Table A.3.
K corrections for TRGB stars.
| HST/WFC3 | HST/ACS | 2MASS | JWST/NIRCAM | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Teff | log g | [Fe/H] | z | E(B-V) | WH, VI | F555W | F814W | F160W | F606W | F814W | J | Ks | F115W | F150W | F200W | F277W |
| (K) | (cgs) | (mag) | (mmag) | |||||||||||||
| 4200 | 0.5 | -1.75 | 0.005 | 0.000 | -2 | -21 | -7 | -8 | -16 | -8 | -7 | 6 | -6 | -7 | 5 | |
| 4200 | 0.5 | -1.75 | 0.005 | 0.002 | -2 | -15 | -4 | -7 | -11 | -4 | -5 | 7 | -4 | -6 | 5 | 4 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.004 | -2 | -9 | 0 | -6 | -5 | -0 | -4 | 7 | -2 | -5 | 6 | 4 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.006 | -2 | -2 | 4 | -4 | 0 | 3 | -2 | 8 | -0 | -4 | 7 | 5 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.008 | -2 | 4 | 7 | -3 | 6 | 7 | -0 | 9 | 2 | -2 | 8 | 6 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.010 | -2 | 10 | 11 | -2 | 12 | 11 | 2 | 10 | 4 | -1 | 9 | 6 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.015 | -1 | 26 | 20 | 1 | 25 | 20 | 6 | 11 | 9 | 2 | 11 | 8 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.020 | -1 | 42 | 29 | 4 | 39 | 29 | 10 | 13 | 13 | 6 | 13 | 10 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.025 | -1 | 57 | 38 | 7 | 53 | 38 | 15 | 15 | 18 | 9 | 15 | 12 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.030 | -1 | 73 | 47 | 11 | 67 | 47 | 19 | 17 | 23 | 12 | 17 | 13 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.040 | -1 | 104 | 66 | 17 | 94 | 65 | 28 | 21 | 33 | 19 | 22 | 17 |
| 4200 | 0.5 | -1.75 | 0.005 | 0.050 | -1 | 135 | 84 | 23 | 122 | 84 | 37 | 24 | 43 | 25 | 26 | 20 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.000 | -4 | -42 | -15 | -16 | -32 | -15 | -13 | 11 | -12 | -15 | 10 | 6 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.002 | -4 | -36 | -11 | -15 | -27 | -11 | -11 | 12 | -10 | -14 | 10 | 7 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.004 | -3 | -30 | -7 | -14 | -21 | -7 | -9 | 13 | -8 | -13 | 11 | 7 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.006 | -3 | -24 | -4 | -13 | -16 | -4 | -7 | 13 | -6 | -11 | 12 | 8 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.008 | -3 | -18 | -0 | -11 | -10 | -0 | -6 | 14 | -4 | -10 | 13 | 9 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.010 | -3 | -11 | 3 | -10 | -5 | 3 | -4 | 15 | -2 | -9 | 14 | 9 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.015 | -3 | 4 | 12 | -7 | 9 | 12 | 1 | 17 | 3 | -5 | 16 | 11 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.020 | -3 | 20 | 22 | -4 | 23 | 22 | 5 | 18 | 8 | -2 | 18 | 13 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.025 | -3 | 35 | 31 | -1 | 36 | 31 | 9 | 20 | 13 | 1 | 20 | 15 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.030 | -3 | 51 | 40 | 2 | 50 | 40 | 14 | 22 | 18 | 4 | 22 | 16 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.040 | -3 | 82 | 58 | 9 | 77 | 58 | 23 | 26 | 27 | 11 | 27 | 20 |
| 4200 | 0.5 | -1.75 | 0.010 | 0.050 | -3 | 113 | 76 | 15 | 105 | 76 | 31 | 29 | 37 | 17 | 31 | 23 |
| … | ||||||||||||||||
Notes. Extinction-dependent K corrections, Kext(Λ), applicable to stars near the TRGB for the restricted ranges of Teff between 3800 and 4500 K, log g ∈ [0.0, 0.5], [Fe/H] ∈ [ − 2.0, −1.75, −1.5], and E(B-V) between 0.000 and 0.050. Extinction applicable to absolute calibration and the foreground is assumed to be corrected, that is, E(B − V)cal = E(B − V)fg = 0.00 mag. The full version of this table is available via the CDS.
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