Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Sommovigo Laura"'
Autor:
Bonato, Matteo, Leisawitz, David, De Zotti, Gianfranco, Sommovigo, Laura, Shivaei, Irene, Urry, C. Megan, Farrah, Duncan, Spencer, Locke, Ricketti, Berke V., Rana, Hannah, Aalto, Susanne, Sanders, David B., Mundy, Lee G.
Far-infrared (FIR) surveys are critical to probing the co-evolution of black holes and galaxies, since of order half the light from accreting black holes and active star formation is emitted in the rest-frame infrared over $0.5\lesssim z \lesssim 10$
Externí odkaz:
http://arxiv.org/abs/2411.01216
Autor:
Schouws, Sander, Bouwens, Rychard J., Ormerod, Katherine, Smit, Renske, Algera, Hiddo, Sommovigo, Laura, Hodge, Jacqueline, Ferrara, Andrea, Oesch, Pascal A., Rowland, Lucie E., van Leeuwen, Ivana, Stefanon, Mauro, Herard-Demanche, Thomas, Fudamoto, Yoshinobu, Röttgering, Huub, van der Werf, Paul
We report the first successful ALMA follow-up observations of a secure $z > 10$ JWST-selected galaxy, by robustly detecting ($6.6\sigma$) the [OIII]$_{88\mu m}\,$ line in JADES-GS-z14-0 (hereafter GS-z14). The ALMA detection yields a spectroscopic re
Externí odkaz:
http://arxiv.org/abs/2409.20549
Autor:
Algera, Hiddo, Inami, Hanae, De Looze, Ilse, Ferrara, Andrea, Hirashita, Hiroyuki, Aravena, Manuel, Bakx, Tom, Bouwens, Rychard, Bowler, Rebecca, Da Cunha, Elisabete, Dayal, Pratika, Fudamoto, Yoshinobu, Hodge, Jacqueline, Hygate, Alexander, van Leeuwen, Ivana, Nanayakkara, Themiya, Palla, Marco, Pallottini, Andrea, Rowland, Lucie, Smit, Renske, Sommovigo, Laura, Stefanon, Mauro, Vijayan, Aswin, van der Werf, Paul
We present new multi-frequency ALMA continuum observations of the massive [$\log_{10}(M_\star/M_\odot) = 10.3_{-0.2}^{+0.1}$], UV-luminous [$M_\mathrm{UV} = -21.7 \pm 0.2$] $z=7.31$ galaxy REBELS-25 in Bands 3, 4, 5, and 9. Combining the new observat
Externí odkaz:
http://arxiv.org/abs/2408.02267
Context. Molecular Clouds (MCs) are the place where stars are formed and their feedback starts to take place, regulating the evolution of galaxies. Therefore, MCs represent the critical scale at which to study how ultra-violet (UV) photons emitted by
Externí odkaz:
http://arxiv.org/abs/2407.01662
Autor:
Bakx, Tom J. L. C., Algera, Hiddo S. B., Venemans, Bram, Sommovigo, Laura, Fujimoto, Seiji, Carniani, Stefano, Hagimoto, Masato, Hashimoto, Takuya, Inoue, Akio K., Salak, Dragan, Serjeant, Stephen, Vallini, Livia, Eales, Stephen, Ferrara, Andrea, Fudamoto, Yoshinobu, Imamura, Chihiro, Inoue, Shigeki, Knudsen, Kirsten K., Matsuo, Hiroshi, Sugahara, Yuma, Tamura, Yoichi, Taniguchi, Akio, Yamanaka, Satoshi
We present Atacama Large Millimetre/submillimetre Array (ALMA) observations of the [O$_{\rm III}$] 88 $\mu$m emission of a sample of thirteen galaxies at $z$ = 6 to 7.6 selected as [C$_{\rm II}$]-emitting companion sources of quasars. To disentangle
Externí odkaz:
http://arxiv.org/abs/2406.19439
Autor:
Rowland, Lucie E., Hodge, Jacqueline, Bouwens, Rychard, Piña, Pavel Mancera, Hygate, Alexander, Algera, Hiddo, Aravena, Manuel, Bowler, Rebecca, da Cunha, Elisabete, Dayal, Pratika, Ferrara, Andrea, Herard-Demanche, Thomas, Inami, Hanae, van Leeuwen, Ivana, de Looze, Ilse, Oesch, Pascal, Pallottini, Andrea, Phillips, Siân, Rybak, Matus, Schouws, Sander, Smit, Renske, Sommovigo, Laura, Stefanon, Mauro, van der Werf, Paul
