Author: "Ishida, M." / Publication Type: Electronic Resources - Searchworks@Jio Institute Digital Library Search Results

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103 results on '"Ishida, M."'

1. Pragmatic solutions to reduce the global burden of stroke: a World Stroke Organization–Lancet Neurology Commission

Author: Feigin, V, Owolabi, M, Abd-Allah, F, Akinyemi, R, Bhattacharjee, N, Brainin, M, Cao, J, Caso, V, Dalton, B, Davis, A, Dempsey, R, Duprey, J, Feng, W, Ford, G, Gall, S, Gandhi, D, Good, D, Hachinski, V, Hacke, W, Hankey, G, Ishida, M, Johnson, W, Kim, J, Lavados, P, Lindsay, P, Mahal, A, Martins, S, Murray, C, Nguyen, T, Norrving, B, Olaiya, M, Olalusi, O, Pandian, J, Phan, H, Platz, T, Ranta, A, Rehman, S, Roth, G, Sebastian, I, Smith, A, Suwanwela, N, Sylaja, P, Thapa, R, Thrift, A, Uvere, E, Vollset, S, Yavagal, D, Yaria, J, Abera, S, Ibrahim, N, Liu, L, Ovbiagele, B, Piradov, M, Abanto, C, Addissie, A, Adeleye, A, Adilbekov, Y, Adilbekova, B, Adoukonou, T, Aguiar de Sousa, D, Akhmetzhanova, Z, Akpalu, A, El Alaoui-Faris, M, Ameriso, S, Andonova, S, Arsovska, A, Awoniyi, F, Bakhiet, M, Barboza, M, Basri, H, Bath, P, Bereczki, D, Beretta, S, Berkowitz, A, Bernhardt, J, Berzina, G, Bhavsar, B, Bisharyan, M, Bohara, M, Bovet, P, Budincevic, H, Cadilhac, D, Cerimagic, D, Charway-Felli, A, Chen, C, Chin, J, Christensen, H, Chwojnicki, K, Conforto, A, Correia, M, Mora Cuervo, D, Czlonkowska, A, D'Amelio, M, Danielyan, K, Davis, S, Demarin, V, Demchuk, A, Dichgans, M, Dokova, K, Donnan, G, Duran, J, Ekeng, G, Elkind, M, Endres, M, Fischer, U, Flomin, Y, Gankpe, F, Gavidia, M, Gaye Saavedra, A, Gebreyohanns, M, George, M, Gierlotka, M, Giroud, M, Gnedovskaya, E, Goncalves, I, Gongora-Rivera, F, Gunaratne, P, Hamadeh, R, Hamzat, T, Heldner, M, Ibrahim, E, Ihle-Hansen, H, Jee, S, Jiann-Shing, J, Johnston, S, Jovanovic, D, Jurjans, K, Kalani, R, Kalkonde, Y, Kamenova, S, Karaszewski, B, Kelly, P, Kiechl, S, Kondybayeva, A, Korv, J, Kozera, G, Kravchenko, M, Krespi, Y, Krishnamurthi, R, Kruja, J, Kutluk, K, Langhorne, P, Law, Z, Lebedynets, D, Lee, T, Leung, T, Liebeskind, D, Lopez-Jaramillo, P, Lotufo, P, Machline-Carrion, M, Maia, L, Malojcic, B, Markus, H, Marquez-Romero, J, Medina, M, Medukhanova, S, Mehndiratta, M, Miglane, E, Mihejeva, I, Mikulik, R, Mirrakhimov, E, Mohl, S, Munakomi, S, Murphy, S, Musa, K, Nasreldein, A, Nogueira, R, Nolte, C, Noubiap, J, Novarro-Escudero, N, Ocampo, C, O'Donnell, M, Ogun, Y, Ogunniyi, A, Oraby, M, Orken, D, Ozdemir, A, Ozturk, S, Paccot, M, Pereira, T, Peeters, A, Potpara, T, Proios, H, Rathore, F, Sacco, R, Sahathevan, R, Sandset, E, Renato Santos, I, Saposnik, G, Sarfo, F, Sargento-Freitas, J, Sharma, M, Shaw, L, Sheth, K, Shin, Y, Shobhana, A, Silva, S, Tedim Cruz, V, Thakur, K, Thapa, L, Toni, D, Topcuoglu, M, Torales, J, Towfighi, A, Truelsen, T, Tsiskaridze, A, Tulloch-Reid, M, Useche, J, Vanacker, P, Vassilopoulou, S, Vukorepa, G, Vuletic, V, Wahab, K, Wang, W, Wijeratne, T, Wojtyniak, B, Wolfe, C, Yacouba, M, Yang, J, Yifru, Y, Yock-Corrales, A, Yonemoto, N, Yperzeele, L, Zagozdzon, P, Feigin V. L., Owolabi M. O., Abd-Allah F., Akinyemi R. O., Bhattacharjee N. V., Brainin M., Cao J., Caso V., Dalton B., Davis A., Dempsey R., Duprey J., Feng W., Ford G. A., Gall S., Gandhi D., Good D. C., Hachinski V., Hacke W., Hankey G. J., Ishida M., Johnson W., Kim J., Lavados P., Lindsay P., Mahal A., Martins S., Murray C., Nguyen T. P., Norrving B., Olaiya M. T., Olalusi O. V., Pandian J., Phan H., Platz T., Ranta A., Rehman S., Roth G., Sebastian I. A., Smith A. E., Suwanwela N. C., Sylaja P. N., Thapa R., Thrift A. G., Uvere E., Vollset S. E., Yavagal D., Yaria J., Abera S. F., Akinyemi R., Dempsey R. J., Ibrahim N. M., Liu L., Ovbiagele B., Piradov M., Suwanwela N., Abanto C., Addissie A., Adeleye A. O., Adilbekov Y., Adilbekova B., Adoukonou T. A., Aguiar de Sousa D., Akhmetzhanova Z., Akpalu A., El Alaoui-Faris M., Ameriso S. F., Andonova S., Arsovska A., Awoniyi F. E., Bakhiet M., Barboza M. A., Basri H., Bath P. M., Bereczki D., Beretta S., Berkowitz A. L., Bernhardt J., Berzina G., Bhavsar B., Bisharyan M. S., Bohara M., Bovet P., Budincevic H., Cadilhac D. A., Cerimagic D., Charway-Felli A., Chen C., Chin J. H., Christensen H., Chwojnicki K., Conforto A. B., Correia M., Mora Cuervo D. L., Czlonkowska A., D'Amelio M., Danielyan K. E., Davis S., Demarin V., Demchuk A. M., Dichgans M., Dokova K., Donnan G., Duran J. C., Ekeng G., Elkind M. S., Endres M., Fischer U., Flomin Y., Gankpe F., Gavidia M., Gaye Saavedra A., Gebreyohanns M., George M., Gierlotka M., Giroud M., Gnedovskaya E. V., Goncalves I. P., Gongora-Rivera F., Gunaratne P. S., Hamadeh R. R., Hamzat T. -H. K., Heldner M. R., Ibrahim E., Ihle-Hansen H., Jee S., Jiann-Shing J., Johnston S. C., Jovanovic D., Jurjans K., Kalani R., Kalkonde Y., Kamenova S., Karaszewski B., Kelly P., Kiechl S., Kondybayeva A., Korv J., Kozera G., Kravchenko M., Krespi Y., Krishnamurthi R., Kruja J., Kutluk K., Langhorne P., Law Z. K., Lebedynets D., Lee T. -H., Leung T. W., Liebeskind D. S., Lopez-Jaramillo P., Lotufo P. A., Machline-Carrion M. J., Maia L. F., Malojcic B., Markus H. S., Marquez-Romero J. M., Medina M. T., Medukhanova S., Mehndiratta M. M., Miglane E., Mihejeva I., Mikulik R., Mirrakhimov E., Mohl S., Munakomi S., Murphy S., Musa K. I., Nasreldein A., Nogueira R. G., Nolte C. H., Noubiap J. J., Novarro-Escudero N., Ocampo C., O'Donnell M., Ogun Y., Ogunniyi A., Oraby M. I., Orken D. N., Ozdemir A. O., Ozturk S., Paccot M., Pereira T., Peeters A., Potpara T., Proios H., Rathore F. A., Sacco R. L., Sahathevan R., Sandset E. S., Renato Santos I., Saposnik G., Sarfo F. S., Sargento-Freitas J., Sharma M., Shaw L., Sheth K. N., Shin Y. -I., Shobhana A., Silva S. N., Tedim Cruz V., Thakur K., Thapa L. J., Toni D., Topcuoglu M. A., Torales J., Towfighi A., Truelsen T., Tsiskaridze A., Tulloch-Reid M., Useche J. N., Vanacker P., Vassilopoulou S., Vukorepa G., Vuletic V., Wahab K. W., Wang W., Wijeratne T., Wojtyniak B., Wolfe C., Yacouba M. N., Yang J., Yifru Y. M., Yock-Corrales A., Yonemoto N., Yperzeele L., Zagozdzon P., Feigin, V, Owolabi, M, Abd-Allah, F, Akinyemi, R, Bhattacharjee, N, Brainin, M, Cao, J, Caso, V, Dalton, B, Davis, A, Dempsey, R, Duprey, J, Feng, W, Ford, G, Gall, S, Gandhi, D, Good, D, Hachinski, V, Hacke, W, Hankey, G, Ishida, M, Johnson, W, Kim, J, Lavados, P, Lindsay, P, Mahal, A, Martins, S, Murray, C, Nguyen, T, Norrving, B, Olaiya, M, Olalusi, O, Pandian, J, Phan, H, Platz, T, Ranta, A, Rehman, S, Roth, G, Sebastian, I, Smith, A, Suwanwela, N, Sylaja, P, Thapa, R, Thrift, A, Uvere, E, Vollset, S, Yavagal, D, Yaria, J, Abera, S, Ibrahim, N, Liu, L, Ovbiagele, B, Piradov, M, Abanto, C, Addissie, A, Adeleye, A, Adilbekov, Y, Adilbekova, B, Adoukonou, T, Aguiar de Sousa, D, Akhmetzhanova, Z, Akpalu, A, El Alaoui-Faris, M, Ameriso, S, Andonova, S, Arsovska, A, Awoniyi, F, Bakhiet, M, Barboza, M, Basri, H, Bath, P, Bereczki, D, Beretta, S, Berkowitz, A, Bernhardt, J, Berzina, G, Bhavsar, B, Bisharyan, M, Bohara, M, Bovet, P, Budincevic, H, Cadilhac, D, Cerimagic, D, Charway-Felli, A, Chen, C, Chin, J, Christensen, H, Chwojnicki, K, Conforto, A, Correia, M, Mora Cuervo, D, Czlonkowska, A, D'Amelio, M, Danielyan, K, Davis, S, Demarin, V, Demchuk, A, Dichgans, M, Dokova, K, Donnan, G, Duran, J, Ekeng, G, Elkind, M, Endres, M, Fischer, U, Flomin, Y, Gankpe, F, Gavidia, M, Gaye Saavedra, A, Gebreyohanns, M, George, M, Gierlotka, M, Giroud, M, Gnedovskaya, E, Goncalves, I, Gongora-Rivera, F, Gunaratne, P, Hamadeh, R, Hamzat, T, Heldner, M, Ibrahim, E, Ihle-Hansen, H, Jee, S, Jiann-Shing, J, Johnston, S, Jovanovic, D, Jurjans, K, Kalani, R, Kalkonde, Y, Kamenova, S, Karaszewski, B, Kelly, P, Kiechl, S, Kondybayeva, A, Korv, J, Kozera, G, Kravchenko, M, Krespi, Y, Krishnamurthi, R, Kruja, J, Kutluk, K, Langhorne, P, Law, Z, Lebedynets, D, Lee, T, Leung, T, Liebeskind, D, Lopez-Jaramillo, P, Lotufo, P, Machline-Carrion, M, Maia, L, Malojcic, B, Markus, H, Marquez-Romero, J, Medina, M, Medukhanova, S, Mehndiratta, M, Miglane, E, Mihejeva, I, Mikulik, R, Mirrakhimov, E, Mohl, S, Munakomi, S, Murphy, S, Musa, K, Nasreldein, A, Nogueira, R, Nolte, C, Noubiap, J, Novarro-Escudero, N, Ocampo, C, O'Donnell, M, Ogun, Y, Ogunniyi, A, Oraby, M, Orken, D, Ozdemir, A, Ozturk, S, Paccot, M, Pereira, T, Peeters, A, Potpara, T, Proios, H, Rathore, F, Sacco, R, Sahathevan, R, Sandset, E, Renato Santos, I, Saposnik, G, Sarfo, F, Sargento-Freitas, J, Sharma, M, Shaw, L, Sheth, K, Shin, Y, Shobhana, A, Silva, S, Tedim Cruz, V, Thakur, K, Thapa, L, Toni, D, Topcuoglu, M, Torales, J, Towfighi, A, Truelsen, T, Tsiskaridze, A, Tulloch-Reid, M, Useche, J, Vanacker, P, Vassilopoulou, S, Vukorepa, G, Vuletic, V, Wahab, K, Wang, W, Wijeratne, T, Wojtyniak, B, Wolfe, C, Yacouba, M, Yang, J, Yifru, Y, Yock-Corrales, A, Yonemoto, N, Yperzeele, L, Zagozdzon, P, Feigin V. L., Owolabi M. O., Abd-Allah F., Akinyemi R. O., Bhattacharjee N. V., Brainin M., Cao J., Caso V., Dalton B., Davis A., Dempsey R., Duprey J., Feng W., Ford G. A., Gall S., Gandhi D., Good D. C., Hachinski V., Hacke W., Hankey G. J., Ishida M., Johnson W., Kim J., Lavados P., Lindsay P., Mahal A., Martins S., Murray C., Nguyen T. P., Norrving B., Olaiya M. T., Olalusi O. V., Pandian J., Phan H., Platz T., Ranta A., Rehman S., Roth G., Sebastian I. A., Smith A. E., Suwanwela N. C., Sylaja P. N., Thapa R., Thrift A. G., Uvere E., Vollset S. E., Yavagal D., Yaria J., Abera S. F., Akinyemi R., Dempsey R. J., Ibrahim N. M., Liu L., Ovbiagele B., Piradov M., Suwanwela N., Abanto C., Addissie A., Adeleye A. O., Adilbekov Y., Adilbekova B., Adoukonou T. A., Aguiar de Sousa D., Akhmetzhanova Z., Akpalu A., El Alaoui-Faris M., Ameriso S. F., Andonova S., Arsovska A., Awoniyi F. E., Bakhiet M., Barboza M. A., Basri H., Bath P. M., Bereczki D., Beretta S., Berkowitz A. L., Bernhardt J., Berzina G., Bhavsar B., Bisharyan M. S., Bohara M., Bovet P., Budincevic H., Cadilhac D. A., Cerimagic D., Charway-Felli A., Chen C., Chin J. H., Christensen H., Chwojnicki K., Conforto A. B., Correia M., Mora Cuervo D. L., Czlonkowska A., D'Amelio M., Danielyan K. E., Davis S., Demarin V., Demchuk A. M., Dichgans M., Dokova K., Donnan G., Duran J. C., Ekeng G., Elkind M. S., Endres M., Fischer U., Flomin Y., Gankpe F., Gavidia M., Gaye Saavedra A., Gebreyohanns M., George M., Gierlotka M., Giroud M., Gnedovskaya E. V., Goncalves I. P., Gongora-Rivera F., Gunaratne P. S., Hamadeh R. R., Hamzat T. -H. K., Heldner M. R., Ibrahim E., Ihle-Hansen H., Jee S., Jiann-Shing J., Johnston S. C., Jovanovic D., Jurjans K., Kalani R., Kalkonde Y., Kamenova S., Karaszewski B., Kelly P., Kiechl S., Kondybayeva A., Korv J., Kozera G., Kravchenko M., Krespi Y., Krishnamurthi R., Kruja J., Kutluk K., Langhorne P., Law Z. K., Lebedynets D., Lee T. -H., Leung T. W., Liebeskind D. S., Lopez-Jaramillo P., Lotufo P. A., Machline-Carrion M. J., Maia L. F., Malojcic B., Markus H. S., Marquez-Romero J. M., Medina M. T., Medukhanova S., Mehndiratta M. M., Miglane E., Mihejeva I., Mikulik R., Mirrakhimov E., Mohl S., Munakomi S., Murphy S., Musa K. I., Nasreldein A., Nogueira R. G., Nolte C. H., Noubiap J. J., Novarro-Escudero N., Ocampo C., O'Donnell M., Ogun Y., Ogunniyi A., Oraby M. I., Orken D. N., Ozdemir A. O., Ozturk S., Paccot M., Pereira T., Peeters A., Potpara T., Proios H., Rathore F. A., Sacco R. L., Sahathevan R., Sandset E. S., Renato Santos I., Saposnik G., Sarfo F. S., Sargento-Freitas J., Sharma M., Shaw L., Sheth K. N., Shin Y. -I., Shobhana A., Silva S. N., Tedim Cruz V., Thakur K., Thapa L. J., Toni D., Topcuoglu M. A., Torales J., Towfighi A., Truelsen T., Tsiskaridze A., Tulloch-Reid M., Useche J. N., Vanacker P., Vassilopoulou S., Vukorepa G., Vuletic V., Wahab K. W., Wang W., Wijeratne T., Wojtyniak B., Wolfe C., Yacouba M. N., Yang J., Yifru Y. M., Yock-Corrales A., Yonemoto N., Yperzeele L., and Zagozdzon P.
Published: 2023

2. The role of imprinted genes in human fetal growth

Author: Ishida, M.
Subjects: 576.5
Abstract: Identifying the genes important for fetal growth will help to understand common, serious complications of pregnancy such as intrauterine growth restriction (IUGR). Of particular interest are imprinted genes, which show monoallelic, parent-of-origin specific expression. Genes that are paternally derived tend to enhance fetal growth whereas maternally expressed genes suppress growth. A significant correlation between lower birth weight and increased expression of maternally expressed, pleckstrin homology-like domain, family A, member 2 (PHLDA2) in term placenta, without loss of imprinting, had been reported previously. We have identified a novel copy number variant (CNV1) in the PHLDA2 promoter which reduced the promoter efficiency in a luciferase reporter gene assay. Meta-analysis of CNV1 genotype data obtained from three independent white European normal birth cohorts (total n = 9,433) showed that maternal inheritance of CNV1 resulted in a 93 g increase in birth weight (P = 0.01). Moreover, when the mother was homozygous for CNV1, the influence on birth weight was 155 g (P = 0.04), a similar magnitude to the reduction caused by maternal smoking. The expression levels of paternally expressed gene 3 (PEG3), delta-like 1 homolog (DLK1) and maternally expressed gene 3 (MEG3) measured by real-time PCR in >110 normal term placentas from a white European cohort did not show correlation with fetal birth size measurements, except for a trend of positive association observed for DLK1 expression and birth weight (P = 0.072). Paternal inheritance of the type 1 diabetes (T1D) protective G allele of rs941576 SNP located in the DLK1-MEG3 locus was shown to be associated with a 132 g (P = 0.011) and 0.5 cm (P = 0.011) reduction in birth weight and head circumference respectively. This newly described PHLDA2 promoter CNV and rs941576 SNP, alongside their expressions, may provide useful genetic biomarkers/indicators for predicting birth size.
Published: 2012

