10.3 Throughputs and Correction Tables
10.3.1 Filter Throughputs and Sensitivities
- WFC F435W
- WFC F475W
- WFC F502N
- WFC F550M
- WFC F555W
- WFC F606W
- WFC F625W
- WFC F658N
- WFC F660N
- WFC F775W
- WFC F814W
- WFC F850LP
- WFC G800L
- WFC CLEAR
- HRC F220W
- HRC F250W
- HRC F330W
- HRC F344N
- HRC F435W
- HRC F475W
- HRC F502N
- HRC F550M
- HRC F555W
- HRC F606W
- HRC F625W
- HRC F658N
- HRC F660N
- HRC F775W
- HRC F814W
- HRC F850LP
- HRC F892N
- HRC G800L
- HRC PR200L
- HRC CLEAR
- SBC F115LP
- SBC F122M
- SBC F125LP
- SBC F140LP
- SBC F150LP
- SBC F165LP
- SBC PR110L
- SBC PR130L
10.3.2 Color Correction Tables
Table 10.1: Color corrections ABV to go from Johnson V magnitude to AB magnitude for the WFC (ACS ISR 2019-10).
Spectrum[a] | F435W | F475W | F502N | F550M | F555W | F606W | F625W |
---|---|---|---|---|---|---|---|
Avg Sky | 0.61 | 0.34 | 0.21 | -0.04 | 0.05 | -0.11 | -0.23 |
Low Sky | 0.60 | 0.33 | 0.20 | -0.04 | 0.05 | -0.10 | -0.22 |
O5V | -0.43 | -0.28 | -0.15 | 0.07 | -0.03 | 0.13 | 0.29 |
B0V | -0.39 | -0.25 | -0.13 | 0.06 | -0.03 | 0.13 | 0.28 |
A0V | -0.10 | -0.09 | -0.07 | 0.03 | 0.00 | 0.09 | 0.17 |
A5V | 0.03 | -0.01 | -0.03 | 0.02 | 0.01 | 0.07 | 0.11 |
F2V | 0.25 | 0.12 | 0.06 | -0.01 | 0.02 | 0.01 | -0.02 |
G2V | 0.59 | 0.31 | 0.17 | -0.04 | 0.04 | -0.07 | -0.16 |
K0V | 0.76 | 0.40 | 0.23 | -0.06 | 0.05 | -0.12 | -0.24 |
M0V | 1.17 | 0.69 | 0.87 | -0.18 | 0.11 | -0.32 | -0.56 |
M6V | 1.19 | 0.71 | 0.98 | -0.19 | 0.13 | -0.35 | -0.60 |
O6I | -0.42 | -0.27 | -0.15 | 0.07 | -0.03 | 0.13 | 0.28 |
B0I | -0.35 | -0.22 | -0.12 | 0.05 | -0.03 | 0.12 | 0.25 |
G0III | 0.58 | 0.30 | 0.17 | -0.03 | 0.04 | -0.07 | -0.16 |
K0III | 1.05 | 0.54 | 0.31 | -0.07 | 0.06 | -0.16 | -0.32 |
M0III | 1.50 | 0.82 | 0.79 | -0.16 | 0.11 | -0.33 | -0.58 |
Elliptical | 0.82 | 0.44 | 0.26 | -0.05 | 0.06 | -0.18 | -0.34 |
Sa | 0.76 | 0.43 | 0.28 | -0.06 | 0.07 | -0.15 | -0.30 |
Sbc | 0.58 | 0.34 | 0.18 | -0.04 | 0.05 | -0.13 | -0.26 |
Scd | 0.48 | 0.26 | 0.03 | -0.02 | 0.04 | -0.10 | -0.20 |
Starburst E(B–V) = 0.51–0.60 | 0.42 | 0.25 | -0.01 | -0.01 | 0.04 | -0.24 | -0.41 |
