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51 - 100 of 922 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 922 match some words.

  1. Results that match 1 of 2 words

  2. CASU WFCAM/VISTA Documentation

    https://people.ast.cam.ac.uk/~wfcam/documentation.html
    1 Mar 2011: VDF-PLA-IOA-00008-0001. WSA science requirements document. 28-10-2002. 20-03-2003 [ps]. ... Example WFCAM FITS header (based on INT CIRSI data). 30-06-2003. 20-06-2003 [fits].

  3. Cambridge XMM XIDOPS WWW Page

    https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/
    16 Nov 2005: 2002-Oct UKIRT run (2002-Oct-19 to 2002-Oct-20).

  4. CASU/ORACDR Pipeline Algorithm Comparative Tests

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/pipeline_tests/index.html
    16 Feb 2004: The mean gaussian width for this particular tile was 2.20 pixels, hence this residual corresponds to roughly 2.5%.

  5. Peer-reviewed Publications See here for latest list of…

    https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Publications.html
    27 Aug 2022: Thermal Inversions, Spectra, and Formation conditions, 2011, ApJ, 743, 191. 20.

  6. SPIRAL spectrograph

    https://people.ast.cam.ac.uk/~optics/spiral/spiral.htm
    16 Jun 2015: URL http://www.ast.cam.ac.uk/optics/spiral/spiral.htm - Revised: 20 Jul 97. We are part of the Institute of Astronomy , which is part of the University of Cambridge.

  7. Educational and Outreach talks for Carolin Crawford in 2006 ...

    https://people.ast.cam.ac.uk/~csc/newcv/2006talks.html
    24 Jul 2019: Oct. 20. Life in the Solar System. KS2 pupils at Whittlesey Primary School. ... Sep. 20. 134340 Pluto. Talk and telescope tour for Alumni of Cambridge University.

  8. CASU WFCAM/VISTA Explanation of documentation numbering system>

    https://people.ast.cam.ac.uk/~wfcam/docs_exp.html
    26 May 2006: scheme.. Dafydd Wyn Evans (dwe @ ast.cam.ac.uk). Last modified: Wed Apr 28 16:20:53 2004.

  9. WFCAM processed data quality control

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/
    3 Sep 2007: 21.15. 0.121. 1525. 2. 20.97. 20.98. 0.136. 1698. 3. 21.10. 21.09.

  10. VHS nominal exposure time and flux limits Waveband Exposure ...

    https://people.ast.cam.ac.uk/~rgm/vhs/vhs-summary.html
    6 Mar 2009: uJy. Y. 1.02. 0.10. 60. 20.3. 20.9? 19.6. 20.2? J. 1.25. ... 0.18. 60. 19.9. 20.9? 19.2. 20.2? H. 1.65. 0.30. 60. 19.0.

  11. Index of /~vasily/itais_party

    https://people.ast.cam.ac.uk/~vasily/itais_party/
    2004-11-29 20:02. 114K. ... 2004-11-29 20:00. 105K.

  12. Martin Rees: Short Articles & Miscellaneous Journalism

    https://people.ast.cam.ac.uk/~mjr/shortpop.html
    18 Oct 2017: Nature, September 2003. Next giant leap for mankind. Daily Telegraph. December 20, 2003. ... Evening Standard, 23 January 2015. Solar eclipse 2015. Daily Telegraph. 20 March 2015.

  13. Index of /~pettini/Stellar Structure Evolution

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/
    2022-11-20 19:26. 1.5M.

  14. CIRSI Hardware Pictures

    https://people.ast.cam.ac.uk/~rgm/cirsi/hardware/
    20 Jan 2000: Last modified: Thu Jan 20 16:00:14 2000.

  15. COHSI

    https://people.ast.cam.ac.uk/~optics/cohsi/cohsi.htm
    16 Jun 2015: Commissioning on UKIRT March 19, 20 & 25-29, 1998.

  16. The LCIR survey at Cambridge

    https://people.ast.cam.ac.uk/~optics/cirsi/lcirs/
    16 Jun 2015: SSA22 22 17 54.0 00 14 34. NICMOS 22hr 22 20 17.2 -24 43 27.

  17. Processing state of WFC data night by night

    https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/nights_status.php
    20. 2001-07-16. WFS-XID. 0.093/0.010/0.024/6.

