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Table 5:

Results of SSC fits to the SED of H 2356-309.
  XMM1a XMM2a RXTE $^{\dagger}$ AH06c

$\delta$ 		18 18 18 18
B [G] 0.16 0.16 0.16 0.16
R [cm] $7.5 \times 10^{15}$ $7.5 \times 10^{15}$ $7.0 \times 10^{15}$ $3.4 \times 10^{15}$
K [cm-3] $8.0 \times 10^{4}$ $8.0 \times 10^{4}$ $2.0 \times 10^{4}$ $1.2 \times 10^{4}$
$\gamma_{\rm min}$ $1.0 \times 10^{3}$ $1.0 \times 10^{3}$ $1.0 \times 10^{3}$ $1.0 \times 10^{3}$
$\gamma_{\rm b}$ $1.0 \times 10^{5}$ $1.0 \times 10^{5}$ $2.5 \times 10^{5}$ $2.5 \times 10^{5}$
$\gamma_{\rm max}$ $3.0 \times 10^{6}$ $3.0 \times 10^{6}$ $3.0 \times 10^{6}$ $3.0 \times 10^{6}$
n1 2.3 2.3 2.0 2.0
n2 3.6 3.5 3.4 4.0

Notes. (a) The XMM1 and XMM2 results refer to the fits to the data from MJD 53 534 and 53 536, respectively. Using the XMM-Newton optical spectrum from MJD 53 536 instead of the average ROTSE-IIIc flux from 2004 for the RXTE campaign yields the same SSC fit parameters as shown in XMM2. (b) This is the result of the original SSC modeling of the RXTE campaign SED of H 2356-309 published in Aharonian et al. 2006b. The RXTE $^{\dagger}$results use the same multi-wavelength data as AH06 along with an improved calibration of the VHE data.


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