3,053 results on '"Pannuti A"'
Search Results
2. Collimation of the kiloparsec-scale radio jets in NGC 2663
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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., and Whiting, M.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
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) allows us to resolve portions of the jets to examine their structure. We combine multiwavelength data: radio observations by the Murchison Widefield Array (MWA), the Australian Square Kilometre Array Pathfinder (ASKAP) and the Australia Telescope Compact Array (ATCA), and X-ray data from Chandra, Swift and SRG/eROSITA. We present intensity, rotation measure, polarisation, spectral index and X-ray environment maps. Regions of the southern jet show simultaneous narrowing and brightening, which can be interpreted as a signature of the recollimation of the jet by external, environmental pressure, though it is also consistent with an intermittent Active Galactic Nuclei (AGN) or complex internal jet structure. X-ray data suggest that the environment is extremely poor; if the jet is indeed recollimating, the large recollimation scale (40 kpc) is consistent with a slow jet in a low-density environment., Comment: 16 pages, 14 figures, Accepted for publication in MNRAS
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- 2022
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3. Digital three-dimensional assessment of free gingival graft remodeling over 12 months
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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., and Pannuti, Cláudio M.
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- 2024
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4. Selective outcome reporting in randomized clinical trials using the third molar surgery model
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Assis Santos, Vinicius Paes de, Sendyk, Daniel Isaac, Barretto, Matheus Dantas de Araújo, Nunes, Julia Puglia, Pannuti, Claudio Mendes, and Deboni, Maria Cristina Zindel
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- 2024
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5. Radio Continuum Sources behind the Large Magellanic Cloud
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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., and Vardoulaki, E.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
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$ at angular resolutions from 45 arcsec to $\sim$3 arcmin. We find 6434 discrete radio sources in total, of which 3789 are detected at two or more radio frequencies. We estimate the median spectral index ($\alpha$; where $S_{v}\sim\nu^\alpha$) of $\alpha = -0.89 $ and mean of $-0.88 \pm 0.48$ for 3636 sources detected exclusively at two frequencies (0.843 and 1.384 GHz) with similar resolution (FWHM $\sim$40-45 arcsec). The large frequency range of the surveys makes it an effective tool to investigate Gigahertz Peak Spectrum (GPS), Compact Steep Spectrum (CSS) and Infrared Faint Radio sources populations within our sample. We find 10 GPS candidates with peak frequencies near 5 GHz, from which we estimate their linear size. 1866 sources from our catalogue are (CSS) candidates with $\alpha <-0.8$. We found six candidates for High Frequency Peaker (HFP) sources, whose radio fluxes peak above 5 GHz and no sources with unconstrained peaks and $\alpha~>0.5$. We found optical counterparts for 343 of the radio continuum sources, of which 128have a redshift measurement. Finally, we investigate the population of 123 Infrared Faint Radio Sources (IFRSs) found in this study., Comment: Accepted for publication in MNRAS
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- 2021
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6. Impact of gingivitis on oral health-related quality of life in 12-year-old schoolchildren of Quito, Ecuador
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Balseca Ibarra, M. C., Medina Vega, M. V., Souto, M. L. S., Romito, G. A., Frias, A. C., Raggio, D. P., Crosato, E. M., Mendes, F. M., and Pannuti, C. M.
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- 2023
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7. LCA and EPD need digitalization
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Pannuti, U.R., primary
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- 2023
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8. Periodontal status among 12-year-old schoolchildren: a population-based cross-sectional study in Quito, Ecuador
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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, and Giuseppe Alexandre ROMITO
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Gingivitis ,Dental Calculus ,Child ,Epidemiology ,Dentistry ,RK1-715 - Abstract
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 sample of 1,100 12-year-old schoolchildren from public schools in the urban area of Quito, Ecuador. We assessed the periodontal health using the Community Periodontal Index (CPI). The prevalence and extent of the periodontal condition was based on the presence of at least one site with bleeding on probing (BOP), and the presence of dental calculus was also evaluated. We used univariate and multiple multilevel Poisson regression analyses to verify the association between the independent variables and the number of sextants with BOP and calculus. The prevalence of BOP and calculus was 92% and 69.9%, respectively. The adjusted mean of the affected sextants was 4.3 and 2.2 for BOP and calculus, respectively. The mother’s schooling and malocclusion were associated with the number of sextants with bleeding. The mother’s schooling and dental caries experience were associated with calculus. Gingival bleeding and the presence of dental calculus are highly prevalent in 12-year-old schoolchildren from Quito. Gingival bleeding is associated with maternal education and malocclusion, and dental calculus is associated with maternal education and dental caries.
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- 2024
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9. New Optically Identified Supernova Remnants in the Large Magellanic Cloud
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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., and Pannuti, Thomas G.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Astrophysics of Galaxies - Abstract
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 newly found objects are located in less dense regions, near or around the edges of the LMC's main body. Together with previously suggested MCSNR J0541-6659, we confirm the SNR nature for two additional new objects: MCSNR J0522-6740 and MCSNRJ0542-7104. Spectroscopic follow-up observations for 12 of the LMC objects confirm high [SII]/H$\alpha$ a emission-line ratios ranging from 0.5 to 1.1. We consider the candidate J0509-6402 to be a special example of the remnant of a possible Type Ia Supernova which is situated some 2$^\circ$ ($\sim 1.75$kpc) north from the main body of the LMC. We also find that the SNR candidates in our sample are significantly larger in size than the currently known LMC SNRs by a factor of $\sim 2$. This could potentially imply that we are discovering a previously unknown but predicted, older class of large LMC SNRs that are only visible optically. Finally, we suggest that most of these LMC SNRs are residing in a very rarefied environment towards the end of their evolutionary span where they become less visible to radio and X-ray telescopes., Comment: 24 pages, 25 figures, to appear in MNRAS
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- 2020
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10. Discovery of recombining plasma associated with the candidate supernova remnant G189.6+3.3 with Suzaku
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Yamauchi, Shigeo, Oya, Moe, Nobukawa, Kumiko K., and Pannuti, Thomas G.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
