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Appendix XXX
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc16 Jun 2015: 23. M_ST4. DATA4. 53. AGND. GND5. 24. M_ST4. DATA4. 54. AGND. ... 22. RESET. 23. SAFETY GND. 24. NC. 25. NC. Changes. v1 Original form. -
Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...
https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf2 Nov 2015: EPIC 203410665 (V V896 Sco) and 203937317(DoAr 24) are both well-known members of ρ Oph thathave been studied in the near-IR (e.g., Furlan et al. ... 204630363 407050 K7.5 0.810.130.13 24.2118.2 — — — 15 C F/(P)TD. -
CIRSI: the Cambridge Infrared Survey Instrument for Wide-Field…
https://people.ast.cam.ac.uk/~optics/papers/CIRSI_SPIE_4008_146.doc16 Jun 2015: CIRSI gives a whole time on one fill of liquid nitrogen in excess of 30 hours in downward looking mode and approximately 24 hours in upward looking mode. -
proceedings2.dvi
https://people.ast.cam.ac.uk/~optics/dazle/publications/5492-1022-dazle.pdf16 Jun 2015: 9.18 12351.9 68.99 48.9 12400.8 16.89 100 Some contamination. 9.24 12423.7 37.60 58.8 12482.5 7.88 100 Some contamination. -
Next Generation Very Large Array Memo No. 6Science Working ...
https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf24 Oct 2015: 24. 5 Chemical evolution of the star and planet forming environ-ment 275.1 Complex organic molecules in Hot Molecular Cores. ... The cyan contours are –6, –3, 3, 6, 12, 24, 48, 96, 192 σI, whereσI = 19.5µJy bm1 is the rms noise in the Stokes I map. -
arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf25 Nov 2015: 110411† 154 7.0‡ 67.3 7.0‡. 125162 272 15‡ 142 12‡. 183324† 25.4 1.1 17.2 3.3198160 30.7 1.2 14.3 1.7221756† ... Star (HD) µra(mas/yr) µdec(mas/yr) vrad(km/s) Parallax(′′ ) Distance (pc). 11413 -48.27 0.24 -4.42 0.30 3.0 0.7 12.96 -
Draft version January 19, 2015Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf19 Jan 2015: 1 1 29/204 0.140.020.03 29/204 0.14. 0.020.03. 2 2 24/182 0.130.020.03 22/179 0.12. ... 6 1o 21/146 0.140.020.03 8/33 0.24. 0.060.09 7/49 0.14. 0.040.06 6/64 0.09. -
Project Reassessment Start Date
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc16 Jun 2015: 5.5.2 SAM Code GOTOBUTTON _Toc361307169 PAGEREF _Toc361307169 24. 5.5.3 Transputer GOTOBUTTON _Toc361307170 PAGEREF _Toc361307170 24. ... 5.5.4 Data Output Format GOTOBUTTON _Toc361307171 PAGEREF _Toc361307171 24. 5.6 Computer Interface GOTOBUTTON -
Draft version May 29, 2015Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf14 Sep 2015: Draft version May 29, 2015Preprint typeset using LATEX style emulateapj v. 5/2/11. A COMPACT CONCENTRATION OF LARGE GRAINS IN THE HD 142527 PROTOPLANETARY DUST TRAP. Simon Casassus1,2, Chris Wright3, Sebastian Marino1,2, Sarah T. Maddison4, Al -
Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pw15.pdf14 Sep 2015: Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed 17 July 2015 (MN LaTEX style file v2.2). Double-ringed debris discs could be the work ofeccentric planets: explaining the strange morphology ofHD 107146. Tim D. Pearce? and Mark C. WyattInstitute -
arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf10 Mar 2015: Theco-added spectrum consists of 27 observations of 20 minutesduration each, over 5 nights between 12 Nov 2013 and 24 Dec2013. ... albe. do. Qabs (24)Qsca (H)Qabs (H)Albedo. Figure 10. Scattering and absorption properties for silicate/organicgrains as a -
MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/rw15.pdf17 Dec 2015: T =2. πb(2)3/2(α). (a2a1. )5/2 f 2(1 L2. L1. )24. -
arX iv:1 412. 0675 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwbb14.pdf15 Jan 2015: arX. iv:1. 412. 0675. v1 [. astr. o-ph. EP. ] 1. Dec. 201. 4DRAF T VERS IONDECEMBER 3, 2014Preprint typeset using LATEX style emulateapj v. 5/2/11. EXO-ZODI MODELLING FOR THE LARGE BINOCULAR TELESCOPE INTERFEROMETER. GRANT M. K ENNEDY1, M ARK C. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/smw15.pdf15 Jan 2015: δE Gm (1 β)2ap. (1 2) , (24). and equating the two energies yields. ... 3. Allow-ing for capture into lower j resonances, the overall captureprobability into the 6:5 mean motion resonance for particleswith similar initial conditions is 0.24. -
arX iv:1 501. 0318 1v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/asgw15.pdf15 Jan 2015: around 24”, while in the SW wing it is present from 1” to 5”; not only is the emission more. ... 24 –. Disk Spine Position: Observations and Models. -200 -100 0 100 200Distance [au]. -
/astro/p7scch2/AUMic/paper/figures/all.eps
https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf16 Jun 2015: arX. iv:1. 506. 0456. 4v1. [ast. ro-p. h.E. P]. 15 J. un 2. 015. Astronomy & Astrophysicsmanuscript no. AUMic c ESO 2015June 16, 2015. Collisional modelling of the AU Microscopii debris discCh. Schüppler1, T. Löhne1, A. V. Krivov 1, S. Ertel2, -
https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_atmosph_transm…
https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_atmosph_transmission_nir.txt16 Jun 2015: # # rgm copied from #http://www.jach.hawaii.edu/JACpublic/UKIRT/astronomy/calib/atmosph_short.lines # 0.9000 9.60168E-01 0.9005 9.60579E-01 0.9010 9.61084E-01 0.9015 9.61924E-01 0.9020 9.63728E-01 0.9025 9.67188E-01 0.9030 9.72331E-01 0.9035 9.78154E
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