CIFASD (Collaborative Initiative on Fetal Alcohol Spectrum Disorders) is a multisite consortium supported by the National Institute on Alcohol Abuse and Alcoholism (NIAAA). The purpose of this consortium is to inform and develop effective interventions and treatment approaches for Fetal Alcohol Spectrum Disorders (FASD), through multidisciplinary research involving basic, behavioral, and clinical investigators and projects. We hope to develop an infrastructure to foster collaboration and coordinate basic, clinical, and translational research on FASD., Data were collected across multiple grant cycles spanning 2003 – present. For data from 2003-2022 (Phases 1-4), please go to https://cifasd.org/data-sharing/ to request these CIFASD data. Data from 2022 (Phase 5) and beyond are deposited into the NIAAA Data Archive ( https://www.niaaa.nih.gov/research/niaaa-data-archive). , CIFASD investigators designed and implemented the study and/or provided data but did not necessarily participate in the analysis or writing of this report. A list of CIFASD investigators and projects can be found at https://cifasd.org/research/ . , and CIFASD has received support from NIAAA under award numbers: U01AA014786, U01AA014790, U01AA014809, U01AA014812, U01AA014829, U01AA014834, U01AA014835, U01AA017120, U01AA017122, U01AA017123, U01AA017124, U01AA021651, U01AA026101, U01AA026102, U01AA026103, U01AA026104, U01AA026108, U01AA030164, U01AA030185, U01AA030187, U24AA014811, U24AA014815, U24AA014818, U24AA014828, U24AA014830, U24AA030169, UH2AA026106, UH2AA026109, UH2AA029050, UH2AA029056, UH2AA029062, and UH2AA030186.
This dataset was generated from experiments using purified materials. Experiments were designed to study phase separation of SARS-CoV-2 Nucleocapsid protein.
Soil geochemical analysis was performed using samples from around the US. The sampling and analysis protocols differ by data source (this is available at www.mapmyenvironment.com). The data in this table is soil lead concentration in parts per million binned by municipality in which it was collected.
Rare Earth Elements (REE) phosphates (monazite, xenotime, and rhabdophane) are critical REE-bearing minerals typically formed in hydrothermal and magmatic ore deposits. The ther-modynamic properties of those REE minerals are crucial to understanding the solubility, speciation, and transport of REE complexes. However, the reported standard state Gibbs free energy of for-mation (∆Gof) for these minerals in the literature vary up to 25 kJ mol−1. Here, we present linear free energy relationships that allow the evaluation and estimation of the ∆Gof values at 25 °C and 1 bar for the three minerals from the ionic radius (rREE3+) and the non-solvation Gibbs energy contribution to the REE3+ aqua ion (∆Gon, REE3+): ∆Gof, monazite – 399.71 rREE3+ = 1.0059 ∆Gon, REE3+ – 2522.51; ∆Gof, xenotime – 344.08 rREE3+ = 0.9909 ∆Gon, REE3+ – 2451.53; ∆Gof, rhabdophane – 416.17 rREE3+ = 1.0067 ∆Gon, REE3+ – 2688.86. Moreover, based on the new dataset derived for REE end-members, we re-fitted the binary Margules parameter (W) from previous theoretical calculations into linear correlations: W + 0.00204 ∆Go'n, monazite = 39.3549 ∆V + 0.0641; W + 0.00255 ∆Go'n, xenotime = 25.4885 ∆V – 0.0062. The internally con-sistent thermodynamic properties of these REE phosphates are incorporated into the computer program SUPCRTBL, which is freely available at the site https://models.earth.indiana.edu.
Citation to related publication:
Title:
Recommended standard thermodynamic dataset of monazite, xenotime, and rhabdophane
