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http://www.naic.edu/~astro/spectral_line/handbook_old/app/old_hi.html.
http://www.naic.edu/~astro/spectral_line/handbook_old/app/old_hi.html.
1. http://www.naic.edu/~astro/spectral_line/handbook_old/app/analyz_instruc.html
Next: Trouble Shooting at the Telescope Up: Spectral Line Appendices Previous: Basic Analyz Routines - For use with data taken AFTER March 6, 2000 . ... setvel : Uses the "optical" definition to convert frequencies to velocity, and then stores the velocities in register 41. ... Line 1 - The area, central velocity, and width at 50% of the mean flux. ... rcl 8;sto 501 To begin working on your data again, you must the restore both the data and frequecy info: rcl 500;sto 43;rcl 501;sto 8 . ... sto 43 . ...
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Ссылки http://www.naic.edu/~astro/spectral_line/handbook_old/app/analyz_instruc.html -- 17.7 Кб -- 18.05.2001
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2. http://www.naic.edu/~phil/mbeam/hipass.pdf
... 2.3 Data acquisition Spectra generated by the Multibeam correlator contain the usual structure seen in spectra from other H i instruments: a bandpass spectrum which is the sum of the sky , ground and receiver temperatures multiplied by the product of the filters in the receiver chain; superimposed on this is a noise ... Note also that sources extended much beyond ,40 arcmin can be imaged poorly in HIPASS images because of the bandpass sidelobe effect described in Section 3.3. ...
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Ссылки http://www.naic.edu/~phil/mbeam/hipass.pdf -- 370.1 Кб -- 14.03.2003
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