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| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,87 @@ | ||
| # %ECSV 0.9 | ||
| # --- | ||
| # datatype: | ||
| # - {name: wavelength, unit: Angstrom, datatype: float64} | ||
| # - {name: response, datatype: float64} | ||
| # meta: !!omap | ||
| # - {band_name: H} | ||
| # - {description: 'Instrument: 2MASS Cameras in Mt. Hopkins, AZ, and CTIO, Chile | ||
| # | ||
| # Determined by: Cohen, Wheaton & Megeath (2003), AJ, 126, 1990 with notes: | ||
| # | ||
| # "Table 1 - 2MASS Isophotal Bandpasses and Fluxes-for-0-magnitude from Cohen et al. (2003) | ||
| # Band Lambda (micron) Bandwidth (micron) Fnu - 0 mag (Jy) Flambda - 0 mag (W cm-2 micron-1) | ||
| # J 1.235 0.006 0.162 0.001 1594 27.8 3.129E-13 5.464E-15 | ||
| # H 1.662 0.009 0.251 0.002 1024 20.0 1.133E-13 2.212E-15 | ||
| # Ks 2.159 0.011 0.262 0.002 666.7 12.6 4.283E-14 8.053E-16 | ||
| # | ||
| # Figures 1, 2, and 3 present the 2MASS J, H and Ks relative spectral | ||
| # response curves (RSRs), peak-normalized to unity. These curves are | ||
| # derived by Cohen et al. (2003) and are photon-counting RSRs suitable | ||
| # for integrating over stellar spectra when using or generating synthetic | ||
| # photometry. These RSRs are consistent with the absolute calibration of | ||
| # 2MASS given in Table 1 above." | ||
| # | ||
| # Notes: | ||
| # I am not in a position to judge the quality of these curves, but | ||
| # have no reason to doubt them. - Michael Blanton 2005-07-06'} | ||
| # - {group_name: twomass} | ||
| wavelength response | ||
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| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,136 @@ | ||
| # %ECSV 0.9 | ||
| # --- | ||
| # datatype: | ||
| # - {name: wavelength, unit: Angstrom, datatype: float64} | ||
| # - {name: response, datatype: float64} | ||
| # meta: !!omap | ||
| # - {band_name: J} | ||
| # - {description: 'Instrument: 2MASS Cameras in Mt. Hopkins, AZ, and CTIO, Chile | ||
| # | ||
| # Determined by: Cohen, Wheaton & Megeath (2003), AJ, 126, 1990 with notes: | ||
| # | ||
| # "Table 1 - 2MASS Isophotal Bandpasses and Fluxes-for-0-magnitude from Cohen et al. (2003) | ||
| # Band Lambda (micron) Bandwidth (micron) Fnu - 0 mag (Jy) Flambda - 0 mag (W cm-2 micron-1) | ||
| # J 1.235 0.006 0.162 0.001 1594 27.8 3.129E-13 5.464E-15 | ||
| # H 1.662 0.009 0.251 0.002 1024 20.0 1.133E-13 2.212E-15 | ||
| # Ks 2.159 0.011 0.262 0.002 666.7 12.6 4.283E-14 8.053E-16 | ||
| # | ||
| # Figures 1, 2, and 3 present the 2MASS J, H and Ks relative spectral | ||
| # response curves (RSRs), peak-normalized to unity. These curves are | ||
| # derived by Cohen et al. (2003) and are photon-counting RSRs suitable | ||
| # for integrating over stellar spectra when using or generating synthetic | ||
| # photometry. These RSRs are consistent with the absolute calibration of | ||
| # 2MASS given in Table 1 above." | ||
| # | ||
| # Notes: | ||
| # I am not in a position to judge the quality of these curves, but | ||
| # have no reason to doubt them. - Michael Blanton 2005-07-06'} | ||
| # - {group_name: twomass} | ||
| wavelength response | ||
| 10620.0 0 | ||
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| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,105 @@ | ||
| # %ECSV 0.9 | ||
| # --- | ||
| # datatype: | ||
| # - {name: wavelength, unit: Angstrom, datatype: float64} | ||
| # - {name: response, datatype: float64} | ||
| # meta: !!omap | ||
| # - {band_name: Ks} | ||
| # - {description: 'Instrument: 2MASS Cameras in Mt. Hopkins, AZ, and CTIO, Chile | ||
| # | ||
| # Determined by: Cohen, Wheaton & Megeath (2003), AJ, 126, 1990 with notes: | ||
| # | ||
| # "Table 1 - 2MASS Isophotal Bandpasses and Fluxes-for-0-magnitude from Cohen et al. (2003) | ||
| # Band Lambda (micron) Bandwidth (micron) Fnu - 0 mag (Jy) Flambda - 0 mag (W cm-2 micron-1) | ||
| # J 1.235 0.006 0.162 0.001 1594 27.8 3.129E-13 5.464E-15 | ||
| # H 1.662 0.009 0.251 0.002 1024 20.0 1.133E-13 2.212E-15 | ||
| # Ks 2.159 0.011 0.262 0.002 666.7 12.6 4.283E-14 8.053E-16 | ||
| # | ||
| # Figures 1, 2, and 3 present the 2MASS J, H and Ks relative spectral | ||
| # response curves (RSRs), peak-normalized to unity. These curves are | ||
| # derived by Cohen et al. (2003) and are photon-counting RSRs suitable | ||
| # for integrating over stellar spectra when using or generating synthetic | ||
| # photometry. These RSRs are consistent with the absolute calibration of | ||
| # 2MASS given in Table 1 above." | ||
| # | ||
| # Notes: | ||
| # I am not in a position to judge the quality of these curves, but | ||
| # have no reason to doubt them. - Michael Blanton 2005-07-06'} | ||
| # - {group_name: twomass} | ||
| wavelength response | ||
| 18970.0 0 | ||
| 19150.0 0 | ||
| 19270.0 0 | ||
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