WMAP 3-yr sources at 16 and 33GHz. II. (Franzen+, 2009)

Bibcode
2011yCat..74000995F
Franzen, T. M. O.; Davies, M. L.; Davies, R. D.; Davis, R. J.; Feroz, F.; Genova-Santos, R.; Grainge, K. J. B.; Green, D. A.; Hobson, M. P.; Hurley-Walker, N.; Lasenby, A. N.; Lopez-Caniego, M.; Olamaie, M.; Padilla-Torres, C. P.; Pooley, G. G.; Rebolo, R.; Rodriguez-Gonzalvez, C.; Saunders, R. D. E.; Scaife, A. M. M.; Scott, P. F.; Shimwell, T. W.; Titterington, D. J.; Waldram, E. M.; Watson, R. A.; Zwart, J. T. L.
Referencia bibliográfica

VizieR On-line Data Catalog: J/MNRAS/400/995. Originally published in: 2009MNRAS.400..995F

Fecha de publicación:
10
2011
Número de autores
25
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Using the Arcminute Microkelvin Imager (AMI) at 16GHz and the Very Small Array (VSA) at 33GHz to make follow-up observations of sources in the New Extragalactic WMAP Point Source catalogue, we have investigated the flux density variability in a complete sample of 97 sources over time-scales of a few months to ~1.5yr. (1 data file).
Tipo
Sin árbitro
Fuentes de radio

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