3. Primary stroke prevention worldwide: translating evidence into action

Author: Owolabi, M, Thrift, A, Mahal, A, Ishida, M, Martins, S, Johnson, W, Pandian, J, Abd-Allah, F, Yaria, J, Phan, H, Roth, G, Gall, S, Beare, R, Phan, T, Mikulik, R, Akinyemi, R, Norrving, B, Brainin, M, Feigin, V, Abanto, C, Abera, S, Addissie, A, Adebayo, O, Adeleye, A, Adilbekov, Y, Adilbekova, B, Adoukonou, T, Aguiar de Sousa, D, Ajagbe, T, Akhmetzhanova, Z, Akpalu, A, Alvarez Ahlgren, J, Ameriso, S, Andonova, S, Awoniyi, F, Bakhiet, M, Barboza, M, Basri, H, Bath, P, Bello, O, Bereczki, D, Beretta, S, Berkowitz, A, Bernabe-Ortiz, A, Bernhardt, J, Berzina, G, Bisharyan, M, Bovet, P, Budincevic, H, Cadilhac, D, Caso, V, Chen, C, Chin, J, Chwojnicki, K, Conforto, A, Cruz, V, D'Amelio, M, Danielyan, K, Davis, S, Demarin, V, Dempsey, R, Dichgans, M, Dokova, K, Donnan, G, Elkind, M, Endres, M, Fischer, U, Gankpe, F, Gaye Saavedra, A, Gil, A, Giroud, M, Gnedovskaya, E, Hachinski, V, Hafdi, M, Hamadeh, R, Hamzat, T, Hankey, G, Heldner, M, Ibrahim, E, Ibrahim, N, Inoue, M, Jee, S, Jeng, J, Kalkonde, Y, Kamenova, S, Karaszewski, B, Kelly, P, Khan, T, Kiechl, S, Kondybayeva, A, Korv, J, Kravchenko, M, Krishnamurthi, R, Kruja, J, Lakkhanaloet, M, Langhorne, P, Lavados, P, Law, Z, Lawal, A, Lazo-Porras, M, Lebedynets, D, Lee, T, Leung, T, Liebeskind, D, Lindsay, P, Lopez-Jaramillo, P, Lotufo, P, Machline-Carrion, J, Makanjuola, A, Markus, H, Marquez-Romero, J, Medina, M, Medukhanova, S, Mehndiratta, M, Merkin, A, Mirrakhimov, E, Mohl, S, Moscoso-Porras, M, Muller-Stierlin, A, Murphy, S, Musa, K, Nasreldein, A, Nogueira, R, Nolte, C, Noubiap, J, Novarro-Escudero, N, Ogun, Y, Oguntoye, R, Oraby, M, Osundina, M, Ovbiagele, B, Orken, D, Ozdemir, A, Ozturk, S, Paccot, M, Phromjai, J, Piradov, P, Platz, T, Potpara, T, Ranta, A, Rathore, F, Richard, E, Sacco, R, Sahathevan, R, Santos Carquin, I, Saposnik, G, Sarfo, F, Sharma, M, Sheth, K, Shobhana, A, Suwanwela, N, Svyato, I, Sylaja, P, Tao, X, Thakur, K, Toni, D, Topcuoglu, M, Torales, J, Towfighi, A, Truelsen, T, Tsiskaridze, A, Tulloch-Reid, M, Useche, N, Vanacker, P, Vassilopoulou, S, Vukorepa, G, Vuletic, V, Wahab, K, Wang, W, Wijeratne, T, Wolfe, C, Yifru, Y, Yock-Corrales, A, Yonemoto, N, Yperzeele, L, Zhang, P, Owolabi M. O., Thrift A. G., Mahal A., Ishida M., Martins S., Johnson W. D., Pandian J., Abd-Allah F., Yaria J., Phan H. T., Roth G., Gall S. L., Beare R., Phan T. G., Mikulik R., Akinyemi R. O., Norrving B., Brainin M., Feigin V. L., Abanto C., Abera S. F., Addissie A., Adebayo O., Adeleye A. O., Adilbekov Y., Adilbekova B., Adoukonou T. A., Aguiar de Sousa D., Ajagbe T., Akhmetzhanova Z., Akpalu A., Alvarez Ahlgren J., Ameriso S., Andonova S., Awoniyi F. E., Bakhiet M., Barboza M., Basri H., Bath P., Bello O., Bereczki D., Beretta S., Berkowitz A., Bernabe-Ortiz A., Bernhardt J., Berzina G., Bisharyan M., Bovet P., Budincevic H., Cadilhac D., Caso V., Chen C., Chin J., Chwojnicki K., Conforto A., Cruz V. T., D'Amelio M., Danielyan K., Davis S., Demarin V., Dempsey R., Dichgans M., Dokova K., Donnan G., Elkind M. S., Endres M., Fischer U., Gankpe F., Gaye Saavedra A., Gil A., Giroud M., Gnedovskaya E., Hachinski V., Hafdi M., Hamadeh R., Hamzat T. K., Hankey G., Heldner M., Ibrahim E. A., Ibrahim N. M., Inoue M., Jee S., Jeng J. -S., Kalkonde Y., Kamenova S., Karaszewski B., Kelly P., Khan T., Kiechl S., Kondybayeva A., Korv J., Kravchenko M., Krishnamurthi R. V., Kruja J., Lakkhanaloet M., Langhorne P., Lavados P. M., Law Z. K., Lawal A., Lazo-Porras M., Lebedynets D., Lee T. -H., Leung T., Liebeskind D. S., Lindsay P., Lopez-Jaramillo P., Lotufo P. A., Machline-Carrion J., Makanjuola A., Markus H. S., Marquez-Romero J. M., Medina M., Medukhanova S., Mehndiratta M. M., Merkin A., Mirrakhimov E., Mohl S., Moscoso-Porras M., Muller-Stierlin A., Murphy S., Musa K. I., Nasreldein A., Nogueira R. G., Nolte C., Noubiap J. J., Novarro-Escudero N., Ogun Y., Oguntoye R. A., Oraby M. I., Osundina M., Ovbiagele B., Orken D. N., Ozdemir A. O., Ozturk S., Paccot M., Phromjai J., Piradov P., Platz T., Potpara T., Ranta A., Rathore F., Richard E., Sacco R. L., Sahathevan R., Santos Carquin I., Saposnik G., Sarfo F. S., Sharma M., Sheth K., Shobhana A., Suwanwela N., Svyato I., Sylaja P. N., Tao X., Thakur K. T., Toni D., Topcuoglu M. A., Torales J., Towfighi A., Truelsen T. C., Tsiskaridze A., Tulloch-Reid M., Useche N., Vanacker P., Vassilopoulou S., Vukorepa G., Vuletic V., Wahab K. W., Wang W., Wijeratne T., Wolfe C., Yifru Y. M., Yock-Corrales A., Yonemoto N., Yperzeele L., Zhang P., Owolabi, M, Thrift, A, Mahal, A, Ishida, M, Martins, S, Johnson, W, Pandian, J, Abd-Allah, F, Yaria, J, Phan, H, Roth, G, Gall, S, Beare, R, Phan, T, Mikulik, R, Akinyemi, R, Norrving, B, Brainin, M, Feigin, V, Abanto, C, Abera, S, Addissie, A, Adebayo, O, Adeleye, A, Adilbekov, Y, Adilbekova, B, Adoukonou, T, Aguiar de Sousa, D, Ajagbe, T, Akhmetzhanova, Z, Akpalu, A, Alvarez Ahlgren, J, Ameriso, S, Andonova, S, Awoniyi, F, Bakhiet, M, Barboza, M, Basri, H, Bath, P, Bello, O, Bereczki, D, Beretta, S, Berkowitz, A, Bernabe-Ortiz, A, Bernhardt, J, Berzina, G, Bisharyan, M, Bovet, P, Budincevic, H, Cadilhac, D, Caso, V, Chen, C, Chin, J, Chwojnicki, K, Conforto, A, Cruz, V, D'Amelio, M, Danielyan, K, Davis, S, Demarin, V, Dempsey, R, Dichgans, M, Dokova, K, Donnan, G, Elkind, M, Endres, M, Fischer, U, Gankpe, F, Gaye Saavedra, A, Gil, A, Giroud, M, Gnedovskaya, E, Hachinski, V, Hafdi, M, Hamadeh, R, Hamzat, T, Hankey, G, Heldner, M, Ibrahim, E, Ibrahim, N, Inoue, M, Jee, S, Jeng, J, Kalkonde, Y, Kamenova, S, Karaszewski, B, Kelly, P, Khan, T, Kiechl, S, Kondybayeva, A, Korv, J, Kravchenko, M, Krishnamurthi, R, Kruja, J, Lakkhanaloet, M, Langhorne, P, Lavados, P, Law, Z, Lawal, A, Lazo-Porras, M, Lebedynets, D, Lee, T, Leung, T, Liebeskind, D, Lindsay, P, Lopez-Jaramillo, P, Lotufo, P, Machline-Carrion, J, Makanjuola, A, Markus, H, Marquez-Romero, J, Medina, M, Medukhanova, S, Mehndiratta, M, Merkin, A, Mirrakhimov, E, Mohl, S, Moscoso-Porras, M, Muller-Stierlin, A, Murphy, S, Musa, K, Nasreldein, A, Nogueira, R, Nolte, C, Noubiap, J, Novarro-Escudero, N, Ogun, Y, Oguntoye, R, Oraby, M, Osundina, M, Ovbiagele, B, Orken, D, Ozdemir, A, Ozturk, S, Paccot, M, Phromjai, J, Piradov, P, Platz, T, Potpara, T, Ranta, A, Rathore, F, Richard, E, Sacco, R, Sahathevan, R, Santos Carquin, I, Saposnik, G, Sarfo, F, Sharma, M, Sheth, K, Shobhana, A, Suwanwela, N, Svyato, I, Sylaja, P, Tao, X, Thakur, K, Toni, D, Topcuoglu, M, Torales, J, Towfighi, A, Truelsen, T, Tsiskaridze, A, Tulloch-Reid, M, Useche, N, Vanacker, P, Vassilopoulou, S, Vukorepa, G, Vuletic, V, Wahab, K, Wang, W, Wijeratne, T, Wolfe, C, Yifru, Y, Yock-Corrales, A, Yonemoto, N, Yperzeele, L, Zhang, P, Owolabi M. O., Thrift A. G., Mahal A., Ishida M., Martins S., Johnson W. D., Pandian J., Abd-Allah F., Yaria J., Phan H. T., Roth G., Gall S. L., Beare R., Phan T. G., Mikulik R., Akinyemi R. O., Norrving B., Brainin M., Feigin V. L., Abanto C., Abera S. F., Addissie A., Adebayo O., Adeleye A. O., Adilbekov Y., Adilbekova B., Adoukonou T. A., Aguiar de Sousa D., Ajagbe T., Akhmetzhanova Z., Akpalu A., Alvarez Ahlgren J., Ameriso S., Andonova S., Awoniyi F. E., Bakhiet M., Barboza M., Basri H., Bath P., Bello O., Bereczki D., Beretta S., Berkowitz A., Bernabe-Ortiz A., Bernhardt J., Berzina G., Bisharyan M., Bovet P., Budincevic H., Cadilhac D., Caso V., Chen C., Chin J., Chwojnicki K., Conforto A., Cruz V. T., D'Amelio M., Danielyan K., Davis S., Demarin V., Dempsey R., Dichgans M., Dokova K., Donnan G., Elkind M. S., Endres M., Fischer U., Gankpe F., Gaye Saavedra A., Gil A., Giroud M., Gnedovskaya E., Hachinski V., Hafdi M., Hamadeh R., Hamzat T. K., Hankey G., Heldner M., Ibrahim E. A., Ibrahim N. M., Inoue M., Jee S., Jeng J. -S., Kalkonde Y., Kamenova S., Karaszewski B., Kelly P., Khan T., Kiechl S., Kondybayeva A., Korv J., Kravchenko M., Krishnamurthi R. V., Kruja J., Lakkhanaloet M., Langhorne P., Lavados P. M., Law Z. K., Lawal A., Lazo-Porras M., Lebedynets D., Lee T. -H., Leung T., Liebeskind D. S., Lindsay P., Lopez-Jaramillo P., Lotufo P. A., Machline-Carrion J., Makanjuola A., Markus H. S., Marquez-Romero J. M., Medina M., Medukhanova S., Mehndiratta M. M., Merkin A., Mirrakhimov E., Mohl S., Moscoso-Porras M., Muller-Stierlin A., Murphy S., Musa K. I., Nasreldein A., Nogueira R. G., Nolte C., Noubiap J. J., Novarro-Escudero N., Ogun Y., Oguntoye R. A., Oraby M. I., Osundina M., Ovbiagele B., Orken D. N., Ozdemir A. O., Ozturk S., Paccot M., Phromjai J., Piradov P., Platz T., Potpara T., Ranta A., Rathore F., Richard E., Sacco R. L., Sahathevan R., Santos Carquin I., Saposnik G., Sarfo F. S., Sharma M., Sheth K., Shobhana A., Suwanwela N., Svyato I., Sylaja P. N., Tao X., Thakur K. T., Toni D., Topcuoglu M. A., Torales J., Towfighi A., Truelsen T. C., Tsiskaridze A., Tulloch-Reid M., Useche N., Vanacker P., Vassilopoulou S., Vukorepa G., Vuletic V., Wahab K. W., Wang W., Wijeratne T., Wolfe C., Yifru Y. M., Yock-Corrales A., Yonemoto N., Yperzeele L., and Zhang P.
Abstract: Stroke is the second leading cause of death and the third leading cause of disability worldwide and its burden is increasing rapidly in low-income and middle-income countries, many of which are unable to face the challenges it imposes. In this Health Policy paper on primary stroke prevention, we provide an overview of the current situation regarding primary prevention services, estimate the cost of stroke and stroke prevention, and identify deficiencies in existing guidelines and gaps in primary prevention. We also offer a set of pragmatic solutions for implementation of primary stroke prevention, with an emphasis on the role of governments and population-wide strategies, including task-shifting and sharing and health system re-engineering. Implementation of primary stroke prevention involves patients, health professionals, funders, policy makers, implementation partners, and the entire population along the life course.
Published: 2022