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, a radiative recombining continuum (RRC) from He-like Si was clearly seen near 2.5 keV. This detection of an RRC reveals for the first time that G189.6+3.3 possesses an X-ray-emitting recombining plasma (RP). The extracted X-ray spectrum in the 0.6-10.0 keV energy band is well fitted with a model consisting of a collisional ionization equilibrium plasma component (associated with the interstellar medium) and an RP component (associated with the ejecta). The spectral feature shows that G189.6+3.3 is most likely to be a middle-aged SNR with an RP., Comment: Accepted for publication in PASJ
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- 2020
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11. X-ray emission from the mixed-morphology supernova remnant HB 9
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Saito, Mariko, Yamauchi, Shigeo, Nobukawa, Kumiko K., Bamba, Aya, and Pannuti, Thomas G.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
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 is still unknown. Our results demonstrate that the extracted X-ray spectra are best represented by a model consisting of a collisional ionization equilibrium plasma with a temperature of ~0.1-0.2 keV (interstellar matter component) and an ionizing plasma with a temperature of ~0.6-0.7 keV and an ionization timescale of >1 x 10^{11} cm^{-3} s (ejecta component). No significant X-ray emission was found in the central region above 4 keV. The recombining plasma model reported by a previous work does not explain our spectra., Comment: Accepted for publication in PASJ
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- 2020
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12. Toothpaste-related interests of Google users from different countries
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Bruna DI PROFIO, Matheus LOTTO, Patricia Estefania Ayala AGUIRRE, Cristina Cunha VILLAR, Giuseppe Alexandre ROMITO, Mariana Minatel BRAGA, Thiago CRUVINEL, and Cláudio Mendes PANNUTI
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Consumer Health Information ,Internet Use ,Dental Informatics ,COVID-19 ,Toothpastes ,Dentistry ,RK1-715 - Abstract
Abstract The Internet is a growing source of knowledge and can provide information about oral health. This ecological study aimed to characterize the interests in toothpaste among Google users from different countries. Our hypothesis was that there would be an increase in Google users’ interest in information about toothpaste. This retrospective longitudinal ecological study analyzed the toothpaste-related interest of Google users from 10 countries between January 2004 and December 2020. The monthly variation in relative search volume (RSV) and the main related queries were determined using Google Trends. Autoregressive integrated moving average (ARIMA) forecasting models were built to establish the predictive RSV values for toothpaste for an additional 12 months. Autocorrelation plots and the generalized additive model (GAM) were used to diagnose trends and seasonality in RSV curves. Additionally, the influence of social isolation related to the outbreak of COVID-19 was analyzed. Although not detected by autocorrelation function (ACF) and partial autocorrelation function (PACF) analyses, the heuristic analysis showed an increase in the interest in toothpaste-related information in all countries, with a stable trend observed in the 12-month forecasts, except for the increases in the United Kingdom and South Africa. Also, GAM analyses demonstrated a non-significant monthly or quarterly seasonal influence on data. In addition, social isolation during the COVID-19 pandemic did not influence the online information-seeking behavior of Google Search users linked to this topic. We confirmed the hypothesis that the interest of Google Search users in information about toothpaste increased in all of the 10 assessed countries.
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- 2023
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13. Photobiomodulation therapy and 3% potassium nitrate gel as treatment of cervical dentin hypersensitivity: a randomized clinical trial
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Tolentino, Andrea Barros, Zeola, Livia Favaro, Fernandes, Marcella Rodrigues Ueda, Pannuti, Claudio Mendes, Soares, Paulo Vinícius, and Aranha, Ana Cecilia Correa
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- 2022
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14. The X-ray-Resolved Supernova Remnant S8 in the Dwarf Irregular Galaxy IC 1613
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Schlegel, Eric M., Pannuti, Thomas G., Lozinskaya, T., Moiseev, A., and Lacey, C. K.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We conducted an observation of the nearby irregular galaxy IC 1613 with the Chandra X-ray Observatory using the S3 chip of the ACIS with an effective exposure time of 49.9 ksec. The observation primarily targeted the extensive bubble and star formation region in the northeast quadrant of the galaxy. The only known supernova remnant (SNR) in IC 1613, S8, is also the galaxy's most luminous X-ray source (L_X (0.3-8 keV) ~5-6x10^{36} erg/s). We resolve the SNR with Chandra and compare its nearly circular X-ray morphology with Halpha and radio images. We assign an upper limit on the luminosity of any possible associated compact central object of ~4x10^{35}$ erg/s (0.3-8 keV band) and conclude that we would detect a Crab-like pulsar but not a Cas A-like object. We infer an age for S8 of ~3400-5600 years and compare it to other SNRs in the Local Group. We suggest that S8 is a young composite SNR., Comment: accepted 2019 July 18 for AJ
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- 2019
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15. Multiwavelength Study of the X-Ray Bright Supernova Remnant N300-S26 in NGC 300
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Gross, Jacob, Williams, Benjamin F., Pannuti, Thomas G., Binder, Breanna, Garofali, Kristen, and Hanvey, Zachary G.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present a multiwavelength examination of the supernova remnant (SNR) S26 in the nearby galaxy NGC 300 using data from Chandra X-ray Observatory, XMM-Newton X-ray Observatory, Hubble Space Telescope (HST), the Very Large Array, and the Australia Telescope Compact Array. We simultaneously fit all of the available X-ray data with a thermal plasma model and find a temperature of $0.77 \pm 0.13$ keV with a hydrogen column density of ($9.7^{+6.4}_{-4.8}$)$\times 10^{20}$ cm$^{-2}$. HST imaging allows us to measure a semimajor axis of $0.78 \pm 0.10$ arcsec ($7.5 \pm 1.0$ pc) and a semiminor axis of $0.69^{+0.14}_{-0.12}$ arcsec ($6.7^{+1.2}_{-1.4}$ pc). This precise size helps to constrain the age and velocity of the shock to be ($3.3^{+0.7}_{-0.6}$)$\times 10^{3}$ yr and $411^{+275}_{-122}$ km s$^{-1}$. We also fit photometry of the surrounding stars to infer the age and mass of the progenitor star to be $8 \pm 1$ Myr and $25^{+1}_{-5}$ M$_{\odot}$. Based on measured radio properties of the source and assuming equipartition, the estimated radio luminosity of $\sim 1.7 \times 10^{34}$ erg s$^{-1}$ over the $10^{8}-10^{11}$ Hz frequency range results in a minimum magnetic field associated with this SNR of $0.067$ mG and the minimum energy needed to power the observed synchrotron emission of $1.5 \times 10^{49}$ erg. The size and temperature of N300-S26 appear to be similar to the Galactic SNR G311.5-0.3 except that G311.5-0.3 has a significantly lower X-ray luminosity, is older, and has a slower shock velocity., Comment: 37 pages, 6 figures, 3 tables
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- 2019
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16. Revealing the nature of central emission nebulae in the dwarf galaxy NGC 185
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Vučetić, M. M., Ilić, D., Egorov, O. V., Moiseev, A., Onić, D., Pannuti, T. G., Arbutina, B., Petrov, N., and Urošević, D.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
