J/A+A/580/A28       Astrometric observations of Phobos        (Pasewaldt+, 2015)

Astrometric observations of Phobos with the SRC on Mars Express: New data and comparison of different measurement techniques. Pasewaldt A., Oberst J., Willner K., Beisembin B., Hoffmann H., Matz K.D., Roatsch T., Michael G., Cardesin-Moinelo A., Zubarev A.E. <Astron. Astrophys. 580, A28 (2015)> =2015A&A...580A..28P 2015A&A...580A..28P
ADC_Keywords: Planets ; Positional data Keywords: Astrometry - ephemerides - planets and satellites: individual: Phobos Abstract: Mars Express (MEX) carried out 74 Phobos flybys at distances between 669 and 5579km from April 2008 to August 2011. Images taken with the Super Resolution Channel (SRC) were used to determine the Martian moon's spacecraft-centered right ascension and declination. Image positions of Phobos were measured using the control point and limb fit measurement techniques. Camera pointing and pointing drift were controlled by means of background star observations that were compared to the corresponding positions from the Tycho-2 catalog. Blurred and noisy images were restored by applying an image-based point spread function in a Richardson-Lucy deconvolution. Altogether, we provide 158 astrometric observations of Phobos with estimated uncertainties between 0.224 and 3.405km circular about the direction to the satellite. Control point measurements yield more accurate results than limb fit observations. Description: The data is given in the form of two tables. Each table contains the same set of observations: Data in tablea1.dat has been reduced using MEX navigation orbits and predicted attitude by the European Space Operations Centre (ESOC). tablea2.dat data has been derived using MEX accurate orbits by the Royal Observatory of Belgium (ROB) and measured attitude by the European Space Astronomy Centre (ESAC). From 158 astrometric observations 103 were determined by means of both methods, 27 using only control point measurements, and 28 performing only limb fit observations. Hence, each data table contains 261 entries, namely 130 control point measurements and 131 limb fit observations. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 104 261 Astrometric observations of Phobos reduced with ESOC navigation orbits and ESOC predicted attitude tablea2.dat 104 261 Astrometric observations of Phobos reduced with ROB accurate orbits and ESAC measured attitude -------------------------------------------------------------------------------- See also: J/A+A/487/755 : CCD observations of Martian Satellites (Veiga+, 2008) J/A+A/488/361 : Phobos Mars Express astrometric observations (Willner+, 2008) J/A+A/572/A104 : Astrometric obs. of Phobos and Deimos in 1971 (Robert+, 2014) Byte-by-byte Description of file: tablea1.dat tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Img Image name 13- 22 A10 "Y-M-D" Date Image date (UTC) 23 A1 --- --- [T] 24- 35 A12 "h:m:s" Time Image mid-time (UTC) 36 A1 --- --- [Z] 39- 40 A2 --- Meth Measurement method (1) 43- 50 F8.4 deg RAdeg Right ascension in the spacecraft-centered ICRF 53- 60 F8.4 deg DEdeg Declination in the spacecraft-centered ICRF 63- 70 F8.4 deg ePos [0.002/0.04] 1-σ uncertainty in right ascension and declination 73- 74 I2 --- Np [3/50] Number of measured control points/ percentage of measured limb points 76- 84 F9.2 km Xpos [-6987/8684] X coordinate of Mars Express spacecraft in the Mars-centered ICRF 86- 94 F9.2 km Ypos [-12538/13427] Y coordinate of Mars Express spacecraft in the Mars-centered ICRF 96-104 F9.2 km Zpos [-9140/9796] Z coordinate of Mars Express spacecraft in the Mars-centered ICRF -------------------------------------------------------------------------------- Note (1): Measurement method as follows: CP = Control point measurements LF = Limb fit observation -------------------------------------------------------------------------------- Acknowledgements: Andreas Pasewaldt, andreas.pasewaldt(at)tu-berlin.de
(End) Patricia Vannier [CDS] 30-Apr-2015
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