ライフサイエンスコーパス: hard X-ray

1 lecular systems irradiated by high-intensity hard x-rays.

2 g of materials to light sources for soft and hard x-rays.

3 ) sensitivity, because the Raman method used hard X-rays.

4 rovide an intense, highly coherent source of hard x-rays.

5 The Galactic plane is a strong emitter of hard x-rays (2 to 10 kiloelectron volts), and the emissi

6 t by using both soft X-rays (100-800 eV) and hard X-rays (2000-7000 eV) from two different synchrotro

7 Electron-hole separation following hard X-ray absorption during diffraction analysis of sof

8 se limitations and obviates the need to make hard x-ray absorption gratings of sub-micron periods.

9 In situ hard X-ray absorption spectroscopy (XAS) at metal K-edge

10 rption spectroscopy (XAS), but involves only hard X-rays and can therefore be used to get high-resolu

11 Using hard X-ray angle-resolved photoemission (HARPES) at 3.2

12 Hard X-rays are produced through the process of inverse

13 We present experimental data for hard X-ray ARPES (HARPES) at energies of 3.2 and 6.0 keV

14 trate the presence of a cosmic background of hard X-rays at that early time.

15 rces account for at least 75 per cent of the hard X-ray background.

16 , is reported here for the first time in the hard X-ray band ( 20-160 keV).

17 en demonstrated, and the practical limit for hard x-ray beam size, the limit to trace-element sensiti

18 Here we demonstrate focusing a hard X-ray beam to an 8 nm focus using a volume zone pla

19 We show how bright, tabletop, fully coherent hard X-ray beams can be generated through nonlinear upco

20 We describe how submicrometer hard x-ray beams with the ability to penetrate tens to h

21 Here we report the presence of a distinct hard-X-ray component within the central 4 x 8 parsecs, a

22 nt in the reflection spectrum created by the hard-X-ray continuum irradiating dense accreting matter.

23 Using state-of-the-art time-resolved hard x-ray diffraction microscopy, we directly visualize

24 erous short-duration (about 0.1 s) bursts of hard X-rays during sporadic active periods.

25 The hard X-ray emission from RS Ophiuchi early in the erupti

26 The Galactic ridge hard x-ray emission is diffuse, which indicates omnipres

27 Here, we present a new method for bright hard x-ray emission via ionization injection from the K-

28 ferent times corresponding to peaks of flare hard X-ray emission.

29 trashort (< 50 fs) 9 keV X-ray pulses from a hard X-ray free electron laser, namely the Linac Coheren

30 The advent of hard x-ray free electron lasers (XFELs) capable of produ

31 The recent advent of hard x-ray free electron lasers (XFELs) opens new areas

32 Hard X-ray free electron lasers allow for the first time

33 The advent of hard x-ray free-electron lasers (XFELs) has opened up a

34 with matter has begun with the start-up of a hard-X-ray free-electron laser, the Linac Coherent Light

35 We employ the high-speed synchrotron hard X-ray imaging and diffraction techniques to monitor

36 Here we show that the integral hard-X-ray-induced photoemission yield is modulated by t

37 of chemical reactions by nanomaterials under hard X-ray irradiation.

38 xperiments using either soft or less-intense hard X-rays, it is thought that the induced charge and a

39 ectron microscopy (cryo-TEM) and synchrotron hard X-ray microprobe (SHXM) data sets to precisely dete

40 We used a novel hard x-ray microprobe with suboptical spatial resolution

41 We developed a scanning hard x-ray microscope using a new class of x-ray nano-fo

42 Here, using hard X-ray microscopy--which offers nanoscale resolution

43 Synchrotron hard X-ray microtomography experiments on symmetric lith

44 Observations of diffuse hard-X-ray (more than 10 kiloelectronvolts) emission in

45 st time, implementation of synchrotron-based hard X-ray nanotomography in Al-Cu alloys to measure kin

46 odium-ion batteries with in situ synchrotron hard X-ray nanotomography.

47 Hard X-ray phase-contrast imaging characterizes the elec

48 itially insulating films of WO3 Here, we use hard X-ray photoelectron spectroscopy and spectroscopic

49 d magnetic circular dichroism, combined with hard X-ray photoelectron spectroscopy, we derived a comp

50 /SrTiO3 (001) heterointerface using soft and hard x-ray photoemission spectroscopy in conjunction wit

51 Here, we employed state-of-the-art hard x-ray photoemission spectroscopy with judiciously c

52 ing of the oxide-semiconductor interface via hard x-ray photoemission spectroscopy, we show how to sy

53 Going to hard X-ray photon energies and thus larger electron inel

54 We detected at least 36 new hard x-ray point sources in addition to strong diffuse e

55 A hard X-ray probe such as X-ray Raman scattering (XRS) ca

56 Femtosecond hard x-ray pulses emitted by the Linac Coherent Light So

57 report the generation of mJ-level two-colour hard X-ray pulses of few femtoseconds duration with an X

58 biological systems and complex materials use hard X-ray pulses with extremely high peak intensities (

59 noble gas clusters exposed to high-intensity hard-x-ray pulses at ~5 keV.

60 ed in nuclear transitions) or, equivalently, hard X-ray radiation (the term used when the radiation i

61 Through soft X-ray absorption spectroscopy, hard X-ray Raman scattering, and theoretical simulations

62 Temperature-dependent hard X-ray reflectivity, small- and wide-angle X-ray sca

63 scading following photoabsorption, as in the hard x-ray regime there is no direct energy transfer fro

64 lasma formation mechanism is specific to the hard-x-ray regime and may, thus, also be important for X

65 d frequency upconversion can extend into the hard X-ray region of the spectrum.

66 The combination of the hard x-ray's superior penetration power, high sensitivit

67 port a systematic multi-wavelength survey of hard-X-ray-selected black holes that reveals that radiat

68 Here, we report the discovery of a hard X-ray source that is associated with a Type II-b su

69 e galaxy that is spatially coincident with a hard X-ray source.

70 the Chandra satellite, in which the detected hard X-ray sources account for at least 75 per cent of t

71 Moreover, most of those hard X-ray sources are associated unambiguously with eit

72 The currently known hard x-ray sources are far too few to explain the ridge

73 Hard X-ray spectro-imaging can visualize electrochemical

74 Here we combine operando hard X-ray spectroscopic imaging and phase-field modelin

75 -ray Observatory, we carried out the deepest hard x-ray survey of a Galactic plane region that is dev

76 ealing structural detail simultaneously with hard-X-ray trace-element measurements.

77 on-invasive evaluation of buried layers with hard X-rays under grazing incidence.

78 We have developed hard-X-ray vector nanotomography with which to determine

79 ive optics have largely been unavailable for hard X-rays where many scientific, technological and bio

80 xploring the interactions of high-intensity, hard X-rays with matter has begun with the start-up of a