Zobrazeno 1 - 10
of 2 796
pro vyhledávání: '"Potter S."'
Autor:
Pelgrims, V., Mandarakas, N., Skalidis, R., Tassis, K., Panopoulou, G. V., Pavlidou, V., Blinov, D., Kiehlmann, S., Clark, S. E., Hensley, B. S., Romanopoulos, S., Basyrov, A., Eriksen, H. K., Falalaki, M., Ghosh, T., Gjerløw, E., Kypriotakis, J. A., Maharana, S., Papadaki, A., Pearson, T. J., Potter, S. B., Ramaprakash, A. N., Readhead, A. C. S., Wehus, I. K.
We present the first degree-scale tomography map of the dusty magnetized interstellar medium (ISM) from stellar polarimetry and distance measurements. We used the RoboPol polarimeter at Skinakas Observatory to conduct a survey of starlight polarizati
Externí odkaz:
http://arxiv.org/abs/2404.10821
Autor:
Mandarakas, N., Panopoulou, G. V., Pelgrims, V., Potter, S. B., Pavlidou, V., Ramaprakash, A., Tassis, K., Blinov, D., Kiehlmann, S., Koutsiona, E., Maharana, S., Romanopoulos, S., Skalidis, R., Vervelaki, A., Clark, S. E., Kypriotakis, J. A., Readhead, A. C. S.
Context. Calibration of optical polarimeters relies on the use of stars with negligible polarization (unpolarized standard stars) for determining the instrumental polarization zero-point. For wide-field polarimeters, calibration is often done by imag
Externí odkaz:
http://arxiv.org/abs/2312.06435
Autor:
Liodakis, I., Shablovinskaya, E., Blinov, D., Savchenko, S. S., Malygin, E., Kotov, S., Kiehlmann, S., Readhead, A. C. S., Potter, S. B., Rieger, F. M., Grishina, T. S., Hagen-Thorn, V. A., Kopatskaya, E. N., Larionova, E. G., Morozova, D. A., Troitskiy, I. S., Troitskaya, Y. V., Vasilyev, A. A., Zhovtan, A. V., Borman, G. A.
Optical circular polarization observations can directly test the particle composition in black holes jets. Here we report on the first observations of the BL Lac type object S4 0954+65 in high linear polarized states. While no circular polarization w
Externí odkaz:
http://arxiv.org/abs/2311.03450
Autor:
Pradeep, Kala G., Singh, Kulinder Pal, Dewangan, G. C., Aydi, Elias, Barrett, P. E., Buckley, D. A. H., Girish, V., Page, K. L., Potter, S. B., Schlegel, E. M.
We present multi-wavelength temporal and spectral characteristics of a magnetic cataclysmic variable (MCV) Swift J0503.7-2819, using far ultraviolet (FUV) and X-ray data from AstroSat, supplemented with optical data from the Southern African Large Te
Externí odkaz:
http://arxiv.org/abs/2310.07293
Autor:
O'Connor, B., Gogus, E., Hare, J., Mukai, K., Huppenkothen, D., Brink, J., Buckley, D. A. H., Levan, A., Baring, M. G., Stewart, R., Kouveliotou, C., Woudt, P., Bellm, E., Cenko, S. B., Evans, P. A., Granot, J., Hailey, C., Harrison, F., Hartmann, D., van der Horst, A. J., Kaper, L., Kennea, J. A., Potter, S. B., Slane, P. O., Stern, D., Wijers, R. A. M. J., Younes, G.
Here, we present the results of our multi-wavelength campaign aimed at classifying \textit{Swift} J170800$-$402551.8 as part of the \textit{Swift} Deep Galactic Plane Survey (DGPS). We utilized Target of Opportunity (ToO) observations with \textit{Sw
Externí odkaz:
http://arxiv.org/abs/2307.13959
Autor:
Blinov, D., Maharana, S., Bouzelou, F., Casadio, C., Gjerløw, E., Jormanainen, J., Kiehlmann, S., Kypriotakis, J. A., Liodakis, I., Mandarakas, N., Markopoulioti, L., Panopoulou, G. V., Pelgrims, V., Pouliasi, A., Romanopoulos, S., Skalidis, R., Anche, R. M., Angelakis, E., Antoniadis, J., Medhi, B. J., Hovatta, T., Kus, A., Kylafis, N., Mahabal, A., Myserlis, I., Paleologou, E., Papadakis, I., Pavlidou, V., Papamastorakis, I., Pearson, T. J., Potter, S. B., Ramaprakash, A. N., Readhead, A. C. S., Reig, P., Słowikowska, A., Tassis, K., Zensus, J. A.
Publikováno v:
A&A 677, A144 (2023)
Optical polarimeters are typically calibrated using measurements of stars with known and stable polarization parameters. However, there is a lack of such stars available across the sky. Many of the currently available standards are not suitable for m
Externí odkaz:
http://arxiv.org/abs/2307.06151
Autor:
O'Connor, B., Brink, J., Buckley, D. A. H., Mukai, K., Kouveliotou, C., Gogus, E., Potter, S. B., Woudt, P., Lien, A., Levan, A., Kargaltsev, O., Baring, M. G., Bellm, E., Cenko, S. B., Evans, P. A., Granot, J., Hailey, C., Harrison, F., Hartmann, D., van der Horst, A. J., Huppenkothen, D., Kaper, L., Kennea, J. A., Slane, P. O., Stern, D., Troja, E., Wijers, R. A. M. J., Younes, G.
We present the results of our X-ray, ultraviolet, and optical follow-up campaigns of 1RXS J165424.6-433758, an X-ray source detected with the \textit{Swift} Deep Galactic Plane Survey (DGPS). The source X-ray spectrum (\textit{Swift} and \textit{NuST
Externí odkaz:
http://arxiv.org/abs/2306.05576
Autor:
Maharana, S., Kiehlmann, S., Blinov, D., Pelgrims, V., Pavlidou, V., Tassis, K., Kypriotakis, J. A., Ramaprakash, A. N., Anche, R. M., Basyrov, A., Deka, K., Eriksen, H. K., Ghosh, T., Gjerløw, E., Mandarakas, N., Ntormousi, E., Panopoulou, G. V., Papadaki, A., Pearson, T., Potter, S. B., Readhead, A. C. S., Skalidis, R., Wehus, I. K.
Publikováno v:
A&A 679, A68 (2023)
Next-generation wide-field optical polarimeters like the Wide-Area Linear Optical Polarimeters (WALOPs) have a field of view (FoV) of tens of arcminutes. For efficient and accurate calibration of these instruments, wide-field polarimetric flat source
Externí odkaz:
http://arxiv.org/abs/2305.04270
Autor:
Pelgrims, V., Panopoulou, G. V., Tassis, K., Pavlidou, V., Basyrov, A., Blinov, D., Gjerløw, E., Kiehlmann, S., Mandarakas, N., Papadaki, A., Skalidis, R., Tsouros, A., Anche, R. M., Eriksen, H. K., Ghosh, T., Kypriotakis, J. A., Maharana, S., Ntormousi, E., Pearson, T. J., Potter, S. B., Ramaprakash, A. N., Readhead, A. C. S., Wehus, I. K.
Publikováno v:
A&A 670, A164 (2023)
We present the first Bayesian method for tomographic decomposition of the plane-of-sky orientation of the magnetic field with the use of stellar polarimetry and distance. This standalone tomographic inversion method presents an important step forward
Externí odkaz:
http://arxiv.org/abs/2208.02278
Publikováno v:
In JPRAS Open September 2024 41:203-214