Carbon monoxide line emission as a CMB foreground: Tomography of the star-forming universe with different spectral resolutions

Astronomy and Astrophysics

Volumn 489, Issue 2, 2008, Pages 489-504

  Righi, M ^a   Hernandez Monteagudo C ^a   Sunyaev, R A ^a,b  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b Space Research Institute ^*  (Russian Federation)

Author keywords

Cosmology: cosmic microwave background; Cosmology: theory; Galaxies: intergalactic medium

Indexed keywords

ANGULAR DISTRIBUTION; CARBON MONOXIDE; COSMOLOGY; DIAGNOSTIC RADIOGRAPHY; EMISSION SPECTROSCOPY; IMAGING TECHNIQUES; MEDICAL IMAGING; MERGING; METALS; POWER SPECTRUM; SPECTRAL RESOLUTION; THERMOGRAPHY (TEMPERATURE MEASUREMENT); TOMOGRAPHY;

ANGULAR POWER SPECTRUM; ANGULAR SCALES; CMB EXPERIMENTS; CO LINE; COSMOLOGICAL PARAMETERS; COSMOLOGY: COSMIC MICROWAVE BACKGROUND; COSMOLOGY: THEORY; FINE STRUCTURES; FREQUENCY CHANNELS; GALAXIES: INTERGALACTIC MEDIUM; GHZ BAND; HIGH-REDSHIFT; LINE EMISSIONS; METAL ENRICHMENT; OBSERVATIONAL DATA; ORDERS-OF-MAGNITUDE; PARAMETRIZATION; RED SHIFTING; REIONIZATION; ROTATIONAL LINES; STAR FORMATION; STAR FORMATION RATE; VARYING THICKNESS;

FORMING;

EID: 52949105811     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810199     Document Type: Article

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