Starburst E(B–V) < 0.1 | 0.23 | 0.06 | -1.02 | 0.11 | -0.03 | -0.11 | -0.14 |
Sun | 0.57 | 0.30 | 0.17 | -0.04 | 0.04 | -0.07 | -0.17 |
Vega | -0.10 | -0.09 | -0.08 | 0.03 | 0.00 | 0.09 | 0.17 |
Table 10.1 (continued)
Spectrum[a] | F658N | F660N | F775W | F814W | F850LP | F892N | G800L | CLEAR |
---|---|---|---|---|---|---|---|---|
Avg Sky | -0.25 | -0.28 | -0.40 | -0.42 | -0.48 | -0.48 | -0.36 | -0.06 |
Low Sky | -0.24 | -0.26 | -0.38 | -0.40 | -0.44 | -0.45 | -0.33 | -0.05 |
O5V | 0.40 | 0.39 | 0.68 | 0.76 | 1.01 | 0.98 | 0.56 | 0.06 |
B0V | 0.41 | 0.39 | 0.66 | 0.74 | 0.98 | 0.96 | 0.55 | 0.08 |
A0V | 0.38 | 0.30 | 0.40 | 0.44 | 0.54 | 0.51 | 0.33 | 0.16 |
A5V | 0.31 | 0.22 | 0.27 | 0.30 | 0.39 | 0.37 | 0.23 | 0.15 |
F2V | 0.08 | 0.02 | 0.02 | 0.04 | 0.09 | 0.08 | 0.02 | 0.10 |
G2V | -0.17 | -0.20 | -0.26 | -0.27 | -0.28 | -0.29 | -0.23 | 0.02 |
K0V | -0.28 | -0.30 | -0.40 | -0.42 | -0.46 | -0.47 | -0.36 | -0.04 |
M0V | -0.82 | -0.83 | -1.33 | -1.45 | -1.72 | -1.66 | -1.19 | -0.63 |
M6V | -0.93 | -0.94 | -1.57 | -1.72 | -2.04 | -1.95 | -1.41 | -0.81 |
O6I | 0.39 | 0.38 | 0.67 | 0.74 | 0.99 | 0.97 | 0.55 | 0.06 |
B0I | 0.36 | 0.35 | 0.61 | 0.68 | 0.91 | 0.89 | 0.51 | 0.08 |
G0III | -0.16 | -0.19 | -0.25 | -0.25 | -0.27 | -0.28 | -0.22 | 0.02 |
K0III | -0.39 | -0.40 | -0.55 | -0.58 | -0.67 | -0.70 | -0.50 | -0.10 |
M0III | -0.81 | -0.82 | -1.28 | -1.39 | -1.65 | -1.63 | -1.15 | -0.58 |
Elliptical | -0.45 | -0.46 | -0.69 | -0.75 | -0.90 | -0.91 | -0.61 | -0.21 |
Sa | -0.45 | -0.42 | -0.57 | -0.62 | -0.76 | -0.78 | -0.52 | -0.15 |
Sbc | -0.34 | -0.34 | -0.55 | -0.60 | -0.75 | -0.72 | -0.49 | -0.15 |
Scd | -0.26 | -0.27 | -0.38 | -0.40 | -0.45 | -0.43 | -0.33 | -0.07 |
Starburst E(B–V) = 0.51–0.60 | -1.50 | -0.99 | -0.50 | -0.52 | -0.60 | -0.59 | -0.50 | -0.20 |
Starburst E(B–V) < 0.1 | -1.20 | -0.36 | -0.14 | -0.17 | -0.25 | -0.20 | -0.17 | -0.04 |
Sun | -0.17 | -0.20 | -0.27 | -0.27 | -0.28 | -0.29 | -0.24 | 0.01 |
Vega | 0.38 | 0.29 | 0.39 | 0.43 | 0.53 | 0.50 | 0.32 | 0.15 |
aCastelli & Kurucz models are used for the stellar spectra.
Table 10.2: Color corrections ABV to go from Johnson V magnitude to AB magnitude for the HRC (ACS ISR 2019-10).
