Stress testing ΛCDM with high-redshift galaxy candidates
暂无分享,去创建一个
[1] L. Y. Aaron Yung,et al. Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations , 2022, The Astrophysical Journal Letters.
[2] T. Treu,et al. The brightest galaxies at cosmic dawn , 2022, Monthly Notices of the Royal Astronomical Society.
[3] G. Brammer,et al. A population of red candidate massive galaxies ~600 Myr after the Big Bang , 2022, Nature.
[4] D. Nardiello,et al. Photometry and astrometry with JWST -- I. NIRCam Point Spread Functions and the first JWST colour-magnitude diagrams of a globular cluster , 2022, 2209.06547.
[5] L. Y. Aaron Yung,et al. A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging , 2022, The Astrophysical Journal Letters.
[6] J. Kneib,et al. Revealing Galaxy Candidates out to $z \sim 16$ with JWST Observations of the Lensing Cluster SMACS0723 , 2022, 2207.12338.
[7] J. Dunlop,et al. The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging , 2022, Monthly Notices of the Royal Astronomical Society.
[8] A. Zitrin,et al. First Batch of Candidate Galaxies at Redshifts 11 to 20 Revealed by the James Webb Space Telescope Early Release Observations , 2022, 2207.11558.
[9] C. Conselice,et al. Discovery and properties of ultra-high redshift galaxies (9 < z < 12) in the JWST ERO SMACS 0723 Field , 2022, Monthly Notices of the Royal Astronomical Society.
[10] A. Fontana,et al. Early Results from GLASS-JWST. III. Galaxy Candidates at z ∼9–15 , 2022, The Astrophysical Journal Letters.
[11] R. Bouwens,et al. Two Remarkably Luminous Galaxy Candidates at z ≈ 10–12 Revealed by JWST , 2022, The Astrophysical Journal Letters.
[12] L. Gao,et al. The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5 , 2022, Monthly Notices of the Royal Astronomical Society.
[13] S. Ando,et al. Virial Halo Mass Function in the Planck Cosmology , 2021, The Astrophysical Journal.
[14] M. Boylan-Kolchin,et al. Uncertain times: the redshift–time relation from cosmology and stars , 2021, Monthly Notices of the Royal Astronomical Society.
[15] Tristan L. Smith,et al. Clustering and halo abundances in early dark energy cosmological models , 2020, Monthly Notices of the Royal Astronomical Society.
[16] Jaime Fern'andez del R'io,et al. Array programming with NumPy , 2020, Nature.
[17] Joel Nothman,et al. SciPy 1.0-Fundamental Algorithms for Scientific Computing in Python , 2019, ArXiv.
[18] R. B. Barreiro,et al. Planck 2018 results , 2018, Astronomy & Astrophysics.
[19] Benjamin D. Johnson,et al. A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z ≳ 4 , 2018, The Astrophysical Journal.
[20] J. Silk,et al. The most massive galaxies and black holes allowed by ΛCDM , 2016, 1609.04402.
[21] L. Moscardini,et al. The universality of the virial halo mass function and models for non-universality of other halo definitions , 2015, 1507.05627.
[22] S. Murray. HMF: Halo Mass Function calculator , 2014 .
[23] Chris Power,et al. HMFcalc: An online tool for calculating dark matter halo mass functions , 2013, Astron. Comput..
[24] M. Stiavelli,et al. Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High-z Surveys , 2007, 0712.0398.
[25] G. Lake,et al. Evolution of the mass function of dark matter haloes , 2003, astro-ph/0301270.
[26] Ravi K. Sheth Giuseppe Tormen. Large scale bias and the peak background split , 1999, astro-ph/9901122.
[27] William H. Press,et al. Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation , 1974 .
[28] E. Salpeter. The Luminosity function and stellar evolution , 1955 .