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GRB 080207
Redshift:
z
=
2.0858
RA,Dec:
207.5125 7.5021
Luminosity distance:
D
=
16359.00
Mpc
Error:
0.05 arcmin
Galactic dust extinction:
E
B-V
=
0.02
Duration:
T
90
=
340.00
s
Error:
20.00
Downloads
[EPS]
g- to K-band mosaic of the host from
Svensson et al. (2012)
[EPS]
ISAAC K-band image of the field from
Rossi et al. (2012)
[EPS]
K-band and Spitzer images of the host from
Hunt et al. (2011)
[EPS]
VIMOS R-band image of the field from
Rossi et al. (2012)
[PDF]
2D X-shooter spectrum of the host from
Krühler et al. (2012)
[PDF]
Herschel/PACS 100 μm image superimposed as contours on Spitzer/IRAC 3.6 μm image of the host from
Hunt et al. (2014)
[PDF]
HST image of the host from
Krühler et al. (2012)
[PDF]
Keck/LRIS spectrum of the afterglow from
Prochaska et al. (2009)
[PDF]
NIR image of the host from
Perley et al. (2013)
[PDF]
Optical image of the host from
Perley & Perley (2013)
[PDF]
radio flux contours (2σ plus 1σ increments, red) superimposed on optical/NIR image of the host from
Perley & Perley (2013)
[PDF]
Spitzer/IRAC 3.6 μm image of the host from
Perley et al. (2013)
[PNG]
Keck image of the host from
Perley, D. (2012)
Host
Stellar mass:
log(M
*
/M
☉
) =
11.51
Error:
0.11
Metallicity:
log(Z/Z
☉
) =
-
Error:
-
Star formation rate:
SFR
=
-
M
☉
yr
-1
Error:
-
Specific star formation:
SSFR =
-
Gyr
-1
Error:
-
Optical extinction:
A
V
=
-
Error:
-
Host SED
Obs. Wavelength (Å)
Flux (μJy)
References
4,400
< 0.15
Hunt et al. (2011)
4,730
0.04 ± 0.01
Svensson et al. (2012)
5,997
< 0.3
Svensson et al. (2012)
6,550
0.15 ± 0.025
Hjorth et al. (2012)
6,570
< 0.21
Svensson et al. (2012)
6,600
0.105 ± 0.036
Hunt et al. (2011)
6,895
< 0.24
Svensson et al. (2012)
7,599
0.17 ± 0.05
Svensson et al. (2012)
7,800
< 0.32
Hunt et al. (2011)
7,940
< 0.39
Svensson et al. (2012)
9,250
0.37 ± 0.08
Svensson et al. (2012)
9,250
0.35 ± 0.06
Hunt et al. (2011)
11,170
1.69 ± 0.15
Perley et al. (2013)
11,534
1.75 ± 0.17
Svensson et al. (2012)
12,200
1.06 ± 0.35
Svensson et al. (2012)
12,500
1.6 ± 0.3
Hunt et al. (2011)
15,258
2.43 ± 0.33
Perley et al. (2013)
16,028
2.27 ± 0.34
Svensson et al. (2012)
16,071
2.3 ± 0.4
Hunt et al. (2014)
21,200
6.1 ± 1.5
Perley et al. (2013)
21,550
9.01 ± 0.51
Perley et al. (2013)
21,550
7.52 ± 0.93
Svensson et al. (2012)
21,600
7.3 ± 1
Hunt et al. (2011)
21,890
6.25 ± 1.62
Svensson et al. (2012)
35,500
14.4 ± 0.31
Hunt et al. (2011)
35,500
17.7 ± 0.76
Svensson et al. (2012)
35,700
16.9 ± 0.96
Perley et al. (2013)
44,930
19.9 ± 1.1
Perley et al. (2013)
44,930
20.14 ± 0.65
Svensson et al. (2012)
44,930
15.51 ± 0.44
Hunt et al. (2011)
57,310
18.53 ± 1.58
Hunt et al. (2011)
57,310
30.8 ± 4.3
Svensson et al. (2012)
57,310
29.6 ± 3.2
Perley et al. (2013)
78,720
17.1 ± 2
Perley et al. (2013)
78,720
20.9 ± 4.3
Svensson et al. (2012)
78,720
12.52 ± 1.76
Hunt et al. (2011)
236,800
92.43 ± 6.5
Hunt et al. (2011)
236,800
149 ± 32
Svensson et al. (2012)
236,800
144 ± 29
Perley et al. (2013)
1,000,000
2200 ± 600
Hunt et al. (2014)
1,600,000
5900 ± 1400
Hunt et al. (2014)
2,500,000
< 19500
Hunt et al. (2014)
3,500,000
< 20400
Hunt et al. (2014)
4,510,000
< 53220
Svensson et al. (2012)
5,000,000
21900
Hunt et al. (2014)
8,610,000
< 13122
Svensson et al. (2012)
573,220,000
17.1 ± 2.5
Perley & Perley (2013)
Host emission line fluxes
Emission line
Flux (10
-17
cgs)
References
Virtual Observatory resources
SDSS DR7 image from
SkyServer
DSS image from
STScI
Record created:
5/18/2012 3:08:55 AM
, record modified:
8/20/2015 6:13:34 AM
Revision: 2.1
Last modified on July 13, 2018
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Sandra Savaglio
Visitor number 540908396