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14 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.

16 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.

15 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.

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.

24 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.

26 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

17 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

19 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)!

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!