Zobrazeno 1 - 10
of 202
pro vyhledávání: '"Molenda-Żakowicz J."'
Autor:
Frasca, A., Molenda-Zakowicz, J., Alonso-Santiago, J., Catanzaro, G., De Cat, P., Fu, J. N., Zong, W., Wang, J. X., Cang, T., Wang, J. T.
Publikováno v:
A&A 664, A78 (2022)
In this work we present the results of our analysis of 16,300 medium-resolution LAMOST spectra of late-type stars in the Kepler field with the aim of determining the stellar parameters, activity level, lithium atmospheric content, and binarity. We ha
Externí odkaz:
http://arxiv.org/abs/2205.04757
Autor:
De Cat P., Fu J.N., Yang X.H., Ren A.B., Frasca A., Molenda-Żakowicz J., Catanzaro G., Gray R.O., Corbally C.J., Shi J.R., Zhang H.T., Luo A.L.
Publikováno v:
EPJ Web of Conferences, Vol 101, p 01011 (2015)
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) at the Xinglong observatory in China is a new 4-m telescope equipped with 4,000 optical fibers. In 2010, we initiated the LAMOST-Kepler project. We requested to observe the full f
Externí odkaz:
https://doaj.org/article/c1b9de63081d4e379e49c4e7176f3276
Autor:
Wang, Jiangtao, Fu, Jian-Ning, Zong, Weikai, Smith, M. C., De Cat, Peter, Shi, Jianrong, Luo, Ali, Zhang, Haotong, Frasca, A., Corbally, C. J., Molenda-Żakowicz, J., Catanzaro, G., Gray, R. O., Wang, Jiaxin, Pan, Yang
The LAMOST-\textit{K}2 (L\textit{K}2) project, initiated in 2015, aims to collect low-resolution spectra of targets in the \textit{K}2 campaigns, similar to LAMOST-\textit{Kepler} project. By the end of 2018, a total of 126 L\textit{K}2 plates had be
Externí odkaz:
http://arxiv.org/abs/2010.06827
Autor:
Fu, J. N., De Cat, P., Zong, W., Frasca, A., Gray, R. O., Ren, A. B., Molenda-Żakowicz, J., Corbally, C. J., Catanzaro, G., Shi, J. R., Luo, A. L., Zhang, H. T.
The NASA $Kepler$ mission obtained long-term high-quality photometric observations for a large number of stars in its original field of view from 2009 to 2013. In order to provide reliable stellar parameters in a homogeneous way, the LAMOST telescope
Externí odkaz:
http://arxiv.org/abs/2008.10776
Autor:
Pigulski, A., Baran, A., Bzowski, M., Cugier, H., Czerny, B., Daszynska-Daszkiewicz, J., Dziembowski, W., Handler, G., Kolaczkowski, Z., Krolikowska, M., Krzesinski, J., Maciejewski, G., Michalska, G., Molenda-Zakowicz, J., Moskalik, P., Niedzielski, A., Niemczura, E., Ostrowski, J., Pamyatnykh, A., Ratajczak, M., Rucinski, S., Siwak, M., Smolec, R., Szutowicz, S., Tomov, T., Wyrzykowski, L., Zola, S., Sarna, M.
Time-series photometry from space in the ultraviolet can be presently done with only a few platforms, none of which is able to provide wide-field long-term high-cadence photometry. We present a concept of UVSat, a twin space telescope which will be c
Externí odkaz:
http://arxiv.org/abs/1711.10366
Autor:
Aliçavuş, F. Kahraman, Niemczura, E., Polińska, M., Hełminiak, K. G., Lampens, P., Molenda-Żakowicz, J., Ukita, N., Kambe, E.
