J/AJ/163/45  Infrared absolute calibration. I. Calibration stars  (Rieke+, 2022)
Infrared Absolute Calibration.
I. Comparison of Sirius with Fainter Calibration Stars.
    Rieke G.H., Su K., Sloan G.C., Schlawin E.
   <Astron. J., 163, 45 (2022)>
   =2022AJ....163...45R 2022AJ....163...45R
ADC_Keywords: Stars, standard; Photometry, infrared
Keywords: Fundamental parameters of stars
Abstract:
    A challenge in absolute calibration is to relate very bright stars
    with physical flux measurements to faint ones within range of modern
    instruments, e.g., those on large ground-based telescopes or the James
    Webb Space Telescope (JWST). We propose Sirius as the fiducial color
    standard. It is an A0V star that is slowly rotating and does not have
    infrared excesses due to either hot dust or a planetary debris disk;
    it also has a number of accurate (∼1%-2%) absolute flux measurements.
    We accurately transfer the near-infrared flux from Sirius to
    BD+601753, an unobscured early A-type star (A1V, V∼9.6, E(B-V)∼0.009)
    that is faint enough to serve as a primary absolute flux calibrator
    for JWST. Its near-infrared spectral energy distribution and that of
    Sirius should be virtually identical. We have determined its output
    relative to that of Sirius in a number of different ways, all of which
    give consistent results within ∼1%. We also transfer the calibration
    to GSPC P330-E, a well-calibrated close solar analog (G2V). We have
    emphasized the 2MASS Ks band, since it represents a large number and
    long history of measurements, but the theoretical spectra (i.e., from
    CALSPEC) of these stars can be used to extend this result throughout
    the near- and mid-infrared.
Description:
    To determine the intrinsic color difference between Ks and IRAC Band
    1, we used the observations obtained in Spitzer PID70076. We focus on
    Band 1 to avoid the effects of the strong CO absorption in Band 2 for
    stars later than mid-F type. The data were processed by the Spitzer
    Science Center (SSC) with the final IRAC pipeline. We used the basic
    calibrated data (BCD) images, which have a native scale of
    1.22"/pixel.
File Summary:
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 FileName   Lrecl  Records  Explanations
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ReadMe         80        .  This file
table10.dat    62       89  Transformed photometry
table11.dat    22     1288  Photometry in IRAC band 1
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See also:
 II/246  : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)
 VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)
 III/260 : General Catalogue of Ap and Am stars (Renson+ 2009)
 IV/38   : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)
 II/365  : CatWISE2020 catalog (updated version 28-Jan-2021) (Marocco+, 2020)
 J/ApJ/761/16 : IR colors of the Sun from Line-Depth Ratios (Casagrande+, 2012)
 J/MNRAS/427/343 : Infrared excesses of Hipparcos stars (McDonald+, 2012)
 J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)
 J/MNRAS/440/3430 : SDSS-2MASS-WISE stellar colour locus (Davenport+, 2014)
 J/AJ/149/11  : Spectra of candidate standard stars in mid-IR (Sloan+, 2015)
 J/AJ/161/177 : Spitzer IRAC photometry 36 JWST calibration stars (Krick+, 2021)
Byte-by-byte Description of file: table10.dat
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 Bytes Format Units  Label   Explanations
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  1-  8 A8     ---   Star    Stellar identifier
 10- 14 F5.3   mag   Vmag    [2.89/6.89] Apparent V band Vega magnitude
 16- 21 F6.3   Jy    Flux    [1.02/17.2] Spitzer/IRAC 3.6um flux density
 23- 27 F5.3   mag   Jmag    [2.96/6.19] 2MASS J-band magnitude
 29- 33 F5.3   mag   Hmag    [0/6.17]? 2MASS H-band magnitude
 35- 39 F5.3   mag   Ksmag   [3.02/6.14] 2MASS Ks-band magnitude
 41- 50 A10    ---   Ref     Reference codes (1)
 52- 56 F5.3   mag   3.6mag  [3.01/6.09] Spitzer/IRAC 3.6um magnitude (2)
 58- 62 F5.3   ---   KsmagT  [3.02/6.14] Transformed Ks magnitude based only
                              on heritage photometry (3)
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Note (1): References as follows:
    1 = 2MASS, Cutri+, 2003, II/246
    2 = Su & Rieke, unpublished
    3 = Allen & Cragg, 1983MNRAS.203..777A 1983MNRAS.203..777A
    4 = Bouchet+, 1991A&AS...91..409B 1991A&AS...91..409B
    5 = Alonso+, 1998, J/A+AS/131/209
    6 = Kidger & Martin-Luis, 2003, J/AJ/125/3311
    7 = Aumann & Probst, 1991AJ....368..264A 1991AJ....368..264A
    8 = Carter+, 1990MNRAS.242....1A 1990MNRAS.242....1A
    9 = Glass+, 1974MNSSA..33...71G 1974MNSSA..33...71G
   10 = McGregor+, 1994PASP..106..508M 1994PASP..106..508M
   11 = Johnson+, 1966, II/5
   12 = Groote & Kaufmann, 1983A&AS...53...91G 1983A&AS...53...91G
Note (2): Zero point taken to be 276.5Jy to force zero color for V-Ks=0.
Note (3): The JHK magnitudes in the previous columns include 2MASS photometry
          as well as the transformed heritage photometry whenever unsaturated
          2MASS photometry is available.
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Byte-by-byte Description of file: table11.dat
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 Bytes  Format Units Label Explanations
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  1-  9 A9     ---   Star  Stellar identifier
 11- 16 F6.3   Jy    Flux  [0.16/18.7] Spitzer/IRAC 3.6micron band flux density
 18- 22 F5.3   Jy  e_Flux  [0.003/0.7] Uncertainty in Flux
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History:
    From electronic version of the journal
(End)                          Prepared by [AAS], Coralie Fix [CDS], 08-Apr-2022