Table 1.

Observational properties of 50 GRBs and their host galaxies in radio bands.

GRB|$E_{\rm iso}^a$||$T_{90}^a$|zaFrequencyHost flux densityPeak flux densitybPeak timeReferencescRRF
(1051 erg)(s)(GHz)(μJy)(μJy)(days)(per cent)
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)
Low-luminosity GRBs
020903n0.023130.2501.4343 ± 66294 ± 9136.7328,914.6 ± 14.8
4.8621 ± 34782 ± 2836.7 ± 1.328,92.7 ± 4.4
8.46190 ± 301058 ± 1923.8028,918.0 ± 2.9
031203n0.115300.1051.43254 ± 46h929 ± 6065.5 ± 5.322,927.3 ± 5.3
4.86393 ± 60828 ± 2858.4 ± 2.127,947.5 ± 7.4
8.4653 ± 52724 ± 1948 ± 1.327,97.3 ± 7.2
050416An1.0030.6504.8650.5 ± 41.8485 ± 3648.5 ± 3.530,910.4 ± 8.7
8.4620 ± 51373 ± 3649 ± 3.630,97.3 ± 13.7
060218n0.0031280.0331.4369.5 ± 69.5198 ± 584.929,935.1 ± 36.6
4.8632 ± 32245 ± 503.8 ± 0.729,913.1 ± 13.3
8.4622.8 ± 20.5471 ± 832 ± 0.329,94.8 ± 4.4
100418An0.52070.6208.46366 ± 531218 ± 1247.6 ± 0.623,930.1 ± 4.4
Standard GRBs
9705087.10140.8351.43100 ± 32381 ± 19179.1 ± 7.615,926.3 ± 8.5
4.86104 ± 44780 ± 1357.6 ± 0.915,913.3 ± 5.6
8.468 ± 19958 ± 1137.2 ± 0.417,90.8 ± 2.0
98070369.0900.9661.4368 ± 6.6h263 ± 8125.4 ± 5.53,925.9 ± 8.4
4.8642.1 ± 8.6h1055 ± 309.1 ± 0.23,94.0 ± 0.8
8.4639.3 ± 4.9h1370 ± 3010 ± 0.23,92.9 ± 0.4
9812265.90201.118.4612 ± 22.6137 ± 348.2 ± 1.612,98.8 ± 1.7
000301C43.7102.0344.8685 ± 33240 ± 534.31,935.4 ± 15.8
8.4618 ± 7h520 ± 2414.1 ± 0.524,93.5 ± 1.4
00041875.1301.1191.4348 ± 15h210 ± 18016.564,222.9 ± 20.9
4.86110 ± 52897 ± 3927 ± 14,912.3 ± 5.8
8.4637 ± 12h1085 ± 2218.1 ± 0.34,93.4 ± 1.1
0109219.00240.4504.8627 ± 25161 ± 2031.5 ± 3.317,916.8 ± 15.7
8.4643.7 ± 21.3229 ± 2227.0117,919.1 ± 9.5
01121163.04002.1408.4624 ± 16162 ± 1313.2 ± 1.617,914.8 ± 9.9
020819B7.90500.4108.4644.7 ± 23291 ± 2112.2 ± 1.120,915.4 ± 8.0
02100438.0502.3304.8678 ± 28470 ± 2632.2 ± 1.417,916.6 ± 6.0
8.4659.4 ± 19.5780 ± 2318.7 ± 0.517,97.6 ± 2.5
021211n11.081.0108.4612 ± 3660 ± 288.8511,1120.0 ± 60.7
030329n18.0630.1691.43450 ± 1092232 ± 3078.6 ± 2.15,920.3 ± 4.9
4.86332 ± 51.710337 ± 3332.9 ± 0.15,93.2 ± 0.5
8.46248 ± 48.219567 ± 2817.3 ± 0.15,91.3 ± 0.3
050824n1.50230.8308.4636 ± 27156 ± 347.217,923.1 ± 18.0
070612A9.123690.6174.86222 ± 42.3580 ± 20140.3 ± 5.817,938.3 ± 7.4
8.4668 ± 491028 ± 1684.1 ± 217,96.6 ± 4.8
071010B26.0360.9474.8657 ± 60.4227 ± 11412.5 ± 4.417,925.1 ± 29.5
8.4617 ± 47341 ± 414.2 ± 0.517,95.0 ± 13.8
090328100570.7368.4621 ± 64686 ± 2616.1 ± 0.77,93.1 ± 9.3
09102045.6391.7108.4690 ± 41.1399 ± 2110.9 ± 0.617,922.6 ± 10.4
100814A59.71751.444.5085 ± 27496 ± 2413 ± 117,917.1 ± 5.5
100901A17.84391.4084.5075 ± 40331 ± 304.917,922.7 ± 12.3
High-luminosity GRBs
9708282961470.9581.4314 ± 2257 ± 51208.110,1024.6 ± 44.4
8.4632 ± 20.5144 ± 317.8 ± 1.810,922.2 ± 15.0
9803292100582–3.91.4338 ± 25.5134 ± 43113.5432,3228.4 ± 21.1
4.8622 ± 37171 ± 1491.5 ± 11.332,912.9 ± 21.7
8.4613 ± 11332 ± 1133.5 ± 1.432,93.9 ± 3.3
99012323901001.6008.467.7 ± 11.1260 ± 3224.6521,213.0 ± 4.3
9905069492201.3078.4631 ± 27.6581 ± 452.7031,315.3 ± 4.8
991208n110600.7061.4354.8 ± 44.4263 ± 498.9 ± 1.818,920.8 ± 17.3
8.4637.3 ± 25.81804 ± 247.8 ± 0.118,92.1 ± 1.4
991216675251.0208.4620 ± 24.7960 ± 671.4913,132.1 ± 2.6
