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pro vyhledávání: '"P. Werle"'
Akademický článek
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Autor:
Giunchi, Eric, Scarlata, Claudia, Werle, Ariel, Poggianti, Bianca M., Moretti, Alessia, Gullieuszik, Marco, Vulcani, Bendetta, Ignesti, Alessandro, Marasco, Antonino, Zanella, Anita, Wolter, Anna
The mass function (MF) of young ($\mathrm{age\lesssim 200}$ Myr) stellar clumps is an indicator of the mechanism driving the collapse of the interstellar medium (ISM) into giant molecular clouds. Typically, the clump MF in main-sequence galaxies is d
Externí odkaz:
http://arxiv.org/abs/2502.15554
Autor:
Watson, Peter J., Vulcani, Benedetta, Werle, Ariel, Poggianti, Bianca, Gullieuszik, Marco, Trenti, Michele, Wang, Xin, Roy, Namrata
We present a study of a previously identified candidate ``jellyfish'' galaxy in the Abell 2744 cluster, F0083, which showed faint signs of a tidal interaction in archival imaging. We used publicly available, PSF-matched deep photometric data from the
Externí odkaz:
http://arxiv.org/abs/2409.15215
Autor:
Tomicic, Neven, Werle, Ariel, Vulcani, Benedetta, Ignesti, Alessandro, Moretti, Alessia, Wolter, Anna, George, Koshy, Poggianti, Bianca Maria, Gullieuszik, Marco
Star-formation rates (SFR) in galaxies offer a view of various physical processes across them and are measured using various tracers, such as H$\alpha$ and UV. Different physical mechanisms can affect H$\alpha$ and UV emission, resulting in a discrep
Externí odkaz:
http://arxiv.org/abs/2409.01351
Autor:
Herpich, Fabio R., Almeida-Fernandes, Felipe, Schwarz, Gustavo B. Oliveira, Lima, Erik V. R., Nakazono, Lilianne, Alonso-García, Javier, Fonseca-Faria, Marcos A., Sartori, Marilia J., Bolutavicius, Guilherme F., de Souza, Gabriel Fabiano, Hartmann, Eduardo A., Li, Liana, Espinosa, Luna, Kanaan, Antonio, Schoenell, William, Werle, Ariel, Machado-Pereira, Eduardo, Gutiérrez-Soto, Luis A., Santos-Silva, Thaís, Castelli, Analia V. Smith, Lacerda, Eduardo A. D., Barbosa, Cassio L., Perottoni, Hélio D., Lopes, Carlos E. Ferreira, Valença, Raquel Ruiz, Martho, Pierre Augusto Re, Bom, Clecio R., Bonatto, Charles J., Carvalho, Maiara S., Cernic, Vitor, Fernandes, Roberto Cid, Coelho, Paula, Cortesi, Ariana, Palma, Barbara Cubillos, Doubrawa, Lia, Alberice, Vincenzo Sivero Ferreira, Huaynasi, Fredi Quispe, Perin, Gabriel Jacob, Arancibia, Marcelo Jaque, Krabbe, Angela, Lima-Dias, Ciria, Lomelí-Núñez, Luis, de Oliveira, Raimundo Lopes, Lopes, Amanda R., Figueiredo, André Luiz, Lösch, Elismar, Navarete, Felipe, de Oliveira, Julia Mello, Overzier, Roderik, Placco, Vinicius M., Roig, Fernando V., Rubet, Mariana, Santos, André, Sasse, Victor Hugo, Thaina-Batista, Julia, Torres-Flores, Sergio, Beers, Timothy C., Alvarez-Candal, Alvaro, Akras, Stavros, Panda, Swayamtrupta, Limberg, Guilherme, Castellón, José Luis Nilo, Telles, Eduardo, Lopes, Paulo Afranio, Montaguth, Gissel Dayana Pardo, Silva, Leandro Beraldo e, Humire, Pedro K., Fernandes, Marcelo Borges, Cordeiro, Vinícius, Ribeiro, Tiago, de Oliveira, Claudia Mendes
The Southern Photometric Local Universe Survey (S-PLUS) is a project to map $\sim9300$ sq deg of the sky using twelve bands (seven narrow and five broadbands). Observations are performed with the T80-South telescope, a robotic telescope located at th
Externí odkaz:
http://arxiv.org/abs/2407.20701
Autor:
Perottoni, Hélio D., Placco, Vinicius M., Almeida-Fernandes, Felipe, Herpich, Fábio R., Rossi, Silvia, Beers, Timothy C., Smiljanic, Rodolfo, Amarante, João A. S., Limberg, Guilherme, Werle, Ariel, Rocha-Pinto, Helio J., Silva, Leandro Beraldo e, Daflon, Simone, Alvarez-Candal, Alvaro, Schwarz, Gustavo B Oliveira, Schoenell, William, Ribeiro, Tiago, Kanaan, Antonio
Publikováno v:
A&A 691, A138 (2024)
This paper presents the first public data release of the S-PLUS Ultra-Short Survey (USS), a photometric survey with short exposure times, covering approximately 9300 deg$^{2}$ of the Southern sky. The USS utilizes the Javalambre 12-band magnitude sys
Externí odkaz:
http://arxiv.org/abs/2407.05004
Autor:
Lofaro, Cristina Maria, Rodighiero, Giulia, Enia, Andrea, Werle, Ariel, Bisigello, Laura, Cassata, Paolo, Casasola, Viviana, Renzini, Alvio, Scaloni, Letizia, Bianchetti, Alessandro
The main sequence (MS) of star-forming galaxies (SFGs) is the tight relation between the galaxy stellar mass and its star formation rate (SFR) and was observed up to z ~ 6. The MS relation can be used as a reference for understanding the differences
Externí odkaz:
http://arxiv.org/abs/2403.18156
Autor:
Khoram, Amir H., Poggianti, Bianca, Moretti, Alessia, Vulcani, Benedetta, Radovich, Mario, Werle, Ariel, Gullieuszik, Marco, Richard, Johan
Publikováno v:
A&A 686, A261 (2024)
Extraplanar tails of ionized stripped gas, extending up to several tens of kiloparsecs beyond the stellar disk, are often observed in ram-pressure stripped (RPS) galaxies in low redshift clusters. Recent studies have identified similar tails also at
Externí odkaz:
http://arxiv.org/abs/2402.13315
Autor:
Werle, A., Giunchi, E., Poggianti, B., Gullieuszik, M., Moretti, A., Zanella, A., Tonnesen, S., Fritz, J., Vulcani, B., Bacchini, C., Akerman, N., Kulier, A., Tomicic, N., Smith, R., Wolter, A.
Using images collected with the WFC3 camera on board of the Hubble Space Telescope, we detect stellar clumps in continuum-subtracted $H\alpha$ and ultraviolet (F275W filter), such clumps are often embedded in larger regions (star-forming complexes) d
Externí odkaz:
http://arxiv.org/abs/2312.06879