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Detailed Description of J/AJ/109/1131

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This standardized document follows the rules of the Standard Description for Astronomical Catalogues. For those having to work on this catalogue using FORTRAN programs, this ReadMe file can be transformed into a f77-compliant program which reads the files making up this catalogue, in two versions: either a f77 program loading whole files into arrays, or a f77-program reading each data file line by line.


J/AJ/109/1131          JHK Photometry in Metal Rich Globulars. (Kuchinski+ 1995)
================================================================================
Infrared Array Photometry of Metal-Rich Globular Clusters.
I. Techniques and First Results
    Kuchinski L.E., Frogel J.A., Terndrup D.M., Persson S.E.
   <Astron. J. 109, 1131 (1995)>
   =1995AJ....109.1131K
================================================================================
ADC_Keywords: Photometry, infrared ; Clusters, globular


Abstract:
    As a first step in investigating the properties of heavily reddened,
    metal-rich globular clusters, we present JHK colors and magnitudes for
    four objects: NGC 5927, NGC 6712, NGC 6838 (M71), and Terzan 2. These
    data begin near the top of the giant branch (GB) and extend to stars
    six magnitudes fainter, reaching below the horizontal branch (HB). We
    use our sample and previously published data for two other clusters,
    47 Tucanae and M69, to develop techniques for deriving basic
    properties such as metallicity and distance modulus from observable
    parameters of cluster color-magnitude diagrams (CMDs) in the near-IR.
    We also analyze the horizontal branches of the clusters in an attempt
    to set constraints on mass loss for first-ascent giants. We find that
    the slope of the linear fit to the GB stars brighter than the HB can
    be used to predict metallicity to an accuracy of ± 0.25 dex for
    clusters with [Fe/H] between -1.0 and -0.3. There appears to be no
    significant dependence on [Fe/H] for other reddening-free indices
    measured from the CMD, including the width of the HB and the
    separation between the GB and HB at the level of the HB. Using the
    clusters in our sample that have known distances, we derive a value of
    <M_K0(HB)> = -1.15 ± 0.10 for the extinction-corrected absolute K
    magnitude of the HB. This provides a means of determining the distance
    to clusters for which only infrared CMDs are available. We derive a
    distance modulus to Terzan 2 of 14.37 ± 0.2 which places it within a
    few hundred parsecs of the galactic center. In the J-H,H-K diagram,
    Terzan 2 giants are located near the Baade's Window giants rather than
    in the region populated by nearly all other globular cluster stars.
    The GB of stars in the field around Terzan 2 has a slope that implies
    [Fe/H] = +0.1, comparable to that in Baade's Window.
Objects:
    -----------------------------------------------------------------------
      RA  (2000)  DE    Designation(s)
    -----------------------------------------------------------------------
    15 27 41  -50 39.5  C 1524-505 = NGC 5927
    17 27 33  -30 48.1  C 1724-307 = Terzan 2 = Haute-Provence 3 = VDBH 228
    18 53.0   -08 43    C 1850-087 = NGC 6712
    19 53.7   +18 47    C 1951+186 = NGC 6838 = M 71
    -----------------------------------------------------------------------

File Summary:

