Skip banner and navigation tools.

 |  site map

Swift-XRT spectra of GRB 210517A

Last updated after receiving ObsID 01048783003, version 6

Data were analysed using HEASOFT version 6.32

About these products.

Get another burst.

Add time-sliced spectrum.

The spectral fits assume a redshift: 2.486 (GCN 30037)

Jump to: Time-averaged|Late Time


Time-averaged spectrum (T0 + 70 to 40648 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+74 s

NH (Galactic)1.30 × 1020 cm-2
NH (intrinsic)0 (+1.27 × 1022, -0) cm-2
z of absorber2.486
Photon index3.02 (+13.62, -0.82)
Flux (0.3-10 keV)
(Observed)
5.4 (+2.8, -2.1) × 10-11 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
5.9 (+41.0, -2.5) × 10-11 erg cm-2 s-1
Counts to flux (obs)2.24 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)2.46 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
15.20 (16)
Spectrum exposure12 s

PC mode. Mean photon arrival: T0+3674 s

NH (Galactic)1.30 × 1020 cm-2
NH (intrinsic)2.6 (+7.1, -2.6) × 1021 cm-2
z of absorber2.486
Photon index1.72 (+0.18, -0.16)
Flux (0.3-10 keV)
(Observed)
2.8 (+0.4, -0.3) × 10-12 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
3.0 (+0.3, -0.3) × 10-12 erg cm-2 s-1
Counts to flux (obs)3.71 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)3.90 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
174.60 (225)
Spectrum exposure7.7 ks

[Back to top]

Late Time spectrum (T0 + 4642 to 40648 s)

Download spectral files for Late Time spectrum.

Plots to download

PC mode spectrum of Late Time

PC mode. Mean photon arrival: T0+16631 s

NH (Galactic)1.30 × 1020 cm-2
NH (intrinsic)4.7 (+1.70 × 103, -4.7) × 1019 cm-2
z of absorber2.486
Photon index1.63 (+0.45, -0.29)
Flux (0.3-10 keV)
(Observed)
6.0 (+1.7, -1.6) × 10-13 erg cm-2 s-1
Flux (0.3-10 keV)
(Unabsorbed)
6.2 (+1.9, -1.4) × 10-13 erg cm-2 s-1
Counts to flux (obs)3.95 × 10-11 erg cm-2 ct-1
Counts to flux (unabs)4.04 × 10-11 erg cm-2 ct-1
W-stat (dof)
What's this?
44.45 (62)
Spectrum exposure6.4 ks

[Back to top]