... of pixels (synthesised beams) within the primary FoV is given by P= L D 2 = 6.9 в 103 L 1km 2 12m D 2 (2) The xNTD will have multiple fields of view (M ; nominally 30) yielding a total field of view F , and the system temperature, T , is nominally 50 K ...
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Ссылки http://www.atnf.csiro.au/projects/askap/newdocs/psr_survey.pdf -- 42.6 Кб -- 01.09.2006 Похожие документы
... 103 љ * As suggested by the commonality of the names, these are really the same . ... 124 љ * int m . 125 љ * Array axis number for index vectors. 126 љ * . ... 172 љ int m ; /* Array axis number for index vectors. */ . ...
... ux at a rest-frame wavelength of 0:5m. Note that no data is given for sources that ... B K Model 2 P = 2 C = PL p (m) R 0:5 PKS 0038 020 1.1780 s | ...
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Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/apC.ps.gz -- 57.5 Кб -- 29.03.2006 Похожие документы
... doubleљ . w [10] . љ . intљ . m . љ . intљ . n . љ . int(*љ . ... e.g. TAN is 0 (no parameters), SZP is 103 (1 to 3), and ZPN is 30 (0 to 29 ... in the prologue to each trio of projection routines in prj.c. int prjprm::m ...
... Get the factor to convert the given unit to m. static MSAntennaParse * . ... factor to convert the given unit to m. void casa::MSAntennaParse::makeAntennaList ... Definition at line 103 of file MSAntennaParse.h . ...
... G.P., MANCHESTER, R.N. & DOPITA, M.A.: "The central X-ray source in RCW 103: Evidence for blackbody emission" Astrophys ... R.N., LYNE, A.G., CAMILO, F., D'AMICO, N. & GAENSLER, B.M. "The 69 ms radio pulsar near the supernova remnant RCW 103 ...