Subaru :Subaru Telescope Subaru/HSC :The Hyper Suprime-Cam (HSC) is a gigantic mosaic CCD caThe Hyper Suprime-Cam (HSC) is a gigantic mosaic CCD camera, which is attached at the prime focus of Subaru Telescope.mera, which is attached at the prime focus of Subaru Telescope.id:Subaru/HSC.a → GaiaXPy base XML file. You can download here the GaiaXPy base XML file for the full Subaru/HSC filter set. Please, take a look to the GaiaXPy web page and additional documentation for more information. |
| Subaru/HSC.NB387_filter | 3858.57 | 3858.71 | 3859.73 | 3813.11 | 3906.24 | 56.57 | 3226.10 | 6.5e-9 | Subaru | HSC | HSC NB387 (filter only) | | Subaru/HSC.NB468_filter | 4688.79 | 4689.08 | 4688.51 | 4607.85 | 4769.60 | 90.28 | 4227.32 | 5.76e-9 | Subaru | HSC | HSC NB468 (filter only) | | Subaru/HSC.g_filter | 4710.97 | 4768.83 | 4669.70 | 3942.85 | 5547.08 | 1302.88 | 4033.09 | 5.45e-9 | Subaru | HSC | HSC g (filter only) | | Subaru/HSC.g | 4798.21 | 4850.98 | 4758.71 | 3954.22 | 5547.29 | 1052.67 | 3991.75 | 5.2e-9 | Subaru | HSC | HSC g (full transmission) | | Subaru/HSC.NB515_filter | 5154.80 | 5154.98 | 5154.48 | 5088.06 | 5224.40 | 76.07 | 3830.80 | 4.32e-9 | Subaru | HSC | HSC NB515 (filter only) | | Subaru/HSC.NB527_filter | 5253.45 | 5253.62 | 5253.26 | 5187.65 | 5312.20 | 73.40 | 3761.58 | 4.09e-9 | Subaru | HSC | HSC NB527 (filter only) | | Subaru/HSC.r2_filter | 6183.13 | 6231.09 | 6130.27 | 5021.21 | 7216.76 | 1518.19 | 3192.28 | 2.5e-9 | Subaru | HSC | HSC r2 (filter only) | | Subaru/HSC.r_filter | 6189.59 | 6238.42 | 6135.56 | 5330.23 | 7071.80 | 1381.69 | 3188.43 | 2.5e-9 | Subaru | HSC | HSC r (filter only) | | Subaru/HSC.r | 6218.44 | 6265.24 | 6166.33 | 5001.90 | 7498.20 | 1385.07 | 3170.27 | 2.46e-9 | Subaru | HSC | HSC r (full transmission) | | Subaru/HSC.NB656_filter | 6543.52 | 6543.82 | 6541.18 | 6444.07 | 6643.90 | 109.19 | 2683.13 | 1.88e-9 | Subaru | HSC | HSC NB656 (filter only) | | Subaru/HSC.NB718_filter | 7165.80 | 7166.10 | 7165.52 | 7056.34 | 7268.78 | 107.64 | 2716.95 | 1.59e-9 | Subaru | HSC | HSC NB718 (filter only) | | Subaru/HSC.i_filter | 7698.22 | 7735.66 | 7656.73 | 6800.59 | 8658.53 | 1383.32 | 2514.97 | 1.27e-9 | Subaru | HSC | HSC i (filter only) | | Subaru/HSC.i2_filter | 7720.72 | 7760.98 | 7676.62 | 6881.50 | 8999.20 | 1545.40 | 2507.63 | 1.26e-9 | Subaru | HSC | HSC i2 (filter only) | | Subaru/HSC.i | 7727.01 | 7767.72 | 7682.36 | 6886.12 | 8999.20 | 1503.69 | 2505.44 | 1.26e-9 | Subaru | HSC | HSC i (full transmission) | | Subaru/HSC.NB816_filter | 8168.09 | 8168.36 | 8167.71 | 8055.85 | 8287.64 | 111.93 | 2331.30 | 1.05e-9 | Subaru | HSC | HSC NB816 (filter only) | | Subaru/HSC.z | 8908.50 | 8917.86 | 8906.54 | 8363.85 | 9490.57 | 761.28 | 2252.95 | 8.51e-10 | Subaru | HSC | HSC y (full transmission) | | Subaru/HSC.z_filter | 8921.75 | 8931.42 | 8919.85 | 8364.41 | 9498.95 | 781.38 | 2254.27 | 8.49e-10 | Subaru | HSC | HSC z (filter only) | | Subaru/HSC.NB921_filter | 9204.59 | 