LYRA :The purpose of the LYRA mission is a multi-color all-sky survey of objects from 3m to 16m from the International Space Station. LYRA/LYRA :LYRA photometric bands |
| LYRA/LYRA.1 | 1971.10 | 1973.00 | 1971.29 | 1831.07 | 2157.32 | 112.21 | 740.53 | 5.71e-9 | ISS | LYRA | LYRA 195nm (1) filter | | LYRA/LYRA.2 | 2169.62 | 2171.73 | 2169.10 | 1999.56 | 2363.15 | 130.29 | 764.81 | 4.87e-9 | ISS | LYRA | LYRA 218nm (2) filter | | LYRA/LYRA.3 | 2722.20 | 2726.23 | 2723.79 | 2468.54 | 3078.78 | 203.02 | 927.01 | 3.75e-9 | ISS | LYRA | LYRA 270nm (3) filter | | LYRA/LYRA.4 | 3536.26 | 3549.83 | 3577.77 | 2959.50 | 4110.68 | 422.53 | 1495.65 | 3.5e-9 | ISS | LYRA | LYRA 350nm (4) filter | | LYRA/LYRA.4a | 3746.47 | 3759.09 | 3816.41 | 3200.71 | 4318.03 | 418.70 | 2306.67 | 4.75e-9 | ISS | LYRA | LYRA 374nm (4a) filter | | LYRA/LYRA.5 | 4467.26 | 4517.29 | 4466.60 | 3437.24 | 5664.83 | 1013.30 | 3954.05 | 5.94e-9 | ISS | LYRA | LYRA 440nm (5) filter | | LYRA/LYRA.6 | 5527.96 | 5551.49 | 5506.03 | 4708.35 | 6836.10 | 714.51 | 3559.87 | 3.52e-9 | ISS | LYRA | LYRA 555nm (6) filter | | LYRA/LYRA.pan | 5545.85 | 6596.25 | 5426.01 | 1764.41 | 10805.40 | 5785.99 | 2588.89 | 2.64e-9 | ISS | LYRA | LYRA broad panchromatic filter | | LYRA/LYRA.pan | Filter Description | Filter ID (?) : | LYRA/LYRA.pan |
| Description (?) : | LYRA broad panchromatic filter |
| Phot.System (?) : | LYRA |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | ISS |
| Instrument (?) : | LYRA |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
5545.85 | ------- | (Angstrom) |
| λmean (?) : |
6596.25 | ------- | (Angstrom) |
| λcen (?) : |
6031.56 | ------- | (Angstrom) |
| λeff (?) : |
5426.01 | ------- | (Angstrom) |
| λpeak (?) : |
4270.66 | ------- | (Angstrom) |
| λpivot (?) : |
5545.85 | ------- | (Angstrom) |
| λphot (?) : |
5925.36 | ------- | (Angstrom) |
| λmin (?) : |
1764.41 | ------- | (Angstrom) |
| λmax (?) : |
10805.40 | ------- | (Angstrom) |
| Weff (?) : |
5785.99 | ------- | (Angstrom) |
| FWHM (?) : |
6050.37 | ------- | (Angstrom) |
| Af/AV (?) : |
1.02 | ------- | () |
| Fsun (?) : |
135.04 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
Mironov et al 2016 Transmission components: Filter + CCD + Instrument | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
2.63617e-9 | (erg/cm2/s/A) |
| |
------- |
2588.89 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
LYRA/LYRA.pan/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.69731e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
LYRA/LYRA.pan/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
3565.88 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
LYRA/LYRA.pan/ST |
| |
|
Filter added: 2020-05-29 18:41:58
Last update: 2021-02-25 10:29:51 | | LYRA/LYRA.7 | 6958.36 | 6966.80 | 6950.78 | 6372.44 | 7634.16 | 434.70 | 2815.57 | 1.75e-9 | ISS | LYRA | LYRA 700nm (7) filter | | LYRA/LYRA.7a | 7845.91 | 7864.77 | 7825.79 | 6856.70 | 8954.08 | 760.39 | 2465.75 | 1.21e-9 | ISS | LYRA | LYRA 785nm (7a) filter | | LYRA/LYRA.8 | 8230.08 | 8247.44 | 8213.17 | 7210.74 | 9280.06 | 754.92 | 2340.24 | 1.04e-9 | ISS | LYRA | LYRA 825nm (8) filter | | LYRA/LYRA.9 | 9280.00 | 9299.80 | 9268.86 | 8119.96 | 10410.98 | 892.34 | 2260.18 | 7.89e-10 | ISS | LYRA | LYRA 930nm (9) filter | | LYRA/LYRA.10 | 9646.37 | 9666.30 | 9628.82 | 8453.00 | 10639.98 | 913.42 | 2203.87 | 7.13e-10 | ISS | LYRA | LYRA 1000nm (10) filter |
