J/AJ/124/601  Absolute positions and proper motions in NGC 188  (Platais+, 2002)

WIYN Open Cluster Study. VIII. The geometry and stability of the NOAO CCD Mosaic Imager Platais I., Kozhurina-Platais V., Girard T.M., van Altena W.F., Klemola A.R., Stauffer J.R., Armandroff T.E., Mighell K.J., Dell'Antonio I., Falco E.E., Sarajedini A. <Astron. J. 124, 601 (2002)> =2002AJ....124..601P 2002AJ....124..601P
ADC_Keywords: Clusters, open ; Proper motions ; Photometry, UBV Keywords: astrometry - catalogs - instrumentation: detectors - open clusters and associations: individual (NGC 188) Abstract: The field of direct imaging is experiencing a considerable growth in the number of available CCD mosaic imagers, especially on large telescopes. To fully exploit the astrometric potential of these imaging devices, we develop a technique, utilizing an astrometric standard, for precision transformation of pixel coordinates into a global coordinate system. We have constructed a new astrometric standard set of 1863 stars in the field of NGC 188 to derive the CCD chip constants for the NOAO CCD Mosaic Imager. The multiple-epoch data on the Mosaic's metrics indicate that this CCD mosaic device may have experienced a one-time nonelastic expansion. We also present a new determination of the pixel scale and the optical field angle distortion constants for the KPNO Mayall 4 m telescope prime focus field corrector. To establish a reliable history of the CCD mosaic imager metrics for current and potential future astrometric applications, we recommend obtaining astrometric calibrations for CCD mosaic imagers on a regular basis. Apart from mechanical positioning of the CCD mosaic camera on the telescope, noticeable changes in the thermal environment of CCD mosaic chips should also prompt new astrometric calibrations. It is shown that, following all precautions, the NOAO CCD Mosaic Imager can produce excellent astrometric results on the Mayall 4 m telescope. Description: This file has not been included in the paper, although it was instrumental in deriving the NOAO Mosaic Imager CCD chip constants and distortion coefficients. The file contains an astrometric standard around the open cluster NGC 188. It can serve as a medium depth (V=17) astrometric standard and as a source of absolute proper motions. The typical accuracy of proper motions is 1.5 to 2.0mas/yr for stars brighter than V=14 and reaches 7.0mas/yr at the limiting magnitude. The mean internal precision of the equatorial coordinates is 60 mas or better. The precision of BV photographic photometry, calibrated using the available photoelectric BV photometry, is 0.07mag in each bandpass. The astrometric standard around NGC 188 is based on twenty five 8x10 inch format plates taken with the Lick 51-cm double astrograph (scale 55.1"/mm) located on Mt. Hamilton, California. The basic data on this plate material are provided in Table 1, where the beginning and the end of exposures are given either in Universal Time (UT) or Local Siderial Time (LST) as listed on plate envelopes. In addition, the photographic emulsion, filter and observer are also indicated. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file plates.dat 78 25 Plate material ngc188.dat 64 1863 Catalog of positions, absolute proper motions and BV photographic photometry in the region of open cluster NGC 188 -------------------------------------------------------------------------------- See also: J/AJ/122/1486 : NGC 2451A proper motions and membership (Platais+, 2001) Byte-by-byte Description of file: plates.