fk5 ; circle ( 128.835 , -45.179 , 0.3 ) # color = green text ={5} fk5 ; circle ( 129.349 , -42.897 , 0.3 ) # color = green text ={6} fk5 ; circle ( 135.531 , -40.556 , 0.3 ) # color = green text ={7} fk5 ; circle ( 140.098 , -55.206 , 0.3 ) # color = green text ={154} fk5 ; circle ( 119.926 , -38.726 , 0.3 ) # color = ...
Radio pulsars strictly periodic signals 14.03.2016 B 10 G;E 10 V / cm 12 10 2 Individual pulses and average profile of pulsar 14.03.2016 3 Average profiles of pulsars 14.03.2016 average energy distribution of pulses by phase of period. ... 14.03.2016 5 2695 Giant pulses (GPs) of pulsar Intensity, a.u. Time, ms Pulses that exceed the average profile over 30 times were called giant pulses. ... 2005) 14.03.2016 8 Individual pulses energy distribution 1937+21. ...
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Ссылки http://www.astro.spbu.ru/sobolev100/sites/default/files/kazantsev.pdf -- 2457.2 Кб -- 14.03.2016 Похожие документы
... This permits mapping V2,V3 to RA & DEC. ... The second running was with fine lock data , and with the code being told to output V2,V3s from the input RA, DEC Ex. 1 (coarse track, with velocity correction, ra/ dec output, 2 targets) squonk.stsci.edu% findtarget Is the data in fine lock? no Guide star file coarsefgs FGS A = 2 FGS B = 3 Give file name containing star positions coarsestars Do you wish to perform velocity aberration correction? yes Give the velocity ...
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Ссылки http://www.stsci.edu/hst/observatory/documents/isrs/findtarget.pdf -- 29.1 Кб -- 14.11.2003 Похожие документы
... done Forming the data quality image and setting some BAD pixels test256.fits - testspec1dq.fits Forming the noise image on the background rub1_19.fits - modelback1.fits specholucy input table for 3 point source spectra: X (pix) Y (pix) Slope (/pix) # Table demopos.tab Tue 14:39:34 25-Jan-2005 # row xchan ychan slope # 1 128.000 120.500 0 ... Point sources and background spectra NOT converged !- Point source no. 1; % flux change 17.98404 !- Point source no. 2; % flux change 55.14075 !- ...