|
| JWST/NIRCam.F070W | 7039.12 | 7088.30 | 6988.43 | 6048.20 | 7927.07 | 1212.84 | 2768.40 | 1.67e-9 | JWST | NIRCam | NIRCam F070W filter | | JWST/NIRCam.F090W | 9021.53 | 9083.40 | 8984.98 | 7881.88 | 10243.08 | 1772.74 | 2244.95 | 8.27e-10 | JWST | NIRCam | NIRCam F090W filter | | JWST/NIRCam.F115W | 11542.61 | 11623.88 | 11433.62 | 9975.60 | 13058.40 | 2055.13 | 1746.12 | 3.93e-10 | JWST | NIRCam | NIRCam F115W filter | | JWST/NIRCam.F140M | 14053.23 | 14074.47 | 14023.62 | 13042.25 | 15058.58 | 1367.40 | 1288.65 | 1.96e-10 | JWST | NIRCam | NIRCam F140M filter | | JWST/NIRCam.F150W | 15007.44 | 15104.23 | 14872.56 | 13041.19 | 16948.89 | 2890.43 | 1172.06 | 1.56e-10 | JWST | NIRCam | NIRCam F150W filter | | JWST/NIRCam.F162M | 16272.47 | 16296.59 | 16243.33 | 15126.16 | 17439.17 | 1626.29 | 1023.04 | 1.16e-10 | JWST | NIRCam | NIRCam F162M filter | | JWST/NIRCam.F164N | 16445.36 | 16445.95 | 16446.18 | 16171.41 | 16717.72 | 200.10 | 985.58 | 1.09e-10 | JWST | NIRCam | NIRCam F164N filter | | JWST/NIRCam.F150W2 | 16592.11 | 17865.57 | 14793.71 | 9774.71 | 23946.87 | 9389.16 | 1149.94 | 1.25e-10 | JWST | NIRCam | NIRCam F150W2 filter | | JWST/NIRCam.F182M | 18451.67 | 18494.30 | 18388.83 | 16959.53 | 20010.97 | 2250.81 | 844.94 | 7.44e-11 | JWST | NIRCam | NIRCam F182M filter | | JWST/NIRCam.F187N | 18738.99 | 18739.65 | 18737.22 | 18445.28 | 19029.98 | 236.69 | 794.85 | 6.79e-11 | JWST | NIRCam | NIRCam F187N filter | | JWST/NIRCam.F200W | 19886.48 | 20028.15 | 19680.41 | 17249.08 | 22596.64 | 4190.39 | 757.65 | 5.74e-11 | JWST | NIRCam | NIRCam F200W filter | | JWST/NIRCam.F210M | 20954.51 | 20982.22 | 20908.35 | 19618.54 | 22337.29 | 2055.38 | 688.03 | 4.7e-11 | JWST | NIRCam | NIRCam F210M filter | | JWST/NIRCam.F212N | 21213.18 | 21213.97 | 21211.93 | 20900.93 | 21524.99 | 274.27 | 674.83 | 4.5e-11 | JWST | NIRCam | NIRCam F212N filter | | JWST/NIRCam.F250M | 25032.33 | 25049.39 | 25005.80 | 23935.49 | 26177.91 | 1782.96 | 504.65 | 2.41e-11 | JWST | NIRCam | NIRCam F250M filter | | JWST/NIRCam.F277W | 27617.40 | 27844.64 | 27278.58 | 23673.12 | 32203.22 | 6614.61 | 430.14 | 1.69e-11 | JWST | NIRCam | NIRCam F277W filter | | JWST/NIRCam.F300M | 29891.21 | 29940.44 | 29818.32 | 27703.55 | 32505.92 | 3255.58 | 369.65 | 1.24e-11 | JWST | NIRCam | NIRCam F300M filter | | JWST/NIRCam.F323N | 32368.53 | 32369.29 | 32367.30 | 32046.29 | 32761.07 | 384.89 | 320.94 | 9.18e-12 | JWST | NIRCam | NIRCam F323N filter | | JWST/NIRCam.F322W2 | 32319.76 | 33334.92 | 30731.38 | 23851.45 | 41234.69 | 11332.55 | 343.30 | 9.85e-12 | JWST | NIRCam | NIRCam F322W2 filter | | JWST/NIRCam.F335M | 33620.67 | 33675.24 | 33537.23 | 31203.36 | 36442.23 | 3389.42 | 298.91 | 7.93e-12 | JWST | NIRCam | NIRCam F335M filter | | JWST/NIRCam.F356W | 35683.62 | 35934.49 | 35287.04 | 30732.91 | 40801.26 | 7239.30 | 271.39 | 6.39e-12 | JWST | NIRCam | NIRCam F356W filter | | JWST/NIRCam.F360M | 36241.76 | 36298.10 | 36148.93 | 33260.34 | 39037.39 | 3584.80 | 260.31 | 5.94e-12 | JWST | NIRCam | NIRCam F360M filter | | JWST/NIRCam.F405N | 40516.53 | 40517.39 | 40515.76 | 40097.87 | 40966.10 | 454.87 | 206.97 | 3.78e-12 | JWST | NIRCam | NIRCam F405N filter | | JWST/NIRCam.F410M | 40822.38 | 40886.54 | 40723.18 | 37763.56 | 44048.41 | 4262.86 | 208.75 | 3.76e-12 | JWST | NIRCam | NIRCam F410M filter | | JWST/NIRCam.F430M | 42812.58 | 42829.39 | 42784.79 | 41227.68 | 44448.79 | 2295.14 | 190.70 | 3.12e-12 | JWST | NIRCam | NIRCam F430M filter | | JWST/NIRCam.F430M | Filter Description | Filter ID (?) : | JWST/NIRCam.F430M |
