The Herschel Stripe 82 Survey (HerS): Maps and Early Catalog
arXiv:1308.4399 · doi:10.1088/0067-0049/210/2/22
Abstract
We present the first set of maps and band-merged catalog from the Herschel Stripe 82 Survey (HerS). Observations at 250, 350, and 500 micron were taken with the Spectral and Photometric Imaging Receiver (SPIRE) instrument aboard the Herschel Space Observatory. HerS covers 79 deg along the SDSS Stripe 82 to a depth of 13.0, 12.9, and 14.8 mJy beam (including confusion) at 250, 350, and 500 micron, respectively. HerS was designed to measure correlations with external tracers of the dark matter density field --- either point-like (i.e., galaxies selected from radio to X-ray) or extended (i.e., clusters and gravitational lensing) --- in order to measure the bias and redshift distribution of intensities of infrared-emitting dusty star-forming galaxies and AGN. By locating HeRS in Stripe 82, we maximize the overlap with available and upcoming cosmological surveys. The band-merged catalog contains 3.3x10 sources detected at a significance of >3 (including confusion noise). The maps and catalog are available at http://www.astro.caltech.edu/hers/
Accepted to ApJS. 11 Pages, 7 figures. Data available at http://www.astro.caltech.edu/hers/
References in corpus (11)
- A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
- The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
- The Detection of a Population of Submillimeter-Bright, Strongly-Lensed Galaxies
- Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
- Over half of the far-infrared background light comes from galaxies at z >= 1.2
- HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift
- HerMES: Candidate High-Redshift Galaxies Discovered with Herschel/SPIRE
- A joint analysis of BLAST 250--500um and LABOCA 870um observations in the Extended Chandra Deep Field South
- High-resolution VLA Imaging of SDSS Stripe 82 at 1.4 GHz
- SANEPIC: A Map-Making Method for Timestream Data From Large Arrays
- An In-Depth View of the Mid-Infrared Properties of Point Sources and the Diffuse ISM in the SMC Giant HII Region, N66
Cited by in corpus (106)
- The Atacama Cosmology Telescope: CMB Polarization at
- The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog
- Clustering of intermediate redshift quasars using the final SDSS III-BOSS sample
- The Herschel-ATLAS: a sample of 500μm-selected lensed galaxies over 600 square degrees
- The IAC Stripe 82 Legacy Project: a wide-area survey for faint surface brightness astronomy
- The Atacama Cosmology Telescope: Modeling the Gas Thermodynamics in BOSS CMASS galaxies from Kinematic and Thermal Sunyaev-Zel'dovich Measurements
- Galactic cirri in deep optical imaging
- The Sloan Digital Sky Survey Stripe 82 Imaging Data: Depth-Optimized Co-adds Over 300 Deg^2 in Five Filters
- Decreased Specific Star Formation Rates in AGN Host Galaxies
- HELP: The Herschel Extragalactic Legacy Project
- The star formation rates of active galactic nuclei host galaxies
- The 31 Deg Release of the Stripe 82 X-ray Survey: The Point Source Catalog
- Candidate Gravitationally Lensed Dusty Star-forming Galaxies in the Herschel Wide Area Surveys
- The Spitzer-HETDEX Exploratory Large-Area Survey
- The WISSH quasars Project: II. Giant star nurseries in hyper-luminous quasars
- HELP: A catalogue of 170 million objects, selected at 0.36-4.5 m, from 1270 deg. of prime extragalactic fields
- Star formation black hole growth and dusty tori in the most luminous AGNs at z=2-3.5
- Herschel far-infrared photometry of the Swift Burst Alert Telescope active galactic nuclei sample of the local universe - III. Global star-forming properties and the lack of a connection to nuclear activity
- Early Science with the Large Millimeter Telescope: Observations of Extremely Luminous High-z Sources Identified by Planck
- AGN Populations in Large Volume X-ray Surveys: Photometric Redshifts and Population Types found in the Stripe 82X Survey
- Evidence of suppression of star formation by quasar-driven winds in gas-rich host galaxies at z<1?
