... of late vs early type galaxies II Apply the linearisation formula to get: R=F R R late /F early = 1.70 2 (13) 2 m Flate + m Fearly 20% (14) Managed to `rescue' a normal-distribution like estimate from clearly a non-normally distributed problem Note the ...
... 11 LOCAL OSCILLATOR............................................................................................................................................... 11 CRYOSTAT ............................................................................................................................................................... 11 CONTROL AND M ONITORING ................................................................................................................................ 13M ICROCOMPUTER & CONTROL SOFTWARE ........................................................................................................ 14 A CKNOWLEDGEMENT ............................................................................................................................................ 14 REFERECENES.. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/harp/public/Project_Overview.pdf -- 299.1 Кб -- 13.12.2005 Похожие документы
... Cambridge, 2009 Mar 25 RM Range and Frequency Resolution Default correlator resolution (256 channels per subband) allows one to measure a maximum RM of ±13 000 rad m-2 at 120 MHz |RM| 3 / (2c2ch) 30 200 50 900 120 13 000 240 MHz 100 000 rad m-2 200 MHz ...
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Ссылки http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/anderson_MKSP_hardware.pdf -- 1358.1 Кб -- 07.04.2009 Похожие документы
... The fit to the 24 µm luminosities in Figure 13(d) can be improved by increasing Nc , but this leads to an over-prediction of the 8-µm luminosities in Figure 13(c). 8 µm 24 µm a 9.45 ± 0.05 9.06 ± 0.04 b 0.87 ± 0.08 0.97 ± 0.07 N 75 81 Table 2. ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2008/dustgal1.pdf -- 1286.9 Кб -- 25.11.2009 Похожие документы