J/AJ/161/177 Spitzer IRAC photometry of 36 JWST calibration stars (Krick+, 2021)
Spitzer IRAC photometry of JWST calibration stars.
    Krick J.E., Lowrance P., Carey S., Laine S., Grillmair C., Van Dyk S.D.,
    Glaccum W.J., Ingalls J.G., Rieke G., Hora J.L., Fazio G.G., Gordon K.D.,
    Bohlin R.C.
   <Astron. J., 161, 177-177 (2021)>
   =2021AJ....161..177K 2021AJ....161..177K    (SIMBAD/NED BibCode)
ADC_Keywords: Stars, standard; Photometry, infrared; Spectral types
Keywords: Photometric standard stars; Infrared photometry; Flux calibration
Abstract:
    We present infrared photometry of all 36 potential JWST calibrators
    for which there is archival Spitzer IRAC data. This photometry can
    then be used to inform the stellar models necessary to provide
    absolute calibration for all JWST instruments. We describe in detail
    the steps necessary to measure IRAC photometry from archive retrieval
    to photometric corrections. To validate our photometry, we examine the
    distribution of uncertainties from all detections in all four IRAC
    channels as well as compare the photometry and its uncertainties to
    those from models, ALLWISE, and the literature. Seventy-five percent
    of our detections have standard deviations per star of all
    observations within each channel of less than 3%. The median standard
    deviations are 1.2%, 1.3%, 1.1%, and 1.9% in 3.6-8.0, respectively. We
    find less than 8% standard deviations in differences of our photometry
    with ALLWISE and excellent agreement with literature values (less than
    3% difference), lending credence to our measured fluxes. JWST is
    poised to do groundbreaking science, and accurate calibration and
    cross-calibration with other missions will be part of the
    underpinnings of that science.
Description:
    We use publicly available data from the Spitzer Heritage Archive 5
    (SHA) available on the NASA/IPAC Infrared Science Archive (IRSA).
    The Infrared Array Camera (IRAC) was operational on the Spitzer Space
    Telescope from 2003 to 2020 with four broad mid-infrared bands with
    response covering 3.15-9.25um. The James Webb Space Telescope (JWST)
    is currently scheduled to launch in 2021 and will observe from 0.6 to
    28.3um. This paper provides high-precision IRAC fluxes, where
    available, at 3.6, 4.5, 5.8, and 8.0um (also denoted ch1-ch4,
    respectively).
File Summary:
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 FileName    Lrecl    Records    Explanations
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ReadMe          80          .    This file
table1.dat      74         36   *JWST calibrators observed with Spitzer IRAC
table3.dat      80         36    Measured IRAC fluxes for JWST calibrators
table5.dat      16        391    IRAC channel 1 full array average instrument
                                  response curve
table6.dat      16        401    IRAC channel 2 full array average instrument
                                  response curve
table7.dat      16        311    IRAC channel 3 full array average instrument
                                  response curve
table8.dat      16        311    IRAC channel 4 full array average instrument
                                  response curve
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Note on table1.dat : This list is drawn from the James Webb Space
    Telescope User Documentation on Absolute Flux Calibration,
    https://jwst-docs.stsci.edu/data-processing-and-calibration-files
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See also:
 J/AJ/132/1445 : Standard calibration stars infrared spectra (Engelke+, 2006)
 J/ApJ/790/53  : Photometric data of HD 209458b (Zellem+, 2014)
 J/AJ/150/204  : Spectroscopy of standard stars (Joner+, 2015) 
 http://jwst-docs.stsci.edu/ : JWST User Documentation homepage
 http://irsa.ipac.caltech.edu/ : NASA/IPAC Infrared science archive homepage
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units  Label  Explanations
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   1- 11 A11    ---    Name   Calibrator star name
  13- 14 I2     h      RAh    [0/22] Hour of Right Ascension from SIMBAD (J2000)
  16- 17 I2     min    RAm    Minute of Right Ascension from SIMBAD (J2000)
  19- 23 F5.2   s      RAs    Second of Right Ascension from SIMBAD (J2000)
  25- 25 A1     ---    DE-    [-/+] Sign of the Declination from SIMBAD (J2000)
  26- 27 I2     deg    DEd    Degree of Declination from SIMBAD (J2000)
  29- 30 I2     arcmin DEm    Arcminute of Declination from SIMBAD (J2000)
  32- 35 F4.1   arcsec DEs    Arcsecond of Declination from SIMBAD (J2000)
  37- 41 A5     ---    SpT    Spectral Type
  43- 47 F5.2   mag    Vmag   [4.29/16.7] V-band magnitude
  49- 53 F5.2   mag    Kmag   [4.19/15.5] K-band magnitude
  55- 58 F4.2   mag    AV     [0/0.26]? Extinction, V-band
  60- 74 A15    ---    OName  Other or Alternative names
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Byte-by-byte Description of file: table3.dat
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   Bytes Format Units   Label Explanations
--------------------------------------------------------------------------------
   1- 11 A11    ---     Name  Calibrator star name
  13- 19 F7.2   mJy     F3.6  [0.14/7387]? mean 3.6um flux
  21- 24 F4.2   %     e_F3.6  [0.5/5.3]? Standard deviation for F3.6
  26- 29 I4     ---     NF3.6 [4/7082]? Number of F3.6um measurements
  31- 37 F7.2   mJy     F4.5  [0.11/3659]? mean 4.5um flux
  39- 42 F4.2   %     e_F4.5  [0.7/7.6]? Standard deviation for F4.5
  44- 47 I4     ---     NF4.5 [5/7516]? Number of F4.5um measurements
  49- 54 F6.2   mJy     F5.8  [0.8/970]? mean 5.8um flux
  56- 59 F4.2   %     e_F5.8  [0.3/8.8]? Standard deviation for F5.8
  61- 63 I3     ---     NF5.8 [5/725]? Number of F5.8um measurements
  65- 70 F6.2   mJy     F8.0  [0.45/627]? mean 8.0um flux
  72- 76 F5.2   %     e_F8.0  [0.4/14]? Standard deviation for F8.0
  78- 80 I3     ---     NF8.0 [4/738]? Number of F8.0um measurements
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Byte-by-byte Description of file: table[5678].dat
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   Bytes Format Units Label       Explanations
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   1-  7 F7.5   um      Wave        Wavelength in microns
   9- 16 F8.6   --      Response    Instrument response in electrons/photon (1)
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Note (1): See https://irsa.ipac.caltech.edu/data/SPITZER/docs/irac/
        calibrationfiles/spectralresponse/ for a description of the IRAC
        instrument response curves and the use of these data
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History:
    From electronic version of the journal
(End)                          Prepared by [AAS], Coralie Fix [CDS], 02-Aug-2021