Zobrazeno 1 - 10
of 240
pro vyhledávání: '"Cresci, Giovanni"'
Autor:
Parlanti, Eleonora, Carniani, Stefano, Venturi, Giacomo, Herrera-Camus, Rodrigo, Arribas, Santiago, Bunker, Andrew J., Charlot, Stephane, D'Eugenio, Francesco, Maiolino, Roberto, Perna, Michele, Übler, Hannah, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Lamperti, Isabella, Zamora, Sandra
Galactic outflows driven by star formation or active galactic nuclei are typically formed by multi-phase gas whose temperature spans over 4 orders of magnitude. Probing the different outflow components requires multi-wavelength observations and long
Externí odkaz:
http://arxiv.org/abs/2407.19008
Autor:
Marconcini, Cosimo, D'Eugenio, Francesco, Maiolino, Roberto, Arribas, Santiago, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Perna, Michele, Del Pino, Bruno Rodriguez, Ubler, Hannah, Willott, Chris J., Boker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Lamperti, Isabella, Parlanti, Eleonora, Venturi, Giacomo
We present JWST/NIRSpec integral-field spectroscopy observations of the z ~ 9.11 lensed galaxy MACS1149-JD1, as part of the GA-NIFS programme. The data was obtained with both the G395H grating (R~ 2700) and the prism (R~ 100). This target shows a mai
Externí odkaz:
http://arxiv.org/abs/2407.08616
Autor:
Lamperti, Isabella, Arribas, Santiago, Perna, Michele, Del Pino, Bruno Rodríguez, Circosta, Chiara, Pérez-González, Pablo G., Bunker, Andrew J., Carniani, Stefano, Charlot, Stéphane, D'Eugenio, Francesco, Maiolino, Roberto, Übler, Hannah, Willott, Chris J., Bertola, Elena, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Kumari, Nimisha, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo
We present JWST NIRSpec observations in IFS mode of the galaxy GS5001 at redshift z=3.47, the brightest member of a candidate protocluster in the GOODS-S field. The data cover a field of view (FoV) of 4''$\times$4'' (~$30\times30$~kpc$^2$) and were o
Externí odkaz:
http://arxiv.org/abs/2406.10348
Autor:
Scholtz, Jan, D'Eugenio, Francesco, Maiolino, Roberto, Pérez-González, Pablo G., Circosta, Chiara, Tacchella, Sandro, Williams, Christina C., Alberts, Stacey, Arribas, Santiago, Baker, William M., Bertola, Elena, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Cresci, Giovanni, Jones, Gareth C., Kumari, Nimisha, Lamperti, Isabella, Looser, Tobias J., Del Pino, Bruno Rodríguez, Robertson, Brant, Parlanti, Eleonora, Perna, Michele, Übler, Hannah, Venturi, Giacomo, Witstok, Joris
JWST is discovering increasing numbers of quiescent galaxies 1--2 billion years after the Big Bang, whose redshift, high mass, and old stellar ages indicate that their formation and quenching were surprisingly rapid. This fast-paced evolution seems t
Externí odkaz:
http://arxiv.org/abs/2405.19401
Autor:
Jones, Gareth C., Bunker, Andrew J., Telikova, Kseniia, Arribas, Santiago, Carniani, Stefano, Charlot, Stephane, D'Eugenio, Francesco, Maiolino, Roberto, Perna, Michele, Del Pino, Bruno Rodriguez, Ubler, Hannah, Willott, Chris, Aravena, Manuel, Boker, Torsten, Cresci, Giovanni, Curti, Mirko, Herrera-Camus, Rodrigo, Lamperti, Isabella, Parlanti, Eleonora, Perez-Gonzalez, Pablo G., Villanueva, Vicente
We present observations of the $z\sim5.7$ Lyman-break galaxy HZ10 with the JWST/NIRSpec IFU in high and low spectral resolution (G395H, $R\sim2700$ and PRISM, $R\sim100$, respectively), as part of the GA-NIFS program. By spatially resolving the sourc
Externí odkaz:
http://arxiv.org/abs/2405.12955
Autor:
Pérez-González, Pablo G., D`Eugenio, Francesco, del Pino, Bruno Rodríguez, Übler, Hannah, Maiolino, Roberto, Arribas, Santiago, Cresci, Giovanni, Lamperti, Isabella, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Willott, Christopher J., Böker, Torsten, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo, Barro, Guillermo, Costantin, Luca, Martín-Navarro, Ignacio, Dunlop, James S., Magee, Daniel
Feedback is the key physical mechanism regulating galaxy formation. Stars in galaxies form when baryons radiatively cool down and fall into gravitational wells. Eventually, star formation quenches as gas is depleted and/or perturbed by feedback proce
Externí odkaz:
http://arxiv.org/abs/2405.03744
Autor:
Maiolino, Roberto, Risaliti, Guido, Signorini, Matilde, Trefoloni, Bartolomeo, Juodzbalis, Ignas, Scholtz, Jan, Uebler, Hannah, D'Eugenio, Francesco, Carniani, Stefano, Fabian, Andy, Ji, Xihan, Mazzolari, Giovanni, Bertola, Elena, Brusa, Marcella, Bunker, Andrew J., Charlot, Stephane, Comastri, Andrea, Cresci, Giovanni, DeCoursey, Christa Noel, Egami, Eiichi, Fiore, Fabrizio, Gilli, Roberto, Perna, Michele, Tacchella, Sandro, Venturi, Giacomo
We investigate the X-ray properties of a large sample of 71 broad line and narrow line AGN at 2
Externí odkaz:
http://arxiv.org/abs/2405.00504
Autor:
Fahrion, Katja, Böker, Torsten, Perna, Michele, Beck, Tracy L., Maiolino, Roberto, Arribas, Santiago, Bunker, Andrew J., Charlot, Stephane, Ceci, Matteo, Cresci, Giovanni, De Marchi, Guido, Lützgendorf, Nora, Ulivi, Lorenzo
Publikováno v:
A&A 687, A83 (2024)
We present a detailed study of the centre of NGC4654, a Milky Way-like spiral galaxy in the Virgo cluster that has been reported to host a double stellar nucleus, thus promising a rare view of ongoing star cluster infall into a galaxy nucleus. Analys
Externí odkaz:
http://arxiv.org/abs/2404.08910
Autor:
Ji, Xihan, Übler, Hannah, Maiolino, Roberto, D'Eugenio, Francesco, Arribas, Santiago, Bunker, Andrew J., Charlot, Stéphane, Perna, Michele, Del Pino, Bruno Rodríguez, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Kumari, Nimisha, Lamperti, Isabella
We report the chemical abundance pattern of GS\_3073, a galaxy at $z=5.55$ which was previously confirmed to host an overmassive active black hole, by leveraging the detection of about 40 emission lines, combining JWST/NIRSpec observations and ground
Externí odkaz:
http://arxiv.org/abs/2404.04148
Autor:
Perna, Michele, Arribas, Santiago, Lamperti, Isabella, Pereira-Santaella, Miguel, Ulivi, Lorenzo, Böker, Torsten, Maiolino, Roberto, Bunker, Andrew J., Charlot, Stéphane, Cresci, Giovanni, Del Pino, Bruno Rodríguez, D'Eugenio, Francesco, Übler, Hannah, Fahrion, Katja, Ceci, Matteo
Arp 220 is the nearest ULIRG; it shows evidence of 100 pc-scale molecular outflows likely connected with galaxy-scale outflows traced by ionised and neutral gas. The two highly obscured nuclei of Arp 220 are the site of intense star formation, with e
Externí odkaz:
http://arxiv.org/abs/2403.13948