Determining the motion of the Solar system relative to the cosmic microwave background using Type Ia supernovae

Monthly Notices of the Royal Astronomical Society

Volumn 387, Issue 1, 2008, Pages 371-376

  Gordon, Christopher ^a   Land, Kate ^a   Slosar, Anže ^a,b  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Cosmic microwave background; Solar system: general; Supernovae: general

Indexed keywords

COSMOLOGY; SOLAR SYSTEM; SURVEYS; VELOCITY;

COSMIC MICROWAVES BACKGROUND; ERROR BARS; HIGH-REDSHIFT; LARGE SYNOPTIC SURVEY TELESCOPES; NUMBER DENSITY; PECULIAR VELOCITIES; SOLAR SYSTEM: GENERAL; SUPERNOVAE: GENERAL; SYSTEM MOTION;

SUPERNOVAE;

EID: 44649093900     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13239.x     Document Type: Article

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