  18. WFS Status

    https://people.ast.cam.ac.uk/~mike/casu/WFCsur/wfsj0219.html
    16 Dec 2000: Nominal grid centre 02 19 00.00 -05 00 00.0 j2000 RA step size 32.00 arc mins Dec step size 20.00 arc mins Filters: U B V R ... I Z Nominal Exposures: 600s Nominal 3 degree x 3 degree grid Passbands wfsj0219-0500_001 02 13 38.0 -06 20 00 j2000

  19. The STARS Web Pages

    https://people.ast.cam.ac.uk/~stars/archive/cookbook.html
    5 Apr 2004: 10 11 12 17 18 19 20 21 33 3 17 9 24 30 25 26 27 28 2 4 0 0 0 0 8 9 10 11 12 13 14 ... 15 16 20 22 0 0 0 0 0.80 1.20 9.99 0.00 0.05 0.50 0.15 0.02 0.45 1.0E-04 1.0E15

  20. Last modified

    https://people.ast.cam.ac.uk/~rgm/dazle/DazleNewsReports.html
    30 Jul 2005: Last modified: Sat Jul 30 20:07:01 2005.

  21. Documentation for IDL scripts used in XID work

    https://people.ast.cam.ac.uk/~xmmssc/xidops/docs/idl/
    11 Jan 2002: Last modified: Mon Feb 19 18:20:28 2001.

  22. UKIDSS LAS FOOTPRINT SGC

    https://people.ast.cam.ac.uk/~rgm/ukidss/footprint_sgc/
    22 Jul 2007: Sky brightness: The median values are 20.30, 20.22 and 20.09. Sky noise: Fractional Sigma of Sky Value Distribution, expressed as magnitude. ... The photometric zeropoint distributions are very similar. SEGUE p05 has a similar sky brightness to DR6 with

  23. Useful Material and Other Surveys

    https://people.ast.cam.ac.uk/~rgm/wfcsur/other_surveys.html
    11 May 2000: 20.2. 23.4. 22.6. H. 21.0. 19.6. 23.4. 22.0. K. 21.4. 19.5. ... 950. 20.1. 12.3. Photometric calibrations are enabled by a dedicated 20-inch Photometric Telescope (atmospheric extinction, calibration of fainter stars with respect to brighter fundamental

  24. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html
    3 Sep 2007: Passband. Measured 5-sigma limiting magnitude. Magnitude at 50% completeness. Z. 20.8. ... Software. 5-sigma limiting magnitude. Magnitude at 50% completeness. artdata. 20.00. 19.9.

  25. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/
    3 Sep 2007: Passband. Measured 5-sigma limiting magnitude. Magnitude at 50% completeness. Z. 20.8. ... Software. 5-sigma limiting magnitude. Magnitude at 50% completeness. artdata. 20.00. 19.9.

  26. Astrometric and Photometric Distortion for WFCAM and VISTA

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/astrom/
    28 Sep 2006: World Coordinate Systems and FITS Headers. After a mere 20 years the FITS community finally agreed upon a standard way of defining a World Coordinate System (WCS) for telescopes with focal

  27. 2MASS Second Incremental Data Release Explanatory Supplement: Release …

    https://people.ast.cam.ac.uk/~rgm/2mass/imageheader.html
    6 Aug 2000: U-scan Y at Grid (0,0) SKYVAL = 146.9015198 / GFIND Sky Estimate (Image DN) SKYSIG = 0.8133392334 / Grid Noise Estimate (Image DN) MAGZP = 20.7872 / Calibrated zero point from CALMAN

  28. Index of /~vasily/sdss/dots

    https://people.ast.cam.ac.uk/~vasily/sdss/dots/
    Index of /vasily/sdss/dots. 2009-01-29 12:15. -. 2009-01-29 12:15. 8.8K. 2009-01-29 12:15. 7.7K. 2009-01-29 12:15. 47K. 2009-01-29 12:15. 3.0K. 2009-01-29 12:15. 2.7K. 2009-01-29 12:15. 5.7K. 2009-01-29 12:15. 28K. 2009-01-29 12:15. 8.7K. 2009-01-29

  29. Persistence

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/persistence/
    26 May 2006: The variation measured from faint to bright perturbing star was about 20 counts in the level of the persistent image. ... This indicates that the simple model would only be accurate at the 10-20 counts level.

  30. Contents

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/
    17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range.

  31. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/
    26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation).

  32. Observing Plan

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/20001213-dupont-obsplan/
    16 Jun 2015: RA:12:02:36 Dec:5:56.0. set:. rise : 2:03. [2:20. 9:10? :? :? 22:15.

