The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
arXiv:1710.03773 · doi:10.1051/0004-6361/201731195
Abstract
We have conducted a two-layered spectroscopic survey (1'x1' ultra deep and 3'x3' deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE). The combination of a large field of view, high sensitivity, and wide wavelength coverage provides an order of magnitude improvement in spectroscopically confirmed redshifts in the HUDF; i.e., 1206 secure spectroscopic redshifts for HST continuum selected objects, which corresponds to 15% of the total (7904). The redshift distribution extends well beyond z>3 and to HST/F775W magnitudes as faint as ~30 mag (AB, 1-sigma). In addition, 132 secure redshifts were obtained for sources with no HST counterparts that were discovered in the MUSE data cubes by a blind search for emission-line features. In total, we present 1338 high quality redshifts, which is a factor of eight increase compared with the previously known spectroscopic redshifts in the same field. We assessed redshifts mainly with the spectral features [OII] at z<1.5 (473 objects) and Lya at 2.9<z<6.7 (692 objects). With respect to F775W magnitude, a 50% completeness is reached at 26.5 mag for ultra deep and 25.5 mag for deep fields, and the completeness remains >~20% up to 28-29 mag and ~27 mag, respectively. We used the determined redshifts to test continuum color selection (dropout) diagrams of high-z galaxies. The selection condition for F336W dropouts successfully captures ~80% of the targeted z~2.7 galaxies. However, for higher redshift selections (F435W, F606W, and F775W dropouts), the success rates decrease to ~20-40%. We empirically redefine the selection boundaries to make an attempt to improve them to ~60%. The revised boundaries allow bluer colors that capture Lya emitters with high Lya equivalent widths falling in the broadbands used for the color-color selection. Along with this paper, we release the redshift and line flux catalog.
arXiv comment26 pages, 26 figures, 4 tables, accepted for publication in A&A (MUSE UDF Series Paper II), the redshift catalogs will be available at the CDS
References in corpus (62)
- Stellar population synthesis at the resolution of 2003
- The Sloan Digital Sky Survey: Technical Summary
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
- EAZY: A Fast, Public Photometric Redshift Code
- A Simple Model for the Absorption of Starlight by Dust in Galaxies
- MILES: A Medium resolution INT Library of Empirical Spectra
- Rest-Frame Ultraviolet Spectra of z~3 Lyman Break Galaxies
- Bayesian photometric redshift estimation
- The Structure and Kinematics of the Circum-Galactic Medium from Far-UV Spectra of z~2-3 Galaxies
- An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
- zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
- The Hubble Ultra Deep Field
- The MUSE second-generation VLT instrument
- Passively Evolving Early-type Galaxies at 1.4<z<2.5 in the Hubble Ultra Deep Field
- The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts
- The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for galaxies
- 3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope
- A new photometric technique for the joint selection of star-forming and passive galaxies at 1.4<z<2.5
- The Chandra Deep Field South: Optical Spectroscopy I
- CANDELS Multi-wavelength Catalogs: Source Detection and Photometry in the GOODS-South Field
- Galaxies in the Hubble Ultra Deep Field: I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology
- Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies: - I. New constraints on cosmic reionisation from the luminosity and redshift-dependent fraction of Lyman-alpha emission
- Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
- The Evolutionary History of Lyman Break Galaxies Between Redshift 4 and 6: Observing Successive Generations of Massive Galaxies in Formation
- The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6
- The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection
- The Great Observatories Origins Deep Survey. VLT/FORS2 Spectroscopy in the GOODS-South Field: Part III
- The VIMOS VLT Deep Survey: Public release of 1599 redshifts to IAB<=24 across the Chandra Deep Field South
- Extended Lyman alpha haloes around individual high-redshift galaxies revealed by MUSE
- The Great Observatories Origins Deep Survey - VLT/VIMOS Spectroscopy in the GOODS-South Field: Part II
- The Great Observatories Origins Deep Survey. VLT/VIMOS Spectroscopy in the GOODS-South Field
- ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description