4. The design and performance of the XL-Calibur anticoincidence shield

Author: Iyer, Nirmal, Kiss, M., Pearce, Mark, Stana, T. -A., Awaki, H., Bose, R. G., Dasgupta, A., De Geronimo, G., Gau, E., Hakamata, T., Ishida, M., Ishiwata, K., Kamogawa, W., Kislat, F., Kitaguchi, T., Krawczynski, H., Lisalda, L., Maeda, Y., Matsumoto, H., Miyamoto, A., Miyazawa, T., Mizuno, T., Rauch, B. F., Cavero, N. Rodriguez, Sakamoto, N., Sato, J., Spooner, S., Takahashi, H., Takeo, M., Tamagawa, T., Uchida, Y., West, A. T., Wimalasena, K., Yoshimoto, M., Iyer, Nirmal, Kiss, M., Pearce, Mark, Stana, T. -A., Awaki, H., Bose, R. G., Dasgupta, A., De Geronimo, G., Gau, E., Hakamata, T., Ishida, M., Ishiwata, K., Kamogawa, W., Kislat, F., Kitaguchi, T., Krawczynski, H., Lisalda, L., Maeda, Y., Matsumoto, H., Miyamoto, A., Miyazawa, T., Mizuno, T., Rauch, B. F., Cavero, N. Rodriguez, Sakamoto, N., Sato, J., Spooner, S., Takahashi, H., Takeo, M., Tamagawa, T., Uchida, Y., West, A. T., Wimalasena, K., and Yoshimoto, M.
Abstract: The XL-Calibur balloon-borne hard X-ray polarimetry mission comprises a Compton-scattering polarimeter placed at the focal point of an X-ray mirror. The polarimeter is housed within a BGO anticoincidence shield, which is needed to mitigate the considerable background radiation present at the observation altitude of -40 km. This paper details the design, construction and testing of the anticoincidence shield, as well as the performance measured during the week-long maiden flight from Esrange Space Centre to the Canadian Northwest Territories in July 2022. The in-flight performance of the shield followed design expectations, with a veto threshold <100 keV and a measured background rate of -0.5 Hz (20-40 keV). This is compatible with the scientific goals of the mission, where %-level minimum detectable polarisation is sought for a Hz-level source rate.
Published: 2023
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5. Scaling slowly rotating asteroids by stellar occultations

