| TCS/CAIN3.J | 12631.07 | 12716.27 | 12514.06 | 10824.37 | 14242.51 | 2475.24 | 1527.23 | 2.87e-10 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 J filter |
| TCS/CAIN3.paschen | 12865.62 | 12866.15 | 12867.17 | 12631.57 | 13126.54 | 156.20 | 1382.01 | 2.5e-10 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 paschen filter |
| TCS/CAIN3.Fe | 16516.50 | 16517.08 | 16517.62 | 16235.60 | 16807.23 | 183.96 | 1008.33 | 1.11e-10 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 Fe filter |
| TCS/CAIN3.H | 16637.44 | 16714.07 | 16537.95 | 14703.44 | 18816.55 | 3006.69 | 997.15 | 1.08e-10 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 H filter |
| TCS/CAIN3.H21 | 21401.28 | 21401.63 | 21400.60 | 21194.67 | 21606.42 | 197.72 | 663.31 | 4.34e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 H2 (1-0) filter |
| TCS/CAIN3.H21_b | 21464.24 | 21464.78 | 21462.32 | 21202.24 | 21717.60 | 227.74 | 655.22 | 4.26e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 H2 (1-0) filter |
| TCS/CAIN3.Brg | 21832.76 | 21833.11 | 21833.15 | 21625.04 | 22037.63 | 201.82 | 635.34 | 4.0e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 Br gamma filter |
| TCS/CAIN3.Kshort | 21784.85 | 21841.66 | 21699.89 | 19887.36 | 23869.20 | 2939.09 | 645.21 | 4.08e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 Kshort filter |
| TCS/CAIN3.K | 22173.08 | 22235.05 | 22082.12 | 20148.98 | 24258.25 | 3186.29 | 625.89 | 3.82e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 K filter |
| TCS/CAIN3.K | Filter Description | Filter ID (?) : | TCS/CAIN3.K |
| Description (?) : | Telescopio Carlos Sanchez, CAIN-3 K filter |
| Phot.System (?) : | CAIN3 |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | K |
| Obs. Facility (?) : | TCS |
| Instrument (?) : | CAIN-3 |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
22173.08 | ------- | (Angstrom) |
| λmean (?) : |
22235.05 | ------- | (Angstrom) |
| λcen (?) : |
22220.36 | ------- | (Angstrom) |
| λeff (?) : |
22082.12 | ------- | (Angstrom) |
| λpeak (?) : |
23073.00 | ------- | (Angstrom) |
| λpivot (?) : |
22173.08 | ------- | (Angstrom) |
| λphot (?) : |
22123.45 | ------- | (Angstrom) |
| λmin (?) : |
20148.98 | ------- | (Angstrom) |
| λmax (?) : |
24258.25 | ------- | (Angstrom) |
| Weff (?) : |
3186.29 | ------- | (Angstrom) |
| FWHM (?) : |
3247.08 | ------- | (Angstrom) |
| Af/AV (?) : |
0.121 | ------- | () |
| Fsun (?) : |
8.00 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
IAC Transmission components: Filterid:TCS/CAIN3.K | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.81653e-11 | (erg/cm2/s/A) |
| |
------- |
625.89 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
TCS/CAIN3.K/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
2.21409e-10 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
TCS/CAIN3.K/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
59546.67 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
TCS/CAIN3.K/ST |
| |
|
Filter added: 2011-10-18 08:32:08
Last update: 2021-07-27 20:39:15 |
| TCS/CAIN3.H22_b | 22627.83 | 22628.35 | 22627.05 | 22369.29 | 22878.36 | 233.05 | 602.90 | 3.53e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 H2 (2-1) filter |
| TCS/CAIN3.H22_a | 22628.53 | 22629.20 | 22627.51 | 22328.05 | 22921.91 | 258.22 | 602.88 | 3.53e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 H2 (2-1) filter |
| TCS/CAIN3.Kcont | 22770.84 | 22772.71 | 22768.02 | 22291.61 | 23258.20 | 504.34 | 596.37 | 3.45e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 Kcont filter |
| TCS/CAIN3.Kcont_b | 22781.74 | 22783.55 | 22779.03 | 22317.47 | 23263.03 | 514.91 | 595.87 | 3.44e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 Kcont filter |
| TCS/CAIN3.Kcont_c | 22810.48 | 22812.76 | 22807.07 | 22257.66 | 23387.87 | 516.37 | 594.59 | 3.43e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 Kcont filter |
| TCS/CAIN3.CO_c | 23061.91 | 23062.33 | 23061.29 | 22817.17 | 23283.91 | 214.53 | 583.30 | 3.29e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 CO filter |
| TCS/CAIN3.CO_b | 23110.22 | 23110.65 | 23109.58 | 22859.55 | 23342.84 | 219.71 | 581.21 | 3.26e-11 | TCS | CAIN-3 | Telescopio Carlos Sanchez, CAIN-3 CO 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=22235.049522671&id=TCS/CAIN3.K><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=22082.124965981&id=TCS/CAIN3.K><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=22173.077579535&id=TCS/CAIN3.K><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=22123.451406683&id=TCS/CAIN3.K><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=3186.2909337634,22220.361906812,0.958324&id=TCS/CAIN3.K><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><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}
