On calibration of some distance scales in astrophysics

We present a method for distance calibration without using standard fitting procedures. Instead, we use random resampling to reconstruct the probability density function (PDF) of calibration data points in the fitting plane. The resulting PDF is then used to estimate distance-related properties. The...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2014-05, Vol.440 (3), p.2026-2035
Main Authors: Vukotić, B., Jurković, M., Urošević, D., Arbutina, B.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Calibration
Luminosity
Nebulae
Probability
Supernovae
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Description
Summary:We present a method for distance calibration without using standard fitting procedures. Instead, we use random resampling to reconstruct the probability density function (PDF) of calibration data points in the fitting plane. The resulting PDF is then used to estimate distance-related properties. The method is applied to samples of radio surface brightness to diameter (...) ) data for the Galactic supernova remnants (SNRs) and planetary nebulae (PNe), and period-luminosity (PL) data for the Large Magellanic Cloud (LMC) fundamental mode classical Cepheids. We argue that resulting density maps can provide more accurate and more reliable calibrations than those obtained by standard linear fitting procedures. For the selected sample of the Galactic SNRs, the presented PDF method of distance calibration results in a smaller average distance fractional error of up to ...16 percentage points. Similarly, the fractional error is smaller for up to ...8 and ...0.5 percentage points, for the samples of Galactic PNe and LMC Cepheids, respectively. In addition, we provide a PDF-based calibration data for each of the samples. (ProQuest: ... denotes formulae/symbols omitted.)
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stu405