Spectrum[a] | F220W | F250W | F330W | F344N | F435W | F475W | F502N | F550M | F555W | F606W |
---|---|---|---|---|---|---|---|---|---|---|
Avg Sky | 2.19 | 1.42 | 2.01 | 1.89 | 0.63 | 0.32 | 0.21 | -0.04 | 0.05 | -0.10 |
Low Sky | 5.46 | 3.73 | 2.09 | 1.97 | 0.62 | 0.31 | 0.20 | -0.04 | 0.05 | -0.09 |
O5V | -1.46 | -1.20 | -0.83 | -0.79 | -0.43 | -0.27 | -0.15 | 0.07 | -0.03 | 0.12 |
B0V | -1.23 | -1.00 | -0.67 | -0.64 | -0.39 | -0.24 | -0.13 | 0.06 | -0.03 | 0.12 |
A0V | 1.77 | 1.55 | 1.15 | 1.11 | -0.09 | -0.09 | -0.07 | 0.03 | 0.00 | 0.09 |
A5V | 2.44 | 2.05 | 1.40 | 1.36 | 0.05 | -0.01 | -0.03 | 0.02 | 0.01 | 0.06 |
F2V | 3.38 | 2.49 | 1.46 | 1.40 | 0.26 | 0.12 | 0.06 | -0.01 | 0.02 | 0.01 |
G2V | 5.56 | 3.46 | 1.87 | 1.83 | 0.61 | 0.29 | 0.17 | -0.04 | 0.04 | -0.07 |
K0V | 6.88 | 4.23 | 2.33 | 2.35 | 0.79 | 0.38 | 0.23 | -0.06 | 0.05 | -0.11 |
M0V | 8.24 | 6.96 | 3.81 | 3.79 | 1.19 | 0.66 | 0.87 | -0.17 | 0.12 | -0.29 |
M6V | 8.05 | 6.88 | 3.74 | 3.69 | 1.21 | 0.68 | 0.98 | -0.19 | 0.13 | -0.32 |
O6I | -1.41 | -1.16 | -0.81 | -0.77 | -0.42 | -0.26 | -0.15 | 0.07 | -0.03 | 0.12 |
B0I | -1.05 | -0.89 | -0.64 | -0.61 | -0.36 | -0.22 | -0.12 | 0.05 | -0.03 | 0.11 |
G0III | 5.77 | 3.67 | 2.04 | 1.95 | 0.60 | 0.29 | 0.17 | -0.03 | 0.04 | -0.06 |
K0III | 8.24 | 5.60 | 3.22 | 3.14 | 1.08 | 0.51 | 0.31 | -0.07 | 0.07 | -0.15 |
M0III | 8.43 | 8.10 | 5.11 | 5.12 | 1.53 | 0.78 | 0.79 | -0.16 | 0.12 | -0.31 |
Elliptical | 5.22 | 3.83 | 2.33 | 2.25 | 0.84 | 0.42 | 0.26 | -0.05 | 0.06 | -0.17 |
Sa | 4.58 | 3.68 | 2.38 | 2.31 | 0.79 | 0.41 | 0.28 | -0.06 | 0.07 | -0.13 |
Sbc | 2.99 | 2.64 | 1.88 | 1.78 | 0.60 | 0.32 | 0.18 | -0.04 | 0.05 | -0.12 |
Scd | 2.09 | 1.89 | 1.44 | 1.39 | 0.49 | 0.25 | 0.03 | -0.02 | 0.04 | -0.09 |
Starburst E(B–V) = 0.51–0.60 | 1.53 | 1.35 | 1.05 | 1.09 | 0.43 | 0.24 | -0.01 | 0.00 | 0.04 | -0.22 |
Starburst E(B–V) < 0.1 | 1.10 | 0.97 | 0.79 | 0.80 | 0.24 | 0.05 | -1.02 | 0.11 | -0.03 | -0.10 |
Sun | 5.67 | 3.55 | 1.84 | 1.73 | 0.59 | 0.29 | 0.17 | -0.04 | 0.05 | -0.07 |
Vega | 1.68 | 1.49 | 1.18 | 1.15 | -0.08 | -0.09 | -0.08 | 0.03 | 0.00 | 0.09 |
Table 10.2 (continued)
Spectrum[a] | F625W | F658N | F660N | F775W | F814W | F850LP | F892N | G800L | PR200L | CLEAR |
