{"total":11,"items":[{"citing_arxiv_id":"2606.27195","ref_index":12,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"HALO II: Constraining Hubble constant $H_{0}$ through continuum delay fitting of Fairall 9","primary_cat":"astro-ph.GA","submitted_at":"2026-06-25T15:55:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Using simultaneous modeling of continuum lag-spectrum and broadband SED of Fairall 9 with the H0RIZON-AGN model, the authors obtain H0 = 72.4_{-3.7}^{+3.4} km s^{-1} Mpc^{-1}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25205","ref_index":77,"ref_count":3,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A new $H_0$ measurement with SNe Requiem and Encore using $\\texttt{Gravity.jl}$","primary_cat":"astro-ph.CO","submitted_at":"2026-06-23T21:54:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New H0 = 67.0 +9.3/-7.8 km/s/Mpc from joint lens-model fit to time delays of SN Requiem and SN Encore in MACS J0138.0-2155.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12980","ref_index":7,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Review on Resolving the Hubble Tension via Late-Universe Physics","primary_cat":"astro-ph.CO","submitted_at":"2026-06-11T07:13:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A review of late-universe models concludes that DESI BAO plus uncalibrated supernovae data indicate the Hubble tension originates in new low-redshift physics.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"usually entail an elevated baryon density, thereby exacerbating tensions with Big Bang nucleosynthesis [183,184]. Analyses of quasar lensing suggest that the Hubble constant https://doi.org/10.3390/galaxies1010000 Galaxies2026,1, 0 16 of 33 inferred from strongly lensed quasar time delays (H0LiCOW) exhibits a mild decline with increasing lens redshift [7]. This trend is statistically modest, with a significance of approxi- mately 1.9σ. However, with the inclusion of a new H0 measurement [111], the significance has decreased to 1.7 σ [97]. Although a decreasing trend in H0 has been observed via strongly lensed quasars, it is important to note that time-delay cosmography is a relatively novel probe compared to the well-established observations of SNe Ia."},{"citing_arxiv_id":"2606.02712","ref_index":259,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario","primary_cat":"astro-ph.CO","submitted_at":"2026-06-01T18:00:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"High-redshift datasets constrain the local void gravitational redshift parameter z0 to be consistent with zero but allow the value needed for Hubble tension solution.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23637","ref_index":98,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Long-term optical and near-infrared photometric evolution of SN 2019vxm, an interacting Type IIn supernova","primary_cat":"astro-ph.HE","submitted_at":"2026-05-22T13:51:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Long-term multi-band photometry of SN 2019vxm shows initial thick CSM interaction, photosphere decoupling at 80-100 days, long-lasting dust emission, and a possible outer CSM rebrightening, implying a massive progenitor with extreme pre-explosion mass loss.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13514","ref_index":47,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"COOL-LAMPS IX: A Rare Duo of Quasars Each Lensed by a Single Massive Galaxy Cluster","primary_cat":"astro-ph.GA","submitted_at":"2026-05-13T13:33:24+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A single galaxy cluster lenses two quasars (one Type I at z=1.524, one dust-obscured Type II at z=1.939) into four images each, yielding a projected mass of ~3.3e14 solar masses within 500 kpc and time delays of hundreds to over 1000 days.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05691","ref_index":7,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"From Scalar $H_0$ to $E(z)$: A Reformulation of the Hubble Tension","primary_cat":"astro-ph.CO","submitted_at":"2026-05-07T05:32:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Re-expressing the Hubble tension via posterior-implied E(z) histories yields moderate mismatches (S_hist of 1.65 and 2.55) that correspond to only 1.1-2.1 sigma equivalents, below the usual 4.9 sigma scalar-H0 discrepancy.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Brink,et al.Astrophys. J. Lett.934, no.1, L7 (2022) doi:10.3847/2041- 8213/ac5c5b [arXiv:2112.04510 [astro-ph.CO]]. [6] E. Abdalla, G. Franco Abell' an, A. Aboubrahim, A. Agnello, O. Akarsu, Y. Akrami, G. Alestas, D. Aloni, L. Amendola and L. A. Anchordoqui,et al.JHEAp34, 49-211 (2022) doi:10.1016/j.jheap.2022.04.002 [arXiv:2203.06142 [astro-ph.CO]]. [7] K. C. Wonget al.[H0LiCOW], Mon. Not. Roy. Astron. Soc.498, no.1, 1420-1439 (2020) doi:10.1093/mnras/stz3094 [arXiv:1907.04869 [astro-ph.CO]]. [8] W. L. Freedman, B. F. Madore, D. Hatt, T. J. Hoyt, I. S. Jang, R. L. Beaton, C. R. Burns, M. G. Lee, A. J. Monson and J. R. Neeley,et al.Astrophys. J.882, 34 (2019) doi:10.3847/1538-4357/ab2f73 [arXiv:1907."},{"citing_arxiv_id":"2605.05318","ref_index":69,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"HOLISMOKES XXI: Detecting strongly lensed type Ia supernovae from time series of multi-band LSST-like imaging data -- Part II","primary_cat":"astro-ph.IM","submitted_at":"2026-05-06T18:00:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A convLSTM classifier identifies lensed SNe Ia in simulated LSST-like time series, reaching ~60% true-positive rate at O(10^{-4}) false-positive rate by the seventh epoch even after adding realistic PSF variations and foreground SN contaminants.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.05849","ref_index":12,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Probing the Evolution of Dark Energy: A Joint Analysis of DESI DR2, Pantheon+, and Cosmic Chronometers","primary_cat":"astro-ph.CO","submitted_at":"2026-04-07T13:13:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Joint analysis of DESI DR2, Pantheon+, and cosmic chronometers yields a mild statistical preference for time-varying dark energy over LambdaCDM, though constraints on the evolution remain moderate.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"R. Ch 'avez, F. Bresolin, E. Telles, M. Plionis and S. Basi- lakos, Mon. Not. Roy. Astron. Soc.474(2018) no.1, 1250- 1276 doi:10.1093/mnras/stx2710 [arXiv:1710.05951 [astro- ph.CO]]. [11] A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scol- nic, Astrophys. J.876(2019) no.1, 85 doi:10.3847/1538- 4357/ab1422 [arXiv:1903.07603 [astro-ph.CO]]. [12] K. C. Wonget al.[H0LiCOW], Mon. Not. Roy. Astron. Soc. 498(2020) no.1, 1420-1439 doi:10.1093/mnras/stz3094 [arXiv:1907.04869 [astro-ph.CO]]. [13] W. L. Freedman, B. F. Madore, D. Hatt, T. J. Hoyt, I. S. Jang, R. L. Beaton, C. R. Burns, M. G. Lee, A. J. Mon- son and J. R. Neeley,et al.Astrophys. J.882(2019), 34 doi:10.3847/1538-4357/ab2f73 [arXiv:1907."},{"citing_arxiv_id":"2604.02418","ref_index":44,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Supernova 2025wny: High-angular resolution Keck/NIRC2 observations and preliminary lens modeling","primary_cat":"astro-ph.GA","submitted_at":"2026-04-02T18:00:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"High-resolution Keck observations and dual-code lens modeling of the first lensed Type I superluminous supernova give sub-milliarcsecond position fits and masses of 4.44 and 0.96 times 10^11 solar masses for the primary and secondary lenses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.11041","ref_index":113,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature","primary_cat":"astro-ph.CO","submitted_at":"2025-12-11T19:00:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"KiDS-Legacy cosmic shear plus external probes yields S8 = 0.816 ± 0.006 in Lambda-CDM and consistent bounds on w0, wa, sum m_nu and Omega_K with no strong preference for extensions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}