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Table 5:

$3\sigma $ upper limits for planetary nebulae in the SMC observed with XMM-Newton (Except for SMP SMC 25 for which we report the detected count rate).

Name(1) 		Rate(2) $L_{\rm BB}^{(3)}$ $L_{\rm TB}^{(4)}$ Observation date
  (10-3 cts s-1) (1034 erg s-1) (1034 erg s-1)  

SMP SMC 5 		3.7 67.5 2.5 2006/03/27
SMP SMC 7 1.1 20.5 0.8 2009/10/20
SMP SMC 8 2.2 40.6 1.5 2009/11/09
SMP SMC 9 1.5 27.5 1.0 2009/10/03
SMP SMC 10 2.9 53.5 2.0 2009/09/27
SMP SMC 12* 3.2 93.9 2.7 2007/10/28
SMP SMC 13* 1.7 50.6 1.5 2007/10/28
SMP SMC 14* 2.6 75.0 2.2 2007/10/28
SMP SMC 16 2.5 45.2 1.7 2007/06/23
SMP SMC 18 2.3 43.2 1.6 2007/04/11
SMP SMC 19 1.6 29.5 1.1 2006/11/01
SMP SMC 21 1.7 31.4 1.2 2009/10/09
SMP SMC 23 1.9 35.0 1.3 2009/10/11
SMP SMC 25 $3.2\pm0.9$ 58.5 2.2 2007/06/04
SMP SMC 27 1.2 22.9 0.9 2009/06/29
J2 1.8 33.9 1.3 2009/10/03
J4* 3.5 102.3 3.0 2007/10/28
J5 2.8 51.6 1.9 2009/10/03
J9 3.0 56.2 2.1 2007/04/11
J10 1.9 34.7 1.3 2009/09/27
J12 1.8 33.7 1.3 2009/09/27
J13 7.0 129.1 4.8 2007/06/23
J15 2.3 42.4 1.6 2007/06/23
J16 2.5 46.1 1.7 2007/06/23
J17 2.1 39.3 1.5 2007/04/11
J18 2.0 36.7 1.4 2006/11/01
J21 1.6 28.6 1.1 2009/11/04
J22 3.2 58.5 2.2 2007/06/23
J23 12.7 234.2 8.7 2009/10/11
J24 4.4 80.8 3.0 2009/10/11
J25 1.7 30.8 1.1 2009/10/11
J27 2.4 43.5 1.6 2009/10/11
MG8 1.6 29.1 1.1 2009/09/27
MG9 3.6 66.9 2.5 2007/06/06
MG10 3.2 59.4 2.2 2006/10/03
MG11 1.6 29.1 1.1 2009/11/30
MA14 2.1 38.0 1.4 2009/10/20
MA44 1.8 33.0 1.2 2009/10/18
MA406* 3.0 86.9 2.5 2007/10/28
MA891 4.0 74.5 2.8 2002/03/30
MA1357 4.2 76.9 2.9 2009/10/16
MA1714 1.6 29.0 1.1 2009/11/16
MA1762 2.6 47.4 1.8 2009/11/19
M7 1.9 36.0 1.3 2009/06/29
JD29 1.7 31.5 1.2 2009/10/18
JD51 2.8 51.8 1.9 2009/10/09
JD53 3.5 64.2 2.4 2007/06/06
JD57 1.3 24.2 0.9 2009/09/25

Notes. The sources marked by a star were observed with the medium optical filter, all the others with the thin one. (1) The names indicate the following references: SMP = Sanduleak et al. (1978), J = Jacoby (1980), MG = Morgan & Good (1985), MA = Meyssonnier & Azzopardi (1993), M = Morgan (1995), JD = Jacoby & De Marco (2002); (2) 0.1-1 keV count rate in the EPIC pn camera; (3) unabsorbed 0.1-1 keV luminosity for a black-body spectrum with kT=20 eV, $N_{\rm H}=5\times10^{20}$ cm-2, and d=60 kpc; (4) as (3) but for a thermal bremsstrahlung with kT=100 eV.


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