Search

Your search keyword '"Mori, M"' showing total 17,274 results
Start Over Author "Mori, M"
17,274 results on '"Mori, M"'

201. TeV gamma-ray observations of southern BL Lacs with the CANGAROO 3.8m Imaging Telescope

Author

Roberts, M. D., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Holder, J., Kakimoto, F., Kamei, S., Kawachi, A., Kifune, T., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Matsuoka, T., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Nishijima, K., Oda, S., Ogio, S., Patterson, J. R., Rowell, G. P., Sako, T., Sakurazawa, K., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.

Subjects
Astrophysics
Abstract

Observational and theoretical results indicate that low-redshift BL Lacertae objects are the most likely extragalactic sources to be detectable at TeV energies. In this paper we present the results of observations of 4 BL Lacertae objects (PKS0521-365, EXO0423.4-0840, PKS2005-489 and PKS2316-423) made between 1993 and 1996 with the CANGAROO 3.8m imaging Cherenkov telescope. During the period of these observations the gamma-ray energy threshold of the 3.8m telescope was ~2TeV. Searches for steady long-term emission have been made, and, inspired by the TeV flares detected from Mkn421 and Mkn501, a search on a night-by-night timescale has also been performed for each source. Comprehensive Monte Carlo simulations are used to estimate upper limits for both steady and short timescale emission., Comment: 6 pages including 2 figures

Published
1998

202. Discovery of TeV Gamma Rays from SN1006: Further Evidence for the SNR Origin of Cosmic Rays

Author

Tanimori, T., Hayami, Y., Kamei, S., Dazeley, S. A., Edwards, P. G., Gunji, S., Hara, S., Hara, T., Holder, J., Kawachi, A., Kifune, T., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Matsuoka, T., Mizumoto, Y., Mori, M., Moriya, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Oda, S., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sakurazawa, K., Sako, T., Sato, Y., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.

Subjects
Astrophysics
Abstract

This paper reports the first discovery of TeV gamma-ray emission from a supernova remnant made with the CANGAROO 3.8 m Telescope. TeV gamma rays were detected at the sky position and extension coincident with the north-east (NE) rim of shell-type Supernova remnant (SNR) SN1006 (Type Ia). SN1006 has been a most likely candidate for an extended TeV Gamma-ray source, since the clear synchrotron X-ray emission from the rims was recently observed by ASCA (Koyama et al. 1995), which is a strong evidence of the existence of very high energy electrons up to hundreds of TeV in the SNR. The observed TeV gamma-ray flux was $(2.4\pm 0.5(statistical) \pm 0.7(systematic)) \times 10^{-12}$ cm$^{-2}$ s$^{-1}$ ($\ge 3.0\pm 0.9$ TeV) and $ (4.6\pm 0.6 \pm 1.4) \times 10^{-12}$ cm$^{-2}$ s$^{-1}$ ($\ge 1.7\pm 0.5$ TeV) from the 1996 and 1997 observations, respectively. Also we set an upper limit on the TeV gamma-ray emission from the SW rim, estimated to be $ 1.1 \times 10^{-12}$ cm$^{-2}$ s$^{-1}$ ($\ge 1.7\pm 0.5$ TeV, 95% CL) in the 1997 data. The TeV gamma rays can be attributed to the 2.7 K cosmic background photons up-scattered by electrons of energies up to about 10$^{14}$ eV by the inverse Compton (IC) process. The observed flux of the TeV gamma rays, together with that of the non-thermal X-rays, gives firm constraints on the acceleration process in the SNR shell; a magnetic field of $6.5\pm2$ $\mu$G is inferred from both the synchrotron X-rays and inverse Compton TeV gamma-rays, which gives entirely consistent mechanisms that electrons of energies up to 10$^{14}$ eV are produced via the shock acceleration in SN1006., Comment: 17 pages, 3 figures, LaTeX2.09 with AASTeX 4.0 maros, to appear in Astrophys. J. Lett

Published
1998
Full Text
View/download PDF

207. Detection of Gamma Rays of Up to 50 TeV From the Crab Nebula

Author

Tanimori, T., Sakurazawa, K., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Kamei, S., Kita, R., Kifune, T., Konishi, T., Masaike, A., Matsubara, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.

Subjects
Astrophysics
Abstract

Gamma rays with energies greater than 7 TeV from the Crab pulsar/nebula have been observed at large zenith angles, using the Imaging Atmospheric Technique from Woomera, South Australia. CANGAROO data taken in 1992, 1993 and 1995 indicate that the energy spectrum extends up to at least 50 TeV, without a change of the index of the power law spectrum. The observed differential spectrum is \noindent $(2.01\pm 0.36)\times 10^{-13}(E/{7 TeV})^{-2.53 \pm 0.18} TeV^{-1}cm^{-2}s^{-1}$ between 7 TeV and 50 TeV. There is no apparent cut-off. The spectrum for photon energies above $\sim$10 TeV allows the maximum particle acceleration energy to be inferred, and implies that this unpulsed emission does not originate near the light cylinder of the pulsar, but in the nebula where the magnetic field is not strong enough to allow pair creation from the TeV photons. The hard gamma-ray energy spectrum above 10 TeV also provides information about the varying role of seed photons for the inverse Compton process at these high energies, as well as a possible contribution of $\pi ^{\circ}$-gamma rays from proton collisions., Comment: 19 pages, 4 figures, LaTeX2.09 with AASTeX 4.0 maros, to appear in Astrophys. J. Lett

Published
1997
Full Text
View/download PDF

208. Very High Energy Gamma Rays from the Vela Pulsar Direction

Author

Yoshikoshi, T., Kifune, T., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Kakimoto, F., Konishi, T., Masaike, A., Matsubara, Y., Matsuoka, T., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Oda, S., Ogio, S., Ohsaki, T., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Sakurazawa, K., Susukita, R., Suzuki, A., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., and Yoshida, T.

Subjects
Astrophysics
Abstract

We have observed the Vela pulsar region at TeV energies using the 3.8 m imaging Cherenkov telescope near Woomera, South Australia between January 1993 and March 1995. Evidence of an unpulsed gamma-ray signal has been detected at the 5.8 sigma level. The detected gamma-ray flux is (2.9 +/- 0.5 +/- 0.4) x 10^-12 photons cm^-2 sec^-1 above 2.5 +/- 1.0 TeV and the signal is consistent with steady emission over the two years. The gamma-ray emission region is offset from the Vela pulsar position to the southeast by about 0.13 deg. No pulsed emission modulated with the pulsar period has been detected and the 95 % confidence flux upper limit to the pulsed emission from the pulsar is (3.7 +/- 0.7) x 10^-13 photons cm^-2 sec^-1 above 2.5 +/- 1.0 TeV., Comment: 18 pages, 3 figures, LaTeX with AASTeX, accepted for publication in ApJ Letters

Published
1997
Full Text
View/download PDF

209. Observations of Pulsars, PSR 1509-58 and PSR 1259-63, by CANGAROO 3.8 m Telescope

Author

Sako, T., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Kamei, S., Kifune, T., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Matsuoka, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sakurazawa, K., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.

Subjects
Astrophysics
Abstract

The data for VHE (~TeV) gamma rays from young gamma-ray pulsar PSR1509-58 observed in 1996 with the CANGAROO 3.8m Cerenkov imaging telescope are presented, as well as the additional data from March to June of 1997. The high spin-down luminosity of the pulsar and the plerionic feature around the pulsar observed with radio and X-rays suggest that VHE gamma-ray emission is quite likely above the sensitivity of the CANGAROO telescope. The CANGAROO results on other pulsars, such as PSR1259-63, are also presented. PSR1259-63 is a highly eccentric X-ray binary system, which includes a high mass Be companion star, and a preliminary analysis on the data taken 4 months after the periastron in 1994 suggests emission of VHE gamma rays., Comment: 4 pages, 1 figure, LaTeX 2.09 with epsfig.sty, wrapfig.sty to appear in proceedings of the 25th ICRC, Durban, 1997

Published
1997

210. TeV Gamma-ray Observations of Southern AGN with the CANGAROO 3.8m Telescople

Author

Roberts, M. D., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Kamei, S., Kifune, T., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Rowell, G. P., Sako, T., Sakurazawa, K., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.

