Zobrazeno 1 - 10
of 10 274
pro vyhledávání: '"Lundqvist A"'
Autor:
Nilsson M, Rhedin M, Hendrickx R, Berglund S, Piras A, Blomgran P, Cavallin A, Collins M, Dahl G, Dekkak B, Ericsson T, Hagberg N, Holmberg AA, Leffler A, Lundqvist AJ, Markou T, Pinkerton J, Rönnblom L, Siu S, Taylor V, Wennberg T, Zervas D, Laurence ADJ, Mitra S, Belvisi MG, Birrell M, Borde A
Publikováno v:
Drug Design, Development and Therapy, Vol Volume 16, Pp 2901-2917 (2022)
Magnus Nilsson,1 Magdalena Rhedin,2 Ramon Hendrickx,3 Susanne Berglund,1 Antonio Piras,2 Parmis Blomgran,2 Anders Cavallin,2 Mia Collins,2 Göran Dahl,4 Bilel Dekkak,5 Therese Ericsson,3 Niklas Hagberg,6 Ann Aurell Holmberg,3 Agnes Leffler,2 Anders J
Externí odkaz:
https://doaj.org/article/da0ba90dab5643f491f29e3cf479b99c
Autor:
Kling, Filip Jonsson, Lundqvist, Samuel, Mohammadi, Fatemeh, Orth, Matthias, Sáenz-de-Cabezón, Eduardo
For the almost complete intersection ideals $(x_1^2, \dots, x_n^2, (x_1 + \cdots + x_n)^k)$, we compute their reduced Gr\"obner basis for any term ordering, revealing a combinatorial structure linked to lattice paths, elementary symmetric polynomials
Externí odkaz:
http://arxiv.org/abs/2411.10209
Autor:
Venkattu, Deepika, Lundqvist, Peter, Torres, Miguel Pérez, Bonnassieux, Etienne, Tasse, Cyril, Melchior, Anne-Laure, Combes, Francoise
We present the first LOFAR image of the centre of M31 at a frequency of 150 MHz. We clearly detect three supernova remnants, which, along with archival VLA data at 3 GHz and other published radio and X-ray data allows us to characterize them in detai
Externí odkaz:
http://arxiv.org/abs/2410.22073
[SHORTENED VERSION] Observations of radio emission from young core-collapse supernovae (CCSNe) allow one to study the history of the pre-supernova stellar wind, trace the density structure of the ejected material, and probe the magnetohydrodynamics t
Externí odkaz:
http://arxiv.org/abs/2410.07800
Autor:
Salmaso, I., Cappellaro, E., Tartaglia, L., Anderson, J. P., Benetti, S., Bronikowski, M., Cai, Y. -Z., Charalampopoulos, P., Chen, T. -W., Concepcion, E., Elias-Rosa, N., Galbany, L., Gromadzki, M., Gutiérrez, C. P., Kankare, E., Lundqvist, P., Matilainen, K., Mazzali, P. A., Moran, S., Müller-Bravo, T. E., Nicholl, M., Pastorello, A., Pessi, P. J., Pessi, T., Petrushevska, T., Pignata, G., Reguitti, A., Sollerman, J., Srivastav, S., Stritzinger, M., Tomasella, L., Valerin, G.
Massive stars experience strong mass-loss, producing a dense, H-rich circumstellar medium (CSM). After the explosion, the collision and continued interaction of the supernova (SN) ejecta with the CSM power the light curve through the conversion of ki
Externí odkaz:
http://arxiv.org/abs/2410.06111
Autor:
Reguitti, A., Dastidar, R., Pignata, G., Maeda, K., Moriya, T. J., Kuncarayakti, H., Rodríguez, Ó., Bersten, M., Anderson, J. P., Charalampopoulos, P., Fraser, M., Gromadzki, M., Young, D. R., Benetti, S., Cai, Y. -Z., Elias-Rosa, N., Lundqvist, P., Carini, R., Cosentino, S. P., Galbany, L., Gonzalez-Bañuelos, M., Gutiérrez, C. P., Kopsacheili, M., G., J. A. Pineda, Ramirez, M.
