Table 5: Intrinsic Peak Energy, Isotropic Energy [1, 1000 keV] and redshift values or constraints for 14 XRRs/XRFs: the Type column indicates if the measure of the redshift is obtained from Host Galaxy spectroscopy (HG), or from Optical afterglow spectroscopy (OT). We report also the pseudo-redshift for 6 possibly high redshift GRBs(16).
Burst $ \tilde{E}_{\rm p}$(keV) $ E_{\rm iso}$ (1052 erg) z Type Burst pseudo-redshift
XRR 010921 $129\pm32$ 0.68 0.45 HG (1) XRF 990520 $0.6\pm1.0$
XRR 011030     <3.5 HG (2) XRF 990704 $0.2 \pm 0.1$
XRR 011211 $56\pm63$ 1.7 2.14 OT (3) XRF 011019 $0.6\pm0.6$
XRR 020124 $365\pm80$ 3.7 3.2 OT (4) XRF 021104 $1.2\pm1.1$ (8)
XRF 020427 <9 <0.08 <2.3 HG (2) XRR 021112 $4.6\pm4.3$
XRF 020903 <6 $4.8\times10^{-5}$ 0.25 HG (5) XRF 030823 $0.8\pm0.7$ (8)
XRR 021004 $266\pm176$ 0.9 2.33 OT (6)    
XRR 021211 $93\pm18$ 0.5 1.01 HG (7)    
XRR 030115 $129\pm32$ 0.68 2.2 HG (8)    
XRR 030329 $80\pm3$ 1.03 0.17 OT (9)    
XRR 030323     3.37 HG (10)    
XRR 030324 <555   <2.7 HG (11)    
XRR 030429 $128\pm44$ 0.4 2.65 OT (12)    
XRF 030528 $57\pm9$ 1 0.78 HG (13)    
XRF 030723 <28 <0.5 <2.1 OT (14)    
XRR 031220 $142\pm15$ 0.05 $1.90\pm0.30$ OT (15)    
(1) Bloom et al. (2001), (2) Bloom et al. (2003a), (3) Fruchter et al. (2001), (4) Hjorth et al. (2003), (5) Levan (2002b), (6) Chornock et al. (2002a), (7) Della Valle et al. (2003), (8) Pelangeon et al. (2006), (9) Bloom et al. (2003b), (10) Vreeswijk et al. (2004), (11) Nysewander et al. (2004), (12) Weidinger et al. (2003), (13) Rau et al. (2005), (14) Fynbo et al. (2004), (15) Melandri et al. (2005) (16) http://www.ast.obs-mip.fr/grb/pz

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