#quicklook
📄 Simulating galaxy formation with the IllustrisTNG model

Quicklook:
Pillepich, Annalisa et al. (2018) · Monthly Notices of the Royal Astronomical Society
Reads: 526 · Citations: 1936
DOI: 10.1093/mnras/stx2656

#Astronomy #Astrophysics #Cosmology #MethodsNumerical #GalaxiesEvolution
Simulating galaxy formation with the IllustrisTNG model
We introduce an updated physical model to simulate the formation and evolution of galaxies in cosmological, large-scale gravity+magnetohydrodynamical simulations with the moving mesh code AREPO. The overall framework builds upon the successes of the Illustris galaxy formation mod
ui.adsabs.harvard.edu
January 6, 2026 at 7:23 AM
📄 Magnetogenesis and the Cosmic Web: A Joint Challenge for Radio Observ…

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Vazza, Franco et al. (2021) · Galaxies
Reads: 92 · Citations: 41
DOI: 10.3390/galaxies9040109

#Astronomy #Astrophysics #RadioAstronomy #GalaxyClusters #GeneralTechniques
Magnetogenesis and the Cosmic Web: A Joint Challenge for Radio Observations and Numerical Simulations
The detection of the radio signal from filaments in the cosmic web is crucial to distinguish possible magnetogenesis scenarios. We review the status of the different attempts to detect the cosmic web at radio wavelengths. This is put into the context of the advanced simulations o
ui.adsabs.harvard.edu
January 6, 2026 at 7:19 AM
📄 Verifying the Australian MWA EoR pipeline II: Fundamental limits of t…

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Line, Jack Laurence Bramble et al. (2025) · Publications of the Astronomical Society of Australia
Reads: 119 · Citations: 2
DOI: 10.1017/p…

#Astronomy #Astrophysics #Cosmology #AstronomyDataAnalysis #Reionisat…
Verifying the Australian MWA EoR pipeline II: Fundamental limits of the AusEoRPipe and the impact of instrumental effects
Detection of the weak cosmological signal from high-redshift hydrogen demands careful data analysis and an understanding of the full instrument signal chain. Here, we use the WODEN simulation pipeline to produce realistic data from the Murchison Widefield Array (MWA) Epoch of Rei
ui.adsabs.harvard.edu
January 6, 2026 at 7:12 AM
📄 The JWST EXCELS survey: A spectroscopic investigation of the ionizing…

Quicklook:
Begley, R. et al. (2026) · Monthly Notices of the Royal Astronomical Society
Reads: 12182 · Citations: 3
DOI: 10.1093/mnras/staf1995

#Astronomy #Astrophysics #Cosmology #GalaxiesEvolution #GalaxiesHighredshift
The JWST EXCELS survey: A spectroscopic investigation of the ionizing properties of star-forming galaxies at 1<z<8
Charting the Epoch of Reionization demands robust assessments of what drives the production of ionizing photons in high-redshift star-forming galaxies (SFGs) and requires better predictive capabilities from current observations. Using a sample of <inline-formula><tex-math>$N=159$
ui.adsabs.harvard.edu
January 6, 2026 at 7:08 AM
📄 Deep Residual Learning for Image Recognition

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He, Kaiming et al. (2016) · 2016 IEEE Conference on Computer Vision and Pattern Recognition (CVPR)
Reads: 45017 · Citations: 27779
DOI: 10.1109/CVPR.2016.90

#Astronomy #Astrophysics #AstroAI #ComputerScienceComputerVisionAndPatternReco…
Deep Residual Learning for Image Recognition
Deeper neural networks are more difficult to train. We present a residual learning framework to ease the training of networks that are substantially deeper than those used previously. We explicitly reformulate the layers as learning residual functions with reference to the layer
ui.adsabs.harvard.edu
January 6, 2026 at 7:03 AM
📄 Thevesh/paper-meco-maps: Fix naming of 1958 delim

Quicklook:
Theva, Thevesh et al. (2026) · Zenodo
Reads: 0 · Citations: 1
DOI: 10.5281/zenodo.18093017

#Astronomy #Astrophysics
Thevesh/paper-meco-maps: Fix naming of 1958 delim
The delimitation exercise was conducted and concluded in 1958, not 1959.
ui.adsabs.harvard.edu
January 6, 2026 at 7:03 AM
Sword and Starfall Quick Look
YouTube video by GamerWolfSix
youtu.be
January 6, 2026 at 12:19 AM
Jessica Plichta arrested but I believe over the organized march, not the interview or comments at the time of arrest. Still a very stupid time to pick her up and for pretty lame reasons. AI quick info on her...