Subjects
Astrophysics
Abstract

Since 1992 the CANGAROO 3.8m imaging telescope has been used to search for sources of TeV gamma-rays. Results are presented here for observations of four Southern Hemisphere BL-Lacs - PKS0521-365, PKS2316-423, PKS2005-489 and EXO0423-084. In addition to testing for steady DC emission, a night by night burst excess search has been performed for each source., Comment: 4 pages, 1 figure, LaTeX 2e with epsfig.sty, wrapfig.sty to appear in proceedings of the 25th ICRC, Durban, 1997

Published
1997

211. Very High Energy Gamma Rays from the Vela Pulsar/Nebula

Author

Yoshikoshi, T., Kifune, T., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Kamei, S., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Sakurazawa, K., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., and Yoshida, T.

Subjects
Astrophysics
Abstract

We have observed the Vela pulsar region at TeV energies using the 3.8 m imaging Cherenkov telescope near Woomera, South Australia every year since 1992. This is the first concerted search for pulsed and unpulsed emission from the Vela region, and the imaging technique also allows the location of the emission within the field of view to be examined. A significant excess of gamma-ray-like events is found offset from the Vela pulsar to the southeast by about 0.13deg. The excess shows the behavior expected of gamma-ray images when the asymmetry cut is applied to the data. There is no evidence for the emission being modulated with the pulsar period -- in contrast to earlier claims of signals from the Vela pulsar direction., Comment: 4 pages, 2 figure, LaTeX2.09 with epsfig.sty, to appear in proceedings of the 25th ICRC, Durban, 1997

Published
1997

212. TeV Gamma Ray Emission from Southern Sky Objects and CANGAROO Project

Author

Kifune, T., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Kamei, S., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Matsuoka, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Sakurazawa, K., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.

Subjects
Astrophysics
Abstract

We report recent results of the CANGAROO Collaboration on very high energy gamma ray emission from pulsars, their nebulae, SNR and AGN in the southern sky. Observations are made in South Australia using the imaging technique of detecting atmospheric Cerenkov light from gamma rays higher than about 1 TeV. The detected gamma rays are most likely produced by the inverse Compton process by electrons which also radiate synchrotron X-rays. Together with information from longer wavelengths, our results can be used to infer the strength of magnetic field in the emission region of gamma rays as well as the energy of the progenitor electrons. A description of the CANGAROO project is also given, as well as details of the new telescope of 7 m diameter which is scheduled to be in operation within two years., Comment: 5 pages, 1 figure, LaTeX 2.09 with aipproc.sty & epsfig.sty, to appear in proceedings of the 4th Compton Symposium, Williamsburg, 1997

Published
1997
Full Text
View/download PDF

213. Observation of Spectrum of TeV Gamma Rays up to 60 TeV from the Crab at the Large Zenith Angles

Author

Sakurazawa, K., Tanimori, T., Dazeley, S. A., Edwards, P. G., Hara, T., Kamei, S., Kifune, T., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Matsuoka, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.

Subjects
Astrophysics
Abstract

The CANGAROO experiment has observed gamma-ray above 7TeV from the Crab pulsar/nebula at large zenith angle in Woomera, South Australia. We report the CANGAROO data taken in 1992, 1993 and 1995, from which it appears that the energy spectrum extends at least up to 50 TeV. The observed integral spectrum is (8.4+-1.0) x 10^{-13}(E/7 TeV)^(-1.53+-0.15)cm^{-2}s^{-1} between 7 TeV and 50 TeV. In November 1996, the 3.8m mirror was recoated in Australia, and its reflectivity was improved to be about 90% as twice as before. Due to this recoating, the threshold energy of ~4 TeV for gamma rays has been attained in the observation of the Crab at large zenith angle. Here we also report the preliminary result taken in 1996., Comment: 4 pages, 2 figures, LaTeX 2.09 with epsfig.sty, to appear in proceedings of the 25th ICRC, Durban, 1997

Published
1997

216. IDegLira for the Real-World Treatment of Type 2 Diabetes in Italy: Protocol and Interim Results from the REX Observational Study

Author

Fadini, G, Buzzetti, R, Fittipaldi, M, D'Incau, F, Da Porto, A, Girelli, A, Simoni, L, Lastoria, G, Consoli, A, Iazzetta, N, Di Giovanni, G, Carbonara, O, Aragiusto, C, Carleo, D, Da Rosa, N, Martedi, E, Landolfi, L, Marracino, M, Tortora, A, De Morelli, G, Casarsa, V, Maddaloni, E, Siena, A, Pitocco, D, Tartaglione, L, Rizzi, A, Leonetti, F, Fasolo, M, Morsello, G, Bulzomi, R, Ruga, G, Bianconi, A, Torre, E, Rebora, A, Cecoli, F, Monti, E, Bonfadini, S, Dotti, S, Madaschi, S, Trevisan, R, Albizzi, M, Bellante, R, Corsi, A, Scaranna, C, De Cata, P, Liboa, F, Ghilotti, S, Tortato, E, Lanari, L, Turchi, F, Gabellieri, E, Lamacchia, O, Colucci, C, Mileti, G, Coluzzi, S, Carrieri, F, Rossetti, P, Anzaldi, M, Di Benedetto, A, Ruggeri, D, Scatena, A, Ranchelli, A, Ragusa, I, Gregori, G, Crisci, I, Mori, M, Baccetti, F, Anichini, R, Salutini, E, Vinci, C, Colletti, I, Zanon, M, Altomari, A, Bonora, B, Fadini G. P., Buzzetti R., Fittipaldi M. R., D'Incau F., Da Porto A., Girelli A., Simoni L., Lastoria G., Consoli A., Iazzetta N., Di Giovanni G., Carbonara O., Aragiusto C., Carleo D., Da Rosa N., Martedi E., Landolfi L., Marracino M., Tortora A., De Morelli G., Casarsa V., Maddaloni E., Siena A., Pitocco D., Tartaglione L., Rizzi A., Leonetti F., Fasolo M., Morsello G., Bulzomi R., Ruga G., Bianconi A., Torre E., Rebora A., Cecoli F., Monti E., Bonfadini S., Dotti S., Madaschi S., Trevisan R., Albizzi M., Bellante R., Corsi A., Scaranna C., De Cata P., Liboa F., Ghilotti S., Tortato E., Lanari L., Turchi F., Gabellieri E., Lamacchia O., Colucci C., Mileti G., Coluzzi S., Carrieri F., Rossetti P., Anzaldi M., Di Benedetto A., Ruggeri D., Scatena A., Ranchelli A., Ragusa I., Gregori G., Crisci I., Mori M., Baccetti F., Anichini R., Salutini E., Vinci C., Colletti I., Zanon M. S., Altomari A., Bonora B. M., Fadini, G, Buzzetti, R, Fittipaldi, M, D'Incau, F, Da Porto, A, Girelli, A, Simoni, L, Lastoria, G, Consoli, A, Iazzetta, N, Di Giovanni, G, Carbonara, O, Aragiusto, C, Carleo, D, Da Rosa, N, Martedi, E, Landolfi, L, Marracino, M, Tortora, A, De Morelli, G, Casarsa, V, Maddaloni, E, Siena, A, Pitocco, D, Tartaglione, L, Rizzi, A, Leonetti, F, Fasolo, M, Morsello, G, Bulzomi, R, Ruga, G, Bianconi, A, Torre, E, Rebora, A, Cecoli, F, Monti, E, Bonfadini, S, Dotti, S, Madaschi, S, Trevisan, R, Albizzi, M, Bellante, R, Corsi, A, Scaranna, C, De Cata, P, Liboa, F, Ghilotti, S, Tortato, E, Lanari, L, Turchi, F, Gabellieri, E, Lamacchia, O, Colucci, C, Mileti, G, Coluzzi, S, Carrieri, F, Rossetti, P, Anzaldi, M, Di Benedetto, A, Ruggeri, D, Scatena, A, Ranchelli, A, Ragusa, I, Gregori, G, Crisci, I, Mori, M, Baccetti, F, Anichini, R, Salutini, E, Vinci, C, Colletti, I, Zanon, M, Altomari, A, Bonora, B, Fadini G. P., Buzzetti R., Fittipaldi M. R., D'Incau F., Da Porto A., Girelli A., Simoni L., Lastoria G., Consoli A., Iazzetta N., Di Giovanni G., Carbonara O., Aragiusto C., Carleo D., Da Rosa N., Martedi E., Landolfi L., Marracino M., Tortora A., De Morelli G., Casarsa V., Maddaloni E., Siena A., Pitocco D., Tartaglione L., Rizzi A., Leonetti F., Fasolo M., Morsello G., Bulzomi R., Ruga G., Bianconi A., Torre E., Rebora A., Cecoli F., Monti E., Bonfadini S., Dotti S., Madaschi S., Trevisan R., Albizzi M., Bellante R., Corsi A., Scaranna C., De Cata P., Liboa F., Ghilotti S., Tortato E., Lanari L., Turchi F., Gabellieri E., Lamacchia O., Colucci C., Mileti G., Coluzzi S., Carrieri F., Rossetti P., Anzaldi M., Di Benedetto A., Ruggeri D., Scatena A., Ranchelli A., Ragusa I., Gregori G., Crisci I., Mori M., Baccetti F., Anichini R., Salutini E., Vinci C., Colletti I., Zanon M. S., Altomari A., and Bonora B. M.

