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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:	EB-V =	1.04
Duration:	T₉₀ =	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