---|---|---|---|---|---|---|---|---|---|---|
Avg Sky | -0.22 | -0.25 | -0.28 | -0.40 | -0.43 | -0.48 | -0.48 | -0.35 | 0.19 | 0.26 |
Low Sky | -0.21 | -0.24 | -0.26 | -0.38 | -0.40 | -0.45 | -0.45 | -0.33 | 0.23 | 0.31 |
O5V | 0.29 | 0.40 | 0.38 | 0.67 | 0.77 | 1.03 | 0.98 | 0.56 | -0.41 | -0.53 |
B0V | 0.27 | 0.41 | 0.39 | 0.66 | 0.75 | 1.00 | 0.96 | 0.55 | -0.30 | -0.40 |
A0V | 0.17 | 0.38 | 0.30 | 0.40 | 0.44 | 0.54 | 0.51 | 0.33 | 0.34 | 0.40 |
A5V | 0.11 | 0.31 | 0.22 | 0.27 | 0.31 | 0.39 | 0.37 | 0.23 | 0.37 | 0.44 |
F2V | -0.02 | 0.08 | 0.02 | 0.02 | 0.04 | 0.09 | 0.08 | 0.02 | 0.34 | 0.41 |
G2V | -0.16 | -0.17 | -0.20 | -0.26 | -0.27 | -0.28 | -0.29 | -0.23 | 0.28 | 0.36 |
K0V | -0.24 | -0.28 | -0.30 | -0.40 | -0.42 | -0.46 | -0.47 | -0.35 | 0.24 | 0.32 |
M0V | -0.55 | -0.82 | -0.83 | -1.32 | -1.47 | -1.74 | -1.66 | -1.19 | -0.33 | -0.24 |
M6V | -0.58 | -0.93 | -0.94 | -1.55 | -1.74 | -2.07 | -1.94 | -1.42 | -0.51 | -0.43 |
O6I | 0.28 | 0.38 | 0.38 | 0.66 | 0.76 | 1.01 | 0.97 | 0.55 | -0.39 | -0.51 |
B0I | 0.25 | 0.36 | 0.35 | 0.61 | 0.70 | 0.93 | 0.89 | 0.51 | -0.24 | -0.32 |
G0III | -0.15 | -0.16 | -0.19 | -0.25 | -0.26 | -0.27 | -0.28 | -0.22 | 0.29 | 0.37 |
K0III | -0.32 | -0.39 | -0.40 | -0.55 | -0.59 | -0.68 | -0.70 | -0.50 | 0.18 | 0.27 |
M0III | -0.57 | -0.81 | -0.82 | -1.26 | -1.41 | -1.68 | -1.63 | -1.16 | -0.28 | -0.20 |
Elliptical | -0.33 | -0.45 | -0.46 | -0.68 | -0.76 | -0.91 | -0.91 | -0.62 | 0.07 | 0.15 |
Sa | -0.29 | -0.45 | -0.42 | -0.56 | -0.63 | -0.78 | -0.78 | -0.52 | 0.13 | 0.21 |
Sbc | -0.25 | -0.34 | -0.34 | -0.54 | -0.61 | -0.77 | -0.72 | -0.49 | 0.11 | 0.18 |
Scd | -0.20 | -0.26 | -0.27 | -0.38 | -0.40 | -0.45 | -0.43 | -0.33 | 0.16 | 0.23 |
Starburst E(B–V) = 0.51–0.60 | -0.41 | -1.50 | -1.00 | -0.50 | -0.53 | -0.61 | -0.59 | -0.50 | 0.02 | 0.08 |
Starburst E(B–V) < 0.1 | -0.13 | -1.20 | -0.36 | -0.14 | -0.18 | -0.27 | -0.20 | -0.18 | 0.12 | 0.17 |
Sun | -0.17 | -0.17 | -0.20 | -0.27 | -0.27 | -0.28 | -0.29 | -0.23 | 0.28 | 0.36 |
Vega | 0.17 | 0.38 | 0.29 | 0.39 | 0.43 | 0.53 | 0.49 | 0.32 | 0.34 | 0.40 |
aCastelli & Kurucz models are used for the stellar spectra.
Table 10.3: Color corrections ABV to go from Johnson V magnitude to AB magnitude for the SBC (ACS ISR 2019-10).
Spectrum[a] | F115LP | F122M | F125LP | F140LP | F150LP | F165LP | PR110l | PR130L |
---|---|---|---|---|---|---|---|---|
Avg Sky | -2.67 | -3.69 | -0.29 | 4.31 | 9.03 | 7.56 | -2.12 | -0.26 |
Low Sky | -1.20 | -2.29 | 4.02 | 8.51 | 10.34 | 8.90 | -0.59 | 4.04 |
O5V | -1.95 | -2.00 | -1.95 | -1.87 | -1.81 | -1.74 | -1.94 | -1.94 |
B0V | -1.55 | -1.55 | -1.56 | -1.48 | -1.42 | -1.41 | -1.54 | -1.56 |
A0V | 3.33 | 4.70 | 3.13 | 2.70 | 2.40 | 2.05 | 3.11 | 3.07 |
A5V | 5.97 | 8.22 | 5.78 | 5.14 | 4.47 | 3.23 | 5.59 | 5.58 |
F2V | 8.37 | 10.81 | 8.17 | 7.53 | 6.85 | 5.42 | 7.94 | 7.93 |
G2V[b] | 12.19 | 16.36 | 11.98 | 11.33 | 10.67 | 9.20 | 11.56 | 11.56 |
K0V[b] | 12.91 | 18.58 | 12.70 | 12.05 | 11.39 | 9.91 | 12.26 | 12.26 |
M0V[b] | 14.07 | 25.89 | 13.86 | 13.21 | 12.55 | 11.07 | 13.40 | 13.40 |
M6V[b] | 14.04 | 28.31 | 13.83 | 13.17 | 12.52 | 11.04 | 13.37 | 13.37 |
O6I | -1.82 | -1.86 | -1.81 | -1.75 | -1.70 | -1.66 | -1.81 | -1.81 |
B0I | -1.09 | -1.05 | -1.11 | -1.07 | -1.06 | -1.10 | -1.09 | -1.11 |
G0III[b] | 12.32 | 16.51 | 12.11 | 11.46 | 10.80 | 9.33 | 11.69 | 11.69 |
K0III[b] | 13.74 | 23.50 | 13.53 | 12.87 | 12.22 | 10.74 | 13.07 | 13.07 |
M0III[b] | 14.63 | 30.34 | 14.42 | 13.77 | 13.11 | 11.63 | 13.97 | 13.97 |
Elliptical | 6.66 | 6.80 | 6.62 | 6.54 | 6.48 | 6.33 | 6.62 | 6.60 |
Sa | 5.73 | 5.88 | 5.69 | 5.59 | 5.43 | 5.22 | 5.68 | 5.67 |
Sbc | 4.22 | 4.57 | 4.14 | 3.93 | 3.74 | 3.45 | 4.13 | 4.11 |
Scd | 2.90 | 3.14 | 2.84 | 2.68 | 2.54 | 2.33 | 2.83 | 2.82 |
Starburst E(B–V) = 0.51–0.60 | 2.35 | 2.52 | 2.31 | 2.18 | 2.09 | 1.89 | 2.30 | 2.29 |
Starburst E(B–V) < 0.1 | 1.50 | 1.60 | 1.47 | 1.40 | 1.35 | 1.30 | 1.47 | 1.46 |
Sun | 11.51 | 11.78 | 11.62 | 11.02 | 10.38 | 9.00 | 11.17 | 11.28 |
Vega | 2.76 | 4.02 | 2.56 | 2.17 | 2.00 | 1.87 | 2.57 | 2.52 |
a Castelli & Kurucz models are used for the stellar spectra.
b Stars of stellar type G and later may have chromospheric activity leading to UV emission lines not reproduced by the models, which may affect the color corrections listed here.
Table 10.4: Color corrections to go from GALEX NUV AB magnitude to AB magnitude for the SBC (ACS ISR 2019-10).