  33. WFCAM: DQC information for 20010607_sf

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/dqc.html
    3 Sep 2007: Last updated: Tue Aug 19 14:24:20 2003.

  34. Hawaii / Picnic interface ver 3

    https://people.ast.cam.ac.uk/~optics/cirsi/documents/CIRSI_wiring_amp55.htm
    16 Jun 2015: DPLUS. 20. R. 20. Chips 13. DGND. 21. S. 21. Chips 13. ... DPLUS. 20. j. 20. Chips 24. DGND. 21. k. 21. Chips 24.

  35. Contents

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/index.html
    17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range.

  36. Index of /~vasily/sdss/leos

    https://people.ast.cam.ac.uk/~vasily/sdss/leos/
    Index of /vasily/sdss/leos. 2009-04-24 20:10. 39K.

  37. 1 Introduction

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf2/index.html
    10 Dec 2004: could also be accounted for (the detection limit is about J=20 [Irwin 2003]).

  38. Index of /~vasily/sdss/stellar_halo

    https://people.ast.cam.ac.uk/~vasily/sdss/stellar_halo/
    2006-11-20 19:40. 29K. ... 2006-11-20 20:00. 1.0K.

  39. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html
    26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation).

  40. Educational and Outreach talks and activities for Carolin Crawford ...

    https://people.ast.cam.ac.uk/~csc/newcv/2014talks.html
    24 Jul 2019: Aug. 20. An introduction to the planets. two talks to children attending Bar Hill holiday club. ... Jul. 20. The Red Planet. y10 class at The Hertfordshire & Essex High School, Bishop Stortford.

  41. COHSI

    https://people.ast.cam.ac.uk/~optics/cohsi/
    16 Jun 2015: IFU Commissioning on UKIRT March 19, 20 & 25-29, 1998.

  42. Media Activity for Carolin Crawford in 2015 In our ...

    https://people.ast.cam.ac.uk/~csc/newcv/2015media.html
    24 Jul 2019: 20 Mar. interviews discussing the Solar Eclipse. Naked Scientists BBC Radio Cambs.

  43. 2MASS resources

    https://people.ast.cam.ac.uk/~rgm/vista/airglow/
    20 Nov 1999: Last modified: Sat Nov 20 20:16:23 1999.

  44. Index of /~vasily/sdss/bestruns

    https://people.ast.cam.ac.uk/~vasily/sdss/bestruns/
    2006-09-12 20:10. 17K.

  45. 1 Introduction

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/interpol/index.html
    26 Mar 2004: Transformation. Shift/pixels. x. y. 1. 0.05. 0.10. 2. 0.15. 0.20. 3.

  46. CIRSI ING 2000A

    https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/
    16 Jun 2015: Mon 15 May to Mon 22 May, 2000. 15-17 ITP4-ELAIS(Perez-Fournon) [ Proposal ]. INT pointings18-20 PATT(INT/00A/P10)-SA57(Ellis) [ Proposal ]. 21-22 ITP3- XMM(Barcons) [ Proposal ].

  47. Summary

    https://people.ast.cam.ac.uk/~optics/cirpass/summary.bak
    16 Jun 2015: Last modified: Wed Nov 24 12:12:20 1999.

  48. Index of /~wfcam/docs/reports/vircam_darkreport

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_darkreport/
    Index of /wfcam/docs/reports/vircam_darkreport. 2006-10-04 12:35. 97K. 2006-10-04 12:35. 98K. 2006-10-04 12:35. 95K. 2006-10-04 12:35. 96K. 2006-10-04 12:35. 104K. 2006-10-04 12:35. 104K. 2006-10-04 12:35. 105K. 2006-10-04 12:35. 101K. 2006-10-04

  49. The APM Sky Catalogues: Brief Details of the Catalogues

    https://people.ast.cam.ac.uk/~mike/apmcat/details.html
    29 Nov 1998: The field centres are on a 6 degree grid. The limiting magnitude is 21.5 for the O plates and 20 for the E plates.

  50. https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt

    https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt
    17 Mar 2006: of 20,000 degree decreases by around 10% for the J/K part. ... 90secs in J/K. UKIDSS LAS Survey ---------------- Median limits(5sigma in 2arcsec aperture) Vega Ks 18.2 H 18.8 J 19.6 Y 20.2.

  51. UFTI Service Observation Reductions

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/ufti_service/index.html
    16 Feb 2004: f20030923_00312. The lower lefthand quadrant shows the most worrying trend. These features do decay with time though and return to near normal within 10 to 20 minutes.

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