We present high resolution ($\sim0.14$" = 710 pc) ALMA [CII] 158$\mu$m and dust continuum follow-up observations of REBELS-25, a [CII]-luminous ($L_{\mathrm{[CII]}}=(1.7\pm0.2)\times 10^9 \mathrm{L_{\odot}}$) galaxy at redshift $z=7.3065\pm0.0001$. T
Externí odkaz:
http://arxiv.org/abs/2405.06025
Autor:
van Kampen, Eelco, Bakx, Tom, De Breuck, Carlos, Chen, Chian-Chou, Dannerbauer, Helmut, Magnelli, Benjamin, Montenegro-Montes, Francisco Miguel, Okumura, Teppei, Pu, Sy-Yun, Rybak, Matus, Saintonge, Amelie, Cicone, Claudia, Hatziminaoglou, Evanthia, Hilhorst, Juliette, Klaassen, Pamela, Lee, Minju, Lovell, Christopher C., Lundgren, Andreas, Di Mascolo, Luca, Mroczkowski, Tony, Sommovigo, Laura, Booth, Mark, Cordiner, Martin A., Ivison, Rob, Johnstone, Doug, Liu, Daizhong, Maccarone, Thomas J., Smith, Matthew, Thelen, Alexander E., Wedemeyer, Sven
During the most active period of star formation in galaxies, which occurs in the redshift range 1
Externí odkaz:
http://arxiv.org/abs/2403.02806
Autor:
Lee, Minju M., Schimek, Alice, Cicone, Claudia, Andreani, Paola, Popping, Gergö, Sommovigo, Laura, Appleton, Philip N., Bischetti, Manuela, Cantalupo, Sebastiano, Chen, Chian-Chou, Dannerbauer, Helmut, De Breuck, Carlos, Di Mascolo, Luca, Emonts, Bjorn H. C., Hatziminaoglou, Evanthia, Pensabene, Antonio, Rizzo, Francesca, Rybak, Matus, Shen, Sijing, Lundgren, Andreas, Booth, Mark, Klaassen, Pamela, Mroczkowski, Tony, Cordiner, Martin A., Johnstone, Doug, van Kampen, Eelco, Liu, Daizhong, Maccarone, Thomas, Saintonge, Amélie, Smith, Matthew, Thelen, Alexander E., Wedemeyer, Sven
Our knowledge of galaxy formation and evolution has incredibly progressed through multi-wavelength observational constraints of the interstellar medium (ISM) of galaxies at all cosmic epochs. However, little is known about the physical properties of
Externí odkaz:
http://arxiv.org/abs/2403.00924
Autor:
Di Mascolo, Luca, Perrott, Yvette, Mroczkowski, Tony, Andreon, Stefano, Ettori, Stefano, Simionescu, Aurora, Raghunathan, Srinivasan, van Marrewijk, Joshiwa, Cicone, Claudia, Lee, Minju, Nelson, Dylan, Sommovigo, Laura, Booth, Mark, Klaassen, Pamela, Andreani, Paola, Cordiner, Martin A., Johnstone, Doug, van Kampen, Eelco, Liu, Daizhong, Maccarone, Thomas J., Morris, Thomas W., Saintonge, Amélie, Smith, Matthew, Thelen, Alexander E., Wedemeyer, Sven
An omnipresent feature of the multi-phase ``cosmic web'' is that warm/hot (>$10^5$ K) ionized gas pervades it. This gas constitutes a relevant contribution to the overall universal matter budget across multiple scales, from the several tens of Mpc-sc
Externí odkaz:
http://arxiv.org/abs/2403.00909
Autor:
Vallini, Livia, Witstok, Joris, Sommovigo, Laura, Pallottini, Andrea, Ferrara, Andrea, Carniani, Stefano, Kohandel, Mahsa, Smit, Renske, Gallerani, Simona, Gruppioni, Carlotta
We exploit moderately resolved [OIII], [CII] and dust continuum ALMA observations to derive the gas density ($n$), the gas-phase metallicity ($Z$) and the deviation from the Kennicutt-Schmidt (KS) relation ($\kappa_s$) on ~sub-kpc scales in the inter
Externí odkaz:
http://arxiv.org/abs/2309.07957