In this paper we present new optical observations of the galaxy NGC 185 intended to reveal the status of supernova remnants (SNRs) in this dwarf companion of the Andromeda galaxy. Previously, it was reported that this galaxy hosts one SNR. Our deep photometric study with the 2m telescope at Rozhen National Astronomical Observatory using narrow-band H$\alpha$ and [SII] filters revealed complex structure of the interstellar medium in the center of the galaxy. To confirm the classification and to study the kinematics of the detected nebulae, we carried out spectroscopic observations using the SCORPIO multi-mode spectrograph at the 6m telescope at the Special Astrophysical Observatory of the Russian Academy of Science, both in low- and high-resolution modes. We also searched the archival X-ray and radio data for counterparts of the candidate SNRs identified by our optical observations. Our observations imply the presence of one more SNR, one possible HII region previously cataloged as part of an SNR, and the presence of an additional source of shock ionization in one low-brightness PN. We detected enhanced [SII]/H_alpha and [NII]/H_alpha line ratios, as well as relatively high (up to 90 km s$^{-1}$) expansion velocities of the two observed nebulae, motivating their classification as SNRs (with diameters of 45 pc and 50 pc), confirmed by both photometric and spectral observations. The estimated electron density of emission nebulae is 30 - 200 cm$^{-3}$. Archival XMM-Newton observations indicate the presence of an extended, low-brightness, soft source in projection of one of the optical SNRs, whereas the archival VLA radio image shows weak, unresolved emission in the center of NGC 185., Comment: 15 pages, 14 figures, accepted for publication in A&A
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- 2019
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17. Murchison Widefield Array and XMM-Newton observations of the Galactic supernova remnant G5.9+3.1
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Onić, D., Filipović, M. D., Bojičić, I., Hurley-Walker, N., Arbutina, B., Pannuti, T. G., Maitra, C., Urošević, D., Haberl, F., Maxted, N., Wong, G. F., Rowell, G., Bell, M. E., Callingham, J. R., Dwarakanath, K. S., For, B. -Q., Hancock, P. J., Hindson, L., Johnston-Hollitt, M., Kapińska, A. D., Lenc, E., McKinley, B., Morgan, J., Offringa, A. R., Porter, L. E., Procopio, P., Staveley-Smith, L., Wayth, R. B., Wu, C., and Zheng, Q.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
In this paper we discuss the radio continuum and X-ray properties of the so-far poorly studied Galactic supernova remnant (SNR) G5.9+3.1. We present the radio spectral energy distribution (SED) of the Galactic SNR G5.9+3.1 obtained with the Murchison Widefield Array (MWA). Combining these new observations with the surveys at other radio continuum frequencies, we discuss the integrated radio continuum spectrum of this particular remnant. We have also analyzed an archival XMM-Newton observation, which represents the first detection of X-ray emission from this remnant. The SNR SED is very well explained by a simple power-law relation. The synchrotron radio spectral index of G5.9+3.1, is estimated to be 0.42$\pm$0.03 and the integrated flux density at 1GHz to be around 2.7Jy. Furthermore, we propose that the identified point radio source, located centrally inside the SNR shell, is most probably a compact remnant of the supernova explosion. The shell-like X-ray morphology of G5.9+3.1 as revealed by XMM-Newton broadly matches the spatial distribution of the radio emission, where the radio-bright eastern and western rims are also readily detected in the X-ray while the radio-weak northern and southern rims are weak or absent in the X-ray. Extracted MOS1+MOS2+PN spectra from the whole SNR as well as the north, east, and west rims of the SNR are fit successfully with an optically thin thermal plasma model in collisional ionization equilibrium with a column density N_H~0.80x$10^{22}$ cm$^{-2}$ and fitted temperatures spanning the range kT~0.14-0.23keV for all of the regions. The derived electron number densities n_e for the whole SNR and the rims are also roughly comparable (ranging from ~$0.20f^{-1/2}$ cm$^{-3}$ to ~$0.40f^{-1/2}$ cm$^{-3}$, where f is the volume filling factor). We also estimate the swept-up mass of the X-ray emitting plasma associated with G5.9+3.1 to be ~$46f^{-1/2}M_{\odot}$., Comment: Accepted for publication in A&A
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- 2019
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18. Discovery of a Pulsar-powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEMS5
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Alsaberi, Rami Z. E., Maitra, C., Filipovi'c, M. D., Bozzetto, L. M., Haberl, F., Maggi, P., Sasaki, M., Manjolovi'c, P., Velovi'c, V., Kavanagh, P., Maxted, N. I., Urovsevi'c, D., Rowell, G. P., Wong, G. F., For, B. -Q., O'Brien, A. N., Galvin, T. J., Staveley-Smith, L., Norris, R. P., Jarrett, T., Kothes, R., Luken, K. J., Hurley-Walker, N., Sano, H., Oni'c, D., Dai, S., Pannuti, T. G., Tothill, N. F. H., Crawford, E. J., Yew, M., Bojivci'c, I., D'enes, H., McClure-Griffiths, N., Gurovich, S., and Fukui, Y.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We report the discovery of a new Small Magellanic Cloud Pulsar Wind Nebula (PWN) at the edge of the Supernova Remnant (SNR)-DEM S5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogs PSR B1951+32 and 'the mouse'. It is travelling supersonically through the interstellar medium. We estimate the Pulsar kick velocity to be in the range of 700-2000 km/s for an age between 28-10 kyr. The radio spectral index for this SNR PWN pulsar system is flat (-0.29 $\pm$ 0.01) consistent with other similar objects. We infer that the putative pulsar has a radio spectral index of -1.8, which is typical for Galactic pulsars. We searched for dispersion measures (DMs) up to 1000 cm/pc^3 but found no convincing candidates with a S/N greater than 8. We produce a polarisation map for this PWN at 5500 MHz and find a mean fractional polarisation of P $\sim 23$ percent. The X-ray power-law spectrum (Gamma $\sim 2$) is indicative of non-thermal synchrotron emission as is expected from PWN-pulsar system. Finally, we detect DEM S5 in Infrared (IR) bands. Our IR photometric measurements strongly indicate the presence of shocked gas which is expected for SNRs. However, it is unusual to detect such IR emission in a SNR with a supersonic bow-shock PWN. We also find a low-velocity HI cloud of $\sim 107$ km/s which is possibly interacting with DEM S5. SNR DEM S5 is the first confirmed detection of a pulsar-powered bow shock nebula found outside the Galaxy., Comment: 20 pages, 15 figures, accepted for publication in MNRAS
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- 2019
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19. Current state about root coverage using soft-tissue substitutes in the presence of noncarious cervical lesions: A literature review
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Aldrin André Huaman-Mendoza, Isabella Neme Ribeiro Dos Reis, Juliana Assef Ganhito, Cassio Volponi Carvalho, Giorgio De Michel, and Claudio Mendes Pannuti
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biocompatible materials ,collagen ,dental esthetic ,dentin sensitivity ,acellular dermal matrix graft ,gingival recession ,review ,Dentistry ,RK1-715 - Abstract
About half of the cases of gingival recession are associated with the noncarious cervical lesion (NCCL), resulting in combined defects (CDs). NCCL negatively affects the root coverage outcomes. In addition, considering the morbidity associated with graft harvesting, soft-tissue substitutes (STSs) appeared as a suitable option for connective tissue grafts for surgical root coverage. Currently, the literature addressing the therapy of CDs employing STSs is scarce. Thus, the present review aimed to update the literature and outline the future perspectives about root coverage of CDs using STSs. A detailed literature search was conducted on MEDLINE, Web of Science, EMBASE, LILACS, Scopus, and Google Scholar databases using keywords and Boolean operators. Randomized clinical trials (2) and case reports (6) were included. None of the selected studies reported any adverse effect using STSs. Based on the limited evidence available, we cannot state that STSs may benefit the periodontal clinical and patient-centered outcomes. Randomized controlled trials are needed to assess the long-term outcomes, surgical approaches, and restorative protocols.
