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Home All issues Volume 507 / No 1 (November III 2009) A&A, 507 1 (2009) 549-571 Full HTML
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Table 5:

Source fluxes [mCrab].
Object Name Flux [mCrab]a,b
  25-100 keV 100-200 keV 200-600 keV 600-1000 keV
  SPI ISGRI SPI(B08) SPI ISGRI SPI(B08) SPI ISGRI SPI(B08) SPI
Crab 1000.0 $\pm$ 2.0 1000.0 $\pm$ 2.0 1000.0 $\pm$ 2.0 1000.0 $\pm$ 3.4 1000.0 $\pm$ 3.5 1000.0 $\pm$ 3.7 1000.0 $\pm$ 11.8 1000.0 $\pm$ 18.6 1000.0 $\pm$ 8.3 1000.0 $\pm$ 43.2
Vela Pulsar 10.0 $\pm$ 0.4 7.2 $\pm$ 0.1 9.8 $\pm$ 0.7 11.6 $\pm$ 1.3 10.2 $\pm$ 0.9 12.6 $\pm$ 2.1 5.6 $\pm$ 5.3 0.0+19.0 13.9 $\pm$ 4.9 23.0 $\pm$ 18.5
NGC 4151 35.4 $\pm$ 2.4 32.7 $\pm$ 0.7 31.3 $\pm$ 2.1 43.8 $\pm$ 7.4 34.6 $\pm$ 2.5 22.9 $\pm$ 6.8 28.2 $\pm$ 36.4 0.0+132.5 46.9 $\pm$ 14.1 101.4 $\pm$ 111
NGC 4945 18.7 $\pm$ 1.1 16.4 $\pm$ 0.3 18.3 $\pm$ 1.1 21.4 $\pm$ 3.7 21.5 $\pm$ 1.2 14.3 $\pm$ 4.0 0.5 $\pm$ 27.1 0.0+53.2 20.2 $\pm$ 8.3 5.8 $\pm$ 53.8
Cen A 40.7 $\pm$ 1.1 36.0 $\pm$ 0.3 40.5 $\pm$ 1.3 59.7 $\pm$ 3.7 53.7 $\pm$ 1.2 56.9 $\pm$ 4.6 55.9 $\pm$ 20.7 87.7 $\pm$ 24.2 70.1 $\pm$ 9.8 12.9 $\pm$ 48.7
XTE J1550-564 36.1 $\pm$ 0.6 41.6 $\pm$ 0.3 23.5 $\pm$ 0.7 55.2 $\pm$ 1.7 70.2 $\pm$ 0.9 30.2 $\pm$ 2.5 48.8 $\pm$ 8.4 51.5 $\pm$ 12.1 18.8 $\pm$ 5.5 6.7 $\pm$ 24.4
4U 1630-47 36.5 $\pm$ 1.6 1.8 $\pm$ 0.2c 30.5 $\pm$ 1.3 19.7 $\pm$ 6.0 0.8 $\pm$ 0.3c 21.7 $\pm$ 2.4 2.2 $\pm$ 23.3 19.9 $\pm$ 13.2c 21.4 $\pm$ 5.3 0.0+164.2
Swift J1656.3-3302 3.7 $\pm$ 2.2 - d 6.0 $\pm$ 1.1 8.0 $\pm$ 3.4 - d 5.0 $\pm$ 1.9 15.2 $\pm$ 7.8 - d 17.6 $\pm$ 4.0 24.6 $\pm$ 12.9
OAO 1657-415 66.6 $\pm$ 0.6 51.5 $\pm$ 1.3 51.3 $\pm$ 0.7 15.0 $\pm$ 1.3 7.6 $\pm$ 0.6 10.3 $\pm$ 2.2 15.0 $\pm$ 8.0 0.0+24.9 13.8 $\pm$ 4.8 2.3 $\pm$ 26.6
GX 339-4 34.1 $\pm$ 0.5 11.5 $\pm$ 0.2 38.4 $\pm$ 1.4 32.6 $\pm$ 1.4 12.1 $\pm$ 0.5 35.6 $\pm$ 2.4 30.1 $\pm$ 13.8 0.0+30.3 30.0 $\pm$ 5.2 66.1 $\pm$ 27.4
4U 1700-377 171.7 $\pm$ 0.8 162.3 $\pm$ 3.6 146.3 $\pm$ 1.4 36.0 $\pm$ 1.0 40.9 $\pm$ 1.6 35.5 $\pm$ 2.2 13.6 $\pm$ 8.1 23.4 $\pm$ 17.2 6.4 $\pm$ 4.8 0.0+62.7
IGR J17091-3624 5.2 $\pm$ 0.8 6.1 $\pm$ 0.1 8.9 $\pm$ 0.6 7.2 $\pm$ 5.0 6.3 $\pm$ 0.3 5.6 $\pm$ 2.0 18.5 $\pm$ 8.8 2.7 $\pm$ 13.4 9.8 $\pm$ 4.4 8.7 $\pm$ 19.6
GX 354-0 34.2 $\pm$ 0.5 23.4 $\pm$ 0.1 24.4 $\pm$ 0.5 10.5 $\pm$ 1.1 5.4 $\pm$ 0.2 7.6 $\pm$ 1.8 0.7 $\pm$ 10.0 1.0 $\pm$ 10.5 7.9 $\pm$ 4.1 7.4 $\pm$ 21.4
1E 1740.7-2942 52.8 $\pm$ 0.9 32.7 $\pm$ 0.1 51.1 $\pm$ 1.2 43.0 $\pm$ 2.3 35.0 $\pm$ 0.3 48.3 $\pm$ 1.6 18.5 $\pm$ 10.9 22.1 $\pm$ 6.1 39.2 $\pm$ 3.6 7.8 $\pm$ 34.9
IGR J17464-3213 13.3 $\pm$ 0.6 15.1 $\pm$ 0.1 15.6 $\pm$ 0.7 6.9 $\pm$ 1.1 9.9 $\pm$ 0.2 11.2 $\pm$ 1.6 2.2 $\pm$ 4.4 6.8 $\pm$ 6.3 9.9 $\pm$ 3.6 41.6 $\pm$ 23.1
GRS 1758-258 68.8 $\pm$ 0.7 66.6 $\pm$ 0.2 70.8 $\pm$ 0.9 84.6 $\pm$ 2.1 82.2 $\pm$ 0.5 83.4 $\pm$ 1.6 41.1 $\pm$ 7.2 49.3 $\pm$ 6.0 47.4 $\pm$ 3.6 51.2 $\pm$ 18.0
Ginga 1826-24 75.8 $\pm$ 0.5 73.1 $\pm$ 0.3 74.6 $\pm$ 0.5 30.3 $\pm$ 0.9 34.2 $\pm$ 0.4 33.6 $\pm$ 1.9 18.4 $\pm$ 5.7 0.0+19.8 24.5 $\pm$ 3.9 38.3 $\pm$ 22.4
GRS 1915+105 189.1 $\pm$ 0.8 187.8 $\pm$ 0.5 150.1 $\pm$ 0.9 73.2 $\pm$ 2.2 60.5 $\pm$ 0.5 61.8 $\pm$ 2.3 38.8 $\pm$ 8.7 40.9 $\pm$ 10.2 38.6 $\pm$ 5.2 53.9 $\pm$ 27.2
Cyg X-1 841.0 $\pm$ 1.5 871.6 $\pm$ 1.7 843.8 $\pm$ 1.0 873.7 $\pm$ 3.1 907.6 $\pm$ 3.1 769.9 $\pm$ 3.1 575.5 $\pm$ 9.8 581.3 $\pm$ 16.1 500.6 $\pm$ 6.9 386.4 $\pm$ 37.3
Cyg X-3 117.7 $\pm$ 0.6 111.7 $\pm$ 0.6 101.2 $\pm$ 0.8 34.9 $\pm$ 1.4 25.3 $\pm$ 0.5 25.0 $\pm$ 2.9 26.4 $\pm$ 7.6 21.0 $\pm$ 21.8 14.8 $\pm$ 6.2 52.6 $\pm$ 31.0
Estim. Syst. Errore -0.9 -0.1 - -0.1 -0.4 - -0.1 -1.2 - -0.1

a For the columns ``SPI'' and ``ISGRI'' fluxes are expressed as fractions of the Crab fluxes for the individual instrument given in Table 4. In the columns ``SPI (B08)'' we give the fluxes obtained by Bouchet et al. (2008) (B08) for the available energy ranges (see B08 for their definition of the unit ``mCrab'').
b The statistical errors shown in this table do not take into account the uncertainty of the Crab flux on which the flux values are normalised.
c Spectrum very probably flawed by source contamination from IGR J16358-472; therefore not included in Fig. 23.
d ISGRI spectral fit failed, see Sect. 4.8; therefore not included in Fig. 23.
e See Sect. 4.21.


Source LaTeX | All tables | In the text

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