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Catalogue XRT results for GRB 101017A

Data were analysed using HEASOFT version 6.32

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Summary Information

RA:19h 25m 32.49sLC breaks:4
Dec:-35° 08′ 42.4′′LC type:Oddball.
Err:1.6′′NH,intr.:8.56×1020 cm-2
Gal long:3.458RedshiftUnknown
Gal lat:-21.739Γ1.7
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Jump to: Light curve | Spectra | Compare to other bursts.

If you use any of these data, please cite Evans et al. (2009), which describes how these products were created (see the usage policy for more information).

Light curve

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This light curve comes from the light curve repository (if you use it, please cite Evans et al [2007, 2009]. Flares, marked by cross-hatched regions, are identified automatically, but may have been manually corrected. These are excluded from the fit. Any power-law breaks added to the fit must be required at the 4-σ level (according to an f-test) to be included in the best-fit. Details of all fits attempted are given below the plot. For more information see the light curve fitting documentation.

Fitted light curve of GRB 101017A

Fit Details

Nbreaksχ2dofCommentsImage
0421120Image of this fit
1321118Break required.

(1.08e-05 % probability of chance improvement)
Image of this fit
2232116Break required.

(6.29e-07 % probability of chance improvement)
Image of this fit
3204114Break significance <4-σ
(0.08 % probability of chance improvement)
Image of this fit
4175112Break required.

(2.35e-04 % probability of chance improvement).
This is the best fit.
Image of this fit
5171110Break significance <4-σ
(32.22 % probability of chance improvement)
Image of this fit

There are no flares ignored from this fit.

The best-fitting light curve has 4 breaks.

Click on the number of breaks in the table to the right to change which fit is plotted above and detailed below.

Currently showing the best fit.

α13.26 (+2.03, -0.84)
Tb,193 (+1, -5) s
α2-1.50 (+0.00, +0.83)
Tb,2104 (+2, -2) s
α32.20 (+0.10, -0.10)
Tb,3302 (+24, -60) s
α45 (+3, -2)
Tb,4426 (+85, -54) s
α51.462 (+0.102, -0.097)

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Spectra

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Spectra have been created for each power-law segment in the best fitting light curve (shown above). Times of flaring have not been removed, however this makes little difference to most spectra (see Fig 7/8c of Evans et al. 2009). For more information see the time-resolved spectroscopy documentation.

Jump to: phase1|phase2|phase3|phase4|phase5

phase1 spectrum (T0 + 87 to 93 s)

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Plots to download

WT mode spectrum of GRB 101017A

WT mode. Mean photon arrival: T0+90 s

NH (Galactic)1.19 × 1021 cm-2
NH (intrinsic)1.7 (+2.1, -1.6) × 1021 cm-2
z of absorber0
Photon index0.91 (+0.23, -0.22)
Flux (0.3-10 keV)
(Observed)
5.8 (+0.9, -0.8) × 10-9 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
6.2 (+0.6, -0.7) × 10-9 erg cm-2 s-1
Counts to flux (obs)6.78 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)7.29 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
218.85 (286)
Spectrum exposure6 s

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phase2 spectrum (T0 + 93 to 104 s)

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WT mode spectrum of GRB 101017A

WT mode. Mean photon arrival: T0+99 s

NH (Galactic)1.19 × 1021 cm-2
NH (intrinsic)4.6 (+2.5, -2.0) × 1021 cm-2
z of absorber0
Photon index1.00 (+0.20, -0.19)
Flux (0.3-10 keV)
(Observed)
6.6 (+0.7, -0.7) × 10-9 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
7.5 (+0.6, -0.6) × 10-9 erg cm-2 s-1
Counts to flux (obs)7.27 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)8.23 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
319.26 (429)
Spectrum exposure10 s

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phase3 spectrum (T0 + 104 to 301 s)

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WT and PC mode spectra of GRB 101017A

