Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 81
... Correction ↓ Corrected at 72 Hz No Correction www 10 Corrected at 72 Hz Time ( s ) only able to remove ~ 95 % of the 3.3 Hz resonance . Hence , the residual peak at that frequency is merely an artifact of the finite 72 Hz closed - loop ...
... Correction ↓ Corrected at 72 Hz No Correction www 10 Corrected at 72 Hz Time ( s ) only able to remove ~ 95 % of the 3.3 Hz resonance . Hence , the residual peak at that frequency is merely an artifact of the finite 72 Hz closed - loop ...
Page 83
... correction frequency for a night of moderate 11.5 m s - 1 wind . Note that full tilt correction is only achieved for frequencies above ~ 60 Hz . 8 Christou has kindly performed a numerical simulation of the performance of brightest ...
... correction frequency for a night of moderate 11.5 m s - 1 wind . Note that full tilt correction is only achieved for frequencies above ~ 60 Hz . 8 Christou has kindly performed a numerical simulation of the performance of brightest ...
Page 707
dex . The corrected data are effectively based on the same model - atmosphere grid for the Sun and program stars ( see Sec . 3.5 of Paper III ) . The sign of the applied correction has been checked by comparing François's data with ...
dex . The corrected data are effectively based on the same model - atmosphere grid for the Sun and program stars ( see Sec . 3.5 of Paper III ) . The sign of the applied correction has been checked by comparing François's data with ...
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abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray