Clustering of Local Group distances: publication bias or correlated measurements? II. M31 and beyond

Abstract

The accuracy of extragalactic distance measurements ultimately depends on robust, high-precision determinations of the distances to the galaxies in the local volume. Following our detailed study addressing possible publication bias in the published distance determinations to the Large Magellanic Cloud (LMC), here we extend our distance range of interest to include published distance moduli to M31 and M33, as well as to a number of their well-known dwarf galaxy companions. We aim at reaching consensus on the best, most homogeneous, and internally most consistent set of Local Group distance moduli to adopt for future, more general use based on the largest set of distance determinations to individual Local Group galaxies available to date. Based on a careful, statistically weighted combination of the main stellar population tracers (Cepheids, RR Lyrae variables, and the magnitude of the tip of the red-giant branch), we derive a recommended distance modulus to M31 of $(m-M{)}_0^{M31}=24.46\pm 0.10$ mag---adopting as our calibration an LMC distance modulus of $(m-M{)}_0^{\mathrm{LMC}}=18.50$ mag---and a fully internally consistent set of benchmark distances to key galaxies in the local volume, enabling us to establish a robust and unbiased, near-field extragalactic distance ladder.

arXiv commentAJ, in press; 32 pages in AASTeX preprint format, 6 postscript figures. For online database, see http://astro-expat.info/Data/pubbias.html

References in corpus (75)

• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Dwarf Galaxies of the Local Group
• The observed properties of dwarf galaxies in and around the Local Group
• The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances
• An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent
• A 4% Geometric Distance to the Galaxy NGC4258 from Orbital Motions in a Nuclear Gas Disk
• Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant
• Our Peculiar Motion Away from the Local Void
• The Panchromatic Hubble Andromeda Treasury
• Tip of the Red Giant Branch Distances. II. Zero-Point Calibration
• Palomar/Las Campanas Imaging Atlas of Blue Compact Dwarf galaxies: I. Images and integrated photometry
• The HST Key Project on the Extragalactic Distance Scale XXVI. The Calibration of Population II Secondary Distance Indicators and the Value of the Hubble Constant
• A 15.65 solar mass black hole in an eclipsing binary in the nearby spiral galaxy Messier 33
• The Effect of Metallicity on Cepheid-Based Distances
• Clustering of Local Group distances: publication bias or correlated measurements? I. The Large Magellanic Cloud
• Cepheid Distances to SNe Ia Host Galaxies based on a Revised Photometric Zero-Point of the HST-WFPC2 and New P-L Relations and Metallicity Corrections
• A Bayesian Approach to Locating the Red Giant Branch Tip Magnitude (Part II); Distances to the Satellites of M31
• Photometry and the Metallicity Distribution of the Outer Halo of M31
• Insights into the Cepheid distance scale
• The Geometric Distance and Proper Motion of the Triangulum Galaxy (M33)
• The calibration of the RGB Tip as a Standard Candle: Extension to Near Infrared colors and higher metallicity
• The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33
• First Determination of the Distance and Fundamental Properties of an Eclipsing Binary in The Andromeda Galaxy
• The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789
• The "Tip" of the Red Giant Branch as a distance indicator: results from evolutionary models
• Cepheid Period-Luminosity Relations in the Near-Infrared and the Distance to M31 from the Hubble Space Telescope Wide Field Camera 3
• The Megamaser Cosmology Project: I. VLBI observations of UGC 3789
• A Problem with the Clustering of Recent Measures of the Distance to the Large Magellanic Cloud
• The Planetary Nebula System of M33
• A new analysis of the Red Giant Branch "Tip" distance scale and the value of the Hubble constant
• The VMC Survey IV. The LMC star formation history and disk geometry from four VMC tiles
• The distance to the Andromeda Galaxy from eclipsing binaries
• Deep HST Imaging of IC 1613. I. Variable Stars and Distance
• ACS photometry of extended, luminous globular clusters in the outskirts of M31
• On the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations
• HST/WFPC2 Color-Magnitude Diagrams for Globular Clusters in M31
• The Abundance Scatter in M33 from HII Regions: Is There Any Evidence for Azimuthal Metallicity Variations?
• The Megamaser Cosmology Project. V. An Angular Diameter Distance to NGC 6264 at 140 Mpc
• Sharpening the Tip of the Red Giant Branch
• The Megamaser Cosmology Project. II. The Angular-Diameter Distance to UGC 3789
• The VMC Survey. V. First results for Classical Cepheids
• The Large Magellanic Cloud and the Distance Scale
• A New Distance to M33 Using Blue Supergiants and the FGLR Method
• The DIRECT Project: Influence of Blending on the Cepheid Distance Scale. I. Cepheids in M31
• Determination of the Distance to M33 Based on the Tip of the Red Giant Branch and the Red Clump
• Halos of Spiral Galaxies. I. The Tip of the Red Giant Branch as a Distance Indicator
• Deep HST Imaging of Sextans A. II. Cepheids and Distance
• Cepheid and Tip of the Red Giant Branch Distances To the Dwarf Irregular Galaxy IC10
• Spectroscopy of two PN candidates in IC10
• On the stellar populations in NGC 185 and NGC 205, and the nuclear star cluster in NGC 205 from Hubble Space Telescope observations
• Metallicity-corrected Tip of the Red Giant Branch Distance to NGC 4258
• IC 10: More evidence that it is a blue compact dwarf
• The expansion field: The value of H_0
• The Star Formation History in The Far Outer Disc of M33
• The Araucaria Project. A Distance Determination to the Local Group Spiral M33 from Near-Infrared Photometry of Cepheid Variables
• The Tip of the Red Giant Branch Distance to the Large Magellanic Cloud
• The Local Group Census: planetary nebulae in IC 10, Leo A and Sextans A
• HST observations of the LMC field around SN87A: distance determinations with Red Clump and Tip of the Red Giant Branch stars
• RR Lyrae Variables in Two Fields in the Spheroid of M31
• Eclipsing binaries suitable for distance determination in the Andromeda galaxy
• On the distance and reddening of the starburst galaxy IC10
• A comprehensive study of Cepheid variables in the Andromeda galaxy. Period distribution, blending and distance determination
• Imaging of the Stellar Population of IC10 with Laser Guide Star Adaptive Optics and the Hubble Space Telescope
• RR Lyrae variables in M32 and the disk of M31
• Calibration of the distance scale from galactic Cepheids:II Use of the HIPPARCOS calibration
• The Deepest HST Color-Magnitude Diagram of M32: Evidence for Intermediate-Age Populations
• The Carnegie Hubble Program: The Infrared Leavitt Law in IC 1613
• Reddening and Distance of the Local Group Starburst Galaxy IC 10
• HST/ACS colour-magnitude diagrams of M31 globular clusters
• Calibration of the distance scale from galactic Cepheids: I Calibration based on the GFG sample
• Long-period variables in NGC147 and NGC185
• Nearby Galaxies in the 2micron All Sky Survey I. K-band Luminosity Functions
• The Variable Star Population of the Globular Cluster B514 in the Andromeda Galaxy
• The IC133 Water Vapor Maser in the Galaxy M33: A Geometric Distance
• A kinematic study of planetary nebulae in the dwarf irregular galaxy IC10

