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OBSERVATORY | ![]() |
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OGLE I | 0.96 | 0.01 | 0.28 | 0.01 |
MOA I | 0.96 | 0.01 | 0.29 | 0.01 |
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1.08 | 0.01 | 3.06 | 0.05 |
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0.91 | 0.009 | -27.0 | 0.2 |
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0.99 | 0.17 | 242.3 | 75.0 |
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0.232 | 0.002 | 0.28 | 0.04 |
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6.24 | 0.06 | -3.9 | 0.2 |
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3.94 | 0.04 | 21.8 | 0.1 |
PLANET I South Africa (SAAO) | 5.60 | 0.05 | -1.9 | 1.6 |
PLANET I Australia, Tasmania (UTas) | 2.74 | 0.03 | 163.8 | 1.2 |
PLANET I Chile (Danish) | 14.45 | 0.15 | 13.0 | 0.4 |
PLANET I Australia (Perth) | 0.793 | 0.008 | 6.5 | 0.1 |
PLANET I South Africa (Boyden) | 9.59 | 0.09 | 447.3 | 0.6 |
Robonet R Faulkes North (Hawaii) | 0.115 | 0.001 | -0.26 | 0.02 |
Robonet R Faulkes South (Australia) | 0.129 | 0.001 | -0.229 | 0.009 |
Robonet R Liverpool (Canaries Island) | 2.75 | 0.03 | 17.7 | 0.3 |
Note: source flux and blending for
telescopes that observed OGLE 07-BLG-050. The given values corresponds
to the model with parallax and xallarap, in a case of a solar mass
companion for the source. They do not change significantly for the
other models.
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