Zobrazeno 1 - 10
of 127
pro vyhledávání: '"Magris G"'
Autor:
Delgado, R. M. González, Díaz-García, L. A., de Amorim, A., Bruzual, G., Fernandes, R. Cid, Pérez, E., Bonoli, S., Cenarro, A. J., Coelho, P. R. T., Cortesi, A., García-Benito, R., Fernández, R. López, Martínez-Solaeche, G., Rodríguez-Martín, J. E., Magris, G., Mejía-Narvaez, A., Brito-Silva, D., Abramo, L. R., Diego, J. M., Dupke, R. A., Hernán-Caballero, A., Hernández-Monteagudo, C., López-Sanjuan, C., Marín-Franch, A., Marra, V., Moles, M., Montero-Dorta, A., Queiroz, C., Sodré Jr., L., Varela, J., Ramió, H. Vázquez, Vílchez, J. M., Baqui, P. O., Benítez, N., Cristóbal-Hornillos, D., Ederoclite, A., de Oliveira, C. Mendes, Civera, T., Muniesa, D., Taylor, K., Tempel, E., collaboration, the J-PAS
Publikováno v:
A&A 649, A79 (2021)
J-PAS will soon start imaging 8000 deg2 of the northern sky with its unique set of 56 filters (R $\sim$ 60). Before, we observed 1 deg2 on the AEGIS field with an interim camera with all the J-PAS filters. With this data (miniJPAS), we aim at proving
Externí odkaz:
http://arxiv.org/abs/2102.13121
Autor:
Bonoli, S., Marín-Franch, A., Varela, J., Ramió, H. Vázquez, Abramo, L. R., Cenarro, A. J., Dupke, R. A., Vílchez, J. M., Cristóbal-Hornillos, D., Delgado, R. M. González, Hernández-Monteagudo, C., López-Sanjuan, C., Muniesa, D. J., Civera, T., Ederoclite, A., Hernán-Caballero, A., Marra, V., Baqui, P. O., Cortesi, A., Cypriano, E. S., Daflon, S., de Amorim, A. L., Díaz-García, L. A., Diego, J. M., Martínez-Solaeche, G., Pérez, E., Placco, V. M., Prada, F., Queiroz, C., Alcaniz, J., Alvarez-Candal, A., Cepa, J., Maroto, A. L., Roig, F., Siffert, B. B., Taylor, K., Benitez, N., Moles, M., Sodré Jr., L., Carneiro, S., de Oliveira, C. Mendes, Abdalla, E., Angulo, R. E., Resco, M. Aparicio, Balaguera-Antolínez, A., Ballesteros, F. J., Brito-Silva, D., Broadhurst, T., Carrasco, E. R., Castro, T., Fernandes, R. Cid, Coelho, P., de Melo, R. B., Doubrawa, L., Fernandez-Soto, A., Ferrari, F., Finoguenov, A., García-Benito, R., Iglesias-Páramo, J., Jiménez-Teja, Y., Kitaura, F. S., Laur, J., Lopes, P. A. A., Lucatelli, G., Martínez, V. J., Maturi, M., Quartin, M., Pigozzo, C., Rodrìguez-Martìn, J. E., Salzano, V., Tamm, A., Tempel, E., Umetsu, K., Valdivielso, L., von Marttens, R., Zitrin, A., Díaz-Martín, M. C., López-Alegre, G., López-Sainz, A., Yanes-Díaz, A., Rueda-Teruel, F., Rueda-Teruel, S., Ibañez, J. Abril, Bravo, J. L Antón, Ferrer, R. Bello, Bielsa, S., Casino, J. M., Castillo, J., Chueca, S., Cuesta, L., Calderaro, J. Garzarán, Iglesias-Marzoa, R., Íniguez, C., Gutierrez, J. L. Lamadrid, Lopez-Martinez, F., Lozano-Pérez, D., Sacristán, N. Maícas, Molina-Ibáñez, E. L., Moreno-Signes, A., Llano, S. Rodríguez, Navarro, M. Royo, Rua, V. Tilve, Andrade, U., Alfaro, E. J., Akras, S., Arnalte-Mur, P., Ascaso, B., Barbosa, C. E., Jiménez, J. Beltrán, Benetti, M., Bengaly, C. A. P., Bernui, A., Blanco-Pillado, J. J., Fernandes, M. Borges, Bregman, J. N., Bruzual, G., Calderone, G., Carvano, J. M., Casarini, L., Chies-Santos, A. L, de Carvalho, G. Coutinho, Dimauro, P., Puertas, S. Duarte, Figueruelo, D., González-Serrano, J. I., Guerrero, M. A., Gurung-López, S., Herranz, D., Huertas-Company, M., Irwin, J. A., Izquierdo-Villalba, D., Kanaan, A., Kehrig, C., Kirkpatrick, C. C., Lim, J., Lopes, A. R., de Oliveira, R. Lopes, Marcos-Caballero, A., Martínez-Delgado, D., Martínez-González, E., Martínez-Somonte, G., Oliveira, N., Orsi, A. A., Overzier, R. A., Penna-Lima, M., Reis, R. R. R., Spinoso, D., Tsujikawa, S., Vielva, P., Vitorelli, A. Z., Xia, J. Q., Yuan, H. B., Arroyo-Polonio, A., Dantas, M. L. L., Galarza, C. A., Gonçalves, D. R., Gonçalves, R. S., Gonzalez, J. E., Gonzalez, A. H., Greisel, N., Landim, R. G., Lazzaro, D., Magris, G., Monteiro-Oliveira, R., Pereira, C. B., Rebouças, M. J., Rodriguez-Espinosa, J. M., da Costa, S. Santos, Telles, E.
