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Galaxy evolution in groups and clusters: star formation rates, red sequence fractions, and the persistent bimodality

, , и . (2011)cite arxiv:1107.5311Comment: 13 pages, 5 figures. Submitted to MNRAS.

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Charlie Przetak

Charlie Hargood

Charlie Mahn

Charlie Mansfield

Charlie al- Farr

 

Другие публикации лиц с тем же именем

Forty-Seven Milky Way-Sized, Extremely Diffuse Galaxies in the Coma Cluster, , , , , и . (2014)cite arxiv:1410.8141Comment: Submitted to ApJ Letters. To illustrate how big and fluffy these things are we made a graphic comparing the one with ACS imaging (Fig 4) to several well-known galaxies, if they were at the same distance: http://www.astro.yale.edu/dokkum/coma_udgs/sizes.jpg.The SINFONI Nearby Elliptical Lens Locator Survey: Discovery of two new low-redshift strong lenses and implications for the initial mass function in giant early-type galaxies, , и . (2015)cite arxiv:1503.02661Comment: Accepted for publication in MNRAS.Signatures of unresolved binaries in stellar spectra: implications for spectral fitting, , , , , , , и . (2017)cite arxiv:1709.03983Comment: Submitted to MNRAS. 7 pages, 5 figures.Pixel Color Magnitude Diagrams for Semi-Resolved Stellar Populations: The Star Formation History of Regions within the Disk and Bulge of M31, и . (2016)cite arxiv:1602.05580Comment: 11 pages, 9 figures, submitted to ApJ.Future Prospects: Deep Imaging of Galaxy Outskirts using Telescopes Large and Small, , , , , , , и . (2016)cite arxiv:1612.06415Comment: 27 pages, 10 figures, Invited review, Book chapter in Öutskirts of Galaxies", Eds. J. H. Knapen, J. C. Lee and A. Gil de Paz, Astrophysics and Space Science Library, Springer, in press.A High Stellar Velocity Dispersion and ~100 Globular Clusters for the Ultra Diffuse Galaxy Dragonfly 44, , , , , , , , и . (2016)cite arxiv:1606.06291Comment: Submitted to ApJ Letters.Nebular Continuum and Line Emission in Stellar Population Synthesis Models, , , и . (2016)cite arxiv:1611.08305Comment: 35 pages, 29 figures.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , и 15 other автор(ы). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST, , , , , , , , , и 14 other автор(ы). (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.Modeling the Panchromatic Spectral Energy Distributions of Galaxies. (2013)cite arxiv:1301.7095Comment: 66 pages, 14 figures, to appear in Annual Review of Astronomy and Astrophysics (ARAA), vol 51.