The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection

Abstract

We present the MUSE Hubble Ultra Deep Survey, a mosaic of nine MUSE fields covering 90\% of the entire HUDF region with a 10-hour deep exposure time, plus a deeper 31-hour exposure in a single 1.15 arcmin2 field. The improved observing strategy and advanced data reduction results in datacubes with sub-arcsecond spatial resolution (0.65 arcsec at 7000 A) and accurate astrometry (0.07 arcsec rms). We compare the broadband photometric properties of the datacubes to HST photometry, finding a good agreement in zeropoint up to mAB=28 but with an increasing scatter for faint objects. We have investigated the noise properties and developed an empirical way to account for the impact of the correlation introduced by the 3D drizzle interpolation. The achieved 3 sigma emission line detection limit for a point source is 1.5 and 3.1 10-19 erg.s-1.cm-2 for the single ultra-deep datacube and the mosaic, respectively. We extracted 6288 sources using an optimal extraction scheme that takes the published HST source locations as prior. In parallel, we performed a blind search of emission line galaxies using an original method based on advanced test statistics and filter matching. The blind search results in 1251 emission line galaxy candidates in the mosaic and 306 in the ultradeep datacube, including 72 sources without HST counterparts (mAB>31). In addition 88 sources missed in the HST catalog but with clear HST counterparts were identified. This data set is the deepest spectroscopic survey ever performed. In just over 100 hours of integration time, it provides nearly an order of magnitude more spectroscopic redshifts compared to the data that has been accumulated on the UDF over the past decade. The depth and high quality of these datacubes enables new and detailed studies of the physical properties of the galaxy population and their environments over a large redshift range.

arXiv comment21 pages

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• AutoSpec: Fast Automated Spectral Extraction Software for IFU Datacubes
• GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties
• First resolved stellar halo kinematics of a MW-mass galaxy outside the Local Group: A flat counter-rotating halo in NGC 4945
• Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster IV. A study of the Globular Cluster population in four UDGs
• Discovery of faint double-peak Halpha emission in the halo of low redshift galaxies
• The contribution of faint Lyman-$\alpha$ emitters to extended Lyman-$\alpha$ halos constrained by MUSE clustering measurements
• Relatively young thick disks in star-forming late-type galaxies
• Recovering the pattern speeds of edge-on barred galaxies via an orbit-superposition method
• VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z\sim 0.15$ traced with VLT/MUSE
• The Intrinsic Distribution of Lyman-$\alpha$ Halos
• Extreme Emission-Line Galaxies in the MUSE Hubble Ultra Deep Field Survey
• HeII emitters at cosmic noon and beyond. Characterising the HeII λ1640 emission with MUSE and JWST/NIRSpec
• Resolving stellar populations with integral field spectroscopy
• Classifying spectra of emission-line regions with neural networks -- An application to integral field spectroscopic data of M33
• Stellar angular momentum of disk galaxies at z = 0.7 in the MAGIC survey I. Impact of the environment
• Stellar Dynamical Modeling - Accuracy of 3D Density Estimation for Edge-on Axisymmetric Galaxies
• Galaxy mass dependence of metal-enrichment of nuclear star clusters
• Temperature based radial metallicity gradients in nearby galaxies
• A spectroscopic study of 14 structures behind Holm15A: Detecting a galaxy group candidate at z=0.58
• MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
• MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of $z\sim 1$ star-forming galaxies
• Far-ultraviolet investigation into the galactic globular cluster M30 (NGC 7099): II. Potential X-ray counterparts and variable sources
• MUSE Study of Two Giant Low-surface-brightness Galaxies with Compact Satellites
• Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies
• A deep ALMA Band 3 survey of HDFS/MUSE3D: Survey description and initial results
• SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis
• Resolving circumgalactic gas flows around a z$\approx$3.6 quasar using MUSE and ALMA
• Andromeda's tenuous veil: A likely Milky Way nebula projected toward M31
• PHANGS-MUSE: the HII region luminosity function of local star-forming galaxies
• Cross-checking SMBH mass estimates in NGC 6958 -- I: Stellar dynamics from adaptive optics-assisted MUSE observations
• Nebular abundance gradient in the Cartwheel galaxy using MUSE data
• Updated bounds on Axion-Like Particle Dark Matter with the optical MUSE-Faint survey
• TOPz: Photometric redshifts using template fitting applied to the GAMA survey
• GA-NIFS: AGN activity in a Lyα emitter within a triple-AGN system anchored by a passive galaxy at z=3
• First statistical constraints on galactic scale outflows properties traced by their extended Mg II emission with MUSE
• Accurate spectroscopic redshift estimation using non-negative matrix factorization: application to MUSE spectra
• Gravitational Torques from a Lopsided Young Stellar Component Sustain High Black Hole Accretion Rates in NGC 4593