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26 April 2024 |
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A High Spectral Resolution Observation of the Soft X-ray Diffuse Background with Thermal Detectors | D. McCammon
; R. Almy
; E. Apodaca
; W. Bergmann Tiest
; W. Cui
; S. Deiker
; M. Galeazzi
; M. Juda
; A. Lesser
; T. Mihara
; J. P. Morgenthaler
; W. T. Sanders
; J. Zhang
; E. Figueroa-Feliciano
; R. L. Kelley
; S. H. Moseley
; R. F. Mushotzky
; F. S. Porter
; C. K. Stahle
; A. E. Szymkowiak
; | Date: |
2 May 2002 | Journal: | Astrophys.J. 576 (2002) 188-203 | Subject: | astro-ph | Affiliation: | Physics Department, University of Wisconsin), E. Figueroa-Feliciano, R. L. Kelley, S. H. Moseley, R. F. Mushotzky, F. S. Porter, C. K. Stahle, and A. E. Szymkowiak (NASA Goddard Space Flight Center | Abstract: | 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 rocket. Detector energy resolution ranged from 5-12 eV FWHM, and a composite spectrum of ~ 1 steradian of the background centered at l = 90, b = +60 was obtained with a net resolution of ~ 9 eV. The target area includes bright 1/4 keV regions, but avoids Loop I and the North Polar Spur. Lines of C VI, O VII, and O VIII are clearly detected with intensities of 5.4 +/- 2.3, 4.8 +/- 0.8, and 1.6 +/- 0.4 photons cm^-2 s^-1 sr^-1, respectively. The oxygen lines alone account for a majority of the diffuse background observed in the ROSAT R4 band that is not due to resolved extragalactic discrete sources. We also have a positive detection of the Fe-M line complex near 70 eV at an intensity consistent with previous upper limits that indicate substantial gas phase depletion of iron. We include a detailed description of the instrument and its detectors. | Source: | arXiv, astro-ph/0205012 | Services: | Forum | Review | PDF | Favorites |
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