Government
NASA's new Roman Space Telescope aims to discover 100,000 cosmic explosions
Breakthroughs, discoveries, and DIY tips sent every weekday. While the Hubble and James Webb Space Telescopes continue to offer astronomers revolutionary glimpses of our universe, their upcoming sibling may very well upstage them. Scheduled to launch in 2027, NASA's Nancy Grace Roman Space Telescope is designed with a field of view at least 100 times larger than Hubble's, with the potential to document light from over a billion galaxies over its career. Combined with timelapse recording capabilities, Roman will help researchers to better understand exoplanets, infrared astrophysics, and the nature of dark matter. According to a study published on July 15 in The Astrophysics Journal, Roman is poised to eventually capture an estimated 100,000 celestial explosions over its lifetime.
Trump hosts Qatar's PM for private dinner, meets Bahrain crown prince
President Donald Trump has hosted Qatar's prime minister for a private dinner and met with Bahrain's crown prince at the White House as part of a United States effort to address regional issues, including securing a Gaza ceasefire, and promote diplomatic ties with the Gulf region. Sheikh Mohammed bin Abdulrahman bin Jassim Al Thani, the Qatari prime minister and a member of the country's ruling family, had a private dinner with Trump on Wednesday evening. Before this meal, Trump met with Bahrain Crown Prince Salman bin Hamad Al Khalifa in the Oval Office. With little progress to share on the region's most pressing conflicts, including Israel's war on Gaza, Trump was more focused on Wednesday on promoting diplomatic ties as a vehicle for economic growth. Trump has lavished attention on the Gulf, a wealthy region where members of his family have extensive business relationships.
LEE ZELDIN: Trump's EPA clearing the regulatory path for America to dominate the global AI revolution
Fox News anchor Bret Baier examines the U.S. power supply on'Special Report.' The global race to harness the power of artificial intelligence (AI) has begun. President Donald Trump got it right from the start when he issued an executive order in January to strengthen America's AI โ the next great technological forefront. From Day One as Environmental Protection Agency (EPA) administrator, it was clear that EPA would have a major hand in permitting reform to cut down barriers that have acted as a roadblock so we can bolster the growth of AI and make America the AI capital of the world. In fact, it's an endeavor so important, it is a core pillar of my Powering the Great American Comeback initiative.
Russia-Ukraine war: List of key events, day 1,239
A Russian air raid on a shopping centre and market in Dobropillia, eastern Ukraine, killed at least two people, wounded 22 others and caused widespread damage on Wednesday, the regional governor, Vadym Filashkin, said. Filashkin said the building was struck by a 500kg (1,100-pound) bomb at 5:20pm (14:20 GMT). Russia launched 400 Shahed and decoy drones, as well as one ballistic missile, on Wednesday night, the Ukrainian air force said. The strikes targeted the northeastern city of Kharkiv, the central city of Kryvyi Rih, Vinnytsia in the west, and Odesa in the south. A Ukrainian drone killed one person and injured six others in the Russian city of Belgorod, and injured one person in a village northeast of the city, the regional governor, Vyacheslav Gladkov, said.
Newfluence: Boosting Model interpretability and Understanding in High Dimensions
Zou, Haolin, Auddy, Arnab, Kwon, Yongchan, Rad, Kamiar Rahnama, Maleki, Arian
The increasing complexity of machine learning (ML) and artificial intelligence (AI) models has created a pressing need for tools that help scientists, engineers, and policymakers interpret and refine model decisions and predictions. Influence functions, originating from robust statistics, have emerged as a popular approach for this purpose. However, the heuristic foundations of influence functions rely on low-dimensional assumptions where the number of parameters $p$ is much smaller than the number of observations $n$. In contrast, modern AI models often operate in high-dimensional regimes with large $p$, challenging these assumptions. In this paper, we examine the accuracy of influence functions in high-dimensional settings. Our theoretical and empirical analyses reveal that influence functions cannot reliably fulfill their intended purpose. We then introduce an alternative approximation, called Newfluence, that maintains similar computational efficiency while offering significantly improved accuracy. Newfluence is expected to provide more accurate insights than many existing methods for interpreting complex AI models and diagnosing their issues. Moreover, the high-dimensional framework we develop in this paper can also be applied to analyze other popular techniques, such as Shapley values.
