2021MNRAS.507.3351L


Query : 2021MNRAS.507.3351L

2021MNRAS.507.3351L - Mon. Not. R. Astron. Soc., 507, 3351-3361 (2021/November-1)

A Bayesian inference and model selection algorithm with an optimization scheme to infer the model noise power.

LOPEZ-SANTIAGO J., MARTINO L., VAZQUEZ M.A. and MIGUEZ J.

Abstract (from CDS):

Model fitting is possibly the most extended problem in science. Classical approaches include the use of least-squares fitting procedures and maximum likelihood methods to estimate the value of the parameters in the model. However, in recent years, Bayesian inference tools have gained traction. Usually, Markov chain Monte Carlo (MCMC) methods are applied to inference problems, but they present some disadvantages, particularly when comparing different models fitted to the same data set. Other Bayesian methods can deal with this issue in a natural and effective way. We have implemented an importance sampling (IS) algorithm adapted to Bayesian inference problems in which the power of the noise in the observations is not known a priori. The main advantage of IS is that the model evidence can be derived directly from the so-called importance weights - while MCMC methods demand considerable postprocessing. The use of our adaptive target adaptive importance sampling (ATAIS) method is shown by inferring, on the one hand, the parameters of a simulated flaring event that includes a damped oscillation and, on the other hand, real data from the Kepler mission. ATAIS includes a novel automatic adaptation of the target distribution. It automatically estimates the variance of the noise in the model. ATAIS admits parallelization, which decreases the computational run-times notably. We compare our method against a nested sampling method within a model selection problem.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): methods: data analysis - methods: numerical - methods: statistical - stars: activity - stars: flare

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 UCAC4 704-062773 ** 19 19 18.830904 +50 44 03.69708   15.894 15.922 16.216   DA+dMe 17 0

Query : 2021MNRAS.507.3351L

Basic data :
UCAC4 704-062773 -- Double or Multiple Star
Other object types:
otypes_help
* (2016MNRAS,UCAC4,...), WD* (2010MNRAS), ** (2010MNRAS), MIR (WISEA,WISE), Er* (2016ApJ), NIR (2MASS), Opt (LAMOST)
ICRS coord. (ep=J2000) :
19 19 18.830904 +50 44 03.69708 (Optical) [ 91 83 90 ] B 2012yCat.1322....0Z
FK4 coord. (ep=B1950 eq=1950) :
19 18 01.709078 +50 38 21.89402 [ 91 83 90 ]
Gal coord. (ep=J2000) :
081.985043495 +16.540129973 [ 91 83 90 ]
Proper motions mas/yr :
30.8 90.4 [5.8 5.5 90] C 2012yCat.1322....0Z
Spectral type:
DA+dMe D 2010MNRAS.409.1470O
Fluxes (10) :
B 15.894 [0.03] D 2012yCat.1322....0Z
V 15.922 [0.01] D 2012yCat.1322....0Z
R 16.216 [0.13] E 2012yCat.1322....0Z
G 15.781825 [0.013659] C 2022yCat.1355....0G
J 12.950 [0.026] C 2003yCat.2246....0C
H 12.44 [0.03] C 2003yCat.2246....0C
K 12.141 [0.020] C 2003yCat.2246....0C
g 15.795 [0.01] E 2012yCat.1322....0Z
r 15.892 [0.01] E 2012yCat.1322....0Z
i 15.136 [0.01] E 2012yCat.1322....0Z
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Identifiers (9) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

UCAC4 704-062773 2MASS J19191885+5044038 WISE J191918.88+504404.6
KIC 12156549 TIC 267672376 EQ J1919.3+5044
LAMOST J191918.85+504403.8 WISEA J191918.88+504404.5 Gaia DR3 2133085788052576384

References (17 between 1850 and 2026) (Total 17)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Var : 2    Fe/H : 1    SpT : 3   

   


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UCAC4 704-062773 KIC 12156549 2MASS J19191885+5044038 WISEA J191918.88+504404.5 WISE J191918.88+504404.6
Gaia DR3 2133085788052576384

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