#GRPD #Plichta #AI #research #QuickLook #arrested #Protest #Organizer #dignity
January 5, 2026 at 8:38 PM
Oh, dat is wel een heel interessant programma met veel mogelijkheden! Thanks! En het geeft zelfs nog tips voor andere preview apps:

'File Preview built-in (Press Spacebar). Additional support for QuickLook and Seer'. Die kende ik ook nog niet.
January 5, 2026 at 2:51 PM
📄 MCNPX benchmark for cosmic ray interactions with the Moon

Quicklook:
McKinney, G. W. et al. (2006) · Journal of Geophysical Research (Planets)
Reads: 1 · Citations: 84
DOI: 10.1029/2005JE002551

#Astronomy #Astrophysics #PlanetaryScience #OceanographyGeneralNumericalModeling0545 #0560
MCNPX benchmark for cosmic ray interactions with the Moon
The MCNPX radiation transport code is used to simulate cosmic ray interactions within the Moon. Accurate source, geometric, and physics models are developed to successfully benchmark neutron density results with Apollo 17 measurements. The peak of the MCNPX lunar neutron density
ui.adsabs.harvard.edu
January 4, 2026 at 5:27 AM
📄 The ROSAT mission

Quicklook:
Truemper, J. et al. (1982) · Advances in Space Research
Reads: 5 · Citations: 672
DOI: 10.1016/0273-1177(82)90070-9

#Astronomy #Astrophysics #AstronomicalObservatories #MissionPlanning #RosatMission
The ROSAT mission
A primary scientific objective of the ROSAT mission is to perform the first all-sky survey with an imaging X-ray telescope leading to an improvement in sensitivity by several orders of magnitude compared with previous surveys. A large number of new sources (≳ 10<SUP>5</SUP>) will
ui.adsabs.harvard.edu
January 4, 2026 at 5:21 AM
📄 Observations and Orbits of Comets and a/ Objects

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Skiff, B. A. et al. (2025) · Minor Planet Electronic Circulars
Reads: 2 · Citations: 0
DOI: 10.48377/MPEC/2025-O159

#Astronomy #Astrophysics #SmallSolarSystemBodies #ObservationsAndOrbitsOfCometsAndAObjects #1469
Observations and Orbits of Comets and a/ Objects
NASA ADS abstract
ui.adsabs.harvard.edu
January 4, 2026 at 5:19 AM
Frostpunk 2 Part 9 Outside Resources:
youtu.be/CnEFYA6Lqec
#frostpunk #frostpunk2 #quicklook
Frostpunk 2 Part 9 Outside Resources
YouTube video by GamerWolfSix
youtu.be
January 2, 2026 at 12:34 AM
📄 Differences between CME-driven storms and CIR-driven storms

Quicklook:
Borovsky, Joseph E. et al. (2006) · Journal of Geophysical Research (Space Physics)
Reads: 2 · Citations: 470
DOI: 10.1029/2005JA011447

#Astronomy #Astrophysics #SolarPhysics #MagnetosphericPhysicsMagneticStormsAndSubsto…
Differences between CME-driven storms and CIR-driven storms
Twenty one differences between CME-driven geomagnetic storms and CIR-driven geomagnetic storms are tabulated. (CME-driven includes driving by CME sheaths, by magnetic clouds, and by ejecta; CIR-driven includes driving by the associated recurring high-speed streams.) These differe
ui.adsabs.harvard.edu
December 30, 2025 at 11:48 AM
📄 Restrictions on initial conditions in cosmological scenarios and impl…

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Baumgarte, Thomas W. et al. (2025) · Physical Review D
Reads: 9655 · Citations: 0
DOI: 10.1103/9nsk-jy7f

#Astronomy #Astrophysics #Cosmology #GeneralRelativityAndQuantumCosmology #CosmologyAndNongalacticA…
Restrictions on initial conditions in cosmological scenarios and implications for simulations of primordial black holes and inflation
Numerical relativity simulations provide a means by which to study the evolution and end point of strong overdensities in cosmological spacetimes. Specific applications include studies of primordial black hole formation and the robustness of inflation. Here we adopt a toy model p
ui.adsabs.harvard.edu
December 30, 2025 at 11:41 AM
📄 Modules for Experiments in Stellar Astrophysics (MESA)

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Paxton, Bill et al. (2011) · The Astrophysical Journal Supplement Series
Reads: 482 · Citations: 4139
DOI: 10.1088/0067-0049/192/1/3

