Filter Profile Service
A repository of Filter information for the VO
Astronomy (7450)Planetary science (616)Earth Obs. (2439)

XMM :The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton)
XMM/OM :The Optical/UV Monitor Telescope (XMM-OM)

XMM/OM.UVW2_filter2041.692066.572042.121790.052891.84435.49738.915.31e-9XMMOMXMM OM UVW2 filter transmission only
XMM/OM.UVW22135.602175.322144.891799.803246.22498.34766.354.99e-9XMMOMXMM OM UVW2 filter full effective area
XMM/OM.UVM2_filter2284.662303.832283.801820.842919.17461.94773.904.45e-9XMMOMXMM OM UVM2 filter transmission only
XMM/OM.UVM22326.922347.182327.621883.782994.45478.06781.144.32e-9XMMOMXMM OM UVM2 filter full effective area
XMM/OM.UVW1_filter2895.372947.352934.341795.004033.62743.981044.793.64e-9XMMOMXMM OM UVW1 filter transmission only
XMM/OM.UVW12931.312978.822970.972188.514060.42795.281065.003.62e-9XMMOMXMM OM UVW1 filter full effective area
Filter Description

Filter ID (?) :XMM/OM.UVW1
Description (?) :XMM OM UVW1 filter full effective area
Phot.System (?) :XMM
Detector Type (?) :Photon counter
Band Name (?) :UVW1
Obs. Facility (?) :XMM
Instrument (?) :OM
Comments (?) :Filter effective area including the entire telescope response based on inflight measurements.

Take into account that there is a time-dependent, and filter-dependent decline in sensitivity for the OM since launch (which reaches as much as ~20% (in 2019) in the V and furthest UV bands), and that the filter effective areas provided reflect the case at approximately mission start, so any computation of expected output in the OM at a given epoch after mission start, should take these degradation factors into account. The current document describing the degradation is available at

Mathematical properties

Property Calculated Specified Unit
λref (?) : 2931.31 ------- (Angstrom)
λmean (?) : 2978.82 ------- (Angstrom)
λcen (?) : 2949.83 ------- (Angstrom)
λeff (?) : 2970.97 ------- (Angstrom)
λpeak (?) : 2699.71 ------- (Angstrom)
λpivot (?) : 2931.31 ------- (Angstrom)
λphot (?) : 3007.37 ------- (Angstrom)
λmin (?) : 2188.51 ------- (Angstrom)
λmax (?) : 4060.42 ------- (Angstrom)
Weff (?) : 795.28 ------- (Angstrom)
FWHM (?) : 784.23 ------- (Angstrom)
Af/AV (?) : 1.84 ------- ()
Fsun (?) : 50.76 ------- (erg/cm2/s/A)

Effective area

Data file: ascii, VOTable

Reference for filter response: XMM-Newton Users handbook

Transmission components: Filter + Instrument + Atmosphere

Calibration properties

Vega System
PropertySpecified Calculated Unit
Zero Point (?) : ------- 3.6172e-9(erg/cm2/s/A)
  ------- 1065.00(Jy)
ZP Type (?) : Pogson
PhotCal ID (?) : XMM/OM.UVW1/Vega

AB System
PropertySpecified Calculated Unit
Zero Point (?) : ------- 1.23325e-8(erg/cm2/s/A)
  ------- 3631.00(Jy)
ZP Type (?) : Pogson
PhotCal ID (?) : XMM/OM.UVW1/AB

ST System
PropertySpecified Calculated Unit
Zero Point (?) : ------- 3.631e-9(erg/cm2/s/A)
  ------- 1069.06(Jy)
ZP Type (?) : Pogson
PhotCal ID (?) : XMM/OM.UVW1/ST

Filter added: 2019-03-29 10:44:11
Last update: 2020-12-10 16:34:35
XMM/OM.U_filter3465.513488.823515.743021.723948.39675.131480.543.59e-9XMMOMXMM OM U filter transmission only
XMM/OM.U3477.013503.233534.623020.384781.62651.061505.973.61e-9XMMOMXMM OM U filter full effective area
XMM/OM.B4337.124365.394332.413718.924963.56926.364056.726.48e-9XMMOMXMM OM B filter full effective area
XMM/OM.B_filter4368.974397.824361.933729.134969.38910.234055.036.39e-9XMMOMXMM OM B filter transmission only
XMM/OM.V5424.665437.595412.084929.135957.95666.403637.253.72e-9XMMOMXMM OM V filter full effective area
XMM/OM.V_filter5450.475463.445437.804942.975976.65699.563620.693.67e-9XMMOMXMM OM V filter transmission only

Filter Plots (using a common λ range)

(Plot them zoomed to their own λ range)

© SVO,   10501 filters available,   Last update: 2021-10-25
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 ( supported from the Spanish MINECO through grant AYA2017-84089

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