Abstract

Introduction: IDegLira was shown to maintain glycemic control while reducing risk of hypoglycemia and body weight gain. The REX study was designed to generate real-world evidence on the use of IDegLira in Italian clinical practice in two different subgroups of patients, those switching to IDegLira from a basal insulin-supported oral therapy (BOT group) and those from a basal plus bolus insulin regimen (BB group). Methods: Adult patients with T2D diagnosed for at least 12 months and having started IDegLira 2–3 months prior to enrolment, coming from a BOT or BB regimen, were enrolled in this multicenter observational prospective cohort study conducted in 28 Italian centers. This paper presents the methodological framework of the REX study and provides the interim analysis results describing the patients’ baseline characteristics and the clinical reasons for IDegLira treatment initiation. Results: Of the 360 patients enrolled in the REX study, 331 were considered eligible for this interim analysis, 76.4% in the BOT and 23.6% in the BB group. Mean (SD) HbA1c was 8.5% (1.4) in the BOT and 8.2% (1.7) in the BB group. The most common T2D complications were diabetic macroangiopathy and diabetic nephropathy in both groups. The median (interquartile range) insulin daily dose before IDegLira was 15.0 (10.0–20.0) units in the BOT group and 42 (30.0–52.0) in the BB group. Oral antidiabetics were taken by 98% and 51.3% of patients, respectively. The main reason for switching to IDegLira was the inadequate glycemic control in the BOT group (86% of patients), and the intent to simplify the treatment in the BB group (66.7%). Conclusions: IdegLira is initiated after BOT in inadequately controlled patients to improve glycemic control, whereas in BB patients it is used to simplify the therapeutic regimen. Final results of the REX study will shed light on patients’ outcomes after IdegLira treatment under routine clinical care.

Published
2022

218. OP0128 PHARMACOKINETICS AND PHARMACODYNAMICS OF METHOTREXATE POLYGLUTAMATE IN PATIENTS WITH RHEUMATOID ARTHRITIS TREATED WITH LOW OR HIGH DOSE-METHOTREXATE IN COMBINATION WITH ADALIMUMAB: RESULTS FROM THE MIRACLE TRIAL

Author

Tamai, H., primary, Ikeda, K., additional, Miyamoto, T., additional, Taguchi, H., additional, Kuo, C. F., additional, Shin, K., additional, Hirata, S., additional, Okano, Y., additional, Sato, S., additional, Yasuoka, H., additional, Choi, I. A., additional, Park, S. H., additional, Weng, M. Y., additional, Kuwana, M., additional, Lee, Y. J., additional, Ishii, T., additional, Kim, J., additional, Kameda, H., additional, Kojima, T., additional, Baek, H. J., additional, Hsu, P. N., additional, Huang, C. M., additional, Cheng, T. T., additional, Sung, W. Y., additional, Tsai, W. C., additional, Taninaga, T., additional, Mori, M., additional, Miyagishi, H., additional, Sato, Y., additional, Takeuchi, T., additional, and Kaneko, Y., additional

Published
2023
Full Text
View/download PDF

219. POS0760 LONG-TERM PROGNOSTIC FOLLOW-UP OF PATIENTS WITH REFRACTORY SYSTEMIC JUVENILE IDIOPATHIC ARTHRITIS AFTER THE CLINICAL TRIAL OF TOCILIZUMAB AS A FIRST-LINE BIOLOGIC TREATMENT

Author

Miyamae, T., primary, Kawabe, T., additional, Nishimura, K., additional, Hattori, S., additional, Imagawa, T., additional, Ishii, T., additional, Ito, S., additional, Iwata, N., additional, Kamata, Y., additional, Kamiyama, Y., additional, Mizuta, M., additional, Mori, M., additional, Murase, A., additional, Nakagishi, Y., additional, Nakano, T., additional, Nakayamada, S., additional, Nozawa, T., additional, Ohya, T., additional, Okamoto, N., additional, Sato, K., additional, Sugita, Y., additional, Takei, S., additional, Tanaka, Y., additional, Tomiita, M., additional, Umebayashi, H., additional, Yamasaki, Y., additional, Nishimoto, N., additional, and Yokota, S., additional

Published
2023
Full Text
View/download PDF

221. 602 Efficacy of autologous cell-based therapy for male and female pattern hair loss using dermal sheath cup cells: A single arm, multi-center, confirmatory clinical study

Author

Harada, K., primary, Ohyama, M., additional, Niiyama, S., additional, Irisawa, R., additional, Mae, K., additional, Mori, M., additional, Wakimoto, H., additional, Kinoshita-Ise, M., additional, Fukuyama, M., additional, Hayakawa, R., additional, Takagi, M., additional, Yamazaki, M., additional, Miyoshi, M., additional, Nishikawa, S., additional, Sato, S., additional, Nakazawa, Y., additional, Sugimoto, T., additional, Ogo, M., additional, and Tsuboi, R., additional

Published
2023
Full Text
View/download PDF

222. Clinical Course and Typical Chest CT Findings of Olaparib-induced Lung Injury: A Case Series

Author

Hattori, M., primary, Sato, M., additional, Mikami, Y., additional, Fujii, K., additional, Horiguchi, Y., additional, Shuzui, M., additional, Fukuda, K., additional, Miyamoto, Y., additional, Mori, M., additional, Hinata, M., additional, Kawakami, M., additional, Mitani, A., additional, Tanaka, G., additional, Kage, H., additional, and Nagase, T., additional

Published
2023
Full Text
View/download PDF

223. PD-0232 Skin Dose Predictors of Early-Late Reactions after Whole Breast RT in a Single-Center Large-Cohort

Author

Cicchetti, A., primary, Fodor, A., additional, Mangili, P., additional, Mori, M., additional, Chiara, A., additional, Deantoni, C., additional, Pasetti, M., additional, Palazzo, G., additional, Ubeira-Gabellin, M.G., additional, Rancati, T., additional, Del Vecchio, A., additional, Di Muzio, N.G., additional, and Fiorino, C., additional

Published
2023
Full Text
View/download PDF

226. A sub-Neptune transiting the young field star HD 18599 at 40 pc

Author

de Leon, J P, primary, Livingston, J H, additional, Jenkins, J S, additional, Vines, J I, additional, Wittenmyer, R A, additional, Clark, J T, additional, Winn, J I M, additional, Addison, B, additional, Ballard, S, additional, Bayliss, D, additional, Beichman, C, additional, Benneke, B, additional, Berardo, D A, additional, Bowler, B P, additional, Brown, T, additional, Bryant, E M, additional, Christiansen, J, additional, Ciardi, D, additional, Collins, K A, additional, Collins, K I, additional, Crossfield, I, additional, Deming, D, additional, Dragomir, D, additional, Dressing, C D, additional, Fukui, A, additional, Gan, T, additional, Giacalone, S, additional, Gill, S, additional, Gorjian, V, additional, González Alvarez, E, additional, Hesse, K, additional, Horner, J, additional, Howell, S B, additional, Jenkins, J M, additional, Kane, S R, additional, Kendall, A, additional, Kielkopf, J F, additional, Kreidberg, L, additional, Latham, D W, additional, Liu, H, additional, Lund, M B, additional, Matson, R, additional, Matthews, E, additional, Mengel, M W, additional, Morales, F, additional, Mori, M, additional, Narita, N, additional, Nishiumi, T, additional, Okumura, J, additional, Plavchan, P, additional, Quinn, S, additional, Rabus, M, additional, Ricker, G, additional, Rudat, A, additional, Schlieder, J, additional, Schwarz, R P, additional, Seager, S, additional, Shporer, A, additional, Smith, A M S, additional, Stassun, K, additional, Tamura, M, additional, Tan, T G, additional, Tinney, C, additional, Vanderspek, R, additional, Werner, M W, additional, West, R G, additional, Wright, D, additional, Zhang, H, additional, and Zhou, G, additional

