Sarah Walsh

Viewers first met Mike Youngquist when he began his 90 Day Fiancé journey with Natalie Mordovtseva back in Season 7.

The Disney series Jessie , starring actress Debby Ryan , garnered immense popularity among fans for its entertaining storyline.

At the age of 16, Shawn Johnson stood on top of the world, basking in the glow of Olympic gold in gymnastics.

After Ukrainian native Natalie Mordovtseva walked down the aisle with American Mike Youngquist in 2019, fans of the hit TLC reality TV show 90 Day

In the whirlwind world of reality TV romance, few couples have captured the attention quite like Liz Woods and "Big Ed" Brown . Their time on 90 Day Fiancé: Happily Ever After? was memorable.

Abstract Pathogen host shifts – where a pathogen jumps from one host species to another – are important sources of emerging infectious diseases.

Abstract Locus coeruleus (LC)-derived norepinephrine (NE) drives network and behavioral adaptations to environmental saliencies by reconfiguring

How a 30-something took a trust fall drinking her very first margarita; and the ancient connection between alcohol, agave and anxiety

At low redshifts, the observed baryonic density falls far short of the total number of baryons predicted. Cosmological simulations suggest that these baryons reside in filamentary gas structures, known as the warm-hot intergalactic medium (WHIM). As a result of the high temperatures of these filaments, the matter is highly ionised such that it absorbs and emits far-UV and soft X-ray photons. Athena, the proposed European Space Agency X-ray observatory, aims to detect the “missing” baryons in the WHIM up to redshifts of z = 1 through absorption in active galactic nuclei and gamma-ray burst (GRB) afterglow spectra, allowing for the study of the evolution of these large-scale structures of the Universe. This work simulates WHIM filaments in the spectra of GRB X-ray afterglows with Athena using the SImulation of X-ray TElescopes framework. We investigate the feasibility of their detection with the X-IFU instrument, through O VII (E = 573 eV) and O VIII (E = 674 eV) absorption features, for a range of equivalent widths imprinted onto GRB afterglow spectra of observed starting fluxes ranging between 10−12 and 10−10 erg cm−2 s−1, in the 0.3−10 keV energy band. The analyses of X-IFU spectra by blind line search show that Athena will be able to detect O VII−O VIII absorption pairs with EWO VII > 0.13 eV and EWO VIII > 0.09 eV for afterglows with F > 2 × 10−11 erg cm−2 s−1. This allows for the detection of ≈ 45−137 O VII−O VIII absorbers during the four-year mission lifetime. The work shows that to obtain an O VII−O VIII detection of high statistical significance, the local hydrogen column density should be limited at NH < 8 × 1020 cm−2.Key words: gamma-ray burst: general / large-scale structure of Universe / X-rays: general / intergalactic medium / instrumentation: detectors

On September 23, 2024, Principal Deputy Assistant Attorney General Nicole M. Argentieri announced much-anticipated revisions to the US Department of Justice (DOJ)’s Evaluation of Corporate Compliance Programs (Revised ECCP) in remarks to the Society of Corporate Compliance and Ethics at the 23rd Annual Compliance & Ethics Institute in Grapevine, Texas. The revisions were first previewed by Deputy Attorney General Lisa Monaco in March (for a deeper analysis of those remarks, see our earlier client alert ).