2021AJ....161..281K


Query : 2021AJ....161..281K

2021AJ....161..281K - Astron. J., 161, 281-281 (2021/June-0)

An exploration of three new methods to facilitate the calculation of the significance levels of periodogram peaks by simulation.

KOEN C.

Abstract (from CDS):

At a given frequency ν, calculation of the periodogram entails evaluating two linear combinations C(ν) and S(ν) of the observations. It is pointed out that C and S are normally distributed even for relatively small numbers of observations. This can be used as a basis for simulating periodograms from a multivariate normal distribution with specified covariance structure. The advantage is that computationally expensive evaluations of sinusoids need to be performed only once-in the calculation of the covariances. Furthermore, the large covariance matrix can be factorized, and the factors replaced by low-rank approximations, which alleviates the computer memory demands. The second part of the paper discusses the choice of the degree of oversampling of the periodogram, i.e., the spacing Δνof the frequency grid over which it is calculated. It is shown using Δν∼0.2/ΔT, where ΔT is the time baseline of the observations, leads to an error of only about 1% in the percentiles of the distribution of maximum peak values. The third part of the paper deals with the representation of the distribution of periodogram maxima by the generalized extreme value distribution. Although the generalized extreme value form may formally differ highly significantly from the actual distribution of periodogram maxima, it is demonstrated that it may nonetheless be useful in practical terms. Results are illustrated throughout using three data sets with widely different aliasing properties.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Time series analysis

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 ATO J199.6731-31.7189 EB? 13 18 41.5422475272 -31 43 07.071787848   17.50 15.76 15.74 12.76 M4 8 0

Query : 2021AJ....161..281K

Basic data :
ATO J199.6731-31.7189 -- Eclipsing Binary Candidate
Other object types:
otypes_help
* (UCAC4,GSC2.3,...), EB? (2018AJ), NIR (2MASS), Opt (ATO)
ICRS coord. (ep=J2000) :
13 18 41.5422475272 -31 43 07.071787848 (Optical) [ 0.0219 0.0156 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
13 15 54.1563906441 -31 27 17.994969726 [ 0.0219 0.0156 90 ]
Gal coord. (ep=J2000) :
309.6789411430908 +30.7958111150595 [ 0.0219 0.0156 90 ]
Proper motions mas/yr :
7.286 -62.642 [0.025 0.018 90] A 2020yCat.1350....0G
Parallaxes (mas):
19.3234 [0.0244] A 2020yCat.1350....0G
Spectral type:
M4 D 2019MNRAS.490.1283K
Fluxes (11) :
B 17.50 [0.23] D 2012yCat.1322....0Z
V 15.76 [0.05] D 2012yCat.1322....0Z
R 15.74 [0.07] E 2012yCat.1322....0Z
G 14.286475 [0.006886] C 2020yCat.1350....0G
I 12.76 [0.42] E 2008AJ....136..735L
J 11.175 [0.023] C 2003yCat.2246....0C
H 10.613 [0.023] C 2003yCat.2246....0C
K 10.336 [0.019] C 2003yCat.2246....0C
g 16.52 [0.07] D 2012yCat.1322....0Z
r 15.07 [0.04] D 2012yCat.1322....0Z
i 13.40 [0.08] D 2012yCat.1322....0Z
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Identifiers (8) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

UCAC4 292-070541 ATO J199.6731-31.7189 2MASS J13184154-3143070 Gaia DR3 6181322502977295360
ATO J199.6731-31.7188 GSC2.3 S97D023088 TIC 124604724 Gaia DR2 6181322502977295360

References (8 between 1850 and 2026) (Total 8)
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

Distance : 2    Var : 1    Plx : 2    PM : 2   

   


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UCAC4 292-070541 2MASS J13184154-3143070 Gaia DR3 6181322502977295360 Gaia DR2 6181322502977295360

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