Published
2023
Full Text
View/download PDF

230. Measurement of the cosmogenic neutron yield in Super-Kamiokande with gadolinium loaded water

Author

Shinoki, M., Abe, K., Hayato, Y., Hiraide, K., Hosokawa, K., Ieki, K., Ikeda, M., Kameda, J., Kanemura, Y., Kaneshima, R., Kashiwagi, Y., Kataoka, Y., Miki, S., Mine, S., Miura, M., Moriyama, S., Nakano, Y., Nakahata, M., Nakayama, S., Noguchi, Y., Okamoto, K., Sato, K., Sekiya, H., Shiba, H., Shimizu, K., Shiozawa, M., Sonoda, Y., Suzuki, Y., Takeda, A., Takemoto, Y., Takenaka, A., Tanaka, H., Watanabe, S., Yano, T., Han, S., Kajita, T., Okumura, K., Tashiro, T., Tomiya, T., Wang, X., Yoshida, S., Megias, G. D., Fernandez, P., Labarga, L., Ospina, N., Zaldivar, B., Pointon, B. W., Kearns, E., Raaf, J. L., Wan, L., Wester, T., Bian, J., Griskevich, N. J., Kropp, W. R., Locke, S., Smy, M. B., Sobel, H. W., Takhistov, V., Yankelevich, A., Hill, J., Lee, S. H., Moon, D. H., Park, R. G., Bodur, B., Scholberg, K., Walter, C. W., Beauchêne, A., Bernard, L., Coffani, A., Drapier, O., El Hedri, S., Giampaolo, A., Mueller, Th A., Santos, A. D., Paganini, P., Quilain, B., Ishizuka, T., Nakamura, T., Jang, J. S., Learned, J. G., Choi, K., Cao, S., Anthony, L. H. V., Martin, D., Scott, M., Sztuc, A. A., Uchida, Y., Berardi, V., Catanesi, M. G., Radicioni, E., Calabria, N. F., Langella, A., Machado, L. N., Rosa, G., Collazuol, G., Iacob, F., Lamoureux, M., Mattiazzi, M., Ludovici, L., Gonin, M., Pronost, G., Fujisawa, C., Maekawa, Y., Nishimura, Y., Akutsu, R., Friend, M., Takuya Hasegawa, Ishida, T., Kobayashi, T., Jakkapu, M., Matsubara, T., Nakadaira, T., Nakamura, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Bhuiyan, N., Boschi, T., Burton, G. T., Di Lodovico, F., Gao, J., Goldsack, A., Katori, T., Migenda, J., Taani, M., Xie, Z., Zsoldos, S., Kotsar, Y., Ozaki, H., Suzuki, A. T., Takeuchi, Y., Bronner, C., Feng, J., Kikawa, T., Mori, M., Nakaya, T., Wendell, R. A., Yasutome, K., Jenkins, S. J., Mccauley, N., Mehta, P., Tarrant, A., Tsui, K. M., Fukuda, Y., Itow, Y., Menjo, H., Ninomiya, K., Lagoda, J., Lakshmi, S. M., Mandal, M., Mijakowski, P., Prabhu, Y. S., Zalipska, J., Jia, M., Jiang, J., Jung, C. K., Wilking, M. J., Yanagisawa, C., Harada, M., Ishino, H., Ito, S., Kitagawa, H., Koshio, Y., Nakanishi, F., Sakai, S., Barr, G., Barrow, D., Cook, L., Samani, S., Wark, D., Holin, A., Nova, F., Yang, J. Y., Yang, B. S., Yoo, J., Fannon, J. E. P., Kneale, L., Kneal, K., Malek, M., Mcelwee, J. M., Stone, O., Thiesse, M. D., Thompson, L. F., Okazawa, H., Kim, S. B., Kwon, E., Seo, J. W., Yu, I., Ichikawa, A. K., Nakamura, K. D., Tairafune, S., Nishijima, K., Koshiba, M., Iwamoto, K., Nakagiri, K., Nakajima, Y., Shima, S., Taniuchi, N., Yokoyama, M., Martens, K., Perio, P., Vagins, M. R., Xia, J., Kuze, M., Izumiyama, S., Inomoto, M., Ishitsuka, M., Ito, H., Kinoshita, T., Matsumoto, R., Ommura, Y., Shigeta, N., Suganuma, T., Yamauchi, K., Martin, J. F., Tanaka, H. A., Towstego, T., Gaur, R., Gousy-Leblanc, V., Hartz, M., Konaka, A., Li, X., Prouse, N. W., Chen, S., Xu, B. D., Zhang, B., Posiadala-Zezula, M., Boyd, S. B., Hadley, D., Nicholson, M., O Flaherty, M., Richards, B., Ali, A., Jamieson, B., Marti, Ll, Minamino, A., Pintaudi, G., Sano, S., Suzuki, S., Wada, K., and HEP, INSPIRE

Subjects
muon: energy, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], background, water, FOS: Physical sciences, showers: hadronic, KAMIOKANDE, n: yield: measured, High Energy Physics - Experiment, n: neutrinoproduction, High Energy Physics - Experiment (hep-ex), efficiency, radioactivity, muon: cosmic radiation, fission, gadolinium, experimental results
Abstract

Cosmic-ray muons that enter the Super-Kamiokande detector cause hadronic showers due to spallation in water, producing neutrons and radioactive isotopes. Those are a major background source for studies of MeV-scale neutrinos and searches for rare events. Since 2020, gadolinium was introduced in the ultra-pure water in the Super-Kamiokande detector to improve the detection efficiency of neutrons. In this study, the cosmogenic neutron yield was measured using data acquired during the period after the gadolinium loading. The yield was found to be $(2.76 \pm 0.02\,\mathrm{(stat.) \pm 0.19\,\mathrm{(syst.)}}) \times 10^{-4}\,\mu^{-1} \mathrm{g^{-1} cm^{2}}$ at 259 GeV of average muon energy at the Super-Kamiokande detector., Comment: 10 pages, 10 figures, 3 tables

Published
2023

231. Infrared multispectral monitoring of cereal crops

Author

Rippa M., Curcio R., Di Mola I., Ottaiano L., Cozzolino E., Mori M., Mormile P., Rippa, M., Curcio, R., Di Mola, I., Ottaiano, L., Cozzolino, E., Mori, M., and Mormile, P.

Subjects
Thermography, Cereal, Precision Agriculture, Plant Stre, Digital Agriculture, Infrared Imaging
Abstract

Plants are subjected to a wide range of stresses which reduces the productivity of agricultural crops. In the case of cereal cultivations, climate change impacts on their production mainly through abiotic and biotic stress due for example to heat and water stress but also to pathogens such as bacteria, fungi, nematodes and others. The area under cereal cultivation is increasing worldwide, but, due to these problems, the current rates of yield growth and overall production are not enough to satisfy future demand. For this motivation, there is the needs to monitor and to control the cultivations, also developing new technological solutions useful to better optimize the management strategies, increasing both the quality of products and the quantity of the annual cereal harvest. Infrared imaging is a well-known non-invasive and non-contact technique that represents an outstanding approach of analysis applied in many fields: engineering, medicine, veterinary, cultural heritage and others. In recent years it has been gaining great interest in agriculture as it is well suited to the emerging needs of the precision agriculture management strategies. In this work, we performed an in-field multispectral infrared monitoring of different cereal crops (durum wheat and common wheat) through the use of both LWIR and MWIR cameras. The monitoring carried out made it possible to identify, among the crops analyzed, those subject to higher stress levels and their response to the different spectral ranges used. The results obtained open to the possibility of identifying new figures of merit useful for an effective monitoring of cereal crops and measurable through remote instrumentation.

