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The XMM-Newton Optical/UV Monitor Telescope
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The XMM-OM instrument extends the spectral coverage of the XMM-Newton observatory into the ultraviolet and optical range. It provides imaging and time-resolved data on targets simultaneously with observations in the EPIC and RGS. It also has the ability to track stars in its field of view, thus providing an improved post-facto aspect solution for the spacecraft. An overview of the XMM-OM and its operation is given, together with current information on the performance of the instrument.
Forward citations
Cited by 7 Pith papers
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V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories
V407 Vul is a hierarchical triple: a 569-s AM CVn white-dwarf binary bound to a G-type tertiary at ~120 AU, the first 'verification triple' for LISA.
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Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve
XRISM/Resolve reveals a narrow, blueshifted neutral Fe Kα line (EW ≈ 9 eV, v_out ≈ 2700 km/s) in quasar PDS 456, likely from the outer Broad Line Region at the high-luminosity end of the X-ray Baldwin effect.
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First detection of ultra-fast outflows in a quiescent galaxy
First detection of an ultra-fast outflow (v≈0.07c) in a quiescent galaxy quenched ~9 Gyr ago, suggesting AGN winds can maintain quiescence independent of global star formation.
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The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654
X-ray emission lines and a broad iron feature emerged in changing-look AGN 1ES 1927+654 concurrently with radio-jet formation and declining ionized outflows from 2022 to 2025.
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Structured ionized winds shooting out from a quasar at relativistic speeds
XRISM's Resolve instrument resolves the ultra-fast outflow of quasar PDS 456 into five discrete velocity components, implying a clumpy wind with a mass outflow rate of 60-170 solar masses per year and kinetic power ab...
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Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds
Variable column density and covering factor of three ionized absorbers in clumpy disk winds explain the X-ray variability in I Zw 1 with stable corona.
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SAS in ESA Datalabs: A New Platform for XMM-Newton Analysis
The XMM-SAS Datalab runs XMM-Newton's Science Analysis System in a collaborative cloud JupyterLab environment, and it reproduces a published Vela X-1 analysis with a mean spectral deviation of about 0.18%.
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