Zobrazeno 1 - 10
of 1 287
pro vyhledávání: '"Hogg, D."'
Analyses of quasi-periodic oscillations (QPOs) are important to understanding the dynamic behaviour in many astrophysical objects during transient events like gamma-ray bursts, solar flares, magnetar flares and fast radio bursts. Astrophysicists ofte
Externí odkaz:
http://arxiv.org/abs/2205.12716
Autor:
Specht, D., Poleski, R., Penny, M. T., Kerins, E., McDonald, I., Lee, Chung-Uk, Udalski, A., Bond, I. A., Shvartzvald, Y., Zang, Weicheng, Street, R. A., Hogg, D. W., Gaudi, B. S., Barclay, T., Barentsen, G., Howell, S. B., Mullally, F., Henderson, C. B., Bryson, S. T., Caldwell, D. A., Haas, M. R., Van Cleve, J. E., Larson, K., McCalmont, K., Peterson, C., Putnam, D., Ross, S., Packard, M., Reedy, L., Albrow, Michael D., Chung, Sun-Ju, Jung, Youn Kil, Gould, Andrew, Han, Cheongho, Hwang, Kyu-Ha, Ryu, Yoon-Hyun, Shin, In-Gu, Yang, Hongjing, Yee, Jennifer C., Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Szymański, M. K., Soszyński, I., Ulaczyk, K., Pietrukowicz, P., Kozlowski, Sz., Skowron, J., Mróz, P., Mao, Shude, Fouqué, Pascal, Zhu, Wei, Abe, F., Barry, R., Bennett, D. P., Bhattacharya, A., Fukui, A., Fujii, H., Hirao, Y., Itow, Y., Kirikawa, R., Kondo, I., Koshimoto, N., Matsubara, Y., Matsumoto, S., Miyazaki, S., Muraki, Y., Olmschenk, G., Ranc, C., Okamura, A., Rattenbury, N. J., Satoh, Y., Sumi, T., Suzuki, D., Silva, S. I., Toda, T., Tristram, P. J., Vandorou, A., Yama, H., Beichman, C., Bryden, G., Novati, S. Calchi
We present K2-2016-BLG-0005Lb, a densely sampled, planetary binary caustic-crossing microlensing event found from a blind search of data gathered from Campaign 9 of the Kepler K2 mission (K2C9). K2-2016-BLG-0005Lb is the first bound microlensing exop
Externí odkaz:
http://arxiv.org/abs/2203.16959
Publikováno v:
A&A 646, A24 (2021)
High-contrast imaging surveys for exoplanet detection have shown giant planets at large separations to be rare. It is important to push towards detections at smaller separations, the part of the parameter space containing most planets. The performanc
Externí odkaz:
http://arxiv.org/abs/2011.12311
Excalibur: A Non-Parametric, Hierarchical Wavelength-Calibration Method for a Precision Spectrograph
Excalibur is a non-parametric, hierarchical framework for precision wavelength-calibration of spectrographs. It is designed with the needs of extreme-precision radial velocity (EPRV) in mind, which require that instruments be calibrated or stabilized
Externí odkaz:
http://arxiv.org/abs/2010.13786
Autor:
Minchev, I., Matijevic, G., Hogg, D. W., Guiglion, G., Steinmetz, M., Anders, F., Chiappini, C., Martig, M., Queiroz, A., Scannapieco, C.
Simpson's paradox, or Yule-Simpson effect, arises when a trend appears in different subsets of data but disappears or reverses when these subsets are combined. We describe here seven cases of this phenomenon for chemo-kinematical relations believed t
Externí odkaz:
http://arxiv.org/abs/1902.01421
Observational tests of stellar and Galactic chemical evolution call for the joint knowledge of a star's physical parameters, detailed element abundances, and precise age. For cool main-sequence (MS) stars the abundances of many elements can be measur
Externí odkaz:
http://arxiv.org/abs/1802.06663
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2017, Volume 466, Issue 2, p.2364-2377
Among the population of known galactic black hole X-ray binaries, GRS 1915+105 stands out in multiple ways. It has been in continuous outburst since 1992, and has shown a wide range of different states that can be distinguished by their timing and sp
Externí odkaz:
http://arxiv.org/abs/1611.01332
We present an algorithm capable of detecting diffuse, dim sources of any size in an astronomical image. These sources often defeat traditional methods for source finding, which expand regions around points of high intensity. Extended sources often ha
Externí odkaz:
http://arxiv.org/abs/1601.00266
Autor:
Küpper, A. H. W., Balbinot, E., Bonaca, A., Johnston, K. V., Hogg, D. W., Kroupa, P., Santiago, B. X.
Tidal streams of globular clusters are ideal tracers of the Galactic gravitational potential. Compared to the few known, complex and diffuse dwarf-galaxy streams, they are kinematically cold, have thin morphologies and are abundant in the halo of the
Externí odkaz:
http://arxiv.org/abs/1509.09304