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Giulio Del Zanna -- Spectroscopic diagnostics and applications
www.damtp.cam.ac.uk/user/astro/gd232/research/diagnostics.html11 Jun 2003: Del Zanna G., 2002, proc. workshop on High resolution X-ray spectroscopy with XMM-Newton and Chandra, MSSL, 24 - 25 October 2002. -
The ESO Sky Calendar Tool
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/obsplan/200307/almanac/alm_0728.html18 Jul 2003: before new moon, RA and dec: 8 17 24, 23 33.9 The sun is down for 10.2 hr; 7.5 hr from eve->morn 18 deg twilight. -
https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/wfc_bynight.txt
https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/wfc_bynight.txt19 Feb 2003: Y:Y 2000-06-24:WFS-nonXID:Y:Y /data/cass03a/mike/wfs_jun2000/:Y:Y:Y:Y:Y:Y:Y:0.083/0.005/0.020/15:./lplogs/20000624.int:: ... nonsurvey/itp_dec2000_reduced/:Y:Y:Y:S:S:S:S:0.097/0.005/0.025/23:./lplogs/20001217.int:: 2001-01-24:ITP-AXIS:Y:Y -
The ESO Sky Calendar Tool
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/obsplan/200307/almanac/alm_0729.html18 Jul 2003: Sunset ( 2326 m horizon): 21 13 GDT; Sunrise: 7 24 GDT Evening twilight: 22 34 GDT; LMST at evening twilight: 16 51 Morning twilight: 6 03 GDT; LMST at morning twilight: -
https://www.hep.phy.cam.ac.uk/~lester/dtm662/HepMC/GenEvent.h.patch
https://www.hep.phy.cam.ac.uk/~lester/dtm662/HepMC/GenEvent.h.patch9 Oct 2003: HepMC_Version1.24/HepMC/GenEvent.h Mon Jul 14 22:34:57 2003 --- HepMC_Version1.24_Factor/HepMC/OLD/GenEvent.h Tue Oct 7 17:47:17 2003 20,50 // subject -
The ESO Sky Calendar Tool
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/obsplan/200307/almanac/alm_0730.html18 Jul 2003: Sunset ( 2326 m horizon): 21 12 GDT; Sunrise: 7 24 GDT Evening twilight: 22 33 GDT; LMST at evening twilight: 16 54 Morning twilight: 6 03 GDT; LMST at morning twilight: -
PII: S0304-3991(97)00070-3
https://www2.mrc-lmb.cam.ac.uk/groups/nu/pdf/ultram97.pdf4 Apr 2003: x (A) 2 (4 (0 b&z) cp (dd’. Median 1.3 0.9 0.28 0.29 S.D.d 2.1 1.1 0.24 0.31. ... Range O&24.3 0.0-8.3 O&1.11 O.Gl.99. “All the figures shown were calculated after each whole repeat had been aligned to the reference structure. -
AUTOMATIC COMPLEXITY CONTROL FOR HLDA SYSTEMS X. Liu, M. ...
mi.eng.cam.ac.uk/reports/svr-ftp/liu_icassp2003.pdf19 Sep 2003: Fig. 1. Test set word error rate for all possible models, with thestandard front-end 12, 16 and 24 component performance. ... The best perfor-mance, 36.8%, was obtained using 24 components per state and anHLDA projection from 52 dimensions to 38 -
C:\Documents and Settings\Sergio\My Documents\Papers\Wrinkled…
www-civ.eng.cam.ac.uk/dsl/publications/Barcelonapaper.pdf24 Apr 2003: λ(δ1 δ2)π. (24). Here δ1 and δ2 are the radial displacements of the corners loaded by T1 and T2, respectively;these corner displacements can be estimated from. ... The wavelength predictions are very close.The wrinkle amplitudes have been estimated -
Tale-46.dvi
www.tcm.phy.cam.ac.uk/~dek12/tales/Tale-46.pdf18 Oct 2003: "#$ %&')( ,. -/.1024365"798:;24<>=,:?8@7A0"7CBEDF?84GIHJ.184KL795NMPOQ3R5"790PBS3RT9:1UV8@7924362 BW?8S2? HX=03YBUZ7[0"?BW]:105_.1H8@792@3R2 BW:10TC7a b[c&de],:fBg362LBS]"7h8@792@3R2 ... 34n '51 1. ,3n4. mFÀTC.)24 TC.)2nÀT9.)2ÀÇT9.)2. n)b orm)m[t. :.
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