TheAdvanced Satellite for Cosmology and Astrophysics (ASCA, formerly namedASTRO-D) was the fourth cosmic X-ray astronomy mission byJAXA, and the second for which theUnited States provided part of the scientific payload. The satellite was successfully launched on 20 February 1993. The first eight months of the ASCA mission were devoted to performance verification. Having established the quality of performance of all ASCA's instruments, the spacecraft provided science observations for the remainder of the mission. In this phase the observing program was open toastronomers based at Japanese and U.S. institutions, as well as those located in member states of theEuropean Space Agency.[3][4]
ASCA carried four large-areaX-ray telescopes. At the focus of two of the telescopes is agas imaging spectrometer (GIS), while asolid-state imaging spectrometer (SIS) is at the focus of the other two.[3][4] The GIS is a gas-imaging scintillation proportional counter and is based on the GSPC that flew on the second Japanese X-ray astronomy mission,Tenma. The two identicalcharge-coupled device (CCD) cameras were provided for the two SISs by a hardware team from MIT, Osaka University and ISAS.
The ASCA was launched by ISAS (Institute of Space and Astronautical Sciences), Japan.
The sensitivity of ASCA's instruments allowed for the first detailed, broad-band spectra of distant quasars to be derived. In addition, ASCA's suite of instruments provided the best opportunity at the time for identifying the sources whose combined emission makes up the cosmic X-ray background.[3][5]
It performed over 3000 observations, and produced over 1000 publications in refereed journals so far. The ASCA archive contains significant amounts of data for future analyses. Furthermore, the mission is termed highly successful when reflecting on what scientists in many counties have accomplished using ASCA data up to this time.
The U.S. contributed significantly to ASCA's scientific payloads. In return, 40% of ASCA observing time was made available to U.S. scientists. (ISAS also opened up 10% of the time to ESA scientists as a good-will gesture.) In addition, all ASCA data enter the public domain after a suitable period (1 year for U.S. data, 18 months for Japanese data) and become available to scientists worldwide. The design of ASCA was optimized for X-ray spectroscopy; thus it complementedROSAT (optimized for X-ray imaging) andRXTE (optimized for timing studies). Finally, ASCA results cover almost the entire range of objects, from nearby stars to the most distant objects in the universe.[6]
The mission operated successfully for over 7 years until attitude control was lost on 14 July 2000 during ageomagnetic storm, after which no scientific observations were performed. ASCA reentered the atmosphere on 2 March 2001 after more than 8 years in orbit.
The primary responsibility of the U.S. ASCA GOF was to enable U.S. astronomers to make the best use of the ASCA mission, in close collaboration with the Japanese ASCA team.[7]
^abc"ASCA".NASA Science Missions. NASA. Archived fromthe original on 7 October 2011.
^abTanaka, Yasuo; Inoue, Hajime; Holt, Stephen S. (June 1994). "The X-ray astronomy satellite ASCA".Publications of the Astronomical Society of Japan.46 (3):L37 –L41.Bibcode:1994PASJ...46L..37T.doi:10.1093/pasj/46.3.37.
^Tsusaka, Yoshiyuki; Suzuki, Hisanori; Yamashita, Koujun; Kunieda, Hideyo; Tawara, Yuzuru; et al. (August 1995). "Characterization of the Advanced Satellite for Cosmology and Astrophysics X-ray telescope: Preflight calibration and ray tracing".Applied Optics.34 (22):4848–4856.Bibcode:1995ApOpt..34.4848T.doi:10.1364/AO.34.004848.PMID21052325.
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