Studies of cosmic microwave background structure at Dec. = + 40° - II. Analysis and cosmological interpretation

Monthly Notices of the Royal Astronomical Society

Volumn 289, Issue 3, 1997, Pages 505-514

  Hancock, S ^a   Gutierrez, C M ^b   Davies, R D ^c   Lasenby, A N ^a   Rocha, G ^a   Rebolo, R ^b   Watson, R A ^c   Tegmark, M ^d,e  

^a CAVENDISH LABORATORY   (United Kingdom)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c UNIVERSITY OF MANCHESTER   (United Kingdom)

^d MAX PLANCK INSTITUT FÜR PHYSIK   (Germany)

^e INSTITUTE FOR ADVANCED STUDY   (United States)

Author keywords

Cosmic microwave background; Cosmology: Observations; Large scale structure of Universe

Indexed keywords

AUTOCORRELATION; GRAVITATIONAL EFFECTS; GRAVITY WAVES;

ATMOSPHERIC CONTRIBUTIONS; BACKGROUND SIGNALS; COMMON STRUCTURES; COSMIC MICROWAVES BACKGROUND; COSMOLOGY OBSERVATIONS; FLUCTUATION AMPLITUDES; LARGE SCALE STRUCTURE OF UNIVERSE; LARGE-SCALES; SPECTRAL INDICES; TENERIFE;

COSMOLOGY;

EID: 0012274192     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/289.3.505     Document Type: Article

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