Sloan Digital Sky Survey Imaging of Low Galactic Latitude Fields: Technical Summary and Data Release

Citation:

Finkbeiner DP, Padmanabhan N, Schlegel DJ, Carr MA, Gunn JE, Rockosi CM, Sekiguchi M, Lupton RH, Knapp GR, Ivezić Ž, et al. Sloan Digital Sky Survey Imaging of Low Galactic Latitude Fields: Technical Summary and Data Release. The Astronomical Journal. 2004;128 :2577-2592.

Date Published:

November 1, 2004

Abstract:

The Sloan Digital Sky Survey (SDSS) mosaic camera and telescope haveobtained five-band optical-wavelength imaging near the Galactic planeoutside of the nominal survey boundaries. These additional data wereobtained during commissioning and subsequent testing of the SDSSobserving system, and they provide unique wide-area imaging data inregions of high obscuration and star formation, including numerous youngstellar objects, Herbig-Haro objects, and young star clusters. Becausethese data are outside the survey regions in the Galactic caps, they arenot part of the standard SDSS data releases. This paper presents imagingdata for 832 square degrees of sky (including repeats), in thestar-forming regions of Orion, Taurus, and Cygnus. About 470deg2 are now released to the public, with the remainder tofollow at the time of SDSS Data Release 4. The public data in Orioninclude the star-forming region NGC 2068/NGC 2071/HH 24 and a large partof Barnard's loop.

Notes:

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