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• Clustering of Local Group distances: publication bias or correlated measurements? I. The Large Magellanic Cloud
• Clustering of Local Group distances: publication bias or correlated measurements? III. The Small Magellanic Cloud
• Old-Aged Stellar Population Distance Indicators
• The Hubble Space Telescope Survey of M31 Satellite Galaxies I. RR Lyrae-based Distances and Refined 3D Geometric Structure
• Redshift-Independent Distances in the NASA/IPAC Extragalactic Database: Methodology, Content and Use of NED-D
• Standard Galactic Field RR Lyrae II: A Gaia DR2 calibration of the period-Wesenheit-metallicity relation
• Large Magellanic Cloud Near-Infrared Synoptic Survey. II. The Wesenheit relations and their application to the Distance scale
• Clustering of Local Group distances: publication bias or correlated measurements? IV. The Galactic Center
• The VMC Survey -- XXXIV. Morphology of Stellar Populations in the Magellanic Clouds
• A sub-2% Distance to M31 from Photometrically Homogeneous Near-Infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
• Toward an internally consistent astronomical distance scale
• Stellar substructures in the periphery of the Magellanic Clouds with the VISTA Hemisphere Survey from the red clump and other tracers
• A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude - Rate of Decline Relation for Novae as a Non-Standard Candle, and a Prediction of the Existence of Ultrafast Novae
• Constraining the pitch angle of the Galactic spiral arms in the Milky Way
• The Star Formation History in the M31 Bulge
• The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). III. The Mass Function of Young Star Clusters in M33
• Clustering of Local Group distances: publication bias or correlated measurements? V. Galactic rotation constants
• The TREX Survey: Kinematical Complexity Throughout M33's Stellar Disk and Evidence for a Stellar Halo
• Panchromatic Hubble Andromeda Treasury XIII: The Cepheid period-luminosity relation in M31
• Impact of distance determinations on Galactic structure. I. Young and intermediate-age tracers
• A spectroscopic study of blue supergiant stars in Local Group spiral galaxies: Andromeda and Triangulum
• The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). IV. Star Cluster Catalog
• Evidence for non-axisymmetry in M31 from wide-field kinematics of stars and gas
• Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for Type II Cepheids
• The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
• The potential role of NGC 205 in generating Andromeda's vast thin co-rotating plane of satellite galaxies
• Constrained cosmological simulations of the Local Group using Bayesian hierarchical field-level inference
• Solo dwarfs IV: Comparing and contrasting satellite and isolated dwarf galaxies in the Local Group
• Multiwavelength Characterization of the High Mass X-ray Binary Population of M33
• The HASHTAG project I. A Survey of CO(3-2) Emission from the Star Forming Disc of M31
• Non-Gaussian Error Distributions of Galactic Rotation Speed Measurements
• A Distance Measurement to M33 Using Optical Photometry of Mira Variables
• Massive young stellar objects in the Local Group spiral galaxy M33 identified using machine learning
• VI-Band Follow-Up Observations of Ultra-Long-Period Cepheid Candidates in M31
• New insights into the use of Ultra Long Period Cepheids as cosmological standard candles
• Clustering of Local Group distances: publication bias or correlated measurements? VI. Extending to Virgo cluster distances
• Towards Machine-assisted Meta-Studies: The Hubble Constant
• Clustering of Local Group distances: publication bias or correlated measurements? VII. A distance framework out to 100 Mpc
• A Differential RR Lyrae Line-of-Sight Distance Between M31 and M33
• The Accretion Mode in Sub-Eddington Supermassive Black Holes: Getting into the Central Parsecs of Andromeda
• The HASHTAG project: The First Submillimeter Images of the Andromeda Galaxy from the Ground
• Zwicky Transient Facility and Globular Clusters: the gr-Band Period-Luminosity Relations for Mira Variables at Maximum Light and Their Applications to Local Galaxies
• Period-Luminosity Relations for Galactic Type II Cepheids in the Sloan bands
• The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) II. The Spatially Resolved Recent Star Formation History of M33