Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Mikolajczyk, Przemyslaw"'
Autor:
Herbert, Carys, Froebrich, Dirk, Vanaverbeke, Siegfried, Scholz, Aleks, Eislöffel, Jochen, Urtly, Thomas, Walton, Ivan L., Wiersema, Klaas, Quinn, Nick J., Piehler, Georg, Aimar, Mario Morales, García, Rafael Castillo, Vanmunster, Tonny, Alfaro, Francisco C. Soldán, de la Cuesta, Faustino García, Licchelli, Domenico, Perez, Alex Escartin, Mañanes, Esteban Fernández, Ribes, Noelia Graciá, González, José Luis Salto, Futcher, Stephen R. L., Nelson, Tim, Dvorak, Shawn, Moździerski, Dawid, Kotysz, Krzysztof, Mikołajczyk, Przemysław, Fleming, George, Phillips, Mark, Vale, Tony, Dubois, Franky, Eggenstein, Heinz-Bernd, Heald, Michael A., Lewin, Pablo, OKeeffe, Derek, Popowicz, Adam, Bernacki, Krzysztof, Malcher, Andrzej, Lasota, Slawomir, Fiolka, Jerzy, Dustor, Adam, Percy, Stephen C., Devine, Pat, Patel, Aashini L., Dickers, Matthew D., Dover, Lord, Grozdanova, Ivana I., Urquhart, James S., Lynch, Chris J. R.
We present spot properties on 32 periodic young stellar objects in IC 5070. Long term, $\sim$5 yr, light curves in the $V$, $R$, and $I$-bands are obtained through the HOYS (Hunting Outbursting Young Stars) citizen science project. These are dissecte
Externí odkaz:
http://arxiv.org/abs/2403.10595
Autor:
Froebrich, Dirk, Scholz, Aleks, Campbell-White, Justyn, Vanaverbeke, Siegfried, Herbert, Carys, Eislöffel, Jochen, Urtly, Thomas, Long, Timothy P., Walton, Ivan L., Wiersema, Klaas, Quinn, Nick J., Rodda, Tony, González-Carballo, Juan-Luis, Aimar, Mario Morales, García, Rafael Castillo, Alfaro, Francisco C. Soldán, de la Cuesta, Faustino García, Licchelli, Domenico, Perez, Alex Escartin, González, José Luis Salto, Deldem, Marc, Futcher, Stephen R. L., Nelson, Tim, Dvorak, Shawn, Moździerski, Dawid, Kotysz, Krzysztof, Mikołajczyk, Przemysław, Fleming, George, Phillips, Mark, Vale, Tony, Öğmen, Yenal, Dubois, Franky, Rolfe, Samantha M., Campbell, David A., Eggenstein, Heinz-Bernd, Hambsch, Franz-Josef, Heald, Michael A., Lewin, Pablo, Rose, Adam C., Stone, Geoffrey, Crow, Martin Valentine, Dawes, Simon Francis, OKeeffe, Derek, Popowicz, Adam, Bernacki, Krzysztof, Malcher, Andrzej, Lasota, Slawomir, Fiolka, Jerzy, Dustor, Adam, Vajpayee, Amritanshu, Devine, Pat, Kolb, Matthias, Marquette, Jean-Baptiste, Ruppel, Gregg L., Crowson, Dan R., da Silva, Cledison Marcos, Michaud, Michel, Patel, Aashini L., Dickers, Matthew D., Dover, Lord, Grozdanova, Ivana I., Urquhart, James S., Lynch, Chris J. R.
