J/AN/329/418  UBVRcIc photometry in fields of Seyfert galaxies    (Mihov+, 2008)
Johnson-Cousins magnitudes of comparison stars in the fields of ten
Seyfert galaxies.
    Mihov B.M., Slavcheva-Mihova L.S.
   <Astron. Nachrichten, 329, 418-425 (2008)>
   =2008AN....329..418M 2008AN....329..418M
ADC_Keywords: Galaxies, Seyfert ; Stars, standard ; Photometry, UBVRI
Keywords: galaxies: Seyfert - techniques: photometric
Abstract:
    We present UBVRcIc magnitudes of 49 comparison stars in the fields of
    the Seyfert galaxies Mrk 335, Mrk 79, Mrk 279, Mrk 506, 3C 382,
    3C 390.3, NGC 6814, Mrk 304, Ark 564, and NGC 7469 in order to
    facilitate the photometric monitoring of these objects; 36 of the
    stars have not been calibrated before. The comparison stars are
    situated in 5x5arcmin fields centred on the Seyfert galaxies, their V
    band flux ranges from 11.7 to 18.2mag with a median value of 16.3mag,
    and their B-V colour index ranges from 0.4 to 1.6mag with a median
    value of 0.8mag. The median errors of the calibrated UBVRCIC
    magnitudes are 0.08, 0.04, 0.03, 0.04, and 0.06mag, respectively.
    Comparison stars were calibrated for the first time in three of the
    fields (Mrk 506, 3C 382, and Mrk 304). The comparison sequences in the
    other fields were improved in various aspects. Extra stars were
    calibrated in four fields (Mrk 335, Mrk 79, NGC 6814, and NGC 7469)
    most of these stars are fainter and are situated closer to the Seyfert
    galaxies compared to the existing comparison stars. The passband
    coverage of the sequences in five fields (Mrk 335, Mrk 79, Mrk 279,
    NGC 6814, and Ark 564) was complemented with the U band.
Description:
    All observations were done by the authors using the 2-m telescope of
    NAO during the period 1997-2003.
File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table1.dat     89       10   List of selected Seyfert galaxies
table2.dat    114       49   Apparent Johnson-Cousins UBVRcIc magnitudes of
                              the comparison stars
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See also:
  J/other/Ap/48.304 : BVRI of comparison stars in AGN fields (Doroshenko+, 2005)
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units  Label   Explanations
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   1-  8  A8    ---    Gal     Galaxy name (1)
  10- 47  A38   ---    ONames  Other name(s) (1)
  49- 50  I2    h      RAh     Right ascension (J2000) (1)
  52- 53  I2    min    RAm     Right ascension (J2000) (1)
  55- 60  F6.3  s      RAs     Right ascension (J2000) (1)
      62  A1    ---    DE-     Declination sign (J2000) (1)
  63- 64  I2    deg    DEd     Declination (J2000) (1)
  66- 67  I2    arcmin DEm     Declination (J2000) (1)
  69- 73  F5.2  arcsec DEs     Declination (J2000) (1)
  75- 81  F7.5  ---    z       Redshift (1)
  83- 85  F3.1  ---    SyType  Seyfert type (1)
      87  A1    ---    N       Number of different observing nights
      89  I1    ---    n       ? Number of nights used in the internal check for
                                 variability of the newly calibrated stars (2)
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Note (1): Data taken from NED.
Note (2): No n value means that no new comparison stars were added to the
     corresponding fields
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Byte-by-byte Description of file: table2.dat
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   Bytes Format Units   Label   Explanations
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   1-  8  A8    ---     Gal     Galaxy name
      11  A1    ---     Star    [A-G] Star designation (1)
      13  A1    ---     OName1  Other name
  14- 16  A3    ---   r_OName1  Reference for OName1 (2)
  18- 19  A2    ---     OName2  Other name
      20  A1    ---   r_OName2  Reference for OName2 (2)
      22  A1    ---     OName3  Other name
      23  A1    ---   r_OName3  Reference for OName3 (2)
  25- 26  I2    h       RAh     Right ascension (J2000)
  28- 29  I2    min     RAm     Right ascension (J2000)
  31- 36  F6.3  s       RAs     Right ascension (J2000)
      38  A1    ---     DE-     Declination sign (J2000)
  39- 40  I2    deg     DEd     Declination (J2000)
  42- 43  I2    arcmin  DEm     Declination (J2000)
  45- 49  F5.2  arcsec  DEs     Declination (J2000)
  51- 55  F5.2  mag     Umag    ?=- Johnson U magnitude
  57- 60  F4.2  mag   e_Umag    ?=- rms uncertainty on Umag
      62  I1    ---   o_Umag    ?=- Number of individual estimates used to
                                    obtain the final U magnitude
  64- 68  F5.2  mag     Bmag    Johnson B magnitude
  70- 73  F4.2  mag   e_Bmag    rms uncertainty on Bmag
      75  I1    ---   o_Bmag    Number of individual estimates used to
                                    obtain the final B magnitude
  77- 81  F5.2  mag     Vmag    Johnson V magnitude
  83- 86  F4.2  mag   e_Vmag    rms uncertainty on Vmag
      88  I1    ---   o_Vmag    Number of individual estimates used to
                                    obtain the final V magnitude
  90- 94  F5.2  mag     Rcmag   ?=- Cousins R magnitude
  96- 99  F4.2  mag   e_Rcmag   ?=- rms uncertainty on Rcmag
     101  I1    ---   o_Rcmag   ?=- Number of individual estimates used to
                                    obtain the final Rc magnitude
 103-107  F5.2  mag     Icmag   ?=- Cousins I magnitude
 109-112  F4.2  mag   e_Icmag   ?=- rms uncertainty on Icmag
     114  I1    ---   o_Icmag   ?=- Number of individual estimates used to
                                    obtain the final Ic magnitude
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Note (1): Stars identified as [MS2008] Gal A in Simbad.
Note (2): References as follows:
      a = Penston et al., 1971PASP...83..783P 1971PASP...83..783P, PPS Gal A in Simbad
      b = Curry et al., 1998, IAPPP Comm. 73, 18, [SRB2001] in Simbad
      c = Bachev et al., 2000A&AS..147..175B 2000A&AS..147..175B, [BSD2000] Gal A in Simbad
      d = Shemmer et al., 2001ApJ...561..162S 2001ApJ...561..162S
      e = Doroshenko et al., 2005Ap.....48..156D 2005Ap.....48..156D
      f = Doroshenko et al., 2005, Cat. J/other/Ap/48.304, 
          [DSM2005] Gal N in Simbad
     The stars without other designations have been calibrated for the
     first time by us.
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History:
    From electronic version of the journal
(End)                                      Patricia Vannier [CDS]    13-Jun-2008