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- 2023
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20. VMXR: a EUD Environment for Virtual Merchandizing in XR.
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Alessandro Menale, Jacopo Mereu, Carlo Nuvole, Luigi Pannuti, Emanuele Mario Spano, and Lucio Davide Spano
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- 2023
21. Incidence of peri-implant disease associated with cement- and screw-retained implant-supported prostheses: A systematic review and meta-analysis
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Reis, Isabella Neme Ribeiro dos, Fukuoka, Gisele Lie, Nagay, Bruna Egumi, Pannuti, Claudio Mendes, Spin-Neto, Rubens, and da Silva, Emily Vivianne Freitas
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- 2023
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22. A Morphological Study of the Supernova Remnant RX J0852.0-4622 (Vela Jr.)
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Maxted, Nigel I., Filipovic, M. D., Sano, H., Allen, G. E., Pannuti, T. G., Rowell, G. P., Grech, A., Roper, Q., Wong, G. F., Galvin, T. J., Fukui, Y., Collier, J. D., Crawford, E. J., Grieve, K., Horta, A. D., Manojlovic, P., and O'Brien, A.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We conduct a multi-wavelength morphological study of the Galactic supernova remnant RXJ0852.0-4622 (also known as Vela Jr., Vela Z and G266.2-1.2). RX J0852.0-4622 is coincident with the edge of the larger Vela supernova remnant causing confusion in the attribution of some filamentary structures to either RX J0852.0-4622 or its larger sibling. We find that the RX J0852.0-4622 radio continuum emission can be characterised by a 2-dimensional shell with a radius of 0.90+/-0.01deg (or 11.8+/-0.6pc at an assumed distance of 750pc) centred at (l,b)=(133.08+/-0.01 deg,-46.34+/-0.01deg) (or RA=8h52m19.2s, Dec=-46deg20'24.0'', J2000), consistent with X-ray and gamma-ray emission. Although [OIII] emission features are generally associated with the Vela SNR, one particular [OIII] emission feature, which we denote as "the Vela Claw", morphologically matches a molecular clump that is thought to have been stripped by the stellar progenitor of the RX J0852.0-4622 SNR. We argue that the Vela Claw feature is possibly associated with RX J0852.0-4622. Towards the north-western edge of RX J0852.0-4622, we find a flattening of the radio spectral index towards another molecular clump also thought to be associated with RX J0852.0-4622. It is currently unclear whether this feature and the Vela Claw result from interactions between the RX J0852.0-4622 shock and the ISM., Comment: 15 pages, 7 figures, Accepted for Publication in the Astrophysical Journal (ApJ)
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- 2018
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23. A Multi-Frequency Study of the Milky Way-like Spiral Galaxy NGC 6744
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Yew, Miranda, Filipović, Miroslav D., Roper, Quentin, Collier, Jordan D., Crawford, Evan J., Jarrett, Thomas H., Tothill, Nicholas F. H., O'Brien, Andrew N., Pavlović, Marko Z., Pannuti, Thomas G., Galvin, Timothy J., Kapińska, Anna D., Cluver, Michelle E., Banfield, Julie K., Schlegel, Eric M., Maxted, Nigel, and Grieve, Kevin R.
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Astrophysics - Astrophysics of Galaxies - Abstract
We present a multi-frequency study of the intermediate spiral SAB(r)bc type galaxy NGC 6744, using available data from the Chandra X-Ray telescope, radio continuum data from the Australia Telescope Compact Array and Murchison Widefield Array, and Wide-field Infrared Survey Explorer infrared observations. We identify 117 X-ray sources and 280 radio sources. Of these, we find nine sources in common between the X-ray and radio catalogues, one of which is a faint central black hole with a bolometric radio luminosity similar to the Milky Way's central black hole. We classify 5 objects as supernova remnant candidates, 2 objects as likely supernova remnants, 17 as HII regions, 1 source as an AGN; the remaining 255 radio sources are categorised as background objects and one X-ray source is classified as a foreground star. We find the star-formation rate (SFR) of NGC 6744 to be in the range 2.8 - 4.7 $\rm{M_{\odot}~yr^{-1}}$ signifying the galaxy is still actively forming stars. The specific SFR of NGC 6744 is greater than that of late-type spirals such as the Milky Way, but considerably less that that of a typical starburst galaxy., Comment: accepted for publication in PASA
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- 2018
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24. Adjuvant Chemotherapy and Hormonotherapy in Breast Cancer
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Pannuti, F., primary, Martoni, A., additional, Camaggi, C.M., additional, Fruet, F., additional, and Cilenti, G., additional
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- 2022
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25. Extragalactic Radio Astronomy: Galaxy Classification, Active Galactic Nuclei, Superluminal Motion, Galaxy Clusters, and the Cosmic Microwave Background
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Pannuti, Thomas G., Ashby, Neil, Series Editor, Brantley, William, Series Editor, Deady, Matthew, Series Editor, Fowler, Michael, Series Editor, Hjorth-Jensen, Morten, Series Editor, Inglis, Michael, Series Editor, and Pannuti, Thomas G.
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- 2020
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26. Solar System Radio Astronomy
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Pannuti, Thomas G., Ashby, Neil, Series Editor, Brantley, William, Series Editor, Deady, Matthew, Series Editor, Fowler, Michael, Series Editor, Hjorth-Jensen, Morten, Series Editor, Inglis, Michael, Series Editor, and Pannuti, Thomas G.
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- 2020
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27. Radio Observations: An Introduction to Fourier Transforms, Convolution, Observing Through Earth’s Atmosphere, Single Dish Telescopes, and Interferometers
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Pannuti, Thomas G., Ashby, Neil, Series Editor, Brantley, William, Series Editor, Deady, Matthew, Series Editor, Fowler, Michael, Series Editor, Hjorth-Jensen, Morten, Series Editor, Inglis, Michael, Series Editor, and Pannuti, Thomas G.
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- 2020
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28. Galactic Radio Astronomy: Galactic Structure, HII Regions, Supernova Remnants, Neutron Stars and Pulsars
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Pannuti, Thomas G., Ashby, Neil, Series Editor, Brantley, William, Series Editor, Deady, Matthew, Series Editor, Fowler, Michael, Series Editor, Hjorth-Jensen, Morten, Series Editor, Inglis, Michael, Series Editor, and Pannuti, Thomas G.
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- 2020
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29. Angles, Gravity, Light, the Bohr Model of the Atom and Relativity
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Pannuti, Thomas G., Ashby, Neil, Series Editor, Brantley, William, Series Editor, Deady, Matthew, Series Editor, Fowler, Michael, Series Editor, Hjorth-Jensen, Morten, Series Editor, Inglis, Michael, Series Editor, and Pannuti, Thomas G.
