The H Luminosity Function and Star Formation Rate at in the Cosmos 2 Square-Degree Field
arXiv:0709.1009 · doi:10.1086/523703
Abstract
To derive a new H luminosity function and to understand the clustering properties of star-forming galaxies at , we have made a narrow-band imaging survey for H emitting galaxies in the HST COSMOS 2 square degree field. We used the narrow-band filter NB816 ( Å, Å) and sampled H emitters with $EW_{\rm obs}(\rm Hα+ [N\textsc{ii}]) > 12$ Åin a redshift range between and corresponding to a depth of 70 Mpc. We obtained 980 H emitting galaxies in a sky area of 5540 arcmin, corresponding to a survey volume of . We derive a H luminosity function with a best-fit Schechter function parameter set of , , and . The H luminosity density is ergs s Mpc. After subtracting the AGN contribution (15 %) to the H luminosity density, the star formation rate density is evaluated as $M_{\sun}$ yr Mpc. The angular two-point correlation function of H emitting galaxies of is well fit by a power law form of , corresponding to the correlation function of . We also find that the H emitters with higher H luminosity are more strongly clustered than those with lower luminosity.
arXiv comment13 pages, 9 fifgure, to apper in ApJS
References in corpus (63)
- Star Formation in Galaxies Along the Hubble Sequence
- High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
- The CANADA-FRANCE REDSHIFT SURVEY XIII: The luminosity density and star-formation history of the Universe to z ~ 1
- Estimating Star Formation Rates from Infrared and Radio Luminosities: The Origin of the Radio-Infrared Correlation
- The Luminosity and Color Dependence of the Galaxy Correlation Function
- Infrared luminosity functions from the Chandra Deep Field South : the Spitzer view on the history of dusty star formation at 0<z<1
- The First Release COSMOS Optical and Near-IR Data and Catalog
- Subaru Prime Focus Camera -- Suprime-Cam --
- On the evolution of star forming galaxies
- Nebular Emission from Star-Forming Galaxies
- The 2dF Galaxy Redshift Survey: Luminosity dependence of galaxy clustering
- Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements
- The Evolution of the Global Star Formation History as Measured from the Hubble Deep Field
- The Rest-Frame UV Luminosity Density of Star-Forming Galaxies at Redshifts z>3.5
- Star formation rate indicators in the Sloan Digital Sky Survey
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- The GALEX-VVDS Measurement of the Evolution of the Far-Ultraviolet Luminosity Density and the Cosmic Star Formation Rate
- Dust attenuation in the nearby Universe: comparison between galaxies selected in the ultraviolet or in the infrared
- On Departures From a Power Law in the Galaxy Correlation Function
- The Subaru Deep Field Project: Lyman Emitters at Redshift of 6.6
- The Ha Luminosity Function and Star Formation Rate at z\sim 0.2
- Towards a resolution of the discrepancy between different estimators of star formation rate
- Evidence for a Gradual Decline in the Universal Rest-Frame UV Luminosity Density for z < 1
- The Survey for Ionization in Neutral Gas Galaxies: I. Description and Initial Results
- An Ultraviolet-Selected Galaxy Redshift Survey - II: The Physical Nature of Star Formation in an Enlarged Sample
- Spectrophotometry of nearby field galaxies: the data
- Active Galactic Nuclei in the Sloan Digital Sky Survey: II. Emission-Line Luminosity Function
- The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for Narrow-band Emitters in the Subaru Deep Field
- CFRS XIV: Spectral Properties Of Field Galaxies Up To z = 1
- An Ultraviolet-Selected Galaxy Redshift Survey: New Estimates of the Local Star Formation Rate
- Subaru Deep Survey VI. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Clustering Properties
- Measurement of Star-Formation Rate from H-alpha in field galaxies at z=1
- A large sample of spectroscopic redshifts in the ACS-GOODS region of the HDF-N
- The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data
- The oxygen-II luminosity density of the Universe
- The H Luminosity Function and Global Star Formation Rate From Redshifts of One to Two
