2018
DOI: 10.3899/jrheum.171244
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Dr. Noda, et al reply

Abstract: We appreciate the comments provided by Dr. Bhansing and colleagues 1 in response to our article 2. Recently, Bhansing, et al showed a significant 2-fold increase in the fascia thickness of the deltoid muscles on ultrasonography (US) in patients with dermatomyositis (DM) and polymyositis (PM) relative to healthy controls 3. Additionally, they showed that the deltoid fascial thickness on US in patients with DM and PM was not associated with various clinical variables, including the disease duration, serum creati… Show more

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Cited by 10 publications
(13 citation statements)
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“…The human 5-HT 5A receptor has been claimed to couple to several signal transduction pathways when stably expressed in C6 glioma cells [1472] and electrophysiological recordings from mice and rat prefrontal cortex (layer V pyramidal neurons) demonstrate 5-HT-elicited outward currents mediated via the 5-HT 5A receptor [660]. The human orthologue of the mouse 5-ht 5b receptor is non-functional due to interruption of the gene by stop codons.…”
Section: Nomenclaturementioning
confidence: 99%
“…The human 5-HT 5A receptor has been claimed to couple to several signal transduction pathways when stably expressed in C6 glioma cells [1472] and electrophysiological recordings from mice and rat prefrontal cortex (layer V pyramidal neurons) demonstrate 5-HT-elicited outward currents mediated via the 5-HT 5A receptor [660]. The human orthologue of the mouse 5-ht 5b receptor is non-functional due to interruption of the gene by stop codons.…”
Section: Nomenclaturementioning
confidence: 99%
“…4 and 5, with observational values (see Ref. [9]). Changing the n-3 P 2 model, the cooling curves play different tendency.…”
Section: Cooling Modelmentioning
confidence: 52%
“…Due to thermodynamical effect, the neutrino emissivity by quarks suppresses to almost zero. With this condition, stars having quark phase remain wormer than that without quark phase [9]. We focus on to the nucleon superfluidity.…”
Section: Cooling Modelmentioning
confidence: 99%
“…Including CSC phase, the heavier stars cool slower, and the lighter stars play opposite role [8,9]. Adding the effect of superfluidity and modifying the T CR of neutron 3 P 2 superfluid state, it can change the situation of mass-temperature relation.…”
Section: Discussionmentioning
confidence: 99%
“…3 and 4 with available observational values (see Ref. [8]). Adopting the model-n1 for neutron 3 P 2 superfluidity, the cooling curves show that the heavier star cools faster, and oposite tendency when adopting the model-n2.…”
Section: Cooling Modelmentioning
confidence: 99%