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J/MNRAS/413/1024    Deep proper-motion survey of Blanco 1    (Platais+, 2011)

A deep proper-motion survey of the nearby open cluster Blanco 1. Platais I., Girard T.M., Vieira K., Lopez C.E., Loomis C., Mclean B.J., Pourbaix D., Moraux E., Mermilliod J.-C., James D.J., Cargile P.A., Barnes S.A., Castillo D.J. <Mon. Not. R. Astron. Soc., 413, 1024-1035 (2011)> =2011MNRAS.413.1024P
ADC_Keywords: Clusters, open ; Proper motions Keywords: astrometry - stars: kinematics and dynamics - open clusters and associations: individual: Blanco 1 Abstract: We provide two comprehensive catalogues of positions and proper motions in the area of open cluster Blanco 1. The main catalogue, CtlgM (table1), contains 6271 objects down to V∼18.5 and covers a circular ∼11deg2 area. The accuracy of CtlgM proper motions, at about 0.3-0.5mas/yr for well-measured stars, permits an excellent segregation between the cluster and field stars. Description: Nearly all photographic imaging for the astrometry of Blanco 1 has been obtained at the Cesco Observatory in El Leoncito, Argentina, with the 51-cm double astrograph (scale 55.1arcsec/mm). The earliest epoch of that plate material dates back to 1967, while the most recent CCD observations were obtained in 2007. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 101 6271 Main astrometric catalog CtlgM table3.dat 95 11598 Deep astrometric catalog CtlgD table4.dat 21 20 Cross-identifications with Eggen (1970ApJ...161..159E) table5.dat 16 23 Cross-identifications with Perry et al. (1978PASP...90...81P) table6.dat 13 262 Cross-ids with de Epstein & Epstein (1985AJ.....90.1211D) table7.dat 13 139 Cross-ids with Westerlund et al. (Table 3-4, 1988A&AS...76..101W) table8.dat 26 409 *Cross-ids with Moraux et al. (2007A&A...471..499M) table9.dat 21 148 Cross-ids with Mermilliod et al. (Table 1, 2008A&A...485...95M) table10.dat 31 44 Cross-ids with Micela et al. (Table 4, 1999A&A...344...83M) table11.dat 32 42 Cross-ids with Pillitteri et al. (Table A.1., 2004A&A...421..175P)
Note on table8.dat: original file in J/A+A/471/499 is listed as lmscand.dat
See also: J/A+AS/76/101 : UBV and uvbyb in zeta Scl cluster (Westerlund+, 1988) J/A+A/421/175 : XMM sources in Blanco 1 (Pillitteri+, 2004) J/A+A/471/499 : Low-mass stars and brown dwarfs in Blanco 1 (Moraux+, 2007) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 5 I5 --- CtlgM [1/6271] Sequential identifier 6- 11 F6.2 mag Vmag Photographic V-magnitude 12- 23 F12.7 deg RAdeg Right ascension (J2000), epoch 2000.0 24- 35 F12.7 deg DEdeg Declination (J2000), epoch 2000.0 36- 42 F7.1 mas/yr pmRA Proper motion in RA multiplied by cos(DE) 43- 47 F5.1 mas/yr e_pmRA Standard error of proper motion in RA 48- 54 F7.1 mas/yr pmDE Proper motion in Dec 55- 59 F5.1 mas/yr e_pmDE Standard error of proper motion in DE 60- 62 I3 % Prob [0/99] Cluster membership probability 63- 65 I3 --- Npos [4/64] Number of used positions 66- 68 I3 --- Ndel [0/7] Number of deleted positions 69- 71 I3 yr DEp [22/45] Maximum span of epochs 72- 83 F12.8 rad Xt Tangential coordinate along RA direction 84- 95 F12.8 rad Yt Tangential coordinate along Dec direction 97-101 I5 --- CtlgD [1/11598]? Cross-identification with table3
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 5 I5 --- CtlgD [1/11598] Sequential identifier (1) 6- 11 F6.2 mag Vmag Photographic V-magnitude 12- 23 F12.7 deg RAdeg Right ascension (J2000), epoch 2000.0 24- 35 F12.7 deg DEdeg Declination (J2000), epoch 2000.0 36- 42 F7.1 mas/yr pmRA Proper motion in RA multiplied by cos(Dec) 43- 47 F5.1 mas/yr e_pmRA Standard error of proper motion in RA 48- 54 F7.1 mas/yr pmDE Proper motion in Dec 55- 59 F5.1 mas/yr e_pmDE Standard error of proper motion in Dec 60- 62 I3 % Prob [0/99] Cluster membership probability 63- 65 I3 --- Npos [3/12] Number of used positions 66- 68 I3 --- Ndel [0/3] Number of deleted positions 69- 71 I3 yr DEp [22/45] Maximum span of epochs 72- 83 F12.8 rad Xt Tangential coordinate along RA direction 84- 95 F12.8 rad Yt Tangential coordinate along Dec direction
Note (1): in order not to mix up the numbering systems, anywhere else a composite StarID+100000 number is used.