- Current Performance and On-Going Improvements of the 8.2 m Subaru Telescope
- Photometric Redshifts of Galaxies in COSMOS
- Surface photometry of nearby field galaxies: the data
- Definitive Identification of the Transition between Small- to Large-Scale Clustering for Lyman Break Galaxies
- The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies as a Function of Luminosity at z=1
- The DEEP2 Galaxy Redshift Survey: Clustering of Quasars and Galaxies at z=1
- Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field
- The Ha luminosity function and star formation rate up to z~1
- Star Formation History since z = 1.5 as Inferred from Rest-Frame Ultaviolet Luminosity Density Evolution
- Clustering of Lyman Break Galaxies at z=4 and 5 in The Subaru Deep Field: Luminosity Dependence of The Correlation Function Slope
- Spectral Analysis of the Stromlo-APM Survey I. Spectral Properties of Galaxies
- The Canada-France Redshift Survey XII: Nature of emission-line field galaxy population up to z = 0.3
- Star Formation, Metallicity and Dust Properties Derived from the SAPM Galaxy Survey Spectra
- Spatial analysis of the Halpha emission in the local star-forming UCM galaxies
- Star forming rates between z=0.25 and z=1.2 from the CADIS emission line survey
- The Halpha Luminosity Function and Star Formation Rate at z~0.24 Based on Subaru Deep Imaging Data
- Rapid Evolution in the Most Luminous Galaxies During the First 900 Million Years
- Star Formation in a Complete Spectroscopic Survey of Galaxies
- The Survey for Ionization in Neutral Gas Galaxies- II. The Star Formation Rate Density of the Local Universe
- The [OII]3727 Luminosity function and Star Formation Rate at z~1.2 in the COSMOS 2 Square-degree Field and the Subaru Deep Field
- The [OII]3727 Luminosity Function of the Local Universe
- Star Formation in HI Selected Galaxies I: Sample Characteristics
- Emission Line Galaxies in the STIS Parallel Survey II: Star Formation Density
- H alpha emitting galaxies and the star formation rate density at z~0.24
- The KPNO International Spectroscopic Survey. IV. H-alpha-selected Survey List 2
- Dependence of Dust Obscuration on Star Formation Rates in Galaxies
- Dust Absorption and the Cosmic UV Flux Density
Cited by in corpus (68)
- A large Hα survey at z=2.23, 1.47, 0.84 & 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS
- Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly
- Star formation at z=1.47 from HiZELS: An Hα+[OII] double-blind study
- HiZELS: a high redshift survey of H-alpha emitters. I: the cosmic star-formation rate and clustering at z=2.23
- The dependence of star formation activity on environment and stellar mass at z~1 from the HiZELS H-alpha survey
- The stellar mass function of star-forming galaxies and the mass-dependent SFR function since z=2.23 from HiZELS
- HiZELS: a high redshift survey of H-alpha emitters. II: the nature of star-forming galaxies at z=0.84
- SHARDS: an optical spectro-photometric survey of distant galaxies
- Galaxy And Mass Assembly: Evolution of the Halpha luminosity function and star formation rate density up to z<0.35
- The Subaru COSMOS 20: Subaru Optical Imaging of the HST COSMOS Field with 20 Filters
- Modelling the number density of Halpha emitters for future spectroscopic near-IR space missions
- The clustering of H-alpha emitters at z=2.23 from HiZELS
- The Halpha-based Star Formation Rate Density of the Universe at z=0.84
- The H alpha Galaxy Survey. VIII. Close companions and interactions, and the definition of starbursts
- Triggered Star Formation in Galaxy Pairs at z=0.08-0.38
- The dust un-biased cosmic star formation history from the 20 cm VLA-COSMOS survey
- The rise and fall of star-formation in merging galaxy clusters
- Nebular Attenuation in Hα-selected Star-forming Galaxies at z=0.8 from the NewHα Survey
- MC: Boosted AGN and star-formation activity in CIZA J2242.8+5301, a massive post-merger cluster at z=0.19
- Empirical H-alpha emitter count predictions for dark energy surveys
- The nebular emission of star-forming galaxies in a hierarchical universe
