2025A&A...697A..35R


Query : 2025A&A...697A..35R

2025A&A...697A..35R - Astronomy and Astrophysics, volume 697A35 (2025/5-1)

Singular spectrum analysis of Fermi-LAT blazar light curves: A systematic search for periodicity and trends in the time domain.

RICO A., DOMINGUEZ A., PENIL P., AJELLO M., BUSON S., ADHIKARI S. and MOVAHEDIFAR M.

Abstract (from CDS):

Context. A majority of blazars exhibit variable emission across the entire electromagnetic spectrum, observed over various timescales. In particular, discernible periodic patterns are detected in the γ-ray light curves (LCs) of a few blazars, such as PG 1553+113, S5 1044+71, and PKS 0426-380. The presence of trends, flares, and noise complicates the detection of periodicity, requiring careful analysis to determine whether these patterns are related to emission mechanisms within the source or occur by chance.
Aims. We employ singular spectrum analysis (SSA) for the first time on data from the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope to systematically search for periodicity in the time domain, using 28-day binned LCs. Our aim is to isolate any potential periodic nature of the emission from trends and noise, thereby reducing uncertainties in revealing periodicity. Additionally, we aim to characterize long-term trends and develop a forecasting algorithm based on SSA, enabling accurate predictions of future emission behavior.
Methods. We apply SSA to analyze 494 sources detected by Fermi-LAT, focusing on identifying and isolating oscillatory components from trends and noise in their γ-ray LCs. We calculate the Lomb-Scargle periodogram (LSP) for the oscillatory components extracted by SSA to determine the most significant periods. The local and global significance of these periods is then assessed to validate their authenticity.
Results. Our analysis identifies 46 blazars as potential candidates for quasi-periodic γ-ray emissions, each with a local significance level ≥2σ. Notably, 33 of these candidates exhibit a local significance of ≥4σ (corresponding to a global significance of ≥2.2σ). Our findings introduce 25 new γ-ray candidates, effectively doubling the number of potentially periodic sources. This study provides a foundation for future investigations by identifying promising candidates and highlighting their potential significance within the context of blazar variability.

Abstract Copyright: © The Authors 2025

Journal keyword(s): methods: data analysis - galaxies: active - BL Lacertae objects: general - gamma rays: general

