OBSERVATION SHEET (to be sent with the data after each observation to: phemu.imcce@obspm.fr or to IMCCE, PHEMU21, 77 ave. Denfert-Rochereau, F-75014 PARIS, France) ************************************************************* * In this sheet, fill up the lines after the sign ":". * Use proposed values (in parenthesis). * Leave the comments included in this sheet. * This sheet must be sent as an ASCII file (.txt) * the name of which being defined as follows. * .txt * One or several series of photometric measures associated to the phenomenon * described in the present sheet must be sent under the form of an ASCII file (.dat) * .dat * The structure of the name is given here after. * Observed phenomenon ID is made as follows. * E_aEp_T_ * where * is the predicted date of the middle of the phenomenon, * a is the number of satellite occulting or eclipsing (1,2,3,4), * E = o for occultation, E = e for eclipse, * p is the number of the occulted or eclipsed satellite (1,2,3,4), * T is the type of photometric measure made (0,1,2) as follows, * 0 = occultation * 1 = eclipsed satellite measured alone * 2 = eclipsed and eclipsing satellites measured together * identifies your observing site * Note that this identification must be different for a different * telescope even on the same site. * Please do not use "space" in the name, prefer "_" (underscore) * Example: * E200301062325_2e1_2_OHP_T80 pour sat 2 eclipses sat 1 * observation made at OHP with the 80cm telescope * on January 6, 2003 at 23h25m ************************************************************* --- fill up the sheet starting here --- Observed phenomenon ID: Number of the occulting or eclipsing satellite (1,2,3,4): Number of the occukted or eclipsed satellite (1,2,3,4): (1=Io, 2=Europe, 3=Ganymede, 4=Callisto). Type of photometric measure (0,1,2): (0=occultation) (1= eclipsed satellite measured alone) (2= eclipsed and eclipsing satellites measured together) Name or identification of the site of observation: (each different telescope if so has a different identification even if on the same observing site please do not use "space", prefer "underscore") IAU Code of your site of observation (XXX if not available): OR geographic coordinates of the site (blank if you provided an IAU code) Longitude = (E,W): deg: min: sec: Latitude = (N,S): deg: min: sec: Altitude = m: Type of telescope (refractor, reflector): Designation of the telescope: (please do not use "space", prefer "underscore") Diameter in cm: Focal length in cm: Description of the telescope: (blank if not useful) Filter (put X if no filter): Used detector (CCD, Video, Photometer, Web cam,...): Designation of the receptor: (please do not use "space", prefer "underscore") Description of the receptor: (blank if not useful) Conditions of observation: (seeing, meteo, clouds, absorption ...) Names of the observers and affiliations (one line per observer) Name, Surname, affiliation: Name of the coordinator: E-mail for contact: Format of the data for one observation (of one phenomenon) provide the format of the date UTC (0,1,2,3,4,5): (if not UTC please provide the difference with UTC in the comments below) 0 for decimal julian day (JD) 1 for a gregorian date (year, month, day, hour,minute,second) 2 for decimal days counted from Oh of the day of the middle of the phenomenon 3 for decimal hours counted from Oh of the day of the middle of the phenomenon 4 for decimal seconds counted from Oh of the day of the middle of the phenomenon 5 for units defined below counted from a UTC date provided below unit of time between two measures: date of the origin of the count of the time: provide here the code corresponding to the photometric measure (0,1): 0 for a relative flux (to a multiplicative constant) 1 for a magnitude (to an additive constant) Comments (if needed): --- end of the sheet to be filled up --- ******************************************************** * In the ASCII file .dat * you may put one or several series of photometric measures. * each series starts with a line describing each column * followed by lines of data composed of a date followed by * the photometric measure corresponding to that date * The maximum number of lines is 10000. * Example of file * * date flux sat1&3 flux sat4 ..... * 13.4563421 45889 34887 ..... * .......... ..... ..... ..... * date flux sat1 flux sat3 * 15.6678555 28554 20866 * ........ ..... ..... *********************************************************