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https://people.ast.cam.ac.uk/~wyatt/whgd04.pdf19 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> -
Craig Mackay
https://people.ast.cam.ac.uk/~cdm/cdm_pub_list_130509.htm14 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, -
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https://people.ast.cam.ac.uk/~wyatt/wdt00.pdf19 Apr 2006: ÚTKÖÀÁ3MÞC8ëHÞbß AÜ&Á)ERÝRÖÞYÁKAßDRàYØYÖÀÁRÂWAßØYáYÁRÖÀÞRàCÁ),KÁ)MÁ))¿"RàC%EØ&ÖÀAÂEAYÂEáYØ4RàY.RàCîA¿ÝMÖRRÖÞYA&ïxERRáCRÜ&RÖÀÞYÁ"Aßxï&ÀAÞCERRWÁ)MÁ))¿ð)PRàC. ... AßÁ)¿ÂEáYÀï<ERáCRÜ&R -
Craig Mackay
https://people.ast.cam.ac.uk/~optics/people/cdm_pub_list_130509.htm16 Jun 2015: 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, -
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https://people.ast.cam.ac.uk/~wyatt/wyat02.pdf19 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¥. -
Publications list for Carolin Crawford
https://people.ast.cam.ac.uk/~csc/newcv/Full%20publications%20list%20for%20Carolin%20Crawford.pdf15 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 -
Draft version May 29, 2015Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf14 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. -
Next Generation Very Large Array Memo No. 6Science Working ...
https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf24 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 -
https://people.ast.cam.ac.uk/~vasily/data/TAP_1697550531535.vot
https://people.ast.cam.ac.uk/~vasily/data/TAP_1697550531535.vot17 Oct 2023: ARI's TAP access to the Gaia Archive. Unique source identifier (unique within a particular Data Release) Basis function coefficients for the BP spectrum representation Basis function coefficients for the RP spectrum representation -
Extrasolar Kuiper Belts Mark C. Wyatt Abstract Extrasolar debris ...
https://people.ast.cam.ac.uk/~wyatt/wyat19.pdf26 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
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