Zobrazeno 1 - 10
of 105
pro vyhledávání: '"Puschnig J."'
Autor:
Scaudo, A., Genoni, M., Causi, G. Li, Cabona, L., Landoni, M., Campana, S., Schipani, P., Claudi, R., Aliverti, M., Baruffolo, A., Ben-Ami, S., Biondi, F., Capasso, G., Cosentino, R., D'Alessio, F., D'Avanzo, P., Hershko, O., Kuncarayakti, H., Munari, M., Santhakumari, K. Radhakrishnan, Pignata, G., Rubin, A., Scuderi, S., Vitali, F., Young, D., Achrén, J., Araiza-Duran, J. A., Arcavi, I., Battaini, F., Brucalassi, A., Bruch, R., Cappellaro, E., Colapietro, M., Della Valle, M., De Pascale, M., Di Benedetto, R., D'Orsi, S., Gal-Yam, A., Hernandez, M., Kotilainen, J., Marty, L., Mattila, S., Rappaport, M., Ricci, D., Riva, M., Salasnich, B., Smartt, S., Sanchez, R. Zanmar, Stritzinger, M., Ventura, H., Cupani, G., Porru, M., Franchini, M., Cirami, R., Calderone, G., Covino, S., Smiljanic, R., Monteiro, M., Balestra, A., Sordo, R., Mason, E., Rousseu, S., Leão, I. de Castro, Zanutta, A., Martins, A. de Meideros, Sosnowska, D., Marquart, T., Boisse, I., Sousa, S., Hernandez, J., Piskunov, N., Puschnig, J., Senna, N., Martins, B., Di Marcantonio, P., Marconi, A.
We present our numerical simulation approach for the End-to-End (E2E) model applied to various astronomical spectrographs, such as SOXS (ESO-NTT), CUBES (ESO-VLT), and ANDES (ESO-ELT), covering multiple wavelength regions. The E2E model aim at simula
Externí odkaz:
http://arxiv.org/abs/2407.17542
Autor:
Marconi, A., Abreu, M., Adibekyan, V., Alberti, V., Albrecht, S., Alcaniz, J., Aliverti, M., Prieto, C. Allende, Gómez, J. D. Alvarado, Alves, C. S., Amado, P. J., Amate, M., Andersen, M. I., Antoniucci, S., Artigau, E., Bailet, C., Baker, C., Baldini, V., Balestra, A., Barnes, S. A., Baron, F., Barros, S. C. C., Bauer, S. M., Beaulieu, M., Bellido-Tirado, O., Benneke, B., Bensby, T., Bergin, E. A., Berio, P., Biazzo, K., Bigot, L., Bik, A., Birkby, J. L., Blind, N., Boebion, O., Boisse, I., Bolmont, E., Bolton, J. S., Bonaglia, M., Bonfils, X., Bonhomme, L., Borsa, F., Bouret, J. -C., Brandeker, A., Brandner, W., Broeg, C. H., Brogi, M., Brousseau, D., Brucalassi, A., Brynnel, J., Buchhave, L. A., Buscher, D. F., Cabona, L., Cabral, A., Calderone, G., Calvo-Ortega, R., Cantalloube, F., Martins, B. L. Canto, Carbonaro, L., Caujolle, Y., Chauvin, G., Chazelas, B., Cheffot, A. -L., Cheng, Y. S., Chiavassa, A., Christensen, L., Cirami, R., Cirasuolo, M., Cook, N. J., Cooke, R. J., Coretti, I., Covino, S., Cowan, N., Cresci, G., Cristiani, S., Parro, V. Cunha, Cupani, G., D'Odorico, V., Dadi, K., Leão, I. de Castro, De Cia, A., De Medeiros, J. R., Debras, F., Debus, M., Delorme, A., Demangeon, O., Derie, F., Dessauges-Zavadsky, M., Di Marcantonio, P., Di Stefano, S., Dionies, F., de Souza, A. Domiciano, Doyon, R., Dunn, J., Egner, S., Ehrenreich, D., Faria, J. P., Ferruzzi, D., Feruglio, C., Fisher, M., Fontana, A., Frank, B. S., Fuesslein, C., Fumagalli, M., Fusco, T., Fynbo, J., Gabella, O., Gaessler, W., Gallo, E., Gao, X., Genolet, L., Genoni, M., Giacobbe, P., Giro, E., Goncalves, R. S., Gonzalez, O. A., Hernández, J. I. González, Gouvret, C., Temich, F. Gracia, Haehnelt, M. G., Haniff, C., Hatzes, A., Helled, R., Hoeijmakers, H. J., Hughes, I., Huke, P., Ivanisenko, Y., Järvinen, A. S., Järvinen, S. P., Kaminski, A., Kern, J., Knoche, J., Kordt, A., Korhonen, H., Korn, A. J., Kouach, D., Kowzan, G., Kreidberg, L., Landoni, M., Lanotte, A. A., Lavail, A., Lavie, B., Lee, D., Lehmitz, M., Li, J., Li, W., Liske, J., Lovis, C., Lucatello, S., Lunney, D., MacIntosh, M. J., Madhusudhan, N., Magrini, L., Maiolino, R., Maldonado, J., Malo, L., Man, A. W. S., Marquart, T., Marques, C. M. J., Marques, E. L., Martinez, P., Martins, A., Martins, C. J. A. P., Martins, J. H. C., Maslowski, P., Mason, C. A., Mason, E., McCracken, R. A., Sousa, M. A. F. Melo e, Mergo, P., Micela, G., Milaković, D., Molliere, P., Monteiro, M. A., Montgomery, D., Mordasini, C., Morin, J., Mucciarelli, A., Murphy, M. T., N'Diaye, M., Nardetto, N., Neichel, B., Neri, N., Niedzielski, A. T., Niemczura, E., Nisini, B., Nortmann, L., Noterdaeme, P., Nunes, N. J., Oggioni, L., Olchewsky, F., Oliva, E., Onel, H., Origlia, L., Ostlin, G., Ouellette, N. N. -Q., Palle, E., Papaderos, P., Pariani, G., Pasquini, L., Castro, J. Peñate, Pepe, F., Peroux, C., Levasseur, L. Perreault, Perruchot, S., Petit, P., Pfuhl, O., Pino, L., Piqueras, J., Piskunov, N., Pollo, A., Poppenhaeger, K., Porru, M., Puschnig, J., Quirrenbach, A., Rauscher, E., Rebolo, R., Redaelli, E. M. A., Reffert, S., Reid, D. T., Reiners, A., Richter, P., Riva, M., Rivoire, S., Rodriguez-López, C., Roederer, I. U., Romano, D., Roth, M., Rousseau, S., Rowe, J., Saccardi, A., Salvadori, S., Sanna, N., Santos, N. C., Diaz, P. Santos, Sanz-Forcada, J., Sarajlic, M., Sauvage, J. -F., Savio, D., Scaudo, A, Schäfer, S., Schiavon, R. P., Schmidt, T. M., Selmi, C., Simoes, R., Simonnin, A., Sivanandam, S., Sordet, M., Sordo, R., Sortino, F., Sosnowska, D., Sousa, S. G., Spang, A., Spiga, R., Stempels, E., Stevenson, J. R. Y., Strassmeier, K. G., Mascareño, A. Suárez, Sulich, A., Sun, X., Tanvir, N. R., Tenegi-Sangines, F., Thibault, S., Thompson, S. J., Tisserand, P., Tozzi, A., Turbet, M., Veran, J. -P., Vallee, P., Vanni, I., Varas, R., Vega-Moreno, A., Venn, K. A., Verma, A., Vernet, J., Viel, M., Wade, G., Waring, C., Weber, M., Weder, J., Wehbe, B., Weingrill, J., Woche, M., Xompero, M., Zackrisson, E., Zanutta, A., Osorio, M. R. Zapatero, Zechmeister, M., Zimara, J.
The first generation of ELT instruments includes an optical-infrared high-resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion Echelle Spectrograph). ANDES consists of three fibre-fed spectrographs
Externí odkaz:
http://arxiv.org/abs/2407.14601
Autor:
François, P., Cescutti, G., Bonifacio, P., Caffau, E., Monaco, L., Steffen, M., Puschnig, J., Calura, F., Cristallo, S., Di Marcantonio, P., Dobrovolskas, V., Franchini, M., Gallagher, A. J., Hansen, C. J., Korn, A., Kuvinskas, A., Lallement, R., Lombardo, L., Lucertini, F., Magrini, L., Pinto, A. M. Matas, Matteucci, F., Mucciarelli, A., Sbordone, L., Spite, M., Spitoni, E., Valentini, M.
The MINCE (Measuring at Intermediate metallicity Neutron-Capture Elements) project aims to gather the abundances of neutron-capture elements but also of light elements and iron peak elements in a large sample of giant stars in this metallicity range.
Externí odkaz:
http://arxiv.org/abs/2404.08418
Autor:
Herenz, E. C., Inoue, J., Salas, H., Koenigs, B., Moya-Sierralta, C., Cannon, J. M., Hayes, M., Papaderos, P., Östlin, G., Bik, A., Reste, A. Le, Kusakabe, H., Monreal-Ibero, A., Puschnig, J.
Publikováno v:
A&A 670, A121 (2023)
Context: Outflows from low-mass star-forming galaxies are a fundamental ingredient for models of galaxy evolution and cosmology. Aims: The onset of kpc-scale ionised filaments in the halo of the metal-poor compact dwarf SBS 0335-052E was previously n
Externí odkaz:
http://arxiv.org/abs/2212.01239
Autor:
Reste, A. Le, Hayes, M., Cannon, J. M., Herenz, E. C., Melinder, J., Menacho, V., Östlin, G., Puschnig, J., Rivera-Thorsen, T. E., Kunth, D., Velikonja, N.
The Ly$\alpha$ emission line is one of the main observables of galaxies at high redshift, but its output depends strongly on the neutral gas distribution and kinematics around the star-forming regions where UV photons are produced. We present observa
Externí odkaz:
http://arxiv.org/abs/2206.06374
Autor:
Bešlić, I., Barnes, A. T., Bigiel, F., Puschnig, J., Pety, J., Contreras, C. Herrera, Leroy, A. K., Usero, A., Schinnerer, E., Meidt, S. E., Emsellem, E., Hughes, A., Faesi, C., Kreckel, K., Belfiore, F. M. C., Chevance, M., Brok, J. S. den, Eibensteiner, C., Glover, S. C. O., Grasha, K., Jimenez-Donaire, M. J., Klessen, R. S., Kruijssen, J. M. D., Liu, D., Pessa, I., Querejeta, M., Rosolowsky, E., Saito, T., Santoro, F., Schruba, A., Sormani, M. C., Williams, T. G.
It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required to recover significant emission from dense molecular gas at high spatial resolution, and to cover a
Externí odkaz:
http://arxiv.org/abs/2106.09742
Autor:
Brok, J. S. den, Chatzigiannakis, D., Bigiel, F., Puschnig, J., Barnes, A. T., Leroy, A. K., Jiménez-Donaire, M. J., Usero, A., Schinnerer, E., Rosolowsky, E., Faesi, C. M., Grasha, K., Hughes, A., Kruijssen, J. M. D., Liu, D., Neumann, L., Pety, J., Querejeta, M., Saito, T., Schruba, A., Stuber, S.
Both the CO(2-1) and CO(1-0) lines are used to trace the mass of molecular gas in galaxies. Translating the molecular gas mass estimates between studies using different lines requires a good understanding of the behaviour of the CO(2-1)-to-CO(1-0) ra
Externí odkaz:
http://arxiv.org/abs/2103.10442
Autor:
Harrington, Kevin C., Weiss, Axel, Yun, Min S., Magnelli, Benjamin, Sharon, C. E., Leung, T. K. D., Vishwas, A., Wang, Q. D., Jimenez-Andrade, E. F., Frayer, D. T., Liu, D., Garcia, P., Romano-Diaz, E., Frye, B. L., Jarugula, S., Badescu, T., Berman, D., Dannerbauer, H., Diaz-Sanchez, A., Grassitelli, L., Kamieneski, P., Kim, W. J., Kirkpatrick, A., Lowenthal, J. D., Messias, H., Puschnig, J., Stacey, G. J., Torne, P., Bertoldi, F.
Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and cooling mechanisms. Although it is well known that these galaxies are gas
Externí odkaz:
http://arxiv.org/abs/2010.16231
Autor:
Puschnig, J., Hayes, M., Östlin, G., Cannon, J., Smirnova-Pinchukova, I., Husemann, B., Kunth, D., Bridge, J., Herenz, E. C., Messa, M., Oteo, I.
Publikováno v:
A&A 644, A10 (2020)
We study the global dust and (molecular) gas content in the Lyman Alpha Reference Sample (LARS), i.e. 14 local star-forming galaxies. We characterize their interstellar medium and relate newly derived properties to quantities relevant for Ly$\alpha$
Externí odkaz:
http://arxiv.org/abs/2004.09142
Autor:
Jiménez-Donaire, María J., Bigiel, F., Leroy, A. K., Usero, A., Cormier, D., Puschnig, J., Gallagher, M., Kepley, A., Bolatto, A. D., García-Burillo, S., Hughes, A., Kramer, C., Pety, J., Schinnerer, E., Schruba, A., Schuster, K., Walter, F.
We present EMPIRE, an IRAM 30-m large program that mapped $\lambda = 3{-}4$ mm dense gas tracers at $\sim 1{-}2\,$kpc resolution across the whole star-forming disk of nine nearby, massive, spiral galaxies. We describe the EMPIRE observing and reducti
Externí odkaz:
http://arxiv.org/abs/1906.08779