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 537
... detection network , are given in Appendix C. • able data in order to demonstrate how little data a neural network can require to learn a task . From a pragmatic point of view , we would like to analyze by hand as little data as possible ...
... detection network , are given in Appendix C. • able data in order to demonstrate how little data a neural network can require to learn a task . From a pragmatic point of view , we would like to analyze by hand as little data as possible ...
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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