Subaru :Subaru Telescope Subaru/CIAO :The Coronagraphic Imager with Adaptive Optics (CIAO) is primarily designed for the detection of faint objects near much brighter ones via the use of occulting masks. |
| Subaru/CIAO.z | 10316.41 | 10320.49 | 10314.14 | 9839.67 | 10845.92 | 514.80 | 2064.34 | 5.82e-10 | Subaru | CIAO | CIAO z | | Subaru/CIAO.Jcont | 12117.46 | 12117.97 | 12116.80 | 11916.50 | 12310.52 | 188.82 | 1647.47 | 3.36e-10 | Subaru | CIAO | CIAO Jcont | | Subaru/CIAO.J | 12456.93 | 12484.14 | 12417.40 | 11481.88 | 13494.96 | 1516.74 | 1562.23 | 3.04e-10 | Subaru | CIAO | CIAO J | | Subaru/CIAO.J | Filter Description | Filter ID (?) : | Subaru/CIAO.J |
| Description (?) : | CIAO J |
| Phot.System (?) : | ------ |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | J |
| Obs. Facility (?) : | Subaru |
| Instrument (?) : | CIAO |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
12456.93 | ------- | (Angstrom) |
| λmean (?) : |
12484.14 | ------- | (Angstrom) |
| λcen (?) : |
12471.67 | ------- | (Angstrom) |
| λeff (?) : |
12417.40 | ------- | (Angstrom) |
| λpeak (?) : |
12738.00 | ------- | (Angstrom) |
| λpivot (?) : |
12456.93 | ------- | (Angstrom) |
| λphot (?) : |
12435.55 | ------- | (Angstrom) |
| λmin (?) : |
11481.88 | ------- | (Angstrom) |
| λmax (?) : |
13494.96 | ------- | (Angstrom) |
| Weff (?) : |
1516.74 | ------- | (Angstrom) |
| FWHM (?) : |
1616.81 | ------- | (Angstrom) |
| Af/AV (?) : |
0.303 | ------- | () |
| Fsun (?) : |
44.84 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
CIAO Camera sensitivities Transmission components: Filter | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.03741e-10 | (erg/cm2/s/A) |
| |
------- |
1562.23 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Subaru/CIAO.J/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
7.05969e-10 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Subaru/CIAO.J/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
18675.26 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Subaru/CIAO.J/ST |
| |
|
Filter added: 2017-08-05 19:30:33
Last update: 2020-12-10 16:34:03 | | Subaru/CIAO.Pabeta | 12943.95 | 12944.42 | 12944.90 | 12730.27 | 13137.63 | 186.83 | 1462.59 | 2.62e-10 | Subaru | CIAO | CIAO Pabeta | | Subaru/CIAO.Hcont | 15813.01 | 15813.46 | 15811.78 | 15601.85 | 16018.51 | 212.33 | 1074.06 | 1.29e-10 | Subaru | CIAO | CIAO HCont | | Subaru/CIAO.CH4s | 16048.11 | 16062.36 | 16030.55 | 14941.69 | 17375.05 | 1195.59 | 1060.59 | 1.24e-10 | Subaru | CIAO | CIAO CH4 | | Subaru/CIAO.H | 16229.34 | 16298.26 | 16141.06 | 14510.18 | 18091.02 | 2845.72 | 1045.89 | 1.2e-10 | Subaru | CIAO | CIAO H | | Subaru/CIAO.FeII | 16515.44 | 16516.06 | 16517.54 | 16279.55 | 16764.33 | 251.60 | 1023.96 | 1.13e-10 | Subaru | CIAO | CIAO [FeII] | | Subaru/CIAO.CH4l | 16871.99 | 16888.32 | 16850.93 | 15684.00 | 18228.59 | 1309.20 | 990.12 | 1.05e-10 | Subaru | CIAO | CIAO CH4 off | | Subaru/CIAO.H2v1-0 | 21298.99 | 21299.68 | 21297.88 | 21004.32 | 21604.83 | 310.06 | 685.69 | 4.53e-11 | Subaru | CIAO | CIAO H2 1-0 | | Subaru/CIAO.Ks | 21403.35 | 21461.26 | 21315.12 | 19503.30 | 23390.45 | 3057.40 | 676.31 | 4.46e-11 | Subaru | CIAO | CIAO Ks | | Subaru/CIAO.K | 21939.11 | 22005.42 | 21840.51 | 19859.45 | 24015.16 | 3242.25 | 647.72 | 4.07e-11 | Subaru | CIAO | CIAO K | | Subaru/CIAO.H2v2-1 | 22626.83 | 22627.95 | 22625.15 | 22203.43 | 23020.00 | 379.30 | 617.55 | 3.62e-11 | Subaru | CIAO | CIAO H2 2-1 | | Subaru/CIAO.Kcont | 22853.78 | 22854.62 | 22852.52 | 22460.57 | 23186.46 | 318.24 | 606.88 | 3.48e-11 | Subaru | CIAO | CIAO Kcont | | Subaru/CIAO.COv2-0 | 23066.95 | 23067.75 | 23065.77 | 22715.62 | 23400.00 | 292.31 | 597.27 | 3.37e-11 | Subaru | CIAO | CIAO CO 2-0 | | Subaru/CIAO.H2Oice | 30862.69 | 30877.11 | 30844.24 | 28877.90 | 32750.00 | 1469.40 | 356.06 | 1.12e-11 | Subaru | CIAO | CIAO H2O ice | | Subaru/CIAO.PAH | 33194.60 | 33196.17 | 33195.51 | 32656.47 | 33719.20 | 538.75 | 308.85 | 8.4e-12 | Subaru | CIAO | CIAO PAH | | Subaru/CIAO.Lp | 37571.62 | 37741.31 | 37301.72 | 33056.85 | 42253.89 | 6829.61 | 248.30 | 5.35e-12 | Subaru | CIAO | CIAO L' | | Subaru/CIAO.Mp | 46830.29 | 46848.24 | 46803.76 | 45086.21 | 48871.91 | 2405.97 | 164.74 | 2.25e-12 | Subaru | CIAO | CIAO M' |
|
| 
 ≡ 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=12484.139390087&id=Subaru/CIAO.J><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=12417.396907526&id=Subaru/CIAO.J><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=12456.926422198&id=Subaru/CIAO.J><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=12435.547358648&id=Subaru/CIAO.J><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=1516.7389560605,12471.670288625,0.9352&id=Subaru/CIAO.J><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://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>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}
