Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 92
... reduced in the J band , where order overlap becomes a problem . 3.4 Data Reduction A software package based on IRAF , has been developed to reduce cross - dispersed KSPEC data . The package is primarily intended for quick - look use at ...
... reduced in the J band , where order overlap becomes a problem . 3.4 Data Reduction A software package based on IRAF , has been developed to reduce cross - dispersed KSPEC data . The package is primarily intended for quick - look use at ...
Page 257
... reduced . A blob of flux that is reduced as a blended double star can be reduced as a blended double in every frame , always with exactly the same separation and position angle , but with independently determined magnitudes in each ...
... reduced . A blob of flux that is reduced as a blended double star can be reduced as a blended double in every frame , always with exactly the same separation and position angle , but with independently determined magnitudes in each ...
Page 260
... reduced together , the star - subtracted images combined and visually searched for new stars to add to the solution , and the ensemble of frames reduced again . The individual PC images are sufficiently small in area compared to the ...
... reduced together , the star - subtracted images combined and visually searched for new stars to add to the solution , and the ensemble of frames reduced again . The individual PC images are sufficiently small in area compared to the ...
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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