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- 2020
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30. Emission Mechanisms: Blackbody Radiation, An Introduction to Radiative Transfer, Synchrotron Radiation, Thermal Bremsstrahlung, and Molecular Rotational Transitions
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Pannuti, Thomas G., Ashby, Neil, Series Editor, Brantley, William, Series Editor, Deady, Matthew, Series Editor, Fowler, Michael, Series Editor, Hjorth-Jensen, Morten, Series Editor, Inglis, Michael, Series Editor, and Pannuti, Thomas G.
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- 2020
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31. Introduction: Why Make Astronomical Observations at Radio Frequencies?
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Pannuti, Thomas G., Ashby, Neil, Series Editor, Brantley, William, Series Editor, Deady, Matthew, Series Editor, Fowler, Michael, Series Editor, Hjorth-Jensen, Morten, Series Editor, Inglis, Michael, Series Editor, and Pannuti, Thomas G.
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- 2020
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32. Efficacy of mouthrinses in reducing oral SARS-COV-2 load: a review
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Claudio Mendes PANNUTI, Isabella Neme Ribeiro dos REIS, Nathalia Vilela SOUZA, Maria Luisa Silveira SOUTO, Carlos Guillermo Benítez SILVA, Leticia Mello BEZINELLI, Clarisse Martins MACHADO, Giuseppe Alexandre ROMITO, and Cristina Cunha VILLAR
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SARS-CoV-2 ,COVID-19 ,Mouthwashes ,Saliva ,Dentistry ,RK1-715 - Abstract
Abstract Accumulated evidence has shown that the oral cavity may be an important reservoir for SARS-CoV-2. Some authors have suggested that the use of mouthrinses could reduce SARS-CoV-2 viral load in the saliva. Thus, the aim of this review was to synthesize evidence about the efficacy of mouthrinses in reducing the salivary viral load of SARS-CoV-2. 2. Nine randomized controlled trials (RCTs) have investigated the efficacy of different mouthrinses in reducing salivary SARS-CoV-2 loads. Various active ingredients have been tested in these trials: 0.5%,1% and 2% povidone-iodine, 0.2% and 0.12% chlorhexidine (CHX), 0.075% cetylpyridinium chloride (CPC), 0.075% CPC with Zinc lactate, 1% and 1.5% hydrogen peroxide (HP), 1.5% HP + 0.12% CHX and ß-cyclodextrin and citrox. The studies reported an intra-group reduction in the salivary levels of the virus, when compared with the baseline. However, the majority of these trials failed to demonstrate a significant inter-group difference between active groups and the control group relative to the decrease in salivary SARS-CoV-2 loads. Although promising, these results should be confirmed by larger trials.
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- 2023
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33. Consistency of recommendations of clinical practice guidelines in periodontology: a systematic review
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Marco Antonio ALARCÓN, Tania ARIZA-FREITAS, Natali CHAVEZ-VEREAU, Andrea LÓPEZ-PACHECO, Claudio Mendes PANNUTI, and Lilian MÁLAGA-FIGUEROA
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Periodontics ,Evidence-Based Dentistry ,Dentistry ,Oral Health ,RK1-715 - Abstract
Abstract The aim of this systematic review was to evaluate the methodological quality and the consistency of recommendations of clinical practice guidelines (CPGs) in Periodontology. An electronic search was conducted in two databases, MEDLINE and EMBASE, eight CPGs databases, and home pages of scientific societies in Periodontology up to April 2022. Three reviewers independently assessed methodological quality using the AGREE II instrument. In addition, we evaluated the consistency of the recommendations. Eleven CPGs were included, and the topics developed focused on prevention, diagnosis, risk factors, surgical and non-surgical periodontal treatment, antimicrobial therapy, root coverage, and maintenance. We found that the AGREE domains 2 (Stakeholder involvement) and 5 (Applicability) obtained the lowest scores. Domains 1 (Scope and purpose), 3 (Rigor of development) and 4 (Clarity of presentation) obtained the highest scores among the evaluated CPGs. The clinical recommendations for treatment of periodontal diseases were mostly consistent. Overall, the quality of CPGs used in periodontics was high. There was consistency of recommendations in specific fields. These findings may help researchers to promote CPGs focused on different fields of periodontics that have not yet been developed. Furthermore, the clinician will be able to make better clinical decisions.
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- 2023
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34. Identifying the prevalence of unmet supportive care needs among family caregivers of cancer patients: an Italian investigation on home palliative care setting
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Zavagli, Veronica, Raccichini, Melania, Ostan, Rita, Ercolani, Giacomo, Franchini, Luca, Varani, Silvia, and Pannuti, Raffaella
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- 2022
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35. Supernova Remnants in M33: X-ray Properties as Observed by XMM-Newton
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Garofali, Kristen, Williams, Benjamin F., Plucinsky, Paul P., Gaetz, Terrance J., Wold, Brian, Haberl, Frank, Long, Knox S., Blair, William P., Pannuti, Thomas G., Winkler, P. Frank, and Gross, Jacob
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We have carried out a study of the X-ray properties of the supernova remnant (SNR) population in M33 with XMM-Newton, comprising deep observations of 8 fields in M33 covering all of the area within the D$_{25}$ contours, and with a typical luminosity of 7.1$\times$10$^{34}$ erg s$^{-1}$ (0.2-2.0 keV) . Here we report our work to characterize the X-ray properties of the previously identified SNRs in M33, as well as our search for new X-ray detected SNRs. With our deep observations and large field of view we have detected 105 SNRs at the 3$\sigma$ level, of which 54 SNRs are newly detected in X-rays, and three are newly discovered SNRs. Combining XMM-Newton data with deep Chandra survey data allows detailed spectral fitting of 15 SNRs, for which we have measured temperatures, ionization timescales, and individual abundances. This large sample of SNRs allows us to construct an X-ray luminosity function, and compare its shape to luminosity functions from host galaxies of differing metallicities and star formation rates to look for environmental effects on SNR properties. We conclude that while metallicity may play a role in SNR population characteristics, differing star formation histories on short timescales, and small-scale environmental effects appear to cause more significant differences between X-ray luminosity distributions. In addition, we analyze the X-ray detectability of SNRs, and find that in M33 SNRs with higher [SII]/H$\alpha$ ratios, as well as those with smaller galactocentric distances, are more detectable in X-rays., Comment: 29 pages, 14 figures, 5 tables, accepted for publication in MNRAS
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- 2017
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36. CTIO, ROSAT HRI and Chandra ACIS Observations of the Archetypical Mixed-Morphology Supernova Remnant W28 (G6.4-0.1)
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Pannuti, Thomas G., Rho, Jeonghee, Kargaltsev, Oleg, Rangelov, Blagoy, Kosakowski, Alekzander R., Winkler, P. Frank, Keohane, Jonathan W., Hare, Jeremy, and Ernst, Sonny
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present a joint analysis of optical emission-line and X-ray observations of the archetypical Galactic mixed-morphology supernova remnant (MMSNR) W28 (G6.4-0.1). MMSNRs comprise a class of sources whose shell-like radio morphology contrasts with a filled center in X-rays; the origin of these contrasting morphologies remains uncertain. Our CTIO images reveal enhanced [S II] emission relative to H-alpha along the northern and eastern rims of W28. Hydroxyl (OH) masers are detected along these same rims, supporting prior studies suggesting that W28 is interacting with molecular clouds at these locations, as observed for several other MMSNRs. Our ROSAT HRI mosaic of W28 provides almost complete coverage of the SNR. The X-ray and radio emission is generally anti-correlated, except for the luminous northeastern rim, which is prominent in both bands. Our Chandra observation sampled the X-ray-luminous central diffuse emission. Spectra extracted from the bright central peak and from nearby annular regions are best fit with two over-ionized recombining plasma models. We also find that while the X-ray emission from the central peak is dominated by swept-up material, that from the surrounding regions shows evidence for oxygen-rich ejecta, suggesting that W28 was produced by a massive progenitor. We also analyze the X-ray properties of two X-ray sources (CXOU J175857.55-233400.3 and 3XMM J180058.5-232735) projected into the interior of W28 and conclude that neither is a neutron star associated with the SNR. The former is likely to be a foreground cataclysmic variable or a quiescent low-mass X-ray-binary while the latter is likely to be a coronally-active main sequence star., Comment: Accepted for publication in Astrophysical Journal, 58 pages (manuscript format), 15 figures
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- 2017
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37. Preloading peri‐implant crestal bone loss: A retrospective study of incidence and related factors.
