Zobrazeno 1 - 10
of 2 801
pro vyhledávání: '"Pannuti A"'
We present an analysis of two epochs of ACIS observations of the SA(s)c spiral galaxy NGC 3938 with the Chandra X-ray Observatory. The total exposure time of the observations was 95 ksec with a limiting unabsorbed luminosity of approximately 10^{38}$
Externí odkaz:
http://arxiv.org/abs/2411.19937
Autor:
Velović, Velibor, Filipović, M. D., Barnes, L., Norris, R. P., Tremblay, C. D., Heald, G., Rudnick, L., Shabala, S. S., Pannuti, T. G., Andernach, H., Titov, O., Waddell, S. G. H., Koribalski, B. S., Grupe, D., Jarrett, T., Alsaberi, R. Z. E., Carretti, E., Collier, J. D., Einecke, S., Galvin, T. J., Hotan, A., Manojlović, P., Marvil, J., Nandra, K., Reiprich, T. H., Rowell, G., Salvato, M., Whiting, M.
We present the discovery of highly-collimated radio jets spanning a total of 355 kpc around the nearby elliptical galaxy NGC 2663, and the possible first detection of recollimation on kiloparsec scales. The small distance to the galaxy (~28.5 Mpc) al
Externí odkaz:
http://arxiv.org/abs/2207.06713
Autor:
César Neto, João Batista, Cavalcanti, Marilia C., Silva, Cléverson O., Almeida, Vanessa C., Sapata, Vitor M., Lazarin, Rafael O., Jung, Ronald, Romito, Giuseppe A., Tatakis, Dimitris N., Pannuti, Cláudio M.
Publikováno v:
In Journal of Dentistry September 2024 148
Autor:
Filipović, M. D., Bojičić, I. S., Grieve, K. R., Norris, R. P., Tothill, N. F. H., Shobhana, D., Rudnick, L., Prandoni, I., Andernach, H., Hurley-Walker, N., Alsaberi, R. Z. E., Anderson, C. S., Collier, J. D., Crawford, E. J., For, B. -Q., Galvin, T. J., Haberl, F., Hopkins, A. M., Ingallinera, A., Kavanagh, P. J., Koribalski, B. S., Kothes, R., Leahy, D., Leverenz, H., Maggi, P., Maitra, C., Marvil, J., Pannuti, T. G., Park, L. A. F., Payne, J. L., Pennock, C. M., Riggi, S., Rowell, G., Sano, H., Sasaki, M., Staveley-Smith, L., Trigilio, V., Umana, G., Urošević, D., van Loon, J. Th., Vardoulaki, E.
We present a comprehensive multi-frequency catalogue of radio sources behind the Large Magellanic Cloud between 0.2 and 20 GHz, gathered from a combination of new and legacy radio continuum surveys. This catalogue covers an area of $\sim$144~deg$^2$
Externí odkaz:
http://arxiv.org/abs/2107.10967
Autor:
Assis Santos, Vinicius Paes de, Sendyk, Daniel Isaac, Barretto, Matheus Dantas de Araújo, Nunes, Julia Puglia, Pannuti, Claudio Mendes, Deboni, Maria Cristina Zindel
Publikováno v:
In Journal of Cranio-Maxillo-Facial Surgery June 2024 52(6):755-762
Autor:
Marco MEDINA-VEGA, Mariela Cumandá Balseca IBARRA, Maritza Del Carmen QUEZADA-CONDE, Isabella Neme Ribeiro dos REIS, Antonio Carlos FRIAS, Daniela Prócida RAGGIO, Edgard MICHEL-CROSATO, Fausto Medeiros MENDES, Claudio Mendes PANNUTI, Giuseppe Alexandre ROMITO
Publikováno v:
Brazilian Oral Research, Vol 38 (2024)
Abstract This study aimed to estimate the prevalence and extent of bleeding on probing and calculus in 12-year-old schoolchildren of Quito, Ecuador, and evaluate the associated factors. We conducted an epidemiological survey with a representative sam
Externí odkaz:
https://doaj.org/article/f7069696cecd4d99a5a935c8203c935d
Autor:
Yew, Miranda, Filipović, Miroslav D., Stupar, Milorad, Points, Sean D., Sasaki, Manami, Maggi, Pierre, Haberl, Frank, Kavanagh, Patrick J., Parker, Quentin A., Crawford, Evan J., Vukotić, Branislav, Urošević, Dejan, Sano, Hidetoshi, Seitenzahl, Ivo R., Rowell, Gavin, Leahy, Denis, Bozzetto, Luke M., Maitra, Chandreyee, Leverenz, Howard, Payne, Jeffrey L., Park, Laurence A. F., Alsaberi, Rami Z. E., Pannuti, Thomas G.
We present a new optical sample of three Supernova Remnants and 16 Supernova Remnant (SNR) candidates in the Large Magellanic Cloud(LMC). These objects were originally selected using deep H$\alpha$, [SII] and [OIII] narrow-band imaging. Most of the n
Externí odkaz:
http://arxiv.org/abs/2010.14698
We present the results of an X-ray spectral analysis of the northeast region of the candidate supernova remnant G189.6+3.3 with Suzaku. K-shell lines from highly ionized Ne, Mg, Si, and S were detected in the spectrum for the first time. In addition,
Externí odkaz:
http://arxiv.org/abs/2007.03226
We present the results of a spectral analysis of the central region of the mixed-morphology supernova remnant HB 9. A prior Ginga observation of this source detected a hard X-ray component above 4 keV and the origin of this particular X-ray component
Externí odkaz:
http://arxiv.org/abs/2004.07465
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