Skip banner and navigation tools.

 |  site map

Swift-XRT spectra of GRB 080604

Last updated after receiving ObsID 00313116003, version 17

Data were analysed using HEASOFT version 6.32

About these products.

Get another burst.

Add time-sliced spectrum.

The spectral fits assume a redshift: 1.42 (GCN 7818)

Jump to: Time-averaged|Late Time


Time-averaged spectrum (T0 + 125 to 40235 s)

Download spectral files for Time-averaged spectrum.

Plots to download

WT and PC mode spectra of Time-averaged

WT mode. Mean photon arrival: T0+211 s

NH (Galactic)4.46 × 1020 cm-2
NH (intrinsic)0 (+4.29 × 1020, -0) cm-2
z of absorber1.42
Photon index2.01 (+0.07, -0.06)
Flux (0.3-10 keV)
(Observed)
2.65 (+0.14, -0.11) × 10-10 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
2.97 (+0.13, -0.12) × 10-10 erg cm-2 s-1
Counts to flux (obs)3.13 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)3.51 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
377.25 (437)
Spectrum exposure256 s

PC mode. Mean photon arrival: T0+3740 s

NH (Galactic)4.46 × 1020 cm-2
NH (intrinsic)0 (+2.63 × 1021, -0) cm-2
z of absorber1.42
Photon index1.572 (+0.178, -0.099)
Flux (0.3-10 keV)
(Observed)
1.90 (+0.19, -0.23) × 10-12 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
2.01 (+0.21, -0.21) × 10-12 erg cm-2 s-1
Counts to flux (obs)4.13 × 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?
213.04 (248)
Spectrum exposure16.5 ks

[Back to top]

Late Time spectrum (T0 + 4981 to 40235 s)

Download spectral files for Late Time spectrum.

Plots to download

PC mode spectrum of Late Time

PC mode. Mean photon arrival: T0+22956 s

NH (Galactic)4.46 × 1020 cm-2
NH (intrinsic)2.8 (+9.6, -2.8) × 1021 cm-2
z of absorber1.42
Photon index2.1 (+0.6, -0.5)
Flux (0.3-10 keV)
(Observed)
1.6 (+0.7, -0.5) × 10-13 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
2.0 (+0.6, -0.5) × 10-13 erg cm-2 s-1
Counts to flux (obs)3.17 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)3.85 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
48.70 (47)
Spectrum exposure15.2 ks

[Back to top]