Published
2022

232. Search for proton decay via <math><mi>p</mi><mo>→</mo><msup><mi>μ</mi><mo>+</mo></msup><msup><mi>K</mi><mn>0</mn></msup></math> in 0.37 megaton-years exposure of Super-Kamiokande

Author

Matsumoto, R., Abe, K., Hayato, Y., Hiraide, K., Ieki, K., Ikeda, M., Kameda, J., Kanemura, Y., Kaneshima, R., Kashiwagi, Y., Kataoka, Y., Miki, S., Mine, S., Miura, M., Moriyama, S., Nakano, Y., Nakahata, M., Nakayama, S., Noguchi, Y., Okamoto, K., Sato, K., Sekiya, H., Shiba, H., Shimizu, K., Shiozawa, M., Sonoda, Y., Suzuki, Y., Takeda, A., Takemoto, Y., Takenaka, A., Tanaka, H., Watanabe, S., Yano, T., Han, S., Kajita, T., Okumura, K., Tashiro, T., Tomiya, T., Wang, X., Xia, J., Yoshida, S., Megias, G. D., Fernandez, P., Labarga, L., Ospina, N., Zaldivar, B., Pointon, B. W., Kearns, E., Raaf, J. L., Wan, L., Wester, T., Bian, J., Griskevich, N. J., Kropp, W. R., Locke, S., Smy, M. B., Sobel, H. W., Takhistov, V., Yankelevich, A., Hill, J., Kim, J. Y., Lim, I. T., Park, R. G., Bodur, B., Scholberg, K., Walter, C. W., Bernard, L., Coffani, A., Drapier, O., El Hedri, S., Giampaolo, A., Mueller, Th. A., Santos, A. D., Paganini, P., Quilain, B., Ishizuka, T., Nakamura, T., Jang, J. S., Learned, J. G., Choi, K., Cao, S., Anthony, L. H. V., Martin, D., Scott, M., Sztuc, A. A., Uchida, Y., Berardi, V., Catanesi, M. G., Radicioni, E., Calabria, Nicola, Nascimento Machado, L., De Rosa, G., Collazuol, G., Iacob, F., Lamoureux, M., Mattiazzi, M., Ludovici, L., Gonin, M., Pronost, G., Fujisawa, C., Maekawa, Y., Nishimura, Y., Friend, M., Hasegawa, T., Ishida, T., Kobayashi, T., Jakkapu, M., Matsubara, T., Nakadaira, T., Nakamura, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Boschi, T., Di Lodovico, F., Gao, J., Goldsack, A., Katori, T., Migenda, J., Taani, M., Xie, Z., Zsoldos, S., Kotsar, Y., Ozaki, H., Suzuki, A. T., Takeuchi, Y., Yamamoto, S., Bronner, C., Feng, J., Kikawa, T., Mori, M., Nakaya, T., Wendell, R. A., Yasutome, K., Jenkins, S. J., McCauley, N., Mehta, P., Tsui, K. M., Tarrant, A., Fukuda, Y., Itow, Y., Menjo, H., Ninomiya, K., Lagoda, J., Lakshmi, S. M., Mandal, M., Mijakowski, P., Prabhu, Y. S., Zalipska, J., Jia, M., Jiang, J., Jung, C. K., Wilking, M. J., Yanagisawa, C., Harada, M., Ishino, H., Ito, S., Kitagawa, H., Koshio, Y., Ma, W., Nakanishi, F., Sakai, S., Barr, G., Barrow, D., Cook, L., Samani, S., Wark, D., Holin, A., Nova, F., Yang, J. Y., Malek, M., McElwee, J. M., Stone, O., Thiesse, M. D., Thompson, L. F., Okazawa, H., Kim, S. B., Kwon, E., Seo, J. W., Yu, I., Ichikawa, A. K., Nakamura, K. D., Tairafune, S., Nishijima, K., Koshiba, M., Iwamoto, K., Nakagiri, K., Nakajima, Y., Shima, S., Taniuchi, N., Yokoyama, M., Martens, K., de Perio, P., Vagins, M. R., Kuze, M., Izumiyama, S., Inomoto, M., Ishitsuka, M., Ito, H., Kinoshita, T., Ommura, Y., Shigeta, N., Shinoki, M., Suganuma, T., Yamauchi, K., Martin, J. F., Tanaka, H. A., Towstego, T., Akutsu, R., Gousy-Leblanc, V., Hartz, M., Konaka, A., Li, X., Prouse, N. W., Chen, S., Xu, B. D., Zhang, B., Posiadala-Zezula, M., Boyd, S. B., Hadley, D., Nicholson, M., O’Flaherty, M., Richards, B., Ali, A., Jamieson, B., Marti, Ll., Minamino, A., Pintaudi, G., Sano, S., Suzuki, S., Wada, K., Matsumoto, R., Abe, K., Hayato, Y., Hiraide, K., Ieki, K., Ikeda, M., Kameda, J., Kanemura, Y., Kaneshima, R., Kashiwagi, Y., Kataoka, Y., Miki, S., Mine, S., Miura, M., Moriyama, S., Nakano, Y., Nakahata, M., Nakayama, S., Noguchi, Y., Okamoto, K., Sato, K., Sekiya, H., Shiba, H., Shimizu, K., Shiozawa, M., Sonoda, Y., Suzuki, Y., Takeda, A., Takemoto, Y., Takenaka, A., Tanaka, H., Watanabe, S., Yano, T., Han, S., Kajita, T., Okumura, K., Tashiro, T., Tomiya, T., Wang, X., Xia, J., Yoshida, S., Megias, G. D., Fernandez, P., Labarga, L., Ospina, N., Zaldivar, B., Pointon, B. W., Kearns, E., Raaf, J. L., Wan, L., Wester, T., Bian, J., Griskevich, N. J., Kropp, W. R., Locke, S., Smy, M. B., Sobel, H. W., Takhistov, V., Yankelevich, A., Hill, J., Kim, J. Y., Lim, I. T., Park, R. G., Bodur, B., Scholberg, K., Walter, C. W., Bernard, L., Coffani, A., Drapier, O., El Hedri, S., Giampaolo, A., Mueller, Th. A., Santos, A. D., Paganini, P., Quilain, B., Ishizuka, T., Nakamura, T., Jang, J. S., Learned, J. G., Choi, K., Cao, S., Anthony, L. H. V., Martin, D., Scott, M., Sztuc, A. A., Uchida, Y., Berardi, V., Catanesi, M. G., Radicioni, E., Calabria, Nicola, Nascimento Machado, L., De Rosa, G., Collazuol, G., Iacob, F., Lamoureux, M., Mattiazzi, M., Ludovici, L., Gonin, M., Pronost, G., Fujisawa, C., Maekawa, Y., Nishimura, Y., Friend, M., Hasegawa, T., Ishida, T., Kobayashi, T., Jakkapu, M., Matsubara, T., Nakadaira, T., Nakamura, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Boschi, T., Di Lodovico, F., Gao, J., Goldsack, A., Katori, T., Migenda, J., Taani, M., Xie, Z., Zsoldos, S., Kotsar, Y., Ozaki, H., Suzuki, A. T., Takeuchi, Y., Yamamoto, S., Bronner, C., Feng, J., Kikawa, T., Mori, M., Nakaya, T., Wendell, R. A., Yasutome, K., Jenkins, S. J., Mccauley, N., Mehta, P., Tsui, K. M., Tarrant, A., Fukuda, Y., Itow, Y., Menjo, H., Ninomiya, K., Lagoda, J., Lakshmi, S. M., Mandal, M., Mijakowski, P., Prabhu, Y. S., Zalipska, J., Jia, M., Jiang, J., Jung, C. K., Wilking, M. J., Yanagisawa, C., Harada, M., Ishino, H., Ito, S., Kitagawa, H., Koshio, Y., Ma, W., Nakanishi, F., Sakai, S., Barr, G., Barrow, D., Cook, L., Samani, S., Wark, D., Holin, A., Nova, F., Yang, J. Y., Malek, M., Mcelwee, J. M., Stone, O., Thiesse, M. D., Thompson, L. F., Okazawa, H., Kim, S. B., Kwon, E., Seo, J. W., Yu, I., Ichikawa, A. K., Nakamura, K. D., Tairafune, S., Nishijima, K., Koshiba, M., Iwamoto, K., Nakagiri, K., Nakajima, Y., Shima, S., Taniuchi, N., Yokoyama, M., Martens, K., de Perio, P., Vagins, M. R., Kuze, M., Izumiyama, S., Inomoto, M., Ishitsuka, M., Ito, H., Kinoshita, T., Ommura, Y., Shigeta, N., Shinoki, M., Suganuma, T., Yamauchi, K., Martin, J. F., Tanaka, H. A., Towstego, T., Akutsu, R., Gousy-Leblanc, V., Hartz, M., Konaka, A., Li, X., Prouse, N. W., Chen, S., Xu, B. D., Zhang, B., Posiadala-Zezula, M., Boyd, S. B., Hadley, D., Nicholson, M., O’Flaherty, M., Richards, B., Ali, A., Jamieson, B., Marti, Ll., Minamino, A., Pintaudi, G., Sano, S., Suzuki, S., and Wada, K.

Abstract

We searched for proton decay via p→μ+K0 in 0.37 Mton·years of data collected between 1996 and 2018 from the Super-Kamiokande water Cherenkov experiment. The selection criteria were defined separately for KS0 and KL0 channels. No significant event excess has been observed. As a result of this analysis, which extends the previous search by an additional 0.2 Mton·years of exposure and uses an improved event reconstruction, we set a lower limit of 3.6×1033 years on the proton lifetime.

