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3521. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/analys_data.1.mac
search $1 # plot the data, then try a wide range of smoothings # plot the S/N as a function of boxcar width # data $1 read {y 1} set x=1,$( dimen (y)) limits x y box connect x y stats y a s k vecminmax y mn mx echo sigma=rms= $s for $( dimen (y)) points echo ave $a +- $($s/sqrt( dimen (y))) echo max $mx +- $s (S/N = $($mx/$s)) echo min $mn +- $s (S/N = $(abs($mn/$s))) set dimen (ym)=80 set ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/analys_data.1.mac -- 2.8 Кб -- 04.10.2001
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3522. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/optimal_smooth_demo.mac
# : macro read gauss_test.sm = loads macro into sm # : noisedemo 1000 = runs macro with 1000 pts # define N $1 set x=1,$N # dummy call to get ws dimensioned right get_hist x v ws -.5 .5 .02 set ws=ws*0 erase window 1 1 1 1 set y=x*0 limits 0 $N -.7 0.7 box ptype 1 1 # generate a lot of points to uniformly cover -0.5 to 0.5 # -and- at the same time do averages of 10 samples = pseudo-gaussian do i=1,10 { set t=random($N)-0.5 ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/optimal_smooth_demo.mac -- 4.7 Кб -- 04.10.2001
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3523. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/stacker.sm
data data.6 read {y 1} define DIM (dimen(y)) set dimen(xsum)=128 set dimen(xsum2)=128 set x=1,$DIM define N 0 do i=1,$DIM,128{ set yl=y if(x>=$i&&x<$i+128) set xsum=xsum+yl set xsum2=xsum2+yl**2 define N ($N+1) } set x=1,128 set xave=xsum/$N set err=sqrt((xsum2/$N - xave**2)/$N) limits 0 130 xave box connect x xave cursor erase box ptype 3 20 points x xave error_y x xave err relocate 0 0 draw 130 0 cursor ctype red connect x xave ctype 0 error_y x xave err ctype 0
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/stacker.sm -- 1.5 Кб -- 04.10.2001
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3524. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/dwarfs.PS
... Abstract (Concise summary of the proposal) WSRT observations of two of the dimmest, HI-selected dwarf galaxies SS47 and SS73 will provide reliable coordinates, as well as a rst look at their sizes and kinematical structure. ... Total number of hours requested this semester, including calibration: 26 6. ... To address the nature of these objects, we are studying three extreme examples (see Fig. 1) of tiny HI-selected objects from an Arecibo blind 21cm survey by Spitzak and Schneider 1998. ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/dwarfs.PS -- 1491.0 Кб -- 01.10.2001
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3525. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/0_README
Sample data files: The files data.1 through data.6 contain tables of numbers. Only data.5 has two columns; the other files have one column. The file data.5 contains `complex data' with the first column containing the real parts and the second column containing the imaginary. In sm, you can read data into the program by using the following statements: data datafilename read {y 1} The first line tells sm that the new data will be read from a file named `datafilename'. ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/0_README -- 1.7 Кб -- 27.09.2001
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3526. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/anoise_fft.sm
define hwid 25 set x=1,512 set y=x*0 set w=-1**x define N 512 set x=1,$N do i=1,10 { set t=random($N)-0.5 set y=y+t } set y=y/10 window 1 2 1 2 limits x y box connect x y window 1 2 1 1 set z=x*0 set y=y*w fft 1 y z r i set r=r*w set i=i*w set xt=x-257 set xx=xt concat xt set yy=r concat i limits xx yy ! limits -10 10 yy box connect xt r ctype red connect xt i ctype default
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/anoise_fft.sm -- 1.4 Кб -- 27.09.2001
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3527. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/box_fft.sm
define hwid 15 set x=1,512 set y=x*0 set w=-1**x define N 512 # set random 1001 set x=1,$N do i=1,10 { set t=random($N)-0.5 set y=y+t } set y=y/10 window 1 2 1 2 limits x -.3 .3 smooth y ys $hwid box ltype 1 connect x y ltype 0 ctype red connect x ys ctype default relocate 0 .25 label Boxcar width = $hwid window 1 2 1 1 set z=x*0 set y=ys*w fft 1 y z r i set r=r*w set i=i*w set xt=x-257 set xx=xt concat xt set yy=r concat i limits xx -.007 .007 ! ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/box_fft.sm -- 1.6 Кб -- 27.09.2001
