Contents.
planet: 5 - Jupiter
satellites: J1 - Io : 17,
J2 - Europa :214,
J3 - Ganymede : 33,
J4 - Callisto : 22
total number: 286
type: relative
dates: 1990-1992
observatory: see observatories coordinates below.
Reference.
Emelyanov N. V., Arlot J.-E.
Astrometric results PHEMU-1985 and PHEMU-1991.
Planetary and Space Science.
2020. V. 187. P. 104946.
2020P&SS__18704946E
Informations.
relative to: reference body is an occulted or eclipsed satellite:
J1 - Io :197,
J2 - Europa : 47,
J3 - Ganymede : 35,
J4 - Callisto : 7
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: X, Y (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 1985.
The description of these astrometric data
is given in the relevant article (see Reference).
The coordinates of the observatories are given below.
The first 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 second group of the data see in the following item jg0053 of the NSDC.
Observatory code with geographic coordinates.
Conventional Longitude Latitude
Code name deg ' " deg ' "
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BA1 BARCELONA-CAMPOS-T12_5 W 2 10 6 N 41 22 54
BA2 BARCELONA-FERNANDEZ-T16 W 2 10 6 N 41 22 54
BA3 BARCELONA-TORELL-T26 W 2 10 6 N 41 22 54
BAR BARI-IAF-T12 E 16 51 60 N 41 7 0
BE1 BELGRADE-L65 E 20 30 50 N 44 48 12
BE2 BELOGRADCHIK-T60 E 22 39 60 N 43 13 21
BER BERLIN-T50 E 13 28 36 N 52 29 15
BOR BORDEAUX-T60 W 5 16 30 N 44 50 7
BOW BOWIE-MAL-L15 W 76 45 47 N 38 58 55
BRA BRASOPOLIS-T60 W 45 33 54 S 22 31 6
BRE BRESGAU-L13 E 7 54 20 N 47 54 53
BUC BUCAREST-T50 E 26 5 45 N 44 24 50
CA1 CAIXIAS-RDG-T15 W 9 16 26 N 38 42 17
CA2 CAIXIAS-RDG-T40 W 9 16 26 N 38 42 17
CAT CATANIA-T91 E 15 5 9 N 37 30 13
CLU CLUJ-NAPOCA-T50 E 23 35 52 N 46 42 48
DEV DEVON-DEV W 113 45 30 N 53 23 26
ES1 ESO-T1M_IR W 70 43 48 S 29 15 24
ES2 ESO-T50 W 70 43 48 S 29 15 24
ESS ESSEN-T36 E 7 4 15 N 51 24 35
GEE GEEL-GEL-T20 E 4 59 12 N 51 9 26
GR1 GRASSE-T150_B E 6 55 30 N 43 44 56
GR2 GRASSE-T150_R E 6 55 30 N 43 44 56
GR3 GRASSE-T150_V E 6 55 30 N 43 44 56
HOL HOLTSVILLE-ASL-T20 W 19 6 41 N 40 18 0
HOS HOSTALETS-GEA-T41 E 2 12 30 N 41 32 22
JUN JUNGFRAU-T76 E 7 58 60 N 46 32 53
KA1 KAKUDA-L15 E 14 5 60 N 38 0 0
KA2 KAKUDA-T20 E 141 0 0 N 38 0 0
KAL KALAA-SGHIRA-T10 E 2 46 5 N 21 54 14
KOR KORNTAL-T35 E 9 11 51 N 48 47 0
KV1 KAVALUR-VBO-T102 E 78 40 54 N 12 34 32
KV2 KAVALUR-VBO-T235 E 78 40 54 N 12 34 32
KV3 KAVALUR-VBO-T75 E 78 40 54 N 12 34 32
LAP LA_PRIMAUDIERE-T32 W 1 30 0 N 48 5 0
MA1 MAUNA_KEA-T61 W 156 15 30 N 20 42 36
MA2 MAUNA_KEA-T84 W 156 15 30 N 20 42 36
MAS MASSA-BFF-T31 E 10 4 33 N 44 1 22
MEU MEUDON-T1M E 2 13 53 N 48 48 18
MIL MILANO-BRN-L8 E 9 7 2 N 45 27 19
