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{
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},
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},
{
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},
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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": "X-ray Astrophysics Laboratory",
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},
{
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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": "Geospace Physics Laboratory",
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}
},
{
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}
},
{
"orgName": "Ionospheric, Thermospheric, Mesospheric (ITM) Physics Laboratory",
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}
},
{
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}
},
{
"orgName": "Solar System Exploration Data Services Office",
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"secondary": "dataarchives"
}
},
{
"orgName": "Astrochemistry Laboratory",
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"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "astrochemistry"
}
},
{
"orgName": "Planetary Systems Lab",
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}
},
{
"orgName": "Planetary Magnetospheres Lab",
"orgShortName": "Planetary Magnetospheres Laboratory",
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"router": {
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"secondary": "magnetospheres"
}
},
{
"orgName": "Planetary Geology, Geophysics & Geochemistry Lab",
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"orgCode": "698",
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"router": {
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}
},
{
"orgName": "Planetary Environments Laboratory ",
"orgShortName": "Planetary Environments Laboratory",
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"router": {
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"secondary": "atmosenvironments"
}
}
]
Advanced Telescope for High-ENergy Astrophysics (ATHENA)
ATHENA is an ESA large mission that is slated to launch in the early 2030s. The main science goals of ATHENA address the questions:
* How and why does ordinary matter assemble into the galaxies and galaxy clusters that we see today?
* How do black holes grow and influence their surroundings?
These will be accomplished thanks to a large X-ray mirror with a 5” point spread function that pivots to focus on onto one of two instruments: the X-ray Integral Field Unit (X-IFU) which is an X-ray calorimeter with ~ 2 eV spectral resolution and the Wide-Field Imager (WFI) which is a large field of view (40’ x 40’) active pixel sensor.
ATHENA is an ESA large mission that is slated to launch in the early 2030s. The main science goals of ATHENA address the questions:
* How and why does ordinary matter assemble into the galaxies and galaxy clusters that we see today?
* How do black holes grow and influence their surroundings?
These will be accomplished thanks to a large X-ray mirror with a 5” point spread function that pivots to focus on onto one of two instruments: the X-ray Integral Field Unit (X-IFU) which is an X-ray calorimeter with ~ 2 eV spectral resolution and the Wide-Field Imager (WFI) which is a large field of view (40’ x 40’) active pixel sensor.
Related Publications
2022. "New Measurement Resolves Key Astrophysical Fe XVII Oscillator Strength Problem.", Physical Review Letters, 129 (24): 245001 [10.1103/physrevlett.129.245001] [Journal Article/Letter]
2022. "X-ray spectra of the Fe-L complex. III. Systematic uncertainties in atomic data.", Astronomy & Astrophysics, 664 A62 [10.1051/0004-6361/202039943] [Journal Article/Letter]
2022. "X-Ray Photoabsorption of Density-sensitive Metastable States in Ne vii, Fe xxii, and Fe xxiii.", The Astrophysical Journal, 941 (2): 188 [10.3847/1538-4357/ac9c00] [Journal Article/Letter]