Complete IRAC Mapping of the CFHTLS-DEEP, MUSYC, and NMBS-II Fields

The IRAC mapping of the NMBS-II fields program is an imaging survey at 3.6 and 4.5 m 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 th...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Publications of the Astronomical Society of the Pacific 2018-12, Vol.130 (994), p.1-16
Hauptverfasser: Annunziatella, Marianna, Marchesini, Danilo, Stefanon, Mauro, Muzzin, Adam, Lange-Vagle, Daniel, Cybulski, Ryan, Labbe, Ivo, Kado-Fong, Erin, Bezanson, Rachel, Brammer, Gabriel, Herrera, David, Lundgren, Britt, Marsan, Z. Cemile, Nonino, Mario, Rudnick, Gregory, Saracco, Paolo, Tomer, Tal, Valdes, Frank, van der Burg, Remco F. J., van Dokkum, Pieter, Wake, David, Whitaker, Katherine E.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:The IRAC mapping of the NMBS-II fields program is an imaging survey at 3.6 and 4.5 m 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 m. 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.
ISSN:0004-6280
1538-3873
DOI:10.1088/1538-3873/aae796