Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Delgado, R. M. Gonz��lez"'
Autor:
Vilella-Rojo, G., Logro��o-Garc��a, R., L��pez-Sanjuan, C., Viironen, K., Varela, J., Moles, M., Cenarro, A. J., Crist��bal-Hornillos, D., Ederoclite, A., Hern��ndez-Monteagudo, C., Mar��n-Franch, A., Rami��, H. V��zquez, Galbany, L., Delgado, R. M. Gonz��lez, Hern��n-Caballero, A., Lumbreras-Calle, A., S��nchez-Bl��zquez, P., Sobral, D., V��lchez, J. M., Alcaniz, J., Angulo, R. E., Dupke, R. A., Sodr��, L.
Our goal is to estimate the star formation main sequence (SFMS) and the star formation rate density (SFRD) at z 8 and it is clearly defined by the blue galaxies, with the red galaxies located below them. The SFMS is described as log SFR = 0.83 log M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::65dbcf391661bbaf6a4cce95d74294b3
Autor:
Logro��o-Garc��a, R., Vilella-Rojo, G., L��pez-Sanjuan, C., Varela, J., Viironen, K., Muniesa, D. J., Cenarro, A. J., Crist��bal-Hornillos, D., Ederoclite, A., Mar��n-Franch, A., Moles, M., Rami��, H. V��zquez, Bonoli, S., D��az-Garc��a, L. A., Orsi, A., Roman, I. San, Akras, S., Chies-Santos, A. L., Coelho, P. R. T., Daflon, S., Costa-Duarte, M. V., Dupke, R., Galbany, L., Delgado, R. M. Gonz��lez, Hernandez-Jimenez, J. A., de Oliveira, R. Lopes, de Oliveira, C. Mendes, Oteo, I., Gon��alves, D. R., S��nchez-Portal, M., Schmidtobreick, L., Sodr��, L.
In the present paper we aim to validate a methodology designed to extract the Halpha emission line flux from J-PLUS photometric data. J-PLUS is a multi narrow-band filter survey carried out with the 2 deg2 field of view T80Cam camera, mounted on the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e71646fa8017a78a2bb881f129fecc2f
Autor:
Cortijo-Ferrero, C., Delgado, R. M. Gonz��lez, P��rez, E., Fernandes, R. Cid, S��nchez, S. F., de Amorim, A. L., Di Matteo, P., Garc��a-Benito, R., Lacerda, E. A. D., Fern��ndez, R. L��pez, Tadhunter, C.
The role of major mergers in galaxy evolution is investigated through a detailed characterization of the stellar populations, ionized gas properties, and star formation rates (SFR) in the early-stage merger LIRGs IC 1623 W and NGC 6090, by analysing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::945dbc0b0e0a93040b5c1f17d9d60160
http://arxiv.org/abs/1702.06544
http://arxiv.org/abs/1702.06544
Autor:
Falc��n-Barroso, J., Lyubenova, M., van de Ven, G., M��ndez-Abreu, J., Aguerri, J. A. L., Garc��a-Lorenzo, B., Bekeraite, S., S��nchez, S. F., Husemann, B., Garc��a-Benito, R., Mast, D., Walcher, C. J., Zibetti, S., Barrera-Ballesteros, J. K., Galbany, L., S��nchez-Bl��zquez, P., Singh, R., Bosch, R. C. E. van den, Wild, V., Zhu, L., Bland-Hawthorn, J., Fernandes, R. Cid, de Lorenzo-C��ceres, A., Gallazzi, A., Delgado, R. M. Gonz��lez, Marino, R. A., M��rquez, I., P��rez, E., P��rez, I., Roth, M. M., Rosales-Ortega, F. F., Ru��z-Lara, T., Wisotzki, L., Ziegler, B., collaboration, the CALIFA
Publikováno v:
Astronomy & astrophysics, 597:A48. EDP Sciences
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
E-Prints Complutense. Archivo Institucional de la UCM
Digital.CSIC. Repositorio Institucional del CSIC
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
E-Prints Complutense. Archivo Institucional de la UCM
Digital.CSIC. Repositorio Institucional del CSIC
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
J. Falcón-Barroso et. al.
We present the stellar kinematic maps of a large sample of galaxies from the integral-field spectroscopic survey CALIFA. The sample comprises 300 galaxies displaying a wide range of morphologies across the Hubble seque
We present the stellar kinematic maps of a large sample of galaxies from the integral-field spectroscopic survey CALIFA. The sample comprises 300 galaxies displaying a wide range of morphologies across the Hubble seque
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b7709fa1698d004a0aeff41889baae8
https://research.rug.nl/en/publications/aa2bff86-9073-494f-8a02-50761581bd69
https://research.rug.nl/en/publications/aa2bff86-9073-494f-8a02-50761581bd69
Autor:
Viironen, K., L��pez-Sanjuan, C., Hern��ndez-Monteagudo, C., Chaves-Montero, J., Ascaso, B., Bonoli, S., Crist��bal-Hornillos, D., D��az-Garc��a, L. A., Fern��ndez-Soto, A., M��rquez, I., Masegosa, J., Povi��, M., Varela, J., Cenarro, A. J., Aguerri, J. A. L., Alfaro, E., Aparicio-Villegas, T., Ben��tez, N., Broadhurst, T., Cabrera-Ca��o, J., Castander, F. J., Cepa, J., Cervi��o, M., Delgado, R. M. Gonz��lez, Husillos, C., Infante, L., Mart��nez, V. J., Moles, M., Molino, A., del Olmo, A., Perea, J., Prada, F., Quintana, J. M.
