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},
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},
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}
},
{
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},
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},
{
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},
{
"orgName": "Goddard Institute for Space Studies (GISS)",
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},
{
"orgName": "Mesoscale Atmospheric Processes Laboratory",
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},
{
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}
},
{
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}
},
{
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}
},
{
"orgName": "Ocean Ecology Laboratory",
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}
},
{
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}
},
{
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}
},
{
"orgName": "Terrestrial Information Systems Laboratory",
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}
},
{
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},
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},
{
"orgName": "High Energy Astrophysics Science Archive Research Center (HEASARC) Office",
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},
{
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}
},
{
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}
},
{
"orgName": "Astroparticle Physics Laboratory",
"orgShortName": "Astroparticle Physics Laboratory",
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"router": {
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"secondary": "astroparticles"
}
},
{
"orgName": "X-ray Astrophysics Laboratory",
"orgShortName": "X-ray Astrophysics Laboratory",
"orgCode": "662",
"parentOrgCode": "660",
"router": {
"primary": "astrophysics",
"secondary": "xray"
}
},
{
"orgName": "Gravitational Astrophysics Laboratory",
"orgShortName": "Gravitational Astrophysics Laboratory",
"orgCode": "663",
"parentOrgCode": "660",
"router": {
"primary": "astrophysics",
"secondary": "gravity"
}
},
{
"orgName": "Observational Cosmology Laboratory",
"orgShortName": "Observational Cosmology Laboratory",
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"router": {
"primary": "astrophysics",
"secondary": "cosmology"
}
},
{
"orgName": "Exoplanets and Stellar Astrophysics Laboratory",
"orgShortName": "Exoplanets and Stellar Astrophysics Laboratory",
"orgCode": "667",
"parentOrgCode": "660",
"router": {
"primary": "astrophysics",
"secondary": "exoplanets"
}
},
{
"orgName": "Heliophysics Science Division",
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"parentOrgCode": "600",
"router": {
"primary": "heliophysics",
"secondary": null
}
},
{
"orgName": "Solar Physics Laboratory",
"orgShortName": "Solar Physics Laboratory",
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"parentOrgCode": "670",
"router": {
"primary": "heliophysics",
"secondary": "solar"
}
},
{
"orgName": "Heliospheric Physics Laboratory ",
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"secondary": "heliospheric"
}
},
{
"orgName": "Geospace Physics Laboratory",
"orgShortName": "Geospace Physics Laboratory",
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"parentOrgCode": "670",
"router": {
"primary": "heliophysics",
"secondary": "geospace"
}
},
{
"orgName": "Space Weather Laboratory",
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"primary": "heliophysics",
"secondary": "spaceweather"
}
},
{
"orgName": "Ionospheric, Thermospheric, Mesospheric (ITM) Physics Laboratory",
"orgShortName": "ITM Physics Laboratory",
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"parentOrgCode": "670",
"router": {
"primary": "heliophysics",
"secondary": "itmphysics"
}
},
{
"orgName": "Solar System Exploration Division",
"orgShortName": "Solar System Exploration Division",
"orgCode": "690",
"parentOrgCode": "600",
"router": {
"primary": "solarsystem",
"secondary": null
}
},
{
"orgName": "Solar System Exploration Data Services Office",
"orgShortName": "Solar System Exploration Data Services Office",
"orgCode": "690.1",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "dataarchives"
}
},
{
"orgName": "Astrochemistry Laboratory",
"orgShortName": "Astrochemistry Laboratory",
"orgCode": "691",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "astrochemistry"
}
},
{
"orgName": "Planetary Systems Lab",
"orgShortName": "Planetary Systems Laboratory",
"orgCode": "693",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "planetarysystems"
}
},
{
"orgName": "Planetary Magnetospheres Lab",
"orgShortName": "Planetary Magnetospheres Laboratory",
"orgCode": "695",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "magnetospheres"
}
},
{
"orgName": "Planetary Geology, Geophysics & Geochemistry Lab",
"orgShortName": "Planetary Geology, Geophysics & Geochemistry Lab",
"orgCode": "698",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "p3g"
}
},
{
"orgName": "Planetary Environments Laboratory ",
"orgShortName": "Planetary Environments Laboratory",
"orgCode": "699",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "atmosenvironments"
}
}
]
Operational
X-ray Multi-Mirror Mission (XMM-Newton)
The X-ray Multi-Mirror (XMM-Newton) mission is a joint project of the European Space Agency (ESA) and NASA. XMM-Newton is designed to observe high-energy X-rays emitted by exotic astronomical objects such as pulsars, black holes, and active galaxies. The observatory collects both images and spectra. This means it can measure the energy of the X-rays emitted by an astronomical object, which allows scientists to determine many of its physical characteristics. Besides having funded elements of the XMM-Newton instrument package, NASA also provides the NASA Guest Observer Facility (GOF) for XMM Newton at Goddard Space Flight Center. ESA launched the mission in December 1999.
Organization
The X-ray Multi-Mirror (XMM-Newton) mission is a joint project of the European Space Agency (ESA) and NASA. XMM-Newton is designed to observe high-energy X-rays emitted by exotic astronomical objects such as pulsars, black holes, and active galaxies. The observatory collects both images and spectra. This means it can measure the energy of the X-rays emitted by an astronomical object, which allows scientists to determine many of its physical characteristics. Besides having funded elements of the XMM-Newton instrument package, NASA also provides the NASA Guest Observer Facility (GOF) for XMM Newton at Goddard Space Flight Center. ESA launched the mission in December 1999.
Related Publications
2025. "The XMM Cluster Survey: automating the estimation of hydrostatic mass for large samples of galaxy clusters – I. Methodology, validation, and application to the SDSSRM-XCS sample.", Monthly Notices of the Royal Astronomical Society, 537 (2): 1404-1429 [10.1093/mnras/staf007] [Journal Article/Letter]
2022. "The XMM Cluster Survey: an independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies.", Monthly Notices of the Royal Astronomical Society, 517 (1): 657-674 [10.1093/mnras/stac2463] [Journal Article/Letter]