- The role of cluster mergers and travelling shocks in shaping the H luminosity function at : `sausage' and `toothbrush' clusters
- A Dual Narrowband Survey for Hα Emitters at z=2.2: Demonstration of the Technique and Constraints on the Hα Luminosity Function
- Global Star Formation Rate Density over 0.7<z<1.9
- The Relationship between Stellar Mass, Gas Metallicity, and Star Formation Rate for Halpha-selected Galaxies at z~0.8 from the NewHalpha Survey
- The clustering and evolution of H-alpha emitters at z~1 from HiZELS
- A large H survey of star formation in relaxed and merging galaxy cluster environments at
- Evolution of Star Formation in the UKIDSS Ultra Deep Survey Field - I. Luminosity Functions and Cosmic Star Formation Rate out to z=1.6
- Spectrophotometry with Hectospec, the MMT's Fiber-Fed Spectrograph
- A large narrow band H survey at : the bright end of the luminosity function, cosmic variance and clustering across cosmic time
- Cosmic Star Formation Activity at z=2.2 Probed by H-alpha Emission Line Galaxies
- The clustering of typical Ly emitters from : host halo masses depend on Ly and UV luminosities
- A 16 deg survey of emission-line galaxies at z<1.5 in HSC-SSP PDR1
- Evolution of the Halpha luminosity function
- Calibrating [OII] star-formation rates at z>1 from dual Hα-[OII] imaging from HiZELS
- A Faint Flux-Limited Lyman Alpha Emitter Sample at
- The Wyoming Survey for H-alpha. III. H-alpha Luminosity Functions at z ~ 0.16, 0.24, 0.32, and 0.40
- Environmental Effects on the Star Formation Activity in Galaxies at z=1.2 in the COSMOS Field
- An high definition view of the COSMOS Wall at z~0.73
- The Faint-End Slope of the Redshift 5.7 Lyman Alpha Luminosity Function
- Detections of Faint Lyman-alpha Emitters at z = 5.7: Galaxy Building Blocks and Engines of Reionization
- Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
- A large, deep 3 deg survey of H, [OIII], and [OII] emitters from LAGER: constraining luminosity functions
- Exploring star formation using the filaments in the Sloan Digital Sky Survey Data Release Five (SDSS DR5)
- On-sky characterisation of the VISTA NB118 narrow-band filters at 1.19 micron
- Galaxy And Mass Assembly (GAMA): Bivariate functions of H star forming galaxies
- The clustering of H+[OIII] and [OII] emitters since : dependencies with line luminosity and stellar mass
- Galaxies with Background QSOs, I: A Search for Strong Galactic H-alpha Lines
- The miniJPAS survey: Identification and characterization of the emission line galaxies down to in the AEGIS field
- The Role of Galaxy Interaction in Environmental Dependence of the Star Formation Activity at z~1.2
- Star-Forming Galaxies at z=0.24 in the Subaru Deep Field and the Sloan Digital Sky Survey
- ENISALA: II. Distinct Star Formation and Active Galactic Nucleus Activity in Merging and Relaxed Galaxy Clusters
- The FMOS-COSMOS survey of star-forming galaxies at . V: Properties of dark matter halos containing H emitting galaxies
- Star-forming galaxies at low-redshift in the SHARDS survey
- HiZELS: the High Redshift Emission Line Survey with UKIRT
- A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
- Bulgeless galaxies in the COSMOS field: environment and star formation evolution at
- Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations
- On the triggering of extreme starburst events in low-metallicity galaxies: a deep search for companions of Green Peas
- The OTELO survey. II. The faint-end of the H luminosity function at z 0.40
- A deg blind survey for CII], CIII] and CIV at . II: luminosity functions and cosmic average line ratios
- Near-identical star formation rate densities from H and FUV at redshift zero
- The double galaxy cluster Abell 2465 - II. Star formation in the cluster
- Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
- Euclid preparation. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
- A comprehensive study of H emitters at 0.62 in the DAWN survey: the need for deep and wide regions
- Properties of galaxies at the faint end of the H luminosity function at
- Environmental Effects on the Star Formation Activity at z~0.9 in the COSMOS Field