Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/134659
Title: Constraining very-high-energy and optical emission from FRB 121102 with the MAGIC telescopes
Author: Delfino, Manuel
Cortina, Juan
Hassan, Tarek
Gaug, Markus
Moreno, Victoria
Paredes i Poy, Josep Maria
Ribó Gomis, Marc
Torres Albà, Núria
MAGIC Collaboration
Keywords: Radiació
Raigs gamma
Astronomia de raigs gamma
Radiation
Gamma rays
Gamma ray astronomy
Issue Date: 1-Dec-2018
Publisher: Royal Astronomical Society
Abstract: Fast radio bursts (FRBs) are bright flashes observed typically at GHz frequencies with millisecond duration, whose origin is likely extragalactic. Their nature remains mysterious, motivating searches for counterparts at other wavelengths. FRB 121102 is so far the only source known to repeatedly emit FRBs and is associated with a host galaxy at redshift z ≃ 0.193.We conducted simultaneous observations of FRB 121102 with the Arecibo and MAGIC telescopes during several epochs in 2016-2017. This allowed searches for millisecond time-scale burst emission in very-high-energy (VHE) gamma-rays as well as the optical band. While a total of five FRBs were detected during these observations, no VHE emission was detected, neither of a persistent nature nor burst-like associated with the FRBs. The average integral flux upper limits above 100 GeV at 95 per cent confidence level are 6.6 × 10 -12 photons cm -2 s -1 (corresponding to luminosity LVHE ≲ 10 45 erg s -1 ) over the entire observation period, and 1.2 × 10 -7 photons cm -2 s -1 (LVHE ≳ 10 49 erg s -1 ) over the total duration of the five FRBs. We constrain the optical U-band flux to be below 8.6 mJy at 5σ level for 1-ms intervals around the FRB arrival times. A bright burst with U-band flux 29 mJy and duration ~12 ms was detected 4.3 s before the arrival of one FRB. However, the probability of spuriously detecting such a signal within the sampled time space is 1.5 per cent (2.2, post-trial), i.e. consistent with the expected background. We discuss the implications of the obtained upper limits for constraining FRB models.
Note: Reproducció del document publicat a: https://doi.org/10.1093/mnras/sty2422
It is part of: Monthly Notices of the Royal Astronomical Society, 2018, vol. 481, num. 2, p. 2479-2486
URI: http://hdl.handle.net/2445/134659
Related resource: https://doi.org/10.1093/mnras/sty2422
ISSN: 0035-8711
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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