Context. Knowing the exact shape of the UV luminosity function of high-redshift galaxies is important in order to understand the star formation history of the early universe. However, the uncertainties, especially at the faint and bright ends of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::66df32856caf2af08f8734618112aa9e
Autor:
Roman, I. San, Cenarro, A. J., D��az-Garc��a, L. A., L��pez-Sanjuan, C., Varela, J., Delgado, R. M. Gonz��lez, S��nchez-Bl��zquez, P., Alfaro, E. J., Ascaso, B., Bonoli, S., Borlaff, A., Castander, F. J., Cervi��o, M., Fern��ndez-Soto, A., M��rquez, I., Masegosa, J., Muniesa, D., Povic, M., Viironen, K., Aguerri, J. A. L., Ben��tez, N., Broadhurst, T., Cabrera-Ca��o, J., Cepa, J., Crist��bal-Hornillos, D., Infante, L., Mart��nez, V. J., Moles, M., del Olmo, A., Perea, J., Prada, F., Quintana, J. M.
We present a technique that permits the analysis of stellar population gradients in a relatively low cost way compared to IFU surveys analyzing a vastly larger samples as well as out to larger radii. We developed a technique to analyze unresolved ste
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f0a51401cf02dc869563dcd01e224763
Autor:
L��pez-Sanjuan, C., Tempel, E., Ben��tez, N., Molino, A., Viironen, K., D��az-Garc��a, L. A., Fern��ndez-Soto, A., Santos, W. A., Varela, J., Cenarro, A. J., Moles, M., Arnalte-Mur, P., Ascaso, B., Montero-Dorta, A. D., Povi��, M., Mart��nez, V. J., Nieves-Seoane, L., Stefanon, M., Hurtado-Gil, Ll., M��rquez, I., Perea, J., Aguerri, J. A. L., Alfaro, E., Aparicio-Villegas, T., Broadhurst, T., Cabrera-Ca��o, J., Castander, F. J., Cepa, J., Cervi��o, M., Crist��bal-Hornillos, D., Delgado, R. M. Gonz��lez, Husillos, C., Infante, L., Masegosa, J., del Olmo, A., Prada, F., Quintana, J. M.
Our goal is to study the evolution of the $B-$band luminosity function (LF) since $z=1$ using ALHAMBRA data. We used the photometric redshift and the $I-$band selection magnitude probability distribution functions (PDFs) of those ALHAMBRA galaxies wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6444c922673fb07420a17c1331181a0
Autor:
Barrera-Ballesteros, J. K., Garc��a-Lorenzo, B., Falc��n-Barroso, J., van de Ven, G., Lyubenova, M., Wild, V., M��ndez-Abreu, J., S��nchez, S. F., Marquez, I., Masegosa, J., Monreal-Ibero, A., Ziegler, B., del Olmo, A., Verdes-Montenegro, L., Garc��a-Benito, R., Husemann, B., Mast, D., Kehrig, C., Iglesias-Paramo, J., Marino, R. A., Aguerri, J. A. L., Walcher, C. J., V��lchez, J. M., Bomans, D. J., Cortijo-Ferrero, C., Delgado, R. M. Gonz��lez, Bland-Hawthorn, J., McIntosh, D. H., Bekeraite, Simona, Collaboration, the CALIFA
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and astrophysics, 582:A21. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Universidad Complutense de Madrid
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and astrophysics, 582:A21. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
© 2015 ESO. We present spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close companions, pairs with morphological signatures of interaction, and coalesced merger
Autor:
Delgado, R. M. Gonz��lez, Garc��a-Benito, R., P��rez, E., Fernandes, R. Cid, de Amorim, A. L., Cortijo-Ferrero, C., Lacerda, E. A. D., Fern��ndez, R. L��pez, Vale-Asari, N., S��nchez, S., collaboration, CALIFA
We characterize in detail the radial structure of the stellar population properties of 300 galaxies in the nearby universe, observed with integral field spectroscopy in the CALIFA survey. The sample covers a wide range of Hubble types, from spheroida
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::efaaf0284858455684c10b1d2467aec5
http://arxiv.org/abs/1506.02809
http://arxiv.org/abs/1506.02809
Autor:
Delgado, R. M. Gonz��lez, Garc��a-Benito, R., P��rez, E., Fernandes, R. Cid, de Amorim, A. L., Cortijo-Ferrero, C., Lacerda, E. A. D., Fern��ndez, R. L��pez, S��nchez, S. F., Asari, N. Vale, collaboration, CALIFA
We analyze the spatially resolved star formation history of 300 nearby galaxies from the CALIFA integral field spectroscopic survey to investigate the radial structure and gradients of the present day stellar populations properties as a function of H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c9d89f64143d9712b620bafb503b110
http://arxiv.org/abs/1412.2493
http://arxiv.org/abs/1412.2493