2020AJ....160...29S


Query : 2020AJ....160...29S

2020AJ....160...29S - Astron. J., 160, 29-29 (2020/July-0)

The Breakthrough Listen search for intelligent life: a 3.95-8.00 GHz search for radio technosignatures in the restricted Earth Transit Zone.

SHEIKH S.Z., SIEMION A., ENRIQUEZ J.E., PRICE D.C., ISAACSON H., LEBOFSKY M., GAJJAR V. and KALAS P.

Abstract (from CDS):

We report on a search for artificial narrowband signals of 20 stars within the restricted Earth Transit Zone (rETZ) as a part of the ten-year Breakthrough Listen (BL) search for extraterrestrial intelligence (ETI). The rETZ is the region of the sky from which an observer would see Earth transit the Sun with an impact parameter of less than 0.5. This region of the sky is geometrically unique, providing a potential way for an ETI to discover the solar system. The targets were nearby (7-143 pc) and the search covered an electromagnetic frequency range of 3.95-8.00 GHz. We used the Robert C. Byrd Green Bank Telescope to perform these observations with the standard BL data recorder. We searched these data for artificial narrowband (∼Hz) signals with Doppler drift rates of ±20 Hz s–1. We find no evidence for radio technosignatures from ETI in our observations. The observing campaign would have allowed for detections of emissions that were 10–3 to 0.88 times as powerful as the signaling capability of the Arecibo radar transmitter. We conclude that at least 0.6% of the systems in the rETZ within 150 pc do not possess the type of transmitters searched in this survey. To our knowledge, this is the first targeted search for ETI of the rETZ. All data used in this paper are publicly available via the BL Public Data Archive (http://seti.berkeley.edu/bldr2).

