Zobrazeno 1 - 10
of 191
pro vyhledávání: '"P. Vidal-Garcia"'
Autor:
Silcock, M. S., Curtis-Lake, E., Smith, D. J. B., Wallace, I. E. B., Vidal-García, A., Plat, A., Hirschmann, M., Feltre, A., Chevallard, J., Charlot, S., Carniani, S., Bunker, A. J.
The presence of Active Galactic Nuclei (AGN) in low mass (Mstar $\lesssim$ $10^{9}$ Msun) galaxies at high redshift has been established, and it is important to characterise these objects and the impact of their feedback on the host galaxies. In this
Externí odkaz:
http://arxiv.org/abs/2410.18193
A variable active galactic nucleus at $z=2.06$ triply-imaged by the galaxy cluster MACS J0035.4-2015
Autor:
Furtak, Lukas J., Mainali, Ramesh, Zitrin, Adi, Plat, Adèle, Fujimoto, Seiji, Donahue, Megan, Nelson, Erica J., Bauer, Franz E., Uematsu, Ryosuke, Caminha, Gabriel B., Andrade-Santos, Felipe, Bradley, Larry D., Caputi, Karina I., Charlot, Stéphane, Chevallard, Jacopo, Coe, Dan, Curtis-Lake, Emma, Espada, Daniel, Frye, Brenda L., Knudsen, Kirsten K., Koekemoer, Anton M., Kohno, Kotaro, Kokorev, Vasily, Laporte, Nicolas, Lee, Minju M., Lemaux, Brian C., Magdis, Georgios E., Sharon, Keren, Stark, Daniel P., Su, Yuanyuan, Suess, Katherine A., Ueda, Yoshihiro, Umehata, Hideki, Vidal-García, Alba, Wu, John F.
We report the discovery of a triply imaged active galactic nucleus (AGN), lensed by the galaxy cluster MACS J0035.4-2015 ($z_{\mathrm{d}}=0.352$). The object is detected in Hubble Space Telescope imaging taken for the RELICS program. It appears to ha
Externí odkaz:
http://arxiv.org/abs/2303.00025
Autor:
Feltre, A., Gruppioni, C., Marchetti, L., Mahoro, A., Salvestrini, F., Mignoli, M., Bisigello, L., Calura, F., Charlot, S., Chevallard, J., Romero-Colmenero, E., Curtis-Lake, E., Delvecchio, I., Dors, O. L., Hirschmann, M., Jarrett, T., Marchesi, S., Moloko, M. E., Plat, A., Pozzi, F., Sefako, R., Traina, A., Vaccari, M., Väisänen, P., Vallini, L., Vidal-García, A., Vignali, C.
Line ratio diagnostics provide valuable clues on the source of ionizing radiation in galaxies with intense black hole accretion and starbursting events, such as local Seyfert or galaxies at the peak of the star formation history. We aim to provide a
Externí odkaz:
http://arxiv.org/abs/2301.02252
Autor:
Furtak, Lukas J., Zitrin, Adi, Plat, Adèle, Fujimoto, Seiji, Wang, Bingjie, Nelson, Erica J., Labbé, Ivo, Bezanson, Rachel, Brammer, Gabriel B., van Dokkum, Pieter, Endsley, Ryan, Glazebrook, Karl, Greene, Jenny E., Leja, Joel, Price, Sedona H., Smit, Renske, Stark, Daniel P., Weaver, John R., Whitaker, Katherine E., Atek, Hakim, Chevallard, Jacopo, Curtis-Lake, Emma, Dayal, Pratika, Feltre, Anna, Franx, Marijn, Fudamoto, Yoshinobu, Marchesini, Danilo, Mowla, Lamiya A., Pan, Richard, Suess, Katherine A., Vidal-García, Alba, Williams, Christina C.
