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How well can we really estimate the stellar masses of galaxies from broadband photometry?

P. Mitchell, C. Lacey, C. Baugh, и S. Cole. (2013)cite arxiv:1303.7228Comment: 28 pages, 14 Figures, submitted to MNRAS.

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Katharina C M Heiler

Fumiko M C Fujikawa

Johannes M C Tekathen

Gwendolyn M C Müller

Tanja C M Liebl

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The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmologyJ. Gonzalez, C. Lacey, C. Baugh, C. Frenk, и A. Benson. (2011)cite arxiv:1105.3731 Comment: 17 pages, 11 figures. Submitted to MNRAS.How well can we really estimate the stellar masses of galaxies from broadband photometry?P. Mitchell, C. Lacey, C. Baugh, и S. Cole. (2013)cite arxiv:1303.7228Comment: 28 pages, 14 Figures, submitted to MNRAS.The most luminous quasars do not live in the most massive dark matter haloes at any redshiftN. Fanidakis, A. Maccio, C. Baugh, C. Lacey, и C. Frenk. (2013)cite arxiv:1305.2199Comment: 11 pages, 6 figures, submitted to MNRAS (comments are welcome).The HI mass function as a probe of photoionisation feedback on low mass galaxy formationH. Kim, J. Wyithe, C. Power, J. Park, C. Lagos, и C. Baugh. (2015)cite arxiv:1506.02736Comment: 12 pages, 9 figures, Submitted to MNRAS.What is the best way to measure baryonic acoustic oscillations?A. Sánchez, C. Baugh, и R. Angulo. \mnras, (ноября 2008)The clustering and halo occupation distribution of Lyman-break galaxies at z ~ 4J. Park, H. Kim, J. Wyithe, C. Lacey, C. Baugh, R. Barone-Nugent, M. Trenti, и R. Bouwens. (2015)cite arxiv:1511.01983Comment: 15 pages, 12 figures, submitted to MNRAS.Are Ly\alpha emitters segregated in protoclusters regions?T. Hough, S. Gurung-López, A. Orsi, S. Cora, C. Lacey, и C. Baugh. (2020)cite arxiv:2009.13542Comment: 12 pages, 8 figures, accepted for publication in MNRAS.

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