Simbad objects: 47

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Number of rows : 47
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 SDSS J004348.84+342626.1 Bla 00 43 48.8431545768 +34 26 26.091802608       19.9   ~ 78 1
2 QSO B0109+224 BLL 01 12 05.8247044608 +22 44 38.785880796   16.00 15.66 15.47   ~ 373 2
3 6C 013354+473615 Bla 01 36 58.59480326 +47 51 29.1000720     19.50 19.25 15.21 ~ 537 1
4 QSO B0208-512 BLL 02 10 46.2004407600 -51 01 01.893013392   17.10 16.93 14.82   ~ 485 1
5 3C 66A BLL 02 22 39.6114771888 +43 02 07.799534304   15.71 15.21 14.5   ~ 942 2
6 ICRF J025247.9-221925 Bla 02 52 47.95365568 -22 19 25.4659009       19.83   ~ 130 1
7 PKS J0303-2407 BLL 03 03 26.5025589984 -24 07 11.426291220   16.55 16.18     ~ 249 1
8 QSO B0403-132A BLL 04 05 34.00339116 -13 08 13.6909309   17.37 17.09 16.6   ~ 384 1
9 QSO B0405-385 Bla 04 06 59.03533781 -38 26 28.0423651   19.55 18.0     ~ 250 2
10 3FGL J0427.3-3900 Bla 04 27 18.2 -39 00 35           ~ 25 0
11 PMN J0427-3900 rG 04 27 21.66 -39 01 00.1           ~ 13 1
12 WISEA J042840.41-375619.3 BLL 04 28 40.4241894720 -37 56 19.580735832   18.96 19.0 17.21   ~ 343 1
13 PKS J0449-4350 BLL 04 49 24.6981911928 -43 50 08.960970948 14.95 17.52 15.24 16.27   ~ 190 1
14 QSO J0457-2324 Bla 04 57 03.1791422424 -23 24 52.021129572   18.85 18.5 16.56   ~ 435 1
15 4C -02.19 Bla 05 01 12.80988538 -01 59 14.2564557   19.1 18.06 19.04   ~ 624 1
16 RX J0521.7+2112 BLL 05 21 45.9657388992 +21 12 51.452786736           ~ 162 1
17 QSO B0524-485 Bla 05 26 16.67131784 -48 30 36.7919695     20.0 19.36   ~ 107 1
18 7C 071604.59+331243.00 BLL 07 19 19.41966120 +33 07 09.7087082   17.66 17.05     ~ 130 1
19 8C 0716+714 BLL 07 21 53.4482942664 +71 20 36.363846516   15.5 15.50 14.27   ~ 1388 1
20 QSO B0808+019 BLL 08 11 26.70731711 +01 46 52.2201568   17.58 17.2 17.96   ~ 281 1
21 QSO J0948+0022 Bla 09 48 57.32005819 +00 22 25.5596984   18.85 18.61 18.17   ~ 350 2
22 QSO B1005-333 BLL 10 07 31.38745248 -33 33 06.7169760   20.18 18.0 19.80   ~ 60 1
23 7C 1030+4131 Bla 10 33 03.70787172 +41 16 06.2329333   20.01 19.64 19.97   ~ 234 1
24 6C 104451+715930 Bla 10 48 27.61992778 +71 43 35.9384142     19.0 17.49   ~ 270 1
25 6C 114419+401458 Bla 11 46 58.29791724 +39 58 34.3043988   18.80 18.45 18.58   ~ 261 1
26 4C 04.42 Bla 12 22 22.54962606 +04 13 15.7760715   17.88 17.98 17.06   ~ 354 1
27 8C 1221+809 BLL 12 23 40.49375661 +80 40 04.3404140     19.0 19.3   ~ 119 1
28 1RXS J125311.9+530105 BLL 12 53 11.9204702472 +53 01 11.737422696   18.07 17.51 16.4   ~ 143 1
29 [VV2006] J131250.9-042451 Bla 13 12 50.90123596 -04 24 49.8921276     18.7 19.29   ~ 86 1
30 [VV2006] J132111.2+221613 Bla 13 21 11.20255812 +22 16 12.1083023   19.59 19.23 19.37   ~ 133 1
31 PG 1424+240 BLL 14 27 00.3917926224 +23 48 00.037510776 14.52 14.34 14.95 14.5   ~ 420 1
32 ICRF J142741.3-330531 BLL 14 27 41.3611529328 -33 05 31.504402104       17.48   ~ 73 1
33 RX J1454.4+5124 BLL 14 54 27.1245711624 +51 24 33.731127900   18.76 18.35     ~ 103 1
34 QSO J1512-0906 Bla 15 12 50.53293048 -09 05 59.8297908   16.74 16.54     ~ 1409 1
35 7C 1520+3154 Bla 15 22 09.99173254 +31 44 14.3819383   20.45 19.89 19.87   ~ 230 1
36 PMN J1532-1319 Bla 15 32 45.37473348 -13 19 10.0860403       22.20   ~ 72 1
37 PG 1553+113 BLL 15 55 43.0440048528 +11 11 24.365649948 14.91 14.72 14.57 13.99   ~ 672 1
38 4C 47.44 Bla 16 37 45.13055568 +47 17 33.8311081   17.5   18.69   ~ 183 1
39 4C 48.41 BLL 16 57 46.87895361 +48 08 33.0407928       19.70   ~ 92 1
40 ASASSN -14ct Bla 17 23 50.8444548552 -77 13 50.548166148           ~ 59 2
41 QSO B1903-802 Bla 19 12 40.01907746 -80 10 05.9464844   19.83 19.0 19.54   ~ 89 1
42 7C 2010+4619 BLL 20 12 05.6371245432 +46 28 55.779736836           ~ 92 2
43 QSO B2136-428 BLL 21 39 24.1733820912 -42 35 20.465859048   16.50 16.2 15.7   ~ 97 1
44 PKS J2158-3013 BLL 21 58 52.0652249880 -30 13 32.118447792   13.36 13.09 12.62   ~ 1829 1
45 AT20G J220219-833812 Bla 22 02 19.2376999896 -83 38 11.831685864     18.5 19.3   ~ 69 1
46 NAME BL Lac BLL 22 02 43.2913536816 +42 16 39.979416792   15.66 14.72     ~ 2397 1
47 QSO B2232+282 BLL 22 36 22.47084387 +28 28 57.4132050   19.1 19.0 17.60   ~ 306 2

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