Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Lurie, John"'
Autor:
Lurie, John C., Vyhmeister, Karl, Hawley, Suzanne L., Adilia, Jamel, Chen, Andrea, Davenport, James R. A., Juric, Mario, Puig-Holzman, Michael, Weisenburger, Kolby L.
Few observational constraints exist for the tidal synchronization rate of late-type stars, despite its fundamental role in binary evolution. We visually inspected the light curves of 2278 eclipsing binaries (EBs) from the Kepler Eclipsing Binary Cata
Externí odkaz:
http://arxiv.org/abs/1710.07339
Autor:
Winters, Jennifer G., Sevrinsky, R. Andrew, Jao, Wei-Chun, Henry, Todd J., Riedel, Adric R., Subasavage, John P., Lurie, John C., Ianna, Philip A.
We present 160 new trigonometric parallaxes for 151 M dwarf systems from the REsearch Consortium On Nearby Stars (RECONS) group's long-term astrometry/photometry program at the CTIO/SMARTS 0.9m telescope. Most systems (124 or 82%) are found to lie wi
Externí odkaz:
http://arxiv.org/abs/1610.07552
Autor:
Kizhakkeveettil, Anupama, Bezdjian, Serena, Hurwitz, Eric L., Toler, Andrew W.J., Rossi, Daniel, Uptmor, Sarah, Sagester, Kayla, Bangash, Maria, MacKenzie, Todd A., Lurie, John D., Coulter, Ian, Haldeman, Scott, Whedon, James M.
Publikováno v:
In Journal of Manipulative and Physiological Therapeutics October 2021 44(8):663-673
Autor:
Jurić, Mario, Kantor, Jeffrey, Lim, K-T, Lupton, Robert H., Dubois-Felsmann, Gregory, Jenness, Tim, Axelrod, Tim S., Aleksić, Jovan, Allsman, Roberta A., AlSayyad, Yusra, Alt, Jason, Armstrong, Robert, Basney, Jim, Becker, Andrew C., Becla, Jacek, Bickerton, Steven J., Biswas, Rahul, Bosch, James, Boutigny, Dominique, Kind, Matias Carrasco, Ciardi, David R., Connolly, Andrew J., Daniel, Scott F., Daues, Gregory E., Economou, Frossie, Chiang, Hsin-Fang, Fausti, Angelo, Fisher-Levine, Merlin, Freemon, D. Michael, Gee, Perry, Gris, Philippe, Hernandez, Fabio, Hoblitt, Joshua, Ivezić, Željko, Jammes, Fabrice, Jevremović, Darko, Jones, R. Lynne, Kalmbach, J. Bryce, Kasliwal, Vishal P., Krughoff, K. Simon, Lang, Dustin, Lurie, John, Lust, Nate B., Mullally, Fergal, MacArthur, Lauren A., Melchior, Peter, Moeyens, Joachim, Nidever, David L., Owen, Russell, Parejko, John K, Peterson, J. Matt, Petravick, Donald, Pietrowicz, Stephen R., Price, Paul A., Reiss, David J., Shaw, Richard A., Sick, Jonathan, Slater, Colin T., Strauss, Michael A., Sullivan, Ian S., Swinbank, John D., Van Dyk, Schuyler, Vujčić, Veljko, Withers, Alexander, Yoachim, Peter
The Large Synoptic Survey Telescope (LSST) is a large-aperture, wide-field, ground-based survey system that will image the sky in six optical bands from 320 to 1050 nm, uniformly covering approximately $18,000$deg$^2$ of the sky over 800 times. The L
Externí odkaz:
http://arxiv.org/abs/1512.07914
Autor:
Hosey, Altonio D., Henry, Todd J., Jao, Wei-Chun, Dieterich, Sergio B., Winters, Jennifer G., Lurie, John C., Riedel, Adric R., Subasavage, John P.
We present an analysis of long-term photometric variability for nearby red dwarfs at optical wavelengths. The sample consists of 264 M dwarfs south of DEC = +30 with V-K = 3.96-9.16 and Mv~10-20 (spectral types M2V-M8V), most of which are within 25 p
Externí odkaz:
http://arxiv.org/abs/1503.02100
Autor:
Lurie, John C., Davenport, James R. A., Hawley, Suzanne L., Wilkinson, Tessa D., Wisniewski, John P., Kowalski, Adam F., Hebb, Leslie
We present the flare occurrence rates and starspot evolution for GJ 1245 A and B, two active M5 stars, based on nine months of Kepler short cadence observations, and four years of nearly continuous long cadence observations. The A component is separa
Externí odkaz:
http://arxiv.org/abs/1412.6109
Autor:
Winters, Jennifer G., Henry, Todd J., Lurie, John C., Hambly, Nigel C., Jao, Wei-Chun, Bartlett, Jennifer L., Boyd, Mark R., Dieterich, Sergio B., Finch, Charlie T., Hosey, Altonio D., Ianna, Philip A., Riedel, Adric R., Slatten, Kenneth J., Subasavage, John P.
We present trigonometric, photometric, and photographic distances to 1748 southern ($\delta \leq$0$^\circ$) M dwarf systems with $\mu \ge$ 0\farcs18 yr$^{-1}$, of which 1404 are believed to lie within 25 parsecs of the Sun. The stars have 6.67 $\leq$
Externí odkaz:
http://arxiv.org/abs/1407.7837
Autor:
Lurie, John C., Henry, Todd J., Jao, Wei-Chun, Quinn, Samuel N., Winters, Jennifer G., Ianna, Philip A., Koerner, David W., Riedel, Adric R., Subasavage, John P.
Astrometric measurements are presented for seven nearby stars with previously detected planets: six M dwarfs (GJ 317, GJ 667C, GJ 581, GJ 849, GJ 876, and GJ 1214) and one K dwarf (BD $-$10 3166). Measurements are also presented for six additional ne
Externí odkaz:
http://arxiv.org/abs/1407.4820
Autor:
Mamajek, Eric E., Bartlett, Jennifer L., Seifahrt, Andreas, Henry, Todd J., Dieterich, Sergio B., Lurie, John C., Kenworthy, Matthew A., Jao, Wei-Chun, Riedel, Adric R., Subasavage, John P., Winters, Jennifer G., Finch, Charlie T., Ianna, Philip A., Bean, Jacob
LP 876-10 is a nearby active M4 dwarf in Aquarius at a distance of 7.6 pc. The star is a new addition to the 10-pc census, with a parallax measured via the Research Consortium on Nearby Stars (RECONS) astrometric survey on the Small & Moderate Apertu
Externí odkaz:
http://arxiv.org/abs/1310.0764