- The MUSE 3D view of the Hubble Deep Field South
- Galaxies with Wolf-Rayet signatures in the low-redshift Universe - A survey using the Sloan Digital Sky Survey
- The K20 survey. VII. The spectroscopic catalogue: spectral properties and evolution of the galaxy population
- A Census of Optical and Near-Infrared Selected Star-Forming and Passively Evolving Galaxies at Redshift Z~2
- The Great Observatories Origins Deep Survey VLT/FORS2 Spectroscopy in the GOODS-South Field: Part II
- The Great Observatories Origins Deep Survey - VLT/FORS2 Spectroscopy in the GOODS-South Field
- Spectroscopic Observations of Lyman-Break Galaxies at Redshift ~ 4, 5 and 6 in the GOODS-South Field
- UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field
- The Space Density and Colors of Massive Galaxies at 2<z<3: the Predominance of Distant Red Galaxies
- Noise Based Detection and Segmentation of Nebulous Objects
- Redshift distributions of galaxies in the DES Science Verification shear catalogue and implications for weak lensing
- Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors
- The Population of Weak MgII Absorbers. II The Properties of Single-Cloud Systems
- MARZ: Manual and Automatic Redshifting Software
- Gas Motion Study of Lya Emitters at z~2 Using UV and Optical Spectral Lines
- The VIMOS Ultra Deep Survey First Data Release: spectra and spectroscopic redshifts of 698 objects up to z~6 in CANDELS
- GMASS ultradeep spectroscopy of galaxies at z~2 - VII. Sample selection and spectroscopy
- A young star-forming galaxy at z = 3.5 with an extended Ly\, halo seen with MUSE
- 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
- UVUDF: Ultraviolet Imaging of the Hubble Ultradeep Field with Wide-field Camera 3
- UV-dropout Galaxies in the GOODS-South Field from WFC3 Early Release Science Observations
- The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6
- The MUSE Hubble Ultra Deep Field Survey X. Ly Equivalent Widths at
- A WFC3 Grism Emission Line Redshift Catalog in the GOODS-South Field
- On the realistic validation of photometric redshifts, or why Teddy will never be Happy
- The MUSE Hubble Ultra Deep Field Survey: IV. Global properties of C III] emitters
- A large population of galaxies 9 to 12 billion years back in the history of the Universe
- The MUSE Hubble Ultra Deep Field Survey: VII. FeII* Emission in Star-Forming Galaxies
- The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude
- Emission-Line Galaxies from the PEARS Hubble Ultra Deep Field: A 2-D Detection Method and First Results
Cited by in corpus (132)
- New Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency
- The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection
- Near infrared spectroscopy and star-formation histories of 3<z<4 quiescent galaxies
- JADES NIRSpec Initial Data Release for the Hubble Ultra Deep Field: Redshifts and Line Fluxes of Distant Galaxies from the Deepest JWST Cycle 1 NIRSpec Multi-Object Spectroscopy
- JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results
- The ALMA Spectroscopic Survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history
- Nearly all the sky is covered by Lyman-alpha emission around high redshift galaxies
- An Atlas of MUSE Observations towards Twelve Massive Lensing Clusters
- Red & Dead CANDELS: massive passive galaxies at the dawn of the Universe
- The GREATS H+[OIII] Luminosity Function and Galaxy Properties at : Walking the Way of JWST
- The MUSE-Wide Survey: Survey Description and First Data Release
- The MUSE Hubble Ultra Deep Field surveys: Data release II
- The ALMA Spectroscopic Survey in the HUDF: Multi-band constraints on line luminosity functions and the cosmic density of molecular gas
- 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
- The MUSE Hubble Ultra Deep Field Survey XI. Constraining the low-mass end of the stellar mass - star formation rate relation at
- GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
- The MUSE Hubble Ultra Deep Field Survey XIII. Spatially resolved spectral properties of Lyman alpha haloes around star-forming galaxies at z > 3
- The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the molecular gas in CO-selected galaxies
- The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6
- The MUSE Hubble Ultra Deep Field Survey X. Ly Equivalent Widths at
- The MUSE Deep Lensed Field on the Hubble Frontier Field MACS~J0416
- The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift
- The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
- Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters
- First gas-phase metallicity gradients of galaxies with MUSE
