/ftp/cats/A+A/595/L2



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J/A+A/595/L2     Proper motions in NGC6681 globular cluster     (Massari+, 2016)
The following files can be converted to FITS (extension .fit or fit.gz)
	pm_tab.dat list.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/595/L2
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Beginning of ReadMe : J/A+A/595/L2 Proper motions in NGC6681 globular cluster (Massari+, 2016) ================================================================================ HST-GeMS proper motions in the globular cluster NGC6681. Massari D., Fiorentino G., McConnachie A., Bellini A., Tolstoy E., Turri P., Andersen D., Bono G., Stetson P.B., Veran J.-P. <Astron. Astrophys. 595, L2 (2016)> =2016A&A...595L...2M (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Galaxies, nearby ; Clusters, globular ; Proper motions Keywords: astrometry - proper motions - instrumentation: adaptive optics - globular clusters: individual: NGC6681 - dwarf galaxies: individual: dSph Abstract: For the first time the astrometric capabilities of the MCAO facility GeMS with the GSAOI camera on Gemini-South are tested to quantify the accuracy in determining stellar proper motions in the Galactic globular cluster NGC 6681. Proper motions from HST/ACS for a sample of its stars are already available, and this allows us to construct a distortion-free reference at the epoch of GeMS observations that is used to measure and correct the temporally changing distortions for each GeMS exposure. In this way, we are able to compare the corrected GeMS images with a first-epoch of HST/ACS images to recover the relative proper motion of the Sagittarius dwarf spheroidal galaxy with respect to NGC 6681. We find this to be (pm_alpha_cosdelta, pm_delta_)=(4.09,-3.41)mas/yr, which matches previous HST/ACS measurements with a very good accuracy of 0.03mas/yr and with a comparable precision (r.m.s of 0.43mas/yr). This study successfully demonstrates that high-quality proper motions can be measured for quite large fields of view (85arcsecx85arcsec) with MCAO-assisted, ground-based cameras and provides a first, successful test of the performances of GeMS on multi-epoch data. Description: Magnitude, proper motions and related uncertainties for the stars in common to the HST sample of Massari et al. (2013ApJ...779...81M) (see Fig. 3). Objects: ---------------------------------------------------------- RA (ICRS) DE Designation(s) ---------------------------------------------------------- 18 43 12.76 -32 17 31.6 NGC 6681 = M 70 ----------------------------------------------------------