Recent JWST/NIRCam imaging taken for the ultra-deep UNCOVER program reveals a very red dropout object at $z_{\mathrm{phot}}\simeq7.6$, triply imaged by the galaxy cluster Abell 2744 ($z_{\mathrm{d}}=0.308$). All three images are very compact, i.e. un
Externí odkaz:
http://arxiv.org/abs/2212.10531
Autor:
Hirschmann, Michaela, Charlot, Stephane, Feltre, Anna, Curtis-Lake, Emma, Somerville, Rachel S., Chevallard, Jacopo, Choi, Ena, Nelson, Dylan, Morisset, Christophe, Plat, Adele, Vidal-Garcia, Alba
We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of galaxy populations at redshifts from z$\approx$0 to z=8 in a full cosmological framework. We achieve this by coupling, in post-processing, the cosmological Illu
Externí odkaz:
http://arxiv.org/abs/2212.02522
Autor:
Pacifici, Camilla, Iyer, Kartheik G., Mobasher, Bahram, da Cunha, Elisabete, Acquaviva, Viviana, Burgarella, Denis, Rivera, Gabriela Calistro, Carnall, Adam C., Chang, Yu-Yen, Chartab, Nima, Cooke, Kevin C., Fairhurst, Ciaran, Kartaltepe, Jeyhan, Leja, Joel, Malek, Katarzyna, Salmon, Brett, Torelli, Marianna, Vidal-Garcia, Alba, Boquien, Mederic, Brammer, Gabriel G., Brown, Michael J. I., Capak, Peter L., Chevallard, Jacopo, Circosta, Chiara, Croton, Darren, Davidzon, Iary, Dickinson, Mark, Duncan, Kenneth J., Faber, Sandra M., Ferguson, Harry C., Fontana, Adriano, Guo, Yicheng, Haeussler, Boris, Hemmati, Shoubaneh, Jafariyazani, Marziye, Kassin, Susan A., Larson, Rebecca L., Lee, Bomee, Mantha, Kameswara Bharadwaj, Marchi, Francesca, Nayyeri, Hooshang, Newman, Jeffrey A., Pandya, Viraj, Pforr, Janine, Reddy, Naveen, Sanders, Ryan, Shah, Ekta, Shahidi, Abtin, Stevans, Matthew L., Triani, Dian Puspita, Tyler, Krystal D., Vanderhoof, Brittany N., de la Vega, Alexander, Wang, Weichen, Weston, Madalyn E.
The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy distribution (SED) models which allow us to infer physical parameters
Externí odkaz:
http://arxiv.org/abs/2212.01915
Autor:
Vidal-García, A., Plat, A., Curtis-Lake, E., Feltre, A., Hirschmann, M., Chevallard, J., Charlot, S.
We present the addition of nebular emission from the narrow-line regions (NLR) surrounding active galactic nuclei (AGN) to BEAGLE (BayEsian Analysis of GaLaxy sEds). Using a set of idealised spectra, we fit to a set of observables (emission-line rati
Externí odkaz:
http://arxiv.org/abs/2211.13648
Autor:
Shivaei, Irene, Boogaard, Leindert, Díaz-Santos, Tanio, Battisti, Andrew, Brinchmann, Jarle, da Cunha, Elisabete, Maseda, Michael, Matthee, Jorryt, Monreal-Ibero, Ana, Nanayakkara, Themiya, Popping, Gergö, Vidal-García, Alba, Weilbacher, Peter M.
The UV bump is a broad absorption feature centered at 2175{\AA} that is seen in the attenuation/extinction curve of some galaxies, but its origin is not well known. Here, we use a sample of 86 star-forming galaxies at z=1.7-2.7 with deep rest-frame U
Externí odkaz:
http://arxiv.org/abs/2203.09153
Autor:
Lehmann, Andrew, Godard, Benjamin, Forêts, Gillaume Pineau des, Vidal-García, Alba, Falgarone, Edith
Publikováno v:
A&A 658, A165 (2022)
Shocks, modelled over a broad range of parameters, are used to construct a new tool to deduce the mechanical energy and physical conditions from observed atomic or molecular emission lines. We compute magnetised, molecular shock models with velocitie
Externí odkaz:
http://arxiv.org/abs/2111.14089
Autor:
Orozco-Duarte, Rogelio, Wofford, Aida, Vidal-García, Alba, Bruzual, Gustavo, Charlot, Stephane, Krumholz, Mark R., Hannon, Stephen, Lee, Janice, Wofford, Timothy, Fumagalli, Michele, Dale, Daniel, Messa, Matteo, Grebel, Eva K., Smith, Linda, Grasha, Kathryn, Cook, David
We present a pilot library of synthetic NUV, U, B, V, and I photometry of star clusters with stochastically sampled IMFs and ionized gas for initial masses, $M_i=10^3$, $10^4$, and $10^5$ M$_{\odot}$; $t=1$, 3, 4, and 8 Myr; $Z=0.014$ and $Z=0.002$;
Externí odkaz:
http://arxiv.org/abs/2110.05595