Zobrazeno 1 - 10
of 7 680
pro vyhledávání: '"M Munoz"'
Autor:
Carvajal, J. P., Bauer, F. E., Reyes-Jainaga, I., Förster, F., Arancibia, A. M. Muñoz, Catelan, M., Sánchez-Sáez, P., Ricci, C., Bayo, A.
A significant challenge in the study of transient astrophysical phenomena is the identification of bogus events, with human-made Earth-orbiting satellites and debris remain a key contaminant. Existing pipelines effectively identify satellite trails b
Externí odkaz:
http://arxiv.org/abs/2411.03258
Autor:
Martin-Domenech, Rafael, Öberg, Karin I., Caro, Guillermo M. Muñoz, de Lucas, Héctor Carrascosa, Fuente, Asunción, Rajappan, Mahesh
Understanding the formation of carbonyl sulfide (OCS) in interstellar ices is key to constrain the sulfur chemistry in the interstellar medium (ISM), since it is the only ice S-bearing molecule securely detected thus far. Two general pathways for OCS
Externí odkaz:
http://arxiv.org/abs/2410.07736
Autor:
Ramirez, M., Pignata, G., Förster, Francisco, González-Gaitán, Santiago, Gutiérrez, Claudia P., Ayala, B., Cabrera-Vives, Guillermo, Catelan, Márcio, Arancibia, A. M. Muñoz, Pineda-García, J.
This paper introduces a novel method for creating spectral time series, which can be used for generating synthetic light curves for photometric classification but also for applications like K-corrections and bolometric corrections. This approach is p
Externí odkaz:
http://arxiv.org/abs/2409.10701
The reservoir of sulfur accounting for sulfur depletion in the gas of dense clouds and circumstellar regions is still unclear. One possibility is the formation of sulfur chains, which would be difficult to detect by spectroscopic techniques. This wor
Externí odkaz:
http://arxiv.org/abs/2407.14135
Autor:
Sánchez-Sáez, P., Hernández-García, L., Bernal, S., Bayo, A., Rivera, G. Calistro, Bauer, F. E., Ricci, C., Merloni, A., Graham, M. J., Cartier, R., Arévalo, P., Assef, R. J., Concas, A., Homan, D., Krumpe, M., Lira, P., Malyali, A., Martínez-Aldama, M. L., Arancibia, A. M. Muñoz, Rau, A., Bruni, G., Förster, F., Pavez-Herrera, M., Tubín-Arenas, D., Brightman, M.
The galaxy SDSS1335+0728, which had exhibited no prior optical variations during the preceding two decades, began showing significant nuclear variability in the Zwicky Transient Facility (ZTF) alert stream from December 2019 (as ZTF19acnskyy). Its be
Externí odkaz:
http://arxiv.org/abs/2406.11983
Autor:
Schiltz, L., Escribano, B., Caro, G. M. Muñoz, Cazaux, S., Olivares, C. del Burgo, Carrascosa, H., Boszhuizen, I., Díaz, C. González, Chen, Y. -J., Giuliano, B. M., Caselli, P.
The surfaces of icy moons are primarily composed of water ice that can be mixed with other compounds, such as carbon dioxide. The carbon dioxide (CO$_2)$ stretching fundamental band observed on Europa and Ganymede appears to be a combination of sever
Externí odkaz:
http://arxiv.org/abs/2405.10605
Autor:
Cabrera-Vives, G., Moreno-Cartagena, D., Astorga, N., Reyes-Jainaga, I., Förster, F., Huijse, P., Arredondo, J., Arancibia, A. M. Muñoz, Bayo, A., Catelan, M., Estévez, P. A., Sánchez-Sáez, P., Álvarez, A., Castellanos, P., Gallardo, P., Moya, A., Rodriguez-Mancini, D.
Publikováno v:
A&A 689, A289 (2024)
The advent of next-generation survey instruments, such as the Vera C. Rubin Observatory and its Legacy Survey of Space and Time (LSST), is opening a window for new research in time-domain astronomy. The Extended LSST Astronomical Time-Series Classifi
Externí odkaz:
http://arxiv.org/abs/2405.03078
Autor:
Silva-Farfán, Javier, Förster, Francisco, Moriya, Takashi J., Hernández-García, L., Arancibia, A. M. Muñoz, Sánchez-Sáez, P., Anderson, Joseph P., Tonry, John L., Clocchiatti, Alejandro
We report an analysis of a sample of 186 spectroscopically confirmed Type II supernova (SN) light curves (LCs) obtained from a combination of Zwicky Transient Facility (ZTF) and Asteroid Terrestrial-impact Last Alert System (ATLAS) observations. We i
Externí odkaz:
http://arxiv.org/abs/2404.12620
Autor:
Olivares, C. del Burgo, Carrascosa, H., Escribano, B., Caro, G. M. Muñoz, Martín-Doménech, R.
Acetic acid (CH3COOH) was detected in the gas toward interstellar clouds, hot cores, protostars and comets. Its formation in ice mantles was proposed and acetic acid awaits detection in the infrared spectra of the ice as most other COMs except methan
Externí odkaz:
http://arxiv.org/abs/2312.01845
Autor:
Guerrero, Andrea, Nagar, Neil, Kohno, Kotaro, Fujimoto, Seiji, Kokorev, Vasily, Brammer, Gabriel, Jolly, Jean-Baptiste, Knudsen, Kirsten, Sun, Fengwu, Bauer, Franz E., Caminha, Gabriel B., Caputi, Karina, Neumann, Gerald, Orellana-González, Gustavo, Cerulo, Pierluigi, González-López, Jorge, Laporte, Nicolas, Koekemoer, Anton M., Ao, Yiping, Espada, Daniel, Arancibia, Alejandra M. Muñoz
We develop new tools for continuum and spectral stacking of ALMA data, and apply these to the ALMA Lensing Cluster Survey (ALCS). We derive average dust masses, gas masses and star formation rates (SFR) from the stacked observed 260~GHz continuum of
Externí odkaz:
http://arxiv.org/abs/2309.16832