- Star Formation in Luminous Quasars at 2<z<3
- SpIES: The Spitzer IRAC Equatorial Survey
- Exploring AGN and Star Formation Activity of Massive Galaxies at Cosmic Noon
- SDSS-IV eBOSS Spectroscopy of X-ray and WISE AGN in Stripe 82X: Overview of the Demographics of X-ray and Mid-Infrared Selected Active Galactic Nuclei
- NOEMA redshift measurements of bright Herschel galaxies
- Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel
- Extreme star formation events in quasar hosts over
- The Red Radio Ring: a gravitationally lensed hyperluminous infrared radio galaxy at z=2.553 discovered through citizen science
- Evidence for the Thermal Sunyaev-Zel'dovich Effect Associated with Quasar Feedback
- Total Molecular Gas Masses of Planck - Herschel Selected Strongly Lensed Hyper Luminous Infrared Galaxies
- A Measurement of the Millimeter Emission and the Sunyaev-Zel'dovich Effect Associated with Low-Frequency Radio Sources
- Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE
- The multiplicity of 250-m Herschel sources in the COSMOS field
- Local SDSS galaxies in the Herschel Stripe82 survey: A critical assessment of optically-derived star-formation rates
- On the redshift distribution and physical properties of ACT-selected DSFGs
- A deep / wide 1-2 GHz snapshot survey of SDSS Stripe 82 using the Karl G. Jansky Very Large Array in a compact hybrid configuration
- Co-evolution of Extreme Star Formation and Quasar: hints from {\it Herschel} and the Sloan Digital Sky Survey
- The infra-red luminosities of ~332,000 SDSS galaxies predicted from artificial neural networks and the Herschel Stripe 82 survey
- Radio Properties of the BAT AGN: the FIR-Radio Relation, the Fundamental Plane, and the Main Sequence of Star Formation
- Cross-calibration of CO- vs dust-based gas masses and assessment of the dynamical mass budget in Herschel-SDSS Stripe82 galaxies
- Dynamical analysis of the dark matter and central black hole mass in the dwarf spheroidal Leo I
- The abundance of compact quiescent galaxies since z ~ 0.6
- Atacama Cosmology Telescope: Dusty star-forming galaxies and active galactic nuclei in the equatorial survey
- Herschel observed Stripe 82 quasars and their host galaxies: connections between the AGN activity and the host galaxy star formation
- The Bright Extragalactic ALMA Redshift Survey (BEARS) II: Millimetre photometry of gravitational lens candidates
- A magnified view of circumnuclear star formation and feedback around an AGN at z=2.6
- Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case
- Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
- Significant Suppression of Star Formation in Radio-Quiet AGN Host Galaxies with Kiloparsec-Scale Radio Structures
- ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
- Exploiting NIKA2/XMM-Newton imaging synergy for intermediate mass, high- galaxy clusters within the NIKA2 SZ Large Program
- The co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background
- Infrared luminosity functions and dust mass functions in the EAGLE simulation
- VICS82: the VISTA-CFHT Stripe 82 near-infrared survey
- PASSAGES: The Large Millimeter Telescope and ALMA Observations of Extremely Luminous High Redshift Galaxies Identified by the Planck
- The XMM-Newton survey in the H-ATLAS field
- The Accretion History of AGN: A Newly Defined Population of Cold Quasars
- On Mass Concentrations & Magnitude Gaps of Galaxy Systems in the CS82 Survey
- Prospects for future studies using deep imaging: Analysis of individual Galactic cirrus filaments
- Lurking systematics in predicting galaxy cold gas masses using dust luminosities and star formation rates
- Resolved CO(1-0) emission and gas properties in luminous dusty star forming galaxies at z=2-4
- Cosmology with the submillimetre galaxies magnification bias: Proof of concept
- Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
- Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
- Fractal dimension of optical cirrus in Stripe82
- The Circumgalactic Medium of Submillimeter Galaxies. I. First Results from a Radio-Identified Sample
- Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
- The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
- ALMA resolves the first strongly-lensed Optical/NIR-dark galaxy
- Measurements of the Cross Spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz
- Far-infrared observations of an unbiased sample of gamma-ray burst host galaxies
- Broad-band spectral energy distribution of 3000 Angstroem break quasars from the Sloan Digital Sky Survey
- Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82
- "Red" but Not "Dead": Actively Star-forming Brightest Cluster Galaxies at Low Redshifts
- SHALOS: Statistical Herschel-ATLAS Lensed Objects Selection
- On the multiplicity of ALMA Compact Array counterparts of far-infrared bright quasars
- Correlation of structure and stellar properties of galaxies in Stripe 82
- On the Limited Sizes of Dusty Starbursting Regions at High Redshifts
- A search for candidate strongly-lensed dusty galaxies in the Planck satellite catalogues
- The Subtle Effects of Mergers on Star Formation in Nearby Galaxies
- Obscuration properties of mid-IR selected AGN
- The faint end of the 250 micron luminosity function at z < 0.5
- The far-infrared/radio correlation for a sample of strongly lensed dusty star-forming galaxies detected by Herschel
- A data-scientific noise-removal method for efficient submillimeter spectroscopy with single-dish telescopes
- Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
- Accretion History of AGN: Estimating the Host Galaxy Properties in X-ray Luminous AGN from z=0-3
- [NII] fine-structure emission at 122 and 205um in a galaxy at z=2.6: a globally dense star-forming interstellar medium
- Constraints on galaxy formation from the cosmic-far-infrared-background\,\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
- ALMA 1.1mm Observations of a Conservative Sample of High Redshift Massive Quiescent Galaxies in SHELA
- Star-dust geometry main determinant of dust attenuation in galaxies
- A Systematic Search for Reddest Far-infrared and Sub-millimeter Galaxies: revealing dust-embedded starbursts at high redshifts
- Massive molecular gas reservoir in a luminous sub-millimeter galaxy during cosmic noon
- The Atacama Cosmology Telescope: SZ-based masses and dust emission from IR-selected cluster candidates in the SHELA survey
- "Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift
- A Ly-alpha nebula at z~3.3
- Infrared galaxies detected by the Atacama Cosmology Telescope
- A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
- An ALMA Band 7 survey of SDSS/Herschel quasars in Stripe 82: I. The properties of the 870 micron counterparts
- The molecular-gas properties in the gravitationally lensed merger HATLAS J142935.3-002836
- Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
- The Herschel-SPIRE Dark Field I: The deepest Herschel image of the submillimetre Universe
- The Origin of the Gas and Its Low Star Formation Efficiency in Quiescent Galaxies
- A low-mass galaxy cluster as a test-case study for the NIKA2 SZ Large Program
- The Impact of Far-Infrared/Sub-Millimeter Data on the Star Formation Rates of Massive Dusty Galaxies at Cosmic Noon
- The LMT 2 Millimeter Receiver System (B4R). I. Overview and Results of Science Demonstration