MO1 MONEGRILLO-GEA-T41 E 2 12 30 N 41 32 22
MO2 MONTELUPO-SDN-T20 E 11 0 36 N 43 43 0
MOL MOLLET-GEA-T41 E 2 12 30 N 41 32 22
NI1 NICE-T40_B E 7 18 1 N 43 43 17
NI2 NICE-T40_R E 7 18 1 N 43 43 17
OH1 OHP-T193 E 5 42 60 N 43 55 46
OH2 OHP-T193_IR E 5 42 60 N 43 55 46
OH3 OHP-T80 E 5 42 60 N 43 55 46
OH4 OHP-T80_IR E 5 42 60 N 43 55 46
PAR PARIS-L38 E 2 20 15 N 48 50 0
PED PEDRO_GAO-JAF-T15 W 8 7 60 N 39 53 0
PIC PIC_DU_MIDI-T1M E 0 55 24 N 42 56 12
PIE PIERA-GEA-T41 E 2 12 30 N 41 32 22
REG REGGIO_DI_CALABRIA-GAR-T40 E 15 38 60 N 38 6 25
REU REUX-JBG-T25 E 5 5 27 N 50 14 43
RI1 RIO-DE-JANEIRO-L46 W 43 13 24 S 22 53 44
RI2 RIO_DE_JANEIRO-L46 W 43 13 24 S 22 53 44
ROM ROMA-NAL-T13 E 12 29 60 N 41 46 14
SAB SABADELL-GEA-T20 E 2 12 30 N 41 32 22
SE1 SEVILLA-JIMENEZ-T20_5 W 9 47 13 N 22 51 17
SE2 SEVILLA-PIQUERAS-L6 W 9 47 13 N 22 51 17
SE3 SEVILLE-JIMENEZ-T20_5 W 9 47 13 N 22 51 17
SID SIDING_SPRING-T61 E 149 3 45 S 31 16 24
STQ ST_QUINTI-GEA-T30 E 2 12 30 N 41 32 22
TA1 TABERNES_BLANQUES-RVS-T20 W 0 49 54 N 38 15 37
TA2 TABERNES_BLANQUES-T40 W 0 49 54 N 38 15 37
TEN TENERIFE-IAC-T51 W 16 35 0 N 28 15 0
TER TERAMO-T50 E 13 43 57 N 42 39 27
TIM TIMISOARA-T30 E 21 13 45 N 45 44 15
TO1 TOPEKA-NEKAAL-T25 W 95 41 0 N 39 2 0
TO2 TOPEKA-NEKAAL-T40 W 95 41 0 N 39 2 0
TOK TOKYO-CRL-T150_IR E 139 30 0 N 35 40 0
VER VERSAILLES-DMT-L8 E 2 9 40 N 48 48 16
ZOE ZOETERMEER-T30 E 4 18 0 N 52 4 0
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. X coordinate in arcseconds (topocentric for mutual occultation
or heliocentric for mutual eclipse)
10. Y coordinate in arcseconds (topocentric for mutual occultation
or heliocentric for mutual eclipse)
11. sigma of X in arcseconds
12. sigma of Y in arcseconds
13. "O-C" for X in arcseconds
14. "O-C" for Y in arcseconds
15. Angular separation s (in arcseconds) corresponding to X, Y.
16. Position angle A (in degrees) corresponding to X, Y.
17. Flag Q indicating the quality and the reliability of the result:
Q=0 - there is no doubt about the results;
Q=1 - the flux zero level in the photometry is not correctly excluded;
you can use the position angle as an astrometric result
instead the values $X, Y$.
Q=2 - the flux drop is small and noise signal is big in the photometry,
astrometric results are doubtful.
Q=3 - there is a significant error in the photometric data,
the results are not suitable.
18. The minimum level S min of normalized flux.
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Observ. Year Separation Position
code month X Y sigma X sigma Y O-C(X) O-C(Y) s angle Q
Type date h m s arcsec arcsec arcsec arcsec arcsec arcsec arcsec degrees S min
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