GREX-PLUS Science Book v2

arXiv:2606.05237 · astro-ph.IM, astro-ph.EP, astro-ph.GA, astro-ph.HE, astro-ph.SR · Submitted 2026-06-03 · Read on arXiv

ISAS/JAXA · ISAS/JAXA · ISAS/JAXA · Universita di Bologna · INAF - Osservatorio Astronomico di Padova / Universita di Bologna · INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna · Chiba University · NAOJ · University of Tokyo · Nagoya University · Waseda University · University of Osaka · ISAS/JAXA / University of Tokyo · University of Osaka · Kyoto University · Ludwig-Maximilians-University / University of Nottingham · Tohoku University · NAOJ · University of Tokyo · University of Osaka · Ghent University · University of Tokyo · University of Osaka · Ehime University · Kwansei Gakuin University · Shinshu University · ISAS/JAXA · INAF - Osservatorio Astronomico di Padova · NAOJ · NAOJ · University of Osaka / University of Tokyo / University of Nevada Las Vegas · Kanazawa University · NAOJ · University of Tokyo · University of Occupational and Environmental Health · NAOJ · INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna · INAF - Osservatorio Astronomico di Padova · INAF - Osservatorio Astronomico di Padova · University of Padova · Kyoto Sangyo University · University of Tokyo · Niigata University · Hokkai-Gakuen University · Tohoku University · ASIAA · JAMSTEC · University of Tokyo · NAOJ · Ritsumeikan University · INAF - Astronomical Observatory of Rome · DAWN / Technical University of Denmark · INAF - Osservatorio Astronomico di Padova · NAOJ · NAOJ · INAF - Arcetri Astrophysical Observatory

astro-ph.IM, astro-ph.EP, astro-ph.GA, astro-ph.HE, astro-ph.SR

Submitted: 2026-06-03

Updated: 2026-09-23

Comments: This is a major updated version from arXiv:2304.08104

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• AGN — 210× in this paper · explained in 1 episode
• Metallicity — 49× in this paper · explained in 3 episodes
• Abundance — 46× in this paper · explained in 1 episode
• Wide-Field Camera — 28× in this paper
• Trace — 19× in this paper · explained in 2 episodes
• Aperture — 18× in this paper · explained in 1 episode
• Dust Attenuation — 15× in this paper · explained in 2 episodes
• Core — 14× in this paper · explained in 2 episodes
• Accuracy — 11× in this paper · explained in 1 episode
• Clustering — 10× in this paper · explained in 2 episodes
• James Webb Space Telescope — 9× in this paper
• Active Galactic Nuclei — 8× in this paper
• Stellar Feedback — 8× in this paper · explained in 2 episodes
• Elias — 6× in this paper · explained in 2 episodes
• AGN Feedback — 5× in this paper · explained in 1 episode
• Benchmark — 5× in this paper · explained in 2 episodes
• Extra-Galactic Sciences — 5× in this paper
• Galactic and Planetary Sciences — 5× in this paper
• Little Red Dots — 5× in this paper · explained in 2 episodes
• Consistency — 4× in this paper · explained in 3 episodes
• Fidelity — 4× in this paper · explained in 2 episodes
• High Latitude Wide Area Survey — 4× in this paper
• Active Galactic Nuclei (AGN) — 3× in this paper · explained in 1 episode
• Cataclysmic Variables (CVs) — 3× in this paper · explained in 2 episodes
• High Resolution Spectrometer — 3× in this paper
• Infrared Space Observatory — 3× in this paper
• North Ecliptic Pole — 3× in this paper
• Transmission spectroscopy — 3× in this paper · explained in 2 episodes
• Adam — 2× in this paper · explained in 2 episodes
• Aggregation — 2× in this paper · explained in 1 episode
• Asymptotic Giant Branch — 2× in this paper
• Gravitational Lensing — 2× in this paper · explained in 2 episodes
• Homogeneity — 2× in this paper · explained in 2 episodes
• Hubble Space Telescope — 2× in this paper
• Microlensing — 2× in this paper · explained in 2 episodes
• Short Wavelength Spectrometer — 2× in this paper
• Society of Photo-Optical Instrumentation Engineers — 2× in this paper
• Velocity Dispersion — 2× in this paper · explained in 2 episodes
• Accretion Efficiency — 1× in this paper · explained in 2 episodes
• Adaptive Optics (AO) — 1× in this paper · explained in 2 episodes
• Anisotropy — 1× in this paper · explained in 3 episodes
• Anti-correlation — 1× in this paper · explained in 3 episodes
• COSMOS Deep Drilling Field — 1× in this paper
• Calibration — 1× in this paper · explained in 7 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Environmental Quenching — 1× in this paper · explained in 2 episodes
• European Space Agency — 1× in this paper
• Green Bank Telescope — 1× in this paper
• Legacy Survey of Space and Time — 1× in this paper
• Polycyclic aromatic hydrocarbons (PAHs) — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• Sloan Digital Sky Survey — 1× in this paper
• Thirty Meter Telescope — 1× in this paper
• Verification — 1× in this paper · explained in 2 episodes
• Visible and Infrared Survey Telescope for Astronomy — 1× in this paper

Sources

• JWST ASPIRE: How Did Galaxies Complete Reionization? Evidence for Excess IGM Transmission around ${\rm [O\,{\scriptstyle III}]}$ Emitters during Reionization
• JWST Spectroscopic Insights Into the Diversity of Galaxies in the First 500 Myr: Short-Lived Snapshots Along a Common Evolutionary Pathway
• DeepDive: A deep dive into the physics of the first massive quiescent galaxies in the Universe
• Encyclopedia Magneticum: Scaling Relations from Cosmic Dawn to Present Day
• Diversity and Evolution of Dust Attenuation Curves from Redshift z ~ 1 to 9
• Spatially resolved PAH$_{3.3}$ emission and stellar ages in ram pressure stripped clumps at $z\sim0.3$
• A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13
• No Luminous Little Red Dots: A Sharp Cutoff in Their Luminosity Function
• A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots
• The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s
• LISA Definition Study Report
• GREX-PLUS Science Book
• LSST Science Book, Version 2.0
• PRIMA General Observer Science Book Volume 2
• AGN Variability with Rubin Observatory in the 2030s
• VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability
• Scalable and Robust Multiband Modeling of AGN Light Curves in Rubin-LSST
• Roman Observations Time Allocation Committee: Final Report and Recommendations
• The Detection of Hot Molecular Cores in the Small Magellanic Cloud
• ExoJAX Retrievals of VLT/CRIRES Spectra of Luhman 16AB: C/O Ratios and Systematic Uncertainties

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• Towards independent event horizon imaging of the supermassive black holes in M87 and the Milky Way
• A PINK update: Improvements to the CELEBI fast radio burst data reduction and analysis pipeline