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1 - 10 of 42 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 42 match some words.

  1. Results that match 1 of 2 words

  2. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060105.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060105.txt
    9 Jan 2006: The last GANTT chart we have says 24 March, but it is unclear if this is the current target date.

  3. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html
    26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7.

  4. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/
    26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7.

  5. {\bf WFCAM Catalogues}

    https://people.ast.cam.ac.uk/~wfcam/docs/catalogues.html
    4 Feb 2006: 24 Aperture flux 3 Recommended if a single number is required to represent the flux for ALL. ... 24 arcsec diameter. 45 Error in flux The aperture fluxes can be combined with later-derived aperture.

  6. Oxford Meeting

    https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt
    15 Apr 2006: B440022.122.24.82.6. V550021.321.49.63.5. R600020.420.817.93.9. I750019.520.035.25.2. Z890018.218.7117.26.3. J12,50016.016.9609.39.3.

  7. Placing Our Solar System in Context:[A 12 step program ...

    https://people.ast.cam.ac.uk/~wyatt/mmeyer_etal_ppv.pdf
    19 Apr 2006: MIR.but more common around stars < 100 Myr. MIPS 24 um image of Vega disk. ... MIPS-24 MIPS-70. MIPS-160 JCMT-450CSO-350. HST. Do Stars with Inner Planets (< 5 AU) Also Have Kuiper Disks?

  8. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 Apr 2006: Corresponding peak. signal-to-noise ratios are 27, 48, 24 and 15, respectively. ... We used thestandard g Reticulum to determine the PSF at 24.6 mm.

  9. L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...

    https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf
    19 Apr 2006: 24(40 AU) in ground-based, near-infrared, coronagraphic images.They estimated the disk position angle as , inclination50 1027 deg, and minimum dust mass 0.4 M. ... Trilling &2. Brown (1998) report an H-band disk surface brightness thatfalls below 24 mag

  10. mnr9848.tex

    https://people.ast.cam.ac.uk/~wyatt/gfw05.pdf
    19 Apr 2006: This latter study is based on weak IRAS excesses,and four of the six systems identified with IRAS at 25 µm do nothave 24-µm excesses on re-examination by Spitzer

  11. Modeling the Structures of Dusty Disks: UnseenPlanets? Mark C. ...

    https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf
    19 Apr 2006: to the Sun, at about 23 AU, then migratedoutward to its current 30 AU orbit [24]. ... Sci., 27, 287–312 (1999).24. Malhotra, R., Astron. J., 110, 420–429 (1995).25.

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