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3528. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/cnoise_fft.sm
define hwid 25 set x=1,512 set y=x*0 set w=-1**x define N 512 set x=1,$N do i=1,10 { set t=random($N)-0.5 set y=y+t } set y=y/10 ! window 1 2 1 2 limits x y box ! ... limits -10 10 yy box connect xt r ctype red connect xt i ctype default define hwid 5 set f=x>(57-$hwid) && x < (57+$hwid) ? ... 1 : 0 set f=f+f2 set r=r*f set i=i*f window 1 3 1 2 box connect xt r ctype red connect xt i ctype default set r=r*w set i=i*w fft -1 r i y z set y=y*w window 1 3 1 1 limits x y connect x y ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/cnoise_fft.sm -- 1.7 Кб -- 27.09.2001
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3529. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/han_fft.sm
define hwid 15 set x=1, 512 set y=x*0 set w=-1**x define N 512 # set random 1001 set x=1,$N do i=1,10 { set t=random($N)-0.5 set y=y+t } set y=y/10 window 1 2 1 2 limits x -.3 .3 set filt={ 0.25 .5 0.25 } smooth2 y ys filt box ltype 1 connect x y ltype 0 ctype red connect x ys ctype default relocate 0 .25 label Hanning smooth window 1 2 1 1 set z=x*0 ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/han_fft.sm -- 1.7 Кб -- 27.09.2001
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3530. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/tester.sm
# use in supermongo by saying "input tester.sm" set x=random(1000) set y=random(1000) limits x y box points x y xlabel x ylabel y
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/tester.sm -- 1.1 Кб -- 20.09.2001
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3531. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/box.sm
to operate this progam, copy it to your own directory (as "box.sm"), # start sm, # (start a plot window if there is't one already with device x11). # while in sm, type: input box.sm # define N 10000 # "random" gives random numbers uniformly distributed between 0 and 1. # x & y below each are randomly distributed between -1 and +1. set x=2*random($N)-1 set y=2*random($N)-1 set t= x*x+y*y < 1 ? ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/box.sm -- 1.6 Кб -- 20.09.2001
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3532. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/tester.mac
randtest 2 set x=random($1) set y=random($1) echo $2 limits x y box points x y xlabel x ylabel y
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/tester.mac -- 1.1 Кб -- 13.09.2001
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3533. http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/gauss_test.mac
macro into sm # : noisedemo 1000 0 = runs macro with 1000 pts # = 0 means no errorbars define N $1 define DOERR $2 set x=1,$N # dummy call to get ws dimensioned right get_hist x v ws -.5 .5 .02 set ws=ws*0 erase window 1 1 1 1 set y=x*0 limits 0 $N -.7 0.7 box ptype 1 1 # generate a lot of points to uniformly cover - 0.5 to 0.5 # -and- at the same time do averages of 10 samples = pseudo-gaussian do i=1,10 { ...
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Ссылки http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/gauss_test.mac -- 4.3 Кб -- 11.09.2001
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3534. Software Maintenance Manual
... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document ?Programmatic Requirements for Gemini Instrumentation Development? states the requirements for the Software Maintenance Manual . ...
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Ссылки http://www.mso.anu.edu.au/nifs/manuals/man0003.htm -- 139.3 Кб -- 06.09.2001
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3535. Service and Calibration Manual
... Created: 22 January 2001 . ... SERVICE AND CALIBRATION MANUAL . ... Draft Document Outline. ... 4 Preparing NIFS for Use or Storage . ... The purpose of this Service and Calibration Manual is describe the procedures used to service, maintain, and calibrate the operation of the Gemini Near-infrared Integral Field Spectrograph. ... Section 19.4.2 of the document ?Programmatic Requirements for Gemini Instrumentation Development? states the requirements for the Service and Calibration Manual . ...