| Description (?) : | NIRCam F430M filter |
| Phot.System (?) : | NIRCam |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | JWST |
| Instrument (?) : | NIRCam |
| Comments (?) : | includes NIRCam optics, DBS, QE and JWST Optical Telescope Element |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
42812.58 | ------- | (Angstrom) |
| λmean (?) : |
42829.39 | ------- | (Angstrom) |
| λcen (?) : |
42832.58 | ------- | (Angstrom) |
| λeff (?) : |
42784.79 | ------- | (Angstrom) |
| λpeak (?) : |
42482.70 | ------- | (Angstrom) |
| λpivot (?) : |
42812.58 | ------- | (Angstrom) |
| λphot (?) : |
42795.89 | ------- | (Angstrom) |
| λmin (?) : |
41227.68 | ------- | (Angstrom) |
| λmax (?) : |
44448.79 | ------- | (Angstrom) |
| Weff (?) : |
2295.14 | ------- | (Angstrom) |
| FWHM (?) : |
2315.31 | ------- | (Angstrom) |
| Af/AV (?) : |
0.0548 | ------- | () |
| Fsun (?) : |
0.649 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
James Webb Space Telescope User Documentation Transmission components: Filter + Instrumentid:JWST/NIRCam.F430M
You can download here the GaiaXPy base XML file for the full JWST/NIRCam filter set.
Please, take a look to GaiaXPy documentation for more information. - GaiaXPy base XML file. | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.11904e-12 | (erg/cm2/s/A) |
| |
------- |
190.70 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
JWST/NIRCam.F430M/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
5.93888e-11 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
JWST/NIRCam.F430M/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
221997.59 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
JWST/NIRCam.F430M/ST |
| |
|
Filter added: 2017-03-11 13:02:57
Last update: 2021-07-27 20:03:37 | | JWST/NIRCam.F444W | 44043.15 | 44393.52 | 43504.26 | 38039.57 | 50995.50 | 10676.00 | 184.10 | 2.85e-12 | JWST | NIRCam | NIRCam F444W filter | | JWST/NIRCam.F460M | 46299.28 | 46315.57 | 46269.86 | 44652.64 | 48146.41 | 2309.00 | 164.11 | 2.3e-12 | JWST | NIRCam | NIRCam F460M filter | | JWST/NIRCam.F466N | 46544.30 | 46545.31 | 46540.48 | 46021.35 | 47042.62 | 535.41 | 157.77 | 2.18e-12 | JWST | NIRCam | NIRCam F466N filter | | JWST/NIRCam.F470N | 47077.91 | 47078.82 | 47077.84 | 46553.98 | 47566.82 | 510.27 | 159.50 | 2.16e-12 | JWST | NIRCam | NIRCam F470N filter | | JWST/NIRCam.F480M | 48181.95 | 48213.27 | 48139.11 | 45820.02 | 50919.02 | 3141.37 | 153.22 | 1.98e-12 | JWST | NIRCam | NIRCam F480M 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=42829.393603083&id=JWST/NIRCam.F430M><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=42784.78806412&id=JWST/NIRCam.F430M><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=42812.575646101&id=JWST/NIRCam.F430M><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=42795.894458171&id=JWST/NIRCam.F430M><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=2295.1444214116,42832.58018141,1&id=JWST/NIRCam.F430M><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}
