Table 2:

Masses and radii of 57 transiting exoplanets, stellar masses, as well as most of the spectral types (SPT) taken from the Extrasolar Planets Enyclopaedia; status June 2009; http://www.exoplanet.eu/.
  Exoplanet $\frac{M_{{\rm pl}}}{M_{{\rm Jup}}}$ $\frac{r_{{\rm pl}}}{r_{{\rm Jup}}}$ $\rho_{\rm pl}$ $\frac{M_{{\rm star}}}{M_{{\rm Sun}}}$SPTd$\zeta $ $\frac{\Delta M_{{\rm pl}}}{M_{{\rm pl}^{10\%}}}$ $\frac{\Delta M_{{\rm pl}}}{M_{{\rm pl}^{25\%}}}$ $\frac{\Delta M_{{\rm pl}}}{M_{{\rm pl}^{60\%}}}$ $\frac{\Delta M_{{\rm pl}}}{M_{{\rm pl}^{100\%}}}$
F    [g cm-3]  [AU]  Mass loss [%]  
  CoRoT-3 b21.661.0126.081.37F3V0.0571.080.00020.00050.0010.0017
  CoRoT-4 b0.721.190.531.1F0V0.0901.190.120.30.731.212
  CoRoT-5 b0.461.280.271.00F9V0.0501.531.563.758.32.12.78
  HAT-P-2 b8.620.9512.431.29F80.0681.090.00070.0020.0040.0069
  HAT-P-4 b0.681.270.411.26F0.0451.550.902.175.078.02
  HAT-P-5 b1.061.260.661.16 ${\rm F^{x}}$0.0411.480.421.022.433.95
  HAT-P-6 b1.061.330.561.29F0.0521.390.280.701.682.75
  HAT-P-7 b1.771.360.871.47 ${\rm F^{x}}$0.0381.530.230.561.342.21
  HAT-P-8 b1.521.50.561.28 ${\rm F^{x}}$0.0491.420.230.561.352.23
  HAT-P-9 b0.781.40.351.28F0.0531.480.631.523.585.76
  OGLE2-TR-L9 b4.501.611.341.52F30.0411.390.050.110.270.44
  OGLE-TR-132 b1.141.180.861.26F0.0311.670.61.443.425.5
  OGLE-TR-182 b1.011.130.871.14 ${\rm F^{x}}$0.0511.320.190.461.111.83
  OGLE-TR-211 b1.031.360.511.33 ${\rm F^{x}}$0.0511.430.350.842.023.29
  SWEEPS-043.80.818.871.24 ${\rm F^{x}}$0.0551.120.0030.010.020.04
  TrES-4 b0.921.790.21.38F0.0491.701.273.016.910.73
  WASP-1 b0.891.360.441.24F7V0.0381.691.02.395.548.73
  WASP-12 b1.411.790.311.35F0.0233.685.9712.4923.4631.23
  WASP-14 b7.731.264.81.32F5V0.0371.250.010.020.050.08
  WASP-3 b1.761.310.971.24F7V0.0321.60.310.741.792.93
  WASP-7 b0.960.921.561.28F5V0.0621.210.070.170.40.67
  WASP-13 b0.461.210.321.03F90.0531.451.112.706.129.59
  WASP-15 b0.541.430.231.18F50.0501.621.663.988.7913.43
  X0-3 b11.791.228.121.21F5V0.0451.150.0020.0050.010.019
  X0-4 b1.721.340.891.32F5V0.0561.30.090.220.520.87
G             
  CoRoT-1 b1.031.490.370.95G0V0.0252.361.33.076.9910.81
  CoRoT-2 b3.311.471.310.97G0.0281.560.060.150.350.59
  HAT-P-1 b0.521.230.351.13G0V0.0551.430.320.781.883.07
  HD 149026 b0.360.651.591.3G0IV0.0431.320.160.380.931.53
  HD 17156 b3.211.023.721.24G00.1621.050.00040.0010.0030.004
  HD 209458 b0.691.320.371.01G0V0.0471.490.340.831.983.23
  HD 80606 b4.001.030.450.9G50.4531.02 $3.2\times10^{-5}$ $8.1\times10^{-5}$0.00020.0003
  OGLE-TR-10 b0.631.260.391.18G0.0421.610.481.162.764.46
  OGLE-TR-56 b1.291.30.731.17G0.0232.20.61.463.455.53
  SWEEPS-119.71.138.341.1 ${\rm G^{x}}$0.0301.240.0020.0050.010.02
  TrES-21.21.220.820.98G0V0.0371.470.140.340.831.36
  TrES-31.921.31.10.92G0.0231.810.220.521.262.08
  WASP-4 b1.121.420.490.9G7V0.0232.321.092.605.979.33
  WASP-5 b1.581.091.510.97G4V0.0271.550.110.280.681.12
  WASP-6 b0.51.220.340.88G80.0421.570.661.603.766.04
  WASP-8 b2.231.171.731.00G60.0791.130.0060.0140.0340.057
  WASP-9 b2.301.301.301.01G00.0311.490.070.160.390.65
  X0-1 b0.91.180.671G1V0.0491.350.120.290.691.15
  X0-5 b1.081.091.040.88G8V0.0491.280.060.150.360.59

K
             
  HAT-P-11 b0.080.421.340.81K40.0531.220.160.530.971.59
  HAT-P-3 b0.60.891.050.94K0.0391.380.070.170.410.68
  HAT-P-12 b0.210.960.300.73 ${\rm K^{x}}$0.0381.631.012.465.608.82
  HD 189733 b1.131.140.950.8K1-K20.0311.510.070.180.420.70
  Lupus-TR-3 b0.810.891.430.87K1V0.0461.260.020.060.150.24
  OGLE-TR-111 b0.531.070.540.82K0.0471.370.100.260.621.02
  OGLE-TR-113 b1.321.091.270.78K0.0231.690.100.230.560.93
  TrES-10.611.080.60.87K0V0.0391.480.130.320.761.26
  WASP-10 b3.061.083.010.71K50.0371.230.010.010.030.05
  WASP-11 b0.461.050.50.82K3V0.0441.430.150.380.911.51
  WASP-2 b0.881.021.040.84K1V0.0311.50.080.210.490.82
  X0-2 b0.570.970.770.98K0V0.0371.480.120.300.711.18

M
             
  GJ 436 b0.070.441.060.45M2.50.0291.410.431.412.514.08
Spectral types that are roughly estimated corresponding to the mass sequence are indicated with a superscript x. The lost mass is calculated over a period of 4 Gyr for three different values of heating efficiency (10%, 25%, 60%, 100%). The planetary densities and the Roche lobe related mass loss enhancement factor $\zeta $ are also given.

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