Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 123
... detection to infer the true number of such objects that would be found , were the detection probabilities unity . In practice the range of absolute magnitude , redshift and SEDS of interest and the nonuniform distribution of quasars as ...
... detection to infer the true number of such objects that would be found , were the detection probabilities unity . In practice the range of absolute magnitude , redshift and SEDS of interest and the nonuniform distribution of quasars as ...
Page 257
... detection be statistically significant in every frame for every frame's data to be utilized . A detection can be re- tained if it is a 3o detection or greater in the aggregate of all available data for that particular patch of sky . Its ...
... detection be statistically significant in every frame for every frame's data to be utilized . A detection can be re- tained if it is a 3o detection or greater in the aggregate of all available data for that particular patch of sky . Its ...
Page 356
... detection limits close to σ Dra , 7 Ceti , and e Eridani are still some five magnitudes too bright for the detection of giant planets . Nonetheless , we remain optimistic that , with improved centering , the introduction of frame ...
... detection limits close to σ Dra , 7 Ceti , and e Eridani are still some five magnitudes too bright for the detection of giant planets . Nonetheless , we remain optimistic that , with improved centering , the introduction of frame ...
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absorption abundance accretion analysis asteroids 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 pixel 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 stellar winds subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir