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  2. /astro/p7scch2/AUMic/paper/figures/all.eps

    https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf
    16 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,
  3. 2001B information

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/2001b/
    16 Jun 2015: Aug 10; 02 20 09 9 24.2.
  4. Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...

    https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf
    2 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.
  5. Appendix C - Technical support and warranty

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/appc.htm
    16 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.
  6. Appendix XXX

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc
    16 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.
  7. arX iv:1 412. 0675 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwbb14.pdf
    15 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.
  8. arX iv:1 501. 0131 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf
    8 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
  9. arX iv:1 501. 0318 1v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/asgw15.pdf
    15 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].
  10. arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 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
  11. arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf
    25 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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