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Fjord Secures $4.3M Seed Round for Community Funding

Fjord Secures $4.3 Million Seed Round: A Game Changer for Community-Focused Funding In a pivotal moment for the burgeoning world of blockchain and cryptocurrency, Fjord has successfully closed a remarkable $4.3 million seed funding round. This achievement underscores the critical need for platforms that not only connect innovative projects with dedicated backers but also prioritize fairness and transparency in the funding process. For more insights into Fjord’s potential impact, check out Fjord . A Strong Backing The oversubscribed round was led by Lemniscap , a reputable investment firm known for its focus on emerging crypto assets. Other notable participants included Mechanism Capital , Zee Prime Capital , and Castle Capital , along with a roster of angel investors such as Crypto Kaduna , Fomosaurus , Joshua Rager , and Danny Wilson of Illuvium fame. This diverse group of investors highlights the growing confidence in Fjord's mission and its potential impact on the blockch...

# AI Revolutionizes Astronomy: Supernovae Identified in Real-Time

A group of scientists and astronomers have made a significant breakthrough in the field of astronomy by successfully using artificial intelligence and machine learning to identify and classify a supernova in real-time. The project, known as the Bright Transient Survey (BTS) bot, aims to automate the process of confirming whether a detected event is indeed an exploding star, thus eliminating the need for human intervention. This innovation allows researchers more time to analyze the observed supernova and develop new hypotheses to explain the origin of these cosmic explosions.

The BTSbot project, which launched last week, was led by students and faculty at Northwestern University, a private research institution. By harnessing the power of AI and machine learning, the team behind the project was able to train the bot using tens of thousands of supernovae data points collected since 2018. This vast dataset enabled the development of a model capable of accurately identifying and classifying supernovae exceeding a specific brightness level.

Supernovae are incredibly powerful stellar explosions that release massive amounts of energy, temporarily outshining an entire galaxy. These catastrophic events occur when a star depletes its nuclear fuel at its core, leading to a collapse. The ability to rapidly identify and classify these cosmic events is crucial for astronomers and researchers studying the origins and behavior of stars.

The Zwicky Transient Facility (ZTF), based at the Palomar Observatory in San Diego, California, was founded in 2018 with the goal of rapidly identifying and studying supernovae. Led by Nabeel Rehemtulla and Adam Miller, the BTSbot project leverages the data collected by ZTF to automate the process of identifying and classifying supernovae. By removing the need for human intervention, the research team can now dedicate more time to analyzing their observations and developing new hypotheses.

While some individuals may express concerns about being replaced by AI, the primary goal of the BTSbot project is to improve efficiency and enhance the capabilities of researchers. By automating the process of supernova identification and classification, the project enables scientists to focus on analyzing the observed events and advancing our understanding of these cosmic phenomena. As further refinements are made to the models, the BTSbots may even be able to isolate specific subtypes of stellar explosions, providing even more detailed insights into the nature of supernovae.

In conclusion, the successful use of artificial intelligence and machine learning in the BTSbot project represents a significant step forward in the field of astronomy. By automating the process of identifying and classifying supernovae, researchers can now devote more time to analyzing these cosmic events and developing new hypotheses. This innovation not only improves efficiency but also opens up new possibilities for understanding the origins and behavior of stars.

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