Spectrum[a] | F115LP | F122M | F125LP | F140LP | F150LP | F165LP | PR110l | PR130L |
---|---|---|---|---|---|---|---|---|
Avg Sky | -4.64 | -5.66 | -2.26 | 2.34 | 7.06 | 5.59 | -4.09 | -2.24 |
Low Sky | -6.42 | -7.51 | -1.20 | 3.29 | 5.13 | 3.68 | -5.81 | -1.18 |
O5V | -0.51 | -0.56 | -0.51 | -0.43 | -0.37 | -0.30 | -0.50 | -0.50 |
B0V | -0.35 | -0.35 | -0.36 | -0.27 | -0.21 | -0.20 | -0.34 | -0.35 |
A0V | 1.58 | 2.95 | 1.38 | 0.94 | 0.64 | 0.30 | 1.36 | 1.31 |
A5V | 3.55 | 5.79 | 3.36 | 2.72 | 2.05 | 0.81 | 3.17 | 3.16 |
F2V | 5.05 | 7.49 | 4.85 | 4.20 | 3.53 | 2.10 | 4.61 | 4.61 |
G2V[b] | 6.99 | 11.16 | 6.78 | 6.13 | 5.47 | 4.00 | 6.37 | 6.37 |
K0V[b] | 6.53 | 12.19 | 6.32 | 5.66 | 5.01 | 3.53 | 5.87 | 5.87 |
M0V[b] | 2.85 | 14.67 | 2.64 | 1.98 | 1.33 | -0.15 | 2.18 | 2.18 |
M6V[b] | 2.67 | 16.95 | 2.46 | 1.80 | 1.15 | -0.33 | 2.00 | 2.00 |
O6I | -0.43 | -0.47 | -0.43 | -0.36 | -0.31 | -0.27 | -0.42 | -0.42 |
B0I | -0.07 | -0.02 | -0.09 | -0.04 | -0.03 | -0.07 | -0.07 | -0.08 |
G0III[b] | 6.86 | 11.05 | 6.65 | 6.00 | 5.34 | 3.87 | 6.24 | 6.24 |
K0III[b] | 5.14 | 14.90 | 4.93 | 4.28 | 3.62 | 2.14 | 4.48 | 4.48 |
M0III[b] | 1.42 | 17.12 | 1.21 | 0.55 | -0.10 | -1.59 | 0.75 | 0.75 |
Elliptical | 1.56 | 1.70 | 1.52 | 1.44 | 1.38 | 1.23 | 1.52 | 1.51 |
Sa | 1.21 | 1.36 | 1.17 | 1.07 | 0.91 | 0.70 | 1.16 | 1.15 |
Sbc | 1.26 | 1.61 | 1.18 | 0.97 | 0.78 | 0.49 | 1.17 | 1.15 |
Scd | 0.82 | 1.07 | 0.76 | 0.61 | 0.47 | 0.26 | 0.76 | 0.74 |
Starburst E(B–V) = 0.51–0.60 | 0.81 | 0.98 | 0.77 | 0.65 | 0.55 | 0.36 | 0.76 | 0.75 |
Starburst E(B–V) < 0.1 | 0.40 | 0.50 | 0.37 | 0.30 | 0.25 | 0.20 | 0.37 | 0.36 |
Sun | 6.15 | 6.43 | 6.27 | 5.67 | 5.03 | 3.64 | 5.81 | 5.92 |
Vega | 1.10 | 2.36 | 0.90 | 0.51 | 0.34 | 0.21 | 0.91 | 0.86 |
a Castelli & Kurucz models are used for the stellar spectra.
b Stars of stellar type G and later may have chromospheric activity leading to UV emission lines not reproduced by the models, which may affect the color corrections listed here.
Table 10.5: Color corrections to go from GALEX FUV AB magnitude to AB magnitude for the SBC (ACS ISR 2019-10).
Spectrum[a] | F115LP | F122M | F125LP | F140LP | F150LP | F165LP | PR110l | PR130L |
---|---|---|---|---|---|---|---|---|
Avg Sky | -14.68 | -15.70 | -12.30 | -7.70 | -2.98 | -4.45 | -14.13 | -12.27 |
Low Sky | -13.43 | -14.52 | -8.21 | -3.72 | -1.88 | -3.33 | -12.81 | -8.19 |
O5V | -0.10 | -0.15 | -0.09 | -0.01 | 0.05 | 0.11 | -0.08 | -0.08 |
B0V | -0.09 | -0.09 | -0.10 | -0.01 | 0.05 | 0.06 | -0.08 | -0.09 |
A0V | 0.72 | 2.09 | 0.52 | 0.09 | -0.21 | -0.56 | 0.50 | 0.46 |
A5V | 0.75 | 2.99 | 0.56 | -0.08 | -0.76 | -1.99 | 0.37 | 0.36 |
F2V | 0.20 | 2.65 | 0.00 | -0.64 | -1.31 | -2.75 | -0.23 | -0.24 |
G2V[b] | -2.03 | 2.16 | -2.24 | -2.89 | -3.55 | -5.02 | -2.66 | -2.66 |
K0V[b] | -3.59 | 2.08 | -3.80 | -4.45 | -5.11 | -6.59 | -4.24 | -4.24 |
