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XRF 100316D
Redshift:
z
=
0.0591
RA,Dec:
107.6272 -56.2555
Luminosity distance:
D
=
265.00
Mpc
Error:
0.00 arcmin
Galactic dust extinction:
E
B-V
=
0.12
Duration:
T
90
=
999.99
s
Error:
0.00
Downloads
[EPS]
Close-up view of the spectrum of the SN around the [OI] nebular emission line from
Bufano et al. (2012)
[EPS]
Spectral evolution of the SN in the optical from
Bufano et al. (2012)
[EPS]
VLT/X-shooter spectral evolution of the SN over a period of more than a month from
Bufano et al. (2012)
[EPS]
Emission lines from Gemini spectrum of the explosion site, and flux ratios and other parameters from
Levesque et al. (2011)
[EPS]
Emission lines from Gemini spectrum of the host, and flux ratios and other parameters from
Levesque et al. (2011)
[EPS]
Emission lines in the host from X-shooter spectrum from
Starling et al. (2011)
[EPS]
Gemini g-band image of the host from
Levesque et al. (2011)
[EPS]
NaI D absorption lines in the host from
Bufano et al. (2012)
[EPS]
Optical Magellan and Gemini spectra of the SN from
Chornock et al. (2010)
[EPS]
Optical spectrum of the SN ~186 rest-frame days after the explosion from
Bufano et al. (2012)
[EPS]
VLT/FORS2 R-band image of the field from
Bufano et al. (2012)
[PDF]
2D emission lines of GRB site and host from
Levesque et al. (2011)
[PDF]
Gemini r-band image of the host and afterglow/supernova from
Starling et al. (2011)
[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]
HST image of the host from
Starling et al. (2011)
[PDF]
i-band HST and GROND images of the host and afterglow from
Olivares E. et al. (2012)
[PDF]
Optical and radio continuum images (2800, 2340, 1860 and 1340 GHz) of the host from
Michałowski et al. (2015)
[PDF]
X-shooter spectrum of source A in the host with Hδ and [S II] emission from
Wiersema (2011)
Host
Stellar mass:
log(M
*
/M
☉
) =
8.93
Error:
-
Metallicity:
log(Z/Z
☉
) =
-0.39
Error:
0.10
Star formation rate:
SFR
=
0.14
M
☉
yr
-1
Error:
-
Specific star formation:
SSFR =
-
Gyr
-1
Error:
-
Optical extinction:
A
V
=
-
Error:
-
Host SED
Obs. Wavelength (Å)
Flux (μJy)
References
1,928
115.3 ± 7.2
Starling et al. (2011)
2,246
130 ± 11
Starling et al. (2011)
2,600
116 ± 10
Starling et al. (2011)
3,465
164 ± 18
Starling et al. (2011)
4,392
342 ± 29
Starling et al. (2011)
4,587
216 ± 6
Michałowski et al. (2015)
4,750
400 ± 30
Cano et al. (2011)
5,468
417 ± 40
Starling et al. (2011)
6,220
269.4 ± 7.4
Michałowski et al. (2015)
6,300
508 ± 33
Cano et al. (2011)
7,641
295.4 ± 8.2
Michałowski et al. (2015)
7,800
542 ± 30
Cano et al. (2011)
8,990
321 ± 12
Michałowski et al. (2015)
9,250
562 ± 31
Cano et al. (2011)
12,400
375 ± 17
Michałowski et al. (2015)
16,468
375 ± 21
Michałowski et al. (2015)
21,705
287 ± 24
Michałowski et al. (2015)
1,070,687,000
403 ± 13
Michałowski et al. (2015)
1,275,713,000
441 ± 13
Michałowski et al. (2015)
1,611,787,000
531 ± 13
Michałowski et al. (2015)
2,172,409,000
657 ± 21
Michałowski et al. (2015)
Host emission line fluxes
Emission line
Flux (10
-17
cgs)
References
Hα
257
Starling et al. (2011)
Virtual Observatory resources
SDSS DR7 image from
SkyServer
DSS image from
STScI
Record created:
8/3/2010 11:00:58 AM
, record modified:
9/15/2015 9:24:22 AM
Revision: 2.1
Last modified on July 13, 2018
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Sandra Savaglio
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