Zobrazeno 1 - 10
of 1 010
pro vyhledávání: '"Alfonso, Eduardo"'
Autor:
Pereira-Santaella, Miguel, González-Alfonso, Eduardo, García-Bernete, Ismael, Donnan, Fergus R., Santa-Maria, Miriam G., Goicoechea, Javier R., Lamperti, Isabella, Perna, Michele, Rigopoulou, Dimitra
Publikováno v:
A&A 689, L12 (2024)
We study the 3.4-4.4$\mu$m fundamental rovibrational band of H3+, a key tracer of the ionization of the molecular interstellar medium (ISM), in a sample of 12 local (d< 400 Mpc) ultra/luminous infrared galaxies (U/LIRGs) observed with JWST/NIRSpec. T
Externí odkaz:
http://arxiv.org/abs/2408.14545
Autor:
Lankhaar, Boy, Aalto, Susanne, Wethers, Clare, Moldon, Javier, Beswick, Rob, Gorski, Mark, König, Sabine, Yang, Chentao, Mangum, Jeff, Gallagher, John, Combes, Francoise, Rigopoulou, Dimitra, González-Alfonso, Eduardo, Muller, Sébastien, Garcia-Bernete, Ismael, Henkel, Christian, Nishimura, Yuri, Ricci, Claudio
High resolution (0."037-0."13 [10-35 pc]) e-MERLIN ($\lambda6-18$ cm) and (0."024 [6.5 pc]) ALMA ($\lambda 1.1$ mm) observations have been used to image OH (hydroxyl) and H$_2$CO (formaldehyde) megamaser emission, and HCN 3->2 emission towards the nu
Externí odkaz:
http://arxiv.org/abs/2406.07620
Autor:
Pereira-Santaella, Miguel, García-Bernete, Ismael, González-Alfonso, Eduardo, Alonso-Herrero, Almudena, Colina, Luis, García-Burillo, Santiago, Rigopoulou, Dimitra, Arribas, Santiago, Perna, Michele
Publikováno v:
A&A 685, L13 (2024)
We report the detection of extended (>0.5-1kpc) high-ionization [MgIV] 4.487 $\mu$m (80 eV) emission in four local luminous infrared galaxies observed with JWST/NIRSpec. Excluding the nucleus and outflow of the Type 1 active galactic nucleus (AGN) in
Externí odkaz:
http://arxiv.org/abs/2404.16641
Autor:
González-Alfonso, Eduardo, García-Bernete, Ismael, Pereira-Santaella, Miguel, Neufeld, David A., Fischer, Jacqueline, Donnan, Fergus R.
Mid-infrared (mid-IR) gas-phase molecular bands are powerful diagnostics of the warm interstellar medium. We report the James Webb Space Telescope detection of the CO v=1-0 (4.4-5.0 um) and H2O nu2=1-0 (5.0-7.8um) ro-vibrational bands, both in absorp
Externí odkaz:
http://arxiv.org/abs/2312.04914
Autor:
Quinatoa, Daysi, Yang, Chentao, Ibar, Edo, Humphreys, Elizabeth, Aalto, Susanne, Barcos-Muñoz, Loreto, González-Alfonso, Eduardo, Impellizzeri, Violette, Jaffé, Yara, Liu, Lijie, Martín, Sergio, Weiss, Axel, Zhang, Zhi-Yu
We report the first ground-based detection of the water line p-H2O (211-202) at 752.033 GHz in three z < 0.08 ultra-luminous infrared galaxies (ULIRGs): IRAS 06035-7102, IRAS 17207-0014 and IRAS 09022-3615. Using the Atacama Pathfinder EXperiment (AP
Externí odkaz:
http://arxiv.org/abs/2311.02230
Autor:
Yang, Chentao, Omont, Alain, Martín, Sergio, Bisbas, Thomas G., Cox, Pierre, Beelen, Alexandre, González-Alfonso, Eduardo, Gavazzi, Raphaël, Aalto, Susanne, Andreani, Paola, Ceccarelli, Cecilia, Gao, Yu, Gorski, Mark, Guélin, Michel, Fu, Hai, Ivison, R. J., Knudsen, Kirsten K., Lehnert, Matthew, Messias, Hugo, Muller, Sebastien, Neri, Roberto, Riechers, Dominik, van der Werf, Paul, Zhang, Zhi-Yu
Publikováno v:
A&A 680, A95 (2023)
Understanding the nature of high-$z$ dusty galaxies requires a comprehensive view of their ISM and molecular complexity. However, the molecular ISM at high-$z$ is commonly studied using only a few species beyond CO, limiting our understanding. In thi
Externí odkaz:
http://arxiv.org/abs/2308.07368
Autor:
González-Alfonso, Eduardo, Fischer, Jacqueline, Goicoechea, Javier R., Yang, Chentao, Pereira-Santaella, Miguel, Stewart, Kenneth P.
Publikováno v:
A&A 666, L3 (2022)
H_2O submillimeter emission is a powerful diagnostic of the molecular interstellar medium in a variety of sources, including low- and high-mass star forming regions of the Milky Way, and from local to high redshift galaxies. However, the excitation m
Externí odkaz:
http://arxiv.org/abs/2209.06444
Publikováno v:
In American Journal of Ophthalmology December 2024 268:395-398
Autor:
Sakamoto, Kazushi, Gonzalez-Alfonso, Eduardo, Martin, Sergio, Wilner, David J., Aalto, Susanne, Evans, Aaron S., Harada, Nanase
We observed with ALMA three deeply buried nuclei in two galaxies, NGC 4418 and Arp 220, at $\sim$0.2$''$ resolution over a total bandwidth of 67 GHz in $f_{\rm rest}$ = 215 - 697 GHz. Here we (1) introduce our program, (2) describe our data reduction
Externí odkaz:
http://arxiv.org/abs/2109.06695
Autor:
Spinoglio, Luigi, Mordini, Sabrina, Fernandez-Ontiveros, Juan Antonio, Alonso-Herrero, Almudena, Armus, Lee, Bisigello, Laura, Calura, Francesco, Carrera, Francisco J., Cooray, Asantha, Dannerbauer, Helmut, Decarli, Roberto, Egami, Eiichi, Elbaz, David, Franceschini, Alberto, Alfonso, Eduardo Gonzalez, Graziani, Luca, Gruppioni, Carlotta, Hatziminaoglou, Evanthia, Kaneda, Hidehiro, Kohno, Kotaro, Labiano, Alvaro, Magdis, Georgios, Malkan, Matthew A., Matsuhara, Hideo, Nagao, Tohru, Naylor, David, Pereira-Santaella, Miguel, Pozzi, Francesca, Rodighiero, Giulia, Roelfsema, Peter, Serjeant, Stephen, Vignali, Cristian, Wang, Lingyu, Yamada, Toru
We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering large cosmological volumes over extended fields (1-15 square degrees) with a mid-IR imaging s
Externí odkaz:
http://arxiv.org/abs/2103.03584