Published
2022

233. I risultati della 49a Rete nazionale coordinata dal Crea-It di Roma. Duro, le varietà consigliate

Author

Quaranta F., Arcangeli A., Mortaro R., Zefelippo M., Converso R., Gianinetti A., Reggiani F., De Montis A., Rosta R., Massi A., Mantovani P., Mariotti A., Fabbrini L., Viola P., Ruggeri R., Rossini F., Mazzon V., Belocchi A., Sestili A., Fornara M., Vecchiarelli V., Governatori C., Petrini A., Fuselli D., Santilocchi R., Bianchelli M., Mori M., Di Mola I., Ottaiano L., De Vita P., Paone S., Pecorella I., Pecchioni N., Colonna M., Rosati D. D., Tedone L., Schiavone D., De Mastro G., Preiti G., Badagliacca G., Filippelli S., Giunta F., Motzo R., Balmas V., Carboni G., Dettori M., Mameli L., Frenda A. S., Ingraffia R., Lo Porto A., Randazzo B., Salafia L., Virzì N., Leonardi A., Li Puma E., Quaranta F., Arcangeli A., Mortaro R., Zefelippo M., Converso R., Gianinetti A., Reggiani F., De Montis A., Rosta R., Massi A., Mantovani P., Mariotti A., Fabbrini L., Viola P., Ruggeri R., Rossini F., Mazzon V., Belocchi A., Sestili A., Fornara M., Vecchiarelli V., Governatori C., Petrini A., Fuselli D., Santilocchi R., Bianchelli M., Mori M., Di Mola I., Ottaiano L., De Vita P., Paone S., Pecorella I., Pecchioni N., Colonna M., Rosati D.D., Tedone L., Schiavone D., De Mastro G., Preiti G., Badagliacca G., Filippelli S., Giunta F., Motzo R., Balmas V., Carboni G., Dettori M., Mameli L., Frenda A.S., Ingraffia R., Lo Porto A., Randazzo B., Salafia L., Virzì N., Leonardi A., and Li Puma E.

Subjects
Cereali, Frumento duro, confronto varietale, Settore AGR/02 - Agronomia E Coltivazioni Erbacee
Abstract

Antalis, Rgt Natur e Marco Aurelio hanno ottenuto indici di resa uguali o superiori a 100 in tutti i 6 areali. Produzioni superiori o uguali alle medie in 5 areali su 6 sono state registrate per la novità Federico II, caratterizzata anche da buon peso ettolitrico e tenore proteico, e per Claudio.

Published
2022

240. Results from One Thousand Days of Real-Time, Directional Solar-Neutrino Data

Author

Hirata, K. S., primary, Inoue, K., additional, Kajita, T., additional, Kifune, T., additional, Kihara, K., additional, Nakahata, M., additional, Nakamura, K., additional, Ohara, S., additional, Sato, N., additional, Suzuki, Y., additional, Totsuka, Y., additional, Yaginuma, Y., additional, Mori, M., additional, Oyama, Y., additional, Suzuki, A., additional, Takahashi, K., additional, Yamada, M., additional, Koshiba, M., additional, Suda, T., additional, Tajima, T., additional, Miyano, K., additional, Miyata, H., additional, Takei, H., additional, Fukuda, Y., additional, Kodera, E., additional, Nagashima, Y., additional, Takita, M., additional, Kaneyuki, K., additional, Tanimori, T., additional, Bcicr, E. W., additional, Feldscher, L. R., additional, Frank, E. D., additional, Frati, W., additional, Kim, S. B., additional, Mann, A. K., additional, Newcomer, F. M., additional, Berg, R. Van, additional, and Zhang, W., additional

Published
2018
Full Text
View/download PDF

242. Pre-supernova alert system for super-kamiokande

Author

Kamiokande Collaboration, Machado, L. N., Abe, K., Hayato, Y., Hiraide, K., Ieki, K., Ikeda, M., Kameda, J., Kanemura, Y., Kaneshima, R., Kashiwagi, Y., Kataoka, Y., Miki, S., Mine, S., Miura, M., Moriyama, S., Nakano, Y., Nakahata, M., Nakayama, S., Noguchi, Y., Okamoto, K., Sato, K., Sekiya, H., Shiba, H., Shimizu, K., Shiozawa, M., Sonoda, Y., Suzuki, Y., Takeda, A., Takemoto, Y., Takenaka, A., Tanaka, H., Watanabe, S., Yano, T., de Perio, P., Martens, K., Vagins, M. R., Bian, J., Griskevich, N. J., Kropp, W. R., Locke, S., Smy, M. B., Sobel, H. W., Takhistov, V., Yankelevich, A., Han, S., Kajita, T., Okumura, K., Tashiro, T., Tomiya, T., Wang, X., Xia, J., Yoshida, S., Megias, G. D., Fernandez, P., Labarga, L., Ospina, N., Zaldivar, B., Pointon, B. W., Akutsu, R., Gousy-Leblanc, V., Hartz, M., Konaka, A., Prouse, N. W., Kearns, E., Raaf, J. L., Wan, L., Wester, T., Hill, J., Kim, J. Y., Lim, I. T., Park, R. G., Bodur, B., Scholberg, K., Walter, C. W., Bernard, L., Coffani, A., Drapier, O., Hedri, S. El, Giampaolo, A., Mueller, Th. A., Santos, A. D., Paganini, P., Quilain, B., Ishizuka, T., Nakamura, T., Jang, J. S., Learned, J. G., Cao, S., Choi, K., Anthony, L. H. V., Martin, D., Scott, M., Sztuc, A. A., Uchida, Y., Berardi, V., Catanesi, M. G., Radicioni, E., Calabria, N. F., De Rosa, G., Collazuol, G., Iacob, F., Lamoureux, M., Mattiazzi, M., Ludovici, L., Gonin, M., Pronost, G., Fujisawa, C., Maekawa, Y., Nishimura, Y., Sasaki, R., Friend, M., Hasegawa, T., Ishida, T., Jakkapu, M., Kobayashi, T., Matsubara, T., Nakadaira, T., Nakamura, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Boschi, T., Di Lodovico, F., Gao, J., Goldsack, A., Katori, T., Migenda, J., Taani, M., Zsoldos, S., Kotsar, Y., Ozaki, H., Suzuki, A. T., Takeuchi, Y., Yaamoto, S., Bronner, C., Feng, J., Kikawa, T., Mori, M., Nakaya, T., Wendell, R. A., Yasutome, K., Jenkins, S. J., McCauley, N., Mehta, P., Tsui, K. M., Fukuda, Y., Itow, Y., Menjo, H., Ninomiya, K., Lagoda, J., Lakshmi, S. M., Mandal, M., Mijakowski, P., Prabhu, Y. S., Zalipska, J., Jia, M., Jiang, J., Jung, C. K., Wilking, M. J., Yanagisawa, C., Harada, M., Ishino, H., Ito, S., Kitagawa, H., Koshio, Y., Ma, W., Nakanishi, F., Sakai, S., Barr, G., Barrow, D., Cook, L., Samani, S., Wark, D., Nova, F., Yang, J. Y., Malek, M., McElwee, J. M., Stone, O., Thiesse, M. D., Thompson, L. F., Okazawa, H., Kim, S. B., Seo, J. W., Yu, I., Ichikawa, A. K., Nakamura, K. D., Tairafune, S., Nishijima, K., Iwamoto, K., Nakagiri, K., Nakajima, Y., Taniuchi, N., Yokoyama, M., Izumiyama, S., Kuze, M., Inomoto, M., Ishitsuka, M., Ito, H., Kinoshita, T., Matsumoto, R., Ommura, Y., Shigeta, N., Shinoki, M., Suganuma, T., Yonenaga, M., Martin, J. F., Tanaka, H. A., Towstego, T., Chen, S., Xu, B. D., Zhang, B., Posiadala-Zezula, M., Hadley, D., Nicholson, M., O'Flaherty, M., Richards, B., Ali, A., Jamieson, B., Marti, Ll., Minamino, A., Pintaudi, G., Sano, S., Suzuki, S., Wada, K., Nascimento Machado, L., Abe, K., Hayato, Y., Hiraide, K., Ieki, K., Ikeda, M., Kameda, J., Kanemura, Y., Kaneshima, R., Kashiwagi, Y., Kataoka, Y., Miki, S., Mine, S., Miura, M., Moriyama, S., Nakano, Y., Nakahata, M., Nakayama, S., Noguchi, Y., Okamoto, K., Sato, K., Sekiya, H., Shiba, H., Shimizu, K., Shiozawa, M., Sonoda, Y., Suzuki, Y., Takeda, A., Takemoto, Y., Takenaka, A., Tanaka, H., Watanabe, S., Yano, T., de Perio, P., Martens, K., Vagins, M. R., Bian, J., Griskevich, N. J., Kropp, W. R., Locke, S., Smy, M. B., Sobel, H. W., Takhistov, V., Yankelevich, A., Han, S., Kajita, T., Okumura, K., Tashiro, T., Tomiya, T., Wang, X., Xia, J., Yoshida, S., Megias, G. D., Fernandez, P., Labarga, L., Ospina, N., Zaldivar, B., Pointon, B. W., Akutsu, R., Gousy-Leblanc, V., Hartz, M., Konaka, A., Prouse, N. W., Kearns, E., Raaf, J. L., Wan, L., Wester, T., Hill, J., Kim, J. Y., Lim, I. T., Park, R. G., Bodur, B., Scholberg, K., Walter, C. W., Bernard, L., Coffani, A., Drapier, O., El Hedri, S., Giampaolo, A., Mueller, Th. A., Santos, A. D., Paganini, P., Quilain, B., Ishizuka, T., Nakamura, T., Jang, J. S., Learned, J. G., Cao, S., Choi, K., Anthony, L. H. V., Martin, D., Scott, M., Sztuc, A. A., Uchida, Y., Berardi, V., Catanesi, M. G., Radicioni, E., Calabria, N. F., De Rosa, G., Collazuol, G., Iacob, F., Lamoureux, M., Mattiazzi, M., Ludovici, L., Gonin, M., Pronost, G., Fujisawa, C., Maekawa, Y., Nishimura, Y., Sasaki, R., Friend, M., Hasegawa, T., Ishida, T., Jakkapu, M., Kobayashi, T., Matsubara, T., Nakadaira, T., Nakamura, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Boschi, T., Di Lodovico, F., Gao, J., Goldsack, A., Katori, T., Migenda, J., Taani, M., Zsoldos, S., Kotsar, Y., Ozaki, H., Suzuki, A. T., Takeuchi, Y., Yaamoto, S., Bronner, C., Feng, J., Kikawa, T., Mori, M., Nakaya, T., Wendell, R. A., Yasutome, K., Jenkins, S. J., Mccauley, N., Mehta, P., Tsui, K. M., Fukuda, Y., Itow, Y., Menjo, H., Ninomiya, K., Lagoda, J., Lakshmi, S. M., Mandal, M., Mijakowski, P., Prabhu, Y. S., Zalipska, J., Jia, M., Jiang, J., Jung, C. K., Wilking, M. J., Yanagisawa, C., Harada, M., Ishino, H., Ito, S., Kitagawa, H., Koshio, Y., Ma, W., Nakanishi, F., Sakai, S., Barr, G., Barrow, D., Cook, L., Samani, S., Wark, D., Nova, F., Yang, J. Y., Malek, M., Mcelwee, J. M., Stone, O., Thiesse, M. D., Thompson, L. F., Okazawa, H., Kim, S. B., Seo, J. W., Yu, I., Ichikawa, A. K., Nakamura, K. D., Tairafune, S., Nishijima, K., Iwamoto, K., Nakagiri, K., Nakajima, Y., Taniuchi, N., Yokoyama, M., Izumiyama, S., Kuze, M., Inomoto, M., Ishitsuka, M., Ito, H., Kinoshita, T., Matsumoto, R., Ommura, Y., Shigeta, N., Shinoki, M., Suganuma, T., Yonenaga, M., Martin, J. F., Tanaka, H. A., Towstego, T., Chen, S., Xu, B. D., Zhang, B., Posiadala-Zezula, M., Hadley, D., Nicholson, M., O???flaherty, M., Richards, B., Ali, A., Jamieson, B., Marti, Ll., Minamino, A., Pintaudi, G., Sano, S., Suzuki, S., and Wada, K.

