ライフサイエンスコーパス: far-infrared

1 r companion quasars and appear bright in the far-infrared.

2 ptical devices that operate from the mid- to far-infrared.

3 gh competing influences between the mid- and far-infrared.

4 of hen egg white lysozyme is measured in the far infrared (5-65 cm-1, 0.15-1.95 THz, 0.6-8.1 meV) as

5 -ray total scattering experiments, terahertz far-infrared absorption spectroscopy and solid-state nuc

6 Here we report far-infrared and molecular line observations that demons

7 We report far-infrared and submillimeter observations of supernova

8 We have applied far-infrared and ultrafast optical Kerr effect spectrosc

9 on and solid-state (119)Sn NMR spectroscopy, far-infrared and X-ray absorption spectroscopies, elemen

10 tudies of C3 in the interstellar medium with far-infrared astronomy.

11 internal exciton levels, which occur in the far-infrared at terahertz (1012 s(-1)) frequencies, are

12 Since the initial detection of the far-infrared background (FIRB), higher-resolution experi

13 laxies is to yield extragalactic optical and far-infrared backgrounds with approximately equal energy

14 Finally, we show that the far-infrared black-body irradiance of the stone itself l

15 data and were discovered only through their far-infrared [C II] lines and dust continuum emission as

16 We demonstrate that the far-infrared conductivity is unexpectedly dominated by t

17 Here, Wang et al. demonstrate that the far-infrared conductivity of Pb1-x Sn x Se (x = 0.23-0.2

18 The nondetection of far-infrared continuum emission indicates a deficiency o

19 and enhanced [C II] emission relative to the far-infrared continuum, confirming a strong evolution in

20 es observed to have high luminosities in the far infrared could be obscured QSOs and active nuclei.

21 down-conversion, enhance the sensitivity of far-infrared detection beyond the classical limit, achie

22 lariton class arising in the mid-infrared to far-infrared due to shear phenomena in the dielectric re

23 mission line from singly ionized carbon, the far-infrared dust continuum and the near-ultraviolet con

24 ction approach, which relies on encoding the far-infrared electric field into amplitude modulation of

25 The time-resolved detection of mid- to far-infrared electric fields absorbed and emitted by mol

26 Here we report far-infrared ellipsometry and low-frequency dielectric m

27 emission (that is, [C II]) from gas, and the far-infrared emission from dust, in nine typical star-fo

28 Molecular dynamics (MD) simulations and far-infrared (far-IR) spectroscopy were combined to stud

29 gand bond properties can be unraveled in the far-infrared (far-IR)-terahertz-domain (600-3 cm(-1) or

30 Far infrared (FIR) spectral measurements of wild-type (W

31 vel in the metallic SWNTs that appear in the far-infrared (FIR) region of the spectrum show a dramati

32 ntense electromagnetic (EM) radiation in the far-infrared (FIR) spectral range is an advanced tool fo

33 ves rise to periodic absorption of polarized far-infrared (FIR) waves, enabling the manipulation of t

34 d frequency, ranging from millimeter-wave to far-infrared frequencies.

35 and volume phonon polaritons in the mid- to far-infrared frequency range.

36 (DRS) augmented by time-domain terahertz and far-infrared FTIR spectroscopy.

37 city galaxies, low spatial resolution in the far-infrared has typically led to large uncertainties.

38 rd-to-access spectral regions, i.e. mid- and far-infrared, have long been sought.

39 Far-infrared hydrogen recombination lines H15 alpha (169

40 on laser) with s-SNOM, we employed nanoscale far-infrared hyper-spectral-imaging to uncover a Fabry-P

41 ith high precision with the use of a tunable far-infrared laser spectrometer.

42 the isolated water trimer is investigated by far-infrared laser spectroscopy.

43 lass of compact and wavelength-agile mid-and far-infrared light sources.

44 Here we report observations of a far-infrared-luminous object at redshift 6.900 (less tha

45 of the complex was accurately determined by far-infrared magnetic spectroscopy, directly observing t

46 Here, using far-infrared magneto-spectroscopy we explore the continu

47 ticonfigurational calculations, supported by far-infrared magnetospectroscopy data, reveal that the s

48 Furthermore, far-infrared magnetospectroscopy measurements reveal tha

49 Here we employ far-infrared magnetospectroscopy to directly probe vibro

50 ulator stacks, we demonstrate widely tunable far-infrared notch filters with 8.2 dB rejection ratios

51 new submillimetre observations and archival far-infrared observations to estimate the cloud masses,

52 Accordingly, far-infrared optical responses have been understood in t

53 ifferent spectroscopic techniques, including far-infrared, optical, and magnetic resonance spectrosco

54 inaries, white dwarfs are rarely detected at far-infrared or radio frequencies.

55 Sources and systems for far-infrared or terahertz (1 THz = 10(12) Hz) radiation

56 d to the development of transparent mid- and far-infrared photonic devices such as detectors, modulat

57 cted collective excitations; strong mid- and far-infrared photoresponses; terahertz single-photon det

58 Far infrared radiation (FIR) and hot air drying (HA) wer

59 Non-invasive far infrared radiation (FIR) has been observed to improv

60 three different treatments, namely hot-air, far-infrared radiation (FIR), and cellulase, compared wi

61 Terahertz spectroscopy systems use far-infrared radiation to extract molecular spectral inf

62 on spectrum covers the entire ultraviolet to far-infrared range.

63 ractional light traffic and detection in the far-infrared range.

64 diation in the microwave and terahertz (THz; far-infrared) regimes could have an effect on double-str

65 Terahertz (THz) radiation, which lies in the far-infrared region, is at the interface of electronics

66 , especially at terahertz frequencies in the far-infrared region.

67 Many mid- and far-infrared semiconductor photodetectors rely on a phot

68 Inelastic neutron scattering, far-infrared spectroscopy, and cryogenic nuclear magneti

69 h is confirmed by computational modeling and far-infrared spectroscopy.

70 he vibration-rotation-tunneling dynamics and far-infrared spectrum with rigorous quantum methods.

71 oling-free detectors that can cover the full far-infrared spectrum, marking a notable advancement in

72 on, enabling coverage of the mid-infrared to far-infrared spectrum.

73 of the relatively poor spatial resolution of far-infrared telescopes.

74 s with an absorption band extending into the far-infrared (THz band) region.

75 ic function of the films was determined from far-infrared to ultraviolet energies using a combination

76 hotoresponse over a wide spectral range from far-infrared to ultraviolet radiation.

77 Measurement of the far-infrared vibration-rotation tunneling spectrum of th

78 arides recorded in the previously unexplored far-infrared wavelength range) provide well-resolved and

79 The extragalactic background light at far-infrared wavelengths comes from optically faint, dus

80 measured from dust and cool gas emission at far-infrared wavelengths if the galaxies have become suf

81 r otherwise comparable conditions, green and far-infrared wavelengths were found to be more effective

82 ts low absorptivity (emissivity) at mid- and far-infrared wavelengths.

83 characterized by prodigious emission in the far-infrared, with a flux of at least five millijanskys