000210200100.8508.4618 ± 9h93 ± 218.594,2519.4 ± 10.6
000911n8805001.0594.8610 ± 2571 ± 2311.126,914.1 ± 35.5
8.4633.7 ± 25.2263 ± 333.1 ± 0.326,912.8 ± 9.7
000926270252.0394.8658 ± 41.5460 ± 3116.9 ± 1.519,912.6 ± 9.1
8.4623 ± 9h629 ± 2412.1 ± 0.524,93.7 ± 1.4
0102221331701.4774.8623 ± 8h144 ± 472.324,916.0 ± 7.6
8.4638.8 ± 19.8344 ± 391.3517,1711.3 ± 5.9
0208138001131.2544.8623 ± 42349 ± 435.1517,176.6 ± 12.1
8.4630.8 ± 19.8323 ± 391.2417,179.5 ± 6.2
030226120691.9868.4635 ± 18171 ± 236.7 ± 117,1720.5 ± 10.9
050603500122.8218.4679 ± 49377 ± 5314.1 ± 1.817,1720.9 ± 13.3
050820A2002402.6154.8621 ± 51256 ± 782.1517,68.2 ± 20.1
8.4676 ± 30634 ± 620.936,612.0 ± 4.9
05090413001746.2908.4613 ± 2776 ± 1435.3 ±1.516,917.1 ± 35.7
0510226302000.8098.4641 ± 23268 ± 325.2 ± 0.717,915.3 ± 8.8
High-luminosity GRBs
070125955601.5484.86133 ± 21308 ± 7827.98,943.2 ± 12.9
8.4664 ± 181028 ± 1684.1 ± 28,96.2 ± 1.7
0710033241481.6044.8693 ± 52224 ± 543.817,941.5 ± 25.3
8.46109 ± 45616 ± 576.5 ± 0.517,917.7 ± 7.5
09032341001333.578.4627 ± 38243 ± 1315.6 ± 17,911.1 ± 15.7
090902B30901.8838.4618 ± 1684 ± 1614.1 ± 2.67,921.4 ± 19.5
100414A779261.3688.4620 ± 16524 ± 198 ± 0.317,93.8 ± 3.1
GRBs without known redshifts
980519304.8625 ± 27330 ± 4717.9 ± 2.414,97.6 ± 8.3
8.4649 ± 28205 ± 2312.6 ± 1.314,923.9 ± 13.9
0010073758.4634 ± 61222 ± 337.117,915.3 ± 27.6
001018318.4670 ± 23.3590 ± 684.7 ± 0.617,911.9 ± 4.2
021206204.8658 ± 24480 ± 697 ± 0.817,912.1 ± 5.3
041219A64.8633 ± 48473 ± 286.3 ± 0.917,97.0 ± 10.2
8.4663 ± 42518 ± 1501.6917,1712.2 ± 8.8
050713B1254.8644 ± 69623 ± 5321.0117,177.1 ± 11.1
8.4659 ± 40.5373 ± 2414.1 ± 0.917,915.8 ± 10.9
GRB|$E_{\rm iso}^a$||$T_{90}^a$|zaFrequencyHost flux densityPeak flux densitybPeak timeReferencescRRF
(1051 erg)(s)(GHz)(μJy)(μJy)(days)(per cent)
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)
Low-luminosity GRBs
020903n0.023130.2501.4343 ± 66294 ± 9136.7328,914.6 ± 14.8
4.8621 ± 34782 ± 2836.7 ± 1.328,92.7 ± 4.4
8.46190 ± 301058 ± 1923.8028,918.0 ± 2.9
031203n0.115300.1051.43254 ± 46h929 ± 6065.5 ± 5.322,927.3 ± 5.3
4.86393 ± 60828 ± 2858.4 ± 2.127,947.5 ± 7.4
8.4653 ± 52724 ± 1948 ± 1.327,97.3 ± 7.2
050416An1.0030.6504.8650.5 ± 41.8485 ± 3648.5 ± 3.530,910.4 ± 8.7
8.4620 ± 51373 ± 3649 ± 3.630,97.3 ± 13.7
060218n0.0031280.0331.4369.5 ± 69.5198 ± 584.929,935.1 ± 36.6
4.8632 ± 32245 ± 503.8 ± 0.729,913.1 ± 13.3
8.4622.8 ± 20.5471 ± 832 ± 0.329,94.8 ± 4.4
100418An0.52070.6208.46366 ± 531218 ± 1247.6 ± 0.623,930.1 ± 4.4
Standard GRBs
9705087.10140.8351.43100 ± 32381 ± 19179.1 ± 7.615,926.3 ± 8.5
4.86104 ± 44780 ± 1357.6 ± 0.915,913.3 ± 5.6
8.468 ± 19958 ± 1137.2 ± 0.417,90.8 ± 2.0
98070369.0900.9661.4368 ± 6.6h263 ± 8125.4 ± 5.53,925.9 ± 8.4
4.8642.1 ± 8.6h1055 ± 309.1 ± 0.23,94.0 ± 0.8
8.4639.3 ± 4.9h1370 ± 3010 ± 0.23,92.9 ± 0.4
9812265.90201.118.4612 ± 22.6137 ± 348.2 ± 1.612,98.8 ± 1.7
000301C43.7102.0344.8685 ± 33240 ± 534.31,935.4 ± 15.8
8.4618 ± 7h520 ± 2414.1 ± 0.524,93.5 ± 1.4
00041875.1301.1191.4348 ± 15h210 ± 18016.564,222.9 ± 20.9
4.86110 ± 52897 ± 3927 ± 14,912.3 ± 5.8
8.4637 ± 12h1085 ± 2218.1 ± 0.34,93.4 ± 1.1
0109219.00240.4504.8627 ± 25161 ± 2031.5 ± 3.317,916.8 ± 15.7
8.4643.7 ± 21.3229 ± 2227.0117,919.1 ± 9.5
