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1 - 50 of 346 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 346 match some words.

  1. Results that match 1 of 2 words

  2. Prof Richard McMahon, Institute of Astronomy, Cambridge Home Page

    https://people.ast.cam.ac.uk/~rgm/
    28 Jun 2024: More that 200 papers in refereed journals. 12 papers published in Nature.

  3. Carolin Crawford

    https://people.ast.cam.ac.uk/~csc/cv.html
    15 Feb 2021: During the ten years 2006-2016 I delivered a total of 850 presentations to a total audience of over 62,200 people.

  4. Cambridge XMM Survey Science Centre

    https://people.ast.cam.ac.uk/~xmmssc/
    10 Oct 2008: 2. s. -1. (0.1-10 keV) and contain 100-200 serendipitous" X-ray sources.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2013talks.html
    24 Jul 2019: 3 talks to pupils at Ramsey Junior School. May. 40, 200, 40. ... 200. The science and beauty of nebulae. Talk to sixth-form students attending a space week at Villiers Park.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2012talks.html
    24 Jul 2019: Sep. 200. The sounds of the Universe. Talk at the Horncastle Astronomy Weekend. ... May. 200. Exoplanets and how to find them. Talk to Clacton and District Astro-Soc.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2006talks.html
    24 Jul 2019: Sep. 200. The Invisible Universe. Two presentations and discussion sessions at science-arts workshop for KS3 students in London from Heston Community College, Brentford School for Girls and Syon Park, coordinated ... March. 200. Our place in the Universe.

  8. Cambridge STARS Homepage

    https://people.ast.cam.ac.uk/~stars/
    28 Feb 2013: In most circumstances, just 200 points are sufficient. Simultaneous solution of structure and composition.

  9. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hard3_xwc.html
    25 Mar 2002: 0.853.08. A 1837. 200. 2001-02-22. 1. -1.7. -1.8. 20.7. 0. 22.6. ... 0.210.31. A 1837. 200. 2001-02-22. 1. -1.4. 1.4. 15.5. -1. 17.4.

  10. Observing guide for CIRSI (WFIRC) at LCO du Pont ...

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html
    16 Jun 2015: pc, computer room 200.29.61.153 bodega2.lco.cl bodega2 # Yerko Aviles pc # 200.29.61.154? ... 139 remote.lco.cl remote # # Visitor Laptops # 200.28.111.145 visitor1.lco.cl visitor1 200.28.111.146 visitor2.lco.cl visitor2 17).

  11. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html
    3 Sep 2007: artdata. A full-well capacity of 200,000 electrons was used for the saturation level.

  12. MGB thesis Chapter 5

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter5.htm
    16 Jun 2015: The trolley is set to scan at 200 Hz and forms the main peak in the data.

  13. VizieR Search Page

    https://people.ast.cam.ac.uk/~rgm/apmcat/cds/VizieR-apmcat-poss1-all.html
    27 Jun 2001: Maximum Entries per table:. 10. 20. 50. 100. 200. 1000. 9999.

  14. Other IFUs

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_ifu.html
    16 Jun 2015: software. PIFS. type. slicer. telescope. Palomar 200 inch. wv range. 1-2.5 micron, 1-5 micron.

  15. https://people.ast.cam.ac.uk/~rgm/wfcsur/jsc_ridos.txt

    https://people.ast.cam.ac.uk/~rgm/wfcsur/jsc_ridos.txt
    1 Mar 1998: Hence in total the project life-span would be 4 years, with a survey area of 100-200 square degrees in up to seven colour bands. ... Hence in total the project life-span would be 4 years, with a survey area of 100-200 square degrees in up to seven

  16. Appendix A - Specification

    https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/appa.htm
    15 Nov 1998: IBM or 100% compatible 200 MHz Pentium PC or faster. Hard disk with at least 100 Mbytes of free space (a lot more if you are storing images on this disk).

  17. Pixcel - Remote operation

    https://people.ast.cam.ac.uk/~rgm/cirsi/pixcel/pixcel_19990428_help/remote.htm
    23 Jan 2000: ALLOW=200.28.111.138. This is a comma separated list of machines which are allowed to connect to Pixcel.

