The MUSE-Wide Survey: A determination of the Lyman emitter luminosity function at
arXiv:1810.05037 · doi:10.1051/0004-6361/201834164
Abstract
(Abridged) We investigate the Lyman emitter luminosity function (LAE LF) within the redshift range from the first instalment of the blind integral field spectroscopic survey MUSE-Wide. This initial part of the survey probes a region of 22.2 arcmin in the CANDELS/GOODS-S field. The dataset provided us with 237 LAEs from which we construct the LAE LF in the luminosity range within a volume of Mpc. For the LF construction we utilise three different non-parametric estimators: The classical method, the method, and an improved binned estimator for the differential LF. All three methods deliver consistent results, with the cumulative LAE LF being Mpc and Mpc towards the bright- and faint-end of our survey, respectively. By employing a non-parametric statistical test, as well as by comparing the full sample to sub-samples in redshift bins, we find no supporting evidence for an evolving LAE LF over the probed redshift and luminosity range. We determine the best-fitting Schechter function parameters and with the corresponding normalisation . When correcting for completeness in the LAE LF determinations, we take into account that LAEs exhibit diffuse extended low surface-brightness haloes. We compare the resulting LF to one obtained where we apply a correction assuming compact point-like emission. We find that the standard correction underestimates the LAE LF at the faint end of our survey by a factor of 2.5.
arXiv comment23 pages, 18 figures. A&A in press
References in corpus (76)
- Astropy: A Community Python Package for Astronomy
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics
- The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- The Hubble Ultra Deep Field
- Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models
- UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History
- The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN
- The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
- High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data IV: Luminosity Function from the Fall Equatorial Stripe Sampl
- Diffuse Lyman Alpha Emitting Halos: A Generic Property of High Redshift Star Forming Galaxies
- Ly-alpha Emission-Line Galaxies at z = 3.1 in the Extended Chandra Deep Field South
- The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection
- ZAP -- Enhanced PCA Sky Subtraction for Integral Field Spectroscopy
- Evidence for PopIII-like stellar populations in the most luminous Lyman- emitters at the epoch of re-ionisation: spectroscopic confirmation
- The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs
- High-z Lyman-alpha Emitters. I. A Blank-Field Search for Objects Near Redshift z=3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA22
- The Density of Lyman-alpha Emitters at Very High Redshift
- Extended Lyman alpha haloes around individual high-redshift galaxies revealed by MUSE
- Ly Alpha Emitters at z=5.7 in the Subaru Deep Field
- WFPC2 Observations of the Hubble Deep Field-South
- Subaru Deep Survey II. Luminosity Functions and Clustering Properties of Lya Emitters at z=4.86 in the Subaru Deep Field
- A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems
- The MUSE 3D view of the Hubble Deep Field South
- Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program Strategy and Clustering Properties of ~2,000 Lya Emitters at z=6-7 over the 0.3-0.5 Gpc Survey Area
- The effects of seeing on Sersic profiles. II. The Moffat PSF
- The Luminosity Function of Lyman Alpha Emitters at Redshift z~5.7
- Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at Derived with the Half-Million Dropouts on the 100 deg Sky
- The Lyman-Continuum Photon Production Efficiency xi_{ion} of z~4-5 Galaxies from IRAC-based Halpha Measurements: Implications for the Escape Fraction and Cosmic Reionization
- The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
- The HETDEX Pilot Survey. II. The Evolution of the Ly-alpha Escape Fraction from the UV Slope and Luminosity Function of 1.9<z<3.8 LAEs
- Identification of the brightest Lyα emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era
