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JWST/NIRSpec Prism spectra for 25 z>=10 galaxies finds burstiness correlates with strong UV lines, short depletion times, and DLA-induced redshift biases of 0.39 and 0.14 with marginal impact on UV luminosity density.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30757","ref_index":183,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T18:00:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"SKAO continuum surveys will detect radio emission from JWST AGN and LRDs and distinguish between Compton-thick absorption, intrinsically weak accretion, and dense gas cocoon scenarios.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30746","ref_index":7,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Introducing AuriGLOBES: the effect of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T18:00:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"AuriGLOBES is a new subgrid model implemented in Auriga simulations that incorporates compressive tides and compact-object mass loss to transform an initial Schechter mass function into observed globular cluster populations while reproducing the GC system mass-halo mass relation.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"Lastly, the cloud free-fall time is defined as tff,2D= √ 2π κ ,(6) whereκis the epicyclic frequency that is computed from the tidal tensor at the location of the particle (see appendix B.1), as demonstrated by Pfeffer et al. (2018) and Reina-Campos et al. (2022a). The Toomre mass is obtained from the parent gas cell for each new star particle through MT =4π 5G2 Σ3 g κ4 ,(7) whereΣ g is the local surface gas density estimated assuming hydrostatic equilibrium, i.e. equating the mid-plane pressure of an equilibrium disc to the pressure of the parent gas cell (Krumholz & McKee 2005): Σg = s 2Pg πGϕP ,(8) 4 As noted by Pfeffer et al. (2018), the variation ofϵestimates is much smaller than the dynamical range of the productΓM GMC,max making it"},{"citing_arxiv_id":"2606.30719","ref_index":7,"ref_count":4,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Global trends in morphology from massive to dwarf galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Galaxies become less concentrated, more asymmetric and less clumpy toward lower stellar masses, with bar fraction declining to zero near 10^8 solar masses and CAS parameters losing separating power in the dwarf regime.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30633","ref_index":29,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"GIGA-Lens 2.0: Strong-Lens Modeling on Multiple GPU 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uniform grid, achieving comparable fits with roughly half the pixels per dimension and higher ELBOs on mock data.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30438","ref_index":249,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"CARMApy: An Open-Source Python Framework for Simulating Microphysical Clouds in Planetary Atmospheres","primary_cat":"astro-ph.EP","submitted_at":"2026-06-29T15:13:37+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"CARMApy provides a Python interface to the ExoCARMA microphysics code, enabling simulation of cloud particle size distributions and rates in exoplanet atmospheres with claimed consistency to prior versions and speed gains of 1.9x single-threaded and 3.8x multithreaded.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30390","ref_index":149,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"SN 2019vxm: A luminous and long-lived Type IIn supernova with early flash-ionisation features","primary_cat":"astro-ph.SR","submitted_at":"2026-06-29T14:44:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"SN 2019vxm is a luminous, long-lived Type IIn supernova showing early flash-ionization features, a power-law bolometric light curve, and mid-IR dust formation, with a progenitor mass-loss rate lower limit of at least 0.01 solar masses per year.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30224","ref_index":36,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Cosmology with 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