MER :Mars Exploration Rovers MER/PanCam :The Panoramic Camera is known by its nickname, Pancam. Two cameras work in combination to take detailed, multi-wavelength, 3-D panoramic pictures of the Martian landscape surrounding the rover.id:MER/PanCam.a |
| MER/PanCam.L7 | 4357.85 | 4366.52 | 4356.89 | 3869.50 | 4746.87 | 341.70 | 4217.87 | 6.66e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L7 (blue stereo) filter | | MER/PanCam.R1 | 4357.85 | 4366.52 | 4356.89 | 3869.50 | 4746.87 | 341.70 | 4217.87 | 6.66e-9 | MER | PanCam | Mars Exploration Rover PanCam right camera R1 (blue stereo) filter | | MER/PanCam.L8 | 4429.31 | 4430.52 | 4433.10 | 4289.75 | 4609.45 | 178.24 | 4159.98 | 6.36e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L8 (solar) filter | | MER/PanCam.L6 | 4832.58 | 4835.52 | 4827.56 | 4577.80 | 5127.43 | 286.99 | 3855.37 | 4.95e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L6 (geology) filter | | MER/PanCam.L5 | 5349.86 | 5351.02 | 5348.75 | 5183.61 | 5555.24 | 197.61 | 3696.27 | 3.87e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L5 (geology) filter | | MER/PanCam.L5 | Filter Description | Filter ID (?) : | MER/PanCam.L5 |
| Description (?) : | Mars Exploration Rover PanCam left camera L5 (geology) filter |
| Phot.System (?) : | PanCam |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | MER |
| Instrument (?) : | PanCam |
| Comments (?) : | Normalized total system throughput.
Approx. curve, digitized from Fig. 6 in Bell et al 2003.
|
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
5349.86 | ------- | (Angstrom) |
| λmean (?) : |
5351.02 | ------- | (Angstrom) |
| λcen (?) : |
5347.77 | ------- | (Angstrom) |
| λeff (?) : |
5348.75 | ------- | (Angstrom) |
| λpeak (?) : |
5377.48 | ------- | (Angstrom) |
| λpivot (?) : |
5349.86 | ------- | (Angstrom) |
| λphot (?) : |
5349.52 | ------- | (Angstrom) |
| λmin (?) : |
5183.61 | ------- | (Angstrom) |
| λmax (?) : |
5555.24 | ------- | (Angstrom) |
| Weff (?) : |
197.61 | ------- | (Angstrom) |
| FWHM (?) : |
201.11 | ------- | (Angstrom) |
| Af/AV (?) : |
1.04 | ------- | () |
| Fsun (?) : |
187.81 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
Bell et al 2003 Transmission components: Filter + CCD + Instrument + Other optical componentsid:MER/PanCam.L5 | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.87168e-9 | (erg/cm2/s/A) |
| |
------- |
3696.27 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MER/PanCam.L5/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.80332e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MER/PanCam.L5/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
3466.49 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MER/PanCam.L5/ST |
| |
|
Filter added: 2020-06-27 22:01:02
Last update: 2021-07-27 20:15:58 | | MER/PanCam.L4 | 6012.85 | 6013.92 | 6011.71 | 5826.57 | 6250.92 | 187.68 | 3288.85 | 2.73e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L4 (geology) filter | | MER/PanCam.L3 | 6747.91 | 6748.88 | 6747.32 | 6529.19 | 6990.22 | 162.80 | 2897.35 | 1.91e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L3 (geology) filter | | MER/PanCam.L2 | 7545.53 | 7546.63 | 7544.30 | 7306.53 | 7788.56 | 213.23 | 2560.83 | 1.35e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L2 (red stereo) filter | | MER/PanCam.R2 | 7545.53 | 7546.63 | 7544.30 | 7306.53 | 7788.56 | 213.23 | 2560.83 | 1.35e-9 | MER | PanCam | Mars Exploration Rover PanCam right camera R2 (red stereo) filter | | MER/PanCam.L1 | 7291.45 | 7663.10 | 6912.83 | 4093.77 | 10835.93 | 3214.17 | 2832.75 | 1.6e-9 | MER | PanCam | Mars Exploration Rover PanCam left camera L1 (empty) filter | | MER/PanCam.R3 | 8046.21 | 8047.07 | 8045.23 | 7839.88 | 8258.99 | 204.07 | 2377.37 | 1.1e-9 | MER | PanCam | Mars Exploration Rover PanCam right camera R3 (geology) filter | | MER/PanCam.R4 | 8643.08 | 8643.80 | 8643.09 | 8443.03 | 8855.56 | 183.00 | 2226.40 | 8.93e-10 | MER | PanCam | Mars Exploration Rover PanCam right camera R4 (geology) filter | | MER/PanCam.R8lk | 8640.10 | 8684.43 | 8592.80 | 6904.00 | 9091.08 | 266.91 | 2315.13 | 9.3e-10 | MER | PanCam | Mars Exploration Rover PanCam right camera R8 (solar) filter+leak | | MER/PanCam.R8 | 8824.98 | 8826.30 | 8825.50 | 8542.82 | 9090.85 | 241.38 | 2262.18 | 8.71e-10 | MER | PanCam | Mars Exploration Rover PanCam right camera R8 (solar) filter | | MER/PanCam.R5 | 9044.06 | 9045.48 | 9043.43 | 8814.16 | 9329.56 | 266.01 | 2296.36 | 8.42e-10 | MER | PanCam | Mars Exploration Rover PanCam right camera R5 (geology) filter | | MER/PanCam.R6 | 9346.61 | 9348.07 | 9347.12 | 9052.96 | 9660.81 | 257.93 | 2257.69 | 7.75e-10 | MER | PanCam | Mars Exploration Rover PanCam right camera R6 (geology) filter | | MER/PanCam.R7 | 10124.11 | 10132.65 | 10114.32 | 9693.16 | 11004.45 | 470.87 | 2071.46 | 6.06e-10 | MER | PanCam | Mars Exploration Rover PanCam right camera R7 (geology) filter |
|
| 
 ≡ 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}
 ≡ filter transmission<p>f(λ) ≡ flux of the spectrum<p><u>Property info:</u><ul><li><b>UCD</b>:meta.code<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=5351.0170949316&id=MER/PanCam.L5><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=leff&val=5348.748010616&id=MER/PanCam.L5><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=5349.8580020198&id=MER/PanCam.L5><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=5349.5210955602&id=MER/PanCam.L5><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=197.61313958127,5347.7714681684,1&id=MER/PanCam.L5><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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>',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/extlaw.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/sun.png"><p><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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.<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>Filter transmission is transformed to \"<i>energy counter</i>\" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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}