The Hunting Outbursting Young Stars (HOYS) project performs long-term, optical, multi-filter, high cadence monitoring of 25 nearby young clusters and star forming regions. Utilising Gaia DR3 data we have identified about 17000 potential young stellar
Externí odkaz:
http://arxiv.org/abs/2401.16883
Autor:
Nagy, Zsófia, Park, Sunkyung, Ábrahám, Péter, Kóspál, Ágnes, de Miera, Fernando Cruz-Sáenz, Kun, Mária, Siwak, Michał, Szabó, Zsófia Marianna, Szilágyi, Máté, Fiorellino, Eleonora, Giannini, Teresa, Lee, Jae-Joon, Lee, Jeong-Eun, Marton, Gábor, Szabados, László, Vitali, Fabrizio, Andrzejewski, Jan, Gromadzki, Mariusz, Hodgkin, Simon, Jabłońska, Maja, Mendez, Rene A., Merc, Jaroslav, Michniewicz, Olga, Mikołajczyk, Przemysław J., Pylypenko, Uliana, Ratajczak, Milena, Wyrzykowski, Łukasz, Zejmo, Michal, Zieliński, Paweł
FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that last from decades to a century. Due to the duration of their outbursts, and to the fact that only about two dozens of such sources are known, information on the end of
Externí odkaz:
http://arxiv.org/abs/2307.01629
Autor:
Froebrich, Dirk, Hillenbrand, Lynne A., Herbert, Carys, De, Kishalay, Eislöffel, Jochen, Campbell-White, Justyn, Kahar, Ruhee, Hambsch, Franz-Josef, Urtly, Thomas, Popowicz, Adam, Bernacki, Krzysztof, Malcher, Andrzej, Lasota, Slawomir, Fiolka, Jerzy, Jozwik-Wabik, Piotr, Dubois, Franky, Logie, Ludwig, Rau, Steve, Phillips, Mark, Fleming, George, Farfán, Rafael Gonzalez, Alfaro, Francisco C. Soldán, Nelson, Tim, Futcher, Stephen R. L., Rolfe, Samantha M., Campbell, David A., Vale, Tony, Devine, Pat, Moździerski, Dawid, Mikołajczyk, Przemysław J., Eggenstein, Heinz-Bernd, Rodriguez, Diego, Walton, Ivan L, Vanaverbeke, Siegfried, Merrikin, Barry, Öğmen, Yenal, Perez, Alex Escartin, Aimar, Mario Morales, Piehler, Georg, Dover, Lord, Patel, Aashini L., Miller, Niall, Finch, Jack, Hankins, Matt, Moore, Anna M., Travouillon, Tony, Szczepanski, Marek
This paper is one in a series reporting results from small telescope observations of variable young stars. Here, we study the repeating outbursts of three likely Be stars based on long-term optical, near-infrared, and mid-infrared photometry for all
Externí odkaz:
http://arxiv.org/abs/2302.02696
Autor:
Jiang, Chen, Wu, Tao, Feinstein, Adina D., Stassun, Keivan G., Bedding, Timothy R., Veras, Dimitri, Corsaro, Enrico, Buzasi, Derek L., Stello, Dennis, Li, Yaguang, Mathur, Savita, Garcia, Rafael A., Breton, Sylvain N., Lundkvist, Mia S., Mikolajczyk, Przemyslaw J., Gehan, Charlotte, Campante, Tiago L., Bossini, Diego, Kane, Stephen R., Ong, Jia Mian Joel, Yildiz, Mutlu, Kayhan, Cenk, Orhan, Zeynep Celik, Ortel, Sibel, Zhang, Xinyi, Cunha, Margarida S., de Moura, Bruno Lustosa, Yu, Jie, Huber, Daniel, Ou, Jian-wen, Wittenmyer, Robert A., Gizon, Laurent, Chaplin, William J.
The Transiting Exoplanet Survey Satellite (TESS) mission searches for new exoplanets. The observing strategy of TESS results in high-precision photometry of millions of stars across the sky, allowing for detailed asteroseismic studies of individual s
Externí odkaz:
http://arxiv.org/abs/2302.01102
Autor:
Wielgórski, Piotr, Pietrzyński, Grzegorz, Pilecki, Bogumił, Gieren, Wolfgang, Zgirski, Bartłomiej, Górski, Marek, Hajdu, Gergely, Narloch, Weronika, Karczmarek, Paulina, Smolec, Radosław, Kervella, Pierre, Storm, Jesper, Gallenne, Alexandre, Breuval, Louise, Lewis, Megan, Kałuszyński, Mikołaj, Graczyk, Dariusz, Pych, Wojciech, Suchomska, Ksenia, Taormina, Mónica, Garcia, Gonzalo Rojas, Kotek, Aleksandra, Chini, Rolf, Nuñez, Francisco Pozo, Noroozi, Sadegh, Figaredo, Catalina Sobrino, Haas, Martin, Hodapp, Klaus, Mikołajczyk, Przemysław, Kotysz, Krzysztof, Moździerski, Dawid, Kołaczek-Szymański, Piotr
