Bibcode
Villa, F.; Terenzi, L.; Sandri, M.; Meinhold, P.; Poutanen, T.; Battaglia, P.; Franceschet, C.; Hughes, N.; Laaninen, M.; Lapolla, P.; Bersanelli, M.; Butler, R. C.; Cuttaia, F.; D'Arcangelo, O.; Frailis, M.; Franceschi, E.; Galeotta, S.; Gregorio, A.; Leonardi, R.; Lowe, S. R.; Mandolesi, N.; Maris, M.; Mendes, L.; Mennella, A.; Morgante, G.; Stringhetti, L.; Tomasi, M.; Valenziano, L.; Zacchei, A.; Zonca, A.; Aja, B.; Artal, E.; Balasini, M.; Bernardino, T.; Blackhurst, E.; Boschini, L.; Cappellini, B.; Cavaliere, F.; Colin, A.; Colombo, F.; Davis, R. J.; de La Fuente, L.; Edgeley, J.; Gaier, T.; Galtress, A.; Hoyland, R.; Jukkala, P.; Kettle, D.; Kilpia, V.-H.; Lawrence, C. R.; Lawson, D.; Leahy, J. P.; Leutenegger, P.; Levin, S.; Maino, D.; Malaspina, M.; Mediavilla, A.; Miccolis, M.; Pagan, L.; Pascual, J. P.; Pasian, F.; Pecora, M.; Pospieszalski, M.; Roddis, N.; Salmon, M. J.; Seiffert, M.; Silvestri, R.; Simonetto, A.; Sjoman, P.; Sozzi, C.; Tuovinen, J.; Varis, J.; Wilkinson, A.; Winder, F.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 520, id.A6
Fecha de publicación:
9
2010
Revista
Número de citas
12
Número de citas referidas
11
Descripción
The Low Frequency Instrument (LFI) on-board the ESA Planck satellite
carries eleven radiometer subsystems, called radiometer chain assemblies
(RCAs), each composed of a pair of pseudo-correlation receivers. We
describe the on-ground calibration campaign performed to qualify the
flight model RCAs and to measure their pre-launch performances. Each RCA
was calibrated in a dedicated flight-like cryogenic environment with the
radiometer front-end cooled to 20 K and the back-end at 300 K, and with
an external input load cooled to 4 K. A matched load simulating a
blackbody at different temperatures was placed in front of the sky horn
to derive basic radiometer properties such as noise temperature, gain,
and noise performance, e.g. 1/f noise. The spectral response of each
detector was measured as was their susceptibility to thermal variation.
All eleven LFI RCAs were calibrated. Instrumental parameters measured in
these tests, such as noise temperature, bandwidth, radiometer isolation,
and linearity, provide essential inputs to the Planck-LFI data analysis.