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Vilela, Nathalia, Gurgel, Bruno C. V., Bruzos, Carlos De, Duarte, Wagner R., da Silva, Hélio D. P., Pannuti, Claudio M., and Duarte, Poliana Mendes
- Abstract
Background: The aim of this study was to evaluate the incidence of preloading crestal bone loss (PLCBL) and to identify the patient‐related and implant‐related factors associated with PLCBL. Methods: This retrospective cohort examined the dental records of patients who received at least one dental implant. PLCBL was defined as a reduction ⩾0.5 mm and severe PLCBL (primary variable) as a reduction ⩾1.5 mm in mesial and/or distal bone level, measured from the day of implant placement to uncovering or abutment installation/crown delivery. The incidence of PLCBL and patient and implant variables were recorded. Bivariate analysis and binary logistic regression identified factors associated with PLCBL ⩾0.5 mm and ⩾1.5 mm. Results: A total of 746 dental implants placed in 361 patients from January 2011 to July 2021 was included in the analyses. Of the implants assessed, 24.4% (n = 182) exhibited PLCBL ⩾ 0.5 mm and 10.5% (n = 78) presented severe PLCBL (i.e., ⩾1.5 mm). Males (odds ratio [OR] = 1.85, 95% confidence interval [CI] = 1.11–3.07), patients with diabetes (OR = 3.33, 95% CI = 1.73–6.42), and those allergic to penicillin (OR = 3.13, 95% CI = 1.57–6.22) were more likely to experience severe PLCBL (p < 0.05). Implants placed in the anterior area (OR = 2.08, 95% CI = 1.16–3.73), with bone‐level platform‐abutment connection (OR = 4.73, 95% CI = 1.94–11.49) and inserted supracrestally (OR = 3.77, 95% CI = 1.84–7.72), presented a greater risk of developing severe PLCBL (p < 0.05). Implants placed in a previously grafted area presented a lower likelihood of developing severe PLCBL (OR = 0.489, 95% CI = 0.28–0.84). Conclusion: The incidence of PLCBL ⩾ 0.5 mm and ⩾1.5 mm was 24.4% and 10.5%, respectively. Male sex, diabetes, allergy to penicillin, anterior location, bone‐level platform‐abutment connection, and supracrestal implant placement are potential risk factors for severe PLCBL. A previously grafted area is a potential protective factor. [ABSTRACT FROM AUTHOR]
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- 2024
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38. Periodontal outcomes of surgically exposed and orthodontically aligned buccally impacted maxillary canines: A systematic review and meta-analysis.
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Corrente, Marina Nogueira de Castro Galvão, do Amaral, Guilherme Castro Lima Silva, Ribeiro, Rafael Costa, Pannuti, Cláudio Mendes, Cavalcanti, Laura Grein, and Villar, Cristina Cunha
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DATA extraction ,GREY literature ,CONFIDENCE intervals ,LONGITUDINAL method ,GINGIVA - Abstract
Objective: To compare the periodontal outcomes of surgically exposed and orthodontically aligned buccally impacted maxillary canines to spontaneously erupted maxillary canines. Data sources: An unrestricted search was carried out of indexed databases (Medline, EMBASE, Web of Science and Scopus), reference lists of included studies, and grey literature published until December 2023. Data selection: Observational and experimental studies that addressed the focused question 'Do periodontal outcomes of buccally impacted maxillary canines that were surgically exposed and subsequently extruded and aligned using orthodontic alignment, differ from those of spontaneously erupted maxillary canines?' were included. Data extraction: Study screening, selection and data extraction were performed independently by two authors, with disagreement resolved by a third reviewer. The risk of bias was assessed using the JBI Critical Appraisal Checklist and GRADE approach. Results: A total of 857 citations were found and five studies were eligible for inclusion. Supragingival plaque accumulation and gingival inflammation were similar between impacted canines and their contralaterals in most studies. Meta-analyses revealed no significant differences in keratinised tissue width (prospective studies: MD = −0.28, 95% confidence interval [CI] = −1.13–0.56, I² = 78%; retrospective studies: MD = 0.61, 95% CI = −1.51–2.72, I² = 94%). However, a meta-analysis of prospective studies showed slightly greater mean probing depth for impacted canines compared to their contralateral canines (prospective studies: MD = 0.16, 95% CI = 0.04–0.28, I² = 0%). The evidence certainty for keratinised tissue width and probing depth outcomes was low. Conclusion: Surgically exposed and orthodontically aligned buccally impacted canines have slightly greater probing depths, potential bone loss and increased clinical crown length, compared to their counterparts. However, these small differences (<1 mm) are unlikely to be clinically significant. [ABSTRACT FROM AUTHOR]
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- 2024
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39. Impact of Smoking Cessation on Periodontal Tissues
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Duarte, Poliana Mendes, Nogueira, Cristiana Fernandes Plutarco, Silva, Sarah Monique, Pannuti, Cláudio Mendes, Schey, Karin C., and Miranda, Tamires Szeremeske
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- 2022
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40. Impact of Smoking Cessation on Periodontal Tissues
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Poliana Mendes Duarte, Cristiana Fernandes Plutarco Nogueira, Sarah Monique Silva, Cláudio Mendes Pannuti, Karin C. Schey, and Tamires Szeremeske Miranda
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Periodontitis ,Smoking cessation ,Periodontal therapy ,Tooth loss ,Dentistry ,RK1-715 - Abstract
There is cumulative evidence supporting the negative effects of smoking on periodontal tissues. Smoking cessation can be successfully accomplished through specific programs, including behaviour modification and medications, and has been suggested as a suitable way to reduce the risk of several diseases, including periodontitis. The aim of this review is to provide a concise overview of the current knowledge about the impact of smoking cessation on periodontal tissues and therapy, with data from studies published in the last 15 years. Literature was searched using Medline database from 2005 up to and including September 2020 using medical subject heading (MeSH) terms and other search terms, restricted to the English language. Studies were evaluated and summarised in a narrative review format. Results demonstrated that there is convincing evidence to support the benefits of tobacco cessation in reducing the risk of periodontitis and tooth loss. In addition, the harmful effects of smoking on periodontal tissues seem to be assuaged as the number of years since quitting increases. The existing current evidence, even limited, also shows that smoking cessation may result in additional benefits to the outcome of nonsurgical periodontal treatment. Periodontal care providers should not only check their patient's smoking habit for estimating risk of disease progression and predictability of periodontal therapy, but they should also help smokers improve their oral and systemic health by providing efficient and personalised tobacco‐cessation counselling and treatment.
