The detection and photometric redshift determination of distant galaxies using SIRTF's Infrared Array Camera
arXiv:astro-ph/9903067 · doi:10.1086/316373
Abstract
We investigate the ability of the Space Infrared Telescope Facility's Infrared Array Camera to detect distant (z ~ 3)galaxies and measure their photometric redshifts. Our analysis shows that changing the original long wavelength filter specifications provides significant improvements in performance in this and other areas.
28 pages incl 12 figures; to appear in June 1999 PASP. Fig.12 replaced with corrected version
References in corpus (10)
- High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
- Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
- The Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry
- Dusty star forming galaxies at high redshift
- The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: I. Limits and Detections
- Spectroscopic Confirmation of a Population of Normal Star-Forming Galaxies at Redshifts z>3
- A wide-field K-band survey. The luminosity function of galaxies
- A blind test of photometric redshift prediction
- Emission Features and Source Counts of Galaxies in Mid-Infrared
- Do the Infrared Emission Features Need Ultraviolet Excitation
Cited by in corpus (66)
- The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
- Dusty Star-Forming Galaxies at High Redshift
- SWIRE: The SIRTF Wide-area InfraRed Extragalactic Survey
- Distant Radio Galaxies and their Environments
- The Evolving Luminosity Function of Red Galaxies
- Spitzer Observations of Massive Red Galaxies at High Redshift
- A Spitzer-Selected Galaxy Cluster at z=1.62
- Galaxy Clusters around radio-loud AGN at 1.3 < z < 3.2 as seen by Spitzer
- A Highly Complete Spectroscopic Survey of the GOODS-N Field
- The Relationship Between Stellar and Black-Hole Mass in Submillimeter Galaxies
- A Physical Model for z~2 Dust Obscured Galaxies
- Photometric Redshifts in the IRAC Shallow Survey
- The nature of star formation in distant ultraluminous infrared galaxies selected in a remarkably narrow redshift range
- The 1.6um Bump as a Photometric Redshift Indicator
- A Near-Infrared Spectroscopic Survey of K-selected Galaxies at z ~ 2.3: Comparison of Stellar Population Synthesis Codes and Constraints from the Rest-frame NIR
- The Spitzer High Redshift Radio Galaxy Survey
- Discovery of a Rich Cluster at z = 1.63 using the Rest-Frame 1.6um "Stellar Bump Sequence" Method
- High-Redshift Extremely Red Objects in the HST Ultra Deep Field Revealed by the GOODS IRAC Observations
- Radio imaging of the Subaru/XMM-Newton Deep Field - III. Evolution of the radio luminosity function beyond z=1
- The nature of faint Spitzer-selected dust-obscured galaxies
- A joint analysis of BLAST 250--500um and LABOCA 870um observations in the Extended Chandra Deep Field South
- Mid-infrared properties of X-ray sources in the Extended Groth Strip
- The Taiwan ECDFS Near-Infrared Survey: Ultra-deep J and Ks Imaging in the Extended Chandra Deep Field-South
- The Angular Clustering of Distant Galaxy Clusters
- An AzTEC 1.1 mm survey of the GOODS-N field -- II. Multi-wavelength identifications and redshift distribution
- Cosmic evolution of the galaxy mass and luminosity functions by morphological type from multi-wavelength data in the CDF-South
- AGN and Starburst Classification from Spitzer Mid-Infrared Spectra for High Redshift SWIRE Sources
- Models for Multiband IR Surveys
- The Mid-Infrared Environments of High-Redshift Radio Galaxies
- Dust temperture and the submillimetre-radio flux density ratio as a redshift indicator for distant galaxies
- Simulating the Spitzer mid-IR color-color diagrams
- Synthetic stellar populations: single stellar populations, stellar interior models and primordial proto-galaxies
- Ultradeep Ks Imaging in the GOODS-N
- New light on gamma-ray burst host galaxies with Herschel
- The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- I. Survey motivation, design and data processing
- IRAC Imaging of Lockman Hole
- A mature galaxy cluster at z=1.58 around the radio galaxy 7C1753+6311
- Herschel reveals a T_dust-unbiased selection of z~2 ULIRGs
- A Comparison of X-ray and Mid-Infrared Selection of Obscured AGN
- Accurate Spectral energy distributions and selection effects for high-redshift dusty galaxies: a new hot population to discover with the Spitzer Space Telescope?
- The SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII. The Nature of Faint Submm Galaxies in SHADES, SWIRE and SXDF Surveys
- Spitzer IRS Spectra of Optically Faint Infrared Sources with Weak Spectral Features
- Identification of luminous infrared galaxies at 1<z<2.5
- Spitzer IRAC Infrared Colours of Submillimetre-bright Galaxies
- Anomalously low PAH emission from low-luminosity galaxies
- The extremely red host galaxy of GRB 080207
- MAMBO 1.2mm observations of luminous starbursts at z~2 in the SWIRE fields
- Star Formation and AGN activity in Galaxies classified using the 1.6 μm Bump and PAH features at
- Sub-millimeter detections of Spitzer Space Telescope galaxy populations
- Candidate Clusters of Galaxies at Identified in the Spitzer SPT Deep Field Survey
- Mid-infrared spectroscopy of Spitzer-selected ultra-luminous starbursts at z~2
- Keck spectroscopy of z=1-3 ULIRGs from the Spitzer SWIRE survey
- VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2<z<2.1 selected from Spitzer IRAC 3.6 micron and 4.5 micron photometry
- Confusion limit due to galaxies: using SIRTF's Infrared Array Camera
- Using the 1.6um Bump to Study Rest-frame NIR Selected Galaxies at Redshift 2
- The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
- The ESO-Spitzer Imaging extragalactic Survey (ESIS) II: VIMOS I,z wide field imaging of ELAIS-S1 and selection of distant massive galaxies
- Far-Infrared Spectral Energy Distributions and Photometric Redshifts of Dusty Galaxies
- The Environment on few Mpc scales of Infrared Luminous Galaxies at Redshifts z~1
- Dust-obscured star formation and the contribution of galaxies escaping UV/optical color selections at z~2
- The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field
- The Environments of Luminous Radio - WISE Selected Infrared Galaxies
- Predictions for the Counts of Faint, High-Redshift Galaxies in the Mid-Infrared
- -selected protocluster candidates in the LSST Deep Drilling Fields
- Comparing Ultraviolet and Infrared-Selected Starburst Galaxies in Dust Obscuration and Luminosity
- Dusty Quasars at High Redshifts