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1 argely below the recommended thresholds (< 5 parts per million).
2 th air in the absence or presence of CO (250 parts per million).
3 rs away, varying seasonally from 4.4 to 6.1 parts per million.
4 e C60 isotope is present at a level of a few parts per million.
5 nt and ranged in concentration from 0.1 to 7 parts per million.
6 llowed by a 15-min normalization period at 0 parts per million.
7 ible Earth are indistinguishable within five parts per million.
8 entrations during the EECO were around 1,400 parts per million.
9 don from air at concentrations of only a few parts per million.
10 rred in three sudden steps, each of 10 to 15 parts per million.
11 y, when the partial pressure of CO2 was ~400 parts per million.
12 ospheric concentrations of CO2 less than 430 parts per million.
13 specimens rapidly at concentration levels of parts per million.
14 at measured in terrestrial rocks by 21 +/- 3 parts per million.
15 10 test analytes were in the range of 0-5.4 parts-per-million.
17 well-resolved (182)W excess of 20.6 +/- 5.1 parts per million (+/-2 standard deviations), relative t
19 tracheal LPS and were exposed to acrolein (5 parts per million, 6 h/day), either before or after LPS
20 = 1 soil/dust sample with a lead level > 400 parts per million) among villages in Zamfara State and i
22 its of detection (LODs) range from 0.1 to 24 parts per million and vary inversely with solvent vapor
23 (CO2) levels during the Eocene at 500-3,000 parts per million, and in the absence of tighter constra
24 o 150,000 fwhm, mass accuracies within a few parts per million, and relative mass range up to 8-fold.
25 e obtained at analyte concentrations below 2 parts per million, and responses to below 100 parts per
26 erapy with the lowest dose of celecoxib (500 parts per million), approximating <100 mg of celecoxib/d
28 levels up to maximum Pliocene levels of 450 parts per million) are well described by the currently a
29 The boron concentrations, from 0.7 to 1.6 parts per million, are lower than in most other arc lava
30 e structure, at concentrations of about 7500 parts per million, as much as 40 percent of the strontiu
33 Antarctic ozone minima fall to or below 0.1 parts per million by volume (ppmv) at 18 and 20 km (abou
34 l tracer, because its abundance remains >100 parts per million by volume (ppmv) in the mesosphere.
35 ations increase from current levels near 385 parts per million by volume (ppmv) to a peak of 450-600
36 ioxide concentrations increased by 80 to 100 parts per million by volume 600 +/- 400 years after the
37 te CO2 and low O2 concentration (e.g., 3,200 parts per million by volume and 0.01 bar, respectively)
38 ate water vapor mixing ratios near 40 +/- 20 parts per million by volume between the surface and the
39 nterval with p(co(2)) values of only 200-350 parts per million by volume but nearly ice-free conditio
40 ates that CO(2) remained between 300 and 450 parts per million by volume for these intervals with the
41 strate that pCO2 ranged between 1000 to 1500 parts per million by volume in the middle to late Eocene
42 ween approximately 180 and approximately 280 parts per million by volume over the past 800,000 years,
43 hat increased CO(2) (ranging from 463 to 780 parts per million by volume) stimulates both N(2)O emiss
44 while elevated CO2 (ranging from 550 to 800 parts per million by volume) stimulates the accumulation
46 sulfur content was reduced from 430 to <0.2 parts per million by weight in a commercial diesel at a
47 ed to measure acetone in human breath at sub parts-per-million by volume (ppmv) concentrations using
50 tended to be seen with 2-day lags, where a 1-parts-per-million change in carbon monoxide and a 20-par
51 ed from atom probe tomography (APT) (10's of parts-per-million chemical sensitivity and sub-nanometer
57 arious catalytic/initiation systems that use parts-per-million concentrations of Cu catalysts and can
58 ept superradiance can be used to detect low (parts per million) concentrations of various gases at di
59 narrow filament of enhanced CO2 values ( 3.4 parts per million), consistent with a CO2 point source e
62 induced by extended (48-72 h) low-dose (0.3 parts per million) exposure to ozone, adiponectin-defici
63 er than most SNC meteorites, with up to 6000 parts per million extraterrestrial H(2)O released during
65 pes; the lowest LODs are in the single digit parts per million for single-shot LA signal from a 10-mu
66 ing room air and then room air with NO at 80 parts per million, forearm blood flow was measured in 16
67 ated melt that contained approximately 1,600 parts per million H(2)O and approximately 3,500 parts pe
70 its star, punctuated by a drop of 130 +/- 11 parts per million in flux when the planet passes behind
71 measurements yielded differences of up to 25 parts per million in the 137Ba/136Ba ratio and 60 parts
72 per million in the 137Ba/136Ba ratio and 60 parts per million in the 138Ba/136Ba ratio between chond
76 rs at relatively high concentrations (>/=800 parts per million) in Mars' atmosphere, where it represe
77 shifts in solution ranging from +125 to -90 parts per million indicate an inhomogeneous electron dis
78 e of the water absorption (approximately 250 parts per million) indicates that the planetary atmosphe
79 sevoflurane room air concentration was 0.10 parts per million (interquartile range, 0.07-0.15), 0.17
80 n (interquartile range, 0.14-0.27), and 0.15 parts per million (interquartile range, 0.07-0.19) at ba
81 llion (interquartile range, 0.07-0.15), 0.17 parts per million (interquartile range, 0.14-0.27), and
82 nce chemical shift in the solid state (226.7 parts per million) is almost identical to that in benzen
83 xide, with a threshold of perhaps only a few parts per million, is a selective pulmonary vasodilator
85 from that of chondritic meteorites but is 20 parts per million less than most samples from Earth.
86 tic and antagonistic impacts of trace (i.e., parts per million level) components on the surface compo
88 ses are very fast, and removal of H2S to sub-parts per million levels is achieved at very short (mill
90 ical sensitivity was achieved, down to a sub-parts per million limit of detection with a high dynamic
91 g glacial periods were consistently about 80 parts per million lower than during interglacial periods
92 ites show that their 142Nd/144Nd ratio is 20 parts per million lower than that of most terrestrial ro
97 a control gas (nitrogen) or nitric oxide (80 parts per million), mixed with oxygen from a ventilator.
98 eservoir must have an Nb concentration >/= 2 parts per million, Nb/La >/= 1.2, and Nb/Ta between 19 a
99 and approximately 100% oxygen with 10 to 80 parts per million nitric oxide to evaluate pulmonary vas
102 ximately 1400 parts per million of S and 900 parts per million of Cl in inclusions down to a few hund
103 g aorta transplantation; pre-exposure to 250 parts per million of CO for 1 hour before injury suppres
104 ive (least altered) meteorites contain a few parts per million of micrometre-sized dust which formed
105 Concentrations range from approximately 1400 parts per million of S and 900 parts per million of Cl i
107 f the L enantiomer, low concentrations (<0.1 parts per million) of endogenous D-alanine may be presen
109 , and bicyclic hydrocarbons) are released at parts per million or parts per billion level with temper
110 g low (0.08 parts per million), medium (0.25 parts per million), or high (2.7 parts per million) Se t
111 olivine is not expected to be higher than 50 parts per million owing to partitioning with other mantl
112 in the morning to either filtered air or 0.3 parts per million ozone for 2 hours during 15-minute on-
113 emonstrated current accuracy better than 1.2 parts per million (p.p.m.) and strong evidence, based on
114 76A diet or one supplemented with 250 or 500 parts per million (ppm) aspirin (n = 6 per group) for 7
115 ) that had been dosed with 0.0, 0.1, and 0.6 parts per million (ppm) dietary methylmercury and measur
116 icted to MALDI peaks having less than +/-150 parts per million (ppm) error, thereby holding our analy
117 rites display a deficit of approximately 100 parts per million (ppm) in 144Sm with respect to other m
118 s led to substantial increases of up to 2000 parts per million (ppm) in the concentration of atmosphe
119 Thereafter, they sequentially inhaled 100 parts per million (ppm) NO, 40% O2; 40% O2; and 100 ppm
121 ts consumed a preload solution of either 300 parts per million (ppm) saccharin or water with or witho
123 Nitric oxide was administered at 2, 4, and 6 parts per million (ppm), in a random order, under the co
124 We find pre-CAMP PCO(2) values of ~2000 parts per million (ppm), increasing to ~4400 ppm immedia
128 rological reservoirs, requires separation of parts-per-million (ppm) level Kr from chemically airlike
130 om inexpensive FeCl3 that naturally contains parts-per-million (ppm) levels of Pd can catalyze Suzuki
131 has proven to be efficient with as low as 10 parts-per-million (ppm) of precatalyst in the Buchwald-H
133 rified control diet formulated to contain 50 parts per million [ppm] total zinc; group 2 was fed ad l
134 ich occurs at fluoride concentrations in the parts per million range, is accompanied by a drastic flu
136 ores when operating at tolerances in the low parts-per-million range but become apparent with the con
137 inear calibration plots were down to the sub-parts-per-million range, a sensitivity that is comparabl
140 edium (0.25 parts per million), or high (2.7 parts per million) Se to female C57BL/6 mice and used an
141 2 hours with blood supplemented with CO (300 parts per million) showed significantly decreased portal
142 posing cells to CO at a concentration of 250 parts per million suppressed membrane trafficking of TLR
143 184)W that is significantly higher (about 13 parts per million) than modern terrestrial samples.
144 soluble organic compounds (approximately 100 parts per million) that includes mono- and dicarboxylic
145 ioactive elements potassium (K, 1150 +/- 220 parts per million), thorium (Th, 220 +/- 60 parts per bi
148 peptide masses with an uncertainty of a few parts per million using a high sensitivity linear ion tr
149 ly, yielding a detection limit of 0.830 ppm (parts per million v/v or muL/L hereinafter) and a quanti
150 esent at levels approximately 10(2) to 10(3) parts per million volume (ppmv) (compared with 1.7 ppmv
153 environmentally realistic concentration (0.8 parts per million), we demonstrated that exposure of rat
154 matrices at levels ranging from 0.1 to 10(5) parts per million (weight/weight), worked equally well o
157 red and calculated exact m/z was less than 2 parts per million, which often allowed assignment of uni
158 trations of dispersed oil in the sea are sub-parts-per-million within a day of dispersal, and at such
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