The SDSS Coadd: A Galaxy Photometric Redshift Catalog
arXiv:1111.6620 · doi:10.1088/0004-637X/747/1/59
Abstract
We present and describe a catalog of galaxy photometric redshifts (photo-z's) for the Sloan Digital Sky Survey (SDSS) Coadd Data. We use the Artificial Neural Network (ANN) technique to calculate photo-z's and the Nearest Neighbor Error (NNE) method to estimate photo-z errors for 13 million objects classified as galaxies in the coadd with . The photo-z and photo-z error estimators are trained and validated on a sample of galaxies that have SDSS photometry and spectroscopic redshifts measured by the SDSS Data Release 7 (DR7), the Canadian Network for Observational Cosmology Field Galaxy Survey (CNOC2), the Deep Extragalactic Evolutionary Probe Data Release 3(DEEP2 DR3), the VIsible imaging Multi-Object Spectrograph - Very Large Telescope Deep Survey (VVDS) and the WiggleZ Dark Energy Survey. For the best ANN methods we have tried, we find that 68% of the galaxies in the validation set have a photo-z error smaller than . After presenting our results and quality tests, we provide a short guide for users accessing the public data.
16 pages, 13 figures, submitted to ApJ. Analysis updated to remove proprietary BOSS data comprising small fraction (8%) of original spectroscopic training set and erroneously included. Changes in results are small compared to the errors and the conclusions are unaffected. arXiv admin note: substantial text overlap with arXiv:0708.0030
References in corpus (5)
- The 2.5 m Telescope of the Sloan Digital Sky Survey
- A Survey of z~6 Quasars in the SDSS Deep Stripe: I. a Flux-Limited Sample at z_{AB}<21
- The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey
- A Galaxy Photometric Redshift Catalog for the Sloan Digital Sky Survey Data Release 6
- New Approaches To Photometric Redshift Prediction Via Gaussian Process Regression In The Sloan Digital Sky Survey
Cited by in corpus (33)
- The SDSS Coadd: 275 deg^2 of Deep SDSS Imaging on Stripe 82
- Photometric redshifts for the SDSS Data Release 12
- On the mass and luminosity functions of tidal disruption flares: rate suppression due to black hole event horizons
- Spatial distribution of ultra-diffuse galaxies within large-scale structures
- The 0.1<z<1.65 evolution of the bright end of the [OII] luminosity function
- The Stripe 82 Massive Galaxy Project II: Stellar Mass Completeness of Spectroscopic Galaxy Samples from the Baryon Oscillation Spectroscopic Survey
- The SDSS Coadd: Cosmic Shear Measurement
- Morpho-z: improving photometric redshifts with galaxy morphology
- Dreaming of atmospheres
- The Stripe 82 Massive Galaxy Project I: Catalog Construction
- Integrated approach to cosmology: Combining CMB, large-scale structure and weak lensing
- J-PLUS: On the identification of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs
- The abundance of compact quiescent galaxies since z ~ 0.6
- The Overlooked Potential of Generalized Linear Models in Astronomy-II: Gamma regression and photometric redshifts
- The first analytical expression to estimate photometric redshifts suggested by a machine
- The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: Multiwavelength Counterparts
- Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82
- The Stripe 82 Massive Galaxy Project III: A Lack of Growth Among Massive Galaxies
- The ALHAMBRA survey : band luminosity function of quiescent and star-forming galaxies at by PDF analysis
- Photometric redshift estimation of galaxies in the DESI Legacy Imaging Surveys
- The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey: Cluster catalogue and discovery of two merging cluster candidates
- The SOAR Gravitational Arc Survey - I: Survey overview and photometric catalogs
- Galaxy clusters in the SDSS Stripe 82 based on galaxy photometric redshifts
- The relation between galaxy density and radio jet power for 1.4 GHz VLA selected AGN in Stripe 82
- Do satellite galaxies trace matter in galaxy clusters?
- Compact Groups analysis using weak gravitational lensing II: CFHT Stripe 82 data
- The faint end of the 250 micron luminosity function at z < 0.5
- The SDSS Coadd: Cross-Correlation Weak Lensing and Tomography of Galaxy Clusters
- Mass Calibration of Galaxy Clusters at Redshift 0.1-1.0 using Weak Lensing in the Sloan Digital Sky Survey Stripe 82 Co-add
- The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey II. X-ray and optical properties of the cluster sample
- Spectral Clustering for Optical Confirmation and Redshift Estimation of X-ray Selected Galaxy Cluster Candidates in the SDSS Stripe 82
- Deeper detection limits in astronomical imaging using self-supervised spatiotemporal denoising
- Pz Cats: Photometric redshift catalogs based on DES Y3 BAO sample