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1 years of cosmic history in a short, extreme starburst.
2 disk, rather than in a merger-driven nuclear starburst.
3 star-formation rates in protogalaxies and in starbursts.
4 that can be observed as luminous quasars and starbursts.
5 on of H(2) is not co-spatial with the buried starburst activity and originates outside the obscured r
6 ative corneal curvature is a risk factor for starbursts after laser-assisted in situ keratomileusis (
7 he retina, individual dendritic sectors of a starburst amacrine cell (SAC) are preferentially activat
8 ieving radially symmetric arborization of On starburst amacrine cell (SAC) dendrites and normal SAC s
9 ymmetric GABAergic inhibition exerted by the starburst amacrine cell (SAC), a cholinergic and GABAerg
10 inputs and neurotransmitter release sites on starburst amacrine cell dendrites: the excitatory input
12 Aside from rare counterexamples (e.g. the starburst amacrine cell in retina), neurons are polarize
18 tute a novel cholinergic, non-GABAergic, non-starburst amacrine cell type described for the first tim
20 etina, this study reports that the displaced starburst amacrine cell, a unique cholinergic interneuro
21 scribed of these pairs is the very elaborate starburst amacrine cell, A5, which stains regularly in t
22 n the dendrites of an interneuron, i.e., the starburst amacrine cell, and that these responses are hi
23 neurons, that a presynaptic interneuron, the starburst amacrine cell, delivers direct inhibition to d
26 ; and dendrites of orthotopic- and displaced-starburst amacrine cells (identified by choline acetyltr
27 ccur first in the retina in the dendrites of starburst amacrine cells (interneurons presynaptic to th
28 earch of clues, here we reconstruct Off-type starburst amacrine cells (SACs) and bipolar cells (BCs)
29 rupts self-avoidance of dendrites in retinal starburst amacrine cells (SACs) and cerebellar Purkinje
30 BA release during null-direction motion from starburst amacrine cells (SACs) and DS acetylcholine and
31 he mouse retina to show connectivity between starburst amacrine cells (SACs) and their known synaptic
36 y selective wiring of inhibitory inputs from starburst amacrine cells (SACs) onto four subtypes of ON
38 recordings revealed that distal processes of starburst amacrine cells (SACs) received largely excitat
39 that local inhibition arising from GABAergic starburst amacrine cells (SACs) strongly contributes to
40 try in the inhibitory neurotransmission from starburst amacrine cells (SACs) to direction selective g
41 mission of acetylcholine (ACh) and GABA from starburst amacrine cells (SACs) to direction-selective g
42 lective ganglion cells (DSGCs) and GABAergic starburst amacrine cells (SACs), and the SACs then provi
44 y connected cholinergic interneurons, called starburst amacrine cells (SACs), generates spontaneous r
45 ne receptors (beta2-nAChRs) selectively from starburst amacrine cells (SACs), we show that mutual exc
46 to be initiated by the spontaneous firing of Starburst Amacrine Cells (SACs), whose dense, recurrent
51 established that the inhibition arises from starburst amacrine cells (SBACs) located on the null sid
53 at glycinergic cells inhibit the cholinergic Starburst amacrine cells and are in turn inhibited by GA
55 Cholinergic "retinal waves" are initiated in starburst amacrine cells and propagate to retinal gangli
56 ch costratify near the processes of both the starburst amacrine cells and the ON-OFF directionally se
58 sitive bipolar cell provides input to the ON-starburst amacrine cells and/or the ON-plexus of the ON-
60 lls in the ganglion cell layer revealed that starburst amacrine cells are the most KA-responsive cell
61 allowed imaging spontaneous calcium waves in starburst amacrine cells during development, and light-e
62 the DAPI-3 cell, we have also shown that the starburst amacrine cells exhibit no immunoreactivity for
65 57BL/6J (B6) strain, although the mosaics of starburst amacrine cells in both strains are comparably
67 udy has compared the dendritic morphology of starburst amacrine cells in two different strains of mic
68 that acetylcholine release from presynaptic starburst amacrine cells is crucial for its generation.
69 blocked by TTX, indicating that release from starburst amacrine cells is independent of sodium action
71 ude that the predominant excitatory input to starburst amacrine cells is mediated by AMPA receptors.
73 erned by direction-selective inhibition from starburst amacrine cells occurring during stimulus movem
74 tive release of gamma-aminobutyric acid from starburst amacrine cells onto direction-selective gangli
77 olution localization of GABA(B) receptors on starburst amacrine cells shows that they are discretely
78 (A) strain contains about one-quarter fewer starburst amacrine cells than does the C57BL/6J (B6) str
79 sitize rapidly, enhancing the sensitivity of starburst amacrine cells to moving or other rapidly chan
83 f a mutually inhibitory relationship between starburst amacrine cells with overlapping dendrites.
84 re dictated by recurrent connectivity within starburst amacrine cells, and retinal ganglion cells act
86 e of the neurotransmitter acetylcholine from starburst amacrine cells, the effect of DCG-IV on ON-OFF
89 ing RGC loss in the Ndufs4 KO is the loss of starburst amacrine cells, which may be an important targ
106 natal stages and adult retinas, the presumed starburst amacrine ChAT-IR cells formed two mirror-like
107 In the retina, the beautifully symmetrical 'starburst' amacrine cells interact with each other in a
108 The membrane excitability of cholinergic (starburst) amacrine cells was studied in the rabbit reti
109 h-clamp recordings from pairs of neighboring starburst and ganglion cells show that the rhythmic acti
111 son) showed a correlation with postoperative starbursts and pupil size and a decrease in starbursts w
112 rative dysphotopsia introduces glare, halos, starbursts and shadows in a small number of patients.