9204.94 | 9202.05 | 9082.35 | 9331.36 | 133.53 | 2200.95 | 7.79e-10 | Subaru | HSC | HSC NB921 (filter only) | | Subaru/HSC.NB926_filter | 9253.46 | 9253.84 | 9254.75 | 9113.31 | 9410.97 | 139.69 | 2176.21 | 7.62e-10 | Subaru | HSC | HSC NB926 (filter only) | | Subaru/HSC.IB945_filter | 9447.04 | 9448.69 | 9442.19 | 9192.06 | 9735.04 | 326.68 | 2225.57 | 7.48e-10 | Subaru | HSC | HSC IB945 (filter only) | | Subaru/HSC.NB973_filter | 9697.19 | 9697.53 | 9697.23 | 9542.50 | 9853.24 | 114.78 | 2239.26 | 7.14e-10 | Subaru | HSC | HSC NB973 (filter only) | | Subaru/HSC.Y | 9775.07 | 9789.78 | 9759.62 | 9000.00 | 10756.42 | 824.04 | 2161.26 | 6.78e-10 | Subaru | HSC | HSC y (full transmission) | | Subaru/HSC.Y | Filter Description | Filter ID (?) : | Subaru/HSC.Y |
| Description (?) : | HSC y (full transmission) |
| Phot.System (?) : | ------ |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | Subaru |
| Instrument (?) : | HSC |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
9775.07 | ------- | (Angstrom) |
| λmean (?) : |
9789.78 | ------- | (Angstrom) |
| λcen (?) : |
9745.74 | ------- | (Angstrom) |
| λeff (?) : |
9759.62 | ------- | (Angstrom) |
| λpeak (?) : |
9700.00 | ------- | (Angstrom) |
| λpivot (?) : |
9775.07 | ------- | (Angstrom) |
| λphot (?) : |
9769.16 | ------- | (Angstrom) |
| λmin (?) : |
9000.00 | ------- | (Angstrom) |
| λmax (?) : |
10756.42 | ------- | (Angstrom) |
| Weff (?) : |
824.04 | ------- | (Angstrom) |
| FWHM (?) : |
792.99 | ------- | (Angstrom) |
| Af/AV (?) : |
0.444 | ------- | () |
| Fsun (?) : |
76.23 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
COSMOS filter set Transmission components: Filter + Instrument + Atmosphereid:Subaru/HSC.Y
You can download here the GaiaXPy base XML file for the full Subaru/HSC 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 (?) : |
------- |
6.78091e-10 | (erg/cm2/s/A) |
| |
------- |
2161.26 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Subaru/HSC.Y/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
1.13922e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Subaru/HSC.Y/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
11572.99 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Subaru/HSC.Y/ST |
| |
|
Filter added: 2019-06-12 20:27:06
Last update: 2021-07-27 20:38:22 | | Subaru/HSC.Y_filter | 10019.92 | 10045.14 | 9993.28 | 9000.00 | 10934.85 | 1339.29 | 2106.35 | 6.29e-10 | Subaru | HSC | HSC Y (filter only) |
|
| 
 ≡ 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=9789.7806338315&id=Subaru/HSC.Y><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=9759.6235347984&id=Subaru/HSC.Y><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=9775.0718679352&id=Subaru/HSC.Y><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=9769.1616179971&id=Subaru/HSC.Y><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=824.04394288542,9745.7407727224,1&id=Subaru/HSC.Y><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}