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- 2022
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41. Smoking Cessation therapy is a cost-effective intervention to avoid tooth loss in Brazilian subjects with periodontitis: an economic evaluation
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Maria Luisa Silveira Souto, Fernanda Campos de Almeida Carrer, Mariana Minatel Braga, and Cláudio Mendes Pannuti
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Cigarette smoking ,Smoking cessation ,Periodontitis ,Health economics ,Modelling ,Dentistry ,RK1-715 - Abstract
Abstract Background Smokers present a higher prevalence and severity of periodontitis and, consequently, higher prevalence of tooth loss. Smoking cessation improves the response to periodontal treatment and reduces tooth loss. So, the aim of this study was to evaluate the efficiency in resources allocation when implementing smoking cessation therapy vs. its non-implementation in smokers with periodontitis. Methods We adopted the Brazilian public system perspective to determine the incremental cost-effectiveness (cost per tooth loss avoided) and cost-utility (cost per oral-related quality-adjusted life-year ([QALY] gained) of implementing smoking cessation therapy. Base-case was defined as a 48 years-old male subject and horizon of 30 years. Effects and costs were combined in a decision analytic modeling framework to permit a quantitative approach aiming to estimate the value of the consequences of smoking cessation therapy adjusted for their probability of occurrence. Markov models were carried over annual cycles. Sensitivity analysis tested methodological assumptions. Results Implementing the therapy saved approximately US$ 100 over the time horizon accompanied by a slightly better effect, both in CEA and CUA. Considering uncertainties, the therapy could be cost-effective in the most part of simulated cases, even being cheaper and more effective in 35% of cases in which the oral-health related outcome is used as effect. Considering a willingness-to-pay of US$100 per health effect, smoking cessation therapy was cost-effective, respectively, in 72% and 99% of cases in cost-utility and cost-effectiveness analyses. Conclusions Implementation of smoking cessation therapy may be cost-effective, considering the avoidance of tooth loss and oral health-related consequences to patients.
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- 2021
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42. Impact of COVID-19 on perception and preparedness among clinical year Malaysian undergraduate dental students – A cross-sectional study
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Avita Rath, Melissa Wong Li Zheng, and Claudio Mendes Pannuti
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dental education ,covid-19 ,undergraduate ,online ,malaysia ,educational technology ,Dentistry ,RK1-715 - Abstract
This study aimed to evaluate how quarantine affected final-year dental students' self-perceptions of preparation and assess how online training affected clinical students' education at SEGi University. Year 3 to 5 students (n=140) were asked to fill up an online questionnaire. The first part included the effects of online education experience between the academic years. The second section assessed the graduating class's self-perceived readiness in cognitive, communication and professional abilities. The Chi-square test was used to analyse the association between the groups regarding academic years, gender, and family income. Year 3 students missed educational experiences during lockdown significantly more than years 4 and 5 (p
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- 2022
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43. Influence of supracrestal tissue height on peri-implant hard and soft tissues of single implants placed in the esthetic area using the one abutment-one time approach: a 1-year prospective interventional study.
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Ribeiro dos Reis, Isabella Neme, Fernando Todescan, Francisco, Morente Ruiz, Glaucio, Freitas da Silva, Emily Vivianne, Alexandre Romito, Giuseppe, Spin-Neto, Rubens, and Mendes Pannuti, Claudio
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MAXILLA surgery ,DENTAL implants ,EXPERIMENTAL design ,PILOT projects ,DENTAL crowns ,TEETH ,BONE resorption ,PERIODONTITIS ,TIME ,COSMETIC dentistry ,DENTAL abutments ,RESEARCH funding ,DESCRIPTIVE statistics ,GINGIVA ,LONGITUDINAL method - Abstract
Objective: This pilot, prospective interventional study aimed to analyze the influence of supracrestal tissue height when using the one abutment-one time concept at the time of implant placement, on peri-implant hard and soft tissue remodeling in esthetic areas. The definitive crown was placed 7 days later. Method and materials: Facial mucosal margin position, mesial and distal papilla levels, and mesial and distal marginal bone loss were assessed after 7 days (placement of the definitive crown), and 1,2,3,6, and 12 months after implant placement. Patients were classified according to the supracrestal tissue height as thin (< 3 mm) and thick (> 3 mm). Results: Fifteen patients fulfilled the eligibility criteria and were included in the study. Eight presented a thick supracrestal tissue height and seven a thin supracrestal tissue height. After 12 months, the implant success rate was 100%. The mean recession at the facial mucosal margin position was-0.47 ± 0.57 mm and -0.19 ± 0.41 mm in thin and thick groups, respectively (P = .29). The mean mesial papilla level recession was -0.19±0.06mm in the thin group and -0.01± 0.07 mm in the thick group (P< .01), and the mean distal papilla level recession was -0.15±0.09mm in the thin group and 0.00 ± 0.15 mm in the thick group (P<.05). The mean bone loss was-0.21 ± 0.18 mm and -0.04±0.14 mm in the thin and thick groups, respectively (P<.05). Conclusion: Single maxillary anterior implants with thin supracrestal tissue height (<3 mm) at the time of implant placement had greater bone loss and papillary recession than implants with a thick soft tissue height (≥ 3 mm), even when using the one abutment-one time concept. [ABSTRACT FROM AUTHOR]
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- 2023
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44. Cross-cultural adaptation and validation of Malay version of Rapid Estimate of Adult Literacy in Dentistry (MREALD-30) among Orang Asli population in Malaysia
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Avita Rath, Melissa Wong, Claudio Mendes Pannuti, Priyadarshini Hesarghatta Ramamurthy, Bennete Fernandes, Amelia Shelton, and Khairiyah Abdul Muttalib
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REALD-30 ,Oral health ,Health literacy ,Psychometric evaluation ,Malay ,Malaysia ,Dentistry ,RK1-715 - Abstract
