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Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy. Keith Arnaud NASA Goddard University of Maryland. Practical X-ray spectroscopy. Most X-ray spectra are of moderate or low resolution (eg Chandra ACIS or XMM-Newton EPIC). However, the spectra generally cover a bandpass of more than 1.5 decades in energy.

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482 views • 37 slides
Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy. Keith Arnaud NASA Goddard University of Maryland. Practical X-ray spectroscopy. Most X-ray spectra are of moderate or low resolution (eg Chandra ACIS or XMM-Newton EPIC). However, the spectra generally cover a bandpass of more than 1.5 decades in energy.

★ ★ ★ ★ ★

375 views • 37 slides
Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy. Keith Arnaud NASA Goddard University of Maryland. Practical X-ray spectroscopy. Most X-ray spectra are of moderate or low resolution (eg Chandra ACIS or XMM-Newton EPIC). However, the spectra generally cover a bandpass of more than 1.5 decades in energy.

★ ★ ★ ★ ★

380 views • 37 slides
Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy. Keith Arnaud NASA Goddard University of Maryland. Practical X-ray spectroscopy. Most X-ray spectra are of moderate or low resolution (eg Chandra ACIS or XMM-Newton EPIC). However, the spectra generally cover a bandpass of more than 1.5 decades in energy.

★ ★ ★ ★ ★

300 views • 29 slides
Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy

Lower resolution X-ray spectroscopy. Keith Arnaud NASA/GSFC & UMCP. Practical X-ray spectroscopy. Most X-ray spectra are of moderate or low resolution (eg Chandra ACIS or XMM-Newton EPIC). However, the spectra generally cover a bandpass of more than 1.5 decades in energy.

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268 views • 26 slides
Bkg modeling for hot medium z Clusters

Bkg modeling for hot medium z Clusters

Bkg modeling for hot medium z Clusters. Alberto Leccardi Silvano Molendi. Focus. Bkg treatment for: Low SB Extended emission NOT filling FOV Hard Band 1.5,2.0-10 keV. The Bkg components. 2 Components dominate NXB from high E particles 2) Soft Protons

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296 views • 20 slides
TROPOMI NO 2 Prototype Algorithm

TROPOMI NO 2 Prototype Algorithm

TROPOMI NO 2 Prototype Algorithm. Folkert Boersma, Jos van Geffen, Bram Maasakkers, Maarten Sneep, and Pepijn Veefkind. 1st S5P-TROPOMI Verification Workshop, DLR, De Bilt, 15-16 April 2013s. Algorithm overview. 3-step approach

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337 views • 18 slides

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