Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Christoph T. Lee"'
Autor:
David C. Koo, Omri Ginzburg, Anton M. Koekemoer, Nir Mandelker, Yicheng Guo, Gregory F. Snyder, Joel R. Primack, Christoph T. Lee, Maxwell Metter, Marc Huertas-Company, Haowen Zhang, Mauro Giavalisco, Daniel Ceverino, Avishai Dekel, Sandra M. Faber
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 499 (1), pp.814-835. ⟨10.1093/mnras/staa2777⟩
Mon.Not.Roy.Astron.Soc., 2020, 499 (1), pp.814-835. ⟨10.1093/mnras/staa2777⟩
A significant fraction of high redshift star-forming disc galaxies are known to host giant clumps, whose nature and role in galaxy evolution are yet to be understood. In this work we first present a new method based on neural networks to detect clump
Autor:
Samir Salim, Tomas Dahlen, Susan A. Kassin, Lin Lin, Aaron A. Dutton, Norman A. Grogin, David C. Koo, Avishai Dekel, Jerome J. Fang, Joel R. Primack, A. van der Wel, S. M. Faber, Yifei Luo, Yicheng Guo, Hooshang Nayyeri, Mauro Stefanon, Viraj Pandya, Anton M. Koekemoer, Bahram Mobasher, Rachel S. Somerville, Lei Hao, Aldo Rodríguez-Puebla, Zhu Chen, Fangzhou Jiang, Henry C. Ferguson, P. Santini, Guillermo Barro, Christoph T. Lee, Audrey Galametz
Publikováno v:
The Astrophysical Journal, 899(2), 93
Astrophysical Journal, 899(2). IOP PUBLISHING LTD
Astrophysical Journal, 899(2). IOP PUBLISHING LTD
This paper is one in a series that explores the importance of radius as a second parameter in galaxy evolution. The topic investigated here is the relationship between star formation rate (SFR) and galaxy radius (R-e) for main-sequence star-forming g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d34e86bcf8c0423e2c31926e2ac9dffd
https://ui.adsabs.harvard.edu/abs/2020ApJ...899...93L
https://ui.adsabs.harvard.edu/abs/2020ApJ...899...93L
Autor:
Christoph T. Lee, Peter Behroozi, Joel R. Primack, Doug Hellinger, Aldo Rodríguez-Puebla, Avishai Dekel
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 481:4038-4057
We study the properties of distinct dark matter halos (i.e., those that are not subhalos) that have a final virial mass $M_{\mathrm{vir}}$ at $z = 0$ less than their peak mass ($M_{\mathrm{peak}}$) in the Bolshoi-Planck cosmological simulation. We id
Autor:
Aldo Rodríguez-Puebla, Joel R. Primack, Doug Hellinger, Peter Behroozi, Avishai Dekel, Christoph T. Lee
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 466:3834-3858
We study how properties of discrete dark matter halos depend on halo environment, characterized by the mass density around the halos on scales from 0.5 to 16 $h^{-1}{\rm Mpc}$. We find that low mass halos (those less massive than the characteristic m
Autor:
Christoph T. Lee, Aldo Rodríguez-Puebla, Joel R. Primack, Doug Hellinger, Peter Behroozi, Anatoly Klypin
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 462:893-916
We report and provide fitting functions for the abundance of dark matter halos and subhalos as a function of mass, circular velocity, and redshift from the new Bolshoi-Planck and MultiDark-Planck $\Lambda$CDM cosmological simulations, based on the Pl
Autor:
Christoph T. Lee, Tze Goh, Aldo Rodríguez-Puebla, Joel R. Primack, Kathryn V. Johnston, Doug Hellinger, Elliot Eckholm, Peter Behroozi, Miguel A. Aragon-Calvo
We study the effects of the local environmental density and the cosmic web environment (filaments, walls, and voids) on key properties of dark matter halos using the Bolshoi-Planck LCDM cosmological simulation. The z = 0 simulation is analysed into f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9802e78be3be4074e2b07fa016e440d1
Autor:
Paola Dimauro, D. Tuccillo, David C. Koo, B. Häußler, Mariangela Bernardi, A. Cattaneo, Dale D. Kocevski, Helena Domínguez-Sánchez, Guillermo Barro, Fernando Buitrago, Marc Huertas-Company, Sandra M. Faber, Emanuele Daddi, Fernando Caro, Aldo Rodríguez-Puebla, Mara Salvato, Francesco Shankar, Joel R. Primack, Anton M. Koekemoer, Christoph T. Lee, Simona Mei, Berta Margalef-Bentabol, Pablo G. Pérez-González
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 478 (4), pp.5410-5426. ⟨10.1093/mnras/sty1379⟩
Monthly Notices of the Royal Astronomical Society, 2018, 478 (4), pp.5410-5426. ⟨10.1093/mnras/sty1379⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 478 (4), pp.5410-5426. ⟨10.1093/mnras/sty1379⟩
Monthly Notices of the Royal Astronomical Society, 2018, 478 (4), pp.5410-5426. ⟨10.1093/mnras/sty1379⟩
Understanding how bulges grow in galaxies is critical step towards unveiling the link between galaxy morphology and star-formation. To do so, it is necessary to decompose large sample of galaxies at different epochs into their main components (bulges
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8c6f01fd7927d79595ff901e5deb714
SubHalo Abundance Matching (SHAM) assumes that one (sub)halo property, such as mass Mvir or peak circular velocity Vpeak, determines properties of the galaxy hosted in each (sub)halo such as its luminosity or stellar mass. This assumption implies tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::875a1c22ae10b04b99f81e3ab62e111c
http://arxiv.org/abs/1710.09392
http://arxiv.org/abs/1710.09392