- The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to
- A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). III. A Large Sample of ALMA Sources in the GOODS-S
- The MUSE-Wide Survey: A determination of the Lyman emitter luminosity function at
- MUSEQuBES: Calibrating the redshifts of Ly α emitters using stacked circumgalactic medium absorption profiles
- The ionising photon production efficiency at z~6 for Lyman-alpha emitters using JEMS and MUSE
- The mean H EW and Lyman-continuum photon production efficiency for faint galaxies
- The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The nature of the faintest dusty star-forming galaxies
- The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
- Probing 3D Structure with a Large MUSE Mosaic: Extending the Mass Model of Frontier Field Abell 370
- Exploring HeII1640 emission line properties at
- New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
- Candidate Population III stellar complex at z=6.629 in the MUSE Deep Lensed Field
- No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at
- The MUSE Hubble Ultra Deep Field Survey: IV. Global properties of C III] emitters
- HOLISMOKES. VI. New galaxy-scale strong lens candidates from the HSC-SSP imaging survey
- The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at with JWST/NIRCam in GOODS-S
- Investigating the Effect of Galaxy Interactions on AGN Enhancement at
- Simulating the diversity of shapes of the Lyman- line
- High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
- HOLISMOKES. VIII. High-redshift, strong-lens search in the Hyper Suprime-Cam Subaru Strategic Program
- AstroSat detection of Lyman continuum emission from a z=1.42 galaxy
- The web of the Giant: spectroscopic confirmation of a Large Scale Structure around the z=6.31 quasar SDSS J1030+0524
- Cosmology with dropout selection: Straw-man surveys and CMB lensing
- Spectral shapes of the Lyman-alpha emission from galaxies: I. blueshifted emission and intrinsic invariance with redshift
- The emergence of passive galaxies in the early Universe
- Ionised gas structure of 100 kpc in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7
- The MUSE Hubble Ultra Deep Field Survey: XII. MgII emission and absorption in star-forming galaxies
- Equivalent widths of Lyman emitters in MUSE-Wide and MUSE-Deep
- MUSE Spectroscopic Identifications of Ultra-Faint Emission Line Galaxies with M -15
- ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields
- Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South
- HOLISMOKES -- IV. Efficient mass modeling of strong lenses through deep learning
- MUSEQuBES: Characterizing the circumgalactic medium of redshift Ly emitters
- The [OIII] equivalent width distribution at z : The redshift evolution of the extreme emission line galaxies
- The MUSE Hubble Ultra Deep Field Survey: VII. FeII* Emission in Star-Forming Galaxies
- Investigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0
- Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at z=1.7: star formation promoted by large-scale AGN feedback?
- The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
- The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
- The ALMA Spectroscopic Survey in the HUDF: A model to explain observed 1.1 and 0.85 millimeter dust continuum number counts
- The MUSE eXtremely Deep Field: Individual detections of Lyα haloes around rest-frame UV-selected galaxies at z~2.9-4.4
- The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
- The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude
- A Triple Rollover: A third multiply-imaged source at z~6 behind the Jackpot gravitational lens
- The MUSE Extremely Deep Field: a first panoramic view of an Mg II emitting intragroup medium
- An Hα Impression of Lyα Galaxies at with Deep JWST/NIRCam Imaging
- Early Results from GLASS-JWST XXII: Rest frame UV-optical spectral properties of Lyman-alpha emitting galaxies at 3 z 6
- ORIGIN: Blind detection of faint emission line galaxies in MUSE datacubes
- Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at
- The UV 2175Å Attenuation Bump and its Correlation with PAH Emission at z~2
- Reconstructing the observed ionizing photon production efficiency at z~2 using stellar population models
- Pilot-WINGS: An extended MUSE view of the structure of Abell 370
- Properties and redshift evolution of star-forming galaxies with high [OIII]/[OII] ratios with MUSE at 0.28<z<0.85
- Probing the AGN Unification Model at redshift z 3 with MUSE observations of giant Ly nebulae
- The ALMA Spectroscopic Survey in the HUDF: A Search for [CII] Emitters at
- Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at
- Fluctuation of the background sky in the Hubble Extremely Deep Field (XDF) and its origin
- A MUSE view of the massive merging galaxy cluster ACT-CL J0102-4915 (El Gordo) at z = 0.87: robust strong lensing model and data release
- The Ionised- and Cool-Gas Content of The BR1202-0725 System as seen by MUSE and ALMA
- Simulating JWST/NIRCam Color Selection of High-Redshift Galaxies
- AGN X-ray luminosity function and absorption function in the Early Universe ()
- COOL-LAMPS I. An Extraordinarily Bright Lensed Galaxy at Redshift 5.04
- A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). V. Deep 450 Micron Imaging
- The ALMA Spectroscopic Survey in the HUDF: Constraining cumulative CO emission at with power spectrum analysis of ASPECS LP data from 84 to 115 GHz
- The Tully-Fisher relation in dense groups at in the MAGIC survey
- HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
- Measuring the average molecular gas content of star-forming galaxies at
- The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
- A bottom-up search for Lyman-continuum leakage in the Hubble Ultra Deep Field
- Clustering dependence on Lyman- luminosity from MUSE surveys at
- Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
- A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). IV. The Submillimeter Properties of X-ray Sources in the CDF-S
- Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
- Conditions for direct black hole seed collapse near a radio-loud quasar 1 Gyr after the Big Bang
- The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman- emitters at
- Colour jumps across the spiral arms of Hubble Ultra Deep Field galaxies
- Physical properties of the CDFS X-ray sources through fitting spectral energy distributions
- HOLISMOKES -- XI. Evaluation of supervised neural networks for strong-lens searches in ground-based imaging surveys
- MUSE observations towards the lensing cluster A2744: Intersection between the LBG and LAE populations at z 3-7
- Three Dimensional Optimal Spectral Extraction (TDOSE) from Integral Field Spectroscopy
- The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at with CO stacking of MUSE detected Galaxies
- Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
- ALMA 26 arcmin survey of GOODS-S at one-millimeter (ASAGAO): millimeter properties of stellar mass selected galaxies
- MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
- Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
- New JWST redshifts for the host galaxies of CDF-S XT1 and XT2: understanding their nature
- A Catalog of Emission-Line Galaxies from the Faint Infrared Grism Survey: Studying Environmental Influence on Star Formation
- Tomography of the environment of the COSMOS/AzTEC-3 submillimeter galaxy at z=5.3 revealed by Lyalpha and MUSE observations
- HOLISMOKES XIII: Strong-lens candidates at all mass scales and their environments from the Hyper-Suprime Cam and deep learning
- Discovery of a Very Large (~20 kpc) Galaxy at z=3.72
- A galactic outflow traced by its extended Mg II emission out to a kpc radius in the Hubble Ultra Deep Field with MUSE
- Multi-wavelength Selected Compton-thick AGNs in Chandra Deep Field-South Survey
- Candidate z ~ 2.5 Lyman Continuum Sources in the GOODS Fields
- The MUSE Extremely Deep Field: Classifying the Spectral Shapes of Lya Emitting Galaxies
- 2mm Observations and the Search for High-Redshift Dusty Star-forming Galaxies
- The Lyman-alpha and Continuum Origins Survey II: the connection between the escape of ionizing radiation and Lyman-alpha halos in star-forming galaxies
- The Dwarf Galaxy Population at : A Catalog of Emission Lines and Redshifts from Deep Keck Observations
- Revisiting the Emission Line Source Detection Problem in Integral Field Spectroscopic Data
- A newly identified galaxy group thanks to tidal streams of intragroup light
- CLASH-VLT: Galaxy cluster MACS J0329-0211 and its surroundings using galaxies as kinematic tracers
- Extreme Neutral Outflow in a non-AGN Quiescent Galaxy at z~1.3
- HOLISMOKES XV. Search for strong gravitational lenses combining ground-based and space-based imaging
- The Intrinsic Distribution of Lyman- Halos
- HOLISMOKES XVI: Lens search in HSC-PDR3 with a neural network committee and post-processing for false-positive removal
- Extreme Emission-Line Galaxies in the MUSE Hubble Ultra Deep Field Survey
- On the ages of the stellar populations of galaxies at -7
- Accurate spectroscopic redshift estimation using non-negative matrix factorization: application to MUSE spectra