Analysis of Determinations of the Distance between the Sun and the Galactic Center
arXiv:1301.7011 · doi:10.1134/S1063772913020078
Abstract
The paper investigates the question of whether or not determinations of the distance between the Sun and the Galactic center R0 are affected by the so-called "bandwagon effect", leading to selection effects in published data that tend to be close to expected values, as was suggested by some authors. It is difficult to estimate numerically a systematic uncertainty in R0 due to the bandwagon effect; however, it is highly probable that, even if widely accepted values differ appreciably from the true value, the published results should eventually approach the true value despite the bandwagon effect. This should be manifest as a trend in the published R0 data: if this trend is statistically significant, the presence of the bandwagon effect can be suspected in the data. Fifty two determinations of R0 published over the last 20 years were analyzed. These data reveal no statistically significant trend, suggesting they are unlikely to involve any systematic uncertainty due to the bandwagon effect. At the same time, the published data show a gradual and statistically significant decrease in the uncertainties in the R0 determinations with time.
arXiv commentextended part of arXiv:1202.6128
References in corpus (34)
- Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
- Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- SINFONI in the Galactic Center: young stars and IR flares in the central light month
- The orbit of the star S2 around SgrA* from VLT and Keck data
- Stellar Dynamics in the Galactic centre: Proper Motions and Anisotropy
- A Geometric Determination of the Distance to the Galactic Center
- Distance to M31 With the HST and Hipparcos Red Clump Stars
- Galactic Kinematics of Cepheids from Hipparcos Proper Motions
- Galactocentric Distance With the OGLE and Hipparcos Red Clump Stars
- A Trigonometric Parallax of Sgr B2
- K-Band Calibration of the Red Clump Luminosity
- Globular cluster system and Milky Way properties revisited
- Trigonometric Parallax of W51 Main/South
- The Bar and Spiral Structure Legacy (BeSSeL) Survey: Mapping the Milky Way with VLBI Astrometry
- The structure of the Galactic bar
- The Absolute Magnitude and Kinematics of RR Lyrae Stars via Statistical Parallax
- Kinematics of the old stellar population at the Galactic Center
- Refining the Oort and Galactic constants
- The distance to the Galactic Centre based on Population-II Cepheids and RR Lyrae stars
- Characteristics of the Galaxy according to Cepheids
- A near-infrared survey of Miras and the distance to the Galactic Centre
- The Distance to the Galactic Center Derived From Infrared Photometry of Bulge Red Clump Stars
- Mira Variables in the OGLE Bulge fields
- The Shape and Scale of Galactic Rotation from Cepheid Kinematics
- Astrometry of Galactic Star-Forming Region ON2N with VERA: Estimation of the Galactic Constants
- Mass of the Galaxy Inferred from Outer Rotation Curve
- Distances to Nearby Galaxies: Combining Fragmentary Data Using Four Different Methods
- On accuracy assessment of celestial reference frame VLBI realizations
- Optical Gravitational Lensing Experiment. The Distance Scale: Galactic Bulge - LMC - SMC
- Kinematics of the Scorpius-Centaurus OB Association
- Study of Astronomical and Geodetic Series using the Allan Variance
- The influence of Galactic aberration on precession parameters determined from VLBI observations
- UBVI Color-Magnitude Diagrams in Baade's Window: Metallicity Range, Implications for the Red Clump Method, Color ``Anomaly'' and the Distances to the Galactic Center and the Large Magellanic Cloud
Cited by in corpus (23)
- The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016
- The Milky Way's Supermassive Black Hole: How good a case is it? A Challenge for Astrophysics & Philosophy of Science
- Systematic NLTE study of the -2.6 < [Fe/H] < 0.2 F and G dwarfs in the solar neighbourhood. I. Stellar atmosphere parameters
- Handling the Uncertainties in the Galactic Dark Matter Distribution for Particle Dark Matter Searches
- Proper motions and kinematics of selected bulge globular clusters
- Two estimates of the distance to the Galactic centre
- Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
- Clustering of Local Group distances: publication bias or correlated measurements? IV. The Galactic Center
- Recent advances in the determination of some Galactic constants in the Milky Way
- The Spatially-Resolved Star Formation History of the M31 Outer Disc
- Detecting Axion-like Dark Matter with Linearly Polarized Pulsar Light
- Vertical velocities from proper motions of red clump giants
- Toward an internally consistent astronomical distance scale
- Milky Way rotation curve from proper motions of red clump giants
- Constraining the pitch angle of the Galactic spiral arms in the Milky Way
- Antiproton Limits on Decaying Gravitino Dark Matter
- A Bayesian estimation of the Milky Way's circular velocity curve using Gaia DR3
- Determination of Galactic Rotation Parameters and the Solar Galactocentric Distance Ro from 73 Masers
- Anchors for the Cosmic Distance Scale: the Cepheid QZ Normae in the Open Cluster NGC 6067
- Statistical analysis of the determinations of the Sun's Galactocentric distance
- On the many '3-kiloparsec arms' - shocked wave and nuclear rotation
- Multi-band optical variability of a newly discovered twelve blazars sample from 2013-2019
- National Report for the International Association of Geodesy of the International Union of Geodesy and Geophysics 2011-2014