2017
DOI: 10.1038/pr.2017.125
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Response to Coceani et al.

Abstract: We appreciate the comments of Drs. Coceani, Scebba, and Angeloni. We agree with their point that alterations in calcium entry and sensitization are significant components of the increase in ductus tension that occurs with advancing gestation. As Drs. Coceani, Scebba, and Angeloni point out, the Rho family of GTPases, which affect calcium sensitization by activating Rho kinase and inhibiting myosin phosphatase (1), has been implicated in ductus arteriosus constriction by a number of investigators (2). Our previ… Show more

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Cited by 8 publications
(9 citation statements)
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“…There are several limitations in our present analysis. Previous DA microarray studies have raised concerns about the efficacy and appropriateness of directly comparing different microarray data sets 9,12,71,72 . This is not field-specific, and there are well-known limitations to this type of comparison 7375 .…”
Section: Discussionmentioning
confidence: 99%
“…There are several limitations in our present analysis. Previous DA microarray studies have raised concerns about the efficacy and appropriateness of directly comparing different microarray data sets 9,12,71,72 . This is not field-specific, and there are well-known limitations to this type of comparison 7375 .…”
Section: Discussionmentioning
confidence: 99%
“…Earlier, a similarly intense INOV activity has been observed for the proto-typical NLSy1s J0849+5108 (Maune et al 2014). Such large and frequent INOV is strikingly reminiscent of some prominent BL Lacs, like AO 0235+164 and OJ 287 (e.g., Romero et al 2000;Sagar et al 2004;Goyal et al 2017;Britzen et al 2018).…”
Section: The Nlsy1 1h 0323+342 (Z = 00629)mentioning
confidence: 90%
“…However, no confirmed case is known at sub-milliparsec scales, i.e., separations close enough to be in the GWdominated regime. While ∼150 periodic quasars have been suggested as close BSBH candidates (e.g., Valtonen et al 2008;Graham et al 2015;Charisi et al 2016;Liu et al 2019;Zhu & Thrane 2020), even the most promising candidates are subject to false positives due to quasar's stochastic, red noise variability, given the limited time baseline and relatively low sensitivity of existing surveys (e.g., see Vaughan et al 2016 for evidence against any significant periodicity in PG 1302−102 and Goyal et al 2018 in the case of OJ 287). The study of periodic quasars is important to the searches for close BSBHs in order to test theories of BSBH evolution to shed light on the expected rate of BSBH mergers as GW sources.…”
mentioning
confidence: 99%