Zobrazeno 1 - 10
of 373
pro vyhledávání: '"Sharon Amir"'
Publikováno v:
Reproductive Medicine, Vol 5, Iss 3, Pp 181-185 (2024)
Septic abortion can lead to severe maternal morbidity and mortality. The management of septic abortion can be complicated by a history of radical trachelectomy and transabdominal cerclage placement. A 33-year-old G1P0 at 17 weeks and 6 days gestation
Externí odkaz:
https://doaj.org/article/abc6f0d718b4484d8900538a380a5c04
A rare subclass of Type Ia supernovae (SNe Ia), named after the prototype SN 2003fg, includes some of the brightest SNe Ia, often called "super Chandrasekhar-mass" SNe Ia. We calculate the $\gamma$-ray deposition histories and the $^{56}$Ni mass synt
Externí odkaz:
http://arxiv.org/abs/2407.07417
Autor:
Sharon, Amir, Kushnir, Doron
Type Ia supernovae (SNe Ia) are widely believed to arise from thermonuclear explosions of white dwarfs (WDs). However, ongoing debate surrounds their progenitor systems and the mechanisms triggering these explosions. Recently, Sharon \& Kushnir showe
Externí odkaz:
http://arxiv.org/abs/2407.06859
Autor:
Kushnir, Doron, Sharon, Amir
The recent SH0ES determination of the Hubble constant, $H_0=73.04\pm1.04$ km/s/Mpc, deviates significantly by $\approx5\sigma$ from the \textit{Planck} value, stimulating discussions on cosmological model extensions. To minimize statistical uncertain
Externí odkaz:
http://arxiv.org/abs/2404.16102
Autor:
Keren Tazat PhD, Oleg Reshetnyak MD, Natan Shtraus MSc, Ifat Sayag MSc, Nicola J. Mabjeesh MD, PhD, Sharon Amir PhD
Publikováno v:
Technology in Cancer Research & Treatment, Vol 19 (2020)
Purpose: External beam radiotherapy is one of the treatment options for organ-confined prostate cancer. A total dose of 70 to 81 Gray (Gy) is given daily (1.8-2.5 Gy/d), with a dose rate of 3 to 6 Gy/min over 28 to 45 treatments during 8 to 9 weeks.
Externí odkaz:
https://doaj.org/article/87e9f2ff4246426dae115dd72f98c248
Autor:
Chen, Ping, Gal-Yam, Avishay, Sollerman, Jesper, Schulze, Steve, Post, Richard S., Liu, Chang, Ofek, Eran O., Das, Kaustav K., Fremling, Christoffer, Horesh, Assaf, Katz, Boaz, Kushnir, Doron, Kasliwal, Mansi M., Kulkarni, Shri R., Liu, Dezi, Liu, Xiangkun, Miller, Adam A., Rose, Kovi, Waxman, Eli, Yang, Sheng, Yao, Yuhan, Zackay, Barak, Bellm, Eric C., Dekany, Richard, Drake, Andrew J., Fang, Yuan, Fynbo, Johan P. U., Groom, Steven L., Helou, George, Irani, Ido, Laz, Theophile Jegou du, Liu, Xiaowei, Mazzali, Paolo A., Neill, James D., Qin, Yu-Jing, Riddle, Reed L., Sharon, Amir, Strotjohann, Nora L., Wold, Avery, Yan, Lin
Neutron stars and stellar-mass black holes are the remnants of massive star explosions. Most massive stars reside in close binary systems, and the interplay between the companion star and the newly formed compact object has been theoretically explore
Externí odkaz:
http://arxiv.org/abs/2310.07784
The SH0ES collaboration Hubble constant determination is in a ${\sim}5\sigma$ difference with the $Planck$ value, known as the Hubble tension. The accuracy of the Hubble constant measured with extragalactic Cepheids depends on robust stellar-crowding
Externí odkaz:
http://arxiv.org/abs/2305.14435
Autor:
Schulze, Steve, Fransson, Claes, Kozyreva, Alexandra, Chen, Ting-Wan, Yaron, Ofer, Jerkstrand, Anders, Gal-Yam, Avishay, Sollerman, Jesper, Yan, Lin, Kangas, Tuomas, Leloudas, Giorgos, Omand, Conor M. B., Smartt, Stephen J., Yang, Yi, Nicholl, Matt, Sarin, Nikhil, Yao, Yuhan, Brink, Thomas G., Sharon, Amir, Rossi, Andrea, Chen, Ping, Chen, Zhihao, Cikota, Aleksandar, De, Kishalay, Drake, Andrew J., Filippenko, Alexei V., Fremling, Christoffer, Freour, Laurane, Fynbo, Johan P. U., Ho, Anna Y. Q., Inserra, Cosimo, Irani, Ido, Kuncarayakti, Hanindyo, Lunnan, Ragnhild, Mazzali, Paolo, Ofek, Eran O., Palazzi, Eliana, Perley, Daniel A., Pursiainen, Miika, Rothberg, Barry, Shingles, Luke J., Smith, Ken, Taggart, Kirsty, Tartaglia, Leonardo, Zheng, WeiKang, Anderson, Joseph P., Cassara, Letizia, Christensen, Eric, Djorgovski, S. George, Galbany, Lluis, Gkini, Anamaria, Graham, Matthew J., Gromadzki, Mariusz, Groom, Steven L., Hiramatsu, Daichi, Howell, D. Andrew, Kasliwal, Mansi M., McCully, Curtis, Müller-Bravo, Tomas E., Paiano, Simona, Paraskeva, Emmanouela, Pessi, Priscila J., Polishook, David, Rau, Arne, Rigault, Mickael, Rusholme, Ben
Abridged - Stars with ZAMS masses between 140 and $260 M_\odot$ are thought to explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can produce up to several tens of solar masses of radioactive nickel, resulting i
Externí odkaz:
http://arxiv.org/abs/2305.05796
Autor:
Sharon, Amir, Kushnir, Doron
Calcium-rich supernovae (Ca-rich SNe) are faint, rapidly evolving transients whose progenitor system is yet to be determined. We derive the $\gamma$-ray deposition histories of five Ca-rich SNe from the literature in order to place constraints on pos
Externí odkaz:
http://arxiv.org/abs/2212.14290
Temporal Trends in Patient Characteristics and Clinical Outcomes of TAVR: Over a Decade of Practice.
Autor:
Karra, Nour1 (AUTHOR) nour.karra@sheba.health.gov.il, Sharon, Amir1 (AUTHOR) amirsharon9@gmail.com, Massalha, Eias1,2 (AUTHOR) aias.masalha@sheba.health.gov.il, Fefer, Paul1,2 (AUTHOR) paul.fefer@sheba.health.gov.il, Maor, Elad1,2 (AUTHOR) elad.maor@sheba.health.gov.il, Guetta, Victor1,2 (AUTHOR) victor.guetta@sheba.health.gov.il, Ben-Zekry, Sagit1,2 (AUTHOR) sagit.benzekry@sheba.health.gov.il, Kuperstein, Rafael1,2 (AUTHOR) rafael.kuperstein@sheba.health.gov.il, Matetzky, Shlomi1,2 (AUTHOR) shlomi.matetzky@sheba.health.gov.il, Beigel, Roy1,2 (AUTHOR) roy.beigel@sheba.health.gov.il, Segev, Amit1,2 (AUTHOR) amit.segev@sheba.health.gov.il, Barbash, Israel M.1,2 (AUTHOR) israel.barbash@sheba.health.gov.il
Publikováno v:
Journal of Clinical Medicine. Sep2024, Vol. 13 Issue 17, p5027. 12p.