Linking halo mass to galaxy luminosity

Abstract

In this paper we present a new, essentially empirical, model for the relation between the mass of a dark matter halo/subhalo and the luminosity of a galaxy hosted in it. To estimate this, we replace the assumption of linearity between light and mass fluctuations with the assumption of monotonicity between galaxy light and halo or subhalo mass. We are enabled to proceed with this less restrictive ansatz by the availability of new, very high resolution dark matter simulations and more detailed and comprehensive global galactic luminosity functions. We find that the relation between halo/subhalo mass and hosted galaxy luminosity is fairly well fit by a double power law, while that between halo mass and group luminosity is fairly well fit by a two branch function, with both branches double power laws. Both relations asymptote to $L\propto M^4$ at low $M$, while at high mass the former follows $L\propto M^{0.28}$ and the latter $L\propto M^{0.9}$. We also derive results for the occupation number, luminosity function of cluster galaxies, group luminosity function and multiplicity function. Then, using some additional assumptions, we further derive results for biasing between mass and light and mass and galaxy number, light distribution function and the void probability distribution. Our results for the most part seem to match well with observations and previous expectations. We feel this is a potentially powerful way of modelling this relation, since the main inputs are readily testable against dark matter simulation results and galaxy surveys. (abridged)

13 pages, 11 figures; some modifications to match version accepted by MNRAS

References in corpus (2)

• Voids in the 2dF Galaxy Redshift Survey
• The Dependence of the Galaxy Luminosity Function on Large-Scale Environment

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• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Tracing stars in Milky Way satellites with A-SLOTH
• Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• Quasi-equilibrium models of high-redshift disc galaxy evolution
• Tracing the Nature of Dark Energy with Galaxy Distribution
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• Effects of galaxy-halo alignment and adiabatic contraction on gravitational lens statistics
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• A Steep Slope and Small Scatter for the High-Mass End of the L-$\sigma$ Relation at $z\sim 0.55$
• How do galaxies populate halos in extreme density environments? An analysis of the Halo Occupation Distribution in SDSS
• Using member galaxy luminosities as halo mass proxies of galaxy groups
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Constraints on the Evolution of the Galaxy Stellar Mass Function I: Role of Star Formation, Mergers and Stellar Stripping
• Modeling Redshift-Space Clustering with Abundance Matching
• The Cosmic History of Hot Gas Cooling and Radio AGN Activity in Massive Early-Type Galaxies
• Analytical halo model of galactic conformity
• The Cosmic Web Around The Brightest Galaxies During The Epoch Of Reionization
• Topology of Luminous Red Galaxies from the Sloan Digital Sky Survey
• Robustness of the covariance matrix for galaxy clustering measurements
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• Galaxy clustering at cosmic dawn from JWST/NIRCam observations to redshift z$\sim$11
• Cosmic Flow Measurement and Mock Sampling Algorithm of Cosmicflows-4 Tully-Fisher Catalogue
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Ionization bias and the ghost proximity effect near $z\gtrsim 6$ quasars in the shadow of proximate absorption systems
• Rosella: A mock catalogue from the P-Millennium simulation
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• A Direct Measurement of the High-Mass End of the Velocity Dispersion Function at $z\sim 0.55$ from SDSS-III/BOSS
• Modeling Reionization in a Bursty Universe
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• A minimal empirical model for the cosmic far-infrared background anisotropies
• Biased tracer reconstruction with halo mass information
• Constraining Dark Energy With Stacked Concave Lenses
• The Rise of Dwarfs and the Fall of Giants: Galaxy Formation Feedback Signatures in the Halo Satellite Luminosity Function
• Testing galaxy formation models with galaxy stellar mass functions
• Reionization and feedback in overdense regions at high redshift
• Galaxy clustering measurements out to redshift z$\sim$8 from Hubble Legacy Fields
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Observational challenges in Ly-alpha intensity mapping
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• The Roles of Mass and Environment in the Quenching of Galaxies
• The Velocity Dispersion Function for Quiescent Galaxies in Nine Strong-Lensing Clusters
• Evolution of CIV Absorbers. II. Where does CIV live?
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Dust in High-Redshift Galaxies: Reconciling UV Attenuation and IR Emission
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Impact of tidal environment on galaxy clustering in GAMA
• Abundance matching for low mass galaxies in the CDM and FDM models
• Rapid Simulations of Halo and Subhalo Clustering
• Revealing the Galaxy-Halo Connection Through Machine Learning
• Relating galaxies across different redshift to study galaxy evolution
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• The Circumgalactic Medium in Massive Halos
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• On the weak lensing masses of a new sample of galaxy groups
• A Two-Parameter Matching Scheme for Massive Galaxies and Dark Matter Haloes
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Recovering the Tidal Field in the Projected Galaxy Distribution
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• BreakBRD Galaxies I: Global Properties of Spiral Galaxies with Central Star Formation in Red Disks
• The matter distribution in z ~ 0.5 redshift clusters of galaxies. II : The link between dark and visible matter
• On merger bias and the clustering of quasars
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• Constraining galaxy-halo connection with high-order statistics
• The Dark Matter Halos of HI Selected Galaxies
• Is There a Universal Mass Function?
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Lyman alpha Properties of Simulated Galaxies in Overdense Regions: Effects of Galactic Winds at z > 6
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Multi-wavelength consensus of large-scale linear bias
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• DarkAI: Reconstructing the density, velocity and tidal field of dark matter from a DESI-like bright galaxy sample
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Constraints on the Evolution of the Galaxy Stellar Mass Function II: Quenching Timescale of Galaxies and its Implication for their Star Formation Rate
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• Galaxy-galaxy lensing in the VOICE deep survey
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Clustering properties and halo masses for central galaxies in the local Universe
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• Impact of the turnover in the high-z galaxy luminosity function on the 21-cm signal during Cosmic Dawn and Epoch of Reionization
• Probing Satellite Halos with Weak Gravitational Lensing
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Constraining galaxy properties with complete samples of lenses
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• The invariance of group occupation across the cosmic web
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• Euclid: Improving redshift distribution reconstruction using a deep-to-wide transfer function
• Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
• Testing subhalo abundance matching with galaxy kinematics
• Luminosity Function of Galaxies in Voids: A Modification Inspired by Excursion Set Theory
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• 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