We present time-series photometry of 21 nearby Type II Cepheids in the near-infrared J, H and Ks passbands. We use this photometry, together with the Third Gaia Early Data Release parallaxes, to determine for the first time period-luminosity relation
Externí odkaz:
http://arxiv.org/abs/2112.12122
Autor:
Froebrich, Dirk, Derezea, Efthymia, Scholz, Aleks, Eislöffel, Jochen, Vanaverbeke, Siegfried, Kume, Alfred, Herbert, Carys, Campbell-White, Justyn, Miller, Niall, Stecklum, Bringfried, Makin, Sally V., Urtly, Thomas, Alfaro, Francisco C. Soldán, Schwendeman, Erik, Stone, Geoffrey, Phillips, Mark, Fleming, George, Farfán, Rafael Gonzalez, Vanmunster, Tonny, Heald, Michael A., Mañanes, Esteban Fernández, Nelson, Tim, Eggenstein, Heinz-Bernd, Dubois, Franky, Logie, Ludwig, Rau, Steve, Wiersema, Klaas, Quinn, Nick, Rodriguez, Diego, García, Rafael Castillo, Killestein, Thomas, Vale, Tony, Licchelli, Domenico, Deldem, Marc, Piehler, Georg, Moździerski, Dawid, Kotysz, Krzysztof, Kowalska, Katarzyna, Mikołajczyk, Przemysław, Futcher, Stephen R. L., Long, Timothy P., Aimar, Mario Morales, Merrikin, Barry, Johnstone, Stephen, Dubovský, Pavol A., Kudzej, Igor, Pickard, Roger, Billington, Samuel J., Dover, Lord, Zegmott, Tarik, Evitts, Jack J., Munia, Alejandra Traspas, Price, Mark C.
Studying rotational variability of young stars is enabling us to investigate a multitude of properties of young star-disk systems. We utilise high cadence, multi-wavelength optical time series data from the Hunting Outbursting Young Stars citizen sci
Externí odkaz:
http://arxiv.org/abs/2107.08524
Autor:
Zhang, Jujia, Wang, Xiaofeng, Vinko, Jozsef, Zhai, Qian, Zhang, Tianmeng, Filippenko, Alexei V., Brink, Thomas G., Zheng, WeiKang, Wyrzykowski, Lukasz, Mikolajczyk, Przemyslaw, Huang, Fang, Rui, Liming, Mo, Jun, Sai, Hanna, Zhang, Xinhan, Wang, Huijuan, DerKacy, James M., Baron, Eddie, Sarneczky, K., Bodi, A., Csornyei, G., Hanyecz, O., Ignacz, B., Kalup, Cs., Kriskovics, L., Konyves-Toth, R., Ordasi, A., Pal, A., Sodor, A., Szakats, R., Vida, K., Zsidi, G.
We present extensive observations of SN 2018zd covering the first $\sim450$\,d after the explosion. This SN shows a possible shock-breakout signal $\sim3.6$\,hr after the explosion in the unfiltered light curve, and prominent flash-ionisation spectra
Externí odkaz:
http://arxiv.org/abs/2007.14348
Autor:
Zielinski, Pawel, Wyrzykowski, Lukasz, Mikolajczyk, Przemyslaw, Rybicki, Krzysztof, Kolaczkowski, Zbigniew
We present a new automatic tool for time-domain astronomy - the Cambridge Photometric Calibration Server 2.0 - developed under OPTICON H2020 programme. It has been designed to respond to the need of automated rapid photometric data calibration and di
Externí odkaz:
http://arxiv.org/abs/2006.05160
Autor:
Jiang, Chen, Bedding, Timothy R., Stassun, Keivan G., Veras, Dimitri, Corsaro, Enrico, Buzasi, Derek L., Mikołajczyk, Przemysław, Qian-sheng, Zhang, Jian-wen, Ou, Campante, Tiago L., Rodrigues, Thaíse S., Nsamba, Benard, Bossini, Diego, Kane, Stephen R., Ong, Jia Mian Joel, Yıldız, Mutlu, Orhan, Zeynep Çeiik, Örtel, Sibel, Wu, Tao, Zhang, Xinyi, Li, Tanda, Basu, Sarbani, Cunha, Margarida S., Christensen-Dalsgaard, Jørgen, Chaplin, William J.
The Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission aiming to search for exoplanets that transit bright stars. The high-quality photometric data of TESS are excellent for the asteroseismic study of solar-like stars. In this
Externí odkaz:
http://arxiv.org/abs/2005.00272