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

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: AV = 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)
     323    ±     49      Prochaska et al. (2004)
     504    ±     82      Margutti et al. (2007)
     204.83 ±      4.41   Han et al. (2010)
      64.2                Levesque et al. (2010)
     116.2                Levesque et al. (2010)
     499.73 ±      1.1    Han et al. (2010)
     880    ±    135      Margutti et al. (2007)
     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)
    1135.37 ±      5.21   Han et al. (2010)
     329.5                Levesque et al. (2010)
    1949    ±    263      Margutti et al. (2007)
    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)
    5777    ±    596      Margutti et al. (2007)
    4935    ±     21      Prochaska et al. (2004)
    1078                  Levesque et al. (2010)
    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