Early Results from the IRAC Dark Field Mid-IR Variability Search

Details Early Results from the IRAC Dark Field Mid-IR Variability Search Early Results from the IRAC Dark Field Mid-IR Variability Search

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.0205s&link_type=abstract

American Astronomical Society Meeting 210, #02.05; Bulletin of the American Astronomical Society, Vol. 39, p.93

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Scientific paper

The IRAC Dark Field is a relatively wide area of sky near the north ecliptic pole that is imaged very deeply every few weeks by the Spitzer Space Telescope from 3.6 to 8 microns. With tens of thousands of objects and reaching a Vega L-band magnitude of 21.5, the field opens a new window on variability and transient studies in the mid-IR. We show preliminary results of searching for transient and variable objects, along with additional data from the other Great Observatories and from ground-based imaging which reveal the nature of the underlying host objects.

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