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pro vyhledávání: '"Cabello González, Cristina"'
Autor:
Cabello González, Cristina, Gallego Maestro, Jesús, Cardiel López, Nicolás, Pascual Ramírez, Sergio, Guzmán, R., Herrero, A., Manrique, A., Marín Franch, A., Mas Hesse, J. M., Rodriguez Espinosa, J. M., Salvador Solé, E.
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
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Context. Identifying very high-redshift galaxies is crucial for understanding the formation and evolution of galaxies. However, many questions still remain, and the uncertainty on the epoch of reionization is large. In this approach, some models allo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::e15a956a67ceb687a3a78c7a23325863
https://eprints.ucm.es/id/eprint/74815/1/pascualramirez36libre.pdf
https://eprints.ucm.es/id/eprint/74815/1/pascualramirez36libre.pdf
Autor:
Cardiel López, Nicolás, Zamorano Calvo, Jaime, Bará, Salvador, Sánchez de Miguel, Alejandro, Cabello González, Cristina, Gallego Maestro, Jesús, García, Lucía, González, Rafael, Izquierdo Gómez, Jaime, Pascual Ramírez, Sergio, Sánchez Penim, Ainhoa, Tapia Ayuga, Carlos
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense. Archivo Institucional de la UCM
Although a catalogue of synthetic RGB magnitudes, providing photometric data for a sample of 1346 bright stars, has been recently published, its usefulness is still limited due to the small number of reference stars available, considering that they a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4262f34b085eb1e08ea499125bc60b52
https://eprints.ucm.es/id/eprint/68677/
https://eprints.ucm.es/id/eprint/68677/
Autor:
Cabello González, Cristina
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
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E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
One of the AMIGA (Analytical Model for IGM and GAlaxy evolution) predictions is that the reionization of the intergalactic neutral hydrogen occurred in two stages: a first one at z ≥ 10, due to Pop. III stars, and a second and definitive one at z
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::07be30a82e6edbe545e5441177c20245
https://eprints.ucm.es/id/eprint/45046/1/TFM_final.pdf
https://eprints.ucm.es/id/eprint/45046/1/TFM_final.pdf
Autor:
Cabello González, Cristina
One of the AMIGA (Analytical Model far IGM and GAlaxy evolution) predictions is that the reionization of the intergalactic neutral hydrogen occurred in two stages: a first one at z ≥10, due to Pop. III stars, and a second and definitive one at z
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______126::13526cc0c2a6f3590b4ab92757cc3108
http://eprints.ucm.es/45164/
http://eprints.ucm.es/45164/
Autor:
Cabello González, Cristina
Publikováno v:
idUS. Depósito de Investigación de la Universidad de Sevilla
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instname
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::baa2d448dc69903488b9909edd750a7b