Author: Marciniak, A., Ďurech, J., Choukroun, A., Hanuš, J., Ogłoza, W., Szakáts, R., Molnár, L., Pál, A., Monteiro, F., Frappa, E., Beisker, W., Pavlov, H., Moore, J., Adomavičienė, R., Aikawa, R., Andersson, S., Antonini, P., Argentin, Y., Asai, A., Assoignon, P., Barton, J., Baruffetti, P., Bath, K. L., Behrend, R., Benedyktowicz, L., Bernasconi, L., Biguet, G., Billiani, M., Błażewicz, D., Boninsegna, R., Borkowski, M., Bosch, J., Brazill, S., Bronikowska, M., Bruno, A., Bąk, M. Butkiewicz, Caron, J., Casalnuovo, G., Castellani, J. J., Ceravolo, P., Conjat, M., Delincak, P., Delpau, J., Demeautis, C., Demirkol, A., Dróżdż, M., Duffard, R., Durandet, C., Eisfeldt, D., Evangelista, M., Fauvaud, S., Fauvaud, M., Ferrais, M., Filipek, M., Fini, P., Fukui, K., Gährken, B., Geier, S., George, T., Goffin, B., Golonka, J., Goto, T., Grice, J., Guhl, K., Halíř, K., Hanna, W., Harman, M., Hashimoto, A., Hasubick, W., Higgins, D., Higuchi, M., Hirose, T., Hirsch, R., Hofschulz, O., Horaguchi, T., Horbowicz, J., Ida, M., Ignácz, B., Ishida, M., Isobe, K., Jehin, E., Joachimczyk, B., Jones, A., Juan, J., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kasebe, H., Kattentidt, B., Kim, D. -H., Kim, M. -J., Kitazaki, K., Klotz, A., Komraus, M., Konstanciak, I., Tóth, R. Könyves, Kouno, K., Kowald, E., Krajewski, J., Krannich, G., Kreutzer, A., Kryszczyńska, A., Kubánek, J., Kudak, V., Kugel, F., Kukita, R., Kulczak, P., Lazzaro, D., Licandro, J., Livet, F., Maley, P., Manago, N., Mánek, J., Manna, A., Matsushita, H., Meister, S., Mesquita, W., Messner, S., Michelet, J., Michimani, J., Mieczkowska, I., Morales, N., Motyliński, M., Murawiecka, M., Newman, J., Nikitin, V., Nishimura, M., Oey, J., Oszkiewicz, D., Owada, M., Pakštienė, E., Pawłowski, M., Pereira, W., Perig, V., Perła, J., Pilcher, F., Podlewska-Gaca, E., Polák, J., Polakis, T., Polińska, M., Popowicz, A., Richard, F., Rives, J. J., Rodrigues, T., Rogiński, Ł., Rondón, E., Rottenborn, M., Schäfer, R., Schnabel, C., Schreurs, O., Selva, A., Simon, M., Skiff, B., Skrutskie, M., Skrzypek, J., Sobkowiak, K., Sonbas, E., Sposetti, S., Stuart, P., Szyszka, K., Terakubo, K., Thomas, W., Trela, P., Uchiyama, S., Urbanik, M., Vaudescal, G., Venable, R., Watanabe, Ha., Watanabe, Hi., Winiarski, M., Wróblewski, R., Yamamura, H., Yamashita, M., Yoshihara, H., Zawilski, M., Zelený, P., Żejmo, M., Żukowski, K., Żywica, S., Marciniak, A., Ďurech, J., Choukroun, A., Hanuš, J., Ogłoza, W., Szakáts, R., Molnár, L., Pál, A., Monteiro, F., Frappa, E., Beisker, W., Pavlov, H., Moore, J., Adomavičienė, R., Aikawa, R., Andersson, S., Antonini, P., Argentin, Y., Asai, A., Assoignon, P., Barton, J., Baruffetti, P., Bath, K. L., Behrend, R., Benedyktowicz, L., Bernasconi, L., Biguet, G., Billiani, M., Błażewicz, D., Boninsegna, R., Borkowski, M., Bosch, J., Brazill, S., Bronikowska, M., Bruno, A., Bąk, M. Butkiewicz, Caron, J., Casalnuovo, G., Castellani, J. J., Ceravolo, P., Conjat, M., Delincak, P., Delpau, J., Demeautis, C., Demirkol, A., Dróżdż, M., Duffard, R., Durandet, C., Eisfeldt, D., Evangelista, M., Fauvaud, S., Fauvaud, M., Ferrais, M., Filipek, M., Fini, P., Fukui, K., Gährken, B., Geier, S., George, T., Goffin, B., Golonka, J., Goto, T., Grice, J., Guhl, K., Halíř, K., Hanna, W., Harman, M., Hashimoto, A., Hasubick, W., Higgins, D., Higuchi, M., Hirose, T., Hirsch, R., Hofschulz, O., Horaguchi, T., Horbowicz, J., Ida, M., Ignácz, B., Ishida, M., Isobe, K., Jehin, E., Joachimczyk, B., Jones, A., Juan, J., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kasebe, H., Kattentidt, B., Kim, D. -H., Kim, M. -J., Kitazaki, K., Klotz, A., Komraus, M., Konstanciak, I., Tóth, R. Könyves, Kouno, K., Kowald, E., Krajewski, J., Krannich, G., Kreutzer, A., Kryszczyńska, A., Kubánek, J., Kudak, V., Kugel, F., Kukita, R., Kulczak, P., Lazzaro, D., Licandro, J., Livet, F., Maley, P., Manago, N., Mánek, J., Manna, A., Matsushita, H., Meister, S., Mesquita, W., Messner, S., Michelet, J., Michimani, J., Mieczkowska, I., Morales, N., Motyliński, M., Murawiecka, M., Newman, J., Nikitin, V., Nishimura, M., Oey, J., Oszkiewicz, D., Owada, M., Pakštienė, E., Pawłowski, M., Pereira, W., Perig, V., Perła, J., Pilcher, F., Podlewska-Gaca, E., Polák, J., Polakis, T., Polińska, M., Popowicz, A., Richard, F., Rives, J. J., Rodrigues, T., Rogiński, Ł., Rondón, E., Rottenborn, M., Schäfer, R., Schnabel, C., Schreurs, O., Selva, A., Simon, M., Skiff, B., Skrutskie, M., Skrzypek, J., Sobkowiak, K., Sonbas, E., Sposetti, S., Stuart, P., Szyszka, K., Terakubo, K., Thomas, W., Trela, P., Uchiyama, S., Urbanik, M., Vaudescal, G., Venable, R., Watanabe, Ha., Watanabe, Hi., Winiarski, M., Wróblewski, R., Yamamura, H., Yamashita, M., Yoshihara, H., Zawilski, M., Zelený, P., Żejmo, M., Żukowski, K., and Żywica, S.
Abstract: As evidenced by recent survey results, majority of asteroids are slow rotators (P>12 h), but lack spin and shape models due to selection bias. This bias is skewing our overall understanding of the spins, shapes, and sizes of asteroids, as well as of their other properties. Also, diameter determinations for large (>60km) and medium-sized asteroids (between 30 and 60 km) often vary by over 30% for multiple reasons. Our long-term project is focused on a few tens of slow rotators with periods of up to 60 hours. We aim to obtain their full light curves and reconstruct their spins and shapes. We also precisely scale the models, typically with an accuracy of a few percent. We used wide sets of dense light curves for spin and shape reconstructions via light-curve inversion. Precisely scaling them with thermal data was not possible here because of poor infrared data: large bodies are too bright for WISE mission. Therefore, we recently launched a campaign among stellar occultation observers, to scale these models and to verify the shape solutions, often allowing us to break the mirror pole ambiguity. The presented scheme resulted in shape models for 16 slow rotators, most of them for the first time. Fitting them to stellar occultations resolved previous inconsistencies in size determinations. For around half of the targets, this fitting also allowed us to identify a clearly preferred pole solution, thus removing the ambiguity inherent to light-curve inversion. We also address the influence of the uncertainty of the shape models on the derived diameters. Overall, our project has already provided reliable models for around 50 slow rotators. Such well-determined and scaled asteroid shapes will, e.g. constitute a solid basis for density determinations when coupled with mass information. Spin and shape models continue to fill the gaps caused by various biases., Comment: Accepted to Astronomy & Astrophysics. 12 pages + appendices
Published: 2023
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6. Primary stroke prevention worldwide: translating evidence into action.

