MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of $z\sim 1$ star-forming galaxies

Abstract

In a series of papers on lensed kinematics, we seek to combine the sensitivity of 3D forward modelling to low signal-to-noise ratio outskirts with the enhanced spatial resolution of cluster lensing. In this first paper, we (i) present and validate our methodology, which directly constrains the source parameters by incorporating lensing deflections into the ${\text{GalPaK}}^{\text{3D}}$ forward-modelling algorithm, and (ii) investigate the evolution of the stellar-mass and baryonic-mass Tully-Fisher relations (sTFR and bTFR) since $z\sim 1$. We define a robust sample of strongly lensed star-forming galaxies (SFGs) from the MUSE Lensing Cluster survey, spanning magnifications $\mu =1.4-12.4$ and stellar masses $M_{\star }=10^{8.1}-10^{10.3}{M}_{\odot }$. Using a series of mock galaxies, we find that our method is significantly more reliable at recovering morpho-kinematic properties than approaches that ignore differential magnification, even for relatively modest magnifications ($\mu <6$). Restricting the analysis to 95 rotationally supported SFGs with well-constrained velocities, we find a significant evolution of the sTFR zero-point ($\Delta b^{\mathrm{sTFR}}=-0.42_{-0.05}^{+0.05}\mathrm{dex}$ in stellar mass) but no detectable evolution of the bTFR zero-point ($\Delta b^{\mathrm{bTFR}}=0.00_{-0.06}^{+0.06}\mathrm{dex}$ in baryonic mass) relative to $z\approx 0$. Our results are consistent with a mild evolution of the stellar-to-halo mass ratio and support the view that the sTFR has evolved only weakly over the past $\sim 8$ Gyr, aside from shifts driven by the redshift dependence of halo-defining quantities such as the critical density and overdensity. The absence of detectable evolution in the bTFR zero-point suggests that the increasing contribution of cold gas mass at higher redshift fully compensates the evolution observed in the stellar component alone. [abridged]

21 pages, 12 figures, 4 tables. Accepted for publication in A&A

References in corpus (61)

• Array Programming with NumPy
• The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
• Cosmic Star Formation History
• 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$
• SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves
• The Radial Acceleration Relation in Rotationally Supported Galaxies
• A Bayesian approach to strong lensing modelling of galaxy clusters
• The Evolution of the Star-forming Interstellar Medium across Cosmic Time
• The Data Processing Pipeline for the MUSE Instrument
• The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection
• Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
• Star-Forming Galaxies at Cosmic Noon
• COSMOS2020: The Galaxy Stellar Mass Function: the assembly and star formation cessation of galaxies at $0.2<z\le 7.5$
• A dynamically cold disk galaxy in the early Universe
• The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
• Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100pc scales
• Dynamical properties of z $\sim 4.5$ dusty star-forming galaxies and their connection with local early type galaxies
• An Atlas of MUSE Observations towards Twelve Massive Lensing Clusters
• The Kinematics of z ~ 6 Quasar Host Galaxies
• Rotation Curves in z~1-2 Star-Forming Disks: Evidence for Cored Dark Matter Distributions
• The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies
• Extending the evolution of the stellar mass-size relation at $z\le 2$ to low stellar mass galaxies from HFF and CANDELS
• Fast rotating and low-turbulence discs at $z\simeq 4.5$: Dynamical evidence of their evolution into local early-type galaxies
• Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
• COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history
• Dynamically cold disks in the early Universe: myth or reality?
• MIGHTEE-HI: The baryonic Tully-Fisher relation over the last billion years
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• Kiloparsec view of a typical star-forming galaxy when the Universe was $\sim$1 Gyr old II. Regular rotating disk and evidence for baryon dominance on galactic scales
• Ultra-deep Ks-band Imaging of the Hubble Frontier Fields
• RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales
• First Results from the KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics of Lensed Galaxies at Cosmic Noon
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) : I. Characterisation of extended Lyman-alpha haloes and spatial offsets
• The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas
• Atomic Gas Scaling Relations of Star-forming Galaxies at $z\approx 1$
• Flat Rotation Curves of $z\sim 1$ Star-Forming Galaxies and Evidence of Disk-Scale Length Evolution
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• Self-consistent nonspherical isothermal halos embedding zero-thickness disks
• The dawn of disks: unveiling the turbulent ionised gas kinematics of the galaxy population at $z\sim 4-6$ with JWST/NIRCam grism spectroscopy
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• GLaD: Gravitational Lensing and Dynamics, combined analysis to unveil properties of high-redshift galaxies
• A ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259
• The redshift evolution of the baryonic Tully-Fisher relation in Simba
• The Tully-Fisher relation in dense groups at $z\sim 0.7$ in the MAGIC survey
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
• BUDHIES V: The baryonic Tully-Fisher relation at z=0.2 based on direct HI detections
• Photometric vs dynamical stellar masses and their impact on scaling relations in nearby disc galaxies
• The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
• The KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics and clumpiness of low-mass galaxies at cosmic noon
• LEGA-C: analysis of dynamical masses from ionized gas and stellar kinematics at z~0.8
• Tully-Fisher Relation of Late-type Galaxies at $0.6\le z\le 2.5$
• MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at $z>0.25$
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• MUSE-DARK-I: Dark matter halo properties of intermediate-z star-forming galaxies
• Kinematic scaling relations of disc galaxies from ionised gas at $z\sim 1$ and their connection with dark matter haloes
• PowerBin: Fast Adaptive Data Binning with Centroidal Power Diagrams
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference

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