J/A+A/380/478       BVI photometry in NGC 6101               (Marconi+, 2001)
================================================================================
Mass segregation of different populations inside the cluster NGC 6101.
     Marconi G., Andreuzzi G., Pulone L., Cassisi S., Testa V., Buonanno R.
    <Astron. Astrophys. 380, 478 (2001)>
    =2001A&A...380..478M
================================================================================
ADC_Keywords: Clusters, globular ; Photometry, CCD
Keywords: globular clusters: individual (NGC 6101) -
          stars: fundamental parameters - Hertzsprung-Russell diagram -
          stars: abundances - stars: horizontal branch

Description:
    We used HST-WFPC2 and the 1.54 Danish ESO-telescope at La Silla
    (Chile) to obtain photometry for stars located within 200 arcsec from
    the center of the cluster NGC 6101. HST-WFPC2 data for 1 field
    centered on the cluster, have been collected during HST-cycle 6. The
    resulting V, V-I photometry reach a limiting magnitude of V~25.5.
    Ground observations have been collected on July 1995. The resulting
    photometry containing the stars simultaneously detected in the V, B
    and I filters, is characterized by a limiting magnitude of V~22.5.

Objects:
    -----------------------------------------
       RA   (2000)   DE      Designation(s)
    -----------------------------------------
    16 25 48.6   -72 12 06   NGC 6101
    -----------------------------------------

File Summary:
--------------------------------------------------------------------------------
 FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
hst.dat           51    12012   HST V, V-I photometry for NGC 6101
ground.dat        66     8413   Ground V, V-I, B-V photometry for NGC 6101
--------------------------------------------------------------------------------

Byte-by-byte Description of file: hst.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  7  F7.3  pix     xpos      x coordinate (G1)
   9- 15  F7.3  pix     ypos      y coordinate (G1)
  17- 22  F6.3  mag     Vmag      V magnitude (F555W)
  24- 28  F5.3  mag   e_Vmag      V photometric error
  30- 35  F6.3  mag     V-I       V-I colour index (F555W -F814W)
  37- 41  F5.3  mag   e_V-I       V-I photometric error
  43- 51  F9.3  ---     ID        Identification number (G2)
--------------------------------------------------------------------------------

Byte-by-byte Description of file: ground.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  8  F8.3  pix     xpos      x coordinate (G1)
  10- 17  F8.3  pix     ypos      y coordinate (G1)
  19- 24  F6.3  mag     Vmag      V magnitude
  26- 30  F5.3  mag   e_Vmag      V photometric error
  32- 37  F6.3  mag     V-I       V-I colour index
  39- 43  F5.3  mag   e_V-I       V-I photometric error
  45- 50  F6.3  mag     B-V       B-V colour index
  52- 56  F5.3  mag   e_B-V       B-V photometric error
  58- 66  F9.3  ---     ID        Identification number (G2)
-----------------------------------------------------------------------------

Global notes:
Note (G1): 1 pix = 0.37".
Note (G2): IDs in HST-table have been created also to indicates the camera
      in which each object has been identified:
       PC: 10000 <= ID < 20000
      WF2: 20000 <= ID < 30000
      WF3: 30000 <= ID < 40000
      WF4: 40000 <= ID < 50000
--------------------------------------------------------------------------------

Acknowledgements: Gloria Andreuzzi <gloria@mporzio.astro.it>
================================================================================
(End)                                        Patricia Bauer [CDS]    12-Dec-2001
