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On the nature of the luminous Lya emitter CR7 and its UV components: physical conditions and JWST predictions

, , , , , , , , and . (2017)cite arxiv:1710.08422Comment: Submitted to MNRAS, comments welcomed. 19 pages, 11 figures.

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The Size of BDDs and Other Data Structures in Temporal Logics Model Checking., , and . IEEE Trans. Computers, 65 (10): 3148-3156 (2016)Probing cosmic star formation up to z = 9.4 with GRBs, , and . (2011)cite arxiv:1106.1745Comment: Submitted to MNRAS letters.Treewidth in Verification: Local vs. Global., , and . LPAR, volume 3835 of Lecture Notes in Computer Science, page 489-503. Springer, (2005)On the generalization of continuous-time stochastic processes simulation for industrial production modeling., , , and . SpringSim (ANSS), page 7. SCS/ACM, (2014)The formation of the extremely primitive star SDSS J102915+172927 relies on dust, , , , , , and . (2012)cite arxiv:1203.4234Comment: 5 pages, 3 figures, accepted as a Letter to MNRAS.First Identification of Direct Collapse Black Hole Candidates in the Early Universe in CANDELS/GOODS-S, , , , and . (2016)cite arxiv:1603.08522Comment: Accepted for publication in MNRAS. First published online March 28, 2016 (8 pages).The problematic growth of dust in the interstellar medium, , and . (2016)cite arxiv:1606.07214Comment: 6 pages, MNRAS Letter. Comments welcome.Feedback Limits to Maximum Seed Masses of Black Holes, , and . (2017)cite arxiv:1701.06565Comment: Accepted for publication in ApJ Letters.On the nature of the luminous Lya emitter CR7 and its UV components: physical conditions and JWST predictions, , , , , , , , and . (2017)cite arxiv:1710.08422Comment: Submitted to MNRAS, comments welcomed. 19 pages, 11 figures.Is the star formation rate in $z6$ quasars overestimated?, , , , , , and . (2022)cite arxiv:2211.05790Comment: 9 pages, 6 figures. Accepted for publication by MNRAS.