- Discovery of 9 Ly alpha emitters at redshift z~3.1 using narrow-band imaging and VLT spectroscopy
- Diffuse Lyman-alpha Halos around Galaxies at z=2.2-6.6: Implications for Galaxy Formation and Cosmic Reionization
- HETDEX pilot survey for emission-line galaxies - I. Survey design, performance, and catalog
- Discovery of a Giant Lya Emitter Near the Reionization Epoch
- What is the physical origin of strong Lya emission? II. Gas Kinematics and Distribution of Lya Emitters
- An improved method of constructing binned luminosity functions
- Detection of Lyman-alpha Emitting Galaxies at Redshift z=4.55
- SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7
- Slicing COSMOS with SC4K: the evolution of typical Lya emitters and the Lya escape fraction from z~2 to z~6
- A Luminosity Function of Lyman Alpha Emitting Galaxies at Redshift 4.5
- Bright and Faint Ends of Ly Luminosity Functions at Determined by the Subaru Survey: Implications for AGN, Magnification Bias, and ISM HI Evolution
- The VIMOS VLT Deep Survey: Star Formation Rate Density of Lya emitters from a sample of 217 galaxies with spectroscopic redshifts 2<z<6.6
- The Lyman-alpha luminosity function at z=5.7-6.6 and the steep drop of the faint end: implications for reionization
- Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field
- The MUSE-Wide Survey: A first catalogue of 831 emission line galaxies
- The MUSE Hubble Ultra Deep Field Survey VI: The Faint-End of the Lya Luminosity Function at 2.91 < z < 6.64 and Implications for Reionisation
- Estimating Galaxy Luminosity Functions
- The nature of luminous Lyman-alpha emitters at z~2-3: maximal dust-poor starbursts and highly ionising AGN
- The ionizing photon production efficiency of compact z~0.3 Lyman continuum leakers and comparison with high redshift galaxies
- Shedding Light on the Galaxy Luminosity Function
- An Ultraluminous Lyman Alpha Emitter with a Blue Wing at z=6.6
- LSDCat: Detection and cataloguing of emission-line sources in integral-field spectroscopy datacubes
- The luminosity function of Ly-alpha emitters at 2.3 < z < 4.6 from integral-field spectroscopy
- On the contribution of fluorescence to Ly halos (LAHs) around star forming galaxies
- MUSE Deep-Fields: The Lya Luminosity Function in the Hubble Deep Field South at 2.91 < z < 6.64
- Photometric properties of Ly alpha emitters at z=4.86 in the COSMOS 2 square degree field
- Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at
- Predicting the redshift 2 Halpha luminosity function using [OIII] emission line galaxies
- A High Space Density of Luminous Lyman Alpha Emitters at z~6.5
- Connecting Faint End Slopes of the Lyman- emitter and Lyman-break Galaxy Luminosity Functions
- The Building the Bridge survey for z=3 Ly-alpha emitting galaxies II: Completion of the survey
- MUSE observations of the lensing cluster Abell 1689
- A Faint Flux-Limited Lyman Alpha Emitter Sample at
- A Magellan IMACS Spectroscopic Search for Lyman-Alpha Emitting Galaxies at Redshift 5.7
- Lyman-alpha emission galaxies at a redshift of z = 5.7 in the FORS Deep Field
- The Faint-End Slope of the Redshift 5.7 Lyman Alpha Luminosity Function
- A Subaru Search for Lyman-Alpha Emitters at z=5.8 with an Intermediate-Band Filter
- The DEEP2 Redshift Survey: Lyman Alpha Emitters in the Spectroscopic Database
- A Deep Ly Survey in ECDF-S and COSMOS: I. General Properties of Lyman-alpha Emitters at
- The properties of the brightest Lyman alpha emitters at z~5.7
- Lyman Emitters beyond Redshift 5:The Dawn of Galaxy Formation
- A graphical analysis of the systematic error of classical binned methods in constructing luminosity functions
- Nonparametric Methods in Astronomy: Think, Regress, Observe -- Pick Any Three
Cited by in corpus (54)
- Observations of the Lyman- Universe
- An Atlas of MUSE Observations towards Twelve Massive Lensing Clusters
- The MUSE-Wide Survey: Survey Description and First Data Release
- The MUSE Hubble Ultra Deep Field surveys: Data release II
- MUSE Analysis of Gas around Galaxies (MAGG) -- III: The gas and galaxy environment of z = 3-4.5 quasars
- The X-SHOOTER Lyman- survey at z=2 (XLS-z2) I: What makes a galaxy a Lyman- emitter?