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), High Energy Physics - Experiment (hep-ex), Neutrino astronomy Supernova neutrinos Particle astrophysics Particle physics Silicon burning Core-collapse supernovae, Physics - Instrumentation and Detectors, Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

In 2020, the Super-Kamiokande (SK) experiment moved to a new stage (SK-Gd) in which gadolinium (Gd) sulfate octahydrate was added to the water in the detector, enhancing the efficiency to detect thermal neutrons and consequently improving the sensitivity to low energy electron anti-neutrinos from inverse beta decay (IBD) interactions. SK-Gd has the potential to provide early alerts of incipient core-collapse supernovae through detection of electron anti-neutrinos from thermal and nuclear processes responsible for the cooling of massive stars before the gravitational collapse of their cores. These pre-supernova neutrinos emitted during the silicon burning phase can exceed the energy threshold for IBD reactions. We present the sensitivity of SK-Gd to pre-supernova stars and the techniques used for the development of a pre-supernova alarm based on the detection of these neutrinos in SK, as well as prospects for future SK-Gd phases with higher concentrations of Gd. For the current SK-Gd phase, high-confidence alerts for Betelgeuse could be issued up to nine hours in advance of the core-collapse itself., Comment: 20 pages

Published
2022

243. Search for solar electron anti-neutrinos due to spin-flavor precession in the Sun with Super-Kamiokande-IV

Author

Collaboration, Super-Kamiokande, Abe, K., Bronner, C., Hayato, Y., Ikeda, M., Imaizumi, S., Ito, H., Kameda, J., Kataoka, Y., Miura, M., Moriyama, S., Nagao, Y., Nakahata, M., Nakajima, Y., Nakayama, S., Okada, T., Okamoto, K., Orii, A., Pronost, G., Sekiya, H., Shiozawa, M., Sonoda, Y., Suzuki, Y., Takeda, A., Takemoto, Y., Takenaka, A., Tanaka, H., Yano, T., Akutsu, R., Han, S., Kajita, T., Okumura, K., Tashiro, T., Wang, R., Xia, J., Bravo-Berguño, D., Labarga, L., Marti, Ll., Zaldivar, B., Blaszczyk, F. d. M., Kearns, E., Raaf, J. L., Stone, J. L., Wan, L., Wester, T., Pointin, B. W., Bian, J., Griskevich, N. J., Kropp, W. R., Locke, S., Mine, S., Smy, M. B., Sobel, H. W., Takhistov, V., Weatherly, P., Hill, J., Kim, J. Y., Lim, I. T., Park, R. G., Bodur, B., Scholberg, K., Walter, C. W., Bernard, L., Coffani, A., Drapier, O., Hedri, S. El, Giampaolo, A., Gonin, M., Mueller, Th. A., Paganini, P., Quilain, B., Ishizuka, T., Nakamura, T., Jang, J. S., Learned, J. G., Anthony, L. H. V., Sztuc, A. A., Uchida, Y., Berardi, V., Catanesi, M. G., Radicioni, E., Calabria, N. F., Machado, L. N., De Rosa, G., Collazuol, G., Iacob, F., Lamoureux, M., Ospina, N., Ludovici, L., Nishimura, Y., Cao, S., Friend, M., Hasegawa, T., Ishida, T., Jakkapu, M., Kobayashi, T., Matsubara, T., Nakadaira, T., Nakamura, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Nakano, Y., Shiozawa, T., Suzuki, A. T., Takeuchi, Y., Yamamoto, S., Ali, A., Ashida, Y., Feng, J., Hirota, S., Ichikawa, A. K., Kikawa, T., Mori, M., Nakaya, T., Wendell, R. A., Yasutome, Y., Fernandez, P., McCauley, N., Mehta, P., Pritchard, A., Tsui, K. M., Fukuda, Y., Itow, Y., Menjo, H., Niwa, T., Sato, K., Tsukada, M., Mijakowski, P., Jung, C. K., Vilela, C., Wilking, M. J., Yanagisawa, C., Harada, M., Hagiwara, K., Horai, T., Ishino, H., Ito, S., Koshio, Y., Ma, W., Piplani, N., Sakai, S., Kuno, Y., Barr, G., Barrow, D., Cook, L., Goldsack, A., Samani, S., Simpson, C., Wark, D., Nova, F., Boschi, T., Di Lodovico, F., Taani, M., Migenda, J., Sedgwick, S. Molina, Zsoldos, S., Yang, J. Y., Jenkins, S. J., Malek, M., McElwee, J. M., Stone, O., Thiesse, M. D., Thompson, L. F., Okazawa, H., Kim, S. B., Yu, I., Nishijima, K., Koshiba, M., Iwamoto, K., Ogawa, N., Yokoyama, M., Martens, K., Vagins, M. R., Izumiyama, S., Kuze, M., Tanaka, M., Yoshida, T., Inomoto, M., Ishitsuka, M., Matsumoto, R., Ohta, K., Shinoki, M., Martin, J. F., Tanaka, H. A., Towstego, T., Hartz, M., Konaka, A., de Perio, P., Prouse, N. W., Chen, S., Xu, B. D., Richards, B., Jamieson, B., Walker, J., Minamino, A., Pintaudi, G., Sasaki, R., Posiadala-Zezula, M., Abe, K., Bronner, C., Hayato, Y., Ikeda, M., Imaizumi, S., Ito, H., Kameda, J., Kataoka, Y., Miura, M., Moriyama, S., Nagao, Y., Nakahata, M., Nakajima, Y., Nakayama, S., Okada, T., Okamoto, K., Orii, A., Pronost, G., Sekiya, H., Shiozawa, M., Sonoda, Y., Suzuki, Y., Takeda, A., Takemoto, Y., Takenaka, A., Tanaka, H., Yano, T., Akutsu, R., Han, S., Kajita, T., Okumura, K., Tashiro, T., Wang, R., Xia, J., Bravo-Berguno, D., Labarga, L., Marti, L., Zaldivar, B., Blaszczyk, F. D. M., Kearns, E., Raaf, J. L., Stone, J. L., Wan, L., Wester, T., Pointon, B. W., Bian, J., Griskevich, N. J., Kropp, W. R., Locke, S., Mine, S., Smy, M. B., Sobel, H. W., Takhistov, V., Weatherly, P., Hill, J., Kim, J. Y., Lim, I. T., Park, R. G., Bodur, B., Scholberg, K., Walter, C. W., Bernard, L., Coffani, A., Drapier, O., Hedri, S. E., Giampaolo, A., Gonin, M., Mueller, T. A., Paganini, P., Quilain, B., Ishizuka, T., Nakamura, T., Jang, J. S., Learned, J. G., Anthony, L. H. V., Sztuc, A. A., Uchida, Y., Berardi, V., Catanesi, M. G., Radicioni, E., Calabria, N. F., Machado, L. N., DE