Skip banner and navigation tools.

 |  site map

Catalogue XRT results for GRB 091127

Data were analysed using HEASOFT version 6.35.2

About these products.

Back to list of GRBs.

Summary Information

RA:02h 26m 19.87sLC breaks:3
Dec:-18° 57′ 09.4′′LC type:Canonical.
Err:1.4′′NH,intr.:1.05×1021 cm-2
Gal long:197.398Redshift0.49
Gal lat:-66.738Γ1.7
| |

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

Hide the light curve section.

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 091127

Fit Details

Nbreaksχ2dofCommentsImage
0587203Image of this fit
1383201Break required.

(2.13e-17 % probability of chance improvement)
Image of this fit
2240199Break required.

(6.43e-19 % probability of chance improvement)
Image of this fit
3179197Break required.

(2.99e-11 % probability of chance improvement).
This is the best fit.
Image of this fit
4177195Break significance <4-σ
(45.54 % probability of chance improvement)
Image of this fit
5176193Break significance <4-σ
(48.61 % probability of chance improvement)
Image of this fit

There are 1 flares excluded from the fit:

  • 2.06×104—3.81×105 s

The best-fitting light curve has 3 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.

α10.74 (+0.22, -0.20)
Tb,15445 (+69, -114) s
α28.00 (+0.00, -3.90)
Tb,28241 (+5.08 × 104, -652) s
α30.73 (+0.10, -0.34)
Tb,35.7 (+2.2, -1.3) × 105 s
α41.59 (+0.23, -0.13)

[Back to top]


Spectra

Hide the spectrum section.

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

phase1 spectrum (T0 + 3218 to 3825 s)

Download spectral files for phase1 spectrum.

Plots to download

WT mode spectrum of GRB 091127

WT mode. Mean photon arrival: T0+3514 s

NH (Galactic)3.11 × 1020 cm-2
NH (intrinsic)7 (+3, -3) × 1020 cm-2
z of absorber0.49
Photon index1.77 (+0.06, -0.06)
Flux (0.3-10 keV)
(Observed)
3.00 (+0.12, -0.11) × 10-10 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
3.33 (+0.10, -0.10) × 10-10 erg cm-2 s-1
Counts to flux (obs)3.63 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)4.03 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
516.32 (592)
Spectrum exposure607 s

[Back to top]


phase2 spectrum (T0 + 5786 to 5818 s)

Download spectral files for phase2 spectrum.

Plots to download


[Back to top]


phase3 spectrum (T0 + 9053 to 558847 s)

Download spectral files for phase3 spectrum.

Plots to download

PC mode spectrum of GRB 091127

PC mode. Mean photon arrival: T0+82209 s

NH (Galactic)3.11 × 1020 cm-2
NH (intrinsic)1.0 (+0.4, -0.4) × 1021 cm-2
z of absorber0.49
Photon index1.66 (+0.06, -0.06)
Flux (0.3-10 keV)
(Observed)
5.33 (+0.23, -0.22) × 10-12 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
5.89 (+0.21, -0.20) × 10-12 erg cm-2 s-1
Counts to flux (obs)3.98 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)4.39 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
539.46 (577)
Spectrum exposure45.8 ks

[Back to top]


phase4 spectrum (T0 + 575729 to 16849147 s)

Download spectral files for phase4 spectrum.

Plots to download

PC mode spectrum of GRB 091127

PC mode. Mean photon arrival: T0+1499800 s

NH (Galactic)3.11 × 1020 cm-2
NH (intrinsic)1.1 (+1.3, -1.1) × 1021 cm-2
z of absorber0.49
Photon index1.62 (+0.19, -0.18)
Flux (0.3-10 keV)
(Observed)
6.6 (+0.9, -0.8) × 10-14 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
7.3 (+0.8, -0.7) × 10-14 erg cm-2 s-1
Counts to flux (obs)4.15 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)4.57 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
236.73 (279)
Spectrum exposure427.3 ks

[Back to top]



Comparison with other bursts

Hide the comparison section.

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 091127 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 phase of all Canonical light curves. GRB 091127 is shown in colour; where multiple points appear in a given phase (e.g. WT and PC mode spectra for that phase), the different colours refer to different spectra. 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.

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

[Back to top]