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GRB hosts
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GRB 031203
Redshift:
z
=
0.1055
RA,Dec:
120.6210 -39.8533
Luminosity distance:
D
=
489.00
Mpc
Error:
0.00 arcmin
Galactic dust extinction:
E
B-V
=
1.04
Duration:
T
90
=
20.00
s
Error:
-
Downloads
[EPS]
VLT spectrum of the host with SN contribution from
Margutti et al. (2007)
[JPG]
Image of the host from
Prochaska et al. (2004)
[JPG]
Spectrum of the host from
Prochaska et al. (2004)
[PDF]
HI map superimposed on the optical image of the host from
Michałowski et al. (2015)
[PDF]
HI radio spectrum of the host from
Michałowski et al. (2015)
[PDF]
I-band image of the field from
Thomsen et al. (2004)
[PDF]
Keck spectrum of the host from
Levesque et al. (2010)
[PDF]
Keck spectrum of the host (zoom of blue region) from
Levesque et al. (2010)
[PDF]
NIR X-shooter spectrum of the host galaxy from
Guseva et al. (2011)
[PDF]
Optical and radio continuum images (2800, 2340, 1860 and 1340 GHz) of the host from
Michałowski et al. (2015)
[PDF]
Optical image of the host with radio contours from
Michałowski et al. (2012)
[PDF]
Optical X-shooter spectrum of the host galaxy from
Guseva et al. (2011)
[PDF]
PANIC J-band image of the host and afterglow from
Gal-Yam et al. (2004)
[PDF]
Rest-frame VLT/FORS2 spectrum of the host (left) and Wolf-Rayet bump (right) from
Han et al. (2010)
[PDF]
Spectra of the supernova from
Malesani et al. (2004)
[PDF]
Spitzer image of the host from
Svensson et al. (2010)
[PDF]
Spitzer/IRS high-resolution spectrum of the host from
Watson et al. (2011)
[PDF]
Spitzer/IRS low-resolution spectrum of the host from
Watson et al. (2011)
[PDF]
UV to mid-IR spectra of the host and UV to radio SED of the host from
Watson et al. (2011)
[PDF]
VLT/FORS2 spectrum of the host from
Han et al. (2010)
[PDF]
WISE and Herschel/PACS images of the host from
Symeonidis et al. (2014)
[PDF]
X-shooter spectrum of the host from
Watson et al. (2011)
Host
Stellar mass:
log(M
*
/M
☉
) =
8.82
Error:
0.43
Metallicity:
log(Z/Z
☉
) =
-0.64
Error:
-
Star formation rate:
SFR
=
12.68
M
☉
yr
-1
Error:
-
Specific star formation:
SSFR =
-
Gyr
-1
Error:
-
Optical extinction:
A
V
=
0.03
Error:
0.05
Host SED
Obs. Wavelength (Å)
Flux (μJy)
References
3,620
184 ± 31
Margutti et al. (2007)
4,290
259 ± 12
Margutti et al. (2007)
5,540
419 ± 19
Margutti et al. (2007)
6,570
214.3 ± 3.9
Margutti et al. (2007)
7,680
278 ± 10
Margutti et al. (2007)
7,970
277 ± 18
Cobb et al. (2004)
12,200
181 ± 13
Cobb et al. (2004)
12,200
182.4 ± 3.4
Prochaska et al. (2004)
16,300
140.6 ± 2.6
Prochaska et al. (2004)
21,900
223 ± 4.1
Prochaska et al. (2004)
33,526
110 ± 5
Symeonidis et al. (2014)
35,700
193.2 ± 5.3
Svensson et al. (2010)
35,700
216 ± 3
Castro Cerón et al. (2010)
35,700
193 ± 2
Watson et al. (2011)
46,028
86 ± 9
Symeonidis et al. (2014)
57,700
333 ± 18
Svensson et al. (2010)
57,700
356 ± 13
Watson et al. (2011)
115,608
1740 ± 120
Symeonidis et al. (2014)
220,883
11300 ± 1000
Symeonidis et al. (2014)
240,000
11300 ± 400
Watson et al. (2011)
