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View article: AstroMLab 5: Structured Summaries and Concept Extraction for 400,000 Astrophysics Papers
AstroMLab 5: Structured Summaries and Concept Extraction for 400,000 Astrophysics Papers Open
We present a dataset of 408,590 astrophysics papers from arXiv (astro-ph), spanning 1992 through July 2025. Each paper has been processed through a multi-stage pipeline to produce: (1) structured summaries organized into six semantic secti…
View article: LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data Open
Cosmic microwave background (CMB) photons are deflected by large-scale structure through gravitational lensing. This secondary effect introduces higher-order correlations in CMB anisotropies, which are used to reconstruct lensing deflectio…
View article: SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field Open
We present measurements of the temperature and E-mode polarization angular power spectra of the cosmic microwave background (CMB) from observations of 4% of the sky with SPT-3G, the current camera on the South Pole Telescope (SPT). The map…
View article: Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs Open
Context. The South Pole Telescope third-generation camera (SPT-3G) has observed over 10,000 square degrees of sky at 95, 150, and 220 GHz (3.3, 2.0, 1.4 mm, respectively) overlapping the ongoing 14,000 square-degree Euclid Wide Survey. The…
View article: Constraints on Inflationary Gravitational Waves with Two Years of SPT-3G Data
Constraints on Inflationary Gravitational Waves with Two Years of SPT-3G Data Open
We present a measurement of the $B$-mode polarization power spectrum of the cosmic microwave background anisotropies at 32 $\le$ $\ell$ $<$ 502 for three bands centered at 95, 150, and 220 GHz using data from the SPT-3G receiver on the Sou…
View article: Detection of Thermal Emission at Millimeter Wavelengths from Low-Earth Orbit Satellites
Detection of Thermal Emission at Millimeter Wavelengths from Low-Earth Orbit Satellites Open
The detection of satellite thermal emission at millimeter wavelengths is presented using data from the 3rd-Generation receiver on the South Pole Telescope (SPT-3G). This represents the first reported detection of thermal emission from arti…
View article: Achieving GPT-4o level performance in astronomy with a specialized 8B-parameter large language model
Achieving GPT-4o level performance in astronomy with a specialized 8B-parameter large language model Open
View article: Cosmology from CMB lensing and delensed <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>E</mml:mi><mml:mi>E</mml:mi></mml:math> power spectra using 2019–2020 SPT-3G polarization data
Cosmology from CMB lensing and delensed power spectra using 2019–2020 SPT-3G polarization data Open
International audience
View article: The SPT-Deep Cluster Catalog: Sunyaev-Zel'dovich Selected Clusters from Combined SPT-3G and SPTpol Measurements over 100 Square Degrees
The SPT-Deep Cluster Catalog: Sunyaev-Zel'dovich Selected Clusters from Combined SPT-3G and SPTpol Measurements over 100 Square Degrees Open
We present a catalog of 500 galaxy cluster candidates in the SPT-Deep field: a 100 deg$^2$ field that combines data from the SPT-3G and SPTpol surveys to reach noise levels of 3.0, 2.2, and 9.0 $\mu$K-arcmin at 95, 150, and 220 GHz, respec…
View article: Development of SQUID Array Amplifiers for the LiteBIRD CMB Satellite
Development of SQUID Array Amplifiers for the LiteBIRD CMB Satellite Open
LiteBIRD is an upcoming JAXA-led mission that aims to measure primordial gravitational waves in the B-mode polarization of the cosmic microwave background. It is set to launch in 2032. The LiteBIRD detector array consists of around 5000 TE…
View article: Pointing Accuracy Improvements for the South Pole Telescope with Machine Learning
Pointing Accuracy Improvements for the South Pole Telescope with Machine Learning Open
We present improvements to the pointing accuracy of the South Pole Telescope (SPT) using machine learning. The ability of the SPT to point accurately at the sky is limited by its structural imperfections, which are impacted by the extreme …
View article: The Relational Dynamics of Space-Time
The Relational Dynamics of Space-Time Open
The Relational Dynamics of Space-Time is a groundbreaking theory that redefines space-time as an emergent and discrete structure, arising from fundamental interactions between elementary entities. Rooted in the principle that “nothing is e…
View article: Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space mission
Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space mission Open
Large angular scale surveys in the absence of atmosphere are essential for measuring the primordial B-mode power spectrum of the Cosmic Microwave Background (CMB). Since this proposed measurement is about three to four orders of magnitude …
View article: AstroMLab 3: Achieving GPT-4o Level Performance in Astronomy with a Specialized 8B-Parameter Large Language Model
AstroMLab 3: Achieving GPT-4o Level Performance in Astronomy with a Specialized 8B-Parameter Large Language Model Open
AstroSage-Llama-3.1-8B is a domain-specialized natural-language AI assistant tailored for research in astronomy, astrophysics, and cosmology. Trained on the complete collection of astronomy-related arXiv papers from 2007-2024 along with mi…
View article: AstroMLab 3: Achieving GPT-4o Level Performance in Astronomy with a Specialized 8B-Parameter Large Language Model
AstroMLab 3: Achieving GPT-4o Level Performance in Astronomy with a Specialized 8B-Parameter Large Language Model Open
AstroSage-Llama-3.1-8B is a domain-specialized natural-language AI assistant tailored for research in astronomy, astrophysics, cosmology, and astronomical instrumentation. Trained on the complete collection of astronomy-related arXiv paper…
View article: The LiteBIRD mission to explore cosmic inflation
The LiteBIRD mission to explore cosmic inflation Open
LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the Sun-Ear…
View article: Flaring Stars in a Nontargeted Millimeter-wave Survey with SPT-3G
Flaring Stars in a Nontargeted Millimeter-wave Survey with SPT-3G Open
We present a flare star catalog from 4 yr of nontargeted millimeter-wave survey data from the South Pole Telescope (SPT). The data were taken with the SPT-3G camera and cover a 1500 deg 2 region of the sky from 20 h 40 m 0 s to 3 h 20 m 0 …
View article: LiteBIRD Science Goals and Forecasts. Mapping the Hot Gas in the Universe
LiteBIRD Science Goals and Forecasts. Mapping the Hot Gas in the Universe Open
We assess the capabilities of the LiteBIRD mission to map the hot gas distribution in the Universe through the thermal Sunyaev-Zeldovich (SZ) effect. Our analysis relies on comprehensive simulations incorporating various sources of Galacti…
View article: Systematic effects induced by half-wave plate differential optical load and TES nonlinearity for LiteBIRD
Systematic effects induced by half-wave plate differential optical load and TES nonlinearity for LiteBIRD Open
LiteBIRD, a forthcoming satellite mission, aims to measure the polarization of the Cosmic Microwave Background (CMB) across the entire sky. The experiment will employ three telescopes, Transition-Edge Sensor (TES) bolometers and rotating H…
View article: AstroMLab 1: Who Wins Astronomy Jeopardy!?
