Zobrazeno 1 - 10
of 596
pro vyhledávání: '"Smith, Krista"'
Autor:
van Belle, Gerard T., Ciardi, David, Hillsberry, Daniel, Jorgensen, Anders, Monnier, John, Smith, Krista Lynne, Boyajian, Tabetha, Carpenter, Kenneth, Clark, Catherine, Rau, Gioia, Schaefer, Gail
Publikováno v:
Proc. SPIE 13092-101 July 2024
MoonLITE (Lunar InTerferometry Explorer) is an Astrophysics Pioneers proposal to develop, build, fly, and operate the first separated-aperture optical interferometer in space, delivering sub-mas science results. MoonLITE will leverage the Pioneers op
Externí odkaz:
http://arxiv.org/abs/2408.01392
Autor:
Smith, Krista L.
Publikováno v:
Symmetry 2024, 16(7), 898
This review focuses on diffractive physics, which involves the long-range interactions of the strong nuclear force at high energies described by SU(3) gauge symmetry. It is expected that diffractive processes account for nearly 40% of the total cross
Externí odkaz:
http://arxiv.org/abs/2407.16835
Autor:
Smith, Krista
The PHENIX experiment at RHIC has a unique large rapidity coverage ($1.2 < |y| < 2.2$) for heavy flavor studies in heavy-ion collisions. This kinematic region has a smaller particle density and may undergo different nuclear effects before and after t
Externí odkaz:
http://arxiv.org/abs/2407.02451
Autor:
Smith, Krista Lynne
Publikováno v:
Front. Astron. Space Sci., 06 June 2024 Sec. Cosmology Volume 11
Optical timing with rapid, seconds-to-minutes cadences with high photometric precision and gap-free long baselines is necessary for an unambiguous physical picture of accretion phenomena, and is only possible from space. Exoplanet-hunting missions li
Externí odkaz:
http://arxiv.org/abs/2406.15558
Autor:
Dingler, Ryne, Smith, Krista Lynne
We present a study of high-cadence, high-precision, optical light curves from the TESS satellite of 67 blazars in the southern sky. We provide descriptive flux statistics, power spectral density model parameters, and characteristic variability timesc
Externí odkaz:
http://arxiv.org/abs/2406.10346
In a previous paper, we reported evidence for quasi-periodicities in the \textsl{TESS} light curves of BL Lacerate and two other blazars found serendipitously in the SDSS AGN catalog. In this work, we find tentative evidence for quasi-periodic featur
Externí odkaz:
http://arxiv.org/abs/2402.04352
We report the time series analysis of TESS light curves of three blazars, BL Lacertae, 1RXS J111741.0+254858, and 1RXS J004519.6+212735, obtained using a customized approach for extracting AGN light curves. We find tentative evidence for quasi-period
Externí odkaz:
http://arxiv.org/abs/2312.14144
Autor:
Smith, Krista Lynne, Sartori, Lia
The sampling strategy of the Transiting Exoplanet Survey Satellite (TESS) make TESS light curves extremely valuable to investigate high cadence optical variability of AGN. However, because the TESS instrument was primarily designed for exoplanet scie
Externí odkaz:
http://arxiv.org/abs/2310.08631
Autor:
Boyle, Rebecca, Littlefield, Colin, Garnavich, Peter, Ridden-Harper, Ryan, Szkody, Paula, Boyd, Patricia, Smith, Krista Lynne
We investigate K2BS5, an optical transient that we identified in Campaign 13 of the Kepler/K2 archives by the "K2 Background Survey", and classify it as a new SU UMa-type dwarf nova. Using the light curve generated from Kepler's long-cadence observat
Externí odkaz:
http://arxiv.org/abs/2309.12396
Autor:
Kawamuro, Taiki, Ricci, Claudio, Mushotzky, Richard F., Imanishi, Masatoshi, Bauer, Franz E., Ricci, Federica, Koss, Michael J., Privon, George C., Trakhtenbrot, Benny, Izumi, Takuma, Ichikawa, Kohei, Rojas, Alejandra F., Smith, Krista Lynne, Shimizu, Taro, Oh, Kyuseok, Brok, Jakob S. den, Baba, Shunsuke, Balokovic, Mislav, Chang, Chin-Shin, Kakkad, Darshan, Pfeifle, Ryan W., Temple, Matthew J., Ueda, Yoshihiro, Harrison, Fiona, Powell, Meredith C., Stern, Daniel, Urry, Meg, Sanders, David B.
We present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby ($z <$ 0.05) active galactic nuclei (AGNs) selected from the 70-month Swift/BAT hard X-ray catalog that have precisely determined X-ray spectral properties and su
Externí odkaz:
http://arxiv.org/abs/2309.02776