2021ApJ...918...66A


Query : 2021ApJ...918...66A

2021ApJ...918...66A - Astrophys. J., 918, 66-66 (2021/September-2)

An archival search for neutron-star mergers in gravitational waves and very-high-energy gamma rays.

ADAMS C.B., BENBOW W., BRILL A., BUCKLEY J.H., CAPASSO M., CHRISTIANSEN J.L., CHROMEY A.J., DANIEL M.K., ERRANDO M., FALCONE A., FARRELL K.A., FENG Q., FINLEY J.P., FORTSON L., FURNISS A., GENT A., GIURI C., HANNA D., HASSAN T., HERVET O., HOLDER J., HUGHES G., HUMENSKY T.B., JIN W., KAARET P., KERTZMAN M., KIEDA D., KUMAR S., LANG M.J., LUNDY M., MAIER G., McGRATH C.E., MORIARTY P., MUKHERJEE R., NIETO D., NIEVAS-ROSILLO M., O'BRIEN S., ONG R.A., OTTE A.N., PARK N., PATEL S., PFRANG K., POHL M., PRADO R.R., PUESCHEL E., QUINN J., RAGAN K., REYNOLDS P.T., RIBEIRO D., ROACHE E., RYAN J.L., SANTANDER M., SEMBROSKI G.H., SHANG R., WEINSTEIN A., WILLIAMS D.A., WILLIAMSON T.J. (The VERITAS Collaboration), BARTOS I., CORLEY K.R., MARKA S., MARKA Z., VESKE D. (The Columbia Experimental Gravity Group (GECo)

Abstract (from CDS):

The recent discovery of electromagnetic signals in coincidence with neutron-star mergers has solidified the importance of multimessenger campaigns in studying the most energetic astrophysical events. Pioneering multimessenger observatories, such as LIGO/Virgo and IceCube, record many candidate signals below the detection significance threshold. These sub-threshold event candidates are promising targets for multimessenger studies, as the information provided by them may, when combined with contemporaneous gamma-ray observations, lead to significant detections. Here we describe a new method that uses such candidates to search for transient events using archival very-high-energy gamma-ray data from imaging atmospheric Cherenkov telescopes (IACTs). We demonstrate the application of this method to sub-threshold binary neutron star (BNS) merger candidates identified in Advanced LIGO's first observing run. We identify eight hours of archival VERITAS observations coincident with seven BNS merger candidates and search them for TeV emission. No gamma-ray emission is detected; we calculate upper limits on the integral flux and compare them to a short gamma-ray burst model. We anticipate this search method to serve as a starting point for IACT searches with future LIGO/Virgo data releases as well as in other sub-threshold studies for multimessenger transients, such as IceCube neutrinos. Furthermore, it can be deployed immediately with other current-generation IACTs, and has the potential for real-time use that places a minimal burden on experimental operations. Lastly, this method may serve as a pilot for studies with the Cherenkov Telescope Array, which has the potential to observe even larger fields of view in its divergent pointing mode.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Gamma-ray transient sources - Gamma-ray astronomy - Gamma-ray bursts - Stellar mergers - Gamma-ray bursters - Gamma-ray observatories - Gamma-ray telescopes - Gamma-rays

Simbad objects: 13

goto Full paper

goto View the references in ADS

Number of rows : 13
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 3C 66A BLL 02 22 39.6114771888 +43 02 07.799534304   15.71 15.21 14.5   ~ 942 2
2 2FHL J0245.6+6605 gam 02 45 37.6 +66 05 42           ~ 2 0
3 PSR B0355+54 Psr 03 58 53.7165 +54 13 13.727           ~ 465 1
4 SNR G150.3+04.5 SNR 04 26.5 +54 38           ~ 49 0
5 PMN J0509+0541 BLL 05 09 25.9644373872 +05 41 35.333820420 15.32 14.95 14.78 15.12   ~ 589 2
6 RX J0521.7+2112 BLL 05 21 45.9657388992 +21 12 51.452786736           ~ 162 1
7 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
8 RX J0809.8+5218 BLL 08 09 49.1868285744 +52 18 58.249938744   16.11 15.59 14.6   ~ 302 1
9 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
10 QSO B1959+650 BLL 19 59 59.8520303688 +65 08 54.652536492     12.8 11.21   ~ 699 2
11 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
12 SN 2014C SN* 22 37 05.60 +34 24 31.9           SNIb 167 1
13 GRB 190425 GWE ~ ~           ~ 438 0

To bookmark this query, right click on this link: simbad:objects in 2021ApJ...918...66A and select 'bookmark this link' or equivalent in the popup menu