Small Data Explainer -- The impact of small data methods in everyday life
Hackenberg, Maren, Connor, Sophia G., Kabus, Fabian, Brawner, June, Markham, Ella, Hardalupas, Mahi, Chowdhury, Areeq, Backofen, Rolf, Kรถttgen, Anna, Rohde, Angelika, Binder, Nadine, Binder, Harald, Data, the Collaborative Research Center 1597 Small
The emergence of breakthrough artificial intelligence (AI) techniques has led to a renewed focus on how small data settings, i.e., settings with limited information, can benefit from such developments. This includes societal issues such as how best to include under-represented groups in data-driven policy and decision making, or the health benefits of assistive technologies such as wearables. We provide a conceptual overview, in particular contrasting small data with big data, and identify common themes from exemplary case studies and application areas. Potential solutions are described in a more detailed technical overview of current data analysis and modelling techniques, highlighting contributions from different disciplines, such as knowledge-driven modelling from statistics and data-driven modelling from computer science. By linking application settings, conceptual contributions and specific techniques, we highlight what is already feasible and suggest what an agenda for fully leveraging small data might look like.
Subgraph Generation for Generalizing on Out-of-Distribution Links
Revolinsky, Jay, Shomer, Harry, Tang, Jiliang
Graphs Neural Networks (GNNs) demonstrate high-performance on the link prediction (LP) task. However, these models often rely on all dataset samples being drawn from the same distribution. In addition, graph generative models (GGMs) show a pronounced ability to generate novel output graphs. Despite this, GGM applications remain largely limited to domain-specific tasks. To bridge this gap, we propose FLEX as a GGM framework which leverages two mechanism: (1) structurally-conditioned graph generation, and (2) adversarial co-training between an auto-encoder and GNN. As such, FLEX ensures structural-alignment between sample distributions to enhance link-prediction performance in out-of-distribution (OOD) scenarios. Notably, FLEX does not require expert knowledge to function in different OOD scenarios. Numerous experiments are conducted in synthetic and real-world OOD settings to demonstrate FLEX's performance-enhancing ability, with further analysis for understanding the effects of graph data augmentation on link structures. The source code is available here: https://github.com/revolins/FlexOOD.
Galaxy image simplification using Generative AI
Erukude, Sai Teja, Shamir, Lior
Modern digital sky surveys have been acquiring images of billions of galaxies. While these images often provide sufficient details to analyze the shape of the galaxies, accurate analysis of such high volumes of images requires effective automation. Current solutions often rely on machine learning annotation of the galaxy images based on a set of pre-defined classes. Here we introduce a new approach to galaxy image analysis that is based on generative AI. The method simplifies the galaxy images and automatically converts them into a ``skeletonized" form. The simplified images allow accurate measurements of the galaxy shapes and analysis that is not limited to a certain pre-defined set of classes. We demonstrate the method by applying it to galaxy images acquired by the DESI Legacy Survey. The code and data are publicly available. The method was applied to 125,000 DESI Legacy Survey images, and the catalog of the simplified images is publicly available.
Synthetic Tabular Data Generation: A Comparative Survey for Modern Techniques
Challagundla, Raju, Dorodchi, Mohsen, Wang, Pu, Lee, Minwoo
As privacy regulations become more stringent and access to real-world data becomes increasingly constrained, synthetic data generation has emerged as a vital solution, especially for tabular datasets, which are central to domains like finance, healthcare and the social sciences. This survey presents a comprehensive and focused review of recent advances in synthetic tabular data generation, emphasizing methods that preserve complex feature relationships, maintain statistical fidelity, and satisfy privacy requirements. A key contribution of this work is the introduction of a novel taxonomy based on practical generation objectives, including intended downstream applications, privacy guarantees, and data utility, directly informing methodological design and evaluation strategies. Therefore, this review prioritizes the actionable goals that drive synthetic data creation, including conditional generation and risk-sensitive modeling. Additionally, the survey proposes a benchmark framework to align technical innovation with real-world demands. By bridging theoretical foundations with practical deployment, this work serves as both a roadmap for future research and a guide for implementing synthetic tabular data in privacy-critical environments.
The Safety Gap Toolkit: Evaluating Hidden Dangers of Open-Source Models
Dombrowski, Ann-Kathrin, Bowen, Dillon, Gleave, Adam, Cundy, Chris
Open-weight large language models (LLMs) unlock huge benefits in innovation, personalization, privacy, and democratization. However, their core advantage - modifiability - opens the door to systemic risks: bad actors can trivially subvert current safeguards, turning beneficial models into tools for harm. This leads to a 'safety gap': the difference in dangerous capabilities between a model with intact safeguards and one that has been stripped of those safeguards. We open-source a toolkit to estimate the safety gap for state-of-the-art open-weight models. As a case study, we evaluate biochemical and cyber capabilities, refusal rates, and generation quality of models from two families (Llama-3 and Qwen-2.5) across a range of parameter scales (0.5B to 405B) using different safeguard removal techniques. Our experiments reveal that the safety gap widens as model scale increases and effective dangerous capabilities grow substantially when safeguards are removed. We hope that the Safety Gap Toolkit (https://github.com/AlignmentResearch/safety-gap) will serve as an evaluation framework for common open-source models and as a motivation for developing and testing tamper-resistant safeguards. We welcome contributions to the toolkit from the community.