Energy Spectra of the Soft X-ray Diffuse Emission in Fourteen Fields Observed with Suzaku (2009)
Yoshino, T., Mitsuda, K., Yamasaki, N. Y., Takei, Y., Hagihara, T., Masui, K., ...
The soft diffuse X-ray emission of twelve fields observed with Suzaku are presented together with two additional fields from previous analyses. All have galactic longitudes 65 deg < l < 295 deg to...
The Nature of Unresolved Soft X-ray Emission from the Galactic Disk (2008)
Masui, K., Mitsuda, K., Yamasaki, N. Y., Takei, Y., Kimura, S., Yoshino, T., ...
Although about 40% of the soft X-ray background emission in 0.4 to 1 keV range has extragalactic origins and thus is totally blocked by the Galactic absorption in midplane directions, it decreases at...
X-ray and UV spectroscopy of Galactic diffuse hot gas along the LMC X--3 sight line (2008)
Yao, Y., Wang, Q. D., Hagihara, T., Mitsuda, K., McCammon, D., Yamasaki, N. Y.
We present Suzaku spectra of X-ray emission in the fields just off the LMC X-3 sight line. OVII, OVIII, and NeIX emission lines are clearly detected, suggesting the presence of an optically thin...
Spectrum-Roentgen-Gamma astrophysical mission (2008)
Pavlinsky, M., Sunyaev, R., Churazov, E., Gilfanov, M., Vikhlinin, A., Hasinger, G., ...
The Spektr-RG X-ray calorimeter (2008)
Den Herder, J. W., Kelley, R., McCammon, D., Mitsuda, K., Aarts, H., Van Baren, C., ...
Monfardini, A., Arnaboldi, C., Brofferio, C., Capelli, S., Capozzi, F., Cremonesi, O., ...
Neutrino oscillation experiments have proved that neutrinos are massive particles, but can't determine their absolute mass scale. Therefore the neutrino mass is still an open question in elementary...
A Microcalorimeter and Bolometer Model (2003)
The standard non-equilibrium theory of noise in ideal bolometers and microcalorimeters fails to predict the performance of real devices due to additional effects that become important at low...
McCammon, D., Almy, R., Apodaca, E., Tiest, W. Bergmann, Cui, W., Deiker, S., ...
A high spectral resolution observation of the diffuse X-ray background in the 60 - 1000 eV energy range has been made using an array of thirty-six 1 mm^2 micro-calorimeters flown on a sounding...