The K-Band Galaxy Luminosity Function

Abstract

We measured the K-band luminosity function using a complete sample of 4192 morphologically-typed 2MASS galaxies with 7 < K < 11.25 mag spread over 2.12 str. Early-type (T < -0.5) and late-type (T > -0.5) galaxies have similarly shaped luminosity functions, alpha_e=-0.92+/-0.10 and alpha_l=-0.87+/-0.09. The early-type galaxies are brighter, M_*e=-23.53+/-0.06 mag compared to M_*l=-22.98\pm0.06 mag, but less numerous, n_*e=(0.0045+/-0.0006)h^3/Mpc^3 compared to n_*l=(0.0101+/-0.0013)h^3/Mpc^3 for H_0=100h km/s Mpc, such that the late-type galaxies slightly dominate the K-band luminosity density, j_late/j_early=1.17+/-0.12. Our morphological classifications are internally consistent, consistent with previous classifications and lead to luminosity functions unaffected by the estimated uncertainties in the classifications. These luminosity functions accurately predict the K-band number counts and redshift distributions for K < 18 mag, beyond which the results depend on galaxy evolution and merger histories.

submitted to ApJ, 25 pages, 6 figures, complete redshift survey. Table 1 included in source

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• PKS1932-46: a radio source in an interacting group?
• A Cross-correlation Analysis of AGN and Galaxies using Virtual Observatory: Dependence on Virial Mass of Super-Massive Black Hole
• UV and FIR selected star-forming galaxies at z=0: differences and overlaps
• Long-slit Spectroscopy of Edge-on Low Surface Brightness Galaxies
• K-band Imaging of strong CaII-absorber host galaxies at z~1
• AMI SZ observations and Bayesian analysis of a sample of six redshift-one clusters of galaxies
• Infrared luminosities of galaxies in the Local Volume
• On the Formation of cD Galaxies and their Parent Clusters
• Testing isotropy in the Two Micron All-Sky redshift survey with information entropy
• A Galaxy Merger Scenario for the NGC 1550 Galaxy from Metal Distributions in the X-ray Emitting Plasma
• Consequences of dark matter self-annihilation for galaxy formation
• The Star Formation and Nuclear Accretion Histories of Normal Galaxies in the AGES Survey
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Recovering the Tidal Field in the Projected Galaxy Distribution
• Discovery of Highly Obscured Galaxies in the Zone of Avoidance
• The Infrared Luminosity Function of AKARI 90$\mu$m Galaxies in the Local Universe
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Are z>2 Herschel galaxies proto-spheroids?
• The bivariate K-band-submillimetre luminosity functions of the local HRS galaxy sample
• Universe opacity and EBL
• Slit Observations and Empirical Calculations for HII Regions
• Number Density Evolution of Ks -band Selected High Redshift Galaxy Populations in the AKARI North Ecliptic Pole Field
• Discovery of Two Galaxies Deeply Embedded in the Great Attractor Wall
• Cosmological simulations of the high-redshift radio universe
• Multi-wavelength consensus of large-scale linear bias
• 2MASS Galaxies in the Fornax Cluster Spectroscopic Survey
• Central gas entropy excess as a direct evidence for AGN feedback in galaxy groups and clusters
• The Structure of 2MASS Galaxy Clusters
• Detailed Study of the Ursa Major Supercluster of Galaxies Using the 2MASS and SDSS Catalogs
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Galaxy luminosity function and its cosmological evolution: Testing a new feedback model depending on galaxy-scale dust opacity
• The 2 to 24 micron source counts from the AKARI North Ecliptic Pole survey
• EROs found behind lensing clusters. II. Stellar populations and dust properties of optical dropout EROs and comparison with related objects
• The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. I. Measurement Techniques
• The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. III. Measurement Results
• The Star Formation Reference Survey. IV. Stellar mass distribution of local star-forming galaxies
• Examining the Properties of Low-Luminosity Hosts of Type Ia Supernovae from ASAS-SN
• A near-infrared study of the obscured 3C129 galaxy cluster
• Infrared emission from dust and the spectral features of extragalactic gamma-ray sources
• CLUES to the past: Local Group progenitors amongst high-redshift Lyman Break Galaxies
• Detection of an ultra-bright submillimeter galaxy behind the Small Magellanic Cloud
• Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
• Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
• Thermodynamic evolution of the cosmological baryonic gas : II. Galaxy formation
• Fluctuations of K-band galaxy counts
• Faint Galaxy Number Counts in the Durhamand SDSS Catalogues
• NASIM: Revealing the low surface brightness Universe from legacy VISTA data
• The stellar and hot gas content of low-mass galaxy clusters
• The Luminosity of the Darkness: Schechter function in dark sirens
• Motion of the Local Group as a cosmological probe
• Halo detection via large-scale Bayesian inference
• The most massive galaxies with large depleted cores: structural parameter relations and black hole masses
• The host galaxies of flat-spectrum quasars