Zobrazeno 1 - 10
of 213
pro vyhledávání: '"Pal, Andras"'
Autor:
Van Dyk, Schuyler D., Szalai, Tamas, Cutri, Roc M., Kirkpatrick, J. Davy, Grillmair, Carl J., Fajardo-Acosta, Sergio B., Masiero, Joseph R., Mainzer, Amy K., Gelino, Christopher R., Vinko, Jozsef, Joo, Andras Peter, Pal, Andras, Konyves-Toth, Reka, Kriskovics, Levente, Szakats, Robert, Vida, Krisztian, Zheng, WeiKang, Brink, Thomas G., Filippenko, Alexei V.
The reactivated Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE-R) serendipitously caught the Type II supernova SN 2023ixf in Messier 101 on the rise, starting day 3.6 through day 10.9, and on the late-time decline from days 211 throug
Externí odkaz:
http://arxiv.org/abs/2406.18005
We study the problem of efficiently scheduling a computational DAG on multiple processors. The majority of previous works have developed and compared algorithms for this problem in relatively simple models; in contrast to this, we analyze this proble
Externí odkaz:
http://arxiv.org/abs/2404.15246
Autor:
Fiorellino, Eleonora, Abraham, Peter, Kospal, Agnes, Kun, Maria, Alcala, Juan M., Garatti, Alessio Caratti o, de Miera, Fernando Cruz-Saenz, Garcia-Alvarez, David, Giannini, Teresa, Park, Sunkyung, Siwak, Michal, Szilagyi, Mate, Covino, Elvira, Marton, Gabor, Nagy, Zsofia, Nisini, Brunella, Szabo, Zsofia Marianna, Bora, Zsofia, Cseh, Borbala, Kalup, Csilla, Krezinger, Mate, Kriskovics, Levente, Ogloza, Waldemar, Pal, Andras, Sodor, Adam, Sonbas, Eda, Szakats, Robert, Vida, Krisztian, Vinko, Jozsef, Wyrzykowski, Lukasz, Zielinski, Pawel
Publikováno v:
A&A 686, A160 (2024)
Context. Gaia18cjb is one of the Gaia-alerted eruptive young star candidates which has been experiencing a slow and strong brightening during the last 13 years, similar to some FU Orionis-type objects. Aims. The aim of this work is to derive the youn
Externí odkaz:
http://arxiv.org/abs/2403.08698
Autor:
Kostov, Veselin B., Powell, Brian P., Rappaport, Saul A., Borkovits, Tamas, Gagliano, Robert, Jacobs, Thomas L., Jayaraman, Rahul, Kristiansen, Martti H., LaCourse, Daryll M., Mitnyan, Tibor, Omohundro, Mark, Orosz, Jerome, Pal, Andras, Schmitt, Allan R., Schwengeler, Hans M., Terentev, Ivan A., Torres, Guillermo, Barclay, Thomas, Vanderburg, Andrew, Welsh, William
We present our second catalog of quadruple star candidates, containing 101 systems discovered in TESS Full-Frame Image data. The targets were initially detected as eclipsing binary stars with the help of supervised machine learning methods applied to
Externí odkaz:
http://arxiv.org/abs/2309.14200
This paper presents a comprehensive analysis of four triply eclipsing triple star systems, namely TIC 88206187, TIC 14839347, TIC 298714297, and TIC 66893949. The four systems with third-body eclipses were found in the TESS lightcurves from among a s
Externí odkaz:
http://arxiv.org/abs/2309.01639
Autor:
