Table 1
GRB host galaxy column densities for 29 GRBs.
Galactic parameters | GRB host interstellar and circumstellar parameters | |||||||||
GRB | z | log NH | A V | log NHI | log NSiII | log NSII | log NFeII | log NZnII | log NO,X | A V |
log (cm-2) | mag | log (cm-2) | log (cm-2) | log (cm-2) | log (cm-2) | log (cm-2) | log (cm-2) | mag | ||
|
||||||||||
990123 | 1.600 | 20.26 | 0.05 | ... | ... | ... |
![]() |
13.95 ± 0.051 |
![]() |
<0.252 |
000926 | 2.038 | 20.35 | 0.07 | 21.30 ± 0.203 |
![]() |
... |
![]() |
13.82 ± 0.051 | 0.02 | 0.38 ± 0.052 |
010222 | 1.475 | 20.22 | 0.07 | ... | 16.09 ± 0.051 | ... |
![]() |
13.78 ± 0.071 | 18.75 ± 0.162 |
![]() |
020405 | 0.691 | 20.62 | 0.17 | ... | ... | ... | 15.05 ± 0.754 | ... | <18.695 | 0.42 ± 0.025 |
020813 | 1.255 | 20.79 | 0.34 | ... | 16.29 ± 0.046 | ... | 15.48 ± 0.046 | 13.54 ± 0.066 | ... | ... |
030226* | 1.987 | 20.20 | 0.06 | 20.50 ± 0.307 | 15.07 ± 0.047 | >13.37 |
![]() |
<12.707 | <18.605 | 0.05 ± 0.015 |
1.963 | 20.50 ± 0.307 | 14.97 ± 0.037 | ... |
![]() |
<12.607 | |||||
030323 | 3.371 | 20.61 | 0.15 | 21.90 ± 0.078 |
![]() |
15.84 ± 0.198 | 15.93 ± 0.088 | <14.508 | ... | ... |
050401 | 2.899 | 20.64 | 0.20 | 22.60 ± 0.309 | 16.50 ± 0.409 | ... | 16.00 ± 0.209 | 14.30 ± 0.309 |
![]() |
0.45 ± 0.035 |
050505 | 4.275 | 20.23 | 0.06 | 22.05 ± 0.1011 | 15.70 ± 0.0011 | 16.111 | 15.50 ± 0.0011 | ... | 18.93 ± 0.0510 | ... |
050730 | 3.969 | 20.48 | 0.16 | 22.10 ± 0.1012 | 15.47 ± 0.0312 | 15.11 ± 0.0412 |
![]() |
... |
![]() |
<0.1713 |
050820A | 2.615 | 20.64 | 0.14 | 21.05 ± 0.1012 | >15.4314 | 15.57 ± 0.0414 | 14.82 ± 0.1214 | 12.96 ± 0.0214 |
![]() |
0.27 ± 0.0413 |
050904 | 6.295 | 20.66 | 0.18 | 21.62 ± 0.2015 | <16.6016 | 15.95 ± 0.5516 | ... | ... |
![]() |
<0.0734 |
050922C | 2.199 | 20.73 | 0.32 | 21.55 ± 0.1012 | 14.97 ± 0.0717 | 14.87 ± 0.0512 |
![]() |
... |
![]() |
![]() |
051111 | 1.549 | 20.72 | 0.50 | ... | >16.1414 | ... | 15.32 ± 0.0114 | 13.47 ± 0.0414 |
![]() |
![]() |
060206 | 4.048 | 19.95 | 0.04 | 20.85 ± 0.1018 | 15.23 ± 0.0419 | 15.13 ± 0.0519 | >14.6520 | ... |
![]() |
<0.2413 |
060418 | 1.490 | 20.94 | 0.69 | ... | 15.92 ± 0.0321 | ... | 15.22 ± 0.0314 | 13.09 ± 0.0121 |
![]() |
![]() |
060510B | 4.941 | 20.61 | 0.12 | 21.30 ± 0.1022 | ... |
![]() |
>15.9023 | ... |
![]() |
... |
060526 | 3.221 | 20.70 | 0.21 | 20.01 ± 0.1524 | >14.4824 | 14.58 ± 0.2524 | 14.28 ± 0.2424 | <12.7324 | <18.1213 | <0.5913 |
070802 | 2.450 | 20.46 | 0.08 | 21.50 ± 0.2025 | 16.41 ± 0.1725 | ... | 16.44 ± 0.1225 | 13.97 ± 0.1425 |
![]() |
![]() |
071003 | 1.604 | 21.03 | 0.47 | ... | ... | ... |
![]() |
<12.7527 |
