The United Kingdom Infrared Telescope Infrared Deep Sky Survey First Data Release

By S. Warren, Nigel C. Hambly, S. Dye, O. Almaini, N. Cross, A. Edge, S. Foucaud, Paul Hewett, S. Hodgkin, M. Irwin and 30 more. 2007

178 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/a395be7e99ac3e4d01d10bc340ce5d68013446ea

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Citations in the corpus

The UKIDSS galactic plane survey (2007, background): “The median 5-σ depths in DR2 given by Warren et al.(2007b) are J=19.77, H=19.00, K=18.05 (Vega system).”
Stellar SEDs from 0.3 to 2.5 μm: Tracing the Stellar Locus and Searching for Color Outliers in the SDSS and 2MASS (2007, methodology): “…in the optical (the Panoramic Survey Telescope & Rapid Response System [Pan-STARRS], Kaiser et al. 2002, and SkyMapper, Keller et al. 2007) and near infrared (the United Kingdom Infrared Deep Sky Survey [UKIDSS] Warren et al. 2007) using filter systems that closely resemble those of SDSS and 2MASS.”
Galaxy And Mass Assembly (GAMA): the input catalogue and star–galaxy separation (2009, methodology): “The imaging used in this work has already passed the basic quality assessments discussed in Dye et al. (2006) and Warren et al. (2007).”
The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyr. Evidence for a major build up of the red sequence between z = 2 and z = 1 (2007, methodology): “Finally, we complete our dataset with the J and K photometry from the UKIDSS Ultra Deep Survey (Lawrence et al. 2006) based on the DR1 release (Warren et al. 2007).”
HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHS (2012, methodology): “HXMM02 is in the SXDF region of the XMM-LSS SWIRE field and therefore deep Subaru SuprimeCam and UKIRT WFCAM imaging are available (Furusawa et al. 2008; Warren et al. 2007).”
The luminosity function, halo masses and stellar masses of luminous Lyman-break galaxies at redshifts 5 < z < 6 (2008, methodology): “The data utilized in this paper were taken from the first UKIDSS data release (DR1; Warren et al. 2007), which includedJK imaging of the entire UDS field to5σ depths ofJ = 23.9, K = 23.8 (1.6′′diameter apertures).”
Delay Time Distribution Measurement of Type Ia Supernovae by the Subaru/XMM-Newton Deep Survey and Implications for the Progenitor (2008, unknown): “…data set of SXDS in BV Rc i ′z′ bands obtained by the Subaru/Suprime-Cam (Furusawa et al. 2008), in JK bands obtained by the UKIDSS survey (Warren et al. 2007), and in 3.6 and 4.5 µm bands obtained by the SWIRE survey (Lonsdale et al. 2004), with the limiting magnitudes (3σ) of 28.4,…”
A new measurement of the evolving near-infrared galaxy luminosity function out to z≃ 4: a continuing challenge to theoretical models of galaxy formation (2008, methodology): “For the purpose of this work we used data from the first data release of the survey (DR1; Warren et al. 2007), which includes imaging in the J- and K-bands with 5σ depths of 23.3 and 23.1 respectively within a 3-arcsec diameter aperture.”
WHAT TURNS GALAXIES OFF? THE DIFFERENT MORPHOLOGIES OF STAR-FORMING AND QUIESCENT GALAXIES SINCE z ∼ 2 FROM CANDELS (2011, methodology): “The Williams et al. (2009) catalog usesJ and K-band data for the UKIDDS UDS Data Release 1 (Lawrence et al. 2007; Warren et al. 2007) in conjunction withB, R, i and z-band imaging from the SXDS (Furusawa et al. 2008) and 3.6µm and 4.5µm IRAC imaging data taken as part of the SWIRE survey (Lonsdale…”
The WFCAM Science Archive (2006, methodology): “Although the WSA design does not preclude fully automated QC procedures, presently the UKIDSS data (for example) have a lengthy semi–automated QC process applied, some details of which are given in Dye et al. (2006) and Warren et al. (2007a).”
THE EVOLVING RELATIONS BETWEEN SIZE, MASS, SURFACE DENSITY, AND STAR FORMATION IN 3 × 104 GALAXIES SINCE z = 2 (2009, methodology): “This catalog comprises near-infraredJ andK data taken from the UKIDSS Ultra-Deep Survey Data Release 1 (UDS; Lawrence et al. 2007; Warren et al. 2007a), with overlapping BRi′z′ imaging from the Subaru-XMM Deep Survey (SXDS; Sekiguchi et al. 2004), and 3.6/4.5µm data from the Spitzer Wide-area…”
THE FINAL SDSS HIGH-REDSHIFT QUASAR SAMPLE OF 52 QUASARS AT z > 5.7 (2016, methodology): “…searches for quasars at these redshifts, followed by the Canada-France High-redshift Quasar Survey (CFHQS; Willott et al. 2007), the UKIRT Infrared Deep Sky Survey (UKIDSS; Warren et al. 2007), and the Panoramic Survey Telescope & Rapid Response System 1 (Pan-STARRS1; Kaiser et al. 2010) survey.”
A SURVEY OF z ∼ 6 QUASARS IN THE SLOAN DIGITAL SKY SURVEY DEEP STRIPE. I. A FLUX-LIMITED SAMPLE AT zAB < 21 (2007, methodology): “39+001229.3 (hereafter SDSS J0203+0012), was independently discovered by matching the UKIRT Infrared Deep Sky Survey (UKIDSS; Warren et al. 2007) data to the SDSS data (Venemans et al. 2007).”
Mid- and far-infrared luminosity functions and galaxy evolution from multiwavelength Spitzer observations up to z ~ 2.5 (2009, methodology): “J and K data are also available from the UKIDSS Ultra Deep Survey (Lawrence et al. 2007) based on the DR1 release (Warren et al. 2007).”
STELLAR KINEMATICS OF z ∼ 2 GALAXIES AND THE INSIDE-OUT GROWTH OF QUIESCENT GALAXIES, (2012, methodology): “(4) For UDS-19627 we use ground based data from UKIDSS-UDS, (Lawrence et al. 2007; Warren et al. 2007) Data Release 8 in the J, H, and K- band, as no as HST data is available.”
The star formation history of K-selected galaxies (2008, methodology): “In this work we used data from the DR1 release (Warren et al. 2007), which includes J and K images reaching 5-σ depths of K = 23.6 and J = 23.7 (2-arcsec diameter apertures).”
STELLAR POPULATIONS OF Lyα EMITTERS AT z ∼ 6–7: CONSTRAINTS ON THE ESCAPE FRACTION OF IONIZING PHOTONS FROM GALAXY BUILDING BLOCKS (2010, methodology): “…Wide Field Infrared Camera (WFCAM; Casali et al. 2007) from UKIRT Infrared Deep Sky Survey (UKIDSS) Ultra Deep Survey (UDS; Lawrence et al. 2007; Warren et al. 2007), and 3.6 – 8.0µm images taken with the Spitzer/IRAC from the Spitzer legacy survey of the UDS field (SpUDS; Spitzer Proposal ID…”
The UKIRT wide field camera ZYJHK photometric system: calibration from 2MASS (2008, methodology): “…mounted on UKIRT about 75 per cent of the time, the majority of which is used to perform a set of five public surveys, under the umbrella of the UKIRT Infrared Deep Sky Survey: UKIDSS, (Lawrence et al. 2007, Warren et al. 2007), as well as a number of campaign projects and other smaller programmes.”