Recurrent miscarriage (RM) is a multifactorial disorder with acknowledged genetic heritability that affects ∼3% of couples aiming at childbirth. As copy number variants (CNVs) have been shown to contribute to reproductive disease susceptibility, we aimed to describe genome-wide profile of CNVs and identify common rearrangements modulating risk to RM. Genome-wide screening of Estonian RM patient...

S1 Temporal decay of the average relevance r(t) and activity a(t) in Digg.com social network 5 S2 Temporal decay of the average relevance r(t) in the APS dataset . . . . . . . . . . . . 5 S3 Age distribution of the top 1% nodes in the ranking (APS data and the corresponding calibrated simulation) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 S4 Outdegree distribution...

ABSTRACT We study the population of star-forming clumps in A521-sys1, a $z=1.04$ system gravitationally lensed by foreground ($z=0.25$) cluster Abell 0521. The galaxy presents one complete counter-image with mean magnification $\rm \mu \sim 4$ and wide arc containing two partial images A521-sys1 magnifications reaching $\mu > 20$, allowing investigations down to scales ${\rm R}_{\rm eff}...

The discovery of radio pulsars (PSRs) around the supermassive black hole (SMBH) in our Galactic Center (GC), Sagittarius A* (Sgr A*), will have significant implications for tests gravity. In this paper, we predict restrictions on parameters Yukawa gravity by timing a pulsar Sgr with variety orbital parameters. Based realistic accuracy times arrival (TOAs), $\sigma_{\rm TOA}=100\,\mu{\rm s}$, an...

The massive 3-loop fermion-loop corrections $\propto C_A N_f T_F^2$ and $C_F N_f T_F^2$ to the massive operator matrix elements $A_{Qg}$, $A_{Qq}^{\rm{PS}}$, $A_{qq,Q}^{\rm{PS}}$, $A_{qq,Q}^{\rm{NS}}$ and $A_{qq,Q}^{\rm{NS,TR}} have been obtained for general values of $N$. Thereby the corresponding contributions to the asymptotic heavy flavor Wilson coefficients of the structure function $F_2(x...

We have detected significant Rotation Measure variations for 9 bright pulsars, as a function of pulse longitude. An additional sample of 10 pulsars showed a rather constant RM with phase, yet a small degree of RM fluctuation is visible in at least 3 of those cases. In all cases, we have found that the rotation of the polarization position angle across our 1.4 GHz observing band is consistent wi...