Zobrazeno 1 - 10
of 34
pro vyhledávání: '"LaCluyze, Aaron P."'
Autor:
Slivan, Stephen M., Hosek Jr., Matthew, Kurzner, Max, Sokol, Alyssa, Maynard, Sarah, Payne, Anna V., Radford, Arden, Springmann, Alessondra, Binzel, Richard P., Wilkin, Francis P., Mailhot, Emily A., Midkiff, Alan H., Russell, April, Stephens, Robert D., Gardiner, Vincent, Reichart, Daniel E., Haislip, Joshua, LaCluyze, Aaron, Behrend, Raoul, Roy, René
An observational study of Koronis family members' spin properties was undertaken with two primary objectives: to reduce selection biases for object rotation period and lightcurve amplitude in the sample of members' known spin vectors, and to better c
Externí odkaz:
http://arxiv.org/abs/2212.12355
Autor:
Caddy, Robert V., Layden, Andrew C., Reichart, Daniel E., Haislip, Joshua B., Kouprianov, Vladimir V., Ivarsen, Kevin M., Moore, Justin P., LaCluyze, Aaron P., Linder, Tyler R., Nysewander, Melissa C.
Publikováno v:
PASP 134 094201 (2022)
We present time-series CCD photometry in the $BVRI$ passbands of the recently identified symbiotic nova V1835 Aquilae (NSV 11749) over an interval of 5.1 years with 7-14 day cadence, observed during its quiescence. We find slow light variations with
Externí odkaz:
http://arxiv.org/abs/2209.11251
Most students do not enroll in introductory astronomy as part of their major; for many, it is the last science course they will ever take. Thus, it has great potential to shape students' attitudes toward STEM fields for the rest of their life. We the
Externí odkaz:
http://arxiv.org/abs/1910.12630
Autor:
Folatelli, Gastón, Bersten, Melina C., Kuncarayakti, Hanindyo, Estay, Felipe Olivares, Anderson, Joseph P., Holmbo, Simon, Maeda, Keiichi, Morrell, Nidia, Nomoto, Ken'ichi, Pignata, Giuliano, Stritzinger, Maximilian, Contreras, Carlos, Förster, Francisco, Hamuy, Mario, Phillips, Mark M., Prieto, José Luis, Valenti, Stefano, Afonso, Paulo, Altenmüller, Konrad, Elliott, Jonny, Greiner, Jochen, Updike, Adria, Haislip, Joshua B., LaCluyze, Aaron P., Moore, Justin P., Reichart, Daniel E.
Publikováno v:
2014 ApJ 792 7
We present extensive optical and near-infrared photometric and spectroscopic observations of the stripped-envelope (SE) supernova SN 2010as. Spectroscopic peculiarities, such as initially weak helium features and low expansion velocities with a nearl
Externí odkaz:
http://arxiv.org/abs/1407.6711
Autor:
Jin, Zhi-Ping, Covino, Stefano, Della Valle, Massimo, Ferrero, Patrizia, Fugazza, Dino, Malesani, Daniele, Melandri, Andrea, Pian, Elena, Salvaterra, Ruben, Bersier, David, Campana, Sergio, Cano, Zach, Castro-Tirado, Alberto J., D'Avanzo, Paolo, Fynbo, Johan P. U., Gomboc, Andreja, Gorosabel, Javier, Guidorzi, Cristiano, Haislip, Joshua B., Hjorth, Jens, Kobayashi, Shiho, LaCluyze, Aaron P., Marconi, Gianni, Mazzali, Paolo A., Mundell, Carole G., Piranomonte, Silvia, Reichart, Daniel E., Sánchez-Ramírez, Rubén, Smith, Robert J., Steele, Iain A., Tagliaferri, Gianpiero, Tanvir, Nial R., Valenti, Stefano, Vergani, Susanna D., Vestrand, Thomas, Walker, Emma S., Wozniak, Przemyslaw
Publikováno v:
Astrophys. Journ. 774 (2013) 114
We discuss the results of the analysis of multi-wavelength data for the afterglows of GRB 081007 and GRB 090424, two bursts detected by Swift. One of them, GRB 081007, also shows a spectroscopically confirmed supernova, SN 2008hw, which resembles SN
Externí odkaz:
http://arxiv.org/abs/1306.4585
