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EUD's X-ray Astrophysics Lab

X-ray Astrophysics Missions & Programs

Current Missions

artist's image of RXTE photo of the PCA The Rossi X-ray Timing Explorer (RXTE) was launched in 1995 and features unprecedented time resolution in combination with moderate spectral resolution to explore the variability of X-ray sources. Time scales from microseconds to months are covered in an instantaneous spectral range from 2 to 250 keV. The Proportional Counter Array (PCA) was developed in the EUD. The RXTE project scientist is Jean Swank. The RXTE Guest Observer Facility is in the EUD and the data are archived in the HEASARC.
image of the XRS image of the XRT The Suzaku (formerly Astro-E2) mission is an international collaboration Instruments include the X-ray Imaging Spectrometer (XIS), the Hard X-ray Detector (HXD), and the X-Ray Spectrometer (XRS), an X-ray micro-calorimeter, developed in the EUD. Suzaku's X-ray Telescopes (XRT) were built here in our mirror lab. These telescopes contain about 1400 specially shaped mirrors, nested in about 170 layers. These foils are positioned in the telescope so they focus X-rays at the XIS and XRS instruments and are deliberately designed for maximum collecting area per weight while sacrificing spatial resolution. The XRS team is led by Richard Kelley (PI) and the XRT team is led by Peter Serlemisos.
Other current missions:
XMM-Newton

Future Missions/Programs

artist's conception of Constellation-X array in space The Constellation-X Observatory is a combination of several X-ray telescopes working in unison to generate the observing power of one giant telescope. The current design calls for four identical Spectroscopy X-ray Telescopes (SXTs) and one or two Hard X-ray Telescopes (HXTs) on a single satellite. With the Observatory, scientists will investigate black holes, Einstein's Theory of General Relativity, galaxy formation, the evolution of the Universe on the largest scales, the recycling of matter and energy, and the nature of dark matter and dark energy. The Con-X Project Scientist is Nick White with Deputy Project Scientist Ann Hornschemeier and the GSFC Mission Scientist Robert Petre.
Other future missions include the Beyond Einstein program, Generation-X: An Ultra High Throughput Early Universe X-ray Imager, and MAXIM: Micro-Arcsecond X-ray Imaging Mission (Black Hole Imager)

Past Programs

Ariel V, ASCA, the Broad Band X-ray Telescope (BBXRT), the Calorimeter Sounding Rocket, HEAO-1 (1st High Energy Astrophysics Observatory), HEAO-2 (Einstein Observatory) (2nd High Energy Astrophysics Observatory), OSO-8, and ROSAT. See the HEASARC's list of missions.