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Table A.2

Analysed MAGIC data sets and results using detection cuts to determine the significance and open cuts for the integral fluxes.

Data seta Obs. timeb t eff c S d F(>170 GeV)e
[MJD] [h] [10-12 ph cm-2 s-1]
All data 54 780.419 20.75 3.5 7.4 ± 2.1
Period 1 54 763.433 10.26 1.9 3.2 ± 2.9
Period 2 54 793.858 10.49 3.1 11.5 ± 2.9
21 Oct. 54 759.973 1.42 1.3 10.6 ± 8.0
22 Oct. 54 760.960 1.41 0.6 9.3 ± 7.8
23 Oct. 54 761.954 1.35 1.1 <17.4
24 Oct. 54 762.931 1.42 0.4 <12.5
25 Oct. 54 763.949 3.22 1.5 <15.6
26 Oct. 54 764.946 1.14 0.0 <19.5
28 Oct. 54 766.919 0.30 − 2.0 <1.7
17 Nov. 54 786.862 1.03 2.5 27.0 ± 9.9
18 Nov. 54 787.873 2.14 − 0.1 <19.7
19 Nov. 54 788.888 1.77 2.0 16.0 ± 7.2
24 Nov. 54 793.866 2.12 1.2 9.5 ± 6.6
25 Nov. 54 794.866 2.01 1.4 6.5 ± 6.4
28 Nov. 54 797.841 0.62 − 1.1 <16.5
01 Dec. 54 800.879 0.81 2.0 22.3 ± 10.0

Notes.

(a)

If dates are given, they correspond to the day following the observation night.

(b)

Arithmetic average of observation duration.

(c)

Effective observation time.

(d)

Significance of the signal calculated according to Li & Ma (1983) Eq. (17).

(e)

Measured integral flux. ULs are given with 95% c.l.. We recall that the fluxes and signal significances were determined using different cuts.

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