AstroMLab 1: Who Wins Astronomy Jeopardy!? Open
We present a comprehensive evaluation of proprietary and open-weights large language models using the first astronomy-specific benchmarking dataset. This dataset comprises 4,425 multiple-choice questions curated from the Annual Review of A…
View article: Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensing
Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensing Open
We measure the stacked lensing signal in the direction of galaxy clusters in the Dark Energy Survey Year 3 (DES Y3) redMaPPer sample, using cosmic microwave background (CMB) temperature data from SPT-3G, the third-generation CMB camera on …
View article: MNTES: Modeling Nonlinearity of TES detectors for Enhanced Cosmic Microwave Background measurements with LiteBIRD
MNTES: Modeling Nonlinearity of TES detectors for Enhanced Cosmic Microwave Background measurements with LiteBIRD Open
Traditional methods of converting electronic readout counts to optical power incident on Transition Edge Sensors (TES) for Cosmic Microwave Background (CMB) observations involve a linear approximation. For the upcoming LiteBIRD CMB satelli…
View article: SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region
SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region Open
We present an extension to a Sunyaev–Zel’dovich Effect (SZE) selected cluster catalogue based on observations from the South Pole Telescope (SPT); this catalogue extends to lower signal to noise than the previous SPT–SZ catalogue and there…
View article: Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD
Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD Open
We present a study of the impact of a beam far side-lobe lack of knowledge on the measurement of the Cosmic Microwave Background B -mode signal at large scale. Beam far side-lobes induce a mismatch in the transfer function of Galactic fore…
View article: LiteBIRD science goals and forecasts: improving sensitivity to inflationary gravitational waves with multitracer delensing
LiteBIRD science goals and forecasts: improving sensitivity to inflationary gravitational waves with multitracer delensing Open
We estimate the efficiency of mitigating the lensing B -mode polarization, the so-called delensing, for the LiteBIRD experiment with multiple external data sets of lensing-mass tracers. The current best bound on the tensor-to-scalar ratio,…
View article: Development of the Low Frequency Telescope focal plane detector arrays for LiteBIRD
Development of the Low Frequency Telescope focal plane detector arrays for LiteBIRD Open
LiteBIRD, a forthcoming JAXA mission, aims to accurately study the microwave sky within the 40-400 GHz frequency range divided into 15 distinct nominal bands. The primary objective is to constrain the CMB inflationary signal, specifically …
View article: Understanding the Phase of Responsivity and Noise Sources in Frequency-Domain Multiplexed Readout of Transition Edge Sensor Bolometers
Understanding the Phase of Responsivity and Noise Sources in Frequency-Domain Multiplexed Readout of Transition Edge Sensor Bolometers Open
Cosmic microwave background (CMB) experiments have deployed focal planes with $$\mathcal {O}(10^{4})$$ transition edge sensor (TES) bolometers cooled to sub-Kelvin temperatures by multiplexing the readout of many TES channels onto …
View article: A Method of Measuring TES Complex ETF Response in Frequency-domain Multiplexed Readout by Single Sideband Power Modulation
A Method of Measuring TES Complex ETF Response in Frequency-domain Multiplexed Readout by Single Sideband Power Modulation Open
The digital frequency domain multiplexing (DfMux) technique is widely used for astrophysical instruments with large detector arrays. Detailed detector characterization is required for instrument calibration and systematics control. We cond…
View article: Calibration of detector time constant with a thermal source for the POLARBEAR-2A CMB polarization experiment
Calibration of detector time constant with a thermal source for the POLARBEAR-2A CMB polarization experiment Open
The Simons Array (SA) project is a ground-based Cosmic Microwave Background (CMB) polarization experiment. The SA observes the sky using three telescopes, and POLARBEAR-2A (PB-2A) is the receiver system on the first telescope. For the grou…
View article: First Constraints on the Epoch of Reionization Using the non-Gaussianity\n of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope\n and {\\it Herschel}-SPIRE Observations
First Constraints on the Epoch of Reionization Using the non-Gaussianity\n of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope\n and {\\it Herschel}-SPIRE Observations Open
We report results from an analysis aimed at detecting the trispectrum of the\nkinematic Sunyaev-Zel{'}dovich (kSZ) effect by combining data from the South\nPole Telescope (SPT) and {\\it Herschel}-SPIRE experiments over a 100 ${\\rm\ndeg}^…