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Plate Plate number (1) 9- 18 A10 "YYYY/MM/DD" ObsDate Observation date 21- 28 A8 "HH:MM:SS" ObsTime1 Time of beginning of the observation 29 A1 --- --- [-] 30- 37 A8 "HH:MM:SS" ObsTime2 Time of end of the observation 40- 42 A3 --- n_ObsTime1 UT or LST time of observation 45- 49 A5 --- Emul Emulsion 52- 56 A5 --- Filter Filter 59- 73 A15 --- Obs Observer's name -------------------------------------------------------------------------------- Note (1): Only a selected sample of stars was measured on the plates. All stars down to the plate limit have been measured within a circular area with a 30' radius centered on RA=0h 44m 20s, DE=+85°19'(J2000). In addition, a sample of Hipparcos and Tycho-2 stars were measured in a larger 2x2° area having the same center. In the catalog the Hipparcos and Tycho-2 stars can be identified as those having identification numbers higher than 9800. (Some of them have duplicate entries among the stars in the main body of the catalog.) The details on plate measurements and reductions are given in the paper. -------------------------------------------------------------------------------- Byte-by-byte Description of file: ngc188.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID Object identifier 6- 15 F10.8 rad RArad Right ascension for the epoch J2000 and in the ICRS reference system (i.e. equinox J2000.0) 17- 26 F10.8 rad DErad Declination for the epoch J2000, equinox J2000.0 28- 34 F7.1 mas/yr pmRA Absolute proper motion in right ascension multiplied by cos(DE) 36- 42 F7.1 mas/yr pmDE Absolute proper motion in declination 44- 48 F5.2 mag Vmag Photographic V-magnitude 50- 54 F5.2 mag B-V Photographic B-V color 56- 58 F3.1 mas/yr e_pmRA Estimated standard error of proper motion in one coordinate (mean of RA and DE) 60- 61 I2 --- n_RArad Number of plates used for a solution in right ascension 63- 64 I2 --- n_DErad Number of plates used for a solution in declination -------------------------------------------------------------------------------- History: Copied at http://www.astro.yale.edu/astrom References: Von Hippel & Sarajedini, Pap I 1998AJ....116.1789V 1998AJ....116.1789V Sarajedini et al., Pap II 1999AJ....118.2894S 1999AJ....118.2894S Sarajedini, Pap III 1999AJ....118.2321S 1999AJ....118.2321S Sarajedini et al., Pap IV 1999AJ....118.2894S 1999AJ....118.2894S Barrado et al., Pap V 2001ApJ...549..452B 2001ApJ...549..452B Sills & Sarajedini, Pap VI 2000ApJ...544..944S 2000ApJ...544..944S Platais et al., Pap VII 2001AJ....122.1486P 2001AJ....122.1486P, Cat. J/AJ/122/1486 Stassun et al., Pap IX 2002A&A...382..899S 2002A&A...382..899S, Cat. J/A+A/382/899 Grocholski & Sarajedini Paper X 2002AJ....123.1603G 2002AJ....123.1603G von Hippel et al., Pap XI 2002AJ....124.1555V 2002AJ....124.1555V Deliyannis et al., Pap XII 2002ApJ...577L..39D 2002ApJ...577L..39D Barnes Pap XIII 2003ApJ...586..464B 2003ApJ...586..464B Barnes Pap XIV 2003ApJ...586L.145B 2003ApJ...586L.145B Kafka & Honeycutt, Pap XV 2003AJ....126..276K 2003AJ....126..276K Grocholski & Sarajedini, Pap XVI 2003MNRAS.345.1015G 2003MNRAS.345.1015G Platais et al., Pap XVII 2003AJ....126.2922P 2003AJ....126.2922P, Cat. J/AJ/126/2922 Mathieu et al., Pap XVIII 2004ApJ...602L.121M 2004ApJ...602L.121M Sarajedini, et al., Pap XIX 2004AJ....127..991S 2004AJ....127..991S Kafka et al., Pap XX 2004AJ....127.1622K 2004AJ....127.1622K Steinhauer & Deliyannis, Pap XXI 2004ApJ...614L..65S 2004ApJ...614L..65S Meibom & Mathieu, Pap XXII 2005ApJ...620..970M 2005ApJ...620..970M