Contents. planet: 5 - Jupiter satellites: J1 - Io : 2, J2 - Europa : 0, J3 - Ganymede : 4, J4 - Callisto : 1 total number: 7 type: relative dates: 2021-2021 observatory: see observatories below. Reference. Emelyanov N. V., Arlot J.-E. and 38 co-authors The PHEMU21 catalogue and astrometric results of the observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter made in 2021. Monthly Notices of the Royal Astronomical Society. 2022. V. 516, P. 3685-3691. DOI:10.1093/mnras/stac2538 See Abstract Informations. relative to: reference body is an occulted or eclipsed satellite: J1 - Io : 4, J2 - Europa : 1, J3 - Ganymede : 1, J4 - Callisto : 1 reference frame: astrometric centre of frame: topocenter for mutual occultation or heliocenter for mutual eclipse epoch of equinox: J2000 time scale: UTC reduction: from mutual occultations and eclipses coordinates: Position angle (topocentric for mutual occultation or heliocentric for mutual eclipse) diff. refraction: no information receptor: photometric (see the relevant article) telescope: See in the publication observers: See in the publication data included in standard data file : no Comments. Data are deduced from the photometric observations of the mutual occultations and eclipses made during the international campaign in 2021. The description of these astrometric data is given in the relevant article (see Reference). The coordinates of the observatories are given below. The second group of the data is presented in this item. The "O-C' are given with respect of the theory by V.Lainey (Lainey, V., Arlot, J. E., Karatekin, O., van Hoolst, T. 2009. Nature. V. 459. P 957.) The first group of the data see in the item jg0067 of the NSDC. Observatory code with geographic coordinates. East Altitude m Observers, Longitude Latitude or Affiliations Code deg deg IAU Code --------------------------------------------------------- AUR 1.690555 43.540833 241.0 Andre P., IOTA-ES, Societe Astronomique de France, Adagio Belesta GLE 150.500444 -23.130109 (Q70) Kerr S., Trans-Tasman Occultation Alliance, Murrumbateman Observatory, Australia; GRA 248.131306 33.816694 830.0 George T., IOTA, Scottsdale, AZ USA; OAG 5.340278 43.150555 200.0 Gourdon F., Roger P., OAGC Observatoire Astronomique du Gros Cerveau, Ollioules, France; PAU 248.04778 33;811944 0.0 Maley P., IOTA and NASA Johnson Space Center Astronomical Society, Carefree, AZ, USA MAD 356.338889 40.449167 720.0 Izquierdo J., Agrupacion Astronomica de Madrid, Madrid, Spain; Format. 1. Observatory code see the table above. 2. The type of the phenomenon (eclipse or occultation) including the satellite numbers. The type of phenomenon is coded as n_a o n_p or n_a e n_p for a mutual occultation or eclipse, respectively. Here $n_a$ is the number of the occulting or eclipsing satellite and $n_p$ is the number of the occulted or eclipsed satellite. 3. Year of observation 4. Month of observation 5. Day of observation 6. Hour of the astrometric data (UTC) 7. Minute of the astrometric data (UTC) 8. Seconde of the astrometric data with decimals (UTC) 9. Position angle A in degrees (topocentric for mutual occultation or heliocentric for mutual eclipse) 10. Precision of apparent position along the apparent relative trajectory of the satellite as obtained with the least-square method, in arcseconds 11. O-C along the apparent relative trajectory, in arcseconds. 12. Flag R assigned showing the reason why only one coordinate was determined: R=0 - there is no doubt about the results; R=1 - astrometric results are doubtful. ------------------------------------------------------------ Observ. Year Position sigma code month UTC angle A O-C R Type date h m s deg arcsec arcsec ------------------------------------------------------------