Study of the mass-ratio distribution of spectroscopic binaries. I. A novel algorithm
Sahar Shahaf, Tsevi Mazeh, Simchon Faigler

TL;DR
This paper introduces a new algorithm to accurately determine the mass-ratio distribution of short-period spectroscopic binaries from observational data, accounting for biases and using a novel observable and basis functions.
Contribution
The authors present a novel direct algorithm that uses a new observable and basis functions to derive the MRD, improving accuracy and bias correction over previous methods.
Findings
The algorithm accurately recovers the MRD in simulated data.
It effectively accounts for observational biases and undetected systems.
The method is robust with different basis function choices.
Abstract
We developed a novel direct algorithm to derive the mass-ratio distribution (MRD) of short-period binaries from an observed sample of single-lined spectroscopic binaries (SB1). The algorithm considers a class of parameterized MRDs and finds the set of parameters that best fits the observed sample. The algorithm consists of four parts. First, we define a new observable, the `modified mass function', that can be calculated for each binary in the sample. We show that the distribution of the modified mass function follows the shape of the underlying MRD, turning it more advantageous than the previously used mass function, reduced mass function or reduced mass function logarithm. Second, we derive the likelihood of the sample of modified mass functions to be observed given an assumed MRD. An MCMC search enables the algorithm to find the parameters that best fit the observations. Third, we…
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