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Humans Are Evolving Right Before Our Eyes on The Tibetan Plateau

Humans are not yet done cooking. We’re continuing to evolve and adjust to the world around us, the records of our adaptations written in our bodies.

We know that there are some environments that can make us unwell. Mountain climbers often succumb to altitude sickness – the body’s reaction to a significant drop in atmospheric pressure which means less oxygen is taken in with each breath.

And yet, in high altitudes on the Tibetan Plateau, where oxygen levels in the air people breathe are notably lower than lower altitudes, human communities thrive.

Femtosecond fieldoscopy accesses molecule fingerprints at near-infrared spectral range

In an advance that could revolutionize biomarker detection, researchers at the Max Planck Institute for the Science of Light have developed a novel technique called femtosecond fieldoscopy. This method enables the precise measurement of minute liquid quantities, down to the micromolar level, with unmatched sensitivity in the near-infrared region.

Heliox: Where Evidence Meets Empathy

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Welcome to the Heliox Podcast! Today, we’re in for a mind-bending journey into the future of AI with Ramin Hasani, CEO of Liquid AI. Prepare to be amazed as we explore how a tiny worm’s nervous system could revolutionize artificial intelligence. Hasani shares his vision for smaller, more intelligent AI that might change everything — from healthcare to scientific discovery. We’ll dive into this groundbreaking technology’s exciting possibilities and essential ethical considerations. Get ready for a fascinating glimpse into a future where AI and human potential intertwine in ways we’re only beginning to imagine!

The short history of global living conditions and why it matters that we know it

Love this article from Our World in Data which describes how far we have come as a species and what challenges remain ahead. “Very few think the world is making progress. In this article, we look at the history of global living conditions and show that the world has made immense progress in important aspects.”


The data in this article uses a previous release of the World Bank’s poverty and inequality data in which incomes are expressed in 2011 international-$.

The World Bank has since updated its methods, and now measures incomes in 2017 international-$. As part of this change, the International Poverty Line used to measure extreme poverty has also been updated: from $1.90 (in 2011 prices) to $2.15 (in 2017 prices).

This has had little effect on our overall understanding of poverty and inequality around the world. But because of the change of units, many of the figures mentioned in this article will differ from the latest World Bank figures.

Solving the UV problem of n-type solar

Laboratory testing has revealed that some negatively-doped, ‘n-type’ tunnel oxide passivated contact (TOPCon) and heterojunction (HJT) solar modules are susceptible to ultraviolet (UV) light-related damage and degradation. That could mean trouble down the line, if modules in the field begin to show UV-related performance loss. Manufacturers are implementing solutions at cell and module level.

The Rapid ASKAP Continuum Survey I: Design and first results

The Rapid ASKAP Continuum Survey (RACS) is the first large-area survey to be conducted with the full 36-antenna Australian Square Kilometre Array Pathfinder (ASKAP) telescope. RACS will provide a shallow model of the ASKAP sky that will aid the calibration of future deep ASKAP surveys. RACS will cover the whole sky visible from the ASKAP site in Western Australia and will cover the full ASKAP band of 700‑1800 MHz. The RACS images are generally deeper than the existing NRAO VLA Sky Survey and Sydney University Molonglo Sky Survey radio surveys and have better spatial resolution. All RACS survey products will be public, including radio images (with $\sim$15 arcsec resolution) and catalogues of about three million source components with spectral index and polarisation information. In this paper, we present a description of the RACS survey and the first data release of 903 images covering the sky south of declination $+41^\circ$ made over a 288-MHz band centred at 887.5 MHz.

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