Zobrazeno 1 - 10
of 929
pro vyhledávání: '"Pampliega, A"'
Autor:
Vitte, E., Verhamme, A., Hibon, P., Leclercq, F., Pampliega, B. Alcalde, Kerutt, J., Kusakabe, H., Matthee, J., Guo, Y., Bacon, R., Maseda, M., Richard, J., Pharo, J., Schaye, J., Boogaard, L., Nanayakkara, T., Contini, T.
The Hydrogen Lyman-alpha (Lya) line shows a large variety of shapes which is caused by factors at different scales, from the interstellar medium to the intergalactic medium. This work aims to provide a systematic inventory and classification of the s
Externí odkaz:
http://arxiv.org/abs/2411.14327
Autor:
Solimano, M., González-López, J., Aravena, M., Pampliega, B. Alcalde, Assef, R. J., Béthermin, M., Boquien, M., Bovino, S., Casey, C. M., Cassata, P., da Cunha, E., Davies, R. L., De Looze, I., Ding, X., Díaz-Santos, T., Faisst, A. L., Ferrara, A., Fisher, D. B., Förster-Schreiber, N. M., Fujimoto, S., Ginolfi, M., Gruppioni, C., Guaita, L., Hathi, N., Herrera-Camus, R., Ibar, E., Inami, H., Jones, G. C., Koekemoer, A. M., Lee, L., Li, J., Liu, D., Liu, Z., Molina, J., Ogle, P., Posses, A. C., Pozzi, F., Relaño, M., Riechers, D. A., Romano, M., Spilker, J., Sulzenauer, N., Telikova, K., Vallini, L., Vasan, K. G. C., Veilleux, S., Vergani, D., Villanueva, V., Wang, W., Yan, L., Zamorani, G.
Galaxy protoclusters are sites of rapid growth, with a high density of massive galaxies driving elevated rates of star formation and accretion onto supermassive black holes. Here, we present new JWST/NIRSpec IFU observations of the J1000+0234 group a
Externí odkaz:
http://arxiv.org/abs/2407.13020
Autor:
Kamieneski, Patrick S., Frye, Brenda L., Windhorst, Rogier A., Harrington, Kevin C., Yun, Min S., Noble, Allison, Pascale, Massimo, Foo, Nicholas, Cohen, Seth H., Jansen, Rolf A., Carleton, Timothy, Koekemoer, Anton M., Willmer, Christopher N. A., Summers, Jake S., Garuda, Nikhil, Leimbach, Reagen, Holwerda, Benne W., Pierel, Justin D. R., Jimenez-Andrade, Eric F., Willner, S. P., Pampliega, Belen Alcalde, Vishwas, Amit, Keel, William C., Wang, Q. Daniel, Cheng, Cheng, Coe, Dan, Conselice, Christopher J., D'Silva, Jordan C. J., Driver, Simon P., Grogin, Norman A., Hinrichs, Tyler, Lowenthal, James D., Marshall, Madeline A., Nonino, Mario, Ortiz III, Rafael, Pigarelli, Alex, Pirzkal, Nor, Polletta, Maria del Carmen, Robotham, Aaron S. G., Ryan Jr., Russell E., Yan, Haojing
We present a new parametric lens model for the G165.7+67.0 galaxy cluster, which was discovered with $Planck$ through its bright submillimeter flux, originating from a pair of extraordinary dusty star-forming galaxies (DSFGs) at $z\approx 2.2$. Using
Externí odkaz:
http://arxiv.org/abs/2404.08058
Autor:
Wang, Q. Daniel, Diaz, Carlos Garcia, Kamieneski, Patrick S., Harrington, Kevin C., Yun, Min S., Foo, Nicholas, Frye, Brenda L., Jimenez-Andrade, Eric F., Liu, Daizhong, Lowenthal, James D., Pampliega, Belen Alcalde, Pascale, Massimo, Vishwas, Amit, Gurwell, Mark A.
