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Table 9

Best fitting atmosphere model parameters, metallicity comparison.

Wavelength range Drift Drift, [M/H] = 0.0
Teff (K) log g [M/H] Teff (K) log g

DH Tau Ba
JHK (1.10–2.46 μm) 2700 3.5 –0.6 2000 4.0
J (1.10–1.34 μm) 1600 3.5 0.0 1600 3.5
HK (1.46–2.46 μm) 2700 3.0 –0.6 2700 4.0

GQ Lup Ba
JHK (1.10–2.46 μm) 1700 3.5 0.0 1700 3.5
J (1.10–1.34 μm) 2600 3.5 –0.6 2600 4.0
HK (1.46–2.46 μm) 1600 4.0 –0.6 1700 4.0

CT Cha Ba
JHK (1.10–2.46 μm) 1600 3.0 –0.6 1700 3.5
J (1.10–1.34 μm) 1700 3.0 0.0 1700 3.0
HK (1.46–2.46 μm) 1800 4.0 0.3 1800 4.0

2MASS 1207 A
JHK (1.10–2.46 μm) 2900 4.5 –0.6 3000b 4.5
J (1.10–1.34 μm) 2900 4.5 –0.6 2900b 4.5
HK (1.46–2.46 μm) 2900 4.5 –0.6 3000b 4.5

TWA 5 B
JHK (1.10–2.46 μm) 2200 3.0 0.0 2200 3.0
J (1.10–1.34 μm) 2700 4.0 –0.6 2800 4.5
HK (1.46–2.46 μm) 1800 4.0 0.3 1700 4.5

2MASS 1207 B
JHK (1.10–2.46 μm) 1700 4.0 0.3 1500 4.0
J (1.10–1.34 μm) 1500 3.5 –0.6 1700 4.0
HK (1.46–2.46 μm) 1700 4.0 0.3 1500 3.0

GSC 08047 B
JHK (1.10–2.46 μm) 1900 4.5 0.0 1900 4.5
J (1.10–1.34 μm) 1600 3.5 0.0 1600 3.5
HK (1.46–2.46 μm) 1800 4.5 0.3 1700 4.0

2MASS 0141
JHK (1.10–2.46 μm) 1700 4.0 0.0 1700 4.0
J (1.10–1.34 μm) 1600 3.5 0.0 1600 3.5
HK (1.46–2.46 μm) 1800 5.0 0.3 1800 5.0

AB Pic B
JHK (1.10–2.46 μm) 1600 4.5 0.0 1600 4.5
J (1.10–1.34 μm) 1800 4.5 0.3 1600 3.5
HK (1.46–2.46 μm) 1800 5.0 0.0 1800 5.0

Notes. 

(a)

These star formation region members have been dereddened as described in Sect. 4.

(b)

Note that this Teff falls at the extremes of the grid used.

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