Author: Owolabi M.O., Thrift A.G., Mahal A., Ishida M., Martins S., Johnson W.D., Pandian J., Abd-Allah F., Yaria J., Phan H.T., Roth G., Gall S.L., Beare R., Phan T.G., Mikulik R., Akinyemi R.O., Norrving B., Brainin M., Feigin V.L., Abanto C., Abera S.F., Addissie A., Adebayo O., Adeleye A.O., Adilbekov Y., Adilbekova B., Adoukonou T.A., Aguiar de Sousa D., Ajagbe T., Akhmetzhanova Z., Akpalu A., Alvarez Ahlgren J., Ameriso S., Andonova S., Awoniyi F.E., Bakhiet M., Barboza M., Basri H., Bath P., Bello O., Bereczki D., Beretta S., Berkowitz A., Bernabe-Ortiz A., Bernhardt J., Berzina G., Bisharyan M., Bovet P., Budincevic H., Cadilhac D., Caso V., Chen C., Chin J., Chwojnicki K., Conforto A., Cruz V.T., D'Amelio M., Danielyan K., Davis S., Demarin V., Dempsey R., Dichgans M., Dokova K., Donnan G., Elkind M.S., Endres M., Fischer U., Gankpe F., Gaye Saavedra A., Gil A., Giroud M., Gnedovskaya E., Hachinski V., Hafdi M., Hamadeh R., Hamzat T.K., Hankey G., Heldner M., Ibrahim E.A., Ibrahim N.M., Inoue M., Jee S., Jeng J.-S., Kalkonde Y., Kamenova S., Karaszewski B., Kelly P., Khan T., Kiechl S., Kondybayeva A., Korv J., Kravchenko M., Krishnamurthi R.V., Kruja J., Lakkhanaloet M., Langhorne P., Lavados P.M., Law Z.K., Lawal A., Lazo-Porras M., Lebedynets D., Lee T.-H., Leung T., Liebeskind D.S., Lindsay P., Lopez-Jaramillo P., Lotufo P.A., Machline-Carrion J., Makanjuola A., Markus H.S., Marquez-Romero J.M., Medina M., Medukhanova S., Mehndiratta M.M., Merkin A., Mirrakhimov E., Mohl S., Moscoso-Porras M., Muller-Stierlin A., Murphy S., Musa K.I., Nasreldein A., Nogueira R.G., Nolte C., Noubiap J.J., Novarro-Escudero N., Ogun Y., Oguntoye R.A., Oraby M.I., Osundina M., Ovbiagele B., Orken D.N., Ozdemir A.O., Ozturk S., Paccot M., Phromjai J., Piradov P., Platz T., Potpara T., Ranta A., Rathore F., Richard E., Sacco R.L., Sahathevan R., Santos Carquin I., Saposnik G., Sarfo F.S., Sharma M., Sheth K., Shobhana A., Suwanwela N., Svyato I., Sylaja P.N., Tao X., Thakur K.T., Toni D., Topcuoglu M.A., Torales J., Towfighi A., Truelsen T.C., Tsiskaridze A., Tulloch-Reid M., Useche N., Vanacker P., Vassilopoulou S., Vukorepa G., Vuletic V., Wahab K.W., Wang W., Wijeratne T., Wolfe C., Yifru Y.M., Yock-Corrales A., Yonemoto N., Yperzeele L., Zhang P., Owolabi M.O., Thrift A.G., Mahal A., Ishida M., Martins S., Johnson W.D., Pandian J., Abd-Allah F., Yaria J., Phan H.T., Roth G., Gall S.L., Beare R., Phan T.G., Mikulik R., Akinyemi R.O., Norrving B., Brainin M., Feigin V.L., Abanto C., Abera S.F., Addissie A., Adebayo O., Adeleye A.O., Adilbekov Y., Adilbekova B., Adoukonou T.A., Aguiar de Sousa D., Ajagbe T., Akhmetzhanova Z., Akpalu A., Alvarez Ahlgren J., Ameriso S., Andonova S., Awoniyi F.E., Bakhiet M., Barboza M., Basri H., Bath P., Bello O., Bereczki D., Beretta S., Berkowitz A., Bernabe-Ortiz A., Bernhardt J., Berzina G., Bisharyan M., Bovet P., Budincevic H., Cadilhac D., Caso V., Chen C., Chin J., Chwojnicki K., Conforto A., Cruz V.T., D'Amelio M., Danielyan K., Davis S., Demarin V., Dempsey R., Dichgans M., Dokova K., Donnan G., Elkind M.S., Endres M., Fischer U., Gankpe F., Gaye Saavedra A., Gil A., Giroud M., Gnedovskaya E., Hachinski V., Hafdi M., Hamadeh R., Hamzat T.K., Hankey G., Heldner M., Ibrahim E.A., Ibrahim N.M., Inoue M., Jee S., Jeng J.-S., Kalkonde Y., Kamenova S., Karaszewski B., Kelly P., Khan T., Kiechl S., Kondybayeva A., Korv J., Kravchenko M., Krishnamurthi R.V., Kruja J., Lakkhanaloet M., Langhorne P., Lavados P.M., Law Z.K., Lawal A., Lazo-Porras M., Lebedynets D., Lee T.-H., Leung T., Liebeskind D.S., Lindsay P., Lopez-Jaramillo P., Lotufo P.A., Machline-Carrion J., Makanjuola A., Markus H.S., Marquez-Romero J.M., Medina M., Medukhanova S., Mehndiratta M.M., Merkin A., Mirrakhimov E., Mohl S., Moscoso-Porras M., Muller-Stierlin A., Murphy S., Musa K.I., Nasreldein A., Nogueira R.G., Nolte C., Noubiap J.J., Novarro-Escudero N., Ogun Y., Oguntoye R.A., Oraby M.I., Osundina M., Ovbiagele B., Orken D.N., Ozdemir A.O., Ozturk S., Paccot M., Phromjai J., Piradov P., Platz T., Potpara T., Ranta A., Rathore F., Richard E., Sacco R.L., Sahathevan R., Santos Carquin I., Saposnik G., Sarfo F.S., Sharma M., Sheth K., Shobhana A., Suwanwela N., Svyato I., Sylaja P.N., Tao X., Thakur K.T., Toni D., Topcuoglu M.A., Torales J., Towfighi A., Truelsen T.C., Tsiskaridze A., Tulloch-Reid M., Useche N., Vanacker P., Vassilopoulou S., Vukorepa G., Vuletic V., Wahab K.W., Wang W., Wijeratne T., Wolfe C., Yifru Y.M., Yock-Corrales A., Yonemoto N., Yperzeele L., and Zhang P.
Abstract: Stroke is the second leading cause of death and the third leading cause of disability worldwide and its burden is increasing rapidly in low-income and middle-income countries, many of which are unable to face the challenges it imposes. In this Health Policy paper on primary stroke prevention, we provide an overview of the current situation regarding primary prevention services, estimate the cost of stroke and stroke prevention, and identify deficiencies in existing guidelines and gaps in primary prevention. We also offer a set of pragmatic solutions for implementation of primary stroke prevention, with an emphasis on the role of governments and population-wide strategies, including task-shifting and sharing and health system re-engineering. Implementation of primary stroke prevention involves patients, health professionals, funders, policy makers, implementation partners, and the entire population along the life course.Copyright © 2022 The Author(s). Published by Elsevier Ltd. This is an Open Access article under the CC BY 4.0 license
Published: 2022

7. Out-Of-Pocket Expenditure Associated with Physical Inactivity, Excessive Weight, and Obesity in China: Quantile Regression Approach

Author: Zhao, Y, He, L, Marthias, T, Ishida, M, Anindya, K, Desloge, A, D'Souza, M, Cao, G, Lee, JT, Zhao, Y, He, L, Marthias, T, Ishida, M, Anindya, K, Desloge, A, D'Souza, M, Cao, G, and Lee, JT
Abstract: INTRODUCTION: Previous studies exploring associations of physical inactivity, obesity, and out-of-pocket expenditure (OOPE) mainly used traditional linear regression, and little is known about the effect of both physical inactivity and obesity on OOPE across the percentile distribution. This study aims to assess the effects of physical inactivity and obesity on OOPE in China using a quantile regression approach. METHODS: Study participants included 10,687 respondents aged 45 years and older from the recent wave of the China Health and Retirement Longitudinal Study in 2015. Linear regression and quantile regression models were used to examine the association of physical activity, body weight with annual OOPE. RESULTS: Overall, the proportion of overweight and obesity was 33.2% and 5.8%, respectively. The proportion of individuals performing high-level, moderate-level, and low-level physical activity was 55.2%, 12.7%, and 32.1%, respectively. The effects of low-level physical activity on annual OOPE were small at the bottom quantiles but more pronounced at higher quantiles. Respondents with low-level activity had an increased annual OOPE of 26.9 USD, 150.3 USD, and 1,534.4 USD, at the 10th, 50th, and 90th percentiles, respectively, compared with those with high-level activity. The effects of overweight and obesity on OOPE were also small at the bottom quantiles but more pronounced at higher quantiles. CONCLUSION: Interventions that improve the lifestyles and unhealthy behaviors among people with obesity and physical inactivity are likely to yield substantial financial gains for the individual and health systems in China.
Published: 2022

8. Witnessing Intimate Partner Violence Impacts Schooling and Labor Market Outcomes for Young Women in India

Author: Ludwick, T, Ishida, M, Desai, S, Mahal, A, Ludwick, T, Ishida, M, Desai, S, and Mahal, A
Abstract: Intimate partner violence (IPV) is a major health and social issue that affects around 30 percent of women globally. This study investigates the relationships through which witnessing IPV in adolescence may impact the labor force participation and employment prospects of women in early adulthood, using a unique dataset from Bihar (India), which surveyed youth (primarily girls) in adolescence and again nine years later. The study examined the relationship between exposure to IPV and labor market outcomes among young women, including intermediate factors likely to influence their employment prospects, such as educational attainment, self-efficacy, mental health, and soft skills. Witnessing IPV as an adolescent had a negative effect on educational attainment, mental health, and social and behavioral aspects of young women almost nine years later. IPV was not associated with the likelihood of paid employment or participation in skilled work among women, although it was associated with higher levels of labor force participation. These findings suggest that witnessing IPV should be considered one of multiple forms of violence that may expose young women to longer term vulnerability related to poorer educational and employment prospects, mental health, and social networks, with implications for economic and social development far beyond the family.
Published: 2022