Publikováno v:
A&A 653, A31 (2021)
The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will soon start to scan thousands of square degrees of the northern extragalactic sky with a unique set of $56$ optical filters from a dedicated $2.55$m telescope, JST,
Externí odkaz:
http://arxiv.org/abs/2007.01910
Autor:
Cabrera-Ziri, I., Bastian, N., Hilker, M., Davies, B., Schweizer, F., Kruijssen, J. M. D., Mejía-Narváez, A., Niederhofer, F., Brandt, T. D., Rejkuba, M., Bruzual, G., Magris, G.
The colour-magnitude diagrams of some intermediate-age clusters (1-2 Gyr) star clusters show unexpectedly broad main-sequence turnoffs, raising the possibility that these clusters have experienced more than one episode of star formation. Such a scena
Externí odkaz:
http://arxiv.org/abs/1601.02024
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; 9/26/2024, Vol. 690, p1-11, 11p
Autor:
Verdugo, T., Motta, V., Foëx, G., Forero-Romero, J. E., Muñoz, R. P., Pello, R., Limousin, M., More, A., Cabanac, R., Soucail, G., Blakeslee, J. P., Mejía-Narváez, A. J., Magris, G., Fernández-Trincado, J. G.
Publikováno v:
A&A 571, A65 (2014)
We analyzed the Einstein radius, $\theta_E$, in our sample of SL2S galaxy groups, and compared it with $R_A$ (the distance from the arcs to the center of the lens), using three different approaches: 1.- the velocity dispersion obtained from weak lens
Externí odkaz:
http://arxiv.org/abs/1409.2900
Currently there are two competing scenarios to explain the origin of the stellar population in globular clusters (GCs). The main difference between them is whether or not multiple events of star formation took place within GCs. In this paper we prese
Externí odkaz:
http://arxiv.org/abs/1404.4056
Autor:
Bongiovanni, A., Bruzual, G., Magris, G., Gallego, J., Garcia-Dabo, C. E., Coppi, P., Sabbey, C.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 359 (2005) 930-940
We present the CIDA-UCM-Yale (Centro de Investigaciones de Astronomia, Universidad Complutense de Madrid and Yale University) survey for Halpha+[NII]6549,6584 emission-line galaxies using objective-prism spectra. The most important properties of a ca
Externí odkaz:
http://arxiv.org/abs/astro-ph/0502491
Autor:
Rengstorf, A. W., Mufson, S. L., Abad, C., Adams, B., Andrews, P., Bailyn, C., Baltay, C., Bongiovanni, A., Briceno, C., Bruzual, G., Coppi, P., Della Prugna, F., Emmet, W., Ferrin, I., Fuenmayor, F., Gebhard, M., Hernandez, J., Honeycutt, R. K., Magris, G., Musser, J., Naranjo, O., Oemler, A., Rosenzweig, P., Sabbey, C. N., Sanchez, Ge., Sanchez, Gu., Schaefer, B., Schenner, H., Sinnott, J., Snyder, J. A., Sofia, S., Stock, J., van Altena, W., Vivas, A. K.
Publikováno v:
Astrophys.J. 606 (2004) 741-748
By observing the high galactic latitude equatorial sky in drift scan mode with the QUEST (QUasar Equatorial Survey Team) Phase 1 camera, multi-bandpass photometry on a large strip of sky, resolved over a large range of time scales (from hourly to bie
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310916
Autor:
Baltay, C., Snyder, J. A., Andrews, P., Emmet, W., Schaefer, B., Sinnott, J., Bailyn, C., Coppi, P., Oemler, A., Sabbey, C. N., Sofia, S., van Altena, W., Vivas, A. K., Abad, C., Briceno, C., Bruzual, G., Magris, G., Stock, J., Della Prugna, F., Sanchez, Ge., Sanchez, Gu., Schenner, H., Adams, B., Gebhard, M., Honeycutt, R. K., Musser, J., Harris, F., Geary, J.
Publikováno v:
Publ.Astron.Soc.Pac.114:780-794,2002
We have designed, constructed and put into operation a large area CCD camera that covers a large fraction of the image plane of the 1 meter Schmidt telescope at Llano del Hato in Venezuela. The camera consists of 16 CCD devices arranged in a 4 x 4 mo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0204265
Autor:
Vivas, A. K., Zinn, R., Andrews, P., Bailyn, C., Baltay, C., Coppi, P., Ellman, N., Girard, T., Rabinowitz, D., Schaefer, B., Shin, J., Snyder, J., Sofia, S., van Altena, W., Abad, C., Bongiovanni, A., Briceno, C., Bruzual, G., Della Prugna, F., Herrera, D., Magris, G., Mateu, J., Pacheco, R., Sanchez, Ge., Sanchez, Gu., Schenner, H., Stock, J., Vicente, B., Vieira, K., Ferrin, I., Hernandez, J., Gebhard, M., Honeycutt, R., Muffson, s., Musser, J., Rengstorf, A.
Publikováno v:
Astrophys.J.554:L33-L36,2001
We have measured the periods and light curves of 148 RR Lyrae variables from V=13.5 to 19.7 from the first 100 sq. degrees of the QUEST RR Lyrae survey. Approximately 55% of these stars belong to the clump of stars detected earlier by the Sloan Digit
Externí odkaz:
http://arxiv.org/abs/astro-ph/0105135