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

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

Simbad objects: 52

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Number of rows : 52
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 HD 224700 * 00 00 00.2096521080 +01 05 20.402893572   9.55 9.08     F3V 18 0
2 PSR B0031-07 Psr 00 34 08.9100 -07 21 56.000           ~ 350 0
3 BD+03 108 * 00 48 21.2945993112 +04 08 35.747458548   10.16 9.84     F0 15 0
4 HD 4628 PM* 00 48 22.9759750919 +05 16 50.209484954 7.22 6.64 5.74 4.99 4.52 K2.5V 544 0
5 StKM 1-87 * 00 52 09.3630279744 +06 48 10.847755512   13.265 13.809 11.344   K7V 20 0
6 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
7 G 3-38 PM* 02 03 33.0292200200 +12 35 04.956484842   12.88 13.475 11.057   K7V 27 0
8 HD 12899 Pu* 02 06 41.5936978248 +14 35 01.592391084 8.590 8.510 8.190     F0 25 0
9 NAME W 3 OH HII 02 27 04.1 +61 52 22           ~ 1064 2
10 HD 20477 ** 03 18 19.9834838544 +18 10 17.842792656 8.330 8.160 7.540     G0 43 0
11 BD+18 487 PM* 03 27 55.3048893864 +18 52 56.405603496   9.05 8.48     G0 20 0
12 HD 284145 PM* 04 04 56.5261391592 +20 51 23.322900564   9.82 8.98     G0 15 0
13 HD 26037 * 04 08 14.2214113368 +22 01 16.332928932   9.38 8.88     F5 13 0
14 NAME Per B SyG 04 37 04.37535450 +29 40 13.8179631   21.7       ~ 533 2
15 SH 2-231 Y*O 05 39 13.2 +35 45 48           ~ 135 0
16 SH 2-235 HII 05 41.1 +35 50           ~ 236 0
17 HD 51295 PM* 06 57 46.3368449928 +22 53 33.185616900       7.3   G0 32 0
18 HD 53532 PM* 07 06 16.8020555832 +22 41 00.552345288   8.95 8.27     G0V 66 0
19 BD+18 2056 PM* 08 50 36.8683683576 +17 41 21.546350448       8.7   K0 27 0
20 BD+20 2233 PM* 08 54 00.5026177848 +20 13 49.427873688   9.08 8.61     F7V 29 0
21 HD 81563 PM* 09 26 49.4044938288 +14 55 40.742328108   8.74 8.27     G0 28 0
22 BD+18 2213 PM* 09 30 50.1022718668 +18 15 08.192628847   11.15   9.5   K8 28 0
23 PSR B0950+08 Psr 09 53 09.31210 +07 55 36.9000           ~ 806 2
24 PSR B1133+16 Psr 11 36 03.09460 +15 51 15.9000           ~ 715 0
25 HD 108754 SB* 12 29 42.7349338841 -03 19 58.694940030 9.92 9.74 9.03     G6V 138 0
26 HD 109376 PM* 12 34 13.2718256136 -03 43 16.179678948   9.29 8.57     F5V 21 0
27 HD 109969 PM* 12 38 56.3194700448 -00 51 14.890867200   7.23 7.18     A0V 23 0
28 HD 115153 SB* 13 15 30.7679504352 -08 03 18.498504204   8.77 8.06     G5V 39 0
29 HD 117004 PM* 13 27 29.6588225592 -09 11 33.740395224   10.29 9.48     G5V 15 0
30 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
31 HD 121865 RG* 13 58 26.8406158824 -12 03 33.419301120   8.03 7.05     K0III/IV 31 0
32 HD 123453 ** 14 08 04.09936 -12 55 42.1319           G8/K0(V)+A/F 35 0
33 PSR B1642-03 Psr 16 45 02.0330 -03 17 57.200           ~ 394 0
34 HD 152956 * 16 57 30.2350643808 -22 38 37.141430280   10.37 9.78     G0V 14 0
35 CD-22 11823 PM* 17 05 59.6231095525 -22 51 24.346265942   10.89 10.00     K2 20 0
36 4C -00.67 Sy2 17 20 28.1680537512 -00 58 46.582453920   15.36       ~ 345 1
37 HD 165204 PM* 18 05 46.7342405184 -23 31 03.825836364   9.82 9.05     G6/8V 51 0
38 HD 166052 * 18 09 44.4433591848 -18 50 39.843012984   7.71 7.65     B3IV 24 0
39 GAL 035.03+00.35 cor 18 54 00.60 +02 01 19.3           ~ 48 0
40 HD 174995 ** 18 54 12.7896190588 -22 54 24.959922318   9.40 8.62 9.13   G9 27 0
41 LP 811-17 ** 18 57 32.65010 -19 02 46.8659 13.258 12.087 10.637 9.732 9.117 K9Vk: 19 0
42 IRAS 19050+0806 Y*O 19 07 28.1 +08 10 53           ~ 5 0
43 CD-22 13916 PM* 19 24 34.2352422838 -22 03 43.832212442   12.262 10.899 10.422   K8Vk: 55 0
44 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 801 0
45 V* V4333 Sgr dS* 19 36 26.0756222280 -18 51 10.518287148   6.39 6.12     F0V 42 0
46 DR 21 SFR 20 39 01.6 +42 19 38           O4.5 1121 0
47 NGC 7027 PN 21 07 01.571952 +42 14 10.47120   10.358 8.831 10.157   ~ 2541 1
48 PSR B2145-07.8 Psr 21 45 50.45590 -07 50 18.5900           ~ 336 0
49 BD-11 5779 PM* 22 12 50.8212760972 -10 55 31.349021617   11.634 10.689 10.477   K2V 38 0
50 HD 213677 PM* 22 33 21.5273902045 -09 03 48.798530824   9.30 8.71     G3V 36 0
51 NGC 7538 OpC 23 13 37 +61 30.0           ~ 920 1
52 HD 224448 * 23 58 04.5371997336 -00 07 41.494949976   9.61 9.01     G5V 30 0

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