J/A+A/493/1183 Saturn major satellites observations (1874-2007) (Desmars+, 2009)

A new catalogue of observations of the eight major satellites of Saturn (1874-2007). Desmars J., Vienne A., Arlot J-E. <Astron. Astrophys. 493, 1183 (2009)> =2009A&A...493.1183D 2009A&A...493.1183D
ADC_Keywords: Planets ; Positional data Keywords: catalogs - planets and satellites: individual: Saturn - astrometry Abstract: The last catalogue of observations (Strugnell & Taylor, 1990A&AS...83..289S 1990A&AS...83..289S) includes about 51000 observations (over 3500 nights) of Saturnian satellites from 1874 to 1989. Since 1989, many observations have been published, often in different format, specific to the publication. This new catalogue of observations of the eight major satellites of Saturn includes the observations of Strugnell & Taylor (1990A&AS...83..289S 1990A&AS...83..289S), many other published since 1989 and also old observations forgotten in the previous catalogue. All those observations are tabulated in the consistent format. We precise, for each observation, the corrections applied for reduction like refraction, aberration or phase effects. Furthermore, when it was possible, instrument and catalogue are also indicated. The new catalogue presents more than 130000 observations (over 6000 nights) of the eight major satellites of Saturn from 1874 to 2007. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 99 59540 Catalogue of observations of Saturnian satellites obscodes.dat 81 1403 Observatory codes -------------------------------------------------------------------------------- See also: J/A+AS/139/305 : Position of Saturn's satellites (1982-1988) (Veiga+, 1999) J/A+AS/121/65 : 1990-1994 Saturn's satellites astrometry (Harper+ 1997) J/A+AS/136/257 : Saturn's satellites in 1995/97 (Harper+ 1999) J/A+A/422/377 : 1997-2000 Saturn's satellites astrometry (Qiao+, 2004) J/other/KFNT/15.483 : Positions of Phoebe in 1998 opp. (Ledovskaya+ 1999) J/A+A/391/767 : CCD observations of Phoebe in 1998-1999 (Fienga+, 2002) J/A+A/383/1054 : Astrometry of Pluto and Saturn in 1995-2001 (Rapaport+, 2002) J/AJ/103/983 : Stellar occultation candidates of Saturn (Bosh+, 1992) J/A+A/485/293 : Events of Saturn satellites during 2009 equinox (Arlot+, 2008) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Opp Opposition number (1) 5- 22 A18 --- Date UTC date of observation (YYYY/MM/DD.ddddddd). Not light-time corrected 24- 29 F6.3 s dt ET-UTC (seconds) 31- 33 A3 --- Obs Observatory code (2) 35- 37 I3 --- Ref [1/608] Reference code 39 I1 --- Type [0/3] Observation type (3) 41 I1 --- S [1/8] Observed satellite (4) 42 A1 --- Sr [0-8 *] Reference satellite (4) 44 I1 --- f_Obs1 [0/1] Presence flag for first observation (5) 45 I1 --- f_Obs2 [0/1] Presence flag for second observation (5) 47- 58 F12.7 --- Obs1 ?=0.0000000 First observation of pair, RA, DRAcosDE, DRA or PA (6) 60- 71 F12.7 --- Obs2 ?=0.0000000 Second observation of pair, DE, DDE, DDE or Sep (6) 73 I1 --- Sys [0/4] Reference system (7) 75 I1 --- Fr [0/2] Reference frame (8) 77- 83 F7.3 arcsec (O-C)1 ?=999.999 (O-C) residual for first pair of observation (9) 85- 91 F7.3 arcsec (O-C)2 ?=999.999 (O-C) residual for second pair of observation (9) 93 I1 --- rf [0/3] Refraction correction (10) 95 I1 --- ab [0/3] Aberration correction (10) 97 I1 --- ph [0/3] Phase effects correction (10) 99 I1 --- S2 [1/8]? (optionnal) reference satellite for O-C computation (4) -------------------------------------------------------------------------------- Note (1): Opposition number: 1 = 1610, 257 = 1874, 385 = 2007 Note (2): From Minor Planet Center (code IAU) http://cfa-www.harvard.edu/iau/lists/ObsCodes.html See obscodes.dat file Note (3): Observation type as follows: 0 = α, δ (degrees) 1 = Δα*cos(δ), Δδ (arcsecond) 2 = Δα, Δδ (second, arcsecond) 3 = PA,Sep (position angle,separation) (degrees, arcsecond) Note (4): Reference satellite as follows: * = absolute coordinates 0 = Saturn 1 = Mimas 2 = Enceladus 3 = Tethys 4 = Dione 5 = Rhea 6 = Titan 7 = Hyperion 8 = Iapetus Note (5): Presence flag as follows: 0 = observation missing 1 = observation present Note (6): The content is defined by observation type. 0.0000000 if presence flag = 0 Note (7): Reference system as follows: 0 = mean equator and equinox of B1950 1 = true equator and equinox of date of the observation 2 = mean equator and equinox of J2000 3 = mean equator and equinox at the nearest beginning of a year 4 = mean equator and equinox at 1st January of the year of observation Note (8): Reference frame as follows: 0 = topocentric 1 = geocentric 2 = heliocentric (used for mutual events) Note (9): 999.999 if presence flag = 0; 888.888 if residual great than 100.0 arcsec Note (10): Correction code as follows: 0 = corrected 1 = presumedly corrected 2 = not presumedly corrected 3 = not corrected -------------------------------------------------------------------------------- Byte-by-byte Description of file: obscodes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- Code Observatory code 5- 13 F9.5 deg LON ? East longitude 15- 22 F8.6 --- cosLAT ? Cosinus of latitude 24- 32 F9.6 --- sinLAT ? Sinus of latitude 34- 81 A48 --- Name Observatory name -------------------------------------------------------------------------------- Acknowledgements: Josselin Desmars, desmars(at)imcce.fr
(End) Josselin Desmars [IMCCE, France], Patricia Vannier [CDS] 10-Oct-2008
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line