01121163.04002.1408.4624 ± 16162 ± 1313.2 ± 1.617,914.8 ± 9.9
020819B7.90500.4108.4644.7 ± 23291 ± 2112.2 ± 1.120,915.4 ± 8.0
02100438.0502.3304.8678 ± 28470 ± 2632.2 ± 1.417,916.6 ± 6.0
8.4659.4 ± 19.5780 ± 2318.7 ± 0.517,97.6 ± 2.5
021211n11.081.0108.4612 ± 3660 ± 288.8511,1120.0 ± 60.7
030329n18.0630.1691.43450 ± 1092232 ± 3078.6 ± 2.15,920.3 ± 4.9
4.86332 ± 51.710337 ± 3332.9 ± 0.15,93.2 ± 0.5
8.46248 ± 48.219567 ± 2817.3 ± 0.15,91.3 ± 0.3
050824n1.50230.8308.4636 ± 27156 ± 347.217,923.1 ± 18.0
070612A9.123690.6174.86222 ± 42.3580 ± 20140.3 ± 5.817,938.3 ± 7.4
8.4668 ± 491028 ± 1684.1 ± 217,96.6 ± 4.8
071010B26.0360.9474.8657 ± 60.4227 ± 11412.5 ± 4.417,925.1 ± 29.5
8.4617 ± 47341 ± 414.2 ± 0.517,95.0 ± 13.8
090328100570.7368.4621 ± 64686 ± 2616.1 ± 0.77,93.1 ± 9.3
09102045.6391.7108.4690 ± 41.1399 ± 2110.9 ± 0.617,922.6 ± 10.4
100814A59.71751.444.5085 ± 27496 ± 2413 ± 117,917.1 ± 5.5
100901A17.84391.4084.5075 ± 40331 ± 304.917,922.7 ± 12.3
High-luminosity GRBs
9708282961470.9581.4314 ± 2257 ± 51208.110,1024.6 ± 44.4
8.4632 ± 20.5144 ± 317.8 ± 1.810,922.2 ± 15.0
9803292100582–3.91.4338 ± 25.5134 ± 43113.5432,3228.4 ± 21.1
4.8622 ± 37171 ± 1491.5 ± 11.332,912.9 ± 21.7
8.4613 ± 11332 ± 1133.5 ± 1.432,93.9 ± 3.3
99012323901001.6008.467.7 ± 11.1260 ± 3224.6521,213.0 ± 4.3
9905069492201.3078.4631 ± 27.6581 ± 452.7031,315.3 ± 4.8
991208n110600.7061.4354.8 ± 44.4263 ± 498.9 ± 1.818,920.8 ± 17.3
8.4637.3 ± 25.81804 ± 247.8 ± 0.118,92.1 ± 1.4
991216675251.0208.4620 ± 24.7960 ± 671.4913,132.1 ± 2.6
000210200100.8508.4618 ± 9h93 ± 218.594,2519.4 ± 10.6
000911n8805001.0594.8610 ± 2571 ± 2311.126,914.1 ± 35.5
8.4633.7 ± 25.2263 ± 333.1 ± 0.326,912.8 ± 9.7
000926270252.0394.8658 ± 41.5460 ± 3116.9 ± 1.519,912.6 ± 9.1
8.4623 ± 9h629 ± 2412.1 ± 0.524,93.7 ± 1.4
0102221331701.4774.8623 ± 8h144 ± 472.324,916.0 ± 7.6
8.4638.8 ± 19.8344 ± 391.3517,1711.3 ± 5.9
0208138001131.2544.8623 ± 42349 ± 435.1517,176.6 ± 12.1
8.4630.8 ± 19.8323 ± 391.2417,179.5 ± 6.2
030226120691.9868.4635 ± 18171 ± 236.7 ± 117,1720.5 ± 10.9
050603500122.8218.4679 ± 49377 ± 5314.1 ± 1.817,1720.9 ± 13.3
050820A2002402.6154.8621 ± 51256 ± 782.1517,68.2 ± 20.1
8.4676 ± 30634 ± 620.936,612.0 ± 4.9
05090413001746.2908.4613 ± 2776 ± 1435.3 ±1.516,917.1 ± 35.7
0510226302000.8098.4641 ± 23268 ± 325.2 ± 0.717,915.3 ± 8.8
High-luminosity GRBs
070125955601.5484.86133 ± 21308 ± 7827.98,943.2 ± 12.9
8.4664 ± 181028 ± 1684.1 ± 28,96.2 ± 1.7
0710033241481.6044.8693 ± 52224 ± 543.817,941.5 ± 25.3
8.46109 ± 45616 ± 576.5 ± 0.517,917.7 ± 7.5
09032341001333.578.4627 ± 38243 ± 1315.6 ± 17,911.1 ± 15.7
090902B30901.8838.4618 ± 1684 ± 1614.1 ± 2.67,921.4 ± 19.5
100414A779261.3688.4620 ± 16524 ± 198 ± 0.317,93.8 ± 3.1
GRBs without known redshifts
980519304.8625 ± 27330 ± 4717.9 ± 2.414,97.6 ± 8.3
8.4649 ± 28205 ± 2312.6 ± 1.314,923.9 ± 13.9
0010073758.4634 ± 61222 ± 337.117,915.3 ± 27.6
001018318.4670 ± 23.3590 ± 684.7 ± 0.617,911.9 ± 4.2
021206204.8658 ± 24480 ± 697 ± 0.817,912.1 ± 5.3
041219A64.8633 ± 48473 ± 286.3 ± 0.917,97.0 ± 10.2
8.4663 ± 42518 ± 1501.6917,1712.2 ± 8.8
050713B1254.8644 ± 69623 ± 5321.0117,177.1 ± 11.1
8.4659 ± 40.5373 ± 2414.1 ± 0.917,915.8 ± 10.9

