Filter Profile Service
Carlos Rodrigo
A repository of Filter information for the VO.
 Grant PID2020-112494GBI00 funded by
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Astronomy (7905)Planetary science (616)Earth Obs. (2452)

2MASSAAOADEOSAKARIAkatsukiAlSat1APEXAPOAquaARCHEOPSARGOAstrosatBeijing1Bepi-ColomboBICEP
BLASTBOKBOOMERANGCAHACamerasCassiniCASTORCFHTCHEOPSClementineCMO-SAICOBECOMSContourCorot
COSMOSOMASCSSTCSTARCTIODawnDeepImpactDENISDOTDSCOVREnvisatERBSEROSERSESOEuclid
ExoMarsFengYunFlockFLWOGAIAGALEXGalileoGCOM-CGCPDGeminiGenericGenevaGeoEyeGiottoGOES
GOTOGTCHayabusa2HCTHerschelHimawariHipparcosHSTIAC80IKONOSINGINSATInSightINTIntegral
IRAMIRASIRSIRSFIRTFISOIUEJCMTJPSSJWSTKeckKeplerKOMPSTATKPNOLandsat
LasCumbresLaSillaLBTLCOLICKLiverpoolLMTLROLSSTLYRAMariner10Mars2020MAXIMAMcDMER
MercatorMessengerMeteosatMETOPMEXMiscMKOMMTMOAMOMMOSTMROMSXMTNAOC
NEARNewHorizonsNigeriaSat1NIMBUSNIRTNOAANOAONOTOAFOAJOAN-SPMOAOOdysseyOHPOLIMPO
OSIRIS-REXOSNOVROP200PalomarPAN-STARRSParanalParasolPathfinderPLANCKPleiadesPRIRODAQuickBirdQUIETQUIJOTE
RapidEyeRomanRosettaSALTSAOScorpioSeaStarSeleneSentinelSEOSATSkyMapperSkySatSLOANSMART1SOFIA
SOHOSolarOrbiterSpecialSPECULOOSSPIDERSpitzerSPOTSPTSSOTStardustSTELLASubaruSwiftTAUVEXTCS
TD1TerraTESSTIROS-NTJOTNGTNOTNTTopHatTRMMTYCHOUK-DMCUKIRTVATTVenusExpress
VikingVoyagerWASPWFIRSTWHTWISEWIYNWMAPWorldViewXMMZiYuan

WFIRST :Wide Field Infrared Survey Telescope (WFIRST) is the old name of the Roman Space Telescope. Please, see the Roman section.
WFIRST/WFI :The wide field instrument provides the Wide Field imaging and slitless spectroscopic capabilities required to perform the Dark Energy, Exoplanet Microlensing, and NIR surveys.
These are the old curves (2019/05/31). Please, use the updated versions at Roman/WFIid:WFIRST/WFI.a
→ GaiaXPy base XML file. You can download here the GaiaXPy base XML file for the full WFIRST/WFI filter set. Please, take a look to the GaiaXPy web page and additional documentation for more information.

WFIRST filters:

Filter ID λref λmean λeff λmin λmax Weff ZPν ZPλ Obs. Facility Instrument Description
WFIRST/WFI.R0626308.496454.136152.274438.177898.152128.303184.532.4e-9WFIRSTWFIWFIRST R062 filter
WFIRST/WFI.Z0878679.098748.498639.177160.0310144.481948.462321.429.24e-10WFIRSTWFIWFIRST Z087 filter
WFIRST/WFI.Y10610559.9210645.8710451.478761.7712386.552487.481993.615.36e-10WFIRSTWFIWFIRST Y106 filter
WFIRST/WFI.J12912890.1012995.7012746.2510726.9715087.132987.541485.652.68e-10WFIRSTWFIWFIRST J129 filter
WFIRST/WFI.Prism12434.9313543.2611144.747203.4218691.527299.031705.313.31e-10WFIRSTWFIWFIRST Prism
WFIRST/WFI.Grism14291.8315062.9813273.198921.7320490.348674.781374.002.02e-10WFIRSTWFIWFIRST Grism
WFIRST/WFI.W14614358.6115381.9612989.038903.8920692.977625.081410.572.05e-10WFIRSTWFIWFIRST W146 filter
WFIRST/WFI.H15815754.7815882.9615580.5613152.6918385.383507.571089.501.32e-10WFIRSTWFIWFIRST H158 filter
WFIRST/WFI.F18418404.8818477.7018302.1816044.2920692.972965.89854.917.57e-11WFIRSTWFIWFIRST F184 filter
 

Filter Plots (using a common λ range)

(Plot them zoomed to their own λ range)

© SVO,   (SVO Privacy Policy),   10970 filters available,   Last update: 2023-06-19
 
If your research benefits from the use of the SVO Filter Profile Service, we would appreciate if you could include the following acknowledgement in your publication:

This research has made use of the SVO Filter Profile Service "Carlos Rodrigo", funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00

and we would appreciate if you could include the following references in your publication: