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[PDF] Top 20 Soft x ray appearance potential spectra of La and Ce from 0 to 1400 eV

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Soft x ray appearance potential spectra of La and Ce from 0 to 1400 eV

Soft x ray appearance potential spectra of La and Ce from 0 to 1400 eV

... Soft-x-ray appearance potential spectra of La and Ce from 0 to 1400 eV Abstract The soft-x-ray appearance ... See full document

15

Soft X-ray absorption excess in gamma-ray burst afterglow spectra: Absorption by turbulent ISM

Soft X-ray absorption excess in gamma-ray burst afterglow spectra: Absorption by turbulent ISM

... the soft X-ray absorption for GRBs to estimate and explain the total X-ray absorbing column densi- ties that produce this ...the X-ray absorbing column for GRB ... See full document

10

Anatomy of the AGN in NGC 5548. IX. Photoionized emission features in the soft X-ray spectra

Anatomy of the AGN in NGC 5548. IX. Photoionized emission features in the soft X-ray spectra

... In reality, it is possible that turbulence dissipates within the NELR, in practice, it is difficult to model the emergent spec- trum. On one hand, the extra heating can be included via the external heating option in the ... See full document

11

X-ray spectra of the RIXOS source sample

X-ray spectra of the RIXOS source sample

... 6.4.1 Goodness of fit for a power law Fig. 15 shows the predicted minus observed total counts expressed in terms of the standard deviation for each spectral band for all the AGN. It is clear that for the majority of AGN ... See full document

24

Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer

Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer

... 3.1 Plasma search 3.1.1 Fiducial model We first constructed the spectral model for the entire energy band. The spectrum was fitted reasonably well with a single power-law model with an interstellar extinction, which we ... See full document

17

Solar Flare Composition and Thermodynamics from RESIK X-ray Spectra

Solar Flare Composition and Thermodynamics from RESIK X-ray Spectra

... solar soft X-ray spectra are essential for the diagnostics of hot plasmas associated with flares and active ...conditions, X-ray spectra can also be used to find the ... See full document

29

First Terrestrial Soft X-ray Auroral Observation by The Chandra X-ray Observatory

First Terrestrial Soft X-ray Auroral Observation by The Chandra X-ray Observatory

... electron spectra from ...the X-ray production. In some of the spectra such a hard tail can be seen, but as the flux level falls off rapidly at the high energies, we do not expect the ... See full document

17

Resonant Soft X Ray Inelastic Scattering and Soft X Ray Emission Study of the Electronic Structure of alpha MoO3

Resonant Soft X Ray Inelastic Scattering and Soft X Ray Emission Study of the Electronic Structure of alpha MoO3

... k-selective spectra collected in geometries A and B are particularly well resolved as compared to the other ori- ...away from the k-selective ...away from the k-selective features is due to the ... See full document

8

Discovery of a soft x-ray lag in the ultraluminous x-ray source NGC 1313 X-1.

Discovery of a soft x-ray lag in the ultraluminous x-ray source NGC 1313 X-1.

... Ultraluminous X-ray sources (ULXs) provide a unique opportunity to probe the geometry and energetics of super-Eddington ...1313 X-1 from a recent XMM–Newton campaign. The spectra can be ... See full document

8

Discovery of a soft X-ray lag in the ultraluminous X-ray source NGC 1313 X-1

Discovery of a soft X-ray lag in the ultraluminous X-ray source NGC 1313 X-1

... 3 RESULTS Like other ULXs, NGC 1313 X-1 shows a 0.3–10 keV spec- trum that is broadly described by two thermal components. We demonstrate this point in Fig. 1-left, where we show the unfolded 0.3-10 keV XMM-Newton ... See full document

7

Optimal binning of X-ray spectra and response matrix design

Optimal binning of X-ray spectra and response matrix design

... high-resolution spectra much more complex to handle than low-resolution spectra? The enhanced spectral resolution and sensitivity of the current high-resolution X-ray spectrometers require ... See full document

16

Correlations Between Variations in Solar EUV and Soft X-Ray Irradiance and Photoelectron Energy Spectra Observed on Mars and Earth

Correlations Between Variations in Solar EUV and Soft X-Ray Irradiance and Photoelectron Energy Spectra Observed on Mars and Earth

... electron spectra used must have a minimal solar wind electron ...photoemissions from spacecraft surfaces ...data from the MGS/ER are considered ...steps from 10 eV to 20 keV. The eight ... See full document

10

Al0.52In0.48P avalanche photodiodes for soft X-ray spectroscopy

Al0.52In0.48P avalanche photodiodes for soft X-ray spectroscopy

... information from raw X-ray spectra was converted into energy by using the noise peak and the detected ...keV X-ray peak as ... See full document

13

X-Ray Beam Characteristics And Radiation Dose Deposition To Soft Tissue From Fluoroscopic X-Ray Beams Incorporating Copper Filtration

X-Ray Beam Characteristics And Radiation Dose Deposition To Soft Tissue From Fluoroscopic X-Ray Beams Incorporating Copper Filtration

... entrance from fluoroscopic procedures has been reported by Jones et ...event from a fluoroscopic ...for potential deviations and, if necessary, beam quality ...the X-ray beam field size ... See full document

141

Spectra of pyroelectric X-ray generator

Spectra of pyroelectric X-ray generator

... of X-ray generator based on a pyroelectric crystal LiNbO 3 is ...radiation spectra from the X-ray generator are ...the spectra were performed at heating and cooling of the ... See full document

5

Calculation of x-ray spectra emerging from an x-ray tube. Part I. electron penetration characteristics in x-ray targets.

Calculation of x-ray spectra emerging from an x-ray tube. Part I. electron penetration characteristics in x-ray targets.

... there are x-ray tubes in use within healthcare that possess anodes made of elements that are not high-Z materials. The majority of such tubes are used in mammography. The tube potentials used in these cases ... See full document

32

Optical properties of TiCx (0 64≤x≤0 90) from 0 1 to 30 eV

Optical properties of TiCx (0 64≤x≤0 90) from 0 1 to 30 eV

... (0.64≤x≤0.90) from 0.1 to 30 eV Abstract The stoichiometry-dependent optical properties of bulk samples of TiCx have been determined for four samples in the range ...0.1-30 eV have been ... See full document

9

X-ray and optical studies of soft x-ray transients in M31

X-ray and optical studies of soft x-ray transients in M31

... This Chapter started with a theoretical discussion of the expected light curve behavior, and followed with the observational data (obtained from Chandra, XMM-Newton and Swift) for com- parison. The transients used ... See full document

136

X-ray spectra of the Fe-L complex

X-ray spectra of the Fe-L complex

... high-resolution X-ray ...data from 15 elliptical galaxies and galaxy clusters, we note that the new model gives systematically better fits than the current SPEX ...results from the current ... See full document

29

A method for normalization of X ray absorption spectra

A method for normalization of X ray absorption spectra

... Keywords: X-ray absorption spectroscopy; normalization; ...Introduction X-ray absorption spectroscopy (XAS) is often divided into extended X-ray absorption fine structure (EXAFS) ... See full document

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