| HST/FOC_F96.F140W | 1637.29 | 1916.80 | 1882.32 | 1153.17 | 5104.88 | 523.45 | 485.42 | 5.43e-9 | HST | FOC | F140W filter for HST FOC_F/96 |
| HST/FOC_F96.F130M | 1498.10 | 2046.56 | 2469.03 | 1169.96 | 4631.20 | 148.93 | 235.43 | 3.14e-9 | HST | FOC | F130M filter for HST FOC_F/96 |
| HST/FOC_F96.F170M | 1921.53 | 2112.83 | 2048.51 | 1179.92 | 4397.91 | 323.48 | 706.56 | 5.74e-9 | HST | FOC | F170M filter for HST FOC_F/96 |
| HST/FOC_F96.F175W | 1979.93 | 2175.25 | 2091.21 | 1186.72 | 4830.90 | 988.23 | 715.46 | 5.47e-9 | HST | FOC | F175W filter for HST FOC_F/96 |
| HST/FOC_F96.F210M | 2179.05 | 2212.49 | 2199.94 | 1748.95 | 2719.50 | 256.16 | 789.68 | 4.99e-9 | HST | FOC | F210M filter for HST FOC_F/96 |
| HST/FOC_F96.F190M | 2092.48 | 2238.59 | 2200.28 | 1645.06 | 4626.67 | 355.36 | 802.42 | 5.49e-9 | HST | FOC | F190M filter for HST FOC_F/96 |
| HST/FOC_F96.F120M | 1544.00 | 2290.95 | 3244.11 | 1133.22 | 5356.59 | 162.69 | 202.60 | 2.55e-9 | HST | FOC | F120M filter for HST FOC_F/96 |
| HST/FOC_F96.F152M | 1829.87 | 2314.43 | 2187.91 | 1172.11 | 5776.73 | 424.71 | 644.59 | 5.77e-9 | HST | FOC | F152M filter for HST FOC_F/96 |
| HST/FOC_F96.F220W | 2327.86 | 2379.45 | 2349.67 | 1660.42 | 3635.94 | 559.59 | 808.25 | 4.47e-9 | HST | FOC | F220W filter for HST FOC_F/96 |
| HST/FOC_F96.F231M | 2355.92 | 2379.69 | 2371.48 | 1923.06 | 2934.13 | 273.53 | 796.51 | 4.3e-9 | HST | FOC | F231M filter for HST FOC_F/96 |
| HST/FOC_F96.F165W | 2095.71 | 2380.81 | 2290.69 | 1189.34 | 5491.40 | 1288.07 | 762.26 | 5.2e-9 | HST | FOC | F165W filter for HST FOC_F/96 |
| HST/FOC_F96.F140M | 1876.63 | 2469.81 | 2394.88 | 1162.46 | 5868.31 | 510.78 | 607.39 | 5.17e-9 | HST | FOC | F140M filter for HST FOC_F/96 |
| HST/FOC_F96.F253M | 2552.18 | 2570.60 | 2568.41 | 2093.44 | 3072.33 | 275.11 | 854.48 | 3.93e-9 | HST | FOC | F253M filter for HST FOC_F/96 |
| HST/FOC_F96.F278M | 2809.72 | 2830.24 | 2824.94 | 2227.84 | 3467.18 | 361.79 | 981.72 | 3.73e-9 | HST | FOC | F278M filter for HST FOC_F/96 |
| HST/FOC_F96.F275W | 2800.26 | 2855.72 | 2846.72 | 1706.33 | 4107.65 | 686.63 | 990.13 | 3.79e-9 | HST | FOC | F275W filter for HST FOC_F/96 |
| HST/FOC_F96.F307M | 3061.90 | 3095.89 | 3084.74 | 1661.49 | 3790.61 | 385.64 | 1124.80 | 3.6e-9 | HST | FOC | F307M filter for HST FOC_F/96 |
| HST/FOC_F96.F320W | 3112.75 | 3159.55 | 3139.11 | 2354.92 | 3756.94 | 754.05 | 1123.24 | 3.48e-9 | HST | FOC | F320W filter for HST FOC_F/96 |
| HST/FOC_F96.F342W | 3403.71 | 3425.48 | 3431.94 | 2867.24 | 3928.69 | 667.20 | 1325.52 | 3.43e-9 | HST | FOC | F342W filter for HST FOC_F/96 |
| HST/FOC_F96.F195W | 2402.71 | 3456.85 | 2661.77 | 1167.07 | 5846.49 | 1490.87 | 893.89 | 4.64e-9 | HST | FOC | F195W filter for HST FOC_F/96 |
| HST/FOC_F96.F346M | 3474.46 | 3483.35 | 3483.15 | 3117.79 | 3847.47 | 420.68 | 1313.92 | 3.26e-9 | HST | FOC | F346M filter for HST FOC_F/96 |
