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Craig Mackay
https://people.ast.cam.ac.uk/~cdm/cdm_pub_list_130509.htm14 May 2009: ApJ, 270, 342 (1983). 24. Mackay, C.D. and Astill, D.M., CCD Development at Cambridge, England'. ... 31. Mackay, C.D., CCDs in Astronomy'. Ann. Rev. Ast. And Astrophys., 24, 255, 1986. -
Craig Mackay
https://people.ast.cam.ac.uk/~optics/people/cdm_pub_list_130509.htm16 Jun 2015: ApJ, 270, 342 (1983). 24. Mackay, C.D. and Astill, D.M., CCD Development at Cambridge, England'. ... 31. Mackay, C.D., CCDs in Astronomy'. Ann. Rev. Ast. And Astrophys., 24, 255, 1986. -
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. ... 10. Crawford CS 2007 The Reader , no 24, p 50-52 Heavenly Inspiration. -
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: 24. 5 Chemical evolution of the star and planet forming environ-ment 275.1 Complex organic molecules in Hot Molecular Cores. ... The cyan contours are –6, –3, 3, 6, 12, 24, 48, 96, 192 σI, whereσI = 19.5µJy bm1 is the rms noise in the Stokes I map. -
Extrasolar Kuiper Belts Mark C. Wyatt Abstract Extrasolar debris ...
https://people.ast.cam.ac.uk/~wyatt/wyat19.pdf26 Sep 2019: excess emission abovephotospheric levels at different wavelengths (typically at 24, 70, 100 and 160 µ m).Surveys have been carried out for nearby stars with a variety of spectral types, ... Kenyon and Bromley 2010), sincebroad disks are hot early on and -
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 -
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https://people.ast.cam.ac.uk/~wyatt/wyat99.pdf19 Apr 2006: 2/)C"C$ )!1-N. 2#1 D 4'@! 24"BC #" 1 9 #"S243! S'@ #3<TU,3- #"D32#!24"24,! :<')("!-! ... $-"8 =H0,"80 N,'<Q ; 3j Y-. ) ,"8 2MP 24 3j ;2)! -
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https://people.ast.cam.ac.uk/~wyatt/wdg03.pdf19 Apr 2006: KÂ ,¡ f}{h}z4zC{K}=xzz}¡!Y{K.{h>zC z}2Zx$!{K}¡z z «}zC{}{K./x¡! ... K $}x$?x{K.y2¡«¢o}{KÂ{>¡6zC{YV,| $@{K}6zH{K!VÄ ¡ {K}Y!
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