11. http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/lcu/pcr/user/v2_1/MONI.LST
... Position display AZ */ 13 ftext(m_pos[0],8,4,1,tpa0f); 14 outram(7,7,19,19,0x1f00,0,8,tpa0f); 15 16 /* Position display GD */ 17 ftext(m_pos[1],8,4,1,tpa0f); 18 outram(7,7,41,41,0x1f00,0,8,tpa0f); 19 20 /* Position display CH */ 21 ftext(m_pos[2],8,4,1 ...
12. http://www.naic.edu/general/PDF/RI/Luisa_Lara.pdf
... 23" Arecibo" Nov. 6, 17, 18, 20, 21, and 22" Dec. 14 and 17" 75 m-resolution images and CW echo spectra" " Goldstone" Nov. 20, 21, 22, and 25" 150 m-resolution images and CW echo spectra" " " Evidence for an equatorial ridge " 1999 KW4" " Disk-Integrated ...
13. http://www.naic.edu/~phil/hardware/pdev/fpga/gx/sp/src/ts_mult.v
... input ck; input [17:0] a; // signed input [15:0] b; // unsigned output [17:0] y; // signed `ifdef VIRTEX2 wire [35:0] prod; wire [17:0] yp; MULT18X18S m ( .P ( prod ), .A ( a ), .B ( {1'b0, b, 1'b0} ), .C ( ck ), .CE ( 1'b1 ), .R ( 1'b0 ) ); assign yp ...
14. http://www.naic.edu/vscience/schedule/tpfiles/CooketagT1463tp.pdf
... RQ §P ¤ё IЎ HG FE D )C B f U 6r rf A4 ¦o )p Тh X e o 52 p qf rm @4 98 17 Еj qi `m 5& ep f Ёr h o 52 p %# §4 ) %o §h 32 10 Еj i '& wm ro Bf )( '& m ¦ rp %$ )f h e ў# o S Еa Ca S q `§ ё )S f т )y f wЫ Vf S q `§ ё " !Ё ...
15. http://www.naic.edu/~astro/aotms/performance/99-01.pdf
... Sastr wemust apply MAZ: Sastr = MAZ SF;input = MAZ M,1 F MB Sobs : A+ 16 7 Thus the inverse of full system Mueller matrix is M,1 = MAZ M,1 F MB ; tot A+ and 17 Sastr = M,1 Sobs : tot 18 We beg the reader to forgive our unnecessary duplication of equations ...
16. Thesis Figures
... VLA H I 21cm DEC-VEL maps, in left-to-right order, right ascensions of 3 h 49 m 17 s , 3 h 49 m 00 s , 3 h 48 m 43 s , 3 h 48 m 26 s , 3 h 48 m 09 s , 3 h 47 m 52 s , 3 h 47 m 35 s , 3 h 47 m 19 s , 3 h 47 m 02 s , 3 h 46 m 45 s , 3 h 46 m 28 s , 3 h 46 m ...
17. http://www.naic.edu/~astro/chicago2/talks/Cordes-Radio_Transients.pdf
... Radio LSST highly synergistic Radio LSST also highly synergistic with highenergy instruments and gravitational wave telescopes Tucson Future cm/m Telescopes 17 8/21/2006 Extra Slides 8/21/2006 Tucson Future cm/m Telescopes 18 Raster Scanning for Slow ...
18. http://www.naic.edu/~tghosh/thesis-jf/chapter2.txt
... law over many decades of wavenumber, linking the structures responsible for radio scattering ($10^{9}$ m) with interstellar clouds ($10^{17}$ m) by suggesting that the cloud size represents the outer scale of a turbulent process with a power-law index ...
19. http://www.naic.edu/~astro/frontiers/talks/HC_fpa.pdf
... i Beam Former m . . . . . . MB NA © GermАn CortИs M 2007 17 Focal Phased Arrays National Astronomy and Ionosphere Center Aperture vs. ...
20. http://www.naic.edu/~tghosh/oct07/gbt-sb-mol-v3.ps
... hr, see below) observation of the Sgr B2 (R.A.=17 h 47 m 20.4 s ; Dec=28 # 23 # 05 ... T., 2005, PASJ, 57, L29 17 Aalto, S., Spaans, M., Weidner, M.C., Huttemeister, S ...