9. Primary stroke prevention worldwide: translating evidence into action

Author: Owolabi, MO, Thrift, AG, Mahal, A, Ishida, M, Martins, S, Johnson, W, Pandian, J, Abd-Allah, F, Yaria, J, Phan, HT, Roth, G, Gall, SL, Beare, R, Phan, TG, Mikulik, R, Akinyemi, RO, Norrving, B, Brainin, M, Feigin, VL, Owolabi, MO, Thrift, AG, Mahal, A, Ishida, M, Martins, S, Johnson, W, Pandian, J, Abd-Allah, F, Yaria, J, Phan, HT, Roth, G, Gall, SL, Beare, R, Phan, TG, Mikulik, R, Akinyemi, RO, Norrving, B, Brainin, M, and Feigin, VL
Abstract: Stroke is the second leading cause of death and the third leading cause of disability worldwide and its burden is increasing rapidly in low-income and middle-income countries, many of which are unable to face the challenges it imposes. In this Health Policy paper on primary stroke prevention, we provide an overview of the current situation regarding primary prevention services, estimate the cost of stroke and stroke prevention, and identify deficiencies in existing guidelines and gaps in primary prevention. We also offer a set of pragmatic solutions for implementation of primary stroke prevention, with an emphasis on the role of governments and population-wide strategies, including task-shifting and sharing and health system re-engineering. Implementation of primary stroke prevention involves patients, health professionals, funders, policy makers, implementation partners, and the entire population along the life course.
Published: 2022

10. Mineralogy, geochemistry and microbiology insights into precipitation of stibnite and orpiment at the Daiyon-Yonaguni Knoll (Okinawa Trough) hydrothermal barite deposits

Author: Dekov, V.M., Kyono, K., Yasukawa, K., Guéguen, B., Ivarsson, Magnus, Kamenov, G.D., Yamanaka, T., Asael, D., Ishida, M., Cavalcante, L.L., Kato, Y., Toki, T., Ishibashi, J.-I., Dekov, V.M., Kyono, K., Yasukawa, K., Guéguen, B., Ivarsson, Magnus, Kamenov, G.D., Yamanaka, T., Asael, D., Ishida, M., Cavalcante, L.L., Kato, Y., Toki, T., and Ishibashi, J.-I.
Abstract: Samples of active chimneys, chimney flanges and massive sulfides from the Daiyon-Yonaguni Knoll hydrothermal field are composed of major barite and minor stibnite and orpiment. Barite is inferred to precipitate from focused-discharge fluids composed of >40% hydrothermal end-member fluid at T = 100-240°C, whereas the stibnite and orpiment are later and lower temperature precipitates. The hydrothermal fluids from this field were subject of sub-seafloor boiling and phase separation and, consequently, are brine-rich depleted in volatile and enriched in non-volatile elements. Boiling and phase separation exerted major control on the rare earth elements (REE) partitioning in the vent fluids: high-chlorinity high-temperature fluids were enriched in light REE and low-chlorinity low-temperature fluids were enriched in heavy REE. Y/Ho molar ratio and Ce anomaly of the vent fluids suggest that the seawater has not completely reacted with the basement rocks and has not equilibrated with them. The trace element concentrations in the hydrothermal deposits suggest a complex interplay among hydrothermal, hydrogenetic and microbial processes. Sulfur isotope composition of the sulfides suggests that the sulfide S is a mixture of both basement rock and seawater S with a higher proportion of the basement rock S. The sulfate dissolved in the fluids was subjected to reduction during a slow mixing of hydrothermal fluid and seawater within the chimney walls of the Tiger and Abyss vents and this resulted in a heavy S-isotope composition of the vent fluid sulfate. Lead isotope composition of the hydrothermal deposits indicates mixing relationships suggesting that Pb and potentially other metals with similar geochemical behavior were derived from two or three sources. The Pb isotopes in the hydrothermal deposits imply that an enriched source, either sediments or extended continental lithosphere, and a depleted source, potentially back-arc mafic volcanics, are present in the area of Daiyon
Published: 2022
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11. Epidemiology of physical-mental multimorbidity and its impact among Aboriginal and Torres Strait Islander in Australia: a cross-sectional analysis of a nationally representative sample

Author: Carman, W, Ishida, M, Trounson, JS, Mercer, SW, Anindya, K, Sum, G, Armstrong, G, Oldenburg, B, McPake, B, Lee, JT, Carman, W, Ishida, M, Trounson, JS, Mercer, SW, Anindya, K, Sum, G, Armstrong, G, Oldenburg, B, McPake, B, and Lee, JT
Abstract: OBJECTIVES: This study aimed to examine the differences in multimorbidity between Aboriginal and Torres Strait Islander people and non-Indigenous Australians, and the effect of multimorbidity on health service use and work productivity. SETTING: Cross-sectional sample of the Household, Income and Labour Dynamics in Australia wave 17. PARTICIPANTS: A nationally representative sample of 16 749 respondents aged 18 years and above. OUTCOME MEASURES: Multimorbidity prevalence and pattern, self-reported health, health service use and employment productivity by Indigenous status. RESULTS: Aboriginal respondents reported a higher prevalence of multimorbidity (24.2%) compared with non-Indigenous Australians (20.7%), and the prevalence of mental-physical multimorbidity was almost twice as high (16.1% vs 8.1%). Multimorbidity pattern varies significantly among the Aboriginal and non-Indigenous Australians. Multimorbidity was associated with higher health service use (any overnight admission: adjusted OR=1.52, 95% CI=1.46 to 1.58), reduced employment productivity (days of sick leave: coefficient=0.25, 95% CI=0.19 to 0.31) and lower perceived health status (SF6D score: coefficient=-0.04, 95% CI=-0.05 to -0.04). These associations were found to be comparable in both Aboriginal and non-Indigenous populations. CONCLUSIONS: Multimorbidity prevalence was significantly greater among Aboriginal and Torres Strait Islanders compared with the non-Indigenous population, especially mental-physical multimorbidity. Strategies are required for better prevention and management of multimorbidity for the aboriginal population to reduce health inequalities in Australia.
Published: 2022

12. The design and performance of the XL-Calibur anticoincidence shield

Author: Iyer, N. K., Kiss, M., Pearce, M., Stana, T. -A., Awaki, H., Bose, R. G., Dasgupta, A., De Geronimo, G., Gau, E., Hakamata, T., Ishida, M., Ishiwata, K., Kamogawa, W., Kislat, F., Kitaguchi, T., Krawczynski, H., Lisalda, L., Maeda, Y., Matsumoto, H., Miyamoto, A., Miyazawa, T., Mizuno, T., Rauch, B. F., Cavero, N. Rodriguez, Sakamoto, N., Sato, J., Spooner, S., Takahashi, H., Takeo, M., Tamagawa, T., Uchida, Y., West, A. T., Wimalasena, K., Yoshimoto, M., Iyer, N. K., Kiss, M., Pearce, M., Stana, T. -A., Awaki, H., Bose, R. G., Dasgupta, A., De Geronimo, G., Gau, E., Hakamata, T., Ishida, M., Ishiwata, K., Kamogawa, W., Kislat, F., Kitaguchi, T., Krawczynski, H., Lisalda, L., Maeda, Y., Matsumoto, H., Miyamoto, A., Miyazawa, T., Mizuno, T., Rauch, B. F., Cavero, N. Rodriguez, Sakamoto, N., Sato, J., Spooner, S., Takahashi, H., Takeo, M., Tamagawa, T., Uchida, Y., West, A. T., Wimalasena, K., and Yoshimoto, M.
Abstract: The XL-Calibur balloon-borne hard X-ray polarimetry mission comprises a Compton-scattering polarimeter placed at the focal point of an X-ray mirror. The polarimeter is housed within a BGO anticoincidence shield, which is needed to mitigate the considerable background radiation present at the observation altitude of ~40 km. This paper details the design, construction and testing of the anticoincidence shield, as well as the performance measured during the week-long maiden flight from Esrange Space Centre to the Canadian Northwest Territories in July 2022. The in-flight performance of the shield followed design expectations, with a veto threshold <100 keV and a measured background rate of ~0.5 Hz (20-40 keV). This is compatible with the scientific goals of the mission, where %-level minimum detectable polarisation is sought for a Hz-level source rate., Comment: Submitted to Nuclear Instruments and Methods A
Published: 2022
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13. Pb isotopic constraints on the genesis of the Toyoha indium-bearing polymetallic deposit, Hokkaido, Japan.

