LETGS

E384056

LETGS is a high-resolution X-ray grating spectrometer aboard NASA’s Chandra X-ray Observatory used to disperse and analyze X-ray emissions from cosmic sources.

All labels observed (1)

Label Occurrences
LETGS canonical 2

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf X-ray grating spectrometer
scientific instrument
acronymFor Low Energy Transmission Grating Spectrometer
alternativeName Chandra LETG/HRC-S configuration
configuration Low Energy Transmission Grating Spectrometer
surface form: Low Energy Transmission Grating plus HRC-S
dataProduct high-resolution X-ray spectra
line-resolved spectra of astrophysical sources
designedFor analyzing X-ray emissions from cosmic sources
dispersing X-ray photons by wavelength
high-resolution X-ray spectroscopy
developedBy Smithsonian Astrophysical Observatory
developedFor Marshall Space Flight Center
surface form: NASA Marshall Space Flight Center
enables diagnostics of hot astrophysical plasmas
measurement of Doppler shifts in X-ray lines
measurement of line broadening in X-ray spectra
energyRange soft X-ray band
fullName Low Energy Transmission Grating Spectrometer
hostAgency NASA
hostLaunchDate 1999-07-23
hostMission Chandra X-ray Observatory
launchVehicleOfHost STS-93
surface form: Space Shuttle Columbia STS-93
locatedOn Chandra X-ray Observatory
mountedAt Chandra High Resolution Mirror Assembly focal plane
observatoryProgram Great Observatories program
surface form: NASA Great Observatories program
observatoryType space-based X-ray observatory
observes Galactic sources
cosmic X-ray sources
extragalactic sources
operatedOn Chandra X-ray Observatory
operator NASA
partOf Chandra X-ray Observatory
surface form: Chandra X-ray Observatory payload
resolutionType high spectral resolution
scienceGoal measurement of elemental abundances in astrophysical plasmas
measurement of intergalactic medium absorption
measurement of interstellar absorption features
measurement of plasma temperatures and densities
study of X-ray binaries
study of active galactic nuclei
study of stellar coronae
study of supernova remnants
spectralRange approximately 0.07–10 keV
approximately 1.2–175 Å
status operational
uses HRC-S detector
High Resolution Camera-Spectroscopy (HRC-S)
Rowland circle geometry
transmission grating
transmission grating facets

How these facts were elicited

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.