114 ved that they were formed in intense nuclear starbursts and that they ultimately grew into the most m
116 eparation of 19 kiloparsecs, the two massive starbursts are about to merge and form a passive ellipti
117 ganglion cell that does not stratify in the starburst band, this suggests that its GABA-dependent di
118 ynapses from a type of amacrine cell termed 'starburst' because of its regularly spaced, evenly radia
119 , but so far there has been no evidence that starbursts can propel substantial quantities of cold mol
120 te to the electrical isolation of individual starburst cell dendrites, a property thought essential f
124 We report that the directional responses of starburst-cell dendrites and DS ganglion cells are highl
125 distribution of the two cotransporters along starburst-cell dendrites mediates direction selectivity.
126 evidence that the cholinergic outputs of the starburst cells affect the responses of the ganglion cel
127 tivity and that the directional responses of starburst cells and DS ganglion cells are exquisitely se
128 stead of being direction discriminators, the starburst cells appear to potentiate generically the res
130 ll recording, Zheng et al. now show that the starburst cells are mutually excitatory during early dev
131 h maturation, the nicotinic synapses between starburst cells dramatically diminished, whereas the GAB
132 lamp recordings were made from 110 displaced starburst cells in a thin retina] slice preparation of r
137 ion cells show that the rhythmic activity in starburst cells is closely correlated with that in gangl
138 the directional discrimination in which the starburst cells participate, namely, that their choliner
140 starburst amacrine cell network suggest that starburst cells regulate their dendritic overlap to ensu
142 cking the K-Cl cotransporter resulted in the starburst cells responding equally to light moving in op
143 erstand the intrinsic membrane properties of starburst cells responsible for direction-selective GABA
144 endrites and KCC2 on the distal dendrites of starburst cells results in a GABA-evoked depolarization
146 fter eye opening (P10), such that all of the starburst cells tested before eye opening had conspicuou
147 We show that this transition allows the starburst cells to use their neurotransmitters for two c
150 er, in contrast to ganglion cells, displaced starburst cells usually do not generate spontaneous soma
153 sistently hyperpolarized and depolarized the starburst cells, respectively, and greatly reduced or el
159 at S15 and included not only the presumptive starburst cholinergic amacrine cells but also a populati
160 ed a high level of synaptic intricacy in the starburst circuit and suggested differential, yet synerg
162 contrast sensitivity without glare, halos or starbursts, defocus curves, optical scatter, retinal poi
164 boronated precision macromolecule [boronated starburst dendrimer (BSD)] was chemically linked to EGF
165 bacteria using an optical sensor based on a starburst dendrimer film containing a lipophilic fluorop
169 onal release of gamma-aminobutyric acid from starburst dendrites and that the asymmetric distribution
170 the NKCC2 and KCC2 cotransporters located on starburst dendrites consistently hyperpolarized and depo
171 of the GABA reversal potential in different starburst dendritic compartments indicate that the GABA
173 robably approximately 3, indicating that the starburst-driven wind limits the star-formation activity
174 ymptoms (double images, glare, halos, and/or starbursts), dry eye symptoms, participant satisfaction
175 l symptoms (double images, glare, halos, and starbursts), dry eye symptoms, satisfaction with vision,
176 ure enough to form the most massive, intense starbursts existed at least as early as 880 million year
177 at resemble spherical baskets, cuboid cages, starbursts, flowers, scaffolds, fences, and frameworks,
178 cluster appears to be experiencing a massive starburst (formation of around 740 solar masses a year),
180 g far (more than 10 kiloparsecs) outside the starburst galaxies (which have radii of less than 1 kilo
182 z > 4, indicating that the fraction of dusty starburst galaxies at high redshifts is greater than pre
187 tions indicate additional contributions from starburst galaxies or heavily filtered quasar radiation.
188 onized by the discovery that luminous, dusty starburst galaxies were 1,000 times more abundant in the
191 ocess, especially in the central regions of 'starburst' galaxies where star formation is vigorous.
193 we report observations of NGC 253, a nearby starburst galaxy (distance approximately 3.4 megaparsecs
194 mpact (effective radius 100 parsecs) massive starburst galaxy at redshift 0.7, which is known to driv
195 re we report the identification of a massive starburst galaxy at z = 6.34 through a submillimetre col
197 outside the galactic plane of the archetypal starburst galaxy M82 (refs 4 and 5), but so far there ha
198 solution x-ray observations of the prototype starburst galaxy Messier 82 (M82) obtained with the adva
200 NGC 4449 is a nearby Magellanic irregular starburst galaxy with a B-band absolute magnitude of -18
201 redshift (z) distribution of dusty, massive starbursts has long been suspected to be biased low in z
202 hile positive dysphotopsia (glare, halos and starbursts) has been largely attributed to edge effects
204 , indicating a coordinated conversion of the starburst network excitability from an early hyperexcita
207 g individual amacrine cell circuits like the starburst or A17 circuit have demonstrated that single t
209 e total number of photons emitted during the starburst phase is sufficient to ionize intergalactic me
210 intly to turbulence and gravity, extends the starburst phase of a galaxy instead of quenching it.
216 screen was ejected from the galaxy during a starburst several 10(8) years earlier and has subsequent
218 vy elements through intense, dust-enshrouded starbursts--that is, increased rates of star formation--
220 of glutamate is processed differentially by starbursts via AMPA receptors and DSGCs via NMDA recepto
221 ense gas, an essential feature of an immense starburst, which contributes, together with the active g
222 t have formed at early epochs in spectacular starbursts, which should be luminous phenomena when obse
223 starbursts and pupil size and a decrease in starbursts with wavefront-guided treatments compared wit
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