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1 - 10 of 10 search results for KA :PC53 |u:people.ast.cam.ac.uk where 0 match all words and 10 match some words.
  1. Results that match 1 of 2 words

  2. 19 Apr 2006: X,KVJ?ES¥L7A<ã,/9:A%,/ãFß79¥91Ú7A%Aå@VIS:9:A>?EäAGFKÝM,K?Ä,KLELEVd91VJF?E,KH <FLTVJ,Kä<,KHTä<HdFßTL@æpHJVd0KAÚ7FK9 LEßES:9äFXCáF?7A>?9ä<HdFS:A9:F%91ÚEAS:91,/.# ... Kô5áMä/;Kä<,K?ãA.1A>S:FHdQKA>LCßESVJ?7ï591ÚEVJSVJ?TS:9:.ßEXCA>
  3. Craig  Mackay

    https://people.ast.cam.ac.uk/~cdm/cdm_pub_list_130509.htm
    14 May 2009: Astrophys., 306, L13-L16. 92. Mackay CD, Parry, IR, Piche, F, Ennico, KA, 1996, "Imaging Spectroscopy for Infra-Red Astronomy", in “Recent Developments in Scientific Optical Imaging”, ed M Bonner Denton, ... 93. Piche, F, Parry IR, Ennico, KA, Ellis,
  4. Publications list for Carolin Crawford

    https://people.ast.cam.ac.uk/~csc/newcv/Full%20publications%20list%20for%20Carolin%20Crawford.pdf
    15 Feb 2021: 93. Crawford CS, Fabian AC, Johnstone RM, Arnaud KA 1989 MNRAS 236 277-287 A2597 - Another massive cooling flow. ... 97. Arnaud KA, Johnstone RM, Fabian AC, Crawford CS, Nulsen PEJ, Shafer RA, Mushotzky RF 1987 MNRAS 227 241-256 X-ray observations of the
  5. 19 Apr 2006: ÚTKÖÀÁ3MÞC8ëHÞbß AÜ&Á)ERÝRÖÞYÁKAßDRàYØYÖÀÁRÂWAßØYáYÁRÖÀÞRàCÁ),KÁ)MÁ))¿"RàC%EØ&ÖÀAÂEAYÂEáYØ4RàY.RàCîA¿ÝMÖRRÖÞYA&ïxERRáCRÜ&RÖÀÞYÁ"Aßxï&ÀAÞCERRWÁ)MÁ))¿ð)PRàC. ... AßÁ)¿ÂEáYÀï<ERáCRÜ&R
  6. 19 Apr 2006: "$#&%'$(),.-/#&002134)35%61578%&9:3<;>=:150 #)?9@35(!BA.CDE=F1G0 #HJI$%#K'$LF).CM35(#K35)?N4OP'0 QR?NESUTTVS. WYX[Z] _bacZ]dJefdegebhWji_kZ]_ldJenmoi_bdZpqermsX[t[uWjicvxw. y{z.|}zE$/. F5F$,M,KV:>2J5G<M@¡ M¢£J?b >V¤MG¥.
  7. Draft version May 29, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf
    14 Sep 2015: The ATCA data with the best dynamic range was ob-tained in Ka, i.e. ... The6 km data in Ka were then concatenated with the taskconcat from CASA (McMullin et al.
  8. Next Generation Very Large Array Memo No. 6Science Working ...

    https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf
    24 Oct 2015: With the newly upgradedJVLA, it has been possible to begin performing dust polarization studies atcentimeter wavelengths, using the highest-frequency bands available: K, Ka,and Q bands (18–50 GHz). ... Considering that ALMA will eventually have Band 1
  9. Extrasolar Kuiper Belts Mark C. Wyatt Abstract Extrasolar debris ...

    https://people.ast.cam.ac.uk/~wyatt/wyat19.pdf
    26 Sep 2019: Extrasolar Kuiper Belts. Mark C. Wyatt. Abstract Extrasolar debris disks are the dust disks found around nearby main se-quence stars arising from the break-up of asteroids and comets orbiting the stars.Far-IR surveys (e.g., with Herschel) showed
  10. 19 Apr 2006: KÂ ,¡ f}{h}z4zC{K}=xzz}¡!Y{K.{h>zC z}2Zx$!{K}¡z z «}zC{}{K./x¡! ... K $}x$?x{K.y2¡«¢o}{KÂ{>¡6zC{YV,| $@{K}6zH{K!VÄ ¡ {K}Y!
  11. 19 Apr 2006: #"$ %&! %'( )' '(,-. / ( /! 01. (2. , 03'4!5&6. / -! $. %78 (! / 9 : / ;<'(= >?" (63@$A / BC $ %D$.E. @ > (F E GA H / :/ ='( $<6? " (6I$A /. JLKMKNK. '(0=5 / E! #"$%&')( 2,-!%-/ 0 " / -!1 -/2 2435". 0$6/7$6 , " ( 1- '/7"8,9):,-,$6;9+ 2<!2/7=,)

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