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: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table10.dat 62 89 Transformed photometry table11.dat 22 1288 Photometry in IRAC band 1 -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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) -------------------------------------------------------------------------------- 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. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table11.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 08-Apr-2022
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