Abstract Background The aim of this study was to adapt, translate and validate the Rapid Estimate of Adult Literacy in Dentistry (MREALD-30) instrument for the Orang Asli population in Malaysia. Methods After translation and cross-cultural adaptation, interviews were conducted with 326 participants of the Temuan tribe from village Kampung Tering in Johol, Negeri Sembilan, Malaysia. The instrument's validity was assessed using the scores of MREALD-30, which were compared based on occupation, monthly household income, educational attainment, general literacy, use of dental services, and three dental outcomes. A questionnaire containing socio-behavioral information and validated Malay Oral Health Impact Profile (M-OHIP-14) was also administered. The reliability of the MREALD-30 was assessed by re-administering it to 30 subjects after two weeks. Its correlations evaluated convergent and discriminative validity of MREALD-30 with the level of education and dental visiting habits, monthly household income, respectively. Predictive validity was assessed with M-OHIP-14, while construct validity was evaluated by exploratory factor analysis using the Rasch model. Results The internal consistency of the MREALD-30 measured by Cronbach's alpha was 0.89. The test–retest reliability was excellent (ICC 0.95, k = 0.85). MREALD-30 exhibited good construct validity. Rasch analysis showed two factors, and infit mean-square statistics for MREALD-30 were all within the desired range of 0.50–2.0. The discriminant validity and predictive validity were statistically significant (p
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- 2021
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45. Choice of access route for artificial nutrition in cancer patients: 30 y of activity in a home palliative care setting
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Ruggeri, Enrico, Giannantonio, Marilena, Ostan, Rita, Agostini, Federica, Sasdelli, Anna Simona, Valeriani, Luca, Pironi, Loris, and Pannuti, Raffaella
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- 2021
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46. Gingival phenotype and its relationship with different clinical parameters: a study in a Dominican adult sample
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Collins, James Rudolph, Pannuti, Claudio Mendes, Veras, Kenia, Ogando, Gabriel, and Brache, Michael
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- 2021
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47. Caring Advanced Cancer Patients at Home During COVID-19 Outbreak: Burnout and Psychological Morbidity Among Palliative Care Professionals in Italy
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Varani, Silvia, Ostan, Rita, Franchini, Luca, Ercolani, Giacomo, Pannuti, Raffaella, Biasco, Guido, and Bruera, Eduardo
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- 2021
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48. Characterization of the Notch pathway in nasal polyps of patients with chronic rhinosinusitis: A pilot study
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Giorgio Aquila, Alessandra Alaimo, Luisa Marracino, Valeria Martino, Francesca Camponogara, Francesco Vieceli Dalla Sega, Francesca Fortini, Antonio Pannuti, Claudia Zanotti, Nicola Malagutti, Stefano Pelucchi, and Paola Rizzo
- Subjects
eosinophils ,glucocorticoids ,nasal polyps ,notch pathway ,rhinosinusitis ,translational medicine ,Physiology ,QP1-981 - Abstract
Abstract Chronic rhinosinusitis with nasal polyps is a widespread pathology characterized by persistent inflammation of nasal and paranasal mucosa. Although it represents one of the most frequent diseases of the nasal cavities, its etiology is still not completely elucidated. There is evidence suggesting that the Notch signaling, a highly conserved intercellular pathway known to regulate many cellular processes, including inflammation, is implicated in nasal polyps formation. The purpose of this study was to investigate the expression of genes of the Notch pathway in nasal polyps from patients with chronic rhinosinusitis. Nasal polyps and adjacent mucosa tissue were obtained from 10 patients. RNA was analyzed by quantitative reverse transcriptase‐polymerase chain reaction for the expression level of (1) Notch pathway components such as receptors (NOTCH1‐4), ligands (DLL4, JAGGED‐1), and target genes (HEY1, 2, and HES1) and (2) genes providing information on the pathogenesis of polyposis (C‐MYC and SCGB1A1) and on eosinophils content (CCL26, IL5, and SAA2). We report a Notch‐driven gene expression pattern in nasal polyps which correlates with the expression of genes highly expressed in eosinophils, whose presence is an important parameter to define the pathophysiologic diversity characterizing nasal polyps. Taken together, our results suggest a role for Notch signaling in the pathophysiology of polyposis. Further studies are needed to elucidate the role of Notch in nasal polyps formation and to establish whether it could represent a novel therapeutic target for this pathology.
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- 2022
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49. Does the school environment exert influence on quality of life related to traumatic dental injury in children?
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Maritza Del Carmen QUEZADA-CONDE, Patricia Lourdes ALVAREZ-VELASCO, Mariela Cumanda BALSECA-IBARRA, Raíza Dias FREITAS, Thiago Machado ARDENGHI, Edgard MICHEL-CROSATO, Claudio Mendes PANNUTI, Antonio Carlos FRIAS, Daniela Prócida RAGGIO, and Fausto Medeiros MENDES
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Dental Caries ,Quality of Life ,Cross-sectional Studies ,Dentistry ,RK1-715 - Abstract
Abstract The aim of this cross-sectional study was to assess whether favorable factors related to school characteristics have a positive effect on the impact of traumatic dental injury (TDI) on oral health-related quality of life (OHRQoL). An epidemiological survey of oral health was conducted with 12-year-old schoolchildren from Quito, Ecuador. Children were examined for TDI, dental caries, and malocclusion. Individual socioeconomic data were also collected. Information on the physical environment, health practices, and occurrence of negative episodes at school was collected from the school coordinators. The Child Perceptions Questionnaire 11-14 (CPQ11-14) was used to evaluate the OHRQoL (outcome variable). Multilevel Poisson regression analysis was conducted. Severe TDI was associated with higher CPQ11-14 scores, even in the multiple model adjusted for oral health conditions, sex, individual socioeconomic variables, and school-related variables. Children from schools that had an appropriate tooth-brushing environment for their students exhibited a lower impact on OHRQoL, even after adjustment for the occurrence of TDI and other variables. A favorable school environment may exert a positive effect on OHRQoL, independent of the occurrence of TDI.
- Published
- 2022
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50. Optical observations of the nearby galaxy IC342 with narrow band [SII] and H$\alpha$ filters. II - Detection of 16 Optically-Identified Supernova Remnant Candidates
- Author
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Vucetic, M. M., Ciprijanovic, A., Pavlovic, M. Z., Pannuti, T. G., Petrov, N., Goker, U. D., and Ercan, E. N.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present the detection of 16 optical supernova remnant (SNR) candidates in the nearby spiral galaxy IC342. The candidates were detected by applying [SII]/H$\alpha$ ratio criterion on observations made with the 2 m RCC telescope at Rozhen National Astronomical Observatory in Bulgaria. In this paper, we report the coordinates, diameters, H$\alpha$ and [SII] fluxes for 16 SNRs detected in two fields of view in the IC342 galaxy. Also, we estimate that the contamination of total H$\alpha$ flux from SNRs in the observed portion of IC342 is 1.4%. This would represent the fractional error when the star formation rate (SFR) for this galaxy is derived from the total galaxy's H$\alpha$ emission., Comment: 8 pages, 2 figures, 2 tables; to be published in Serbian Astronomical Jornal
- Published
- 2015
- Full Text
- View/download PDF
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