The miniJPAS survey: The galaxy populations in the most massive cluster in miniJPAS, mJPC2470-1771

Autor: Martín, J. E. Rodríguez, Delgado, R. M. González, Martínez-Solaeche, G., Díaz-García, L. A., de Amorim, A., García-Benito, R., Pérez, E., Fernandes, R. Cid, Carrasco, E. R., Maturi, M., Finoguenov, A., Lopes, P. A. A., Cortesi, A., Lucatelli, G., Diego, J. M., Chies-Santos, A. L., Dupke, R. A., Jiménez-Teja, Y., Vílchez, J. M., Abramo, L. R., Alcaniz, J., Benítez, N., Bonoli, S., Cenarro, A. J., Cristóbal-Hornillos, D., Ederoclite, A., Hernán-Caballero, A., López-Sanjuan, C., Marín-Franch, A., de Oliveira, C. Mendes, Moles, M., Sodré Jr., L., Taylor, K., Varela, J., Ramió, H. Vázquez, Márquez, I.

Publikováno v: A&A 666, A160 (2022)

The miniJPAS is a 1 deg$^2$ survey that uses the Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) filter system (54 narrow-band filters) with the Pathfinder camera. We study mJPC2470-1771, the most massive cluster detected

Externí odkaz: http://arxiv.org/abs/2207.10101

Floating Neutral Detection Using Actual Generation of Form 2S Meters

Autor: I. Vicente, A. Arrinda, J. E. Rodriguez-Seco, L. Piyasinghe

Publikováno v: IEEE Open Access Journal of Power and Energy, Vol 11, Pp 481-492 (2024)

In the low-voltage distribution system of the USA, Canada and some countries of Central and South America, the most used configuration is the single-phase three-wire system (120 V/240 V) also known as the split-phase distribution system. When the neu

Externí odkaz: https://doaj.org/article/c88b70f3f71c4984a3b8b1f036619f13

The multi-wavelength view of shocks in the fastest nova V1674 Her

Autor: K V Sokolovsky, T J Johnson, S Buson, P Jean, C C Cheung, K Mukai, L Chomiuk, E Aydi, B Molina, A Kawash, J D Linford, A J Mioduszewski, M P Rupen, J L Sokoloski, M N Williams, E Steinberg, I Vurm, B D Metzger, K L Page, M Orio, R M Quimby, A W Shafter, H Corbett, S Bolzoni, J DeYoung, K Menzies, F D Romanov, M Richmond, J Ulowetz, T Vanmunster, G Williamson, D J Lane, M Bartnik, M Bellaver, E Bruinsma, E Dugan, J Fedewa, C Gerhard, S Painter, D-M Peterson, J E Rodriguez, C Smith, H Sullivan, S Watson

Classical novae are shock-powered multi-wavelength transients triggered by a thermonuclear runaway on an accreting white dwarf. V1674 Her is the fastest nova ever recorded (time to declined by two magnitudes is t_2=1.1 d) that challenges our understa

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9da3ef0202cf77632a25421fdfd4af80
http://arxiv.org/abs/2302.03043

Six new compact triply eclipsing triples found with TESS

Autor: S A Rappaport, T Borkovits, R Gagliano, T L Jacobs, V B Kostov, B P Powell, I Terentev, M Omohundro, G Torres, A Vanderburg, T Mitnyan, M H Kristiansen, D LaCourse, H M Schwengeler, T G Kaye, A Pál, T Pribulla, I B Bíró, I Csányi, Z Garai, P Zasche, P F L Maxted, J E Rodriguez, D J Stevens

Publikováno v: Rappaport, S A, Borkovits, T, Gagliano, R, Jacobs, T L, Kostov, V B, Powell, B P, Terentev, I, Omohundro, M, Torres, G, Vanderburg, A, Mitnyan, T, Kristiansen, M H, Lacourse, D, Schwengeler, H M, Kaye, T G, Pál, A, Pribulla, T, Bíró, I B, Csányi, I, Garai, Z, Zasche, P, Maxted, P F L, Rodriguez, J E & Stevens, D J 2022, ' Six new compact triply eclipsing triples found with TESS ', Monthly Notices of the Royal Astronomical Society, vol. 513, no. 3, pp. 4341-4360 . https://doi.org/10.1093/mnras/stac957

In this work we report the discovery and analysis of six new compact triply eclipsing triple star systems found with the TESS mission: TICs 37743815, 42565581, 54060695, 178010808, 242132789, and 456194776. All of these exhibit distinct third body ec

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::87058c773399862fdbd861a544d768ff
https://eprints.keele.ac.uk/10984/6/stac957.pdf

Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) VII. Detection of sodium on the long-transiting inflated sub-Saturn KELT-11 b

Autor: D. Mounzer, C. Lovis, J. V. Seidel, O. Attia, R. Allart, V. Bourrier, D. Ehrenreich, A. Wyttenbach, N. Astudillo-Defru, T. G. Beatty, H. Cegla, K. Heng, B. Lavie, M. Lendl, C. Melo, F. Pepe, J. Pepper, J. E. Rodriguez, D. Ségransan, S. Udry, E. Linder, S. Sousa

KELT-11b is an inflated sub-Saturn with a hot atmosphere and that orbits a bright evolved subgiant star, making it a prime choice for atmospheric characterization, but that transits its host star for more than seven hours. We observed this system in

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::01c95c750bb82143b3ba478747d0db43