2010MmSAI..81..460B

Query : 2010MmSAI..81..460B

2010MmSAI..81..460B - Mem. Soc. Astron. Ital., 81, 460-466 (2010)

Can gamma ray bursts be used as effective tracers of star formation to high z?

BECKMAN J. and GIAMMANCO C.

Journal keyword(s):

Simbad objects: 18

goto View the references in ADS

Number of rows : 18
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 587 1
2 SN 2005kr SN* 03 08 29.67 +00 53 20.2   22.1       SNIc 25 1
3 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
4 SN 2006nx SN* 03 33 30.63 -00 40 38.2           SNIb/c 33 1
5 SN 2003bg SN* 04 10 59.43 -31 24 50.4     15.0     SNIc 170 1
6 SN 1997ef SN* 07 57 02.87 +49 33 41.3     16.5     SNIc-BL 281 1
7 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 576 0
8 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
9 SN 2007I SN* 11 59 13.15 -01 36 18.9   19.2 17.9     SNIc-BL 45 1
10 SN 2005nb SN* 12 13 37.61 +16 07 16.2     17.2     SNIc-BL 28 1
11 GRB 060510B gB 15 56 29.200 +78 34 12.00           ~ 155 0
12 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
13 SN 1998ey SN* 21 30 00.67 +26 43 21.4     17.0     SNIc 31 1
14 SN 2005ks SN* 21 37 56.56 -00 01 56.9   22.5       SNIc 23 1
15 SN 2006qk SN* 22 25 32.3 +00 09 14           SNIc: 24 1
16 GRB 020903 gB 22 48 42.34 -20 46 09.3           ~ 248 1
17 SN 2003jd SN* 23 21 03.38 -04 53 45.5   16.34       SNIc-BL 147 1
18 SN 1997dg SN* 23 40 14.21 +26 12 11.8   17.20       SNIa 50 2

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