{"total":10,"items":[{"citing_arxiv_id":"2606.30746","ref_index":140,"ref_count":1,"confidence":0.88,"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":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27426","ref_index":280,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Too shy to spin? 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