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Additional file 1: Supplement Table 1. Fetal adverse outcome by severity of HDP during pregnancy across four subtypes.

Polycyclic aromatic hydrocarbon (PAH) emission serves as a valuable tracer of star formation rate (SFR) and a diagnostic of the physical conditions of the interstellar medium in galaxies. PAH emission is detected in galaxies containing active galactic nuclei (AGNs), both in the integrated mid-infrared (IR) spectra and from spatially resolved spectra of nearby galaxies. However, their applicability to the host galaxies of AGNs as an SFR indicator is controversial given the ability of PAH molecules to survive the harsh radiation field of an active nucleus. Many works have shown that AGNs present distinctive PAH band ratios and mass content from the star-forming galaxies. In this talk, I present our recent study on PAH emissions of a lower-redshift quasar sample. We find that PAHs increasingly underestimate the SFR (by ∼0.5 dex) for quasars with bolometric luminosity > 1046 ergs/s. Furthermore, the PAH ratios indicate that powerful AGNs preferentially destroy small grains and enhance the PAH ionization fraction in their host galaxies. In the end, I discuss how the next-generation observations from the space and ground telescope will advance our understanding of this field., The content of the talk is published in Astrophysical Journal, 925, 218, 2022, with the DOI: https://doi.org/10.3847/1538-4357/ac32e2

Additional file 3: Supplementary Figure 3. Incidence of Low Apgar score by year and gestational age.

Additional file 1: Supplementary Figure 1. Incidence of stillbirth by year and gestational age.

Additional file 5: Supplementary Table 1.Risk of stillbirth at Each Week of Gestation Compared with Remaining in Utero categorized by maternal complication condition. Supplementary Table 2.Risk of SGA at Each Week of Gestation Compared with Remaining in Utero categorized by maternal complication condition. Supplementary Table 3.Risk of low apgar score (

Additional file 2: Supplementary Figure 2. Incidence of SGA by year and gestational age.

Additional file 4: Supplementary Figure 4. Association between maternal complications and adverse perinatal outcomes in women of advanced ages.* *Foetuses staying in utero were used as reference in separate gestational ages, women in medical diseases group or antepartum complications group were compared with uncomplicated women. All results were adjusted for the sampling distribution of the population and clustered of births within hospitals and pregnant woman individuals. Covariates were adjusted as area classification, geographic location, hospital level, infants birth year, education, marriage, parity, prenatal examination, twins born sequence and weight imbalance.

Additional file 1: Table S1. Time trends in uterine rupture rates by the presence of pregnancy complications. Table S2. Risk of uterine rupture with pregnancy complications restricting women without advanced age (���35 years) and multiple gravidities (���4). Table S3. Risk of uterine rupture with pregnancy complications restricting women with offspring having a cephalic lie and a birth weight of less than or equal to 4000 g