Topics

1 - Report on the Kiruna Dec 2000/Jan 2001 campaign and the scientific flight

2 - Organisation of Archeops data analysis

3 - Early discussions about the possibility for a flight next Winter

Conclusions of the meeting

Participants to this meeting

R. Ansari, LAL
E. Aubourg, CEA
S. Bargot, LAL
J. Bartlett, OMP
A. Benoit, CRTBT
J.P. Bernard, IAS
A. Bourrachot, LAL (mardi)
P. Camus, CSNSM
F. Couchot, LAL
J. Delabrouille CDF
F.X. Desert, LAOG
X. Dupac, CESR
P. Filliatre, ISN
Y. Giraud-Heraud, CDF (mardi)
L. Guglielmi, CDF (mardi)
J.C. Hamilton CDF
S. Henrot-Versille, LAL
J. Kaplan, CDF
K. Madet, CRTBT
B. Maffei, QMW
C. Magneville, CEA
F. Naraghi , ISN
F. Nati, ROMA
M. Piat, IAS
N. Ponthieu, ISN
J.L. Puget, IAS (lundi)
C. Renault, ISN
D. Santos, ISN
J.C. Vanel, CDF (mardi)
D. Vibert, IAP
D. Yvon, CEA

Preliminary agenda

Monday

Report on the Kiruna Dec 2000/Jan 2001 campaign and the scientific flight

Early results

       Houskeeping and cryogenics (CRTBT)
       Beams before flight (LAL)
       Noise and expected sensitivity (CRTBT+ISN)
       Jupiter: resolution and time constant and calibration (CDF+IAS)
       Jupiter on the SST: alignement control (ISN+CRTBT)
       Calibration on galaxie (IAS)
       Calibration on Dipole (CDF)
       Parasitic signal and balloon rotation (Arctic camel ?) (CDF)
       Polarization (ISN+CDF)
       add missing blocs in recorder data using CNES telemetry (??)

Organisation of the data reduction

       ArchTOI+pipeline (all)
       Weekly letters
       Workshop in April 2nd-6th
       Publications

Tuesday

Early results (suite)

       Star sensor: star detections (CEA+ISN)
       Star sensor: reconstruction global (LAL)
       Star sensor reconstruction using magneto-metre (CEA)
       Star sensor reconstruction using gyros (CRTBT-ISN)
       Map making (LAL - CESR)

Preliminary conclusion for the 01-29 flight

coverage - pendulation - parasitic signal - expected sensitivity
Report for CNES and scientist organisations

Discussion about the possibility for a flight next winter

       Early discussions about the possibility for a flight next Winter
       Fast telemetry (ISN)
       Inmarsat miniM more reliable
       Gondola "weight watcher" or larger balloon (flight at higher elevation)
       New stellar sensor ? refurbishing pivot
       Bolometers and cold optics
       Other modifications to the experiment

Next data reduction meeting

Last revision: 22/02/2001