We present an analysis of the photometric and spectroscopic dataset of the Type II supernova (SN) 2018ivc in the nearby (10 Mpc) galaxy Messier 77. Thanks to the high cadence of the CHASE survey, we observed the SN rising very rapidly by nearly three
Externí odkaz:
http://arxiv.org/abs/2409.16890
Autor:
Bordiu, C., Filipovic, M. D., Umana, G., Cotton, W. D., Buemi, C., Bufano, F., Camilo, F., Cavallaro, F., Cerrigone, L., Dai, S., Hopkins, A. M., Ingallinera, A., Jarrett, T., Koribalski, B., Lazarevic, S., Leto, P., Loru, S., Lundqvist, P., Mackey, J., Norris, R. P., Payne, J., Rowell, G., Riggi, S., Rizzo, J. R., Ruggeri, A. C., Shabala, S., Smeaton, Z. J., Trigilio, C., Velovic, V.
We present the serendipitous discovery of a new radio-continuum ring-like object nicknamed Kyklos (J1802-3353), with MeerKAT UHF and L-band observations. The radio ring, which resembles the recently discovered odd radio circles (ORCs), has a diameter
Externí odkaz:
http://arxiv.org/abs/2408.07727
Autor:
Gutiérrez, Claudia P., Mattila, Seppo, Lundqvist, Peter, Dessart, Luc, González-Gaitán, Santiago, Jonker, Peter G., Dong, Subo, Coppejans, Deanne, Chen, Ping, Charalampopoulos, Panos, Elias-Rosa, Nancy, Reynolds, Thomas, Kochanek, Christopher, Fraser, Morgan, Pastorello, Andrea, Gromadzki, Mariusz, Neustadt, Jack, Benetti, Stefano, Kankare, Erkki, Kangas, Tuomas, Kotak, Rubina, Stritzinger, Maximilian D., Wevers, Thomas, Zhang, Bing, Bersier, David, Bose, Subhash, Buckley, David A. H., Dastidar, Raya, Gangopadhyay, Anjasha, Hamanowicz, Aleksandra, Kollmeier, Juna, Mao, Jirong, Misra, Kuntal, Potter, Stephen B., Prieto, Jose L., Romero-Colmenero, Encarni, Singh, Mridweeka, Somero, Auni, Terreran, Giacomo, Vaisanen, Petri, Wyrzykowski, Lukasz
We present ultraviolet, optical and near-infrared photometric and optical spectroscopic observations of the luminous, fast blue optical transient (LFBOT), CSS161010:045834-081803 (CSS161010). The transient was found in a low-redshift (z=0.033) dwarf
Externí odkaz:
http://arxiv.org/abs/2408.04698
Autor:
Valerin, G., Pastorello, A., Mason, E., Reguitti, A., Benetti, S., Cai, Y. -Z., Chen, T. -W., Eappachen, D., Elias-Rosa, N., Fraser, M., Gangopadhyay, A., Hsiao, E. Y., Howell, D. A., Inserra, C., Izzo, L., Jencson, J., Kankare, E., Kotak, R., Lundqvist, P., Mazzali, P. A., Misra, K., Pignata, G., Prentice, S. J., Sand, D. J., Smartt, S. J., Stritzinger, M. D., Tartaglia, L., Valenti, S., Anderson, J. P., Andrews, J. E., Amaro, R. C., Barbarino, C., Brennan, S., Bufano, F., Callis, E., Cappellaro, E., Dastidar, R., Della Valle, M., Fiore, A., Fulton, M. D., Galbany, L., Gromadzki, M., Heikkilä, T., Hiramatsu, D., Karamehmetoglu, E., Kuncarayakti, H., Leloudas, G., Limongi, M., Lundquist, M., McCully, C., Müller-Bravo, T. E., Nicholl, M., Ochner, P., Gonzalez, E. Padilla, Paraskeva, E., Pellegrino, C., Rau, A., Reichart, D. E., Reynolds, T. M., Roy, R., Salmaso, I., Shahbandeh, M., Singh, M., Sollerman, J., Turatto, M., Tomasella, L., Wyatt, S., Young, D. R.
We investigate the spectroscopic characteristics of Intermediate Luminosity Red Transients (ILRTs), a class of elusive objects with peak luminosity between that of classical novae and standard supernovae. We present the extensive optical and near-inf
Externí odkaz:
http://arxiv.org/abs/2407.21733
Autor:
Berman, Leah, Lundqvist, Signe, Schulze, Bernd, Servatius, Brigitte, Servatius, Herman, Stokes, Klara, Whiteley, Walter
In this paper, we establish a general setup for studying incidence-preserving motions of projective geometric configurations of points and lines via a "projective rigidity matrix". The spaces of infinitesimal motions of a point-line configuration and
Externí odkaz:
http://arxiv.org/abs/2407.17836