The Infrared Array Camera (IRAC) Shallow Survey

By Peter Eisenhardt, Daniel Stern, M. Brodwin, G. Fazio, G. Rieke, M. Rieke, M. Werner, E. L. Wright, L. Allen, R. Arendt and 17 more. 2004

166 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/76441be3e259d14622d6bb7a16edefed01df2982

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Citations in the corpus

Number Counts at 3 μm < λ < 10 μm from the Spitzer Space Telescope (2004, background): “The limiting magnitudes for 5σ detection are 18.4, 17.7, 15.5, and 14.8 (12, 15, 74, 76 µJy) at the four IRAC wavelengths (Eisenhardt et al. 2004).”
MID-INFRARED SELECTION OF ACTIVE GALACTIC NUCLEI WITH THE WIDE-FIELD INFRARED SURVEY EXPLORER. II. PROPERTIES OF WISE-SELECTED ACTIVE GALACTIC NUCLEI IN THE NDWFS BOÖTES FIELD (2012, methodology): “The whole field was observed with 90 seconds of exposure per position in the IRAC Shallow Survey (Eisenhardt et al. 2004).”
The Evolving Luminosity Function of Red Galaxies (2006, background): “Eisenhardt et al. (2004) present an overview of the survey design, reduction, calibration, and preliminary results.”
A CORRELATION BETWEEN STAR FORMATION RATE AND AVERAGE BLACK HOLE ACCRETION IN STAR-FORMING GALAXIES (2013, methodology): “…for our sample of IRselected SF galaxies, we also supplemented the data with photometric redshifts measured using the data from the 8.5 deg2 Spitzer IRAC Shallow Survey (ISS, Eisenhardt et al. 2004; Stern et al. 2005) and the 10 deg2 Spitzer Deep Wide Field Survey (SDWFS, Ashby et al. 2009).”
THE SPITZER–WISE SURVEY OF THE ECLIPTIC POLES (2011, result): “The observed lower density in the EP-S is a consequence of the relatively incomplete (across the field) depth of the EP-S IRAC observations compared to the uniform EP-N and the IRAC Shallow Survey (Eisenhardt et al. 2004).”
Clustered and Triggered Star Formation in W5: Observations with Spitzer (2008, methodology): “…averaged distribution of AGN in W5, using a sample of AGN extracted by Stern et al. (2005) from the Spitzer IRAC shallow survey of the Boötes field (Eisenhardt et al. 2004), convolved with our extinction map (as described in § 2.1) and with completeness estimates derived for our Spitzer survey of…”
LOW-RESOLUTION SPECTRAL TEMPLATES FOR ACTIVE GALACTIC NUCLEI AND GALAXIES FROM 0.03 TO 30 μm (2010, methodology): “The IRAC Shallow Survey (Eisenhardt et al. 2004), which we used in A08, is a subset of the SDWFS data.”
THE SPITZER DEEP, WIDE-FIELD SURVEY (2009, methodology): “The latter are drawn from the original ISS and constitute the first SDWFS epoch.”
Clusters of Galaxies in the First Half of the Universe from the IRAC Shallow Survey (2008, methodology): “The IRAC Shallow Survey was executed using guaranteed observing time contributed by G. Fazio, G. Rieke, M. Rieke, M.Werner, and E.Wright.”
Infrared Luminosity Functions from the Chandra Deep Field-South: The Spitzer View on the History of Dusty Star Formation at 0 ≲ z ≲ 1* (2005, background): “…its first extragalactic surveys have already unveiled a huge number of faint and high redshift sources (see for instance Fazio et al. 2004; Eisenhardt et al. 2004; Papovich et al. 2004; Marleau et al. 2004; Lonsdale et al. 2004; Chary et al. 2004; Yan et al. 2004; Dole et al. 2004a in the…”
Red Galaxy Growth and the Halo Occupation Distribution (2008, methodology): “In this paper we determine the HODusing the measurements of the luminosity function and clustering of 0:2 z 1:0 red galaxies selected from the Boötes field of the NOAO Deep WideField Survey (NDWFS) and Spitzer IRAC Shallow Survey.”
THE ERA OF STAR FORMATION IN GALAXY CLUSTERS (2013, methodology): “…Cluster Survey The IRAC Shallow Cluster Survey (ISCS; E08) is a wide-field infrared-selected galaxy cluster survey carried out using the Spitzer/IRAC Shallow Survey imaging (Eisenhardt et al. 2004) of the 8.5 deg2 Boötes field of the NOAO Deep, Wide-Field Survey (NDWFS; Jannuzi and Dey 1999).”
LOFAR 150-MHz observations of the Boötes field: catalogue and source counts (2016, background): “There is a wealth of ancillary data available for this field, including X-ray (Murray et al. 2005; Kenter et al. 2005), UV (GALEX; Martin et al. 2003), and mid-infrared (Eisenhardt et al. 2004).”
Spectral Energy Distributions and Multiwavelength Selection of Type 1 Quasars (2006, methodology): “The colored dashes show the flux density limits for the Spitzer-XFLS, Spitzer-NOAO/Boötes (Jannuzi & Dey 1999; Eisenhardt et al. 2004), 2MASS, SDSS (imaging), SDSS (z < 3 quasar spectroscopy), and GALEX.”
THE PRISM MULTI-OBJECT SURVEY (PRIMUS). I. SURVEY OVERVIEW AND CHARACTERISTICS (2010, background): “…Extragalactic Survey (SWIRE, Lonsdale et al. 2003), the Spitzer Deep, Wide-Field Survey (SDWFS Ashby et al. 2009) and Spitzer GTO shallow program (Eisenhardt et al. 2004), the GALEX Deep Imaging Survey (DIS), and companion deep optical imaging are covering about 70 deg2 to depths that reach…”
The Stellar Mass Assembly of Galaxies from z = 0 to z = 4: Analysis of a Sample Selected in the Rest-Frame Near-Infrared with Spitzer (2007, background): “An object was also considered a star if it satisfied any of these color equations (when fluxes were available), extracted from Eisenhardt et al. (2004), Rowan-Robinson et al. (2005), and Daddi et al. (2004): a) [3.6] − [8.0] > −2 and [3.6]− [8.0] < −1 and [8.0] < 20., or [3.6]− [4.5] > −1 and…”
The WISE AGN Catalog (2017, background): “For example, Gorjian et al. (2008) finds that 97.5% of X-ray sources identified in the 5 ks XBoötes survey Chandra observations (Murray et al. 2005) have counterparts in the 90 s observations of the Spitzer IRAC Shallow Survey (Eisenhardt et al. 2004), with an additional ∼1% of the X-ray sources ex”