![]() |
... |
071031 | 2.692 | 20.09 | 0.04 | 22.15 ± 0.0512 | ... | ... | 15.83 ± 0.0212 | 13.02 ± 0.0212 |
![]() |
<0.1126 |
080319B | 0.937 | 20.05 | 0.03 | ... | ... | ... |
![]() |
... |
![]() |
![]() |
080330 | 1.511 | 20.09 | 0.05 | ... | >15.4129 | ... | 14.70 ± 0.0929 | 12.79 ± 0.0629 |
![]() |
<0.1926 |
080413A | 2.433 | 20.94 | 0.48 | 21.85 ± 0.1512 | ... | ... | 15.57 ± 0.0412 | 12.85 ± 0.0612 |
![]() |
<0.8813 |
080607 | 3.036 | 20.23 | 0.07 | 22.70 ± 0.1530 | >16.2029 | >16.1430 | >16.3530 | >13.6030 |
![]() |
... |
080721 | 2.591 | 20.84 | 0.31 | 21.60 ± 0.1031 | >16.0031 | ... | ... | ... |
![]() |
![]() |
090323 | 3.577 | 20.23 | 0.08 | 19.62 ± 0.335 | 15.46 ± 0.135 | 15.41 ± 0.045 | 14.91 ± 0.055 | <12.75 | <18.655 | 0.10 ± 0.045 |
3.567 | 20.72 ± 0.095 | 15.80 ± 0.055 | 15.80 ± 0.025 | 15.00 ± 0.055 | 13.57 ± 0.045 | |||||
090328 | 0.736 | 20.70 | 0.18 | ... | ... | ... |
![]() |
... |
![]() |
0.34 ± 0.045 |
090926A | 2.106 | 20.44 | 0.07 | 21.73 ± 0.0733 | 14.97 ± 0.2633 | 14.96 ± 0.1533 | 14.36 ± 0.1433 | <13.0033 | <18.745 | <0.15 |
Notes. Columns list redshift, Galactic column density and visual extinction in the line-of-sight to the GRB, the H i, Si ii, S ii, Fe ii and Zn ii column density with corresponding references, the oxygen column density measured from the X-ray spectra, NO,X, and the best-fit visual extinction, AV, with both corresponding references given. For GRB 030226 and GRB 090323, two absorbing components were detected within the GBR host galaxy, and the optical column densities for both are given where applicable.
Where two host galaxy absorption systems are reported, we used the combined column densities of the two systems in our analysis.
References. 1 Savaglio et al. (2003); 2 Starling et al. (2007); 3 Hjorth et al. (2003); 4 Masetti et al. (2003); 5 this work; 6 Savaglio & Fall (2004); 7 Shin et al. (2006); 8 Vreeswijk et al. (2004); 9 Watson et al. (2006); 10 Evans et al. (2009); 11 Berger et al. (2006); 12 Ledoux et al. (2009); 13 Schady et al. (in prep); 14 Prochaska et al. (2007a); 15 Totani (2006); 16 Kawai et al. (2006); 17 Piranomonte et al. (2008); 18 Fynbo et al. (2006); 19 Thöne et al. (2008a); 20 Aoki et al. (2009); 21 Vreeswijk et al. (2007); 22 Chary et al. (2007); 23 Price et al. (2007); 24 Thöne et al. (2008b); 25 Elíasdóttir et al. (2009); 26 Greiner et al. (2010); 27 Perley et al. (2008a); 28 D’Elia et al. (2009); 29 D’Elia et al. (2009); 30 Prochaska et al. (2009); 31 Starling et al. (2009); 32 McBreen et al. (2010); 33 Rau et al. (2010); 34 Zafar et al. (2010).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.