FIREWORKS U38-to-24 μm Photometry of the GOODS Chandra Deep Field-South: Multiwavelength Catalog and Total Infrared Properties of Distant Ks-selected Galaxies

By S. Wuyts, I. Labbé, N. F. Förster Schreiber, M. Franx, G. Rudnick, G. Brammer, P. V. van Dokkum. 2008

265 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/97a2839a63acbffdf940a6f15960933a2775361a

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Instrumentation

Citations in the corpus

THE CHANDRA COSMOS SURVEY. III. OPTICAL AND INFRARED IDENTIFICATION OF X-RAY POINT SOURCES (2012, result): “These results are comparable in precision to those achieved typically for non-active galaxies (Cardamone et al. 2008, Wuyts et al. 2008, Ilbert et al. 2009, Barro et al. 2011) and to those reached only recently for photometric redshift of AGN (Salvato et al. 2009, Cardamone et al. 2008, Luo et al.…”
3D-HST WFC3-SELECTED PHOTOMETRIC CATALOGS IN THE FIVE CANDELS/3D-HST FIELDS: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR MASSES (2014, methodology): “5 data release, Retzlaff et al. 2010) to a uniform PSF (see Wuyts et al. 2008 for details).”
THE COSMOS-WIRCam NEAR-INFRARED IMAGING SURVEY. I. BzK-SELECTED PASSIVE AND STAR-FORMING GALAXY CANDIDATES AT z ≳ 1.4 (2009, methodology): “This K-band selected catalogue, as well as the FIREWORKS catalog by Wuyts et al. (2008), are based on the ESO Imaging Survey coverage of the GOODS-South field14 These studies have investigated, amongst other topics, the evolution of the mass function atz ∼ 2 and what number of red sequence galaxies…”
STELLAR KINEMATICS OF z ∼ 2 GALAXIES AND THE INSIDE-OUT GROWTH OF QUIESCENT GALAXIES, (2012, methodology): “We derive stellar masses for this sample by running the stellar population code FAST on available catalogs, i.e., FIREWORKS (Wuyts et al. 2008) for the CDS-S, R. Skelton et al. (in preparation) for the HDF-N, and FIRES (Förster Schreiber et al. 2006) for MS 1054-0321.”
Panchromatic spectral energy distributions of Herschel sources (2013, result): “Also the Wuyts et al. (2008) approach produces scatter lower than 10%, when compared to the above mentioned three techniques.”
CANDELS: CONSTRAINING THE AGN–MERGER CONNECTION WITH HOST MORPHOLOGIES AT z ∼ 2 (2011, methodology): “Redshifts for the matched hosts were obtained from a variety of publicly available spectroscopic redshift catalogs (the bulk of these redshifts come from Silverman et al. 2010) and the photometric redshifts in the FIREWORKS catalog (Wuyts et al. 2008).”
Structure and Star Formation in Galaxies out to z = 3: Evidence for Surface Density Dependent Evolution and Upsizing (2008, methodology): “Wuyts et al. (2008) homogonized the PSFs of the GOODS ACS and VLT Near-IR imaging data, to derive optical-near-ir photometry, basedon a K-selected sample.”
CANDELS MULTI-WAVELENGTH CATALOGS: SOURCE DETECTION AND PHOTOMETRY IN THE GOODS-SOUTH FIELD (2013, methodology): “We carry out a test, equivalent to the “empty aperture” method of measuring the variance within empty apertures of various sizes placed throughout the images (e.g., Wuyts et al. 2008; Whitaker et al. 2011; Coe et al. 2013), to examine the noise properties of our HST images.”
The evolution of the dust temperatures of galaxies in the SFR–M∗ plane up to z ~ 2 (2013, methodology): “In the GOODS-S field we used the Ks (<24.3, 5σ) selected FIREWORKS catalogue of Wuyts et al. (2008), which provides photometry in 16 bands from U to IRAC wavelengths.”
CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY (2011, unknown): “Object IDs are from the FIREWORKS (Wuyts et al. 2008) and MUSYC (Cardamone et al. 2010) catalogs.”
THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ⩽ z < 0.8 IN THE DEEP2/AEGIS SURVEY (2012, methodology): “Franx et al. (2008) intercompared several of the aforementioned color-parameter correlations in the redshift range0< z< 3 using data from the FIREWORKS catalog (Wuyts et al. 2008).”
CLASH: THREE STRONGLY LENSED IMAGES OF A CANDIDATE z ≈ 11 GALAXY (2012, methodology): “The FIREWORKS data set includes 0.38–24µm photometry of galaxies down to mag ∼ 24.3 (5-σ K-band) and spectroscopic redshifts out to z ∼ 3.7.”
UVUDF: ULTRAVIOLET THROUGH NEAR-INFRARED CATALOG AND PHOTOMETRIC REDSHIFTS OF GALAXIES IN THE HUBBLE ULTRA DEEP FIELD (2015, methodology): “This does not significantly affect our quality checks below, as there are over 6000 redshifts in the FIREWORKS catalog which are used in refining the templates.”
Deriving Physical Properties from Broadband Photometry with Prospector: Description of the Model and a Demonstration of its Accuracy Using 129 Galaxies in the Local Universe (2016, unknown): “Many studies use broadband photometry in the MIR to estimate total IR luminosities, either by using fixed IR templates (e.g., Daddi et al. 2007; Wuyts et al. 2008; Buat et al. 2009; Whitaker et al. 2014) or by fitting IR models to a limited wavelength range (e.g., Chang et al. 2015).”
3D-HST: A WIDE-FIELD GRISM SPECTROSCOPIC SURVEY WITH THE HUBBLE SPACE TELESCOPE (2012, methodology): “Currently we simply match the F140W-selected objects within the 3D-HST fields to the deepest K-selected catalogs available with broad multiwavelength coverage: AEGIS, COSMOS, Whitaker et al. (2011); GOODS-S, Wuyts et al. (2008); GOODS-N, Kajisawa et al. (2011); and UDS, Williams et al. (2009).”
Deep Spitzer 24 μm COSMOS Imaging. I. The Evolution of Luminous Dusty Galaxies—Confronting the Models (2009, background): “It implies that the predicted source density of massive galaxies with strong on-going activity of star formation such as those recently discovered at high redshift with Spitzer (e.g., Daddi et al. 2005; Reddy et al. 2006; Papovich et al. 2006; Wuyts et al. 2008) is too low.”
PHAT: PHoto-z Accuracy Testing (2010, methodology): “This library is further calibrated using the FIREWORKS photometry and spectroscopic redshifts from Wuyts et al. (2008).”