The Galaxy-Halo Connection Over The Last 13.3 Gyrs

Abstract

We present new determinations of the stellar-to-halo mass relation (SHMR) at $z=0-10$ that match the evolution of the galaxy stellar mass function, the SFR$-M_{\ast }$ relation,and the cosmic star formation rate. We utilize a compilation of 40 observational studies from the literature and correct them for potential biases. Using our robust determinations of halo mass assembly and the SHMR, we infer star formation histories, merger rates, and structural properties for average galaxies, combining star-forming and quenched galaxies. Our main findings: (1) The halo mass $M_{50}$ above which 50\% of galaxies are quenched coincides with sSFR/sMAR$\sim 1$, where sMAR is the specific halo mass accretion rate. (2) $M_{50}$ increases with redshift, presumably due to cold streams being more efficient at high redshift while virial shocks and AGN feedback become more relevant at lower redshifts. (3) The ratio sSFR/sMAR has a peak value, which occurs around $M_{\mathrm{vir}}\sim 2\times 10^{11}{M}_{\odot }$. (4) The stellar mass density within 1 kpc, ${\Sigma }_1$, is a good indicator of the galactic global sSFR. (5) Galaxies are statistically quenched after they reach a maximum in ${\Sigma }_1$, consistent with theoretical expectations of the gas compaction model; this maximum depends on redshift. (6) In-situ star formation is responsible for most galactic stellar mass growth, especially for lower-mass galaxies. (7) Galaxies grow inside out. The marked change in the slope of the size--mass relation when galaxies became quenched, from $d\log R_{\mathrm{eff}}/d\log M_{\ast }\sim 0.35$ to $\sim 2.5$, could be the result of dry minor mergers.

arXiv comment42 pages, 31 Figures. Accepted for publication in MNRAS. Typos corrected. The results presented in this paper are available via an interactive website: https://132.248.1.39/galaxy/galaxy_halo.html

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• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
• A Search for Satellite Galaxies of Nearby Star-Forming Galaxies with Resolved Stars in LBT-SONG
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• MUSE-ALMA Haloes VIII: Statistical Study of Circumgalactic Medium Gas
• The global and radial stellar mass assembly of Milky Way-sized galaxies
• Towards a higher mass for NGC1052-DF2: an analysis based on full distribution functions
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• Magnification Bias of Distant Galaxies in the Hubble Frontier Fields: Testing Wave vs. Particle Dark Matter Predictions
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Extending the Chemical Reach of the H3 Survey: Detailed Abundances of the Dwarf-galaxy Stellar Stream Wukong/LMS-1
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• The SLUGGS Survey: The Inner Dark Matter Density Slope of the Massive Elliptical Galaxy NGC 1407
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• Dark matter and no dark matter: On the halo mass of NGC 1052
• Phase spirals in cosmological simulations of Milky Way-size galaxies
• New empirical constraints on the cosmological evolution of gas and stars in galaxies
• ALMA [CII] 158um imaging of an HI-Selected Major Merger at z~4
• Hedgehog: An Isolated Quiescent Dwarf Galaxy at 2.4 Mpc
• Dynamics of Stellar Disk Tilting from Satellite Mergers
• A Unified Exploration of the Chronology of the Galaxy
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• MUSE-ALMA Halos XI: Gas flows in the circumgalactic medium
• Constraining Dark Energy With Stacked Concave Lenses
• Conditions for Clump Survival in High-z Disc Galaxies
• The Mass Growth and Stellar Ages of Galaxies: Observations versus Simulations
• The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
• The differences between mass- and light-derived structural parameters over time for MaNGA Elliptical galaxies
• Revealing the Galaxy-Halo Connection Through Machine Learning
• Abundance matching for low mass galaxies in the CDM and FDM models
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample
• DHOST gravity in Ultra-diffuse galaxies -- Part II: NGC 1052-DF4 and Dragonfly 44
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• The star-forming main sequence and the contribution of dust-obscured star formation since $z\sim 4$ from the FUV+IR luminosity functions
• Fast generation of mock galaxy catalogues with COLA
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Approximations to galaxy star formation rate histories: properties and uses of two examples
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Satellite galaxy abundance dependency on cosmology in Magneticum simulations
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• No Evolution in the Half-mass Radius of Milky Way-type Galaxies over the Last 10 Gyr
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Galaxy-galaxy lensing in the VOICE deep survey
• The size function of massive satellites from the $R_e-R_h$ and $M_{star}-M_h$ relations: constraining the role of environment
• Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since $z=2$
• Testing non-local gravity through Ultra-Diffuse Galaxies kinematics
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Spectral Evidence of Solar Neighborhood Analogs in CALIFA Galaxies
• Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals
• Hermeian haloes: extreme objects with two interactions in the past
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• Galaxy mass dependence of metal-enrichment of nuclear star clusters
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Zangetsu: A Candidate of Isolated, Quiescent, and Backsplash Ultra-Diffuse Galaxy in the COSMOS Field
• Observing galaxy mergers at the epoch of reionization
• Formation of galactic bulges from the cold gas filaments in high-redshift dark matter halos
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• SDSS-IV MaNGA: Stellar rotational support in disk galaxies vs. central surface density and stellar population age
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• A Search for Wandering Black Holes in the Milky Way with Gaia and DECaLS
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• DHOST gravity in Ultra-diffuse galaxies -- Part I: the case of NGC1052-DF2
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• A Salpeter IMF and an NFW halo: Disentangling the dark and stellar mass of an elliptical galaxy through precise lens modelling of a double-source-plane system