$\delta$ Scuti stars are remarkable objects for asteroseismology. In spite of decades of investigations, there are still important questions about these pulsating stars to be answered, such as their positions in $\log$$T_{\rm eff}$ $-$ $\log g$ diagr
Externí odkaz:
http://arxiv.org/abs/1706.04782
Autor:
Guzik, J. A., Houdek, G., Chaplin, W. J., Smalley, B., Kurtz, D. W., Gilliland, R. L., Mullally, F., Rowe, J. F., Bryson, S. T., Still, M. D., Antoci, V., Appourchaux, T., Basu, S., Bedding, T. R., Benomar, O., Garcia, R. A., Huber, D., Kjeldsen, H., Latham, D. W., Metcalfe, T. S., Pápics, P. I., White, T. R., Aerts, C., Ballot, J., Boyajian, T. S., Briquet, M., Bruntt, H., Buchhave, L. A., Campante, T. L., Catanzaro, G., Christensen-Dalsgaard, J., Davies, G. R., Doğan, G., Dragomir, D., Doyle, A. P., Elsworth, Y., Frasca, A., Gaulme, P., Gruberbauer, M., Handberg, R., Hekker, S., Karoff, C., Lehmann, H., Mathias, P., Mathur, S., Miglio, A., Molenda-Żakowicz, J., Mosser, B., Murphy, S. J., Régulo, C., Ripepi, V., Salabert, D., Sousa, S. G., Stello, D., Uytterhoeven, K.
$\theta$ Cygni is an F3 spectral-type main-sequence star with visual magnitude V=4.48. This star was the brightest star observed by the original Kepler spacecraft mission. Short-cadence (58.8 s) photometric data using a custom aperture were obtained
Externí odkaz:
http://arxiv.org/abs/1607.01035
Autor:
Frasca, A., Molenda-Zakowicz, J., De Cat, P., Catanzaro, G., Fu, J. N., Ren, A. B., Luo, A. L., Shi, J. R., Wu, Y., Zhang, H. T.
Publikováno v:
A&A 594, A39 (2016)
The LAMOST-Kepler survey, whose spectra are analyzed in the present paper, is the first large spectroscopic project aimed at characterizing these sources. Our work is focused at selecting emission-line objects and chromospherically active stars and o
Externí odkaz:
http://arxiv.org/abs/1606.09149
Autor:
De Cat, P., Fu, J. N., Ren, A. B., Yang, X. H., Shi, J. R., Luo, A. L., Yang, M., Wang, J. L., Zhang, H. T., Shi, H. M., Zhang, W., Dong, Subo, Catanzaro, G., Corbally, C. J., Frasca, A., Gray, R. O., Molenda-Zakowicz, J., Uytterhoeven, K., Briquet, M., Bruntt, H., Frandsen, S., Kiss, L., Kurtz, D. W., Marconi, M., Niemczura, E., Oestensen, R. H., Ripepi, V., Smalley, B., Southworth, J., Szabo, R., Telting, J. H., Karoff, C., Aguirre, V. Silva, Wu, Y., Hou, Y. H., Jin, G., Zhou, X. L.
The nearly continuous light curves with micromagnitude precision provided by the space mission Kepler are revolutionising our view of pulsating stars. They have revealed a vast sea of low-amplitude pulsation modes that were undetectable from Earth. T
Externí odkaz:
http://arxiv.org/abs/1508.06391
Autor:
Jerzykiewicz, M., Handler, G., Daszynska-Daszkiewicz, J., Pigulski, A., Poretti, E., Rodriguez, E., Amado, P. J., Kolaczkowski, Z., Uytterhoeven, K., Dorokhova, T. N., Dorokhov, N. I., Lorenz, D., Zsuffa, D., Kim, S. -L., Bourge, P. -O., Acke, B., De Ridder, J., Verhoelst, T., Drummond, R., Movchan, A. I., Lee, J. -A., Steslicki, M., Molenda-Zakowicz, J., Garrido, R., Kim, S. -H., Michalska, G., Paparo, M., Antoci, V., Aerts, C.
A multisite photometric campaign for the Beta Cephei and eclipsing variable 16 Lacertae is reported. 749 h of high-quality differential photoelectric Stromgren, Johnson and Geneva time-series photometry were obtained with ten telescopes during 185 ni
Externí odkaz:
http://arxiv.org/abs/1508.05250