 50% completeness level, and more passive, fainter galaxies with somewhat less sensitivity. The new catalog makes it possible to study for the first time with statistical precision how galaxies evolved in the universe into predominantly two kinds: bluish, active spiral galaxies, and red, passive elliptical galaxies.

More information: Guo, Y. et al. Candels Multi-Wavelength Catalogs: Source Detection and Photometry in the Goods-South Field, ApJS, 207, 24, 2013.

Provided by Harvard-Smithsonian Center for Astrophysics

"Catalogs of distant, faint sources dark fields [rejected]" August 21, 2013