J/AJ/152/192  WOCS. LXXII. A uvbyCaHb study of NGC 2506  (Anthony-Twarog+, 2016)

WIYN open cluster study. LXXII. A uvbyCaHβ CCD analysis of the metal-deficient open cluster NGC 2506. Anthony-Twarog B.J., Deliyannis C.P., Twarog B.A. <Astron. J., 152, 192-192 (2016)> =2016AJ....152..192A 2016AJ....152..192A (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, open ; Photometry, CCD ; Photometry, uvby ; Photometry, beta Keywords: methods: observational - techniques: photometric - open clusters and associations: individual: NGC 2506 Abstract: Precision uvbyCaHβ photometry of the metal-deficient, old open cluster NGC2506 is presented. The survey covers an area of 20'*20' and extends to V∼18 for b-y and Hβ and to V∼17.0 for c1 and hk. For V brighter than 16.0, photometric scatter among the indices leads to the recovery of six known variables within the cluster core and five new variables in the outer 5' of the survey field. Proper motions, radial velocities, and precise multicolor indices are used to isolate a highly probable sample of cluster members from the very rich color-magnitude diagram. From 257 highly probable members at the cluster turnoff, we derive a reddening estimate of E(b-y)=0.042±0.001 (E(B-V)=0.058±0.001), where the errors refer to the internal standard errors of the mean. [Fe/H] is derived from the A/F dwarf members using both m1 and hk, leading to [Fe/H]=-0.296±0.011 (sem) and -0.317±0.004 (sem), respectively. The weighted average, heavily dominated by hk, is [Fe/H]=-0.316±0.033. Based on red giant members, we place an upper limit of ±0.010 on the variation in the reddening across the face of the cluster. We also identify two dozen potential red giant cluster members outside the cluster core. Victoria-Regina isochrones on the Stromgren system produce an excellent match to the cluster for an apparent modulus of (m-M)=12.75±0.1 and an age of 1.85±0.05Gyr. Description: NGC2506 was observed using the 1.0m telescope operated by the SMARTS consortium at Cerro Tololo Inter-American Observatory (CTIO) over the UT dates 2011 December 16-22. The telescope was equipped with an STA 4000*4000 CCD camera yielding a field of view of 20' on a side at the Cassegrain focus of the 1.0m telescope. Filters owned by the University of Kansas were used to obtain images in each of the extended Stromgren system bandpasses (uvbyCa and the two Hβ bandpasses). With the exception of 2011 December 20/21, all of the nights were photometric. Table2 describes calibrated photometry for 2229 stars. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 156 2229 Stromgren photometry in NGC 2506 -------------------------------------------------------------------------------- See also: B/ocl : Optically visible open clusters and Candidates (Dias+ 2002-2015) II/215 : uvby-beta Catalogue (Hauck+ 1997) J/A+A/585/A150 : On the metallicity of open clusters. III. (Netopil+, 2016) J/AJ/150/134 : uvbyCaHβ photometry of NGC 752 (Twarog+, 2015) J/AJ/148/51 : WIYN Open Cluster. LXI. NGC 6819 (Anthony-Twarog+, 2014) J/MNRAS/419/1350 : Red giants abundances in 4 open clusters (Reddy+, 2012) J/AJ/139/2034 : NGC 6253 stars equivalent widths (Anthony-Twarog+, 2010) J/A+A/485/303 : RVs for 1309 stars and 166 OCl (Mermilliod+, 2008) J/A+A/465/965 : BI light curve of NGC 2506 variables (Arentoft+, 2007) J/AJ/131/461 : Stromgren photometry of NGC 2420 (Anthony-Twarog+, 2006) J/A+A/438/1163 : Catalogue of Open Cluster Data (COCD) (Kharchenko+, 2005) J/AJ/129/872 : Stromgren photometry of NGC 2243 (Anthony-Twarog+, 2005) J/AJ/127/1000 : Stromgren photometry of NGC 3680 (Anthony-Twarog+, 2004) J/AJ/125/1383 : Stromgren photometry of NGC 6253 (Anthony-Twarog+, 2003) J/AJ/119/2282 : Stromgren photometry of IC 4651 (Anthony-Twarog+, 2000) J/AJ/109/2828 : CaII H and K filter photometry II. (Twarog+ 1995) http://webda.physics.muni.cz/ : WEBDA database Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 8 F7.2 pix Xpos [-552.35/656.22] WEBDA X pixel coordinate 10- 16 F7.2 pix Ypos [-615.61/637.53] WEBDA Y pixel coordinate 18- 27 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 29- 38 F10.6 deg DEdeg Declination in decimal degrees (J2000) 40- 43 I4 --- WEBDA [1101/5387]? WEBDA identification number 45- 48 F4.2 --- Mm [0/1]? Membership probability (1) 50- 55 F6.3 mag Vmag [10.76/18] The V-band magnitude 57- 62 F6.3 mag b-y [0.013/1.221] The Stromgren (b-y) color index 64- 69 F6.3 mag m1 [-0.165/0.867]?=9.999 The Stromgren metallicity index m1=(v-b)-(b-y) 71- 76 F6.3 mag c1 [-0.177/1.21]?=9.999 The Stromgren discontinuity index c1=(u-v)-(v-b) 78- 83 F6.3 mag hk [-0.053/1.937]?=9.999 The Stromgren hk index 85- 90 F6.3 mag Hb [2.37/9.51]?=9.999 The Hβ index 92- 97 F6.3 mag e_Vmag [0/0.092] The 1σ uncertainty in Vmag 99-104 F6.3 mag e_b-y [0.001/0.12] The 1σ uncertainty in b-y 106-111 F6.3 mag e_m1 [0.002/0.29]?=9.999 The 1σ uncertainty in m1 113-118 F6.3 mag e_c1 [0.002/0.4]?=9.999 The 1σ uncertainty in c1 120-125 F6.3 mag e_hk [0.002/0.25]?=9.999 The 1σ uncertainty in hk 127-132 F6.3 mag e_Hb [0.001/0.19]?=9.999 The 1σ uncertainty in Hb 134-135 A2 --- Class Calibration classification (B, BV, D, DV, G, or GV) (2) 137-138 I2 --- Ny [2/23] Number of y filter observations 140-141 I2 --- Nb [2/14] Number of b filter observations 143-144 I2 --- Nv [0/9] Number of v filter observations 146-147 I2 --- Nu [0/14] Number of u filter observations 149-150 I2 --- NCa [0/14] Number of Ca filter observations 152-153 I2 --- Nn [0/8] Number of Hβ narrow filter observations 155-156 I2 --- Nw [0/8] Number of Hβ wide filter observations -------------------------------------------------------------------------------- Note (1): Chiu & Van Altena (1981ApJ...243..827C 1981ApJ...243..827C). Note (2): The classification scheme is defined as follows: B = Blue dwarf; BV = Blue dwarf Variable; G = cool Giant; GV = cool Giant Variable; D = cool Dwarf; DV = cool Dwarf Variable. -------------------------------------------------------------------------------- History: From electronic version of the journal References: von Hippel et al., 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 & Deliyannis, Pap VI 2000ApJ...544..944S 2000ApJ...544..944S Platais et al., Pap VII 2001AJ....122.1486P 2001AJ....122.1486P, Cat. J/AJ/122/1486 Platais et al., Pap VIII 2002AJ....124..601P 2002AJ....124..601P, Cat. J/AJ/124/601 Stassun et al., Pap IX 2002A&A...382..899S 2002A&A...382..899S, Cat. 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(End) Prepared by [AAS]; Sylvain Guehenneux [CDS] 10-Feb-2017
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