Zobrazeno 1 - 10
of 175
pro vyhledávání: '"Poshyachinda S"'
Autor:
Steeghs, D., Galloway, D. K., Ackley, K., Dyer, M. J., Lyman, J., Ulaczyk, K., Cutter, R., Mong, Y. L., Dhillon, V., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Nuttall, L. K., Palle, E., Breton, R. P., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkila, T., Irawati, P., Kennedy, M. R., Killestein, T., Kuncarayakti, H., Levan, A. J., Littlefair, S., Makrygianni, L., Marsh, T., Mata-Sanchez, D., Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Mullaney, J., Noysena, K., Patel, M., Rol, E., Sawangwit, U., Stanway, E. R., Starling, R., Strom, P., Tooke, S., West, R., White, D. J., Wiersema, K.
The Gravitational-wave Optical Transient Observer (GOTO) is an array of wide-field optical telescopes, designed to exploit new discoveries from the next generation of gravitational wave detectors (LIGO, Virgo, KAGRA), study rapidly evolving transient
Externí odkaz:
http://arxiv.org/abs/2110.05539
Autor:
Rattanamala, R., Awiphan, S., Komonjinda, S., Phriksee, A., Sappankum, P., A-thano, N., Chitchak, S., Rittipruk, P., Sawangwit, U., Poshyachinda, S., Reichart, D. E., Haislip, J. B.
We present the binary model and the eclipse timing variations of the eclipsing binary RR Cae, which consists of a white dwarf eclipsed by an M-type dwarf companion. The multi-wavelength optical photometry from the Transiting Exoplanet Survey Satellit
Externí odkaz:
http://arxiv.org/abs/2109.09397
In this study, all unpublished time series photometric data of BM UMa ($q \sim$ 2.0, P = 0.2712\,d) from available archives were re-investigated together with new data taken from the TNT-2.4m of the Thai National Observatory (TNO). Based on period an
Externí odkaz:
http://arxiv.org/abs/2108.13615
Autor:
Makrygianni, L., Mullaney, J., Dhillon, V., Littlefair, S., Ackley, K., Dyer, M. J., Lyman, J., Ulaczyk, K., Cutter, R., Mong, Y. -L., Steeghs, D., Galloway, D. K., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Nuttall, L., Pallé, E., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Breton, R., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkilä, T., Irawati, P., Kennedy, M., Killestein, T., Levan, A., Marsh, T., Mata-Sanchez, D., Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Strøm, P. A., Tooke, S., Wiersema, K.
We have adapted the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Science Pipelines to process data from the Gravitational-Wave Optical Transient Observer (GOTO) prototype. In this paper, we describe how we used the Rubin Observato
Externí odkaz:
http://arxiv.org/abs/2105.05128
Autor:
Hayes, J. J. C., Priyadarshi, A., Kerins, E., Awiphan, S., McDonald, I., A-thano, N., Morgan, J. S., Humpage, A., Charles, S., Wright, M., Joshi, Y. C., Jiang, Ing-Guey, Inyanya, T., Padjaroen, T., Munsaket, P., Chuanraksasat, P., Komonjinda, S., Kittara, P., Dhillon, V. S., Marsh, T. R., Reichart, D. E., Poshyachinda, S.
We present TransitFit, a package designed to fit exoplanetary transit light-curves. TransitFit offers multi-epoch, multi-wavelength fitting of multi-telescope transit data. TransitFit allows per-telescope detrending to be performed simultaneously wit
Externí odkaz:
http://arxiv.org/abs/2103.12139
Autor:
Alagao, M. A., Kawinkij, A., Buisset, C., Prasit, A., Lépine, T., Rabbia, Y., Berdeu, A., Thiébaut, É., Langlois, M., Tallon, M., Awiphan, S., Semenko, E., Rittipruk, P., Mkrtichian, D., Leckngam, A., Thuammasorn, G., Kaewsamoeta, P., Inpan, A., Kuha, T., Laoyang, A., Somboonchai, W., Kanthum, S., Poshyachinda, S., Soonthornthum, B.
The evanescent wave coronagraph uses the principle of frustrated total internal reflection (FTIR) to suppress the light coming from the star and study its close environment. Its focal plane mask is composed of a lens and a prism placed in contact wit
Externí odkaz:
http://arxiv.org/abs/2103.10044
Autor:
Killestein, T. L., Lyman, J., Steeghs, D., Ackley, K., Dyer, M. J., Ulaczyk, K., Cutter, R., Mong, Y. -L., Galloway, D. K., Dhillon, V., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Breton, R. P., Nuttall, L. K., Pallé, E., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkilä, T., Irawati, P., Kennedy, M. R., Levan, A., Littlefair, S., Makrygianni, L., Sánchez, D. Mata, Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Mullaney, J., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Strøm, P. A., Tooke, S., Wiersema, K., Williams, S. C.
Large-scale sky surveys have played a transformative role in our understanding of astrophysical transients, only made possible by increasingly powerful machine learning-based filtering to accurately sift through the vast quantities of incoming data g
Externí odkaz:
http://arxiv.org/abs/2102.09892
Autor:
Chote, P., Gaensicke, B. T., McCormac, J., Aungwerojwit, A., Bayliss, D., Burleigh, M. R., Casewell, S. L., Eigmueller, Ph., Gill, S., Goad, M. R., Hermes, J. J., Jenkins, J. S., Mukadam, A. S., Poshyachinda, S., Raynard, L., Reichart, D. E., Szkody, P., Toloza, O., West, R. G., Wheatley, P. J.
Light curves of the accreting white dwarf pulsator GW Librae spanning a 7.5 month period in 2017 were obtained as part of the Next Generation Transit Survey. This data set comprises 787 hours of photometry from 148 clear nights, allowing the behaviou
Externí odkaz:
http://arxiv.org/abs/2101.08786
Autor:
Zheltobryukhov, M., Zubko, E., Chornaya, E., Luk'yanyk, I., Ivanova, O., Kochergin, A., Kornienko, G., Mkrtichian, D., Poshyachinda, S., Molotov, I. E., Kim, S. S., Videen, G.
We measure the degree of linear polarization of comet 46P/Wirtanen during two months, embracing the perihelion passage in 2018 December with phase angles ranging from {\alpha}=18.1 to 46.4 deg. The polarimetric response PQ obtained resembles what was
Externí odkaz:
http://arxiv.org/abs/2012.12781
Autor:
Mullaney, J. R., Makrygianni, L., Dhillon, V., Littlefair, S., Ackley, K., Dyer, M., Lyman, J., Ulaczyk, K., Cutter, R., Mong, Y. L., Steeghs, D., Galloway, D. K., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Nuttall, L., Pallé, E., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Breton, R., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkilä, T., Irawati, P., Kennedy, M., Killestein, T., Levan, A., Marsh, T., Mata-Sanchez, D., Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Tooke, S., Wiersema, K.
The past few decades have seen the burgeoning of wide field, high cadence surveys, the most formidable of which will be the Legacy Survey of Space and Time (LSST) to be conducted by the Vera C. Rubin Observatory. So new is the field of systematic tim
Externí odkaz:
http://arxiv.org/abs/2010.15142