1 haemoglobin concentrations (assessed with a
photometric analyser) of the children were measured.
2 Single-cell
photometric analyses were consistent with an altered int
3 Photometric analysis of chloroplast movements in various
4 Photometric analysis of the fragments indicates that the
5 Photometric analysis showed that the supernatant and mem
6 his study suggest potential benefit in using
photometric analysis to assess gingival changes after th
7 With a
photometric analysis we estimate its absolute magnitude
8 The total betalain content was estimated by
photometric analysis.
9 Photometric and chromatographic methods as well as mass
10 pared with the established ELISA concept for
photometric and CL detection.
11 It is shown by
photometric and fluorimetric analysis, along with suppor
12 ydrophobic C18 monolithic column and on-line
photometric and fluorimetric detection for the determina
13 Photometric and spectral measurements on individual SWCN
14 Here we report
photometric and spectroscopic observations of SN1993J te
15 Using
photometric and spectroscopic sensors, we observed up to
16 t hXK acts only on d-xylulose, and a coupled
photometric assay established its key kinetic parameters
17 ed by these methods with those obtained by a
photometric assay that quantified the reduction of 3-(4,
18 titative assessment using a simple and quick
photometric assay.
19 ared with those obtained using the classical
photometric assay.
20 l mediator using cyclic voltammetry (CV) and
photometric assay.
21 density were determined by using a standard
photometric assay.
22 < 5%, n = 3) and correlation with classical
photometric assays (r >= 0.91).
23 of the enzyme activity at flow conditions by
photometric assays reveals that the enzyme activities of
24 apes, we find a geometric albedo of in the V
photometric band, which establishes that KBO 55636 is sm
25 thermal emission has been measured in broad
photometric bands(23-26).
26 ophysiology, in vivo optogenetics with fiber
photometric calcium measurements, and chemogenetics to u
27 models), where it also serves as the primary
photometric calibrator.
28 In this work, we conducted a
photometric campaign during 1998 KY(26)'s close approach
29 Photometric changes lagged and were maintained as nerve
30 icitly modeling and estimating geometric and
photometric changes.
31 raints," which link variations in intensity (
photometric constraints) to the sign and direction of 3D
32 we report an extensive multi-colour optical
photometric data set of V404 Cygni, an X-ray transient s
33 Ten days of
photometric data were obtained during the commissioning
34 n, but they complicate the interpretation of
photometric data.
35 and compactness of the galaxy inferred from
photometric data.
36 )] using gas chromatography with ultraviolet
photometric detection (GC-UV) at 254 nm.
37 mance liquid chromatographic separation, and
photometric detection are employed to determine the redu
38 of using deep UV-LEDs as the light source in
photometric detection for even lower-wavelength-absorbin
39 ary zone electrophoresis (CZE) with indirect
photometric detection is a viable approach to the separa
40 The
photometric detection is performed using dedicated flow-
41 A new enzymatic assay, based on
photometric detection of ammonia with ninhydrin, was dev
42 of biological materials followed by on-chip
photometric detection, (ii) flow-through bioaccessibilit
43 rry leaf using gas chromatography with flame
photometric detection, and confirmed using gas chromatog
44 03.2% and 92.0-106.5% using fluorimetric and
photometric detection, respectively.
45 pressure liquid chromatography with indirect
photometric detection.
46 o develop microfluidic methods for improving
photometric detection.
47 ction enabled better analytical results than
photometric detection.
48 to HPLC-UV and gas chromatography with flame
photometric detector (GC-FPD), respectively; was carried
49 using gas chromatography with a pulsed flame
photometric detector (GC-PFPD).
50 A microcountercurrent flame
photometric detector (microcc-FPD) was adapted and optim
51 (UV-LED) is employed within an on-capillary
photometric detector and applied in capillary ion-exchan
52 The injection repeatability as observed by a
photometric detector is better than 1.2% (n = 100).
53 metry (GC-O) and coupled with a pulsed flame
photometric detector.
54 imultaneous detection by MS and pulsed flame
photometric detectors (PFPD) provided additional selecti
55 raviolet excitation fluorescence (sugar) and
photometric determination (oil).
56 cally using a platelet aggregometer or other
photometric device equipped with a stirred cell.
57 identified (in a PNAS work) the first three
photometric DS candidates: JADES-GS-z11-0, JADES-GS-z12-
58 obtained in the same eyes using the flicker
photometric electroretinogram (ERG), although the compar
59 e cone photopigments was assessed by flicker
photometric electroretinography (ERG).
60 CL detection, performing similarly well to a
photometric ELISA (0.13 ng/mL), which demonstrates the h
61 etermination of the unreacted thiol with the
photometric Ellman's test.
62 ions presented on a CRT by using the flicker
photometric ERG.
63 be z = 6.29 +/- 0.01, in agreement with our
photometric estimate.
64 etry (MS), nitrogen phosphorous (NPD), flame
photometric (
FPD) detectors, as well as gas chromatograp
65 om curved surfaces are ordinarily adorned by
photometric highlights and lowlights in the position of
66 ductivity, diffusion-ordered NMR (DOSY), and
photometric kinetic measurements is employed to analyze
67 avelength spectroscopic and short-wavelength
photometric light curves span 2.0-4.0 micrometres, exhib
68 inties of 5%, as determined from RV data and
photometric light curves.
69 facturer's established positive and negative
photometric light unit (PLU) cutoff values.
