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J/A+A/548/A90
  Looking for the rainbow on exoplanets (Karalidi+, 2012)
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2012A&A...548A..90K
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1.J/A+A/548/A90/fig5Planet with various cloud coverages at 550nm (1001 rows)
2.J/A+A/548/A90/fig7Planet with various cloud coverages at 865nm (360 rows)
3.J/A+A/548/A90/fig8Planet with two cloud layers of liquid water with various optical thicknesses at 550nm (G2) (91 rows)
4.J/A+A/548/A90/fig9Planet with two cloud layers, top layer icy cloud of variable optical thickness (540 rows)
5.J/A+A/548/A90/fig10Planet with two cloud layers, top layer icy cloud of thickness b=2 at various wavelengths (270 rows)
6.J/A+A/548/A90/fig11Planet with two cloud layers (top layer ice); the top layer covers a variable percentage of the underlying liquid water clouds (360 rows)
7.J/A+A/548/A90/fig12Planet with two cloud layers (top layer ice); the top layer covers 40% of the underlying liquid water clouds at various wavelengths (270 rows)
8.J/A+A/548/A90/fig14Model planet with 2 cloud layers: an ice water cloud and a liquid water cloud layer; based on data from MODIS/Aqua database. (180 rows)

Simple ConstraintList Of Constraints
 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1+2+6)Cov % [0/100] Cloud coverage (phys.area)
   (ALL)phi deg [0/180] Phase angle α (Note G1)   (src.orbital)
  (1+2+4+5+6+7+8)pi*Fn  Reflected total flux, π*Fn (phys.albedo)
  (1+2+5)pi*Fnp  Polarized flux, π*Fn,p (phys.albedo)
  (1+2+4+5+6+7+8)P  Degree of polarization (phys.polarization)
  (3)pi*Fn(10,1)  Reflected flux for bB=10, bA=1 (Note G2)   (phys.albedo)
  (3)pi*Fnp(10,1)  Polarized flux for bB=10, bA=1 (Note G2)   (phys.albedo)
  (3)P(10,1)  Polarization degree for bB=10, bA=1 (Note G2)   (phys.polarization)
  (3)pi*Fn(2,1)  Reflected flux for bB=2, bA=1 (Note G2)   (phys.albedo)
  (3)pi*Fnp(2,1)  Polarized flux for bB=2, bA=1 (Note G2)   (phys.albedo)

ALL cols		    
 (i)indexed column
  (3)P(2,1)  Polarization degree for bB=2, bA=1 (Note G2)   (phys.polarization)
  (3)pi*Fn(0,1)  Reflected flux for bB=0, bA=1 (Note G2)   (phys.albedo)
  (3)pi*Fnp(0,1)  Polarized flux for bB=0, bA=1 (Note G2)   (phys.albedo)
  (3)P(0,1)  Polarization degree for bB=0, bA=1 (Note G2)   (phys.polarization)
  (3)pi*Fn(10,0)  Reflected flux for bB=10, bA=0 (Note G2)   (phys.albedo)
  (3)pi*Fnp(10,0)  Polarized flux for bB=10, bA=0 (Note G2)   (phys.albedo)
  (3)P(10,0)  Polarization degree for bB=10, bA=0 (Note G2)   (phys.polarization)
  (3)pi*Fn(2,0)  Reflected flux for bB=2, bA=0 (Note G2)   (phys.albedo)
  (3)pi*Fnp(2,0)  Polarized flux for bB=2, bA=0 (Note G2)   (phys.albedo)
  (3)P(2,0)  Polarization degree for bB=2, bA=0 (Note G2)   (phys.polarization)
  (4+7+8)lambda nm Wavelength λ (em.wl)
  (5)b  Ice cloud optical thickness (phys.absorption.opticalDepth)

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