INT :Isaac Newton Telescope. INT/OASIS :The optical integral-field spectrograph OASIS is installed at one of the science ports of NAOMI, in the William Herschel Telescope's Adaptive Optics-dedicated Nasmyth enclosure.id:INT/OASIS.a → GaiaXPy base XML file. You can download here the GaiaXPy base XML file for the full INT/OASIS filter set. Please, take a look to the GaiaXPy web page and additional documentation for more information. |
| INT/OASIS.MR454 | 4524.94 | 4542.07 | 4507.54 | 4100.00 | 5000.00 | 759.56 | 4140.66 | 6.06e-9 | INT | OASIS | OASIS MR454, ING#582 | | INT/OASIS.HR502 | 5022.66 | 5025.69 | 5025.68 | 4820.00 | 5240.00 | 331.21 | 3791.64 | 4.51e-9 | INT | OASIS | OASIS HR502, ING#590 | | INT/OASIS.MR516 | 5137.96 | 5152.97 | 5130.59 | 4720.00 | 5600.00 | 721.32 | 3755.36 | 4.26e-9 | INT | OASIS | OASIS MR516, ING#583 | | INT/OASIS.HR530 | 5296.34 | 5299.60 | 5293.08 | 5080.00 | 5520.00 | 344.09 | 3738.06 | 3.99e-9 | INT | OASIS | OASIS HR530, ING#591 | | INT/OASIS.MR591 | 5898.08 | 5912.53 | 5883.09 | 5460.00 | 6405.00 | 775.50 | 3362.68 | 2.9e-9 | INT | OASIS | OASIS MR591, ING#584 | | INT/OASIS.HR638 | 6375.35 | 6377.72 | 6370.88 | 6160.00 | 6600.00 | 327.27 | 3049.67 | 2.25e-9 | INT | OASIS | OASIS HR638, ING#592 | | INT/OASIS.MR661 | 6596.03 | 6608.28 | 6583.78 | 6160.87 | 7100.00 | 767.79 | 2929.73 | 2.02e-9 | INT | OASIS | OASIS MR661, ING#585 | | INT/OASIS.HR667 | 6660.52 | 6662.84 | 6662.01 | 6442.37 | 6897.16 | 332.54 | 2827.59 | 1.91e-9 | INT | OASIS | OASIS HR667, ING#593 | | INT/OASIS.MR735 | 7339.31 | 7350.76 | 7326.68 | 6885.81 | 7832.56 | 796.98 | 2648.35 | 1.47e-9 | INT | OASIS | OASIS MR735, ING#586 | | INT/OASIS.MR807 | 8064.63 | 8073.88 | 8054.52 | 7624.76 | 8537.59 | 734.58 | 2370.74 | 1.09e-9 | INT | OASIS | OASIS MR807, ING#587 | | INT/OASIS.MR875 | 8742.24 | 8751.60 | 8741.63 | 8300.00 | 9230.29 | 786.88 | 2257.90 | 8.86e-10 | INT | OASIS | OASIS MR875, ING#588 | | INT/OASIS.LR951 | 9465.99 | 9505.58 | 9436.25 | 8510.16 | 10517.03 | 1649.63 | 2197.45 | 7.35e-10 | INT | OASIS | OASIS LR951, ING#581 | | INT/OASIS.LR951 | Filter Description | Filter ID (?) : | INT/OASIS.LR951 |
| Description (?) : | OASIS LR951, ING#581 |
| Phot.System (?) : | OASIS |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | INT |
| Instrument (?) : | OASIS |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
9465.99 | ------- | (Angstrom) |
| λmean (?) : |
9505.58 | ------- | (Angstrom) |
| λcen (?) : |
9515.40 | ------- | (Angstrom) |
| λeff (?) : |
9436.25 | ------- | (Angstrom) |
| λpeak (?) : |
9120.00 | ------- | (Angstrom) |
| λpivot (?) : |
9465.99 | ------- | (Angstrom) |
| λphot (?) : |
9462.14 | ------- | (Angstrom) |
| λmin (?) : |
8510.16 | ------- | (Angstrom) |
| λmax (?) : |
10517.03 | ------- | (Angstrom) |
| Weff (?) : |
1649.63 | ------- | (Angstrom) |
| FWHM (?) : |
1726.81 | ------- | (Angstrom) |
| Af/AV (?) : |
0.469 | ------- | () |
| Fsun (?) : |
81.03 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
ING Filter Database Transmission components: Filterid:INT/OASIS.LR951
You can download here the GaiaXPy base XML file for the full INT/OASIS 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 (?) : |
------- |
7.35202e-10 | (erg/cm2/s/A) |
| |
------- |
2197.45 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
INT/OASIS.LR951/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
1.21483e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
INT/OASIS.LR951/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
10852.70 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
INT/OASIS.LR951/ST |
| |
|
Filter added: 2011-10-18 05:20:04
Last update: 2021-07-27 19:41:07 | | INT/OASIS.MR952 | 9525.33 | 9532.73 | 9521.18 | 9081.27 | 9989.62 | 704.87 | 2216.37 | 7.32e-10 | INT | OASIS | OASIS MR952, ING#589 |
|
| 
 ≡ 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=9505.5789975917&id=INT/OASIS.LR951><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=9436.2505850384&id=INT/OASIS.LR951><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=9465.9936831618&id=INT/OASIS.LR951><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=9462.1428233032&id=INT/OASIS.LR951><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=1649.628607223,9515.4034898086,0.93547&id=INT/OASIS.LR951><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}
