OAN-SPM :San Pedro Martir National Astronomical Observatory (OAN-SPM) OAN-SPM/OPTICAM :OPTICAM is a triple-band high-time resolution optical system in development as a collaborative work between the Astronomy Group of the University of Southampton and the Institute of Astronomy of the Universidad Nacional Autonoma de Mexico. |
| OAN-SPM/OPTICAM.u_fil | 3506.86 | 3520.88 | 3536.27 | 3150.00 | 3850.00 | 578.38 | 1425.57 | 3.48e-9 | OAN-SPM | OPTICAM | OPTICAM u filter (filter only) | | OAN-SPM/OPTICAM.u | 3565.44 | 3578.18 | 3598.17 | 3150.00 | 3850.00 | 375.12 | 1518.79 | 3.58e-9 | OAN-SPM | OPTICAM | OPTICAM u filter (+CCD) | | OAN-SPM/OPTICAM.g_fil | 4726.81 | 4783.43 | 4685.60 | 3990.14 | 5520.00 | 1281.26 | 4028.34 | 5.41e-9 | OAN-SPM | OPTICAM | OPTICAM g filter (filter only) | | OAN-SPM/OPTICAM.g | 4806.36 | 4858.09 | 4767.20 | 4000.00 | 5520.00 | 1071.48 | 3988.58 | 5.18e-9 | OAN-SPM | OPTICAM | OPTICAM g filter (+CCD) | | OAN-SPM/OPTICAM.r | 6257.52 | 6291.48 | 6218.89 | 5591.90 | 6988.83 | 1264.57 | 3139.12 | 2.4e-9 | OAN-SPM | OPTICAM | OPTICAM r filter (+CCD) | | OAN-SPM/OPTICAM.r_fil | 6269.35 | 6303.67 | 6230.29 | 5592.25 | 6989.09 | 1194.32 | 3132.46 | 2.39e-9 | OAN-SPM | OPTICAM | OPTICAM r filter (filter only) | | OAN-SPM/OPTICAM.i | 7580.91 | 7617.30 | 7541.19 | 6833.33 | 8632.47 | 1288.67 | 2559.92 | 1.34e-9 | OAN-SPM | OPTICAM | OPTICAM i filter (+CCD) | | OAN-SPM/OPTICAM.i_fil | 7664.18 | 7702.17 | 7622.00 | 6835.47 | 8640.52 | 1393.96 | 2528.24 | 1.29e-9 | OAN-SPM | OPTICAM | OPTICAM i filter (filter only) | | OAN-SPM/OPTICAM.z | 8874.17 | 8911.64 | 8856.75 | 8044.68 | 10346.80 | 1010.13 | 2243.84 | 8.54e-10 | OAN-SPM | OPTICAM | OPTICAM z filter (+CCD) | | OAN-SPM/OPTICAM.z_fil | 9601.39 | 9699.97 | 9520.41 | 8066.99 | 11009.20 | 2404.58 | 2143.22 | 6.97e-10 | OAN-SPM | OPTICAM | OPTICAM z filter (filter only) |
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 ≡ filter transmission<p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl<li><b>Utype</b>: <i>photdm:PhotometryFilter.SpectralAxis.Coverage.Location.Value</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission<br> Vg(λ) ≡ Vega spectrum.<p><u>More info:</u><p>Vega spectrum from calspec database.<ul><li><a href="https://ui.adsabs.harvard.edu/abs/2014PASP..126..711B/abstract" target="_blank">Bohlin, Gordon, & Tremblay (2014)</a>.<li><a href="https://www.stsci.edu/hst/instrumentation/reference-data-for-calibration-and-tools/astronomical-catalogs/calspec" target="_blank">STScI current calspec</a>.<li><a href="morefiles/vega.dat" target="_blank">Vega spectrum file</a> (units: Angstrom erg/cm2/s/A).</ul><p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl.effective</ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission<p>Equivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve.<p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:instr.bandwidth<li><b>Utype</b>: <i>photdm:PhotometryFilter.SpectralAxis.Coverage.Bounds.Extent</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission (energy counter).<br> Vg(λ) ≡ Vega spectrum.<p><i>(T(λ) must be multiplied by λ for photon counting devices)</i><p>F<sub>0,ν</sub>(Jy) = (2.9979246)<sup>-1</sup> 10<sup>5</sup> * λ<sub>ref</sub><sup>2</sup> * F<sub>0,λ</sub>(erg/cm<sup>2</sup>/s/A)<p>In the case that filter owner specifies its own values, they will be the ones provided by the service when queried through the VO.<p><u>Property info:</u><ul><li><b>Unit</b>:Jy<li><b>UCD</b>:phot.flux.density<li><b>Utype</b>: <i>photdm:PhotCal.ZeroPoint.Flux.value</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission (energy counter).<br> Vg(λ) ≡ Vega spectrum.<p><i>(T(λ) must be multiplied by λ for photon counting devices)</i><p><u>Property info:</u><ul><li><b>Unit</b>:erg/cm2/s/A<li><b>Utype</b>: <i>PhotCal.ZeroPoint</i></ul></td></table>',WIDTH,400)){kind=link}
