2024A&A...686A.158S


Query : 2024A&A...686A.158S

2024A&A...686A.158S - Astronomy and Astrophysics, volume 686A158 (2024/6-1)

FINKER: Frequency Identification through Nonparametric KErnel Regression in astronomical time series.

STOPPA F., JOHNSTON C., CATOR E., NELEMANS G. and GROOT P.J.

Abstract (from CDS):

Context. Optimal frequency identification in astronomical datasets is crucial for variable star studies, exoplanet detection, and astero-seismology. Traditional period-finding methods often rely on specific parametric assumptions, employ binning procedures, or overlook the regression nature of the problem, limiting their applicability and precision.
Aims. We introduce a universal- nonparametric kernel regression method for optimal frequency determination that is generalizable, efficient, and robust across various astronomical data types.
Methods. FINKER uses nonparametric kernel regression on folded datasets at different frequencies, selecting the optimal frequency by minimising squared residuals. This technique inherently incorporates a weighting system that accounts for measurement uncertainties and facilitates multi-band data analysis. We evaluated our method's performance across a range of frequencies pertinent to diverse data types and compared it with an established period-finding algorithm, conditional entropy.
Results. The method demonstrates superior performance in accuracy and robustness compared to existing algorithms, requiring fewer observations to reliably identify significant frequencies. It exhibits resilience against noise and adapts well to datasets with varying complexity.

Abstract Copyright: © The Authors 2024

Journal keyword(s): methods: data analysis - methods: statistical - techniques: radial velocities - binaries: eclipsing - stars: variables: RR Lyrae

Simbad objects: 12

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Number of rows : 12
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 V* V772 Cas a2* 01 42 02.9108207472 +61 02 17.656928916   6.647 6.677     B8IIIp(Si) 58 0
2 ATO J052.9483-28.2188 EB* 03 31 47.6024244705 -28 13 07.973101221   14.373 13.981 14.201   ~ 4 0
3 CRTS J033427.7-271223 RR* 03 34 27.8275740072 -27 12 22.366573524   16.68 15.49 15.08 14.98 ~ 10 0
4 BPS CS 29526-0042 RR* 03 35 00.4498438464 -27 28 55.044781536   15.07 14.68 15.03 13.99 ~ 13 0
5 GALEX J041016.8-083419 WD* 04 10 16.7969256504 -08 34 19.310390328           DA 6 0
6 ZTF J053708.26-245014.6 WD* 05 37 08.2527999720 -24 50 14.907939612           DA 5 0
7 ZTF J063808.71+091027.4 EB* 06 38 08.7236222084 +09 10 27.659546282           ~ 4 0
8 HD 114520 SB* 13 10 52.3488452472 +21 14 01.518823320   7.28 6.82     F5IV-VSr 53 0
9 LAMOST J140702.58+211600.1 WD* 14 07 02.5848000 +21 16 00.156000           D+dM4 4 0
10 MLT J162036.64-614110.5 EB* 16 20 36.6473370186 -61 41 10.587383353           ~ 2 0
11 HD 165246 SB* 18 06 04.6792554840 -24 11 43.890335448 6.90 7.70 7.60 8.77   O8V(n) 93 0
12 HD 188891 EB* 19 55 44.7623727072 +40 23 30.252212484 6.55 7.29 7.30     B1V 58 0

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