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 12 A12 --- HD/CoD HD or CoD designation (1) 13- 18 I6 --- CtlgM Cross-identification with CtlgM 20- 21 I2 % Prob [0/99] Cluster membership probability
Note (1): star marked as HD 224949 is actually HD 224948.
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 6 I6 --- HD HD number 9- 13 I5 --- CtlgM Cross-identification with CtlgM 15- 16 I2 % Prob [0/99] Cluster membership probability
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 3 I3 --- ZS Star number from de Epstein & Epstein (1985AJ.....90.1211D), <Cl* Blanco 1 ZS NNNa> in Simbad (1) 5- 10 I6 --- Ctlg Cross-identification with CtlgM or CtlgD (G1) 12- 13 I2 % Prob [0/99]?=-1 Cluster membership probability
Note (1): star 30a is re-assigned as star 262. Star 133 is missing in our catalogs.
Byte-by-byte Description of file: table7.dat
Bytes Format Units Label Explanations
1- 3 I3 --- WGL Star number from Westerlund et al. (1988A&AS...76..101W), <Cl* Blanco 1 WGL NNN> in Simbad 6- 10 I5 --- CtlgM Cross-identification with CtlgM 11- 13 I3 % Prob [0/99] Cluster membership probability
Byte-by-byte Description of file: table8.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Name Object name from Moraux et al. (2007A&A...471..499M), <[MBS2007b] FNN-NN-NNN> in Simbad 12- 17 I6 --- Ctlg Cross-identification with CtlgM or CtlgD (G1) 18- 20 I3 % Prob [0/99] Cluster membership probability 21- 26 F6.2 mag Vmag Photographic V-magnitude
Byte-by-byte Description of file: table9.dat
Bytes Format Units Label Explanations
1- 4 I4 --- MPJ Star number from Mermilliod et al. (2008A&A...485...95M), <Cl* Blanco 1 MPJ NNN> in Simbad 7- 11 I5 --- CtlgM Cross-identification with CtlgM 12- 14 I3 % Prob [0/99] Cluster membership probability 15- 21 F7.2 km/s RV Mean radial velocity (Mermilliod et al., 2008A&A...485...95M)
Byte-by-byte Description of file: table10.dat
Bytes Format Units Label Explanations
1- 3 I3 --- BlX BLX source number from Micela et al. (1999A&A...344...83M), <BlX NN> in Simbad 5- 10 I6 --- Ctlg Cross-identification with CtlgM or CtlgD (G1) 11- 16 F6.2 mag Vmag Photographic V magnitude 17- 19 I3 % Prob [0/99] Cluster membership probability 20- 25 F6.1 arcsec dRA Difference "Micela-Ctlg" in RA*cos(Dec) 26- 31 F6.1 arcsec dDE Difference "Micela-Ctlg" in DE
Byte-by-byte Description of file: table11.dat
Bytes Format Units Label Explanations
2- 4 I3 --- Opt Source number from Pillitteri et al. (2004A&A...421..175P), <[PMS2004] Opt NNN> in Simbad 6- 11 I6 --- Ctlg Cross-identification with CtlgM or CtlgD (G1) 12- 17 F6.2 mag Vmag Photographic V magnitude 18- 20 I3 % Prob [0/99] Cluster membership probability 21- 26 F6.1 arcsec dRA Difference "Pillitteri-Ctlg" in RA*cos(DE) 27- 32 F6.1 arcsec dDE Difference "Pillitteri-Ctlg" in DE
Global notes: Note (G1): For CtlgM, No. 1 to 6271; for CtlgD No. 100001 to 111598.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 14-Nov-2011
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

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