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Did you mean pc524 |u:people.ast.cam.ac.uk?
1 - 10 of 77 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 77 match some words.

  1. Results that match 1 of 2 words

  2. 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

  3. 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.

  4. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/smw15.pdf
    15 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.

  5. 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].

  6. Draft version January 19, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf
    19 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.

  7. 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

  8. https://people.ast.cam.ac.uk/~optics/cirsi/ociw/g133_dupont.tcs

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/g133_dupont.tcs
    16 Jun 2015: position! G133_NW_D 01 03 42.43 -06 34 24.2 J2000.0 G133_NW_A 01 03 29.57 -06 34 24.2 J2000.0 G133_NW_C 01 ... G133_NE_D 01 04 30.43 -06 34 24.2 J2000.0 G133_NE_A 01 04 17.57 -06 34 24.2 J2000.0 G133_NE_C 01 04

  9. The LCIR survey at Cambridge

    https://people.ast.cam.ac.uk/~optics/cirsi/lcirs/
    16 Jun 2015: Wavebands and limiting magnitudes. band Nominal limiting mag 5sigma is 1.5 diameter aperture U from WHT [24.5] B from WHT [25.5] V from CTIO BTC 26.5 R ... SSA22 22 17 54.0 00 14 34. NICMOS 22hr 22 20 17.2 -24 43 27.

  10. CIRPASS

    https://people.ast.cam.ac.uk/~optics/cirpass/proposing.html
    16 Jun 2015: Last modified: Wed Nov 24 12:12:42 1999.

  11. https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-sds-1_dupont.tcs

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-sds-1_dupont.tcs
    16 Jun 2015: position! XMM-SDS-1-C_D | 02:18:06.41 | -04:58:24.2 | 2000 | 0 | XMM-SDS-1-C_A | 02:17:53.59 | -04:58:24.2 | 2000 | 0 | ... SDS-1-C_X | 02:18:00.00 | -05:00:00.0 | 2000 | 0 | XMM-SDS-1-NW_D | 02:17:42.41 | -04:52:24.2 | 2000 | 0 |

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