R. Angulo, and O. Hahn. (2021)cite arxiv:2112.05165Comment: 171 pages, 30 figures, 1018 references. Review article (in press) for 'Living Reviews in Computational Astrophysics'. The article will be updated regularly, thus, comments and suggestions will be very welcome.
O. Philcox, and M. Ivanov. (2021)cite arxiv:2112.04515Comment: 20+8 pages, 12 figures. Data available at https://github.com/oliverphilcox/BOSS-Without-Windows.
K. Luken, R. Padhy, and X. Wang. (2021)cite arxiv:2111.13806Comment: 9 Pages, accepted at the Machine Learning for Physical Sciences workshop at NeurIPS 2021.
J. Muñoz, Y. Qin, A. Mesinger, S. Murray, B. Greig, and C. Mason. (2021)cite arxiv:2110.13919Comment: 23+3 pages, 23+3 figures. Comments welcome. Simulation output available at https://www.dropbox.com/sh/dqh9r6wb0s68jfo/AACc9ZCqsN0SQ_JJN7GRVuqDa?dl=0.
J. Weaver, O. Kauffmann, O. Ilbert, H. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. Hsieh and 47 other author(s). (2021)cite arxiv:2110.13923Comment: 39 pages, 21 figures, accepted for publication in The Astrophysical Journal Supplement Series. Production of IRAC mosaics are presented in Moneti et al. "Euclid Preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields" which has been posted simultaneously. Catalogs can be accessed online now at https://cosmos2020.calet.org.
J. Matthee, R. Naidu, G. Pezzulli, M. Gronke, D. Sobral, P. Oesch, M. Hayes, D. Erb, D. Schaerer, R. Amorín and 5 other author(s). (2021)cite arxiv:2110.11967Comment: Submitted to MNRAS. Figure 2 shows the main result -- the comoving emissivity due to bright LAEs. Our fiducial model is based on results presented in our companion paper -- Naidu & Matthee et al. 2021. Comments welcome.
R. Naidu, J. Matthee, P. Oesch, C. Conroy, D. Sobral, G. Pezzulli, M. Hayes, D. Erb, R. Amorín, M. Gronke and 7 other author(s). (2021)cite arxiv:2110.11961Comment: Submitted to MNRAS. Figure 4 and Table 2 show key results from the stacks. Figure 8 presents a unifying scheme for the LyC duty cycle. Our companion paper (Matthee & Naidu et al. 2021) works out implications of these results for the cosmic UV background at $z\approx2-8$. Comments warmly welcomed and greatly appreciated!.
K. Ren, and M. Trenti. (2021)cite arxiv:2110.03853Comment: 13 pages, 4 figures; accepted for publication in ApJ; data products available at https://github.com/renkeven/QuasarEvolutionData.