| HST/FOC_F96.F372M | 3710.33 | 3718.89 | 3765.55 | 3350.19 | 4156.88 | 405.62 | 2015.17 | 4.39e-9 | HST | FOC | F372M filter for HST FOC_F/96 |
| HST/FOC_F96.F410M | 4087.55 | 4089.78 | 4089.02 | 3881.93 | 4326.23 | 200.29 | 4177.42 | 7.5e-9 | HST | FOC | F410M filter for HST FOC_F/96 |
| HST/FOC_F96.F430W | 4117.14 | 4149.25 | 4161.46 | 3536.80 | 5071.46 | 842.22 | 3625.58 | 6.41e-9 | HST | FOC | F430W filter for HST FOC_F/96 |
| HST/FOC_F96.F437M | 4255.07 | 4325.07 | 4330.36 | 2946.70 | 4709.77 | 389.04 | 4019.03 | 6.65e-9 | HST | FOC | F437M filter for HST FOC_F/96 |
| HST/FOC_F96.F470M | 4702.56 | 4704.55 | 4699.34 | 4431.46 | 4945.39 | 209.28 | 4167.67 | 5.65e-9 | HST | FOC | F470M filter for HST FOC_F/96 |
| HST/FOC_F96.F470M | Filter Description | Filter ID (?) : | HST/FOC_F96.F470M |
| Description (?) : | F470M filter for HST FOC_F/96 |
| Phot.System (?) : | FOC-F96 |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | HST |
| Instrument (?) : | FOC |
| Comments (?) : | Response calculated using the stsynphot python package by STScI. In particular, function stsynphot.band("foc,f/96,f470m"). Please, take a look to stsynphot documentation and HST instrument documentation |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
4702.56 | ------- | (Angstrom) |
| λmean (?) : |
4704.55 | ------- | (Angstrom) |
| λcen (?) : |
4702.95 | ------- | (Angstrom) |
| λeff (?) : |
4699.34 | ------- | (Angstrom) |
| λpeak (?) : |
4710.00 | ------- | (Angstrom) |
| λpivot (?) : |
4702.56 | ------- | (Angstrom) |
| λphot (?) : |
4700.63 | ------- | (Angstrom) |
| λmin (?) : |
4431.46 | ------- | (Angstrom) |
| λmax (?) : |
4945.39 | ------- | (Angstrom) |
| Weff (?) : |
209.28 | ------- | (Angstrom) |
| FWHM (?) : |
209.51 | ------- | (Angstrom) |
| Af/AV (?) : |
1.21 | ------- | () |
| Fsun (?) : |
201.48 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
stsynphot documentation Transmission components: Filter + CCD + Instrumentid:HST/FOC_F96.F470M
You can download here the GaiaXPy base XML file for the full HST/FOC_F96 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 (?) : |
------- |
5.64995e-9 | (erg/cm2/s/A) |
| |
------- |
4167.67 | (Jy) |
| PhotCal ID (?) : |
HST/FOC_F96.F470M/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
4.92241e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
HST/FOC_F96.F470M/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
2678.40 | (Jy) |
| PhotCal ID (?) : |
HST/FOC_F96.F470M/ST |
| |
|
Filter added: 2019-07-16 12:13:58
Last update: 2022-03-01 15:10:59 |
| HST/FOC_F96.F486N | 4867.55 | 4867.69 | 4868.56 | 4811.13 | 4927.07 | 35.97 | 2834.85 | 3.59e-9 | HST | FOC | F/486N filter for HST FOC_F/96 |
| HST/FOC_F96.F502M | 4985.68 | 4993.46 | 4982.91 | 4645.42 | 5393.08 | 440.75 | 3812.37 | 4.6e-9 | HST | FOC | F502M filter for HST FOC_F/96 |
| HST/FOC_F96.F501N | 5019.58 | 5019.88 | 5019.32 | 4940.67 | 5099.49 | 73.47 | 3944.65 | 4.69e-9 | HST | FOC | F501N filter for HST FOC_F/96 |
