Zobrazeno 1 - 10
of 959
pro vyhledávání: '"Healy, A. F."'
Autor:
Koehn, Hauke, Rose, Henrik, Pang, Peter T. H., Somasundaram, Rahul, Reed, Brendan T., Tews, Ingo, Abac, Adrian, Komoltsev, Oleg, Kunert, Nina, Kurkela, Aleksi, Coughlin, Michael W., Healy, Brian F., Dietrich, Tim
Through continuous progress in nuclear theory and experiment and an increasing number of neutron-star observations, a multitude of information about the equation of state (EOS) for matter at extreme densities is available. To constrain the EOS across
Externí odkaz:
http://arxiv.org/abs/2402.04172
Autor:
Healy, Brian F., Coughlin, Michael W., Mahabal, Ashish A., Laz, Theophile Jegou du, Drake, Andrew, Graham, Matthew J., Hillenbrand, Lynne A., van Roestel, Jan, Szkody, Paula, Zielske, LeighAnna, Guiga, Mohammed, Hassan, Muhammad Yusuf, Hughes, Jill L., Nir, Guy, Parikh, Saagar, Park, Sungmin, Purohit, Palak, Rebbapragada, Umaa, Reed, Draco, Warshofsky, Daniel, Wold, Avery, Bloom, Joshua S., Masci, Frank J., Riddle, Reed, Smith, Roger
The classification of variable objects provides insight into a wide variety of astrophysics ranging from stellar interiors to galactic nuclei. The Zwicky Transient Facility (ZTF) provides time series observations that record the variability of more t
Externí odkaz:
http://arxiv.org/abs/2312.00143
Autor:
Reggiani, Henrique, Galarza, Jhon Yana, Schlaufman, Kevin C., Sing, David K., Healy, Brian F., McWilliam, Andrew, Lothringer, Joshua D., Pueyo, Laurent
It has been suggested that $\beta$ Pic b has a supersolar metallicity and subsolar C/O ratio. Assuming solar carbon and oxygen abundances for the star $\beta$ Pic and therefore the planet's parent protoplanetary disk, $\beta$ Pic b's C/O ratio sugges
Externí odkaz:
http://arxiv.org/abs/2311.12210
Autor:
Ofek, E. O., Strotjohann, N L., Arcavi, I., Gal-Yam, A., Kushnir, D., Waxman, E., Kasliwal, M. M., Drake, A., Graham, M., Purdum, J., Rusholme, B., Sharma, Y., Smith, R., Wold, A., Healy, B. F.
Rapid identification of the optical counterparts of Neutron Star (NS) merger events discovered by gravitational wave detectors may require observing a large error region and sifting through a large number of transients to identify the object of inter
Externí odkaz:
http://arxiv.org/abs/2311.04863
Autor:
Hussenot-Desenonges, T., Wouters, T., Guessoum, N., Abdi, I., Abulwfa, A., Adami, C., Fernández, J. F. Agüí, Ahumada, T., Aivazyan, V., Akl, D., Anand, S., Andrade, C. M., Antier, S., Ata, S. A., D'Avanzo, P., Azzam, Y. A., Baransky, A., Basa, S., Blazek, M., Bendjoya, P., Beradze, S., Boumis, P., Bremer, M., Brivio, R., Buat, V., Bulla, M., Burkhonov, O., Burns, E., Cenko, S. B., Corradi, W., Coughlin, M. W., Daigne, F., Dietrich, T., Dornic, D., Ducoin, J. -G., Duverne, P. -A., Elhosseiny, E. G., Elnagahy, F. I., El-Sadek, M. A., Ferro, M., Floc'h, E. Le, Freeberg, M., Fynbo, J. P. U., Götz, D., Gurbanov, E., Hamed, G. M., Hasanov, E., Healy, B. F., Heintz, K. E., Hello, P., Inasaridze, R., Iskandar, A., Ismailov, N., Izzo, L., Jhawar, S., Laz, T. Jegou du, Kamel, T. M., Karpov, S., Klotz, A., Koulouridis, E., Kuin, N. P., Kochiashvili, N., Leonini, S., Lu, K. -X., Malesani, D. B., Masek, M., Mao, J., Melandri, A., Mihov, B. M., Natsvlishvili, R., Navarete, F., Nedora, V., Nicolas, J., Odeh, M., Palmerio, J., Pang, P. T. H., De Pasquale, M., Peng, H. W., Pormente, S., Peloton, J., Pradier, T., Pyshna, O., Rajabov, Y., Rakotondrainibe, N. A., Rivet, J. -P., Rousselot, L., Saccardi, A., Sasaki, N., Schneider, B., Serrau, M., Shokry, A., Slavcheva-Mihova, L., Simon, A., Sokoliuk, O., Srinivasaragavan, G., Strausbaugh, R., Tanvir, N. R., Takey, A., Thöne, C. C., Tillayev, Y., Melo, I. Tosta e, Turpin, D., Postigo, A. de Ugarte, Vasylenko, V., Vergani, S. D., Vidadi, Z., Xu, D., Wang, L. T., Wang, X. F., Winters, J. M., Zhang, X -L., Zhu, Z.
