Liverpool :The Liverpool Telescope Liverpool/RATCam :RATCam was the Liverpool Telescope's main workhorse optical CCD camera and was funded by PPARC (now STFC). |
| Liverpool/RATCam.sdss-u | 3508.36 | 3522.23 | 3541.04 | 3019.20 | 3978.67 | 497.73 | 1440.47 | 3.44e-9 | LT | RATCam | RATCam SDSS u' filter | | Liverpool/RATCam.bessel-B | 4344.33 | 4384.83 | 4348.66 | 3568.70 | 5731.30 | 999.48 | 3955.97 | 6.27e-9 | LT | RATCam | RATCam Bessel B filter | | Liverpool/RATCam.sdss-g | 4765.21 | 4813.94 | 4730.20 | 3944.75 | 5532.10 | 1268.68 | 3940.53 | 5.28e-9 | LT | RATCam | RATCam SDSS g' filter | | Liverpool/RATCam.bessel-V | 5377.11 | 5406.46 | 5355.29 | 4742.00 | 6466.00 | 911.01 | 3634.34 | 3.8e-9 | LT | RATCam | RATCam Bessel V filter | | Liverpool/RATCam.sdss-r | 6208.47 | 6248.13 | 6163.77 | 5423.44 | 7022.00 | 1294.91 | 3136.14 | 2.47e-9 | LT | RATCam | RATCam SDSS r' filter | | Liverpool/RATCam.sdss-r | Filter Description | Filter ID (?) : | Liverpool/RATCam.sdss-r |
| Description (?) : | RATCam SDSS r' filter |
| Phot.System (?) : | ------ |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | r |
| Obs. Facility (?) : | LT |
| Instrument (?) : | RATCam |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
6208.47 | ------- | (Angstrom) |
| λmean (?) : |
6248.13 | ------- | (Angstrom) |
| λcen (?) : |
6253.54 | ------- | (Angstrom) |
| λeff (?) : |
6163.77 | ------- | (Angstrom) |
| λpeak (?) : |
6110.00 | ------- | (Angstrom) |
| λpivot (?) : |
6208.47 | ------- | (Angstrom) |
| λphot (?) : |
6190.24 | ------- | (Angstrom) |
| λmin (?) : |
5423.44 | ------- | (Angstrom) |
| λmax (?) : |
7022.00 | ------- | (Angstrom) |
| Weff (?) : |
1294.91 | ------- | (Angstrom) |
| FWHM (?) : |
1405.00 | ------- | (Angstrom) |
| Af/AV (?) : |
0.88 | ------- | () |
| Fsun (?) : |
167.92 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
The Liverpool Telescope, RATCam Transmission components: Filter | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
2.4747e-9 | (erg/cm2/s/A) |
| |
------- |
3136.14 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Liverpool/RATCam.sdss-r/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
2.86519e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Liverpool/RATCam.sdss-r/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
4601.49 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Liverpool/RATCam.sdss-r/ST |
| |
|
Filter added: 2017-08-05 13:57:04
Last update: 2020-12-10 16:32:50 | | Liverpool/RATCam.Halpha | 6566.44 | 6566.73 | 6566.37 | 6465.39 | 6669.22 | 105.90 | 2660.95 | 1.85e-9 | LT | RATCam | RATCam Halpha filter | | Liverpool/RATCam.sdss-i | 7712.26 | 7764.09 | 7654.60 | 6576.80 | 8791.20 | 1682.94 | 2499.37 | 1.28e-9 | LT | RATCam | RATCam SDSS i' filter | | Liverpool/RATCam.sdss-z | 10508.92 | 10817.26 | 10212.20 | 7867.80 | 13400.00 | 4981.36 | 1879.55 | 5.4e-10 | LT | RATCam | RATCam SDSS z' filter |
| Filter Plots
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© SVO, 8999 filters available, Last update: 2021-01-18 | 
 ≡ 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://ssb.stsci.edu/cdbs_open/cdbs/current_calspec/" target="_blank">STScI current calspec</a>.<li><a href="morefiles/vega.dat" target="_blank">Vega spectrum</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=6248.131865465&id=Liverpool/RATCam.sdss-r><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<br> Vg(λ) ≡ Vega spectrum.<p><img src=showgraph.php?what=leff&val=6163.7733251331&id=Liverpool/RATCam.sdss-r><p><u>More info:</u><p>Vega spectrum from calspec database.<ul><li><a href="https://ssb.stsci.edu/cdbs_open/cdbs/current_calspec/" target="_blank">STScI current calspec</a>.<li><a href="morefiles/vega.dat" target="_blank">Vega spectrum</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=6208.4707860815&id=Liverpool/RATCam.sdss-r><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<br> Vg(λ) ≡ Vega spectrum<p><img src=showgraph.php?what=lphot&val=6190.2370474534&id=Liverpool/RATCam.sdss-r><p><u>More info:</u><p>Vega spectrum from calspec database.<ul><li><a href="https://ssb.stsci.edu/cdbs_open/cdbs/current_calspec/" target="_blank">STScI current calspec</a>.<li><a href="morefiles/vega.dat" target="_blank">Vega spectrum</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=1294.9073730696,6253.5416666667,0.95&id=Liverpool/RATCam.sdss-r><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.<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://ssb.stsci.edu/cdbs_open/cdbs/current_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<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://ssb.stsci.edu/cdbs_open/cdbs/current_calspec/" target="_blank">STScI current calspec</a>.<li><a href="morefiles/vega.dat" target="_blank">Vega spectrum</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}