FileName Lrecl Records Explanations
× ReadMe 80 . This file × table3.dat 68 174 NGC 5927 data × table4.dat 74 848 Terzan 2 data × table5.dat 68 161 NGC 6712 data (LCO) × table6.dat 68 312 NGC 6712 data (OSIRIS) × table7.dat 68 326 NGC 6838 (M 71) data
See also: J/AJ/109/1154 : Paper II, JHK Photometry of Liller 1 (Frogel+ 1995) J/AJ/110/2844 : Paper III: JHK Photometry of M 71, NGC 5927, NGC 6624, NGC 6440, NGC 6712 (Kuchinski+ 1995) J/AJ/121/3114 : UBVR photometry of NGC 6712 with VLT (Paltrinieri+, 2001) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 4 I4 --- ID ID number 5- 16 F12.1 pix Xpos X coordinate on frame 17- 28 F12.1 pix Ypos Y coordinate on frame 29- 38 F10.3 mag Kmag Observed K magnitude 39- 47 F9.3 mag J-K Observed J-K color 48- 56 F9.3 mag H-K Observed H-K color 57- 62 A6 --- Code *Code for data set 63- 68 A6 --- Note *Notes
Note on Code: 3 = 3s exposure, 10 = 10s exposure, 20 = 20s exposure Note on Note: NO = DOPHOT error > 0.06 mag, F? = possible field star
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 4 I4 --- ID ID number 5- 16 F12.1 pix Xpos X coordinate on frame 17- 28 F12.1 pix Ypos Y coordinate on frame 29- 38 F10.3 mag Kmag Observed K magnitude 39- 47 F9.3 mag J-K Observed J-K color 48- 56 F9.3 mag H-K Observed H-K color 57- 62 A6 --- Ring *Ring designation 63- 68 A6 --- Code *Code for data set 69- 74 A6 --- Note Notes, NO = DoPHOT error > 0.06 mag
Note on Ring: Cluster Center at x=75, y=40 (pixels), scale = 0.52 arcsec/pixel I = R < 75 pixels (39 arcsec) from cluster center II = 75 pixels (39 arcsec) < R < 110 pixels (57.2 arcsec) III = 110 pixels (57.2 arcsec) < R < 150 pixels (78 arcsec) IV = R > 150 pixels (78 arcsec) Note on Code: 3 = 3sec exposure, 10 = 10sec exposure, 20 = 20sec exposure A3 = 3sec good seeing exposure, AL = good seeing, long exposure
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 4 I4 --- ID ID number 5- 16 F12.1 pix Xpos X coordinate on frame 17- 28 F12.1 pix Ypos Y coordinate on frame 29- 38 F10.3 mag Kmag Observed K magnitude 39- 47 F9.3 mag J-K Observed J-K color 48- 56 F9.3 mag H-K Observed H-K color 57- 62 A6 --- Code *Code for data set 63- 68 A6 --- Note Notes, NO = DoPHOT error > 0.06 mag
Note on Code: A3 = 3sec "A" frame data, AL = long exposure "A" data
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 4 I4 --- ID ID number 5- 16 F12.1 pix Xpos X coordinate on frame 17- 28 F12.1 pix Ypos Y coordinate on frame 29- 38 F10.3 mag Kmag Observed K magnitude 39- 47 F9.3 mag J-K Observed J-K color 48- 56 F9.3 mag H-K Observed H-K color 57- 62 A6 --- Ring *Ring designation 63- 68 A6 --- Note Notes, NO = DoPHOT error > 0.06 mag
Note on Ring: Cluster Center at x=135, y=130 (pixels), scale = 1.55 arcsec/pixel I = R < 60 pixels (93 arcsec) from cluster center II = R > 60 pixels (93 arcsec)
Byte-by-byte Description of file: table7.dat
Bytes Format Units Label Explanations
1- 4 I4 --- ID ID number 5- 16 F12.1 pix Xpos X coordinate on frame 17- 28 F12.1 pix Ypos Y coordinate on frame 29- 38 F10.3 mag Kmag Observed K magnitude 39- 47 F9.3 mag J-K Observed J-K color 48- 56 F9.3 mag H-K Observed H-K color 57- 62 A6 --- Ring *Ring designation 63- 68 A6 --- Note Notes, NO = DoPHOT error > 0.06 mag
Note on Ring: Cluster Center at x=125, y=130 (pixels), scale = 1.55 arcsec/pixel I = R < 90 pixels (140 arcsec) from cluster center II = R > 90 pixels (140 arcsec)
Author's address: Leslie Kuchinski Origin: AAS CD-ROM series, Volume 4, 1995 Lee Brotzman [ADS] 03-May-1995 ================================================================================ (End) [CDS] 11-Jul-1995

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