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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=,)

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>

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¥.

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

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!

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

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

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

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

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.