College de France (PCC), Paris
Status of available data and programs
E. Aubourg , C. Renault and FX. Desert
Pointing reconstruction
Discussions on the 3 solutions: A. Bourrachot, E. Aubourg, A. Benoit
Optical characterisation
S. Henrot-Versille, J.-C. Hamilton
High Frequency noise
P. Filliatre
Low Frequency noise
K. Madet, A. Amblard
Calibration
Responsivity
Jupiter
Dipole
Galaxy
Map-making
O. Dore
X. Dupac
Cl estimates
O. Dore
S. Henrot-Versille
General discussions on the way forward
Conclusions on the work to be done
archtoi improvements: E. Aubourg, C. Renault
---> Bugs and offsets
Pointing:
---> Stars and stellar candidates: 2 catalogs
---> Comparison of 3 methods
HF rise: E. Aubourg, M. Piat, AB
HF peaks and bumps: P. Filliatre
---> all flight, Constrained noise ? Study timelines before/after
decorrelation. 72 et al. specific analysis.
Flagging: P. Filliatre, FXD
---> Tail of glitches, slow glitches, other bad data ToBeDone
Time-dependent response and Bolometer model: K. Madet, FXD
---> Give responsivity correction factor
Photometric model: E. Wakui, B. Maffei, FXD, A. Amblard
---> Give emissivity of all components (0.1K, 1.6K, 10K, telescope,
atm...)
Beam & Jupiter calibration, Glitches: SHV, JCH, MP
---> Check on photometry via simulation, effect of variable
speed on
beam, include non-linearity and different current config, make code
available, Optical and electronic Cross-talk. Calibration table on
CVS. Compare positions with theoretical ones. Redo with new
pointings and clean data. Include non linearity,
compressor-decompressor. Understanding slow glitches. Time variability.
Map-making: X. Dupac, O. Dore, F. Bouchet & D. Vibert, D. Yvon,
JCH, archeops++ group
---> Multibolometer maps. Data with holes. Date with prefiltering
or
with Low Frequency decorrelation. Monte-Carlo simulations for noise
estimates (which are very important).
C_l: O. Dore, SHV et lal.
astroph-0104443, hierarchical decomposition
Cosmological parameter estimates
---> S. Bargot and M. Douspis, J. Bartlett
Polarisation: ISN+CdF
---> Investigate polarised systematic effects
Use of differential GPS: Ch. Magneville
---> Use it or not? Should be available for August flight
or put accurate gyros: 1
or 3 ?
Ad-hoc committee CNES : 21 May 2001
August test flight for Inmarsat fast telemetry will also test Russian
side: 2hours at 25 km, 1 gyro, fast+slow Inmarsat, folding boom.
Possibility of going farther than Ural; Big helicopter to carry the
whole payload back.
Bolometer status: relations with Caltech, Planck...
Biarritz presentation + paper : beams, 545GHz
Next data reduction meeting
Tuesday 19 or 26 June 2001 in Grenoble
Last revision: 09/05/2001