M0V[b] | -10.07 | 1.75 | -10.28 | -10.93 | -11.59 | -13.07 | -10.73 | -10.73 |
M6V[b] | -12.63 | 1.63 | -12.84 | -13.49 | -14.15 | -15.63 | -13.29 | -13.29 |
O6I | -0.11 | -0.15 | -0.10 | -0.02 | 0.06 | 0.13 | -0.09 | -0.10 |
B0I | -0.10 | -0.10 | -0.12 | -0.01 | 0.06 | 0.03 | -0.09 | -0.11 |
G0III[b] | -2.05 | 2.14 | -2.26 | -2.92 | -3.57 | -5.05 | -2.68 | -2.68 |
K0III[b] | -7.19 | 1.57 | -7.40 | -8.05 | -8.71 | -10.19 | -7.86 | -7.86 |
M0III[b] | -12.32 | 1.36 | -12.53 | -13.18 | -13.84 | -15.32 | -12.98 | -12.98 |
Elliptical | 0.11 | 0.26 | 0.07 | -0.01 | -0.07 | -0.22 | 0.07 | 0.06 |
Sa | 0.19 | 0.35 | 0.15 | 0.05 | -0.11 | -0.32 | 0.15 | 0.13 |
Sbc | 0.33 | 0.67 | 0.25 | 0.03 | -0.15 | -0.44 | 0.24 | 0.22 |
Scd | 0.25 | 0.49 | 0.19 | 0.03 | -0.11 | -0.32 | 0.18 | 0.17 |
Starburst E(B–V) = 0.51–0.60 | 0.20 | 0.37 | 0.16 | 0.04 | -0.06 | -0.25 | 0.15 | 0.14 |
Starburst E(B–V) < 0.1 | 0.13 | 0.23 | 0.10 | 0.03 | -0.03 | -0.08 | 0.10 | 0.09 |
Sun | -0.94 | -0.66 | -0.83 | -1.43 | -2.06 | -3.45 | -1.28 | -1.17 |
Vega | 0.65 | 1.90 | 0.45 | 0.06 | -0.11 | -0.25 | 0.46 | 0.40 |
a Castelli & Kurucz models are used for the stellar spectra.
b Stars of stellar type G and later may have chromospheric activity leading to UV emission lines not reproduced by the models, which may affect the color corrections listed here.
-
ACS Instrument Handbook
- • Acknowledgments
- • Chapter 1: Introduction
- Chapter 2: Considerations and Changes After SM4
- Chapter 3: ACS Capabilities, Design and Operations
- Chapter 4: Detector Performance
- Chapter 5: Imaging
- Chapter 6: Polarimetry, Coronagraphy, Prism and Grism Spectroscopy
-
Chapter 7: Observing Techniques
- • 7.1 Designing an ACS Observing Proposal
- • 7.2 SBC Bright Object Protection
- • 7.3 Operating Modes
- • 7.4 Patterns and Dithering
- • 7.5 A Road Map for Optimizing Observations
- • 7.6 CCD Gain Selection
- • 7.7 ACS Apertures
- • 7.8 Specifying Orientation on the Sky
- • 7.9 Parallel Observations
- • 7.10 Pointing Stability for Moving Targets
- Chapter 8: Overheads and Orbit-Time Determination
- Chapter 9: Exposure-Time Calculations
-
Chapter 10: Imaging Reference Material
- • 10.1 Introduction
- • 10.2 Using the Information in this Chapter
-
10.3 Throughputs and Correction Tables
- • WFC F435W
- • WFC F475W
- • WFC F502N
- • WFC F550M
- • WFC F555W
- • WFC F606W
- • WFC F625W
- • WFC F658N
- • WFC F660N
- • WFC F775W
- • WFC F814W
- • WFC F850LP
- • WFC G800L
- • WFC CLEAR
- • HRC F220W
- • HRC F250W
- • HRC F330W
- • HRC F344N
- • HRC F435W
- • HRC F475W
- • HRC F502N
- • HRC F550M
- • HRC F555W
- • HRC F606W
- • HRC F625W
- • HRC F658N
- • HRC F660N
- • HRC F775W
- • HRC F814W
- • HRC F850LP
- • HRC F892N
- • HRC G800L
- • HRC PR200L
- • HRC CLEAR
- • SBC F115LP
- • SBC F122M
- • SBC F125LP
- • SBC F140LP
- • SBC F150LP
- • SBC F165LP
- • SBC PR110L
- • SBC PR130L
- • 10.4 Geometric Distortion in ACS
- • Glossary