Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 118
... survey described below more imaginative than A , B , and C. Notwithstanding the uninspiring termi- nology , the differences among survey types are important . 4.1 Survey Type A : Find a Quasar The least demanding surveys might be termed ...
... survey described below more imaginative than A , B , and C. Notwithstanding the uninspiring termi- nology , the differences among survey types are important . 4.1 Survey Type A : Find a Quasar The least demanding surveys might be termed ...
Page 120
... survey is as large as in published work , and most previously known quasars in the area were recovered independently , therefore our survey is highly complete . " Common prac- tice is then to apply a small correction , of order 10 ...
... survey is as large as in published work , and most previously known quasars in the area were recovered independently , therefore our survey is highly complete . " Common prac- tice is then to apply a small correction , of order 10 ...
Page 286
... survey of the cluster was that of Cannon ( 1968 ) using plates separated by 32 yr with a scale of 8.2 / mm . Though the area covered by the survey was smaller ( 30 ′ by 30 ′ ) , it extended to mp ~ 17 . The key conclusion of Cannon ...
... survey of the cluster was that of Cannon ( 1968 ) using plates separated by 32 yr with a scale of 8.2 / mm . Though the area covered by the survey was smaller ( 30 ′ by 30 ′ ) , it extended to mp ~ 17 . The key conclusion of Cannon ...
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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