aRefer to Chandra & Frail (2012).

bObserved radio peak flux density.

cReferences are in the following order: host radio flux density, radio peak flux density.

Abbreviations for the references are as follows: (1) Berger et al. (2000), (2) Berger et al. (2001a), (3) Berger et al. (2001b), (4) Berger et al. (2003a), (5) Berger et al. (2003c), (6) Cenko et al. (2006), (7) Cenko et al. (2011), (8) Chandra et al. (2008), (9) Chandra & Frail (2012), (10) Djorgovski et al. (2001), (11) Fox et al. (2003), (12) Frail et al. (1999), (13) Frail et al. (2000a), (14) Frail et al. (2000b), (15) Frail, Waxman & Kulkarni (2000), (16) Frail et al. (2006), (17) Frail & Chandra (2014, private communication), (18) Galama et al. (2003), (19) Harrison et al. (2001), (20) Jakobsson et al. (2005), (21) Kulkarni et al. (1999), (22) Michałowski et al. (2012), (23) Moin et al. (2013), (24) Perley & Perley (2013), (25) Piro et al. (2002), (26) Price et al. (2002), (27) Soderberg et al. (2004a), (28) Soderberg et al. (2004b), (29) Soderberg et al. (2006), (30) Soderberg et al. (2007), (31) Taylor et al. (2000), (32) Yost et al. (2002).

hHost flux densities have been reported in Berger et al. (2001b), Berger et al. (2003a), Michałowski et al. (2012) and Perley & Perley (2013).

nSN/GRB, i.e. SN-associated GRBs.

These values are the maximum observed flux densities, which are taken as the observed peak flux densities.

