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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absorption abundance accretion analysis asteroids astrometry Astronomical Society binary bright calibration catalog central star chromospheric clouds color comets correction derived detection detector diagram disk distribution eclipse emission errors estimate evolution expansion velocities Fe/H field flux frame function galactic galaxies GCLF giant branch globular clusters H II regions Hyades indices infrared ionized km s¹ light curve lines luminosity magnitude main sequence main-sequence mass measured MNRAS objects observations Observatory obtained open clusters optical orbital parameters PASP period phase photometric pixels planetary nebulae plotted quasars radial velocities radius range ratio red giants reddening redshift region residuals rotation sample scale scatter secondary solar sources spectral type spectroscopic spectrum standard stellar subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir