2021PASP..133a4401Y


Query : 2021PASP..133a4401Y

2021PASP..133a4401Y - Publ. Astron. Soc. Pac., 133, part no 1, 4401-14401 (2021/January-0)

Searching for possible exoplanet transits from BRITE data through a machine learning technique.

YEH L.-C. and JIANG I.-G.

Abstract (from CDS):

The photometric light curves of BRITE satellites were examined through a machine learning technique to investigate whether there are possible exoplanets moving around nearby bright stars. Focusing on different transit periods, several convolutional neural networks were constructed to search for transit candidates. The convolutional neural networks were trained with synthetic transit signals combined with BRITE light curves until the accuracy rate was higher than 99.7%. Our method could efficiently lead to a small number of possible transit candidates. Among these ten candidates, two of them, HD37465, and HD186882 systems, were followed up through future observations with a higher priority. The codes of convolutional neural networks employed in this study are publicly available at http://www.phys.nthu.edu.tw/~jiang/BRITE2020YehJiangCNN.tar.gz.

Abstract Copyright: © 2020. The Astronomical Society of the Pacific. All rights reserved.

Journal keyword(s): Time series analysis - Exoplanet detection methods - Exoplanet systems

Simbad objects: 33

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Number of rows : 33
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 * alf Per V* 03 24 19.3700924 +49 51 40.245455 2.64 2.27 1.79     F5Ib 870 1
2 * eta Tau Be* 03 47 29.0765529 +24 06 18.488347 2.44 2.78 2.87 2.84 2.88 B7III 557 1
3 * nu. Eri bC* 04 36 19.1419185396 -03 21 08.857744927 2.82 3.737 3.928     B2III 407 0
4 * pi.03 Ori PM* 04 49 50.4112051485 +06 57 40.600622266 3.620 3.630 3.190 2.77 2.51 F6V 601 0
5 * bet Eri PM* 05 07 50.9748851089 -05 05 11.389142292 3.02 2.92 2.79 2.65 2.57 A3IV 231 0
6 * tau Ori * 05 17 36.3903358088 -06 50 39.866785352 3.01 3.47 3.59     B6III 198 0
7 * gam Ori V* 05 25 07.86325 +06 20 58.9318 0.54 1.42 1.64 1.73 1.95 B2III 542 1
8 * ups Ori SB* 05 31 55.8599595648 -07 18 05.535884975 3.30 4.36 4.63 4.75 5.01 O9.7V 426 0
9 * iot Ori SB* 05 35 25.9861932063 -05 54 35.598684624 1.45 2.53 2.77     O9IIIvar 793 0
10 * sig Ori Y*O 05 38 44.7653828520 -02 36 00.283179888 2.54 3.58 3.79 3.87 4.11 O9.5V+B0.2V(n) 855 0
11 HD 37465 PM* 05 43 56.7725460864 +66 37 34.042452708   8.03 6.80     K0 13 0
12 * bet Pic PM* 05 47 17.0876901 -51 03 59.441135 4.13 4.03 3.86 3.74 3.58 A6V 2087 1
13 * bet Pic b Pl 05 47 17.0876901 -51 03 59.441135           ~ 627 1
14 * a Pup SB* 07 52 13.0318512432 -40 34 32.814235704   4.717 3.696     K1/2II+A 89 0
15 HD 64740 * 07 53 03.6344819483 -49 36 46.956285817 3.48 4.40 4.63 4.76 4.97 B2V 223 0
16 * h01 Pup s*r 08 11 21.4934302224 -39 37 06.758795424 7.79 6.03 4.42 3.22 2.34 K4.5Ib 71 0
17 * eps Car A * 08 22 30.833784 -59 30 34.13052   3.86 2.01     K3:III 7 0
18 * bet Pyx * 08 40 06.1432829632 -35 18 30.078413177   4.885 3.954     G5II/III 82 0
19 * alf Pyx V* 08 43 35.5374303414 -33 11 10.979806079 2.65 3.50 3.68 3.76 3.93 B1.5III 224 0
20 * d Vel * 08 44 23.9470741416 -42 38 57.398847432   4.917 4.046     G6III 86 0
21 * c Car PM* 08 55 02.8480985300 -60 38 40.594250640 3.28 3.74 3.80     B8II-III 83 0
22 * c Vel PM* 09 04 09.2796508887 -47 05 51.846278984 6.16 4.95 3.75 2.93 2.33 K2III 72 0
23 * a Car SB* 09 10 58.0852959464 -58 58 00.841998284 2.56 3.25 3.40     B2IV-V 148 0
24 * iot Car V* 09 17 05.4068572 -59 16 30.835305 2.60 2.44 2.26 2.02 1.82 A7Ib 166 0
25 * kap Vel SB* 09 22 06.8176100 -55 00 38.401683 1.5 2.324 2.473     B2IV 172 0
26 * psi Vel ** 09 30 41.99958 -40 28 00.2616 3.89 3.96 3.60 3.24 3.02 F3VFe-0.7 123 0
27 * zet Cen SB* 13 55 32.38565 -47 17 18.1482 1.42 2.33 2.55 2.69 2.89 B2.5IV 184 0
28 * zet Lup PM* 15 12 17.0955222617 -52 05 57.295332603 4.99 4.33 3.41     G8III 115 0
29 Kepler-411 Er* 19 10 25.3469947368 +49 31 23.712634632   13.70 12.55 12.26   K3V 129 0
30 * del Cyg B * 19 44 58.3835689212 +45 07 49.482245212   6.48 6.23     F1V 4 1
31 * del Cyg PM* 19 44 58.4769226339 +45 07 50.932673095 2.75 2.85 2.87 2.88 2.90 B9.5IV 303 0
32 * lam Cyg ** 20 47 24.53766 +36 29 26.5737 3.93 4.43 4.54 4.58 4.69 B5V 312 0
33 * tau Cyg dS* 21 14 47.49252 +38 02 43.1441 4.140 4.120 3.730 3.38 3.14 F2IV 287 0

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