Table A.3.
AGILE Coverage and MCAL upper limits (ULs) during the R3 radio bursts.
| Burst | MCAL | MCAL | GRID | UL | UL |
|---|---|---|---|---|---|
| ID | FoV | D.A. | FoV | (3σ) | (sub-ms) |
| [erg cm−2] | [erg cm−2] | ||||
| SRT-P-01 | NO | NO | NO | earth occultation | |
| SRT-P-02 | NO | NO | NO | earth occultation | |
| SRT-P-03 | YES | NO | NO | — | 1.15×10−8 |
| SRT-P-04 | YES | NO | YES | — | 2.55×10−8 |
| SRT-P-05 | YES | NO | NO | — | 6.88×10−8 |
| SRT-P-06 | NO | NO | NO | earth occultation | |
| SRT-P-07 | NO | NO | NO | earth occultation | |
| SRT-P-08 | NO | NO | NO | earth occultation | |
| SRT-P-09 | YES | NO | NO | — | 6.88×10−8 |
| SRT-P-10 | YES | NO | NO | — | 6.88×10−8 |
| SRT-P-11 | YES | YES | NO | 1.07×10−6 | 1.03×10−7 |
| SRT-P-12 | NO | NO | NO | idle mode | |
| SRT-P-13 | YES | NO | NO | — | 1.83×10−8 |
| SRT-P-14 | YES | NO | NO | — | 3.60×10−8 |
| uGMRT-01 | YES | YES | NO | 1.03×10−6 | 1.00×10−7 |
| uGMRT-02 | NO | NO | NO | earth occultation | |
| uGMRT-03 | NO | NO | NO | earth occultation | |
| uGMRT-04 | NO | NO | NO | idle mode | |
| uGMRT-05 | NO | NO | NO | idle mode | |
| uGMRT-06 | YES | YES | NO | 1.09×10−7 | 1.06×10−8 |
| uGMRT-07 | YES | YES | NO | 2.36×10−7 | 2.29×10−8 |
Notes. The second and fourth columns report the presence and absence of the source in the FoV of the onboard detector, respectively. The third column reports the presence and absence of MCAL data acquisition. ULs (3σ) are evaluated on existing MCAL data acquisitions at the burst times and correspond to a fluence of 3σ above the background; ULs (sub-ms) are evaluated on the basis of the data acquisition (if present); otherwise, they refer to the UL fluences which would be required to issue a trigger with the onboard sub-ms MCAL trigger logic timescale (see Ursi et al. 2022). In presence of MCAL data acquisition, we show UL intervals obtained applying the spatial response matrix corresponding to source direction at burst times.
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