Table 1.

Observational properties of 50 GRBs and their host galaxies in radio bands.

GRB|$E_{\rm iso}^a$||$T_{90}^a$|zaFrequencyHost flux densityPeak flux densitybPeak timeReferencescRRF
(1051 erg)(s)(GHz)(μJy)(μJy)(days)(per cent)
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)
Low-luminosity GRBs
020903n0.023130.2501.4343 ± 66294 ± 9136.7328,914.6 ± 14.8
4.8621 ± 34782 ± 2836.7 ± 1.328,92.7 ± 4.4
8.46190 ± 301058 ± 1923.8028,918.0 ± 2.9
031203n0.115300.1051.43254 ± 46h929 ± 6065.5 ± 5.322,927.3 ± 5.3
4.86393 ± 60828 ± 2858.4 ± 2.127,947.5 ± 7.4
8.4653 ± 52724 ± 1948 ± 1.327,97.3 ± 7.2
050416An1.0030.6504.8650.5 ± 41.8485 ± 3648.5 ± 3.530,910.4 ± 8.7
8.4620 ± 51373 ± 3649 ± 3.630,97.3 ± 13.7
060218n0.0031280.0331.4369.5 ± 69.5198 ± 584.929,935.1 ± 36.6
4.8632 ± 32245 ± 503.8 ± 0.729,913.1 ± 13.3
8.4622.8 ± 20.5471 ± 832 ± 0.329,94.8 ± 4.4
100418An0.52070.6208.46366 ± 531218 ± 1247.6 ± 0.623,930.1 ± 4.4
Standard GRBs
9705087.10140.8351.43100 ± 32381 ± 19179.1 ± 7.615,926.3 ± 8.5
4.86104 ± 44780 ± 1357.6 ± 0.915,913.3 ± 5.6
8.468 ± 19958 ± 1137.2 ± 0.417,90.8 ± 2.0
98070369.0900.9661.4368 ± 6.6h263 ± 8125.4 ± 5.53,925.9 ± 8.4
4.8642.1 ± 8.6h1055 ± 309.1 ± 0.23,94.0 ± 0.8
8.4639.3 ± 4.9h1370 ± 3010 ± 0.23,92.9 ± 0.4
9812265.90201.118.4612 ± 22.6137 ± 348.2 ± 1.612,98.8 ± 1.7
000301C43.7102.0344.8685 ± 33240 ± 534.31,935.4 ± 15.8
8.4618 ± 7h520 ± 2414.1 ± 0.524,93.5 ± 1.4
00041875.1301.1191.4348 ± 15h210 ± 18016.564,222.9 ± 20.9
4.86110 ± 52897 ± 3927 ± 14,912.3 ± 5.8
8.4637 ± 12h1085 ± 2218.1 ± 0.34,93.4 ± 1.1
0109219.00240.4504.8627 ± 25161 ± 2031.5 ± 3.317,916.8 ± 15.7
8.4643.7 ± 21.3229 ± 2227.0117,919.1 ± 9.5
01121163.04002.1408.4624 ± 16162 ± 1313.2 ± 1.617,914.8 ± 9.9
020819B7.90500.4108.4644.7 ± 23291 ± 2112.2 ± 1.120,915.4 ± 8.0
02100438.0502.3304.8678 ± 28470 ± 2632.2 ± 1.417,916.6 ± 6.0
8.4659.4 ± 19.5780 ± 2318.7 ± 0.517,97.6 ± 2.5
021211n11.081.0108.4612 ± 3660 ± 288.8511,1120.0 ± 60.7
030329n18.0630.1691.43450 ± 1092232 ± 3078.6 ± 2.15,920.3 ± 4.9
4.86332 ± 51.710337 ± 3332.9 ± 0.15,93.2 ± 0.5
8.46248 ± 48.219567 ± 2817.3 ± 0.15,91.3 ± 0.3
050824n1.50230.8308.4636 ± 27156 ± 347.217,923.1 ± 18.0
070612A9.123690.6174.86222 ± 42.3580 ± 20140.3 ± 5.817,938.3 ± 7.4
8.4668 ± 491028 ± 1684.1 ± 217,96.6 ± 4.8
071010B26.0360.9474.8657 ± 60.4227 ± 11412.5 ± 4.417,925.1 ± 29.5
8.4617 ± 47341 ± 414.2 ± 0.517,95.0 ± 13.8
090328100570.7368.4621 ± 64686 ± 2616.1 ± 0.77,93.1 ± 9.3
09102045.6391.7108.4690 ± 41.1399 ± 2110.9 ± 0.617,922.6 ± 10.4
100814A59.71751.444.5085 ± 27496 ± 2413 ± 117,917.1 ± 5.5
100901A17.84391.4084.5075 ± 40331 ± 304.917,922.7 ± 12.3
High-luminosity GRBs
9708282961470.9581.4314 ± 2257 ± 51208.110,1024.6 ± 44.4
8.4632 ± 20.5144 ± 317.8 ± 1.810,922.2 ± 15.0
9803292100582–3.91.4338 ± 25.5134 ± 43113.5432,3228.4 ± 21.1
4.8622 ± 37171 ± 1491.5 ± 11.332,912.9 ± 21.7
8.4613 ± 11332 ± 1133.5 ± 1.432,93.9 ± 3.3
99012323901001.6008.467.7 ± 11.1260 ± 3224.6521,213.0 ± 4.3
9905069492201.3078.4631 ± 27.6581 ± 452.7031,315.3 ± 4.8
991208n110600.7061.4354.8 ± 44.4263 ± 498.9 ± 1.818,920.8 ± 17.3
8.4637.3 ± 25.81804 ± 247.8 ± 0.118,92.1 ± 1.4
991216675251.0208.4620 ± 24.7960 ± 671.4913,132.1 ± 2.6
000210200100.8508.4618 ± 9h93 ± 218.594,2519.4 ± 10.6
000911n8805001.0594.8610 ± 2571 ± 2311.126,914.1 ± 35.5
8.4633.7 ± 25.2263 ± 333.1 ± 0.326,912.8 ± 9.7
000926270252.0394.8658 ± 41.5460 ± 3116.9 ± 1.519,912.6 ± 9.1
8.4623 ± 9h629 ± 2412.1 ± 0.524,93.7 ± 1.4
0102221331701.4774.8623 ± 8h144 ± 472.324,916.0 ± 7.6
8.4638.8 ± 19.8344 ± 391.3517,1711.3 ± 5.9
0208138001131.2544.8623 ± 42349 ± 435.1517,176.6 ± 12.1
8.4630.8 ± 19.8323 ± 391.2417,179.5 ± 6.2
030226120691.9868.4635 ± 18171 ± 236.7 ± 117,1720.5 ± 10.9
050603500122.8218.4679 ± 49377 ± 5314.1 ± 1.817,1720.9 ± 13.3
050820A2002402.6154.8621 ± 51256 ± 782.1517,68.2 ± 20.1
8.4676 ± 30634 ± 620.936,612.0 ± 4.9
05090413001746.2908.4613 ± 2776 ± 1435.3 ±1.516,917.1 ± 35.7
0510226302000.8098.4641 ± 23268 ± 325.2 ± 0.717,915.3 ± 8.8
High-luminosity GRBs
070125955601.5484.86133 ± 21308 ± 7827.98,943.2 ± 12.9
8.4664 ± 181028 ± 1684.1 ± 28,96.2 ± 1.7
0710033241481.6044.8693 ± 52224 ± 543.817,941.5 ± 25.3
8.46109 ± 45616 ± 576.5 ± 0.517,917.7 ± 7.5
09032341001333.578.4627 ± 38243 ± 1315.6 ± 17,911.1 ± 15.7
090902B30901.8838.4618 ± 1684 ± 1614.1 ± 2.67,921.4 ± 19.5
100414A779261.3688.4620 ± 16524 ± 198 ± 0.317,93.8 ± 3.1
GRBs without known redshifts
980519304.8625 ± 27330 ± 4717.9 ± 2.414,97.6 ± 8.3
8.4649 ± 28205 ± 2312.6 ± 1.314,923.9 ± 13.9
0010073758.4634 ± 61222 ± 337.117,915.3 ± 27.6
001018318.4670 ± 23.3590 ± 684.7 ± 0.617,911.9 ± 4.2
021206204.8658 ± 24480 ± 697 ± 0.817,912.1 ± 5.3
041219A64.8633 ± 48473 ± 286.3 ± 0.917,97.0 ± 10.2
8.4663 ± 42518 ± 1501.6917,1712.2 ± 8.8
050713B1254.8644 ± 69623 ± 5321.0117,177.1 ± 11.1
8.4659 ± 40.5373 ± 2414.1 ± 0.917,915.8 ± 10.9
GRB|$E_{\rm iso}^a$||$T_{90}^a$|zaFrequencyHost flux densityPeak flux densitybPeak timeReferencescRRF
(1051 erg)(s)(GHz)(μJy)(μJy)(days)(per cent)
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)
Low-luminosity GRBs
020903n0.023130.2501.4343 ± 66294 ± 9136.7328,914.6 ± 14.8
4.8621 ± 34782 ± 2836.7 ± 1.328,92.7 ± 4.4
8.46190 ± 301058 ± 1923.8028,918.0 ± 2.9
031203n0.115300.1051.43254 ± 46h929 ± 6065.5 ± 5.322,927.3 ± 5.3
4.86393 ± 60828 ± 2858.4 ± 2.127,947.5 ± 7.4
8.4653 ± 52724 ± 1948 ± 1.327,97.3 ± 7.2
050416An1.0030.6504.8650.5 ± 41.8485 ± 3648.5 ± 3.530,910.4 ± 8.7
8.4620 ± 51373 ± 3649 ± 3.630,97.3 ± 13.7
060218n0.0031280.0331.4369.5 ± 69.5198 ± 584.929,935.1 ± 36.6
4.8632 ± 32245 ± 503.8 ± 0.729,913.1 ± 13.3
8.4622.8 ± 20.5471 ± 832 ± 0.329,94.8 ± 4.4
100418An0.52070.6208.46366 ± 531218 ± 1247.6 ± 0.623,930.1 ± 4.4
Standard GRBs
9705087.10140.8351.43100 ± 32381 ± 19179.1 ± 7.615,926.3 ± 8.5
4.86104 ± 44780 ± 1357.6 ± 0.915,913.3 ± 5.6
8.468 ± 19958 ± 1137.2 ± 0.417,90.8 ± 2.0
98070369.0900.9661.4368 ± 6.6h263 ± 8125.4 ± 5.53,925.9 ± 8.4
4.8642.1 ± 8.6h1055 ± 309.1 ± 0.23,94.0 ± 0.8
8.4639.3 ± 4.9h1370 ± 3010 ± 0.23,92.9 ± 0.4
9812265.90201.118.4612 ± 22.6137 ± 348.2 ± 1.612,98.8 ± 1.7
000301C43.7102.0344.8685 ± 33240 ± 534.31,935.4 ± 15.8
8.4618 ± 7h520 ± 2414.1 ± 0.524,93.5 ± 1.4
00041875.1301.1191.4348 ± 15h210 ± 18016.564,222.9 ± 20.9
4.86110 ± 52897 ± 3927 ± 14,912.3 ± 5.8
8.4637 ± 12h1085 ± 2218.1 ± 0.34,93.4 ± 1.1
0109219.00240.4504.8627 ± 25161 ± 2031.5 ± 3.317,916.8 ± 15.7
8.4643.7 ± 21.3229 ± 2227.0117,919.1 ± 9.5
01121163.04002.1408.4624 ± 16162 ± 1313.2 ± 1.617,914.8 ± 9.9
020819B7.90500.4108.4644.7 ± 23291 ± 2112.2 ± 1.120,915.4 ± 8.0
02100438.0502.3304.8678 ± 28470 ± 2632.2 ± 1.417,916.6 ± 6.0
8.4659.4 ± 19.5780 ± 2318.7 ± 0.517,97.6 ± 2.5
021211n11.081.0108.4612 ± 3660 ± 288.8511,1120.0 ± 60.7
030329n18.0630.1691.43450 ± 1092232 ± 3078.6 ± 2.15,920.3 ± 4.9
4.86332 ± 51.710337 ± 3332.9 ± 0.15,93.2 ± 0.5
8.46248 ± 48.219567 ± 2817.3 ± 0.15,91.3 ± 0.3
050824n1.50230.8308.4636 ± 27156 ± 347.217,923.1 ± 18.0
070612A9.123690.6174.86222 ± 42.3580 ± 20140.3 ± 5.817,938.3 ± 7.4
8.4668 ± 491028 ± 1684.1 ± 217,96.6 ± 4.8
071010B26.0360.9474.8657 ± 60.4227 ± 11412.5 ± 4.417,925.1 ± 29.5
8.4617 ± 47341 ± 414.2 ± 0.517,95.0 ± 13.8
090328100570.7368.4621 ± 64686 ± 2616.1 ± 0.77,93.1 ± 9.3
09102045.6391.7108.4690 ± 41.1399 ± 2110.9 ± 0.617,922.6 ± 10.4
100814A59.71751.444.5085 ± 27496 ± 2413 ± 117,917.1 ± 5.5
100901A17.84391.4084.5075 ± 40331 ± 304.917,922.7 ± 12.3
High-luminosity GRBs
9708282961470.9581.4314 ± 2257 ± 51208.110,1024.6 ± 44.4
8.4632 ± 20.5144 ± 317.8 ± 1.810,922.2 ± 15.0
9803292100582–3.91.4338 ± 25.5134 ± 43113.5432,3228.4 ± 21.1
4.8622 ± 37171 ± 1491.5 ± 11.332,912.9 ± 21.7
8.4613 ± 11332 ± 1133.5 ± 1.432,93.9 ± 3.3
99012323901001.6008.467.7 ± 11.1260 ± 3224.6521,213.0 ± 4.3
9905069492201.3078.4631 ± 27.6581 ± 452.7031,315.3 ± 4.8
991208n110600.7061.4354.8 ± 44.4263 ± 498.9 ± 1.818,920.8 ± 17.3
8.4637.3 ± 25.81804 ± 247.8 ± 0.118,92.1 ± 1.4
991216675251.0208.4620 ± 24.7960 ± 671.4913,132.1 ± 2.6
000210200100.8508.4618 ± 9h93 ± 218.594,2519.4 ± 10.6
000911n8805001.0594.8610 ± 2571 ± 2311.126,914.1 ± 35.5
8.4633.7 ± 25.2263 ± 333.1 ± 0.326,912.8 ± 9.7
000926270252.0394.8658 ± 41.5460 ± 3116.9 ± 1.519,912.6 ± 9.1
8.4623 ± 9h629 ± 2412.1 ± 0.524,93.7 ± 1.4
0102221331701.4774.8623 ± 8h144 ± 472.324,916.0 ± 7.6
8.4638.8 ± 19.8344 ± 391.3517,1711.3 ± 5.9
0208138001131.2544.8623 ± 42349 ± 435.1517,176.6 ± 12.1
8.4630.8 ± 19.8323 ± 391.2417,179.5 ± 6.2
030226120691.9868.4635 ± 18171 ± 236.7 ± 117,1720.5 ± 10.9
050603500122.8218.4679 ± 49377 ± 5314.1 ± 1.817,1720.9 ± 13.3
050820A2002402.6154.8621 ± 51256 ± 782.1517,68.2 ± 20.1
8.4676 ± 30634 ± 620.936,612.0 ± 4.9
05090413001746.2908.4613 ± 2776 ± 1435.3 ±1.516,917.1 ± 35.7
0510226302000.8098.4641 ± 23268 ± 325.2 ± 0.717,915.3 ± 8.8
High-luminosity GRBs
070125955601.5484.86133 ± 21308 ± 7827.98,943.2 ± 12.9
8.4664 ± 181028 ± 1684.1 ± 28,96.2 ± 1.7
0710033241481.6044.8693 ± 52224 ± 543.817,941.5 ± 25.3
8.46109 ± 45616 ± 576.5 ± 0.517,917.7 ± 7.5
09032341001333.578.4627 ± 38243 ± 1315.6 ± 17,911.1 ± 15.7
090902B30901.8838.4618 ± 1684 ± 1614.1 ± 2.67,921.4 ± 19.5
100414A779261.3688.4620 ± 16524 ± 198 ± 0.317,93.8 ± 3.1
GRBs without known redshifts
980519304.8625 ± 27330 ± 4717.9 ± 2.414,97.6 ± 8.3
8.4649 ± 28205 ± 2312.6 ± 1.314,923.9 ± 13.9
0010073758.4634 ± 61222 ± 337.117,915.3 ± 27.6
001018318.4670 ± 23.3590 ± 684.7 ± 0.617,911.9 ± 4.2
021206204.8658 ± 24480 ± 697 ± 0.817,912.1 ± 5.3
041219A64.8633 ± 48473 ± 286.3 ± 0.917,97.0 ± 10.2
8.4663 ± 42518 ± 1501.6917,1712.2 ± 8.8
050713B1254.8644 ± 69623 ± 5321.0117,177.1 ± 11.1
8.4659 ± 40.5373 ± 2414.1 ± 0.917,915.8 ± 10.9

aRefer to Chandra & Frail (2012).

bObserved radio peak flux density.

cReferences are in the following order: host radio flux density, radio peak flux density.

Abbreviations for the references are as follows: (1) Berger et al. (2000), (2) Berger et al. (2001a), (3) Berger et al. (2001b), (4) Berger et al. (2003a), (5) Berger et al. (2003c), (6) Cenko et al. (2006), (7) Cenko et al. (2011), (8) Chandra et al. (2008), (9) Chandra & Frail (2012), (10) Djorgovski et al. (2001), (11) Fox et al. (2003), (12) Frail et al. (1999), (13) Frail et al. (2000a), (14) Frail et al. (2000b), (15) Frail, Waxman & Kulkarni (2000), (16) Frail et al. (2006), (17) Frail & Chandra (2014, private communication), (18) Galama et al. (2003), (19) Harrison et al. (2001), (20) Jakobsson et al. (2005), (21) Kulkarni et al. (1999), (22) Michałowski et al. (2012), (23) Moin et al. (2013), (24) Perley & Perley (2013), (25) Piro et al. (2002), (26) Price et al. (2002), (27) Soderberg et al. (2004a), (28) Soderberg et al. (2004b), (29) Soderberg et al. (2006), (30) Soderberg et al. (2007), (31) Taylor et al. (2000), (32) Yost et al. (2002).

hHost flux densities have been reported in Berger et al. (2001b), Berger et al. (2003a), Michałowski et al. (2012) and Perley & Perley (2013).

nSN/GRB, i.e. SN-associated GRBs.

These values are the maximum observed flux densities, which are taken as the observed peak flux densities.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close