Zobrazeno 1 - 10
of 11 116
pro vyhledávání: '"Pérez S"'
Autor:
Perez, S. E., Cervantes-Vergara, B. A., Estrada, J., Holland, S., Rodrigues, D., Tiffenberg, J.
Understanding and characterizing very low-energy ($\sim$eV) background sources is a must in rare-event searches. Oscura, an experiment aiming to probe electron recoils from sub-GeV dark matter using a 10-kg skipper-CCD detector, has recently fabricat
Externí odkaz:
http://arxiv.org/abs/2406.18502
Autor:
Nogueira, P. H., Lazzoni, C., Zurlo, A., Bhowmik, T., Donoso-Oliva, C., Desidera, S., Milli, J., Pérez, S., Delorme, P., Fernadez, A., Langlois, M., Petrus, S., Cabrera-Vives, G., Chauvin, G.
Publikováno v:
A&A 687, A301 (2024)
$\eta$ Tel is an 18 Myr system with a 2.09 M$_{\odot}$ A-type star and an M7-M8 brown dwarf companion, $\eta$ Tel B, separated by 4.2'' (208 au). High-contrast imaging campaigns over 20 years have enabled orbital and photometric characterization. $\e
Externí odkaz:
http://arxiv.org/abs/2405.04723
Autor:
Hales, A. S., Gupta, A., Ruiz-Rodriguez, D., Williams, J. P., Perez, S., Cieza, L., Gonzalez-Ruilova, C., Pineda, J. E., Santamaria-Miranda, A., Tobin, J., Weber, P., Zhu, Z., Zurlo, A.
Publikováno v:
2024, ApJ, 966, 96H
We present ALMA 12-m, 7-m & Total Power (TP) Array observations of the FU Orionis outbursting system, covering spatial scales ranging from 160 to 25,000 au. The high-resolution interferometric data reveals an elongated $^{12}$CO(2-1) feature previous
Externí odkaz:
http://arxiv.org/abs/2405.03033
Polarimetric differential imaging with VLT/NACO. A comprehensive PDI pipeline for NACO data (PIPPIN)
Autor:
de Regt, S., Ginski, C., Kenworthy, M. A., Caceres, C., Garufi, A., Gledhill, T. M., Hales, A. S., Huelamo, N., Kospal, A., Millar-Blanchaer, M. A., Perez, S., Schreiber, M. R.
The observed diversity of exoplanets can possibly be traced back to the planet formation processes. Planet-disk interactions induce sub-structures in the circumstellar disk that can be revealed via scattered light observations. However, a high-contra
Externí odkaz:
http://arxiv.org/abs/2404.02222
Autor:
Zurlo, A., Weber, P., Pérez, S., Cieza, L., Ginski, C., van Holstein, R. G., Principe, D., Garufi, A., Hales, A., Kastner, J., Rigliaco, E., Ruane, G., Benisty, M., Manara, C.
Eruptive stars are a class of young stellar objects that show an abrupt increase in their luminosity. These burst-like episodes are thought to dominate the stellar accretion process during the class 0/class I stage. We present an overview of a survey
Externí odkaz:
http://arxiv.org/abs/2403.12124
Autor:
Garufi, A., Ginski, C., van Holstein, R. G., Benisty, M., Manara, C. F., Pérez, S., Pinilla, P., Ribas, Á., Weber, P., Williams, J., Cieza, L., Dominik, C., Facchini, S., Huang, J., Zurlo, A., Bae, J., Hagelberg, J., Henning, Th., Hogerheijde, M. R., Janson, M., Ménard, F., Messina, S., Meyer, M. R., Pinte, C., Quanz, S. P., Rigliaco, E., Roccatagliata, V., Schmid, H. M., Szulágyi, J., van Boekel, R., Wahhaj, Z., Antichi, J., Baruffolo, A., Moulin, T.
The sample of planet-forming disks observed by high-contrast imaging campaigns over the last decade is mature enough to enable the demographical analysis of individual star-forming regions. We present the full census of Taurus sources with VLT/SPHERE
Externí odkaz:
http://arxiv.org/abs/2403.02158
We study the emission of gravitational waves from spheroidal magnetized strange stars for both an isolated slowly rotating star and a binary system. In the first case, we compute the quadrupole moment and the amplitude of gravitational waves that may
Externí odkaz:
http://arxiv.org/abs/2401.11799
Autor:
Depaoli, E., Rodrigues, D., Sidelnik, I., Bellino, P., Botti, A., Delgado, D., Cababie, M., Chierchie, F., Estrada, J., Moroni, G. Fernandez, Perez, S., Tiffenberg, J.
Charge Coupled Devices (CCD) are used for reactor neutrino experiments and already shown their potential in constraining new physics models. The prospect of a Skipper-CCD experiment looking for standard and beyond standard model physics (BSM) in a nu
Externí odkaz:
http://arxiv.org/abs/2401.07885
Autor:
Aguilar-Arevalo, A. A., Barrow, J. L., Bhat, C., Bogenschuetz, J., Bonifazi, C., Bross, A., Cervantes, B., D'Olivo, J., De Roeck, A., Dutta, B., Eads, M., Eldred, J., Estrada, J., Fava, A., Vilela, C. Fernandes, Moroni, G. Fernandez, Flaugher, B., Gardiner, S., Gurung, G., Gutierrez, P., Jang, W. Y., Kelly, K. J., Kim, D., Kobilarcik, T., Liu, Z., Lyu, K. F., Machado, P., Mahapatra, R., Marjanovic, M., Mastbaum, A., Pandey, V., Pellico, W., Perez, S., Reichenbacher, J., Rodrigues, D., Sousa, A., Simons, B., Snowden-Ifft, D., Tan, C. -Y., Toups, M., Tran, N., Tsai, Y. -T., Van de Water, R. G., Vilar, R., Westerdale, S., Yu, J., Zettlemoyer, J., Zwaska, R.
The Fermilab Proton-Improvement-Plan-II (PIP-II) is being implemented in order to support the precision neutrino oscillation measurements at the Deep Underground Neutrino Experiment, the U.S. flagship neutrino experiment. The PIP-II LINAC is presentl
Externí odkaz:
http://arxiv.org/abs/2311.09915
Autor:
Weber, P., Pérez, S., Zurlo, A., Miley, J., Hales, A., Cieza, L., Principe, D., Cárcamo, M., Garufi, A., Kóspál, Á., Takami, M., Kastner, J., Zhu, Z., Williams, J.
The formation of giant planets has traditionally been divided into two pathways: core accretion and gravitational instability. However, in recent years, gravitational instability has become less favored, primarily due to the scarcity of observations
Externí odkaz:
http://arxiv.org/abs/2307.13433