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Detailed Description of J/A+AS/119/547
J/A+AS/119/547      IR photometry of ESO calibration stars (van der Bliek+ 1996)
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Infrared aperture photometry at ESO (1983-1994) and its future use.
       Van der Bliek N.S., Manfroid J., Bouchet P.
      <Astron. Astrophys. Suppl. Ser. 119, 547 (1996)>
      =1996A&AS..119..547V      (SIMBAD/NED BibCode)
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ADC_Keywords: Infrared sources ; Photometry, infrared

Keywords: instrumentation: photometers - techniques: photometric -
          infrared: stars

Description:
    We describe the infrared (IR) photometric system for the single
    channel photometers at ESO, which have been used from 1983 until 1994.
    In addition to the broadband near infrared (NIR, 1-5µm) photometric
    system presented in 1991 by Bouchet et al. and Bersanelli et al., we
    describe a narrow-band NIR photometric system and a mid infrared (MIR,
    7-20µm) photometric system. We also extend the set of NIR standard
    stars by Bouchet et al. towards fainter objects (K=~9). The
    photometric data of the standard stars in these systems were extracted
    from the complete IR photometric data archive of ESO, covering 10
    years. The zeropoints of the NIR photometry are set by assuming that
    HR 3314 has a V-magnitude of 3.89, and that V-K=-0.05, J-K=-0.01,
    H-K=-0.01, K-L'=0.00, K-M=0.00. The zeropoints of the MIR photometry
    are set by assuming that the colours of{beta} Hyi (HR 0098) and
    {alpha} CenA (HR 5459) are equal to the colours of the Sun. We adopt
    the absolute calibration of Megessier (1995A&A...296..771M) for the
    NIR and we argue that this calibration can be extrapolated to 20µm,
    using the MIR calibrations by Rieke et al. (1985AJ.....90..900R) and
    Cohen et al. (1992AJ....104.1650C). The definition of the zeropoints
    is consistent with the absolute calibration. We obtained accurate
    ({sigma}=~0.02mag.) NIR photometry of about 240 standard stars and MIR
    photometry of about 40 standard stars ({sigma}=~0.04mag). Comparison
    of our NIR photometric system with other well established systems
    shows that there are some small colour dependencies and zeropoint
    offsets which are always smaller than about 0.02mag. except for the L'
    band.

File Summary:

FileName Lrecl Records Explanations
ReadMe 80 . This file table5 122 253 NIR (JHKL'M) broad band photometry of ESO calibration stars table6 122 113 MIR broad band photometry of ESO calibration stars table7 121 43 MIR photometry of ESO calibration stars
Byte-by-byte Description of file: table5
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star designation 11- 12 I2 h RAh Right Ascension 2000 (hours) 14- 15 I2 min RAm Right Ascension 2000 (minutes) 17- 18 I2 s RAs Right Ascension 2000 (seconds) 20 A1 --- DE- Declination 2000 (sign) 21- 22 I2 deg DEd Declination 2000 (degrees) 24- 25 I2 arcmin DEm Declination 2000 (minutes) 27- 28 I2 arcsec DEs ? Declination 2000 (seconds) 30- 37 A8 --- Sp Spectral Type & Luminosity Class 39- 44 F6.3 mag Jmag J magnitude (1.24 microns) 46- 50 F5.3 mag e_Jmag Standard deviation of Jmag 52- 54 I3 --- o_Jmag Number of observations in Jmag 56- 61 F6.3 mag Hmag H magnitude (1.63 microns) 63- 67 F5.3 mag e_Hmag Standard deviation of Hmag 69- 71 I3 --- o_Hmag Number of observations in Hmag 73- 78 F6.3 mag Kmag K magnitude (2.19 microns) 80- 84 F5.3 mag e_Kmag Standard deviation of Kmag 86- 88 I3 --- o_Kmag Number of observations in Kmag 90- 95 F6.3 mag L'mag ? L' magnitude (3.79 microns) 97-101 F5.3 mag e_L'mag ? Standard deviation of L'mag 103-105 I3 --- o_L'mag ? Number of observations in L'mag 107-112 F6.3 mag Mmag ? M magnitude (4.64 microns) 114-118 F5.3 mag e_Mmag ? Standard deviation of Mmag 120-122 I3 --- o_Mmag ? Number of observations in Mmag
Byte-by-byte Description of file: table6
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star designation 11- 12 I2 h RAh Right Ascension 2000 (hours) 14- 15 I2 min RAm Right Ascension 2000 (minutes) 17- 18 I2 s RAs Right Ascension 2000 (seconds) 20 A1 --- DE- Declination 2000 (sign) 21- 22 I2 deg DEd Declination 2000 (degrees) 24- 25 I2 arcmin DEm Declination 2000 (minutes) 27- 28 I2 arcsec DEs ? Declination 2000 (seconds) 30- 37 A8 --- Sp Spectral Type & Luminosity Class 39- 44 F6.3 mag H0 H_0 magnitude (1.58 microns) 46- 50 F5.3 mag e_H0 Standard deviation of H_0 52- 54 I3 --- o_H0 Number of observations in H_0 56- 61 F6.3 mag BrGamma Br_gamma magnitude (2.16 microns) 63- 67 F5.3 mag e_BrGamma Standard deviation of Br_gamma 69- 71 I3 --- o_BrGamma Number of observations in Br_gamma 73- 78 F6.3 mag K0 K_0 magnitude (2.22 microns) 80- 84 F5.3 mag e_K0 Standard deviation of K_0 86- 88 I3 --- o_K0 Number of observations in K_0 90- 95 F6.3 mag CO ? CO magnitude (2.29 microns) 97-101 F5.3 mag e_CO ? Standard deviation of CO 103-105 I3 --- o_CO ? Number of observations in CO 107-112 F6.3 mag L0 ? L_0 magnitude (3.70 microns) 114-118 F5.3 mag e_L0 ? Standard deviation of L_0 120-122 I3 --- o_L0 ? Number of observations in L_0
Byte-by-byte Description of file: table7
Bytes Format Units Label Explanations
1- 8 A8 --- Name Star designation 10- 11 I2 h RAh Right Ascension 2000 (hours) 13- 14 I2 min RAm Right Ascension 2000 (minutes) 16- 17 I2 s RAs Right Ascension 2000 (seconds) 19 A1 --- DE- Declination 2000 (sign) 20- 21 I2 deg DEd Declination 2000 (degrees) 23- 24 I2 arcmin DEm Declination 2000 (minutes) 26- 27 I2 arcsec DEs Declination 2000 (seconds) 29- 36 A8 --- Sp Spectral Type & Luminosity Class 38- 43 F6.3 mag Nmag ? N magnitude (10.36 microns) 45- 49 F5.3 mag e_Nmag ? Standard deviation of Nmag 51- 53 I3 --- o_Nmag ? Number of observations in Nmag 55- 60 F6.3 mag N1 N1 magnitude (8.38 microns) 62- 66 F5.3 mag e_N1 Standard deviation of N1 68- 70 I3 --- o_N1 Number of observations in N1 72- 77 F6.3 mag N2 N2 magnitude (9.69 microns) 79- 83 F5.3 mag e_N2 Standard deviation of N2 85- 87 I3 --- o_N2 Number of observations in N2 89- 94 F6.3 mag N3 N3 magnitude (12.89 microns) 96-100 F5.3 mag e_N3 Standard deviation of N3 102-104 I3 --- o_N3 Number of observations in N3 106-111 F6.3 mag Q0 ? Q0 magnitude (18.06 microns) 113-117 F5.3 mag e_Q0 ? Standard deviation of Q0 119-121 I3 --- o_Q0 ? Number of observations in Q0
Acknowledgements: Nicole van der Bliek ================================================================================ (End) Patricia Bauer [CDS] 02-Apr-1996
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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