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Space / Plasma physics / X-ray astronomy / X-ray telescopes / Lockman Hole / Ursa Major constellation / Chandra X-ray Observatory / X-ray / Power law / Astronomy / Observational astronomy / Electromagnetic radiation


Chandra Multi-wavelength Project (ChaMP). II. First Results of X-ray Source Properties D.-W. Kim, B. J. Wilkes, P. J. Green, R. A. Cameron, J. J. Drake, N. R. Evans, P. Freeman, T. J. Gaetz, H. Ghosh, F. R. Harnden, Jr.,
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Document Date: 2003-09-19 16:23:08


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City

Cambridge / /

Facility

Smithsonian Astrophysical Observatory / /

IndustryTerm

energy band / power-law emission model / follow-up optical imaging / power-law / energy bands / inter-chip / softest energy band / energy conversion factors / typical power-law spectrum / Optical imaging data / broken power law model / power law / power law fit / selected energy bands / homogeneous data products / break energy / /

MusicGroup

Colors / X-ray / ECF / Log / Energy / /

Organization

Smithsonian / /

Person

Chandra Deep Field-North / Chandra Deep / M. Karovska / V / Chandra Multi / F. R. Harnden / Jr. / /

Position

representative / Marshall / /

ProvinceOrState

Massachusetts / /

Technology

X-ray / FI chips / spectroscopy / /

URL

http /

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