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Gamma rays from the quasar PKS 1441+25: story of an escape

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2015)cite arxiv:1512.04434Comment: 7 pages, 3 figures, published in ApJ Letters 815, L22 (2015).

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Quasars Probing Quasars VI. Excess HI Absorption Within One Proper Mpc of z~2 Quasars, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1308.6222Comment: Accepted to ApJ; 38 pages, 25 figures. Comments still welcome.Gaia GraL: Gaia DR2 Gravitational Lens Systems. VI. Spectroscopic Confirmation and Modeling of Quadruply-Imaged Lensed Quasars, , , , , , , , , and 16 other author(s). (2020)cite arxiv:2012.10051Comment: 18 pages, 8 figures; submitted to ApJ.A Highly Magnified Gravitationally Lensed Red QSO at z = 2.5 with a Significant Flux Ratio Anomaly, , , , , , , , , and 5 other author(s). (2022)cite arxiv:2211.03866Comment: Accepted for publication in ApJ; 29 pages, 18 figures, 8 tables. arXiv admin note: text overlap with arXiv:1807.05434.A fast radio burst localised to a massive galaxy, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1907.01542Comment: Submitted version of article published online at Nature via Accelerated Article Preview (https://doi.org/10.1038/s41586-019-1389-7). 34 pages, 6 figures, 2 tables.Gamma rays from the quasar PKS 1441+25: story of an escape, , , , , , , , , and 96 other author(s). (2015)cite arxiv:1512.04434Comment: 7 pages, 3 figures, published in ApJ Letters 815, L22 (2015).Extreme Variability in a Broad Absorption Line Quasar, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1704.03923Comment: 6 pages, 4 figures; accepted for publication in ApJ.Clustering on very small scales from a large sample of confirmed quasar pairs: Does quasar clustering track from Mpc to kpc scales?, , , , , , and . (2017)cite arxiv:1702.03491Comment: 16 pages, 8 figures, 6 tables, Accepted for publication in MNRAS.