Zobrazeno 1 - 10
of 3 365
pro vyhledávání: '"A. Toloza"'
Autor:
S. Gianessi, M. Polo, L. Stevanato, M. Lunardon, T. Francke, S. E. Oswald, H. Said Ahmed, A. Toloza, G. Weltin, G. Dercon, E. Fulajtar, L. Heng, G. Baroni
Publikováno v:
Geoscientific Instrumentation, Methods and Data Systems, Vol 13, Pp 9-25 (2024)
Cosmic-ray neutron sensing (CRNS) has emerged as a reliable method for soil moisture and snow estimation. However, the applicability of this method beyond research has been limited due to, among others, the use of relatively large and expensive senso
Externí odkaz:
https://doaj.org/article/6525c4f1bb694b5aafbfcf9e0f3b9110
Autor:
Cunningham, Tim, Caiazzo, Ilaria, Prusinski, Nikolaus Z., Fuller, James, Raymond, John C., Kulkarni, S. R., Neill, James D., Duffell, Paul, Martin, Chris, Toloza, Odette, Charbonneau, David, Kenyon, Scott J., Lin, Zeren, Matuszewski, Mateusz, McGurk, Rosalie, Polin, Abigail, Yao, Philippe Z.
The recently discovered Pa 30 nebula, the putative type Iax supernova remnant associated with the historical supernova of 1181 AD, shows puzzling characteristics that make it unique among known supernova remnants. In particular, Pa 30 exhibits a comp
Externí odkaz:
http://arxiv.org/abs/2410.10940
In the context of spatial econometrics, it is very useful to have methodologies that allow modeling the spatial dependence of the observed variables and obtaining more precise predictions of both the mean and the variability of the response variable,
Externí odkaz:
http://arxiv.org/abs/2409.08912
Publikováno v:
SOIL, Vol 6, Pp 179-194 (2020)
This study compares the distribution of bulk soil organic carbon (SOC), its fractions (unprotected and physically, chemically, and biochemically protected), available phosphorus (Pavail), organic nitrogen (Norg), and stable isotope (δ15N and δ13C)
Externí odkaz:
https://doaj.org/article/3a9900b43e8844daaa40318ecb984900
Autor:
Garbutt, J. A., Parsons, S. G., Toloza, O., Gänsicke, B. T., Hernandez, M. S., Koester, D., Lagos, F., Raddi, R., Rebassa-Mansergas, A., Ren, J. J., Schreiber, M. R., Zorotovic, M.
White dwarfs with a F, G or K type companion represent the last common ancestor for a plethora of exotic systems throughout the galaxy, though to this point very few of them have been fully characterised in terms of orbital period and component masse
Externí odkaz:
http://arxiv.org/abs/2403.07985
In recent years, synthesis and experimental research of fractalized materials has evolved in a paradigmatic crossover with topological phases of matter. We present here a theoretical investigation of the helical edge transport in Sierpinski carpets (
Externí odkaz:
http://arxiv.org/abs/2401.16014
Autor:
Hernandez, Mercedes S., Schreiber, Matthias R., Landstreet, John D., Bagnulo, Stefano, Parsons, Steven G., Chavarria, Martin, Toloza, Odette, Bell, Keaton J.
Recent surveys of close white dwarf binaries as well as single white dwarfs have provided evidence for the late appearance of magnetic fields in white dwarfs, and a possible generation mechanism a crystallization and rotation-driven dynamo has been s
Externí odkaz:
http://arxiv.org/abs/2401.15158
Autor:
Uzundag, Murat, De Gerónimo, Francisco C., Córsico, Alejandro H., Silvotti, Roberto, Bradley, Paul A., Montgomery, Michael H., Catelan, Márcio, Toloza, Odette, Bell, Keaton J., Kepler, S. O., Althaus, Leandro G., Kleinman, Scot J., Kilic, Mukremin, Mullally, Susan E., Gänsicke, Boris T., Bąkowska, Karolina, Barber, Sam, Nitta, Atsuko
G\,29$-$38 (TIC~422526868) is one of the brightest ($V=13.1$) and closest ($d = 17.51$\,pc) pulsating white dwarfs with a hydrogen-rich atmosphere (DAV/ZZ Ceti class). It was observed by the {\sl TESS} spacecraft in sectors 42 and 56. The atmosphere
Externí odkaz:
http://arxiv.org/abs/2309.04809
Autor:
Sahu, Snehalata, Gaensicke, Boris T., Tremblay, Pier-Emmanuel, Koester, Detlev, Hermes, J. J., Wilson, David J., Toloza, Odette, Hoskin, Matthew J., Farihi, Jay, Manser, Christopher J., Redfield, Seth
White dwarf studies carry significant implications across multiple fields of astrophysics, including exoplanets, supernova explosions, and cosmological investigations. Thus, accurate determinations of their fundamental parameters (Teff and log g) are
Externí odkaz:
http://arxiv.org/abs/2309.00239
Autor:
Inight, K., Gänsicke, Boris T., Schwope, A., Anderson, S. F., Badenes, C., Breedt, E., Chandra, V., Davies, B. D. R., Fusillo, N. P. Gentile, Green, M. J., Hermes, J. J., Huamani, I. Achaica, Hwang, H., Knauff, K., Kurpas, J., Long, K. S., Malanushenko, V., Morrison, S., C., I. J. Quiroz, Ramos, G. N. Aichele, Roman-Lopes, A., Schreiber, M. R., Standke, A., Stütz, L., Thorstensen, J. R., Toloza, O., Tovmassian, G., Zakamska, N. L.
Publikováno v:
2023MNRAS.525.3597I
SDSS-V is carrying out a dedicated survey for white dwarfs, single and in binaries, and we report the analysis of the spectroscopy of cataclysmic variables (CVs) and CV candidates obtained during the final plug plate observations of SDSS. We identify
Externí odkaz:
http://arxiv.org/abs/2305.13371