2022MNRAS.514.4489M


Query : 2022MNRAS.514.4489M

2022MNRAS.514.4489M - Mon. Not. R. Astron. Soc., 514, 4489-4505 (2022/August-2)

PIPS, an advanced platform for period detection in time series - I. Fourier-likelihood periodogram and application to RR Lyrae stars.

MURAKAMI Y.S., JENNINGS C., HOFFMAN A.M., SAVEL A.B., SUNSERI J., BAER-WAY R., STAHL B.E., ALTUNIN I., GIRISH N. and FILIPPENKO A.V.

Abstract (from CDS):

We describe the Period detection and Identification Pipeline Suite (PIPS) - a new, fast, and statistically robust platform for period detection and analysis of astrophysical time-series data. PIPS is an open-source Python package that provides various pre-implemented methods and a customizable framework for automated, robust period measurements with principled uncertainties and statistical significance calculations. In addition to detailing the general algorithm that underlies PIPS, this paper discusses one of PIPS' central and novel features, the Fourier-likelihood periodogram, and compares its performance to existing methods. The resulting improved performance implies that one can construct deeper, larger, and more reliable sets of derived properties from various observations, including all-sky surveys. We present a comprehensive validation of PIPS against artificially generated data, which demonstrates the reliable performance of our algorithm for a class of periodic variable stars (RR Lyrae stars).

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): methods: data analysis - methods: statistical - stars: variables

Simbad objects: 2

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Number of rows : 2
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 M 3 GlC 13 42 11.62 +28 22 38.2     6.39     ~ 2593 0
2 NGC 7078 564 RR* 21 29 58.1933027208 +12 12 09.883495224   16.241 15.795   15.178 ~ 22 0

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