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 retained if it is a 30 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 retained if it is a 30 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 , τ Ceti , and € 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 , τ Ceti , and € 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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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