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Home All issues Volume 495 / No 3 (March I 2009) A&A, 495 3 (2009) 899-900 Full HTML
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Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361:20077899]

 

 

Table 1:

Best-fit parameters from the fits to the spectra of Elias 29, during 6 different time intervals (PN data only), using an absorbed 1T thermal model.
Time interval $N({\rm H})$ kT Z $E\!M$ $\chi^2$/d.o.f. P $F_{\rm X}$
  N22 keV $Z_{\odot}$ $E\!M_{53}$     F-13
seg1 5.7 $\pm$ 0.7 4.6 $\pm$ 0.9 1.0 $\pm$ 0.3 0.7 $\pm$ 0.3 1.0 0.6 1.8
flare 9.5 $\pm$ 2.0 4.1 $\pm$ 1.5 0.9 $\pm$ 0.3 4.5 $\pm$ 3.4 0.9 0.5 7.5
seg2 8.1 $\pm$ 1.3 3.1 $\pm$ 0.8 1.0 $\pm$ 0.3 0.7 $\pm$ 0.5 1.5 0.0 1.1
seg3 6.6 $\pm$ 0.8 3.4 $\pm$ 0.7 0.7 $\pm$ 0.2 0.8 $\pm$ 0.4 1.0 0.5 1.3
seg4 7.7 $\pm$ 0.6 3.7 $\pm$ 0.5 0.7 $\pm$ 0.1 1.7 $\pm$ 0.5 1.4 0.0 2.7
seg5 4.9 $\pm$ 0.4 4.7 $\pm$ 0.8 0.6 $\pm$ 0.1 1.1 $\pm$ 0.3 1.3 0.1 2.5
Note: units are $N_{22} = 10^{22}~{\rm cm^{-2}}$, $E\!M_{53} = 10^{53}$ cm-3, and F-13= 10-13 erg cm-2 s-1. The spectral fits were carried out in the energy range 1.0-9.0 keV. Flux values refer to energy range 1.0-7.5 keV. The error bars are at 1$\sigma$. Reduced $\chi^2$ and null-hypothesis probability (P) for the fits are also given.


Source LaTeX | All tables | In the text

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