WT mode. Mean photon arrival: T0+163 s

NH (Galactic)1.19 × 1021 cm-2
NH (intrinsic)3.1 (+0.6, -0.5) × 1021 cm-2
z of absorber0
Photon index1.39 (+0.08, -0.08)
Flux (0.3-10 keV)
(Observed)
1.56 (+0.07, -0.07) × 10-9 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
1.89 (+0.07, -0.07) × 10-9 erg cm-2 s-1
Counts to flux (obs)5.58 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)6.76 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
653.58 (673)
Spectrum exposure193 s

PC mode. Mean photon arrival: T0+300 s

NH (Galactic)1.19 × 1021 cm-2
NH (intrinsic)5 (+10, -5) × 1021 cm-2
z of absorber0
Photon index3.1 (+1.3, -1.6)
Flux (0.3-10 keV)
(Observed)
9 (+9, -4) × 10-11 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
3.9 (+457.2, -1.8) × 10-10 erg cm-2 s-1
Counts to flux (obs)2.63 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)1.15 × 10-10 erg cm-2 ct-1
W-stat (dof)
What's this?
5.13 (7)
Spectrum exposure5 s

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phase4 spectrum (T0 + 304 to 425 s)

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PC mode spectrum of GRB 101017A

PC mode. Mean photon arrival: T0+349 s

NH (Galactic)1.19 × 1021 cm-2
NH (intrinsic)1.9 (+2.5, -1.9) × 1021 cm-2
z of absorber0
Photon index1.9 (+0.5, -0.5)
Flux (0.3-10 keV)
(Observed)
1.3 (+0.4, -0.3) × 10-10 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
1.8 (+0.6, -0.3) × 10-10 erg cm-2 s-1
Counts to flux (obs)4.09 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)5.66 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
67.19 (83)
Spectrum exposure122 s

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phase5 spectrum (T0 + 426 to 121143 s)

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Plots to download

PC mode spectrum of GRB 101017A

PC mode. Mean photon arrival: T0+7709 s

NH (Galactic)1.19 × 1021 cm-2
NH (intrinsic)1.8 (+1.9, -1.4) × 1021 cm-2
z of absorber0
Photon index1.8 (+0.3, -0.3)
Flux (0.3-10 keV)
(Observed)
7.0 (+1.4, -1.2) × 10-13 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
9.5 (+1.2, -1.3) × 10-13 erg cm-2 s-1
Counts to flux (obs)4.19 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)5.65 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
176.01 (184)
Spectrum exposure29.0 ks

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Comparison with other bursts

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Parameter distributions

The plots below show the probability density functions of the temporal and time-averaged spectral parameters for all GRBs, with the data for GRB 101017A shown on in colour. Click the images for larger versions.

For all plots, the solid vertical lines mark the values for this GRB, and the dashed lines the 1-σ uncertainties. For α and Tb, the colour changes for each phase. For the spectral parameters, the WT fits are shown in blue and the PC in red. These figures correspond to Figs. 5,6, 7a and 8a of Evans et al. (2009). See the PDF documentation for more information.

Temporal indicesBreak TimesNHSpectral indices
Comparison of decay indices Comparison of light curve break times Comparison of intrinsic column densities Comparison of spectral energy indices

Closure Relationships

The plots below show (α, β) scatter plots for each of the different types/phases of light curves (see light-curve types), since GRB 101017A is of type, "Oddball," which has no scatter plots of its own. GRB 101017A is shown in colour, with each light curve phase, or XRT mode marked by a different colour. α and β are the temporal and spectral energy power-law indices respectively. The shaded regions mark those allowed by the standard closure relationships. These figures correspond to Fig. 10 of Evans et al. (2009). See the closure relationship documentation for more information.

No break
Comparison of nobreak closures
One-break, steep first
Steep phase
One-break, steep first
Shallow phase
Comparison of One-break, steep first, steep phase closuresComparison of One-break, steep first, shallow phase closures
One-break, shallow first
Shallow phase
One-break, shallow first
Steep phase
Comparison of One-break, shallow first, shallow phase closuresComparison of One-break, shallow first, steep phase closures
Canonical
Steep phase
Canonical
Plateau
Canonical
'Normal'
Canonical
Post jet-break
Comparison of Canonical, steep phase closuresComparison of Canonical, plateau phase closuresComparison of Canonical, normal phase closuresComparison of Canonical, post jet-break phase closures

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