pith. machine review for the scientific record. sign in

arxiv: 1703.09824 · v1 · submitted 2017-03-28 · 🌌 astro-ph.IM

Recognition: unknown

Understanding the Lomb-Scargle Periodogram

Authors on Pith no claims yet
classification 🌌 astro-ph.IM
keywords lomb-scargleperiodogramconsiderationsimportantpracticalalgorithmapplicationassumptions
0
0 comments X
read the original abstract

The Lomb-Scargle periodogram is a well-known algorithm for detecting and characterizing periodic signals in unevenly-sampled data. This paper presents a conceptual introduction to the Lomb-Scargle periodogram and important practical considerations for its use. Rather than a rigorous mathematical treatment, the goal of this paper is to build intuition about what assumptions are implicit in the use of the Lomb-Scargle periodogram and related estimators of periodicity, so as to motivate important practical considerations required in its proper application and interpretation.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 14 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. AGILE detection of transient {\gamma}-ray emission from the region of the supergiant fast X-ray transient source IGR J17354-3255

    astro-ph.HE 2026-05 unverdicted novelty 7.0

    AGILE archival data reveal gamma-ray flares from a source matching IGR J17354-3255, with orbital phase correlation supporting physical association and high-energy emission from SFXTs.

  2. An eclipsing CEMP candidate discovered in a search for dwarf carbon stars in post-common envelope binaries

    astro-ph.SR 2026-05 unverdicted novelty 6.0

    The first eclipsing CEMP candidate is identified in a 1.224-day binary, with 3.5% of dwarf carbon stars showing short-period variability consistent with tidally locked post-common envelope systems and supporting wind ...

  3. The 2MIG isolated AGNs. 3. Optical--IR variability and dust reverberation in the NLSy1 galaxies Mrk~42 and Mrk~493

    astro-ph.GA 2026-05 unverdicted novelty 6.0

    Optical-MIR lags of 39.1 days and 79.4 days are measured in Mrk 42 and Mrk 493, yielding dust reverberation radii of 0.032 pc and 0.065 pc with R_dust/R_BLR ratios of approximately 6-7.

  4. Detection of optical quasi-periodic oscillation in the blazar 3C 454.3

    astro-ph.HE 2026-04 unverdicted novelty 6.0

    Detection of a persistent ~433-day optical QPO in blazar 3C 454.3 at 2.53σ significance using Lomb-Scargle, WWZ, and PDM methods, with a new test for seasonal gaps.

  5. Short timescale variation in the submillimeter flux of Sagittarius A*

    astro-ph.GA 2026-04 unverdicted novelty 6.0

    Sgr A* exhibits a white-noise-like flat variability regime in its 340 GHz flux on timescales below 2.3 to 6.3 minutes, transitioning to red-noise-like behavior at longer timescales, with no evidence for narrow periodi...

  6. GSC 08227-00723: An Unusually Large PSH Excess AH Pic Candidate

    astro-ph.SR 2026-05 unverdicted novelty 5.0

    GSC 08227-00723 is classified as a new AH Pic-type nova-like variable with recurrent stunted outbursts and an exceptionally large positive superhump excess of approximately 0.19.

  7. Multi-wavelength outburst activity from EP J174942.2-384834: a very faint X-ray transient discovered by Einstein Probe

    astro-ph.HE 2026-05 accept novelty 5.0

    EP J174942.2-384834 is classified as a very faint X-ray transient black hole candidate based on its hard X-ray spectra, optical/UV brightening correlated with X-rays, and lack of radio emission.

  8. Multiwavelength Characterization of a New Magnetic Cataclysmic Variable 2CXO J050740.7-091337

    astro-ph.HE 2026-05 accept novelty 5.0

    2CXO J0507 is a polar-type magnetic cataclysmic variable featuring a white dwarf with B ≈ 30 MG and an orbital period of 2.34 hours, identified through multiwavelength archival and follow-up data.

  9. Random Polarization Position Angle Behaviors across Bursts of Repeating Fast Radio Bursts

    astro-ph.HE 2026-05 unverdicted novelty 5.0

    Polarization position angles of repeating FRBs are Gaussian distributed with no periodicity, arising from geometric projection in a stochastically varying magnetosphere that also explains non-repeating FRBs.

  10. A Search for Rotation Measure Flare Candidates in Repeating Fast Radio Bursts

    astro-ph.HE 2026-04 unverdicted novelty 5.0

    A search of repeating FRBs identifies RM flare candidates in FRB 20121102A, FRB 20201124A, and FRB 20180916B, suggesting such events may be common and tied to dynamic magneto-ionic environments.

  11. The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars Within 500 pc

    astro-ph.SR 2026-03 unverdicted novelty 5.0

    The TESS All-Sky Rotation Survey provides periods for 1,046,317 stars within 500 pc, with an estimated 93% being true rotation periods, and includes a method to correct half-period aliases.

  12. On the origin of variability in $\alpha$ Cygni variable $\epsilon$ Ori (HD 37128) using TESS observations and modelling

    astro-ph.SR 2026-05 conditional novelty 4.0

    Linear stability analysis and non-linear hydrodynamical simulations link the stochastic low-frequency variability of ε Ori to strange-mode instabilities that excite finite-amplitude pulsations.

  13. A Search for Variability of Ultracool Dwarfs with the Zwicky Transient Facility

    astro-ph.SR 2026-05 unverdicted novelty 4.0

    ZTF data yielded 32 robust ultracool dwarf rotation periods including 12 new detections, with a trend of decreasing periods toward later spectral types in dwarfs older than 100 Myr.

  14. A Search for High Frequency Oscillations in TESS Cycle 7

    astro-ph.SR 2026-05 unverdicted novelty 3.0

    A homogeneous search of TESS Cycle 7 20-second cadence light curves identifies 73 rapid oscillators (24 white dwarfs, 31 hot subdwarfs, 18 A-F stars) with measured frequencies and amplitudes after vetting.