2020A&A...641A...2P

Query : 2020A&A...641A...2P

2020A&A...641A...2P - Astronomy and Astrophysics, volume 641A, 2-2 (2020/9-1)

Planck 2018 results. II. Low Frequency Instrument data processing.

PLANCK COLLABORATION, AKRAMI Y., ARGUESO F., ASHDOWN M., AUMONT J., BACCIGALUPI C., BALLARDINI M., BANDAY A.J., BARREIRO R.B., BARTOLO N., BASAK S., BENABED K., BERNARD J.-P., BERSANELLI M., BIELEWICZ P., BONAVERA L., BOND J.R., BORRILL J., BOUCHET F.R., BOULANGER F., BUCHER M., BURIGANA C., BUTLER R.C., CALABRESE E., CARDOSO J.-F., COLOMBO L.P.L., CRILL B.P., CUTTAIA F., DE BERNARDIS P., DE ROSA A., DE ZOTTI G., DELABROUILLE J., DI VALENTINO E., DICKINSON C., DIEGO J.M., DONZELLI S., DUCOUT A., DUPAC X., EFSTATHIOU G., ELSNER F., ENSSLIN T.A., ERIKSEN H.K., FANTAYE Y., FINELLI F., FRAILIS M., FRANCESCHI E., FROLOV A., GALEOTTA S., GALLI S., GANGA K., GENOVA-SANTOS R.T., GERBINO M., GHOSH T., GONZALEZ-NUEVO J., GORSKI K.M., GRATTON S., GRUPPUSO A., GUDMUNDSSON J.E., HANDLEY W., HANSEN F.K., HERRANZ D., HIVON E., HUANG Z., JAFFE A.H., JONES W.C., KARAKCI A., KEIHANEN E., KESKITALO R., KIIVERI K., KIM J., KISNER T.S., KRACHMALNICOFF N., KUNZ M., KURKI-SUONIO H., LAMARRE J.-M., LASENBY A., LATTANZI M., LAWRENCE C.R., LEAHY J.P., LEVRIER F., LIGUORI M., LILJE P.B., LINDHOLM V., LOPEZ-CANIEGO M., MA Y.-Z., MACIAS-PEREZ J.F., MAGGIO G., MAINO D., MANDOLESI N., MANGILLI A., MARIS M., MARTIN P.G., MARTINEZ-GONZALEZ E., MATARRESE S., MAURI N., McEWEN J.D., MEINHOLD P.R., MELCHIORRI A., MENNELLA A., MIGLIACCIO M., MOLINARI D., MONTIER L., MORGANTE G., MOSS A., NATOLI P., PAGANO L., PAOLETTI D., PARTRIDGE B., PATANCHON G., PATRIZII L., PEEL M., PERROTTA F., PETTORINO V., PIACENTINI F., POLENTA G., PUGET J.-L., RACHEN J.P., RACINE B., REINECKE M., REMAZEILLES M., RENZI A., ROCHA G., ROUDIER G., RUBINO-MARTIN J.A., SALVATI L., SANDRI M., SAVELAINEN M., SCOTT D., SELJEBOTN D.S., SIRIGNANO C., SIRRI G., SPENCER L.D., SUUR-USKI A.-S., TAUBER J.A., TAVAGNACCO D., TENTI M., TERENZI L., TOFFOLATTI L., TOMASI M., TROMBETTI T., VALIVIITA J., VANSYNGEL F., VAN TENT B., VIELVA P., VILLA F., VITTORIO N., WANDELT B.D., WATSON R., WEHUS I.K., ZACCHEI A. and ZONCA A.

Abstract (from CDS):

We present a final description of the data-processing pipeline for the Planck Low Frequency Instrument (LFI), implemented for the 2018 data release. Several improvements have been made with respect to the previous release, especially in the calibration process and in the correction of instrumental features such as the effects of nonlinearity in the response of the analogue-to-digital converters. We provide a brief pedagogical introduction to the complete pipeline, as well as a detailed description of the important changes implemented. Self-consistency of the pipeline is demonstrated using dedicated simulations and null tests. We present the final version of the LFI full sky maps at 30, 44, and 70GHz, both in temperature and polarization, together with a refined estimate of the solar dipole and a final assessment of the main LFI instrumental parameters.

Abstract Copyright: © ESO 2020

Journal keyword(s): space vehicles: instruments - methods: data analysis - cosmic background radiation

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 NAME North Polar Spur ISM 12 00 +00.0           ~ 372 1
2 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 14413 0

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