The GOODS-MUSIC sample: a multicolour catalog of near-IR selected galaxies in the GOODS-South field
arXiv:astro-ph/0603094 · doi:10.1051/0004-6361:20053979
Abstract
We present a high quality multiwavelength (from 0.3 to 8.0 micron) catalog of the large and deep area in the GOODS Southern Field covered by the deep near-IR observations obtained with the ESO VLT. The catalog is entirely based on public data: in our analysis, we have included the F435W, F606W, F775W and F850LP ACS images, the JHKs VLT data, the Spitzer data provided by IRAC instrument (3.6, 4.5, 5.8 and 8.0 micron), and publicly available U-band data from the 2.2ESO and VLT-VIMOS. We describe in detail the procedures adopted to obtain this multiwavelength catalog. In particular, we developed a specific software for the accurate "PSF-matching" of space and ground-based images of different resolution and depth (ConvPhot), of which we analyse performances and limitations. We have included both z-selected, as well as Ks-selected objects, yielding a unique, self-consistent catalog. The largest fraction of the sample is 90% complete at z~26 or Ks~23.8 (AB scale). Finally, we cross-correlated our data with all the spectroscopic catalogs available to date, assigning a spectroscopic redshift to more than 1000 sources. The final catalog is made up of 14847 objects, at least 72 of which are known stars, 68 are AGNs, and 928 galaxies with spectroscopic redshift (668 galaxies with reliable redshift determination). We applied our photometric redshift code to this data set, and the comparison with the spectroscopic sample shows that the quality of the resulting photometric redshifts is excellent, with an average scatter of only 0.06. The full catalog, which we named GOODS-MUSIC (MUltiwavelength Southern Infrared Catalog), including the spectroscopic information, is made publicly available, together with the software specifically designed to this end.
Accepted for publication in Astronomy and Astrophysics, uses aa.cls, 20 pages, 16 figures. Further information at http://lbc.oa-roma.inaf.it/goods
Cited by in corpus (99)
- EAZY: A Fast, Public Photometric Redshift Code
- A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
- 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
- Rates and properties of type Ia supernovae as a function of mass and star-formation in their host galaxies
- The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
- Structure and star formation in galaxies out to z=3: evidence for surface density dependent evolution and upsizing
- The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
- Photometric redshift and classification for the XMM-COSMOS sources
- Absorption Properties and Evolution of Active Galactic Nuclei
- The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields
- The Multiwavelength Survey by Yale-Chile (MUSYC): Deep Medium-Band optical imaging and high quality 32-band photometric redshifts in the ECDF-S
- The Great Observatories Origins Deep Survey. VLT/VIMOS Spectroscopy in the GOODS-South Field
- Unveiling obscured accretion in the Chandra Deep Field South
- Spitzer's Contribution to the AGN Population
- The evolution of the near-IR galaxy Luminosity Function and colour bimodality up to z ~ 2 from the UKIDSS Ultra Deep Survey Early Data Release
- Over half of the far-infrared background light comes from galaxies at z >= 1.2
- UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field
- Deep U band and R imaging of GOODS-South: Observations,data reduction and first results
- The star-formation history of K-selected galaxies
- The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z=1.5-10 UV-selected Galaxies and the Implied High-Redshift Star Formation History
- A Public, K-Selected, Optical-to-Near-Infrared Catalog of the Extended Chandra Deep Field South (ECDFS) from the MUltiwavelength Survey by Yale-Chile (MUSYC)
- Stellar mass estimates in early-type galaxies: procedures, uncertainties and models dependence
- The Stellar Mass Density at z~6 from Spitzer Imaging of i-drop Galaxies
- Frontier Fields: High-Redshift Predictions and Early Results
- The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts
- MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3
- A joint analysis of BLAST 250--500um and LABOCA 870um observations in the Extended Chandra Deep Field South
- Effects of Dust Geometry in Lyman Alpha Galaxies at z = 4.4
- A comparison among LBGs, DRGs and BzK galaxies: their contribution to the stellar mass density in the GOODS-MUSIC sample
- Mapping the average AGN accretion rate in the SFR-M* plane for Herschel selected galaxies at 0<z<2.5
- Tracing the Mass-Dependent Star Formation History of Late-Type Galaxies using X-ray Emission: Results from the Chandra Deep Fields
- Coevolution of metallicity and star formation in galaxies to z=3.7: I. A fundamental plane
- The physical properties of Lyalpha emitting galaxies: not just primeval galaxies?
- Cosmic shear analysis of archival HST/ACS data: I. Comparison of early ACS pure parallel data to the HST/GEMS Survey
- A systematic search for very massive galaxies at z > 4
- GaBoDS: The Garching-Bonn Deep Survey: VI. Cosmic shear analysis
- The evolution of the quenching of star formation in cluster galaxies since z 1
- The systematic search for active galactic nuclei in the Deep Field South
- Physical properties of z~4 LBGs: differences between galaxies with and without Ly-alpha emission
- The rise and fall of star-formation in merging galaxy clusters
- Exploring the evolutionary paths of the most massive galaxies since z~2
- The host galaxies of X-ray selected Active Galactic Nuclei to z=2.5: Structure, star-formation and their relationships from CANDELS and Herschel/PACS
- Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
- Herschel-ATLAS: Properties of dusty massive galaxies at low and high redshifts
- Low accretion rates at the AGN cosmic downsizing epoch
- Reproducing the assembly of massive galaxies within the hierarchical cosmogony
- The effect of stellar feedback and quasar winds on the AGN population
- The impact of Spitzer infrared data on stellar mass estimates - and a revised galaxy stellar mass function at 0 < z < 5
- Unveiling the oldest and most massive galaxies at very high redshift
- Bayesian Single-Epoch Photometric Classification of Supernovae
- Black hole accretion preferentially occurs in gas rich galaxies
- The number density of superdense early-type galaxies at 1<z<2 and the local cluster galaxies
- The Chandra Deep Fields: Lifting the Veil on Distant Active Galactic Nuclei and X-Ray Emitting Galaxies
- The discovery of a significant sample of massive galaxies at redshifts 5 < z < 6 in the UKIDSS Ultra Deep Survey Early Data Release
- Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field South
- The VLA Survey of the Chandra Deep Field South. II. Identification and host galaxy properties of submillijansky sources
- Variability-selected active galactic nuclei from supernova search in the Chandra deep field south
- Cluster and field elliptical galaxies at z~1.3. The marginal role of the environment and the relevance of the galaxy central regions
- ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields
- The quiescent fraction of isolated low surface brightness galaxies: Observational constraints
- A Photometrically Detected Forming Cluster of Galaxies at Redshift 1.6 in the GOODS Field
- The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
- Emission-Line Galaxies from the PEARS Hubble Ultra Deep Field: A 2-D Detection Method and First Results
- Photometric Redshifts in the Hawaii-Hubble Deep Field-North (H-HDF-N)
- The ASTRODEEP Frontier Fields Catalogues III. Multiwavelength photometry and rest frame properties of MACS-J0717 and MACS-J1149
- Revealing impacts of stellar mass and environment on galaxy quenching
- Star formation and quenching among the most massive galaxies at z~1.7
- A new (2+1)D cluster finding algorithm based on photometric redshifts: large scale structure in the Chandra Deep Field South
- The red and blue galaxy populations in the GOODS field: evidence for an excess of red dwarfs
- The population of early-type galaxies: how it evolves with time and how it differs from passive and late-type galaxies
- Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9
- The Expected Detection of Dust Emission from High-Redshift Lyman Alpha Galaxies
- GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity
- The VANDELS survey: Discovery of massive overdensities of galaxies at z>2
- On the nature of the extragalactic number counts in the K-band
- A deep i-selected multi-waveband galaxy catalogue in the COSMOS field
- Unveiling the nature of 11 dusty star-forming galaxies at the peak of cosmic star formation history
- Clustering of star-forming galaxies detected in mid-infrared with the Spitzer wide-area survey
- The ALHAMBRA survey : band luminosity function of quiescent and star-forming galaxies at by PDF analysis
- Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
- An ALMA view of 11 Dusty Star Forming Galaxies at the peak of Cosmic Star Formation History
- The evolution of star formation activity in galaxy groups
- A multi-wavelength study of a massive, active galaxy at : coupling the kinematics of the ionized and molecular gas
- Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-Triggered AGN-Galaxy Coevolution Models?
- Properties of LBGs with [OIII] detection at z 3.5: The importance of including nebular emission data in SED fitting
- Spectroscopic follow-up of variability-selected active galactic nuclei in the Chandra Deep Field South
- Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies
- A maximum likelihood method for bidimensional experimental distributions, and its application to the galaxy merger fraction
- A Catalog of Emission-Line Galaxies from the Faint Infrared Grism Survey: Studying Environmental Influence on Star Formation
- Selection of AGN candidates in the GOODS-South Field through SPITZER/MIPS 24 m variability
- Number Density Evolution of Ks -band Selected High Redshift Galaxy Populations in the AKARI North Ecliptic Pole Field
- Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies at z ~ 1.4
- SDSS-IV MaNGA: The Nature of an Off-galaxy H Blob -- A Multi-wavelength View of Offset Cooling in a Merging Galaxy Group
- Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
- UV slope of z3 bright () Lyman-break galaxies in the COSMOS field
- EROs found behind lensing clusters: II.Empirical properties, classification, and SED modelling based on multi-wavelength observations
- The distant red galaxy neighbour population of 1 < z < 2 QSOs and optically obscured sources
- Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
- Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS