Author Notes
Categorizing variable stars can reveal information ranging from stellar properties to cosmic distances. Traditionally, the classification process relied on human expertise and limited data. With the emergence of transformative machine learning methodologies and large-scale cosmological surveys, we are able to perform more efficient, accurate, and robust handling of expansive databases. This review traces the evolution of the classification of variable stars and highlights advancements from the latest surveys and cutting-edge technology. Reviewing papers in the field provides new insights into potential directions for improving classification methods.
REFERENCES
1.
2.
A.
Udalski
, M.
Szymanski
, J.
Kaluzny
, M.
Kubiak
, and M.
Mateo
, “The optical gravitational lensing experiment
,” 3. Acta Astron.
42
, 253
–284
(1992
).3.
I.
Nun
, P.
Protopapas
, B.
Sim
, M.
Zhu
, R.
Dave
, N.
Castro
, and K.
Pichara
, “FATS: Feature Analysis for Time Series
,” preprint arXiv:1506.00010 [astro-ph.IM] (2015
).4.
J.
Govea
, T.
Gomez
, G. W.
Preston
, and C.
Sneden
, “The chemical compositions of RR Lyrae type C variable stars
,” Astrophys. J.
782
, 59
(2014
).5.
P. T.
Oosterhoff
, “Some remarks on the variable stars in globular clusters
,” Observatory
62
, 104
–109
(1939
).6.
G. L. H.
Harris
, M.
Rejkuba
, and W. E.
Harris
, “The distance to NGC 5128 (Centaurus A)
,” Publ. Astron. Soc. Aust.
27
, 457
–462
(2013
).7.
E.
Pigott
, “IX. Observations and remarks on those stars which the astronomers of the last century suspected to be changeable
,” Philos. Trans. Soc. London
76
, 189
–219
(1786
).8.
E.
Zsoldos
, “Three early variable star catalogues
,” J. Hist. Astron.
25
, 92
–98
(1994
).9.
J. R.
Percy
, Understanding Variable Stars
(Cambridge University Press
, Cambridge
, 2007
), oCLC: ocm81453063.10.
N. N.
Samus
, E. V.
Kazarovets
, O. V.
Durlevich
, N. N.
Kireeva
, and E. N.
Pastukhova
, “General catalogue of variable stars: Version GCVS 5.1
,” Astron. Rep.
61
, 80
–88
(2017
).11.
J. A.
Mattei
and A.
Henden
, “Variable Star
,” in McGraw-Hill Dictionary of Scientific and Technical Terms
(McGraw-Hill Education
, 1995
).12.
L.
Eyer
and N.
Mowlavi
, “Variable stars across the observational HR diagram
,” J. Phys. Conf. Ser.
118
, 012010
(2008
).13.
A.
Udalski
, M. K.
Szymański
, and G.
Szymański
, “OGLE-IV: Fourth phase of the Optical Gravitational Lensing Experiment
,” preprint arXiv:1504.05966 [astro-ph.SR] (2015).14.
F.
Pedregosa
, G.
Varoquaux
, A.
Gramfort
, V.
Michel
, B.
Thirion
, O.
Grisel
, M.
Blondel
, A.
Müller
, J.
Nothman
, G.
Louppe
, ., “Scikit-learn: Machine learning in Python
,” preprint arXiv:1201.0490 [cs.LG].15.
L.
Breiman
, “Random forest
,” Mach. Learn.
45
, 5
–32
(2001
).16.
T.
Szklenár
, A.
Boái
, D.
Tarczay-Nehéz
, K.
Vida
, G.
Mező
, and R.
Szabó
, “Variable star classification with a multiple-input neural network
,” Astrophys. J.
938
, 37
(2022
).17.
J.
Bergstra
, D.
Yamins
, and D. D.
Cox
, “Hyperopt: A Python library for optimizing the hyperparameters of machine learning algorithms
,” (2013
).18.
I. N.
Pashchenko
, K. V.
Sokolovsky
, and P.
Gavras
, “Machine learning search for variable stars
,” Mon. Not. R. Astron. Soc.
475
, 2326
–2343
(2018
).19.
T.
Fushiki
, “Estimation of prediction error by using K-fold cross-validation
,” Stat. Comput.
21
, 137
–146
(2011
).20.
G. C.
Clayton
, “The R Coronae Borealis stars
,” Publ. Astron. Soc. Pac.
108
, 225
(1996
).21.
A.
Mammone
, M.
Turchi
, and N.
Cristianini
, “Support vector machines
,” WIREs Computational Statistics
1
, 283
–289
(2009
).22.
Z.
Hosenie
, R. J.
Lyon
, B. W.
Stappers
, and A.
Mootoovaloo
, “Comparing multiclass, binary, and hierarchical machine learning classification schemes for variable stars
,” Mon. Not. R. Astron. Soc.
488
, 4858
–4872
(2019
).23.
P. F. L.
Maxted
and R. J.
Hutcheon
, “Discovery and characterisation of long-period eclipsing binary stars from Kepler K2 campaigns 1, 2, and 3
,” Astron. Astrophys.
616
, A38
(2018
).24.
B. V.
Alexeev
, “Nonlocal Theory of Variable Stars
,” in Nonlocal Astrophysics
(Elsevier
, New York
, 2017
), pp. 321
–377
.
This content is only available via PDF.
© 2024 Author(s).
2024
Author(s)
Published by AIP Publishing.