Zobrazeno 1 - 10
of 706
pro vyhledávání: '"Álvarez, Sergio A."'
Autor:
Yuan, Yuxuan, Martin-Alvarez, Sergio, Haehnelt, Martin G., Garel, Thibault, Keating, Laura, Witstok, Joris, Sijacki, Debora
The visibility of the Lyman-$\alpha$ (Ly$\alpha$) emission from reionization-epoch galaxies depends sensitively on the extent of the intrinsic \lya emission redwards of 1215.67~\AA. The prominent red peak resulting from resonant radiative transfer in
Externí odkaz:
http://arxiv.org/abs/2412.07970
We study star formation variability, or burstiness, as a method to constrain and compare different galaxy formation models at high redshift using the Azahar simulation suite. The models range from magneto-hydrodynamics with a magneto-thermo-turbulent
Externí odkaz:
http://arxiv.org/abs/2410.00113
Understanding the role that magnetic fields play on the stage of galaxy formation requires accurate methods for inferring the properties of extragalactic magnetic fields. Radio synchrotron emission has been the most promising avenue to infer magnetic
Externí odkaz:
http://arxiv.org/abs/2409.08437
Autor:
Martin-Alvarez, Sergio, Iršič, Vid, Koudmani, Sophie, Bourne, Martin, Bigwood, Leah, Sijacki, Debora
Understanding the impact of baryonic physics on cosmic structure formation is crucial for accurate cosmological predictions, especially as we usher in the era of large galaxy surveys with the Rubin Observatory as well as the Euclid and Roman Space Te
Externí odkaz:
http://arxiv.org/abs/2407.18349
Autor:
Sanati, Mahsa, Martin-Alvarez, Sergio, Schober, Jennifer, Revaz, Yves, Slyz, Adrianne, Devriendt, Julien
Publikováno v:
A&A 690, A59 (2024)
The true nature of primordial magnetic fields (PMFs) and their role in the formation of galaxies still remains elusive. To shed light on these unknowns, we investigate their impact by varying two sets of properties: (i) accounting for the effect of P
Externí odkaz:
http://arxiv.org/abs/2403.05672
Ly$\alpha$ emission is an exceptionally informative tracer of the life cycle of evolving galaxies and the escape of ionising photons. However, theoretical studies of Ly$\alpha$ emission are often limited by insufficient numerical resolution, incomple
Externí odkaz:
http://arxiv.org/abs/2401.02572
Autor:
Martin-Alvarez, Sergio, Lopez-Rodriguez, Enrique, Dacunha, Tara, Clark, Susan E., Borlaff, Alejandro S., Beck, Rainer, Montero, Francisco Rodríguez, Jung, S. Lyla, Devriendt, Julien, Slyz, Adrianne, Roman-Duval, Julia, Ntormousi, Evangelia, Tahani, Mehrnoosh, Subramanian, Kandaswamy, Dale, Daniel A., Marcum, Pamela M., Tassis, Konstantinos, del Moral-Castro, Ignacio, Tram, Le Ngoc, Jarvis, Matt J.
The structure of magnetic fields in galaxies remains poorly constrained, despite the importance of magnetism in the evolution of galaxies. Radio synchrotron and far-infrared (FIR) polarization and polarimetric observations are the best methods to mea
Externí odkaz:
http://arxiv.org/abs/2311.06356
Autor:
Montero, Francisco Rodríguez, Martin-Alvarez, Sergio, Slyz, Adrianne, Devriendt, Julien, Dubois, Yohan, Sijacki, Debora
During the last decade, cosmological simulations have managed to reproduce realistic and morphologically diverse galaxies, spanning the Hubble sequence. Central to this success was a phenomenological calibration of the few included feedback processes
Externí odkaz:
http://arxiv.org/abs/2307.13733
Autor:
Witten, Callum, Laporte, Nicolas, Martin-Alvarez, Sergio, Sijacki, Debora, Yuan, Yuxuan, Haehnelt, Martin G., Baker, William M., Dunlop, James S., Ellis, Richard S., Grogin, Norman A., Illingworth, Garth, Katz, Harley, Koekemoer, Anton M., Magee, Daniel, Maiolino, Roberto, McClymont, William, Pérez-González, Pablo G., Puskás, David, Roberts-Borsani, Guido, Santini, Paola, Simmonds, Charlotte
During the epoch of reionisation the first galaxies were enshrouded in pristine neutral gas, with one of the brightest emission lines in star-forming galaxies, Lyman-$\alpha$ (Ly$\alpha$), expected to remain undetected until the Universe became ionis
Externí odkaz:
http://arxiv.org/abs/2303.16225
Autor:
Borlaff, Alejandro S., Lopez-Rodriguez, Enrique, Beck, Rainer, Clark, Susan E., Ntormousi, Evangelia, Tassis, Konstantinos, Martin-Alvarez, Sergio, Tahani, Mehrnoosh, Dale, Daniel A., Castro, Ignacio del Moral, Roman-Duval, Julia, Marcum, Pamela M., Beckman, John E., Subramanian, Kandaswamy, Eftekharzadeh, Sarah, Proudfit, Leslie
We present the analysis of the magnetic field ($B$-field) structure of galaxies measured with far-infrared (FIR) and radio (3 and 6 cm) polarimetric observations. We use the first data release of the Survey on extragALactic magnetiSm with SOFIA (SALS
Externí odkaz:
http://arxiv.org/abs/2303.13586