70 In the present study, a
photometric LOX assay including adequate sample workup w
71 ercept is related to an object's luminance-a
photometric measure of light intensity relevant for cone
72 We analyzed
photometric measurements and images of comet C/LINEAR be
73 Photometric measurements are recommended for a simple an
74 the microscope provides a powerful tool for
photometric measurements of dynamics requiring submillis
75 Recent
photometric measurements of fireballs reveal strong mill
76 Our ocular transmission
photometric measurements revealed that the distribution
77 We used
photometric measurements to explore two possible scenari
78 Photometric measurements were made during perfusion of t
79 omnographic recordings combined with in vivo
photometric measurements.
80 A new
photometric method is introduced for assessment of gingi
81 zation with Enhanced Resolution (SIMPLER), a
photometric method to decode the axial position of singl
82 Both quantitative video imaging and a new
photometric method were utilized to determine the rates
83 The analytical features of the
photometric method, which does not allow the quantificat
84 ement with those determined using a standard
photometric method.
85 ric method and between 2.4% and 6.2% for the
photometric method.
86 Applying imaging and single-cell
photometric methods, we find that the probe rhod-2 selec
87 light in their operation, through use of (i)
photometric methods, where ambient light contributes dir
88 signed high-throughput methyl viologen-based
photometric microtiter plate assay was established to de
89 ronics and energy harvesters with injectable
photometric modules in a class of fully wireless, batter
90 tene acetals) were studied kinetically using
photometric monitoring at 20 degrees C.
91 Here we report the results of a
photometric monitoring campaign of that star from the gr
92 Continuous
photometric monitoring of 2',7'-bis(carboxyethyl)-5, 6-c
93 Spectroscopic and
photometric monitoring of the supernova leads us to sugg
94 measured, including geometric, textural, and
photometric nuclear features and DNA ploidy.
95 L) as achromatic, both contribute to flicker
photometric nulls without producing visible colour varia
96 New multicolour
photometric observations confirm the longevity of the se
97 We report precise optical
photometric observations of a small near-Earth asteroid,
98 Narrowband
photometric observations of comet Hale-Bopp (C/1995 O1)
99 Here we report 8-microm
photometric observations of the planet HD 80606b during
100 Here we present spectroscopic and
photometric observations of TIC 241249530 b, a high-mass
101 Comparison of early
photometric observations of type Ic supernovae with theo
102 Here, we report on sensitive
photometric observations, based on imaging from the STER
103 Combining these data with
photometric observations, we find that Hi'iaka is a tria
104 f an Earth-like planet could be derived from
photometric observations.
105 been investigated by titrations followed by
photometric or conductometric methods as well as by isot
106 rformed to evaluate the relationship between
photometric outcomes and continuous, dichotomous, and ca
107 evels were continuously monitored using a UV
photometric ozone analyzer and a fast mobility particle
108 A flicker
photometric paradigm was used to equate the ERG response
109 The
photometric parameters were appropriate for backlighting
110 The spectral and
photometric peculiarities were best explained by models
111 Bennu's disk-integrated
photometric phase function validates measurements from t
112 The depth of the occultation is similar in
photometric precision to the detection of a transiting E
113 Using simultaneous
photometric presynaptic Ca(2+) and striatal field potent
114 We also determined the trajectories and
photometric properties of several gravitationally bound
115 raft surveyed Bennu's immediate environment,
photometric properties, and rotation state.
116 In parallel,
photometric recording from cholinergic terminals in the
117 Photometric recordings and calibrated closed-loop optoge
118 Photometric recordings during negative emotional contagi
119 We used long-term
photometric recordings in mice to study a population of
120 Combining polysomnographic and
photometric recordings in mice, we show that CRH release
121 tect the optical afterglow, we determine the
photometric redshift of the burst to be z = 6.39 - 0.12
122 Although such
photometric redshifts are generally robust, they can suf
123 h a compact over-density of galaxies(2) with
photometric redshifts of 1.9 +/- 0.2.
124 Galaxies at the centres of several ORCs have
photometric redshifts of z 0.3-0.6, implying physical sc
125 Using
photometric reflectance data of >1,300 bird specimens dr
126 rties is commonly provided by single-viewing
photometric satellite sensors that are not sensitive to
127 in PR and other peroxisomal functions in the
photometric screen will enable further investigation of
128 Here we present
photometric secondary eclipse observations of the Earth-
129 Photometric stereo is a three dimensional (3D) imaging t
130 wing fast reconstruction of 3D objects using
photometric stereo.
131 Our
photometric studies confirmed the production of ~60 muM
132 Simultaneous pulsed flame
photometric (
sulfur-specific) detection differentiated P
133 With the advent of large
photometric surveys(8) and the astrometric survey(9), th
134 Signal to noise in any
photometric system is also dependent on the amount of li
135 d recorded their mechanical responses with a
photometric system.
136 inhibitor by rapid acid quenching as well as
photometric techniques.
137 ured with GD-based amperometric and GO-based
photometric test strips generally were within error tole
138 eStep) of glucose measurements with GO-based
photometric test strips, and 4.6% (Accu-Chek Advantage H
139 strips, and have minimal effect on GO-based
photometric test strips.
140 A
photometric transit search excludes companions with size
141 The sugars were quantified using
photometric- (
UV; 303 nm) and fluorescence-detection (la
142 c structure, mass transfer, magnetic fields,
photometric variability and the origin of chemical anoma
143 Our observations show that GJ 887 has
photometric variability below 500 parts per million, whi
144 We combine radial velocity and
photometric variability data to show that the bright, ra
145 The
photometric variability period of the giant is consisten
146 eves ~10-fold greater sensitivity than prior
photometric voltage sensing, allows hour-long recordings
147 resent Supercritical Illumination Microscopy
Photometric z-Localization with Enhanced Resolution (SIM