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1 - 20 of 42 search results for katalk:za31 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. Dark Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_darkreport/vircam_darkreport.html
    21 Oct 2006: Figure 24 below shows this for detector 15 on the mean dark frame. ... Figure 24 A hot pixel cluster on a mean dark frame for detector 15.

  3. 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

  4. CASU analysis of WFCAM commissioning data - I

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/index.html
    2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2.

  5. 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.

  6. 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.

  7. {\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.

  8. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt
    9 Aug 2006: 3. Report from VDMT MJI and STH attended the VDMT meeting in Edinburgh on 24 July. ... MJI reported on the main points: The UK review of VDFS will be held in Cambridge on 24/25 October.

  9. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060919.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060919.txt
    1 Oct 2006: JRL volunteered. MJI gave further details of the review. Planned Start 24 October Tuesday 10:30 End 25 October Wednesday 15:30 Lunch will be provided on both days and it ... APM3: We were reminded that the home disks of apm3 have now been united with

  10. CASU analysis of WFCAM commissioning data - I

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/
    2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2.

  11. Flat Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/
    8 Dec 2006: 1.32 /- 0.05. 0.53 /- 0.01. 8. 2.23 /- 0.24. 0.61 /- 0.03. ... figure 5.10 Detector 10 (0.10%). figure 5.11 Detector 11 (0.24%). figure 5.12 Detector 12 (0.22%).

  12. Flat Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/vircam_flatreport.html
    8 Dec 2006: 1.32 /- 0.05. 0.53 /- 0.01. 8. 2.23 /- 0.24. 0.61 /- 0.03. ... figure 5.10 Detector 10 (0.10%). figure 5.11 Detector 11 (0.24%). figure 5.12 Detector 12 (0.22%).

  13. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt
    6 Nov 2006: The UK VDFS review was held on 24/25 October at Cambridge.

  14. 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.

  15. 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?

  16. Pipeline CalibrationSimon Hodgkin(paper in prep) Outline • UKIRT…

    https://people.ast.cam.ac.uk/~wfcam/talks/hodgkin_ukidss_jul06.pdf
    3 Aug 2006: The observations span 05A and 05B, and comprise around 21 obs for the P272 field, and 24 for the P545 field.

  17. ..............................................................…

    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.

  18. 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

  19. mnr_7037.tex

    https://people.ast.cam.ac.uk/~wyatt/gw03.pdf
    19 Apr 2006: G8V 1HD 18757 22.9 G4V 2 Wide binaryHD 19373 10.5 G0V 1HD 20407 24.4 G3V 1HD 20766 12.1 G2V 2,‘B’ Wide binary (secondary)HD 20807 ... 1 G1V 2 Wide binary (primary); IRAS discHD 20619 24.7 G5V 1HD 20630 9.2 G5V 1 YoungHD 20794 6.1 G8V 1 ISO discHD

  20. 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.

  21. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: 6 Su et al. Fig. 9.— Radial dependent [24][70] distribution for the Vegadisk. ... To produce the observed [24][70]color, additional components must be invoked. 4.4.

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