| HST/FOC_F96.F550M | 5507.30 | 5508.67 | 5505.99 | 5304.59 | 5727.65 | 185.52 | 3599.37 | 3.56e-9 | HST | FOC | F550M filter for HST FOC_F/96 |
| HST/FOC_F96.F600M | 5788.26 | 6710.61 | 5814.05 | 3591.13 | 6444.28 | 444.34 | 3047.88 | 2.73e-9 | HST | FOC | F600M filter for HST FOC_F/96 |
| HST/FOC_F96.F6ND | 3539.88 | 8502.30 | 3747.42 | 1158.65 | 30000.00 | 3366.60 | 1503.83 | 3.6e-9 | HST | FOC | F6ND filter for HST FOC_F/96 |
| HST/FOC_F96.F2ND | 3801.01 | 8561.07 | 3901.22 | 1176.27 | 30000.00 | 3072.44 | 1751.39 | 3.63e-9 | HST | FOC | F2ND filter for HST FOC_F/96 |
| HST/FOC_F96.F1ND | 3822.66 | 8667.75 | 3916.90 | 1171.21 | 30000.00 | 3063.25 | 1765.51 | 3.62e-9 | HST | FOC | F1ND filter for HST FOC_F/96 |
| HST/FOC_F96.PRISM1 | 3956.05 | 9074.26 | 3984.53 | 1190.33 | 30000.00 | 3170.68 | 1863.02 | 3.57e-9 | HST | FOC | PRISM1 filter for HST FOC_F/96 |
| HST/FOC_F96.PRISM2 | 4093.18 | 9166.08 | 4040.80 | 1626.95 | 30000.00 | 3066.17 | 1989.06 | 3.56e-9 | HST | FOC | PRISM2 filter for HST FOC_F/96 |
| HST/FOC_F96.F130LP | 4017.27 | 9265.56 | 4007.41 | 1238.95 | 30000.00 | 3187.12 | 1899.93 | 3.53e-9 | HST | FOC | F130LP filter for HST FOC_F/96 |
| HST/FOC_F96.POL0 | 4034.36 | 9292.44 | 4015.31 | 1196.45 | 30000.00 | 3176.26 | 1911.75 | 3.52e-9 | HST | FOC | POL0 filter for HST FOC_F/96 |
| HST/FOC_F96.POL120 | 4053.43 | 9327.43 | 4019.95 | 1272.82 | 30000.00 | 3172.71 | 1927.44 | 3.52e-9 | HST | FOC | POL120 filter for HST FOC_F/96 |
| HST/FOC_F96.POL60 | 4228.50 | 9415.88 | 4095.83 | 1929.85 | 30000.00 | 3045.73 | 2081.14 | 3.49e-9 | HST | FOC | POL60 filter for HST FOC_F/96 |
| HST/FOC_F96.F4ND | 4115.68 | 9956.52 | 4044.80 | 1181.81 | 30000.00 | 3422.35 | 1891.73 | 3.35e-9 | HST | FOC | F4ND filter for HST FOC_F/96 |
| HST/FOC_F96.F8ND | 4485.71 | 11838.89 | 4180.76 | 1177.31 | 30000.00 | 4124.06 | 1948.27 | 2.9e-9 | HST | FOC | F8ND filter for HST FOC_F/96 |
| HST/FOC_F96.F370LP | 5771.95 | 12775.13 | 4622.63 | 3596.51 | 30000.00 | 2363.80 | 3680.33 | 3.31e-9 | HST | FOC | F370LP filter for HST FOC_F/96 |
| HST/FOC_F96.F480LP | 8788.98 | 18306.14 | 5903.71 | 4674.44 | 30000.00 | 3102.62 | 3250.04 | 1.26e-9 | HST | FOC | F/480LP filter for HST FOC_F/96 |
| HST/FOC_F96.F630M | 15767.98 | 23482.98 | 10476.14 | 6206.49 | 30000.00 | 14247.16 | 1725.90 | 2.08e-10 | HST | FOC | F630M filter for HST FOC_F/96 |
 ≡ 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=4704.5535349757&id=HST/FOC_F96.F470M><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=4699.3428392495&id=HST/FOC_F96.F470M><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=4702.5627005639&id=HST/FOC_F96.F470M><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=4700.6319176826&id=HST/FOC_F96.F470M><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=209.27592031192,4702.9511529156,1&id=HST/FOC_F96.F470M><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}