Autor:
Schaefer, Bradley E., Pagnotta, Ashley, LaCluyze, Aaron, Reichart, Daniel E., Ivarsen, Kevin M., Haislip, Joshua B., Nysewander, Melissa C., Moore, Justin P., Oksanen, Arto, Worters, Hannah L., Sefako, Ramotholo R., Mentz, Jaco, Dvorak, Shawn, Gomez, Tomas, Harris, Barbara G., Henden, Arne, Tan, Thiam Guan, Templeton, Matthew, Allen, W. H., Monard, Berto, Rea, Robert D., Roberts, George, Stein, William, Maehara, Hiroyuki, Richards, Thomas, Stockdale, Chris, Krajci, Tom, Sjoberg, George, McCormick, Jennie, Revnivtsev, Mikhail, Molkov, Sergei, Suleimanov, Valery, Darnley, Matthew J., Bode, Michael F., Handler, Gerald, Lepine, Sebastien, Shara, Michael
The eruption of the recurrent nova U Scorpii on 28 January 2010 is now the all-time best observed nova event. We report 36,776 magnitudes throughout its 67 day eruption, for an average of one measure every 2.6 minutes. This unique and unprecedented c
Externí odkaz:
http://arxiv.org/abs/1108.1214
Autor:
Sarty, Gordon E., Pilecki, Bogumil, Reichart, Daniel E., Ivarsen, Kevin M., Haislip, Joshua B., Nysewander, Melissa C., LaCluyze, Aaron P., Johnston, Helen M., Shobbrook, Robert R., Kiss, Laszlo L., Wu, Kinwah
We searched for long period variation in V-band, Ic-band and RXTE X-ray light curves of the High Mass X-ray Binaries (HMXBs) LS 1698 / RX J1037.5-5647, HD 110432 / 1H 1249-637 and HD 161103 / RX J1744.7-2713 in an attempt to discover orbitally induce
Externí odkaz:
http://arxiv.org/abs/1105.2025
Autor:
Pignata, Giuliano, Stritzinger, Maximilian, Soderberg, Alicia, Mazzali, Paolo, Phillips, M. M., Morrell, Nidia, Anderson, J. P., Boldt, Luis, Campillay, Abdo, Contreras, Carlos, Folatelli, Gastón, Förster, Francisco, González, Sergio, Hamuy, Mario, Krzeminski, Wojtek, Maza, José, Roth, Miguel, Levesque, Francisco Salgado Emily M., Rest, Armin, Crain, J. Adam, Foster, Andrew C., Haislip, Joshua B., Ivarsen, Kevin M., LaCluyze, Aaron P., Nysewander, Melissa C., Reichart, Daniel E.
Ultraviolet, optical, and near-infrared photometry and optical spectroscopy of the broad-lined Type Ic supernova (SN) 2009bb are presented, following the flux evolution from -10 to +285 days past B-band maximum. Thanks to the very early discovery, it
Externí odkaz:
http://arxiv.org/abs/1011.6126
Autor:
Rabidoux, Katie, Smith, Horace A., Pritzl, Barton J., Osborn, Wayne, Kuehn, Charles, Randall, Jill, Lustig, R., Wells, K., Taylor, Lisa, De Lee, Nathan, Kinemuchi, K., LaCluyzé, Aaron, Hartley, D., Greenwood, C., Ingber, M., Ireland, M., Pellegrini, E., Anderson, Mary, Purdum, Gene, Lacy, J., Curtis, M., Smolinski, Jason, Danford, Stephen
Light curves in the B, V, and I_c passbands have been obtained for the type II Cepheids V154 in M3 and V42 and V84 in M5. Alternating cycle behavior, similar to that seen among RV Tauri variables, is confirmed for V84. Old and new observations, spann
Externí odkaz:
http://arxiv.org/abs/1003.5924
Autor:
LaCluyze, Aaron, Smith, Horace A., Gill, E. -M., Hedden, A., Kinemuchi, Karen, Rosas, A. M., Pritzl, Barton J., Sharpee, Brian, Wilkinson, Christopher, Robinson, K. W., Baldwin, Marvin E., Samolyk, Gerard
New CCD photometry has been obtained for the RR Lyrae variable star XZ Cygni. An analysis of old and new photometry confirms earlier results that XZ Cygni exhibits the Blazhko Effect and that its Blazhko period has changed over time. These changes in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0401314