2023AJ....165..132L


Query : 2023AJ....165..132L

2023AJ....165..132L - Astron. J., 165, 132 (2023/March-0)

Multibeam Blind Search of Targeted SETI Observations toward 33 Exoplanet Systems with FAST.

LUAN X.-H., TAO Z.-Z., ZHAO H.-C., HUANG B.-L., LI S.-Y., LIU C., WANG H.-F., LIU W.-F., ZHANG T.-J., GAJJAR V. and WERTHIMER D.

Abstract (from CDS):

The search for extraterrestrial intelligence (SETI) is to search for technosignatures associated with extraterrestrial life, such as engineered radio signals. In this paper, we apply the multibeam coincidence matching (MBCM) strategy, and propose a new search mode based on the MBCM which we call the MBCM blind search mode. In our recent targeted SETI research, 33 exoplanet systems are observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). With this blind search mode, we search for narrowband drifting signals across 1.05-1.45 GHz in two orthogonal linear polarization directions separately. There are two special signals, one of which can only be detected by the blind search mode while the other can be found by both blind and targeted search modes. This result reveals huge advantages of the new blind search mode. However, we eliminate the possibility of the special signals being ETI signals based on much evidence, such as the polarization, drift, frequency, and beam coverage characteristics. Our observations achieve an unprecedented sensitivity and our work provides a deeper understanding to the polarization analysis of extraterrestrial signals.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Astrobiology - Search for extraterrestrial intelligence - Technosignatures - Exoplanets

Simbad objects: 15

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Number of rows : 15
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 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
3 BD+47 612 PM* 02 22 14.6437562448 +47 52 48.104862600   10.85   9.104   M0V 176 0
4 HD 30562 PM* 04 48 36.3850851388 -05 40 26.557737782   6.40 5.77     G2IV 281 1
5 LP 656-38 PM* 05 01 57.4261317472 -06 56 46.376281497   13.92 12.196 11.791 9.175 M4.0Ve 188 0
6 HD 69830 PM* 08 18 23.9469682407 -12 37 55.817187530   6.74 5.95     G8:V 587 1
7 HD 82943 PM* 09 34 50.7353072232 -12 07 46.369202196   7.17 6.53     F9VFe+0.5 498 2
8 * 38 Vir ** 12 53 11.1567755256 -03 33 11.151261180   6.61 6.11     F6V 107 0
9 BD-12 4523 BY* 16 30 18.0583947383 -12 39 45.321217732 12.829 11.638 10.072 8.917 7.421 M3V 365 0
10 Kepler-438 Er* 18 46 34.9967842656 +41 57 03.934427796           M1V 45 0
11 TYC 472-734-1 * 19 16 33.3150403896 +05 06 08.332049880   12.48 12.60     ~ 1 0
12 ATO J289.1824+05.1208 LP? 19 16 43.7972041454 +05 07 15.322868575   16.451 14.064 13.384   ~ 3 0
13 HD 180617 PM* 19 16 55.2565688720 +05 10 08.040554168 11.768 10.63 9.115 8.076 6.782 M3-V 475 0
14 HD 197037 PM* 20 39 32.9599353024 +42 14 54.778250868       6.61   G0 81 1
15 HD 210277 PM* 22 09 29.8657847411 -07 32 55.162082226   8.85 8.57 7.36   G8V 366 1

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