GRB~230812B is a bright and relatively nearby ($z =0.36$) long gamma-ray burst (GRB) that has generated significant interest in the community and has thus been observed over the entire electromagnetic spectrum. We report over 80 observations in X-ray
Externí odkaz:
http://arxiv.org/abs/2310.14310
Autor:
Coughlin, Michael W., Bloom, Joshua S., Nir, Guy, Antier, Sarah, Laz, Theophile Jegou du, van der Walt, Stéfan, Crellin-Quick, Arien, Culino, Thomas, Duev, Dmitry A., Goldstein, Daniel A., Healy, Brian F., Karambelkar, Viraj, Lilleboe, Jada, Shin, Kyung Min, Singer, Leo P., Ahumada, Tomas, Anand, Shreya, Bellm, Eric C., Dekany, Richard, Graham, Matthew J., Kasliwal, Mansi M., Kostadinova, Ivona, Kiendrebeogo, R. Weizmann, Kulkarni, Shrinivas R., Jenkins, Sydney, LeBaron, Natalie, Mahabal, Ashish A., Neill, James D., Parazin, B., Peloton, Julien, Perley, Daniel A., Riddle, Reed, Rusholme, Ben, van Santen, Jakob, Sollerman, Jesper, Stein, Robert, Turpin, Damien, Wold, Avery, Amat, Carla, Bonnefon, Adrien, Bonnefoy, Adrien, Flament, Manon, Kerkow, Frank, Kishore, Sulekha, Jani, Shloke, Mahanty, Stephen K., Liu, Céline, Llinares, Laura, Makarison, Jolyane, Olliéric, Alix, Perez, Inès, Pont, Lydie, Sharma, Vyom
SkyPortal is an open-source software package designed to efficiently discover interesting transients, manage follow-up, perform characterization, and visualize the results. By enabling fast access to archival and catalog data, cross-matching heteroge
Externí odkaz:
http://arxiv.org/abs/2305.00108
Autor:
Ngeow, Chow-Choong, Bhardwaj, Anupam, Graham, Matthew J., Healy, Brian F., Laher, Russ R., Riddle, Reed, Wold, Avery
SX Phoenicis (SXP) variables are short period pulsating stars that exhibit a period-luminosity (PL) relation. We derived the gri-band PL and extinction-free period-Wesenheit (PW) relations, as well as the period-color (PC) and reddening-free period-Q
Externí odkaz:
http://arxiv.org/abs/2303.07554
We analyze spectroscopic and photometric data to determine the projected inclinations of stars in 11 open clusters, placing constraints on the spin-axis distributions of six clusters. We combine these results with four additional clusters studied by
Externí odkaz:
http://arxiv.org/abs/2301.10249
Autor:
Reggiani, Henrique, Schlaufman, Kevin C., Healy, Brian F., Lothringer, Joshua D., Sing, David K.
Idealized protoplanetary disk and giant planet formation models have been interpreted to suggest that a giant planet's atmospheric abundances can be used to infer its formation location in its parent protoplanetary disk. It has recently been reported
Externí odkaz:
http://arxiv.org/abs/2201.08508
We analyze spectroscopic and photometric data to determine the projected inclinations of stars in three open clusters: the Pleiades, Praesepe, and M35. We determine the $\sin i$ values of 42, 35, and 67 stars in each cluster, respectively, and from t
Externí odkaz:
http://arxiv.org/abs/2109.08692