ROSA, Gianfranca, Collazuol, G., Iacob, F., Lamoureux, M., Ospina, N., Ludovici, L., Nishimura, Y., Cao, S., Friend, M., Hasegawa, T., Ishida, T., Jakkapu, M., Kobayashi, T., Matsubara, T., Nakadaira, T., Nakamura, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Nakano, Y., Shiozawa, T., Suzuki, A. T., Takeuchi, Y., Yamamoto, S., Ali, A., Ashida, Y., Feng, J., Hirota, S., Ichikawa, A. K., Kikawa, T., Mori, M., Nakaya, T., Wendell, R. A., Yasutome, Y., Fernandez, P., Mccauley, N., Mehta, P., Pritchard, A., Tsui, K. M., Fukuda, Y., Itow, Y., Menjo, H., Niwa, T., Sato, K., Tsukada, M., Mijakowski, P., Jung, C. K., Vilela, C., Wilking, M. J., Yanagisawa, C., Harada, M., Hagiwara, K., Horai, T., Ishino, H., Ito, S., Koshio, Y., Ma, W., Piplani, N., Sakai, S., Kuno, Y., Barr, G., Barrow, D., Cook, L., Goldsack, A., Samani, S., Simpson, C., Wark, D., Nova, F., Boschi, T., Di Lodovico, F., Taani, M., Migenda, J., Sedgwick, S. M., Zsoldos, S., Yang, J. Y., Jenkins, S. J., Malek, M., Mcelwee, J. M., Stone, O., Thiesse, M. D., Thompson, L. F., Okazawa, H., Kim, S. B., Yu, I., Nishijima, K., Koshiba, M., Iwamoto, K., Ogawa, N., Yokoyama, M., Martens, K., Vagins, M. R., Izumiyama, S., Kuze, M., Tanaka, M., Yoshida, T., Inomoto, M., Ishitsuka, M., Matsumoto, R., Ohta, K., Shinoki, M., Martin, J. F., Tanaka, H. A., Towstego, T., Hartz, M., Konaka, A., de Perio, P., Prouse, N. W., Chen, S., Xu, B. D., Richards, B., Jamieson, B., Walker, J., Minamino, A., Pintaudi, G., Sasaki, R., Posiadala-Zezula, M., Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Super-Kamiokande, and UAM. Departamento de Física Teórica

Subjects
Physics - Instrumentation and Detectors, neutrino: solar, water, FOS: Physical sciences, antineutrino/e: energy spectrum, KAMIOKANDE, antineutrino/e: particle identification, Solar neutrino, neutrino: flux, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), neutrino: energy, precession, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutron tagging, Neutrino-antineutrino oscillation, background, new physics: search for, High Energy Physics::Phenomenology, Física, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), semileptonic decay, sensitivity, neutrino: magnetic moment, Electron antineutrinos Neutrino–antineutrino oscillation Neutron tagging Solar neutrino Water Cherenkov detector, nucleus: fusion, Electron antineutrinos, Electron antineutrino, Water Cherenkov detector, Neutrino–antineutrino oscillation, High Energy Physics::Experiment, upgrade, gadolinium, signature, experimental results
Abstract

Due to a very low production rate of electron anti-neutrinos ($\bar{\nu}_e$) via nuclear fusion in the Sun, a flux of solar $\bar{\nu}_e$ is unexpected. An appearance of $\bar{\nu}_e$ in solar neutrino flux opens a new window for the new physics beyond the standard model. In particular, a spin-flavor precession process is expected to convert an electron neutrino into an electron anti-neutrino (${\nu_e\to\bar{\nu}_e}$) when neutrino has a finite magnetic moment. In this work, we have searched for solar $\bar{\nu}_e$ in the Super-Kamiokande experiment, using neutron tagging to identify their inverse beta decay signature. We identified 78 $\bar{\nu}_e$ candidates for neutrino energies of 9.3 to 17.3 MeV in 2970.1 live days with a fiducial volume of 22.5 kiloton water (183.0 kton$\cdot$year exposure). The energy spectrum has been consistent with background predictions and we thus derived a 90% confidence level upper limit of ${4.7\times10^{-4}}$ on the $\nu_e\to\bar{\nu}_e$ conversion probability in the Sun. We used this result to evaluate the sensitivity of future experiments, notably the Super-Kamiokande Gadolinium (SK-Gd) upgrade., Comment: 16 pages, 10 figures, 7 tables

Published
2022

249. Lower-than-expected flare temperatures for TRAPPIST-1

Author

Maas, A. J., primary, Ilin, E., additional, Oshagh, M., additional, Pallé, E., additional, Parviainen, H., additional, Molaverdikhani, K., additional, Quirrenbach, A., additional, Esparza-Borges, E., additional, Murgas, F., additional, Béjar, V. J. S., additional, Narita, N., additional, Fukui, A., additional, Lin, C.-L., additional, Mori, M., additional, and Klagyivik, P., additional

Published
2022
Full Text
View/download PDF

250. Direct Measurement of the Cosmic-Ray Helium Spectrum from 40 GeV to 250 TeV with the Calorimetric Electron Telescope on the International Space Station

Author

Adriani, O, Akaike, Y, Asano, K, Asaoka, Y, Berti, E, Bigongiari, G, Binns, W R, Bongi, M, Brogi, P, Bruno, A, Buckley, J H, Cannady, N, Castellini, G, Checchia, C, Cherry, M L, Collazuol, G, de Nolfo, G A, Ebisawa, K, Ficklin, A W, Fuke, H, Gonzi, S, Guzik, T G, Hams, T, Hibino, K, Ichimura, M, Ioka, K, Ishizaki, W, Israel, M H, Kasahara, K, Kataoka, J, Kataoka, R, Katayose, Y, Kato, C, Kawanaka, N, Kawakubo, Y, Kobayashi, K, Kohri, K, Krawczynski, H S, Krizmanic, J F, Maestro, P, Marrocchesi, P S, Messineo, A M, Mitchell, J W, Miyake, S, Moiseev, A A, Mori, M, Mori, N, Motz, H M, Munakata, K, Nakahira, S, Nishimura, J, Okuno, S, Ormes, J F, Ozawa, S, Pacini, L, Papini, P, Rauch, B F, Ricciarini, S B, Sakai, K, Sakamoto, T, Sasaki, M, Shimizu, Y, Shiomi, A, Spillantini, P, Stolzi, F, Sugita, S, Sulaj, A, Takita, M, Tamura, T, Terasawa, T, Torii, S, Tsunesada, Y, Uchihori, Y, Vannuccini, E, Wefel, J P, Yamaoka, K, Yanagita, S, Yoshida, A, Yoshida, K, and Zober, W V

Subjects
Cosmic Rays Composition and Propagation Cosmic Rays and Astroparticle Detectors
Published
2023

Catalog

Books, media, physical & digital resources
See catalog results