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/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, -
2001B information
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/2001b/16 Jun 2015: Aug 10; 02 20 09 9 24.2. -
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. -
Appendix C - Technical support and warranty
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/appc.htm16 Jun 2015: If a question cannot be answered immediately, due to the complexity of the enquiry for instance, further assistance will be provided with 24 hours of the enquiry being logged. -
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. -
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. -
arX iv:1 501. 0131 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf8 Jan 2015: K2.5V 0.072 1.30 n (T08)9826 υ And 01:36:47.84 41:24:19.6 3.5 F9V 0.136 2.36 n (A13) n ... 55.84 -09:27:29.7 3.2 K2V 0.172 7.39 n (A13) y (B09)22484 LHS 1569 03:36:52.38 00:24:06.0 14.0 F8V -
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]. -
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 -
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
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