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CONTENT

Observational data from the campaign of observation
of the mutual events of the Galilean satellites of Jupiter for the occurrence of 2009



Data1: 
Files of astrometric positions deduced from the observations of the events
   and provided in the paper Arlot, Emelyanov et al., A&A, in press as tables 6 and 7:
   astrometric-results-table6.txt
   astrometric-results-table7.txt
   The data provided are as follows:
These astrometric results are obtained from the photometric data arrived from three sources:
source A - database transmitted by J.-E. Arlot (The International Campaign PHEMU 2009)
source B - database transmitted by Roberto Vieira Martins (Observations made in Brasil)
source R - database transmitted by N. Emelianov (Published astrometric results derived
             from photometric observations of russian observers) 

Explanations for the Table 6 of astrometric results (first type).
 
Date - date of observation.
Type - the type of the phenomenon (eclipse or occultation)
     including the satellite numbers in the form "nem" or "nom",
     where n is the number of the occulting or eclipsing satellite
and m - is the number of the occulted or eclipsed satellite.
Obs - observatory code (see below).
UTC - the time instant in the UTC scale (h, m, s).
X, Y - X=Delta(alpha)*cos(delta), Y=Delta(delta)
     (occulting satellite relative to occulted one
     or eclipsing satellite relative to eclipsed one)
     in arcseconds in ICRF.
sigmaX, sigmaY - rms of X, Y, correspondingly, in arcseconds.
     This is because of random errors of the photometry.
O-C_X, O-C_Y - differences of X, Y from the results
     of the satellites motion theory ( V. Lainey 1.1 ), in arcseconds.
s, pos - apparent distance (arcsec) and positional angle (deg.),
     accorsding to X, Y .
Q - index of the result quality, following from processing:
     Q=0 - normal result,
     Q=1 - doubtful photometric data
     Q=2 - result following from low quality photometry.
     Q=3 - result is very different from other observatory one.
Smin - minimum of the normalized modelled flux. 

Explanations for the Table 7 of astrometric results (second type).
 
Date - date of observation.
Type - the type of the phenomenon (eclipse or occultation)
     including the satellite numbers in the form "nem" or "nom",
     where n is the number of the occulting or eclipsing satellite
and m - is the number of the occulted or eclipsed satellite.
Obs - observatory code.
UTC - the time instant in the UTC scale (h, m, s).
pos - position angle (degrees, ICRF) of the occulting or eclipsing satellite
     relative to the occulted or eclipsed one.
prec. - precision (arcsec) of apparent position
     along the apparent relative trajectory of the satellite
     as obtained with the least-square method.
Q - sign showing the reason why only one coordinate was determined:
     Q=0 - normal result,
     Q=1 - doubtful photometric data
     Q=2 - result following from low quality photometry.
     Q=3 - result is very different from other observatory one.
In these cases the apparent relative position of the satellite
measured across the apparent trajectory can not be determined
accurately enough and therefore position angles can be determined only
up to ± 180 degrees. 



Data2: 
1)The photometric light curves under ascii files 
   Content of each file: 
one photometric observed flux on each line (date, flux from 0 -no flux, total
event- to 1-flux outside the event- and modelled flux fitted on the observation)
Each file contains 3 quantities:
1. date in minutes from 0 h (UTC) of the day.
2. observed flux
3. modelled flux
Files under the form: GYYYYMMDD_XXX_YYY_n.txt
where DDDD is the year, MM the monthg and DD the day:
      XXX is the event as 1O3 means J1 occults J3 and 4E2 means J4 eclipses J2
      YYY is the observing site as described in the file phemu09-sites.txt
      n is 0, 1, ... for several observations at the same instrument and for
        several reductions using a different reference satellite.

2)The list of the observing sites
the file phemu09-sites-tables-3-and-4.txt contains the list of the observing sites
with positions, telescopes and detectors used.