Browsing by Author "Aravena, M."

Now showing items 1-5 of 5

    • Molecular gas budget and characterization of intermediate-mass star-forming galaxies at z approximate to 2-3 
      Solimano, M.; González López, J.; Barrientos, L. F.; Aravena, M.; López, S.; Tejos, N.; Sharon, K.; Dahle, H.; Bayliss, M.; Ledoux, C.; Rigby, J. R.; Gladders, M. (EDP Sciences, 2021)
      Star-forming galaxies (SFGs) with stellar masses below 10(10) M-circle dot make up the bulk of the galaxy population at z > 2. The properties of the cold gas in these galaxies can only be probed in very deep observations ...
    • Normal, dust-obscured galaxies in the epoch of reionization 
      Fudamoto, Y.; Oesch, P. A.; Schouws, S.; Stefanon, M.; Smit, R.; Bouwens, R. J.; Bowler, R. A. A.; Endsley, R.; González, V.; Inami, H.; Labbe, I.; Stark, D.; Aravena, M.; Barrufet, L.; da Cunha, E.; Dayal, P.; Ferrara, A.; Graziani, L.; Hodge, J.; Hutter, A.; Li, Y.; De Looze, I.; Nanayakkara, T.; Pallottini, A.; Riechers, D.; Schneider, R.; Ucci, G.; van der Werf, P.; White, C. (Nature, 2021)
      Two serendipitously detected dust-obscured galaxies are reported at z = 6.7 and 7.4, with estimates that such galaxies provide an additional 10-25% contribution to the total star formation rate density at z > 6. Over ...
    • Photon dominated regions in NGC 3603 [CI] and mid-J CO line emission 
      Röllig, M.; Kramer, C.; Rajbahak, C.; Minamidani, T.; Sun, K.; Simon, R.; Ossenkopf, V.; Cubick, M.; Hitschfeld, M.; Aravena, M.; Bensch, F.; Bertoldi, F.; Bronfman Aguiló, Leonardo; Fujishita, M.; Fukui, Y.; Graf, U. U.; Honingh, N.; Ito, S.; Jakob, H.; Jacobs, K.; Klein, U.; Koo, B.-C.; May Humeres, Jorge; Miller, M.; Miyamoto, Y.; Mizuno, N.; Onishi, T.; Park, Y.-S.; Pineda, J.; Rabanus, D.; Sasago, H.; Schieder, R.; Stutzki, J.; Yamamoto, H.; Yonekura, Y. (2011-01)
      Aims. We aim at deriving the excitation conditions of the interstellar gas as well as the local FUV intensities in the molecular cloud surrounding NGC 3603 to get a coherent picture of how the gas is energized by the central ...
    • Reionization era bright emission line survey: selection and characterization of luminous interstellar medium ... 
      Bouwens, R. J.; Smit, R.; Schouws, S.; Stefanon, M.; Bowler, R.; Endsley, R.; González Corvalán, Valentino Gastón; Inami, H.; Stark, D.; Oesch, P.; Hodge, J.; Aravena, M.; Da Cunha, E.; Dayal, P.; De Looze, I.; Ferrara, A.; Fudamoto, Y.; Graziani, L.; Li, C.; Nanayakkara, T.; Pallottini, A.; Schneider, R.; Sommovigo, L.; Topping, M.; Van der Werf, P.; Algera, H.; Barrufet, L.; Hygate, A.; Labbé, I.; Riechers, D.; Witstok, J. (IOP, 2022)
      The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA Large Program (LP) that is identifying and performing a first characterization of many of the most luminous star-forming galaxies known in the z ...
    • VALES V: A kinematic analysis of the molecular gas content in H-ATLAS galaxies at z ~ 0.03-0.35 using ALMA 
      Molina, J.; Ibar, Edo; Villanueva, V.; Escala, A.; Cheng, C.; Baes, M.; Messias, H.; Yang, C.; Bauer, F. E.; van der Werf,; Leiton, R.; Aravena, M.; Swinbank, A. M.; Michalowski, M. J.; Muñoz-Arancibia, A. M.; Orellana, G.; Hughes, T. M.; Farrah, D.; De Zotti, G.; Lara-Lóp (Oxford University Press, 2019)
      © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.We present Atacama Large Millimeter/submillimeter Array (ALMA) resolved observations of molecular gas in galaxies up ...