|
| 
 ≡ 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}
 ≡ filter transmission<p>f(λ) ≡ flux of the spectrum<p><u>Property info:</u><ul><li><b>Utype</b>: <i>photdm:PhotometricSystem.detectorType</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission<p><img src=showgraph.php?what=lmean&val=6596.2527106396&id=LYRA/LYRA.pan><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>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission (photon counter)<br> Vg(λ) ≡ Vega spectrum<p><img src=showgraph.php?what=leff&val=5426.0087977458&id=LYRA/LYRA.pan><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>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission<p><img src=showgraph.php?what=lpiv&val=5545.8516535769&id=LYRA/LYRA.pan><p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl</ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission (photon counter)<br> Vg(λ) ≡ Vega spectrum<p><img src=showgraph.php?what=lphot&val=5925.3574484351&id=LYRA/LYRA.pan><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</ul></td></table>',STICKY,true,CLOSEBTN,true,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><img src=showgraph.php?what=weff&val=5785.9857532412,6031.5603549786,0.65860834&id=LYRA/LYRA.pan><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>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
![(?)](javascript:Tip('<b>A<sub>f</sub>/A<sub>V</sub></b><br><table cellpadding=20><td class=helptd>Ratio between extintion at λ<sub>ref</sub> and visual extintion. <p>Calculated by the service using the extinction law by <a href="http://adsabs.harvard.edu/abs/1999PASP..111...63F" target="_blank">Fitzpatrick (1999)</a> improved by <a href="http://adsabs.harvard.edu/abs/2005ApJ...619..931I" target="_blank">Indebetouw et al (2005)</a> in the infrared. <p><img src=images/extinctionlaw.png><p>You can download the corresponding <a href=\"getextlaw.php\" target=\"_blank\">data file</a> for the opacity k<sub>λ</sub>. The extinction at each wavelength is calculated as: A<sub>λ</sub> = A<sub>V</sub> * k<sub>λ</sub>/k<sub>V</sub>, where k<sub>λ</sub> is the opacity for a given λ and k<sub>V</sub>=211.4<p><p><u>Property info:</u><ul></ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission (photon counter).<br> Sun(λ) ≡ Sun spectrum.<p><img src=images/sunspec.png><p><p><u>More info:</u><p>Sun spectrum from calspec database: sun_reference_stis_002 composed with sun_mod_001 for larger wavelengths.<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/sun.dat" target="_blank">Sun composed spectrum</a> (units: Angstrom erg/cm2/s/A).</ul><p><u>Property info:</u><ul><li><b>Unit</b>:erg/cm2/s/A<li><b>UCD</b>:phot.flux.density</ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission (photon counter).<br> Vg(λ) ≡ Vega spectrum.<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>VO PhotDM Utypes</u>: <br><i>PhotCal.MagnitudeSystem.type</i> -> VEGAmag <br><i>PhotCal.ZeroPoint.Flux.value</i> -> F<sub>0</sub><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>UCD</b>:phot.flux.density<li><b>Utype</b>: <i>photdm:PhotCal.ZeroPoint.Flux.value</i></ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
