J/A+A/429/837    IJKs photometry of late-type stars in NGC 6822   (Cioni+, 2005)
Near-IR observations of NGC 6822: AGB stars, distance, metallicity and
structure.
    Cioni M.-R.L., Habing H.J.
   <Astron. Astrophys. 429, 837 (2005)>
   =2005A&A...429..837C 2005A&A...429..837C
ADC_Keywords: Galaxies, photometry ; Photometry, infrared ; Stars, late-type
Keywords: stars: late-type - stars: distances - galaxies: local group -
          galaxies: abundances - galaxies: photometry - infrared: stars
Abstract:
    Observations in the IJKs wave bands covering the central 20'x20' of
    the Local Group galaxy NGC 6822 have been made with the William
    Herschel Telescope in La Palma. They have allowed us to characterize,
    for the first time in the near-infrared across the whole galaxy, its
    late-type stellar population (i.e. red giant and asymptotic giant
    branch stars) and to derive from the ratio between carbon-rich and
    oxygen-rich asymptotic giant branch stars an indication about spatial
    variations in metallicity. These amount to about 1.56dex, twice of
    what has been previously found within each Magellanic Cloud using the
    same technique. We have calibrated our photometry on the DENIS
    (I-band) and 2MASS (J and Ks bands) data and obtained a distance
    modulus of (m-M)0=23.34(0.12) from the position of the tip of the
    RGB. The large scale distribution of late-type stars suggests that
    either the galaxy is viewed under a high inclination angle or it has a
    non-negligible thickness.
Description:
    Observations were performed with the William Herschel Telescope in La
    Palma during two runs in July 2002. The Isaac Newton Group Red Imaging
    Device was used to observe in the J and Ks band from 20th to 22nd July
    while observations in the I band were obtained using the Prime Focus
    imaging camera on July 14th.
Objects:
    ----------------------------------------------------------
       RA   (2000)   DE      Designation(s)
    ----------------------------------------------------------
    19 44 57.8   -14 48 11   NGC 6822 = IC 4895
    ----------------------------------------------------------
File Summary:
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 FileName   Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe         80        .   This file
table1.dat     64     9375   NGC 6822 catalogue of sources detected in the
                             three wave bands, I, J and Ks
table2.dat     63    16354   NGC 6822 catalogue of sources detected in both
                             J and Ks bands, but not in I band.
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See also:
         B/denis : The DENIS database (DENIS Consortium, 2003)
         II/246  : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)
         II/228  : DENIS Catalogue toward Magellanic Clouds (DCMC) (Cioni+ 2000)
   J/AJ/123/832  : C star population in NGC 6822 (Letarte+, 2002)
   J/AJ/121/2020 : CTIO and WFPC2 photometry in NGC 6822 (Bianchi+, 2001)
   J/AJ/109/173  : BVR photometry of NGC 6822 (Marconi+ 1995)
   J/AJ/110/2715 : UBV photometry in NGC 6822, M31 and M33 (Massey+ 1995)
Byte-by-byte Description of file: table1.dat table2.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 10  F10.6 deg     RAdeg     Right ascension (J2000)
  12- 21  F10.6 deg     DEdeg     Declination (J2000)
  23- 27  F5.2  mag     Imag      ? I magnitude
  29- 32  F4.2  mag   e_Imag      ? Error in I magnitude
  34- 35  I2    ---   f_Imag      ? SExtractor flag in I magnitude (1)
  37- 41  F5.2  mag     Jmag      J magnitude
  43- 46  F4.2  mag   e_Jmag      Error in J magnitude
  48- 49  I2    ---   f_Jmag      [0/2] SExtractor flag in J magnitude (1)
  51- 55  F5.2  mag     Ksmag     Ks magnitude
  57- 60  F4.2  mag   e_Ksmag     Error in Ks magnitude
  62- 63  I2    ---   f_Ksmag     SExtractor flag in Ks magnitude (1)
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Note (1): SExtractor flag is 2 when the object was originally blended 
     with another one.
--------------------------------------------------------------------------------
Acknowledgements:  Maria-Rosa Cioni, mcioni(at)eso.org
(End)                                        Patricia Vannier [CDS]  26-Oct-2004