Yadavalli, S. Karthik, Villar, V. Ashley, Izzo, Luca, Zenati, Yossef, Foley, Ryan J., Wheeler, J. Craig, Angus, Charlotte R., Bánhidi, Dominik, Auchettl, Katie, Bíró, Barna Imre, Bódi, Attila, Bodola, Zsófia, de Boer, Thomas, Chambers, Kenneth C., Chornock, Ryan, Coulter, David A., Csányi, István, Cseh, Borbála, Dandu, Srujan, Davis, Kyle W., Dickinson, Connor Braden, Farias, Diego, Farah, Joseph, Gall, Christa, Gao, Hua, Howell, D. Andrew, Jacobson-Galan, Wynn V., Khetan, Nandita, Kilpatrick, Charles D., Könyves-Tóth, Réka, Kriskovics, Levente, LeBaron, Natalie, Loertscher, Kayla, Saux, X. K. Le, Margutti, Rafaella, Magnier, Eugene A., McCully, Curtis, McGill, Peter, Miao, Hao-Yu, Newsome, Megan, Gonzalez, Estefania Padilla, Pál, András, Pál, Boróka H., Pan, Yen-Chen, Politsch, Collin A., Ransome, Conor L., Ramirez-Ruiz, Enrico, Rest, Armin, Rest, Sofia, Robinson, Olivia, Sears, Huei, Scheer, Jackson, Sódor, Ádám, Swift, Jonathan, Székely, Péter, Szakáts, Róbert, Szalai, Tamás, Taggart, Kirsty, Terreran, Giacomo, Venkatraman, Padma, Vinkó, József, Yang, Grace, Zhou, Henry
We present the photometric and spectroscopic evolution of SN 2022oqm, a nearby multi-peaked hydrogen- and helium-weak calcium-rich transient (CaRT). SN 2022oqm was detected 13.1 kpc from its host galaxy, the face-on spiral galaxy NGC 5875. Extensive
Externí odkaz:
http://arxiv.org/abs/2308.12991
Autor:
Molnár, László, Plachy, Emese, Bódi, Attila, Pál, András, Joyce, Meridith, Kalup, Csilla, Johnson, Christian I., Dencs, Zoltán, Mészáros, Szabolcs, Netzel, Henryka, Kinemuchi, Karen, Kollmeier, Juna A., Prieto, Jose Luis, Derekas, Aliz
Publikováno v:
A&A 678, A104 (2023)
The globular cluster Messier 80 was monitored by the Kepler space telescope for 80 days during the K2 mission. Continuous, high-precision photometry of such an old, compact cluster allows us to study its variable star population in unprecedented deta
Externí odkaz:
http://arxiv.org/abs/2308.01560
Autor:
Pribulla, Theodor, Borkovits, Tamás, Jayaraman, Rahul, Rappaport, Saul, Mitnyan, Tibor, Zasche, Petr, Komžík, Richard, Pál, András, Uhlař, Robert, Mašek, Martin, Henzl, Zbyněk, Bíró, Imre Barna, Csányi, István, Stuik, Remko, Kristiansen, Martti H., Schwengeler, Hans M., Gagliano, Robert, Jacobs, Thomas L., Omohundro, Mark, Kostov, Veselin, Powell, Brian P., Terentev, Ivan A., Vanderburg, Andrew, LaCourse, Daryll, Rodriguez, Joseph E., Bakos, Gáspár, Csubry, Zoltán, Hartman, Joel
We have found that the 2+2 quadruple star system BU CMi is currently the most compact quadruple system known, with an extremely short outer period of only 121 days. The previous record holder was TIC 219006972 (Kostov et al. 2023), with a period of 1
Externí odkaz:
http://arxiv.org/abs/2307.01521
Autor:
Barna, Barnabas, Nagy, Andrea P., Bora, Zsofia, Czavalinga, Donat R., Konyves-Toth, Reka, Szalai, Tamas, Szekely, Peter, Zsiros, Szanna, Banhidi, Dominik, Biro, Barna I., Csanyi, Istvan, Kriskovics, Levente, Pal, Andras, Szabo, Zsofia M., Szakats, Robert, Vida, Krisztian, Bodola, Zsofia, Vinko, Jozsef
Publikováno v:
A&A 677, A183 (2023)
The nearby spiral galaxy NGC 3147 hosted three Type Ia supernovae (SNe Ia) in the past decades, which have been subjects of intense follow-up observations. Simultaneous analysis of their data provides a unique opportunity for testing the different li
Externí odkaz:
http://arxiv.org/abs/2307.01290
There is a lack of exoplanets with sizes similar to Neptune orbiting their host stars with periods $\lesssim 3$ days -- hence the name ``sub-Jovian/Neptune desert''. Recently, several exoplanets have been confirmed to reside in the desert transformin
Externí odkaz:
http://arxiv.org/abs/2304.05707