  18. Observing guide for CIRSI (WFIRC) at LCO du Pont ...

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html
    16 Jun 2015: pc, computer room 200.29.61.153 bodega2.lco.cl bodega2 # Yerko Aviles pc # 200.29.61.154? ... 139 remote.lco.cl remote # # Visitor Laptops # 200.28.111.145 visitor1.lco.cl visitor1 200.28.111.146 visitor2.lco.cl visitor2 17).

  19. Astroparticle_16

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf
    13 Mar 2012: Photon easy to detect and measure! [GeV]Tγp. 200 300 400 500 600 700. ... n=4.0 0.6 - 1.0!•MPL = 1029 200 - 100 GeV! 3/12/12 Astroparticle 23.

  20. VIRCAM Pipeline: vircam_tfits

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/group__vircam__tfits.html
    10 Apr 2013: Returns:. The output vircam_tfits object list. Author:. Jim Lewis, CASU. Definition at line 200 of file vircam_tfits.c.

  21. Chapter 1 - Installation

    https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter1.htm
    15 Nov 1998: IBM or 100% compatible 200 MHz or better Pentium PC. Hard disk with at least 100 Mbytes of free space (a lot more if you are storing images on this disk).

  22. CIRPASS data reduction cookbook SN1987a

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/cookbook_sn1987a_old_200307.php
    imreplace.upper = 200. imreplace.radius = 0. imrep. imreplace.images = "badpix". imreplace.value = 1. ... imreplace.imaginary = 0. imreplace.lower = 200. imreplace.upper = INDEF. imreplace.radius = 0.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2019talks.html
    25 Oct 2019: Your place in the cosmos. Lowestoft First Light Festival. Jun. 200.

  24. New Page 1

    https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm
    16 Jun 2015: This involved using the One-Mile Radio Telescope of the Mullard Radio Astronomy Observatory to observe a sample of 200 bright radio sources in the 3C revised catalogue, at galactic latitudes

  25. lecture8_debrisdiskapp

    https://people.ast.cam.ac.uk/~wyatt/lecture8_debrisdiskapp.pdf
    17 Feb 2009: Spiral structure at 200 AU implies planet at 150 AU • Same structure seen in Saturn’s rings (Charnoz et al. ... Numerical integrations of star, migrating planet, 200 planetesimals giving capture probabilities for 3:2 resonance:.

  26. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/
    3 Sep 2007: artdata. A full-well capacity of 200,000 electrons was used for the saturation level.

  27. Chapter 4 - Controls Reference

    https://people.ast.cam.ac.uk/~rgm/cirsi/pixcel/pixcel_19990428_help/chapter4.htm
    23 Jan 2000: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  28. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 Apr 2006: This 200-AU-sized regioncoincides with the slightly tilted inner disk identified optically withthe Hubble Space Telescope5. ... The possible relationship of these components has yetto be explored, but the lower inferred temperatures of the clumpparticles

  29. VIRCAM Pipeline: vircam_matchxy.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__matchxy_8c-source.html
    10 Apr 2013: 00334 00335 cpl_msg_info(fctid,"Doing the matching for extension %d",j); 00336 (void)ps.cat1f), 00337 vircam_tfits_get_table(ps.cat2f),200.0, 00338 &(vircam_matchxy_config.xoff),

  30. Astroparticle_15

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_15.pdf
    25 Mar 2011: R is now 200 microns. This is very large on a quantum scale, but small on the scale used to test gravity in experiments – close to current limit of 100

  31. arX iv:0 704. 0873 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf
    18 Apr 2007: 200. 7. Mon. Not. R. Astron. Soc. 000, 1–6 (2006) Printed 9 April 2007 (MN LATEX style file v2.2). ... Doppler systems arepredicted here to form from 5-200 Jupiter masses of gas inthe disk, enough to make gas giant planets.

  32. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 Jun 2007: Dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.

