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2018PASP..130l4501A - Publ. Astron. Soc. Pac., 130, part no 12, 4501-124501 (2018/December-0)

Complete IRAC mapping of the CFHTLS-DEEP, MUSYC, and NMBS-II fields.

ANNUNZIATELLA M., MARCHESINI D., STEFANON M., MUZZIN A., LANGE-VAGLE D., CYBULSKI R., LABBE I., KADO-FONG E., BEZANSON R., BRAMMER G., HERRERA D., LUNDGREN B., MARSAN Z.C., NONINO M., RUDNICK G., SARACCO P., TOMER T., VALDES F., VAN DER BURG R.F.J., VAN DOKKUM P., WAKE D. and WHITAKER K.E.

Abstract (from CDS):

The IRAC mapping of the NMBS-II fields program is an imaging survey at 3.6 and 4.5 µm with the Spitzer Infrared Array Camera (IRAC). The observations cover three Canada-France-Hawaii Telescope Legacy Survey Deep (CFHTLS-D) fields, including one also imaged by AEGIS, and two MUSYC fields. These are then combined with archival data from all previous programs into deep mosaics. The resulting imaging covers a combined area of about 3 deg2, with at least ∼2 hr integration time for each field. In this work, we present our data reduction techniques and document the resulting coverage maps at 3.6 and 4.5 µm. All of the images are W-registered to the reference image, which is either the z-band stack image of the 25% best-seeing images from the CFHTLS-D for CFHTLS-D1, CFHTLS-D3, and CFHTLS-D4, or the K-band images obtained at the Blanco 4-m telescope at CTIO for MUSYC1030 and MUSYC1255. We make all images and coverage maps described here publicly available via the Spitzer Science Center.

Abstract Copyright: © 2018. The Astronomical Society of the Pacific. All rights reserved.

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