Zobrazeno 1 - 10
of 3 378
pro vyhledávání: '"Krolikowski, P."'
Autor:
Getman, Konstantin V., Kochukhov, Oleg, Ninan, Joe P., Feigelson, Eric D., Airapetian, Vladimir S., Waggoner, Abygail R., Cleeves, L. Ilsedore, Forbrich, Jan, Dzib, Sergio A., Law, Charles J., Rab, Christian, Krolikowski, Daniel M.
We explore the empirical power-law relationship between X-ray luminosity (Lx) and total surface magnetic flux (Phi), established across solar magnetic elements, time- and disk-averaged emission from the Sun, older active stars, and pre-main-sequence
Externí odkaz:
http://arxiv.org/abs/2501.01321
Autor:
Beard, Corey, Robertson, Paul, Lubin, Jack, Han, Te, Holcomb, Rae, Premnath, Pranav, Butler, R. Paul, Dalba, Paul A., Holden, Brad, Blake, Cullen H., Diddams, Scott A., Gupta, Arvind F., Halverson, Samuel, Krolikowski, Daniel M., Li, Dan, Lin, Andrea S. J., Logsdon, Sarah E., Lubar, Emily, Mahadevan, Suvrath, McElwain, Michael W., Ninan, Joe P., Paredes, Leonardo A., Roy, Arpita, Schwab, Christian, Stefansson, Gudmundur, Terrien, Ryan C., Wright, Jason T.
Stellar activity contamination of radial velocity (RV) data is one of the top challenges plaguing the field of extreme precision RV (EPRV) science. Previous work has shown that photometry can be very effective at removing such signals from RV data, e
Externí odkaz:
http://arxiv.org/abs/2412.11329
Autor:
Barber, Madyson G., Mann, Andrew W., Vanderburg, Andrew, Krolikowski, Daniel, Kraus, Adam, Ansdell, Megan, Pearce, Logan, Mace, Gregory N., Andrews, Sean M., Boyle, Andrew W., Collins, Karen A., De Furio, Matthew, Dragomir, Diana, Espaillat, Catherine, Feinstein, Adina D., Fields, Matthew, Jaffe, Daniel, Murillo, Ana Isabel Lopez, Murgas, Felipe, Newton, Elisabeth R., Palle, Enric, Sawczynec, Erica, Schwarz, Richard P., Thao, Pa Chia, Tofflemire, Benjamin M., Watkins, Cristilyn N., Jenkins, Jon M., Latham, David W., Ricker, George, Seager, Sara, Vanderspek, Roland, Winn, Joshua N., Charbonneau, David, Essack, Zahra, Rodriguez, David R., Shporer, Avi, Twicken, Joseph D., Villaseñor, Jesus Noel
Publikováno v:
Nature 635, 574-577 (2024)
Astronomers have found more than a dozen planets transiting 10-40 million year old stars, but even younger transiting planets have remained elusive. A possible reason for the lack of such discoveries is that newly formed planets are not yet in a conf
Externí odkaz:
http://arxiv.org/abs/2411.18683
Autor:
Stefansson, Gudmundur, Mahadevan, Suvrath, Winn, Joshua, Marcussen, Marcus, Kanodia, Shubham, Albrecht, Simon, Fitzmaurice, Evan, Mikulskitye, One, Cañas, Caleb, Espinoza-Retamal, Juan Ignacio, Zwart, Yiri, Krolikowski, Daniel, Hotnisky, Andrew, Robertson, Paul, Alvarado-Montes, Jaime A., Bender, Chad, Blake, Cullen, Callingham, Joe, Cochran, William, Delamer, Megan, Diddams, Scott, Dong, Jiayin, Fernandes, Rachel, Giovanazzi, Mark, Halverson, Samuel, Libby-Roberts, Jessica, Logsdon, Sarah E, McElwain, Michael, Ninan, Joe, Rajagopal, Jayadev, Reji, Varghese, Roy, Arpita, Schwab, Christian, Wright, Jason
Gaia astrometry of nearby stars is precise enough to detect the tiny displacements induced by substellar companions, but radial velocity data are needed for definitive confirmation. Here we present radial velocity follow-up observations of 28 M and K
Externí odkaz:
http://arxiv.org/abs/2410.05654
Publikováno v:
J. Mol. Liquids 318 (2020) 114265
The solid-liquid equilibria and excess enthalpies of the binary systems of propiophenone and {N-methylformamide, or N,N-dimethylformamide, or N,N-dimethylacetamide, or N-methyl-2-pyrrolidone} were measured. The SLE datawere determined by the cloud-po
Externí odkaz:
http://arxiv.org/abs/2409.13277
Publikováno v:
J. Mol. Liquids 296 (2019) 112058
Solid-liquid equilibria for the binary systems of acetophenone and {N-methylformamide, or N,Ndimethylformamide, or N,N-dimethylacetamide, or N-methyl-2-pyrrolidone} were determined by the cloudpoint and DSC techniques. For the same systems, excess en
Externí odkaz:
http://arxiv.org/abs/2409.12768
Autor:
Gupta, Arvind F., Luhn, Jacob K., Wright, Jason T., Mahadevan, Suvrath, Robertson, Paul, Krolikowski, Daniel M., Ford, Eric B., Cañas, Caleb I., Halverson, Samuel, Lin, Andrea S. J., Kanodia, Shubham, Fitzmaurice, Evan, Gilbertson, Christian, Bender, Chad F., Blake, Cullen H., Dong, Jiayin, Giovinazzi, Mark R., Logsdon, Sarah E., Monson, Andrew, Ninan, Joe P., Rajagopal, Jayadev, Roy, Arpita, Schwab, Christian, Stefánsson, Guðmundur
With close to three years of observations in hand, the NEID Earth Twin Survey (NETS) is starting to unearth new astrophysical signals for a curated sample of bright, radial velocity (RV)-quiet stars. We present the discovery of the first NETS exoplan
Externí odkaz:
http://arxiv.org/abs/2409.12315
Young associations record complete histories of star forming events through their demographics and dynamics, and Gaia has greatly expanded our knowledge of these associations. We present the first structural and dynamical overview study of the Cep-He
Externí odkaz:
http://arxiv.org/abs/2406.19530
Autor:
Alshahwan, Nadia, Blasi, Arianna, Bojarczuk, Kinga, Ciancone, Andrea, Gucevska, Natalija, Harman, Mark, Schellaert, Simon, Harper, Inna, Jia, Yue, Królikowski, Michał, Lewis, Will, Martac, Dragos, Rojas, Rubmary, Ustiuzhanina, Kate
This paper reports the results of the deployment of Rich-State Simulated Populations at Meta for both automated and manual testing. We use simulated users (aka test users) to mimic user interactions and acquire state in much the same way that real us
Externí odkaz:
http://arxiv.org/abs/2403.15374
Autor:
Krolikowski, Daniel M., Kraus, Adam L., Tofflemire, Benjamin M., Morley, Caroline V., Mann, Andrew W., Vanderburg, Andrew
Young exoplanets trace planetary evolution, particularly the atmospheric mass loss that is most dynamic in youth. However, the high activity level of young stars can mask or mimic the spectroscopic signals of atmospheric mass loss. This includes the
Externí odkaz:
http://arxiv.org/abs/2311.04971