ライフサイエンスコーパス: spectrograph

1 n and dispersed along one axis of a CCD by a spectrograph.

2 al lines, and the selected parameters of the spectrograph.

3 y detector coupled to a Mattauch-Herzog mass spectrograph.

4 axies were studied with the Planetary Nebula Spectrograph.

5 rough a push-broom motor driving a line-scan spectrograph.

6 its thousands of modes on a high-resolution spectrograph.

7 grated spectra are recorded using de Broglie spectrographs.

8 esolvable using typical astronomical grating spectrographs.

9 lving power of high-resolution astrophysical spectrographs.

10 usly by the ultraviolet and infrared imaging spectrographs.

11 The Imaging Ultraviolet Spectrograph, a remote sensing instrument on the Mars At

12 This cell was coupled to a spectrograph, allowing in situ absorbance monitoring of

13 1 resolution with a holographic transmissive spectrograph and a cryogenically cooled CCD.

14 tion components simultaneously with a single spectrograph and detector.

15 servations from the Interface Region Imaging Spectrograph and the Swedish 1-m Solar Telescope.

16 either requires a complicated setup with two spectrographs and detectors or two measurements must be

17 and exposure cell with dedicated optics and spectrograph, and a liquid chromatography (LC) system.

18 pulsed tunable dye laser, a high-resolution spectrograph, and an intensified charged-couple device.

19 beams is imaged onto the slit of an imaging spectrograph as two spatially separated signals, i.e., t

20 ocal Group, with the Space Telescope Imaging Spectrograph at a resolution at least a factor of 10 hig

21 spectrum as revealed by the Hamilton echelle Spectrograph at Lick Observatory (resolution approximate

22 ry nebulae secured with the Hamilton Echelle spectrograph at Lick Observatory combined with previousl

23 interferometer and, separately, the CRIRES+ spectrograph at the Very Large Telescope.

24 erence tomography, optical spectroscopy, and spectrograph calibration.

25 is analyzed with a high resolution, compact spectrograph consisting of an echelle grating and a high

26 995, the Hubble Space Telescope Faint Object Spectrograph detected ultraviolet fluorescent emissions

27 collected by the Cassini Ultraviolet Imaging Spectrograph during targeted flybys.

28 Use of a state-of-the-art imaging spectrograph enables high-precision wavenumber duplicabi

29 optical fibers in two vertical lines at the spectrograph entrance.

30 004, just before the Space Telescope Imaging Spectrograph failed, we find that the Lyalpha and Halpha

31 nd fitted to a Mattauch-Herzog geometry mass spectrograph for the simultaneous acquisition of multipl

32 infrared (PA-IR) technique, which utilizes a spectrograph for wavelength dispersion and a mid-infrare

33 demand precise calibration of astrophysical spectrographs in the blue-green, where stellar absorptio

34 servations with the Interface Region Imaging Spectrograph (IRIS) at the solar limb reveal a plethora

35 vations with NASA's Interface Region Imaging Spectrograph (IRIS) reveal a chromosphere and TR that ar

36 servations with the Interface Region Imaging Spectrograph (IRIS) reveal rapid variability (~20 to 60

37 observations by the Interface Region Imaging Spectrograph (IRIS) reveal that it is difficult to deter

38 en motion capture (mocap) technology and the spectrograph is flawed because only vocal articulators a

39 A Mattauch-Herzog geometry mass spectrograph (MHMS) has been equipped with a novel array

40 , has been coupled to a Mattauch-Herzog mass spectrograph (MHMS) with an inductively coupled plasma i

41 ode of the Near Infrared Imager and Slitless Spectrograph (NIRISS) instrument on the JWST.

42 T) and the Near Infrared Imager and Slitless Spectrograph (NIRISS).

43 sigma emission lines, with the Near-InfraRed Spectrograph (NIRSpec) and Near-InfraRed Camera (NIRCam)

44 (ref. (9)), obtained with the Near Infrared Spectrograph (NIRSpec) G395H grating of JWST.

45 es Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec).

46 r the Big Bang, using the JWST Near-Infrared Spectrograph (NIRSpec).

47 Cassini's UltraViolet Imaging Spectrograph observed stellar occultations on two flybys

48 spectrum obtained with the Hamilton Echelle spectrograph on the 3-m Shane Telescope, implies a densi

49 d with the University College London Echelle Spectrograph on the 3.9-m Anglo-Australian Telescope, re

50 e nightside of Venus with HIRES, the echelle spectrograph on the W. M. Keck I 10-meter telescope.

51 kirts of 42 galaxies with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope, we dete

52 D 181327 debris disk using the near-infrared spectrograph onboard the James Webb Space Telescope.

53 man Alpha Mapping Project (LAMP) ultraviolet spectrograph onboard the Lunar Reconnaissance Orbiter (L

54 cattering signals is dispersed by an imaging spectrograph onto a CCD detector, giving 16 independent

55 servations from the Interface Region Imaging Spectrograph reveal the prevalence of intermittent small

56 perture (CA) with multiple thin slits at the spectrograph's entrance to measure the convoluted spectr

57 nced Deep Extragalactic Survey-Near-Infrared Spectrograph spectroscopic confirmation of two luminous

58 moon Europa taken by Space Telescope Imaging Spectrograph (STIS) of the Hubble Space Telescope (HST)

59 ined with the Hubble space telescope imaging spectrograph (STIS).

60 resnel spectrometer that contains a complete spectrograph system, including the detection hardware an

61 coupled plasma Mattauch-Herzog geometry mass spectrograph, thereby offering simultaneous acquisition

62 ment of the detector and modification of the spectrograph to incorporate larger optical components, m

63 ber bundle was incorporated into the imaging spectrograph to provide multiple horizontally shifted sp

64 But it has proved difficult for existing spectrographs to characterize them using their ultraviol

65 e such Doppler shift resolution via improved spectrograph wavelength calibration, with recent encoura

66 ppressing coronagraph, and an integral field spectrograph with low spectral resolution but high spati