700,000
39000 ± 18000
Symeonidis et al. (2014)
800,000
< 40000
Watson et al. (2011)
1,000,000
< 70000
Symeonidis et al. (2014)
1,600,000
< 149000
Symeonidis et al. (2014)
8,700,000
< 9000
Watson et al. (2011)
545,000,000
216 ± 50
Stanway et al. (2010)
1,070,687,000
324 ± 13
Michałowski et al. (2015)
1,260,000,000
191 ± 37
Watson et al. (2011)
1,275,713,000
319 ± 12
Michałowski et al. (2015)
1,611,787,000
324 ± 11
Michałowski et al. (2015)
2,160,000,000
254 ± 46
Watson et al. (2011)
2,172,409,000
383 ± 20
Michałowski et al. (2015)
Host emission line fluxes
Emission line
Flux (10
-17
cgs)
References
[O
II
] λ3727
2157 ± 374
Margutti et al. (2007)
[O
II
] λ3727
943.07 ± 4.8
Han et al. (2010)
[O
II
] λ3727
1238 ± 103
Prochaska et al. (2004)
[O
II
] λ3727
221.9
Levesque et al. (2010)
[Ne
III
] λ3869
111.2
Levesque et al. (2010)
[Ne
III
] λ3869
1073 ± 181
Margutti et al. (2007)
[Ne
III
] λ3869
731 ± 65
Prochaska et al. (2004)
[Ne
III
] λ3970
288 ± 54
Prochaska et al. (2004)
Hδ
323 ± 49
Prochaska et al. (2004)
Hδ
504 ± 82
Margutti et al. (2007)
Hδ
204.83 ± 4.41
Han et al. (2010)
Hδ
64.2
Levesque et al. (2010)
Hγ
116.2
Levesque et al. (2010)
Hγ
499.73 ± 1.1
Han et al. (2010)
Hγ
880 ± 135
Margutti et al. (2007)
Hγ
699 ± 35
Prochaska et al. (2004)
[O
III
] λ4364
158 ± 30
Prochaska et al. (2004)
[O
III
] λ4364
147 ± 22
Margutti et al. (2007)
[O
III
] λ4364
79.1 ± 1.25
Han et al. (2010)
[O
III
] λ4364
36.8
Levesque et al. (2010)
Hβ
1135.37 ± 5.21
Han et al. (2010)
Hβ
329.5
Levesque et al. (2010)
Hβ
1949 ± 263
Margutti et al. (2007)
Hβ
1677 ± 26
Prochaska et al. (2004)
[O
III
] λ4959
3584 ± 33
Prochaska et al. (2004)
[O
III
] λ4959
4167 ± 551
Margutti et al. (2007)
[O
III
] λ4959
739
Levesque et al. (2010)
[O
III
] λ4959
2404.78 ± 5.32
Han et al. (2010)
[O
III
] λ5007
7238.76 ± 4.68
Han et al. (2010)
[O
III
] λ5007
2268
Levesque et al. (2010)
[O
III
] λ5007
12467 ± 1631
Margutti et al. (2007)
[O
III
] λ5007
10880 ± 54
Prochaska et al. (2004)
[He
I
] λ5877
210 ± 9.2
Prochaska et al. (2004)
[He
I
] λ5877
270 ± 30
Margutti et al. (2007)
Hα
5777 ± 596
Margutti et al. (2007)
Hα
4935 ± 21
Prochaska et al. (2004)
Hα
1078
Levesque et al. (2010)
Hα
3636.63 ± 4.96
Han et al. (2010)
[N
II
] λ6585
109.04 ± 4.21
Han et al. (2010)
[N
II
] λ6585
75.2
Levesque et al. (2010)
[N
II
] λ6585
265.9 ± 8.4
Prochaska et al. (2004)
[N
II
] λ6585
283 ± 29
Margutti et al. (2007)
[He
I
] λ6680
63.8 ± 6.4
Margutti et al. (2007)
[S
II
] λ6718
196 ± 19
Margutti et al. (2007)
[S
II
] λ6718
149.9 ± 5.9
Prochaska et al. (2004)
[S
II
] λ6718
58.9
Levesque et al. (2010)
[S
II
] λ6718
129.55 ± 4.33
Han et al. (2010)
[S
II
] λ6733
94.63 ± 2.89
Han et al. (2010)
[S
II
] λ6733
46.03
Levesque et al. (2010)
[S
II
] λ6733
125.3 ± 4.9
Prochaska et al. (2004)
[S
II
] λ6733
157 ± 16
Margutti et al. (2007)
Virtual Observatory resources
SDSS DR7 image from
SkyServer
DSS image from
STScI
Record created:
11/7/2006 10:50:01 AM
, record modified:
8/25/2015 8:41:48 AM
Revision: 2.1
Last modified on July 13, 2018
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