von Hippel et al., Pap XXIII 2006ApJ...645.1436V 2006ApJ...645.1436V Hole et al. Pap XXIV 2009AJ....138..159H 2009AJ....138..159H, Cat. J/AJ/138/159 James et al., Pap XXV Platais et al., Pap XXVI 2007A&A...461..509P 2007A&A...461..509P, Cat. J/A+A/461/509 Kafka et al., Pap XXVII Giampapa et al., Pap XXVIII 2006ApJ...651..444G 2006ApJ...651..444G Meibom et al., Pap XXIX 2006ApJ...653..621M 2006ApJ...653..621M Jeffery et al., Pap XXX 2007ApJ...658..391J 2007ApJ...658..391J Meibom et al., Pap XXXI 2007ApJ...665L.155M 2007ApJ...665L.155M Geller et al., Pap XXXII 2008AJ....135.2264G 2008AJ....135.2264G, Cat. J/AJ/135/2264 Yadav et al., Pap XXXIII 2008A&A...484..609Y 2008A&A...484..609Y, Cat. J/A+A/484/609 Meibom et al., Pap XXXIV 2009ApJ...695..679M 2009ApJ...695..679M, Cat. J/ApJ/695/679 Platais et al., Pap XXXV 2008MNRAS.391.1482P 2008MNRAS.391.1482P, Cat. J/MNRAS/391/1482 Geller et al., Pap XXXVI 2009AJ....137.3743G 2009AJ....137.3743G, Cat. J/AJ/137/3743 Meibom et al., Pap XXXVII 2009AJ....137.5086M 2009AJ....137.5086M, Cat. J/AJ/137/5086 Geller et al., Pap XXXVIII 2010AJ....139.1383G 2010AJ....139.1383G, Cat. J/AJ/139/1383 Anthony-Twarog et al., Pap XXXIX 2010AJ....139.2034A 2010AJ....139.2034A, Cat. J/AJ/139/2034 Sarajedini et al., Pap XL 2009ApJ...698.1872S 2009ApJ...698.1872S Chumak et al., Pap XLI 2010MNRAS.402.1841C 2010MNRAS.402.1841C Casetti-Dinescu et al., Pap XLII 2010AJ....139.1889C 2010AJ....139.1889C James et al., Pap XLIII 2010A&A...515A.100J 2010A&A...515A.100J, Cat. J/A+A/515/A100 Platais et al., Pap XLIV 2011MNRAS.413.1024P 2011MNRAS.413.1024P, Cat. J/MNRAS/413/1024 Meibom et al., Pap XLV 2011ApJ...733..115M 2011ApJ...733..115M, Cat. J/ApJ/733/115 Platais et al., Pap XLVI 2011ApJ...733L...1P 2011ApJ...733L...1P Gosnell et al., Pap XLVII 2012ApJ...745...57G 2012ApJ...745...57G Geller & Mathieu Pap XLVIII 2012AJ....144...54G 2012AJ....144...54G Platais et al., Pap XLIX 2012ApJ...751L...8P 2012ApJ...751L...8P Cummings et al., Pap L 2012AJ....144..137C 2012AJ....144..137C Geller et al., Pap LI 2013AJ....145....8G 2013AJ....145....8G Yang et al., Pap LII 2013ApJ...762....3Y 2013ApJ...762....3Y Sandquist et al., Pap LIII 2013ApJ...762...58S 2013ApJ...762...58S Anthony-Twarog, Pap LIV 2013ApJ...767L..19A 2013ApJ...767L..19A Platais et al., Pap LV 2013AJ....146...43P 2013AJ....146...43P, Cat. J/AJ/146/43 Pap LVI Maderak et al., Pap LVII 2013AJ....146..143M 2013AJ....146..143M Pap LVIII Tofflemire et al., Pap LIX 2014AJ....148...61T 2014AJ....148...61T, Cat. J/AJ/148/61 Milliman et al., Pap LX 2014AJ....148...38M 2014AJ....148...38M, Cat. J/AJ/148/38 Anthony-Twarog et al., Pap LXI 2014AJ....148...51A 2014AJ....148...51A, Cat. J/AJ/148/51 Thompson et al., Pap LXII 2014AJ....148...85T 2014AJ....148...85T, Cat. J/AJ/148/85 Maderak et al., Pap LXIII 2015AJ....149..141M 2015AJ....149..141M Pap LXIV Lee-Brown et al., Pap LXV 2015AJ....149..121L 2015AJ....149..121L, Cat. J/AJ/149/121 Leiner et al., Pap LXVI 2015AJ....150...10L 2015AJ....150...10L, Cat. J/AJ/150/10 Geller et al. Pap LXVII 2015AJ....150...97G 2015AJ....150...97G, cat. J/AJ/150/97 Pap LXVIII Pap LXIX Pap LXX Milliman et al., Pap LXXI 2016AJ....151..152M 2016AJ....151..152M, cat. J/AJ/151/152 Anthony-Twarog et al., Pap LXXII 2016AJ....152..192A 2016AJ....152..192A, cat. J/AJ/152/192 Pap LXXIII Pap LXXIV Cummings et al., Pap LXXV 2017AJ....153..128C 2017AJ....153..128C Anthony-Twarog et al., Pap LXXVI 2018AJ....155..138A 2018AJ....155..138A
(End) Patricia Bauer [CDS] 21-Jan-2002
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