  33. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf
    10 Nov 2017: Evidence for kinematically distinct outflows – discrete mass-loss episodes (strongly asymmetric)• Expansion velocities 40-50km/s• Kinematic age estimates for features, from distance/velocity, are 200, 400 and 900 years• Smallest

  34. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hr3-err_gt0.html
    27 Mar 2002: 0.853.08. A 1837. 200. 2001-02-22. Y. -1.7. -1.8. 20.7. 0. 22.6. ... 0.210.31. A 1837. 200. 2001-02-22. Y. -1.4. 1.4. 15.5. -1. 17.4.

  35. https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt
    16 Jun 2015: 13. -5. 199. 200. 12. -4. 200. 201. 11. -3. 201.

  36. Chapter 1 - Installation

    https://people.ast.cam.ac.uk/~rgm/cirsi/pixcel/pixcel_19990428_help/chapter1.htm
    23 Jan 2000: IBM or 100% compatible 200 MHz or better Pentium PC. Hard disk with at least 100 Mbytes of free space (a lot more if you are storing images on this disk).

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

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf
    5 Jun 2007: The Y-J colour is ESSENTIAL since the so called ’rare’ L and T dwarfs outnumberthe quasars by a factor of 200:1 based on the well established space densities of ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467

  38. DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/hmsu22.pdf
    25 Oct 2022: 8. 10. 12. km/s 200 150 100 50 0 50 100 150 200Radius [au]. ... 10. 12. km/s 200 150 100 50 0 50 100 150 200Radius [au].

  39. Chapter 2 : Operating the software

    https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter2.htm
    15 Nov 1998: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  40. MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: Rrk = Σirki=ick. ni4(Dk Di). 2 πvrelV. , (11). 100 200 300 400 500k-i. ... 0.08. 0.10. Vol. atile. Fra. ctio. n. 0 Myrs 10 Myrs 100 Myrs 200 Myrs.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2014talks.html
    24 Jul 2019: Mar. 350, 200. Your place in the cosmos. Talk to high school pupils from Finland. ... Mar. 200. The Northern Lights. Talk at Public Open Evening, IoA.

  42. CIRSI Hardware Pictures

    https://people.ast.cam.ac.uk/~rgm/cirsi/hardware/
    20 Jan 2000: The overall weight of everything that is on the telescope is almost exactly 200 kg, with /- a fill of LN2.

  43. MNRAS 000, 1–11 (2015) Preprint 9 November 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/khhw18.pdf
    9 Nov 2018: In total the datacomprise four years of photometry for roughly 200,000 dis-tinct stars.

  44. INT Wide Angle Survey

    https://people.ast.cam.ac.uk/~rgm/wfcsur/
    1 Nov 2000: 07 50.0 20 30. 200, 22. 1. o. x1. o. vi.

  45. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hard2.html
    20 Mar 2002: 0.49. 0.20. A 1837. 200. 2001-02-22.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2015talks.html
    24 Jul 2019: Mar. 40. Solar Eclipses. Year 8 at Harlow Academy. Mar. 200.

  47. Difference imaging

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/subtract2/index.html
    11 Jun 2004: These subsections are roughly 1000 x 1000 pixels in size centred at (1024,2048) with the intensity scaled linearly from the average "sky" level to cover the range /-200 counts in

  48. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_030417.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_030417.txt
    5 May 2003: JRL to ponder. The tape systems will be Ultrium LTO-2 with a native capacity of 200 GB.

  49. Prochaska atomic data

    https://people.ast.cam.ac.uk/~rfc/atomdat.html
    22 Mar 2005: O I  922.200  2.45e-4 3.21e6  M03. O I  921.857  1.08e-3 1.00E7  M03.

  50. Chapter 4 - Controls Reference

    https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter4.htm
    15 Nov 1998: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  51. 1906.08797

    https://people.ast.cam.ac.uk/~wyatt/smkb19.pdf
    20 Nov 2019: temperature, and 40 K for the modified blackbody (theblackbody function is divided by 0.9 beyond 200 µm)of the disk. ... 230.02 mag 1J 1.2 5.420.03 mag 5H 1.6 5.280.04 mag 5KS 2.2 5.200.02 mag 5.

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