Mercator :The Mercator telescope is a modern semi-robotic telescope, installed at the Roque de los Muchachos Observatory on La Palma (Canary Islands, Spain) at an altitude of 2333 m above sea level. Mercator/MAIA :MAIA, the Mercator Advanced Imager for Asteroseismology is a new fast 3-channel photometric instrument. id:Mercator/MAIA.a → GaiaXPy base XML file. You can download here the GaiaXPy base XML file for the full Mercator/MAIA filter set. Please, take a look to the GaiaXPy web page and additional documentation for more information. |
| Mercator/MAIA.u | 3632.24 | 3641.85 | 3667.99 | 3189.96 | 3880.00 | 306.41 | 1672.98 | 3.8e-9 | Mercator | MAIA | MAIA u filter | | Mercator/MAIA.g | 4820.57 | 4868.64 | 4784.27 | 3967.16 | 5577.87 | 1117.86 | 3979.31 | 5.13e-9 | Mercator | MAIA | MAIA g filter | | Mercator/MAIA.r | 6376.42 | 6412.47 | 6335.48 | 5417.00 | 7099.00 | 1097.07 | 3073.33 | 2.27e-9 | Mercator | MAIA | MAIA r filter |
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 ≡ filter transmission<p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl</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.bandwidth.extent.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>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}
