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http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/e0017_0035.sky2/GAL-Survey-115/id12_GAL-Survey-115.reg.

1. http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/e0035_0080.sky2/GAL-Survey-115-clean/id12_GAL-Survey-115-clean.reg
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 = ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/e0035_0080.sky2/GAL-Survey-115-clean/id12_GAL-Survey-115-clean.reg -- 1.8 Кб -- 18.06.2012
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2. http://www.astro.spbu.ru/sobolev100/sites/default/files/kazantsev.pdf
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. ...
[ Текст ]  Ссылки http://www.astro.spbu.ru/sobolev100/sites/default/files/kazantsev.pdf -- 2457.2 Кб -- 14.03.2016
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3. http://www.atnf.csiro.au/pub/people/vlbi/v175/v175c/v175cpa.systemp
System Temperature Log **** Log started: 014 14-JAN-2005 12:23:11 UT Cal size used (A): 1.00 (B): 1.00 014 14-JAN-2005 12:24:15 Tsys gain , a/b : 111.480 136.200 102.340 173.100 014 14-JAN-2005 12:24:31 Tsys gain , a/b : 113.338 133.900 103.100 171.850 014 14-JAN-2005 12:24:47 Tsys gain , a/b : 112.159 135.350 103.001 172.000 014 14-JAN-2005 12:25:03 Tsys ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pub/people/vlbi/v175/v175c/v175cpa.systemp -- 21.1 Кб -- 27.01.2005
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4. http://www.stsci.edu/hst/observatory/documents/isrs/findtarget.pdf
... 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 ...
[ Текст ]  Ссылки http://www.stsci.edu/hst/observatory/documents/isrs/findtarget.pdf -- 29.1 Кб -- 14.11.2003
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Еще в разделе: (Показать все результаты (>2) - www.stsci.edu/ )

5. http://www.winer.org/Downloads/MPEC2010-E52.pdf
MPEC 2010-E52 : DAILY ORBIT UPDATE (2010 MAR. ... A form allowing access to any MPEC is at the bottom of this page. ... K03E11C K03E16J K03E18C K03E19Y K03E26E K03E32X K03E46F K03F01M K03F07W K03F17X K03F34M K03F47Y K03F69F K03F75U K03F77U K03F80F 15.4 0.15 18.7 0.15 16.1 0.15 15.4 0.15 16.9 0.15 anguage to 15 15.9 0. this .2 ! 0.15 15 page 16.4 0.15 17.2 0.15 15.7 0.15 17.0 0.15 15.4 0.15 15.5 0.15 17.1 0.15 14.9 0.15 17.1 0.15 14.7 0.15 16.4 0.15 16.2 ...
[ Текст ]  Ссылки http://www.winer.org/Downloads/MPEC2010-E52.pdf -- 114.3 Кб -- 11.12.2013
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6. SPECINHOLUCY (V1.00) --- Dec02 stecf.specres --- SPECINHOLUCY (V1.00)
specinholucy -- Extract point source spectra from longslit spectrum image with inhomogeneous background spectrum using an iterative technique based on Richardson-Lucy restoration specinholucy inpima errima dqima poitab Rootab poi_back bakima bakerr bakdq psfima psfmeth psfb interpol posmeth icsum skernel niter epspoi epsbac ntrial seed dqlim verbose . ... The name of the input longslit spectrum image. errima = "" [file name] . ... Point sources and background spectra NOT converged !- ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/specres/specinholucy.hlp.html -- 20.8 Кб -- 08.06.2006
[ Сохраненная копия ]  Ссылки http://www.eso.org/~jwalsh/specres/specinholucy.hlp.html -- 20.8 Кб -- 13.12.2010
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7. http://www.stecf.org/software/IRAFtools/stecf-iraf/specres/demo/extra/rub1.txt
... 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 !- ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/specres/demo/extra/rub1.txt -- 52.2 Кб -- 08.06.2006
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