- The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift
- RASCAS: RAdiation SCattering in Astrophysical Simulations
- LAGER Ly Luminosity Function at , Implications for Reionization
- (Re)Solving Reionization with Lyα: How Bright Lyα Emitters account for the Cosmic Ionizing Background
- MUSE Analysis of Gas around Galaxies (MAGG) -- I: Survey design and the environment of a near pristine gas cloud at z~3.5
- Lyman- as a tracer of cosmic reionisation in the SPHINX radiation-hydrodynamics cosmological simulation
- MUSE Analysis of Gas around Galaxies (MAGG) -- IV: The gaseous environment of 3-4 Lyman-alpha emitting galaxies
- The role of galaxies and AGN in reionising the IGM -- III : IGM-galaxy cross-correlations at z~6 from 8 quasar fields with DEIMOS and MUSE
- Spectral shapes of the Lyman-alpha emission from galaxies: I. blueshifted emission and intrinsic invariance with redshift
- The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework
- Equivalent widths of Lyman emitters in MUSE-Wide and MUSE-Deep
- Faint end of the luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE
- Deciphering Lyman blob 1 with deep MUSE observations
- GA-NIFS: High number of dual active galactic nuclei at z~3
- Stars and gas in the most metal-poor galaxies I: COS and MUSE observations of SBS 0335-052E
- J-PLUS: Unveiling the brightest-end of the Lyα luminosity function at 2.0<z<3.3 over 1000 deg^2
- Dissecting the interstellar medium of a z=6.3 galaxy: X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A
- First HETDEX Spectroscopic Determinations of Ly and UV Luminosity Functions at : Bridging a Gap Between Faint AGN and Bright Galaxies
- MUSE Analysis of Gas around Galaxies (MAGG) -- V: Linking ionized gas traced by CIV and SiIV absorbers to Ly emitting galaxies at
- Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at
- Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913
- Spectral Shapes of the Lya Emission from Galaxies. II. the influence of stellar properties and nebular conditions on the emergent Lya profiles
- Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionised bubble at z = 6.53
- Bright Lyman emitters among Spitzer SMUVS galaxies in the MUSE/COSMOS field
- Measuring the average molecular gas content of star-forming galaxies at
- Clustering dependence on Lyman- luminosity from MUSE surveys at
- Probing the faint end Luminosity Function of Lyman Alpha Emitters at 3<z<7 behind 17 MUSE lensing clusters
- Lyman-alpha radiation pressure: an analytical exploration
- The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman- emitters at
- Deciphering stellar metallicities in the early Universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
- Evolution of the Lyman-α emitting fraction and UV properties of lensed star-forming galaxies between 2.9 < z < 6.7
- Three Dimensional Optimal Spectral Extraction (TDOSE) from Integral Field Spectroscopy
- A flexible method for estimating luminosity functions via Kernel Density Estimation
- A Spectroscopic Survey of Ly Emitters at over 1.2 Deg
- Linking UV spectral properties of MUSE Ly-alpha emitters at z>3 to Lyman continuum escape
- Accretion-Driven Sources in Spatially Resolved Ly Emitters
- The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX) II. Luminosity Function
- Lyman Alpha line properties at and their environmental dependence: a case study around a massive proto-cluster
- The OTELO survey: Faint end of the luminosity function of [OII] emitters at <z>= 1.43
- Revisiting the Emission Line Source Detection Problem in Integral Field Spectroscopic Data
- MUSE Analysis of Gas around Galaxies (MAGG) -- VI. The cool and enriched gas environment of z3 Ly emitters
- Probing the cosmic web in Ly emission over large scales: an Intensity Mapping forecast for DECaLS/BASS and DESI
- The contribution of faint Lyman- emitters to extended Lyman- halos constrained by MUSE clustering measurements
- The Intrinsic Distribution of Lyman- Halos
- Discovery of faint double-peak Halpha emission in the halo of low redshift galaxies
- Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
- Discovery of a damped Ly galaxy at z 3 towards the quasar SDSS J011852+040644
- Bayesian luminosity function estimation in multi-depth datasets with selection effects: A case study for Lyman emitters