DESCRIPCIÓN DE LA DINÁMICA DE CARBONO EN SUELOS FORESTALES MEDIANTE UN MODELO DE RESERVORIOS

Autor: Gustavo Orellana-Rivadeneyra, María L Sandoval-Solís, Gladys Linares-Fleites, Norma E García-Calderón, José V Tamariz-Flores

Publikováno v: Avances en Ciencias e Ingeniería, Vol 3, Iss 1, Pp 123-135 (2012)

Se propone una aproximación sobre variables medioambientales mediante funciones de distribución dependientes del tiempo para simplificar un modelo de la dinámica del carbono orgánico en el suelo. El modelo se basa en el concepto de reservorios, q

Externí odkaz: https://doaj.org/article/109da279b9e64049b4f4339a00010a43

Properties of Host Galaxies of Submillimeter Sources as Revealed by JWST Early Release Observations in SMACS J0723.3–7327

Autor: Cheng Cheng, Haojing Yan, Jia-Sheng Huang, Christopher N. A. Willmer, Zhiyuan Ma, Gustavo Orellana-González

Publikováno v: The Astrophysical Journal Letters. 936:L19

Using the 0.9--4.4~$\mu$m imaging data from the James Webb Space Telescope (JWST) Early Release Observation in the SMACS J0723.3-7327 galaxy cluster field, we discuss the properties of three submillimeter galaxies (SMGs) detected by the Atacama Large

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d5eadad4b4cf80c1eef182ba184aecf
https://doi.org/10.3847/2041-8213/ac8d08

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UV and NIR size of the low-mass field galaxies: the UV compact galaxies

Autor: Jiasheng Huang, Cheng Cheng, Sophia Dai, Lizhi Xie, Wei Du, Shumei Wu, Xu Shao, C. K. Xu, Roger Leiton, Gustavo Orellana-González, Nicole Araneda, Zhizheng Pan, P. Assmann

Publikováno v: Astronomy & Astrophysics. 633:A105

Most of the massive star-forming galaxies are found to have `inside-out' stellar mass growth modes, which means the inner parts of the galaxies mainly consist of the older stellar population, while the star forming in the outskirt of the galaxy is st

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5169ccc37a1a961245928490956bef1f
https://doi.org/10.1051/0004-6361/201936186

Infrared color selection of massive galaxies at z > 3

Autor: S. M. Faber, Anton M. Koekemoer, Maurilio Pannella, David Elbaz, Laure Ciesla, Stéphanie Juneau, Nathan Bourne, E. Daddi, K. Boutsia, David C. Koo, M. L. N. Ashby, Fernando Buitrago, Nimish P. Hathi, James Dunlop, Gustavo Orellana, Pablo G. Pérez-González, J.-S. Huang, Steve Finkelstein, Ray A. Lucas, Guillermo Barro, Paola Santini, Corentin Schreiber, Yu Lu, Adriano Fontana, Xinwen Shu, Henry C. Ferguson, Marco Castellano, Steven P. Willner, Avishai Dekel, Michał J. Michałowski, Mauro Giavalisco, Tao Wang

Publikováno v: E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname

We introduce a new color-selection technique to identify high-redshift, massive galaxies that are systematically missed by Lyman-break selection. The new selection is based on the H_{160} and IRAC 4.5um bands, specifically H - [4.5] > 2.25 mag. These

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0060e5a0e43ebbb494c9d1c16c67166
https://eprints.ucm.es/id/eprint/35791/1/perezgonzalez158libre.pdf