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The microwave background anisotropies: Observations
Pages 29-34

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From page 29...
... PriIlcetoT1 Univ~rsily~ Pr~ceto:~l N] (78544 1~ 1be stranded hot Big Bang cosmological milder cosmic microbe b~c~round r~dlabon {CHBR)
From page 30...
... {i~ ma. 2 indicates that accurate measurements of tab ~nis~tropv power spectrum can distinguish ban these vitriols module Theoretical cosmologists c~1i~uc 10 WOW oul the possible consequences of accurate measurements of the anisotropy
From page 31...
... Fauna #~ or ~ortb~rD Chile. As Abe accuracy of C~BR Isotropy measurements increases, foreground emission from our: GU^y becomes a more important issue.
From page 32...
... . ~ :1 strolls ~illd~icatio~ -that fibs C~MBR aniso1ropy is larger at medium angular scales <100 ~ / ~ LOO)
From page 33...
... iUm-SCaIC CMBR aniSO1,OPy mO8SUrOmeC1S.? FUI1~Sky maps OF t6C SCuS~Ly 8~d angina, [CSO1UtiOO nCOJ03 tO rC~EZO {[C ~11 SCI0DtiEC PO[0ntiB1 Of 1bC aOiSOtrO~ Si~Da1 arc bOSY , ~ done Tom $p~ce.Th~ COBE sledge bad dcmonslra1edth~ m~n<~dv~nlazesofusingcxp~rime~tsi~spac~lo m~kehi~hR , a.
From page 34...
... shag relic~l groups slave ester emoted He acctlr~tcy to ~llicll successful HOP and Fl A~C~K missions Ban measure Iran cosmoIogic~1 parameters {11, 12\ Or. tbesc shad be Egged ~ ~ Hugh india1~n off Ah p<~)


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