Hyper-luminous infrared galaxies (HyLIRGs) are the most extreme star-forming systems observed in the early Universe, and their properties still elude comprehensive understanding. We have undertaken a large XMM-Newton observing program to probe the to
Externí odkaz:
http://arxiv.org/abs/2312.05442
Autor:
Gottumukkala, R., Barrufet, L., Oesch, P. A., Weibel, A., Allen, N., Pampliega, B. Alcalde, Nelson, E. J., Williams, C. C., Brammer, G., Fudamoto, Y., González, V., Heintz, K. E., Illingworth, G., Magee, D., Naidu, R. P., Shuntov, M., Stefanon, M., Toft, S., Valentino, F., Xiao, M.
With the advent of JWST, we can probe the rest-frame optical emission of galaxies at $z>3$ with high sensitivity and spatial resolution, making it possible to accurately characterise red, optically-faint galaxies and thus move towards a more complete
Externí odkaz:
http://arxiv.org/abs/2310.03787
Autor:
Mérida, Rosa M., Pérez-González, Pablo G., Sánchez-Blázquez, Patricia, García-Argumánez, Ángela, Annunziatella, Marianna, Costantin, Luca, Lumbreras-Calle, Alejandro, Alcalde-Pampliega, Belén, Barro, Guillermo, Espino-Briones, Néstor, Koekemoer, Anton M.
We investigate the star formation main sequence (MS) (SFR-M$_{\star}$) down to 10$^{8-9}\mathrm{M}_\odot$ using a sample of 34,061 newly-discovered ultra-faint ($27\lesssim i \lesssim 30$ mag) galaxies at $1
Externí odkaz:
http://arxiv.org/abs/2303.16234
Autor:
Anna Riera-Martín, Antonio Oliver-Roig, Susana Cormenzana, Miguel Richart-Martínez, Ana Martínez-Pampliega
Publikováno v:
PeerJ, Vol 12, p e18015 (2024)
Background Becoming a mother is a very important process because of the impact it can have on women and their families. Currently, there is no validated questionnaire that evaluates the process of becoming a mother in the Spanish population. Moreover
Externí odkaz:
https://doaj.org/article/19564d233f1d42d3bec2536963164af2
Autor:
Griffiths, Alex, Conselice, Christopher J., Ferreira, Leonardo, Ceverino, Daniel, Perez-Gonzalez, Pablo G., Vega, Olga, Rosa-Gonzalez, Daniel, Koekemoer, Anton M., Marchesini, Danilo, Espinosa, Jose Miguel Rodrıguez, Rodrıguez-Munoz, Lucıa, Pampliega, Belen Alcalde, Terlevich, Elena
We present an investigation on escape fractions of UV photons from a unique sample of lensed low-mass emission line selected galaxies at z < 3.5 found in the SHARDS Hubble Frontier Fields medium-band survey. We have used this deep imaging survey to l
Externí odkaz:
http://arxiv.org/abs/2211.06162
Autor:
Shah, Ekta A., Kartaltepe, Jeyhan S., Magagnoli, Christina T., Cox, Isabella G., Wetherell, Caleb T., Vanderhoof, Brittany N., Cooke, Kevin C., Calabro, Antonello, Chartab, Nima, Conselice, Christopher J., Croton, Darren J., de la Vega, Alexander, Hathi, Nimish P., Ilbert, Olivier, Inami, Hanae, Kocevski, Dale D., Koekemoer, Anton M., Lemaux, Brian C., Lubin, Lori, Mantha, Kameswara Bharadwaj, Marchesi, Stefano, Martig, Marie, Moreno, Jorge, Pampliega, Belen Alcalde, Patton, David R., Salvato, Mara, Treister, Ezequiel
Observations and simulations of interacting galaxies and mergers in the local universe have shown that interactions can significantly enhance the star formation rates (SFR) and fueling of Active Galactic Nuclei (AGN). However, at higher redshift, som
Externí odkaz:
http://arxiv.org/abs/2209.15587
Autor:
Annunziatella, Marianna, Pérez-González, PabloG., Argumánez, Ángela García, Barro, Guillermo, Pampliega, Belén Alcalde, Costantin, Luca, Koekemoer, Anton M., Mérida, Rosa M.
We investigate how the environment affects the assembly history of massive galaxies. For that purpose, we make use of SHARDS and HST spectro-photometric data, whose depth, spectral resolution, and wavelength coverage allow to perform a detailed analy
Externí odkaz:
http://arxiv.org/abs/2209.11784