ライフサイエンスコーパス: far-infrared

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

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

3 ptical devices that operate from the mid- to 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 Here we report far-infrared and molecular line observations that demons

6 We report far-infrared and submillimeter observations of supernova

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

27 Far-infrared hydrogen recombination lines H15 alpha (169

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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