#Astronomy #Astrophysics #SolarPhysics #MethodsNumerical #StarsEvolution
Modules for Experiments in Stellar Astrophysics (MESA)
Stellar physics and evolution calculations enable a broad range of research in astrophysics. Modules for Experiments in Stellar Astrophysics (MESA) is a suite of open source, robust, efficient, thread-safe libraries for a wide range of applications in computational stellar astrop
ui.adsabs.harvard.edu
December 30, 2025 at 11:32 AM
It's been a while. I loved the vibes. I bought it based entirely on a Giant Bomb quicklook.
December 30, 2025 at 3:46 AM
Nerus Quick Look
YouTube video by GamerWolfSix
youtu.be
December 29, 2025 at 10:44 PM
📄 Field testing and evaluation of a solar-blind UV communication link f…

Quicklook:
Shaw, Gary A. et al. (2004) · Unattended/Unmanned Ground, Ocean, and Air Sensor Technologies and Applications VI
Reads: 0 · Citations: 13


#Astronomy #Astrophysics #SolarPhysics
Field testing and evaluation of a solar-blind UV communication link for unattended ground sensors
Non-line-of-sight ultraviolet (UV) communication technology to support unattended ground sensor communication is described. The concept exploits atmospheric scattering of ultraviolet light to achieve modest data rates under non line-of-sight (ground-to-ground) and obstructed line
ui.adsabs.harvard.edu
December 29, 2025 at 7:31 AM
📄 Random Forests.

Quicklook:
Breiman, Leo et al. (2001) · Machine Learning
Reads: 14 · Citations: 31413
DOI: 10.1023/A:1010933404324

#Astronomy #Astrophysics #AstroAI #MachineLearning
Random Forests.
Random forests are a combination of tree predictors such that each tree depends on the values of a random vector sampled independently and with the same distribution for all trees in the forest. The generalization error for forests converges a.s. to a limit as the number of trees
ui.adsabs.harvard.edu
December 29, 2025 at 7:28 AM
📄 Space Weather Modeling Framework: A new tool for the space science co…

Quicklook:
Tóth, GáBor et al. (2005) · Journal of Geophysical Research (Space Physics)
Reads: 4 · Citations: 663
DOI: 10.1029/2005JA011126

#Astronomy #Astrophysics #SolarPhysics #SpaceWeatherForecasting2722 #SpaceWeather…
Space Weather Modeling Framework: A new tool for the space science community
The Space Weather Modeling Framework (SWMF) provides a high-performance flexible framework for physics-based space weather simulations, as well as for various space physics applications. The SWMF integrates numerical models of the Solar Corona, Eruptive Event Generator, Inner Hel
ui.adsabs.harvard.edu
December 29, 2025 at 7:21 AM
📄 Astrochemistry During the Formation of Stars

Quicklook:
Jørgensen, Jes K. et al. (2020) · Annual Review of Astronomy and Astrophysics
Reads: 144 · Citations: 249
DOI: 10.1146/annurev-astro-032620-021927

#Astronomy #Astrophysics #SolarPhysics #AstrophysicsSolarAndStellarAstrophysics #Astroph…
Astrochemistry During the Formation of Stars
Star-forming regions show a rich and varied chemistry, including the presence of complex organic molecules—in both the cold gas distributed on large scales and the hot regions close to young stars where protoplanetary disks arise. Recent advances in observational techniques have
ui.adsabs.harvard.edu
December 28, 2025 at 3:46 PM
📄 Planck 2013 results. XVI. Cosmological parameters

Quicklook:
Planck Collaboration et al. (2014) · Astronomy and Astrophysics
Reads: 1097 · Citations: 8359
DOI: 10.1051/0004-6361/201321591

#Astronomy #Astrophysics #Cosmology #CosmicBackgroundRadiation #CosmologicalParameters
Planck 2013 results. XVI. Cosmological parameters
This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. We find that the Planck spectra at high multipoles (ℓ ≳ 40) are extremely well described by the standard spati
ui.adsabs.harvard.edu
December 28, 2025 at 2:02 PM
📄 Limits on the 21 cm Power Spectrum at z = 6.5–7.0 from Murchison Wide…

Quicklook:
Nunhokee, C. D. et al. (2025) · The Astrophysical Journal
Reads: 284 · Citations: 19
DOI: 10.3847/1538-4357/adda45

#Astronomy #Astrophysics #Cosmology #Reionization #HILineEmission
Limits on the 21 cm Power Spectrum at z = 6.5–7.0 from Murchison Widefield Array Observations
This paper presents the spherically averaged 21 cm power spectrum derived from Epoch of Reionization (EoR) observations conducted with the Murchison Widefield Array (MWA). The analysis uses EoR0-field data, centered at (R.A. = 0h, decl. = ‑27<SUP>∘</SUP>), collected between 2013
ui.adsabs.harvard.edu
December 28, 2025 at 1:55 PM