2024RAA....24f5020W


Query : 2024RAA....24f5020W

2024RAA....24f5020W - Research in Astron. and astroph., 24, part no 6, 5020 (2024/June-0)

The Influence of the Sun and Moon on the Observation of Very High Energy Gamma-ray Sources Using EAS Arrays.

WEN T., CHEN S. and DAI B.

Abstract (from CDS):

With great advance of ground-based extensive air shower arrays, such as LHAASO and HAWC, many very high energy (VHE) gamma-ray sources have been discovered and are being monitored regardless of the day and the night. Hence, the Sun and Moon would have some impacts on the observation of gamma-ray sources, which have not been taken into account in previous analysis. In this paper, the influence of the Sun and Moon on the observation of very high energy gamma-ray sources when they are near the line of sight of the Sun or Moon is estimated. The tracks of all the known VHE sources are scanned and several VHE sources are found to be very close to the line of sight of the Sun or Moon during some period. The absorption of very high energy gamma rays by sunlight is estimated with detailed method and some useful conclusions are achieved. The main influence is the block of the Sun and Moon on gamma rays and the shadow on the cosmic ray background. The influence is investigated considering the detector angular resolution and some strategies on data analysis are proposed to avoid the underestimation of the gamma-ray emission.

Abstract Copyright: © 2024. National Astronomical Observatories

Journal keyword(s): astroparticle physics - Sun: general - methods: observational - Sun: UV radiation

Simbad objects: 20

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Number of rows : 20
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 GRB 180720B gB 00 02 06.99 -02 55 07.8           ~ 215 0
2 RX J0319.8+1845 BLL 03 19 51.8082475320 +18 45 34.562475432           ~ 223 1
3 RX J0521.7+2112 BLL 05 21 45.9657388992 +21 12 51.452786736           ~ 162 1
4 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
5 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
6 HAWC J0543+233 gam 05 43.1 +23 24           ~ 9 0
7 IC 443 SNR 06 17 00.0000000 +22 34 11.998901           ~ 1314 1
8 RX J0650.7+2502 BLL 06 50 46.4900658984 +25 02 59.625654828 16.17 15.97 15.79 16.3   ~ 175 2
9 PG 0851+202 BLL 08 54 48.8749846272 +20 06 30.639583620   15.649 15.146 15.446   ~ 2513 1
10 3C 279 Bla 12 56 11.16657958 -05 47 21.5251510   18.01 17.75 15.87   ~ 3205 2
11 2HWC J1309-054 gam 13 09.2 -05 29           ~ 5 0
12 NAME Kepler's SN SNR 17 30 40.51 -21 29 14.4           ~ 851 3
13 SNR G004.5+06.2 SNR 17 33.4 -21 34           ~ 22 0
14 Cl Terzan 5 Cl* 17 48 05.00 -24 46 48.0           ~ 948 1
15 HESS J1800-240B gam 17 57 11 -24 05.5           ~ 30 0
16 HESS J1800-240C gam 17 58 52 -24 03.1           ~ 22 0
17 SNR G006.4-00.1 SNR 18 00 31.2011719 -23 25 48.001099           ~ 782 1
18 4FGL J1801.8-2358 gam 18 01 49.1 -23 58 58           ~ 33 0
19 1AGLR J1807-2103 gam 18 03 52.1 -21 10 54           ~ 79 0
20 Fermi J1808.2-2029 gam 18 08 00.0 -20 24 00           ~ 20 0

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