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Ссылки http://www.mso.anu.edu.au/nifs/manuals/man0002.htm -- 129.0 Кб -- 06.09.2001
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3536. NIFS User's Manual
... NIFS USER'S MANUAL . ... 8.2.1 BIAS Frames . ... This section will describe how to activate the GCAL flat field lamp, deploy the ISS science fold mirror to point to GCAL, configure the NIFS OIWFS, configure the NIFS OIWFS detector, and record a sequence of lamp on/off flat field frames. ... This section will describe how to configure ALTAIR, deploy the ISS science fold mirror to point to ALTAIR, configure the NIFS OIWFS, configure the NIFS OIWFS detector, and record a sequence of sky flats. ...
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Ссылки http://www.mso.anu.edu.au/nifs/manuals/man0001.htm -- 1260.1 Кб -- 06.09.2001
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3537. http://www.mso.anu.edu.au/pfrancis/roleplay/drake.doc
... The Milky Way is 30,000 light years across, about 1000 light years thick, and contains about 1011 stars (1 followed by 11 zeros, ie, 100,000,000,000, or one hundred thousand million stars). ... Life is tough! ... That means that life was well established when the Earth was only 1,000 million years old. ... It tells you that life got started on Earth pretty well as soon as it could! 4,000 million years ago, the Earth had only just solidified, and it was taking a punishing beating from meteorites. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/drake.doc -- 55.0 Кб -- 05.09.2001
[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/drake.doc -- 55.0 Кб -- 05.09.2001
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[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/drake.doc -- 55.0 Кб -- 05.09.2001
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3538. http://www.mso.anu.edu.au/pfrancis/roleplay/tac_roleplay_proposals.pdf
т n ej w 6 6 2Ї яu @q Vi V &y ?y Vv p v y ф hy q | ... pп hy i nt {j p? zy іy s ?h 6t Vv zu p Ry Шt } hu Іi e| pt ny Dm h h zt y o} j p v u z y Dp nh 6m 6 u ї} hy i їh к м Vк к Т VС м т Ў? о Ш V} hu Іi ?| pt hy ot 6m 6 y V~ zu h pt oy pm Fy 2? 6y o j @ Q i Ph eг h 6w nv hj zp z ny nm m pu 6y r p z py 6y v 6t r p ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/tac_roleplay_proposals.pdf -- 77.7 Кб -- 21.06.2001
[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/tac_roleplay_proposals.pdf -- 77.7 Кб -- 21.06.2001
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[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/tac_roleplay_proposals.pdf -- 77.7 Кб -- 21.06.2001
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3539. http://www.mso.anu.edu.au/pfrancis/roleplay/tac_roleplay_roles.pdf
Tp E H up 7H q yp t R 7V 7f sV TV TV gC ub D gV sb gH 7f 4 7C | ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/tac_roleplay_roles.pdf -- 63.6 Кб -- 21.06.2001
[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/tac_roleplay_roles.pdf -- 63.6 Кб -- 21.06.2001
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[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/tac_roleplay_roles.pdf -- 63.6 Кб -- 21.06.2001
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3540. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.blue_cuar
This CuAr arc unexpectedly has many lines of TiI in it. Lines of Ar I, Ar II and TiI Mean dispersion = 1.10 angstroms / channel Start wavelength = 3412.12 angstroms End wavelength = 5386.81 angstroms Central wavelength = 4394.55 angstroms 68 lines identified from /data/maestro1/ bessell /sp753b Channel Wavelength Calculated Discrepancy Line # 74.5088 3491.5359 3491.4761 -0.0598 1 95.5725 3514.3877 3514.2627 - ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.blue_cuar -- 5.8 Кб -- 14.06.2001
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