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1 - 10 of 29 search results for TALK:Vb20 24 / |u:people.ast.cam.ac.uk where 0 match all words and 29 match some words.

  1. Results that match 1 of 2 words

  2. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070201.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070201.txt
    14 Feb 2007: 21-24) and I am in the processes of dumping to disk the tapes with the fixed chips 1 & 2 hoping to get the remaining chips soon. ... Dec. 21-24). No data for 06B have been transferred yet to ESO because of the missing NDR data: it made sense to us to

  3. https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/summary.list

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/summary.list
    3 Sep 2007: 1.311 2001-06-08 01:08:24 24.07 J 0.81 1450.9 7.5 0.21 0.11 0.25 w_20010607_06614_2 1637-046B ... 1.311 2001-06-08 01:08:24 24.07 J 0.96 1588.9 8.1 0.17 0.11 0.28 w_20010607_06614_3 1637-046B

  4. Microsoft PowerPoint - wyattpub

    https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf
    24 Apr 2007: stars at 24,70,160μm• Akari (2006-) currently doing all-sky survey 2-180μm• Herschel (2008-) observations at 60-670μm• Spica (2017+) planned 5-200μm. ... Structure is wavelength dependent!850μm. (Holland et al. 2006)24 and 70μm. (Su et al.

  5. MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...

    https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf
    3 Jul 2007: 1), which fits the three longest wavelength fluxes, but cannotreproduce the 24 m flux. ... 1999, ApJ, 512, 377Hildebrand, R. 1983, QJRAS, 24, 267Holland, W. S., et al.

  6. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p1.pdf
    5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)

  7. Submitted to ApJ, 3 January 2007, accepted 22 March ...

    https://people.ast.cam.ac.uk/~wyatt/wssr07.pdf
    23 Mar 2007: The 150t1age line delineatingthe upper envelope of the 24 µm detections (Rieke et al. ... 4.2.1. Sample of 46 A star disks detected at 24 and 70µm.

  8. https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/summary.lis…

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/summary.list
    3 Sep 2007: 1.311 2001-06-07 21:23:46 24.08 J 0.97 1936.2 4.5 0.12 0.05 0.30 w_20010607_06523_sf_2 CIRSI_NGC135A ... 1.311 2001-06-08 05:12:43 24.01 J 0.97 1398.8 3.6 0.08 0.03 0.36.

  9. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/
    3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made.

  10. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html
    3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made.

  11. https://people.ast.cam.ac.uk/~rgm/vhs/newsletter/VHS_Newsletter_1.txt

    https://people.ast.cam.ac.uk/~rgm/vhs/newsletter/VHS_Newsletter_1.txt
    19 Feb 2007: 24.1, 23.7, 23.3 and 22.6 respectively. ... respectively with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.

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