Author: Ishida M., Araki S., Fujinaga K., Hieda Y., Iwamori H., Kato Y., Nakamura H., Shimizu T., Tanimzu M., Ishida M., Araki S., Fujinaga K., Hieda Y., Iwamori H., Kato Y., Nakamura H., Shimizu T., and Tanimzu M.
Abstract: The Toyoha epithermal polymetallic deposit has produced 4 700 t indium and used to be the largest indium producer in the world in the 1990s. The Pb isotopic composition of sulphides (sphalerite, galena, pyrite and wurtzite) was investigated from the indium-poor, earlier veins and the indium-rich later veins, together with the volcanic and sedimentary rocks in the Toyoha area. Data show that the Pb isotopic composition of the earlier veins fall within the range of volcanic rocks of the Toyoha area. On the other hand, the later veins yield isotopic compositions between the Toyoha volcanic rocks and the quaternary basalt of SW Hokkaido. This suggests that the sulphide and igneous rocks share a common source; e.g., Pb in both the sulphide and the magmas was derived from a deep geofluid from the subducted Pacific plate or, a fluid expelled at relatively shallow depths from the magmas significantly contributed to the ore forming fluid and metals, including the indium-rich later veins of the Toyoha deposit., The Toyoha epithermal polymetallic deposit has produced 4 700 t indium and used to be the largest indium producer in the world in the 1990s. The Pb isotopic composition of sulphides (sphalerite, galena, pyrite and wurtzite) was investigated from the indium-poor, earlier veins and the indium-rich later veins, together with the volcanic and sedimentary rocks in the Toyoha area. Data show that the Pb isotopic composition of the earlier veins fall within the range of volcanic rocks of the Toyoha area. On the other hand, the later veins yield isotopic compositions between the Toyoha volcanic rocks and the quaternary basalt of SW Hokkaido. This suggests that the sulphide and igneous rocks share a common source; e.g., Pb in both the sulphide and the magmas was derived from a deep geofluid from the subducted Pacific plate or, a fluid expelled at relatively shallow depths from the magmas significantly contributed to the ore forming fluid and metals, including the indium-rich later veins of the Toyoha deposit.
Published: 2021

14. Impact of non-communicable disease multimorbidity on health service use, catastrophic health expenditure and productivity loss in Indonesia: a population-based panel data analysis study

Author: Marthias, T, Anindya, K, Ng, N, McPake, B, Atun, R, Arfyanto, H, Hulse, ESG, Zhao, Y, Jusril, H, Pan, T, Ishida, M, Lee, JT, Marthias, T, Anindya, K, Ng, N, McPake, B, Atun, R, Arfyanto, H, Hulse, ESG, Zhao, Y, Jusril, H, Pan, T, Ishida, M, and Lee, JT
Abstract: OBJECTIVES: To examine non-communicable diseases (NCDs) multimorbidity level and its relation to households' socioeconomic characteristics, health service use, catastrophic health expenditures and productivity loss. DESIGN: This study used panel data of the Indonesian Family Life Survey conducted in 2007 (Wave 4) and 2014 (Wave 5). SETTING: The original sampling frame was based on 13 out of 27 provinces in 1993, representing 83% of the Indonesian population. PARTICIPANTS: We included respondents aged 50 years and above in 2007, excluding those who did not participate in both Waves 4 and 5. The total number of participants in this study are 3678 respondents. PRIMARY OUTCOME MEASURES: We examined three main outcomes; health service use (outpatient and inpatient care), financial burden (catastrophic health expenditure) and productivity loss (labour participation, days primary activity missed, days confined in bed). We applied multilevel mixed-effects regression models to assess the associations between NCD multimorbidity and outcome variables, RESULTS: Women were more likely to have NCD multimorbidity than men and the prevalence of NCD multimorbidity increased with higher socioeconomic status. NCD multimorbidity was associated with a higher number of outpatient visits (compared with those without NCD, incidence rate ratio (IRR) 4.25, 95% CI 3.33 to 5.42 for individuals with >3 NCDs) and inpatient visits (IRR 3.68, 95% CI 2.21 to 6.12 for individuals with >3 NCDs). NCD multimorbidity was also associated with a greater likelihood of experiencing catastrophic health expenditure (for >3 NCDs, adjusted OR (aOR) 1.69, 95% CI 1.02 to 2.81) and lower participation in the labour force (aOR 0.23, 95% CI 0.16 to 0.33) compared with no NCD. CONCLUSIONS: NCD multimorbidity is associated with substantial direct and indirect costs to individuals, households and the wider society. Our study highlights the importance of preparing health systems for addressing the burden of multimorbidi
Published: 2021

15. Efficacy of duloxetine in patients with knee osteoarthritis or chronic low back pain with early pain reduction: An exploratory post-hoc analysis of Japanese phase 3, 1-year extension studies

Author: Itoh N, Uchio Y, Tsuji T, Ishida M, Ochiai T, Konno S., Uchio, Yuji, Itoh N, Uchio Y, Tsuji T, Ishida M, Ochiai T, Konno S., and Uchio, Yuji
Published: 2021

16. N-Confused Phlorin-Prodigiosin Chimera : meso-Aryl Oxidation and π-Extension Triggered by Peripheral Coordination

Author: Su, G., Li, Q., Ishida, M., Li, C., Sha, F., Wu, X. -Y, Wang, L., Baryshnikov, Gleb V., Li, D., Ågren, Hans, Furuta, H., Xie, Y., Su, G., Li, Q., Ishida, M., Li, C., Sha, F., Wu, X. -Y, Wang, L., Baryshnikov, Gleb V., Li, D., Ågren, Hans, Furuta, H., and Xie, Y.
Abstract: An N-confused phlorin isomer bearing a dipyrrin moiety at the α-position of the confused pyrrole ring (1) was synthesized. PdII and BIII coordination at the peripheral prodigiosin-like moiety of 1 afforded the corresponding complexes 2 and 3. Reflux of 2 in triethylamine (TEA) converted the meso-phenyl into the PdII-coordinating phenoxy group to afford 4. Under the same reaction conditions, TEA was linked to the α-position of the dipyrrin unit in 3 as an N,N-diethylaminovinyl group to afford 5. Furthermore, peripheral coordination of BIII in 3 and 5 improved the planarity of the phlorin macrocycle and thus facilitated the coordination of AgIII at the inner cavity to afford 3-Ag and 5-Ag, respectively. These results provide an effective approach for developing unique porphyrinoids through peripheral coordination., QC 20200424
Published: 2020
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17. The Joint Effect of Physical Multimorbidity and Mental Health Conditions Among Adults in Australia

Author: Ishida, M, Hulse, ESG, Mahar, RK, Gunn, J, Atun, R, McPake, B, Tenneti, N, Anindya, K, Armstrong, G, Mulcahy, P, Carman, W, Lee, JT, Ishida, M, Hulse, ESG, Mahar, RK, Gunn, J, Atun, R, McPake, B, Tenneti, N, Anindya, K, Armstrong, G, Mulcahy, P, Carman, W, and Lee, JT
Abstract: INTRODUCTION: The prevalence of chronic physical and mental health conditions is rising globally. Little evidence exists on the joint effect of physical and mental health conditions on health care use, work productivity, and health-related quality of life in Australia. METHODS: We analyzed data from the Household, Income and Labour Dynamics in Australia (HILDA) Survey, waves 9 (2009), 13 (2013), and 17 (2017). Economic effects associated with multimorbidity were measured through health service use, work productivity loss, and health-related quality of life. We used generalized estimating equations to assess the effect of the association between physical multimorbidity and mental health conditions and economic outcomes. RESULTS: From 2009 through 2017 the prevalence of physical multimorbidity increased from 15.1% to 16.2%, and the prevalence of mental health conditions increased from 11.2% to 17.3%. The number of physical health conditions was associated with the number of health services used (general practitioner visits, incidence rate ratio = 1.41), work productivity loss (labor force participation, adjusted odds ratio = 0.71), and reduced health-related quality of life (SF-6D score: Coefficient = -0.03). These effects were exacerbated by the presence of mental health conditions and low socioeconomic status. CONCLUSION: Having multiple physical health conditions (physical multimorbidity) creates substantial health and financial burdens on individuals, the health system, and society, including increased use of health services, loss of work productivity, and decreased health-related quality of life. The adverse effects of multimorbidity on health, quality of life, and economic well-being are exacerbated by the co-occurrence of mental health conditions and low socioeconomic status.
Published: 2020

18. Implications of multimorbidity on healthcare utilisation and work productivity by socioeconomic groups: Cross-sectional analyses of Australia and Japan

Author: Kabir, R, Sum, G, Ishida, M, Koh, GC-H, Singh, A, Oldenburg, B, Lee, JT, Kabir, R, Sum, G, Ishida, M, Koh, GC-H, Singh, A, Oldenburg, B, and Lee, JT
Abstract: BACKGROUND: Multimorbidity, the presence of 2 or more non-communicable diseases (NCDs), is a major contributor to inequalities of health in Australia and Japan. We use nationally representative data to examine (i) the relationships between multimorbidity with healthcare utilisation and productivity loss and (ii) whether these relationships differed by socioeconomic groups. METHODS: Cross-sectional analyses using the Household, Income, and Labour Dynamics in Australia (HILDA) and the Japanese Study of Aging and Retirement (JSTAR) surveys. We examined 6,382 (HILDA) and 3,503 (JSTAR) adults aged ≥50 years. We applied multivariable regression, logistic and negative binomial models. RESULTS: Prevalence of multimorbidity was overall 38.6% (46.0%, 36.1%, 28.9% amongst those in the lowest, middle and highest education group, respectively) in Australia, and 28.4% (33.9%, 24.6%, 16.6% amongst those in the lowest, middle and highest education group, respectively) in Japan. In Australia and Japan, more NCDs was associated with greater healthcare utilisation. In Australia and Japan, more NCDs was associated with higher mean number of sick leave days amongst the employed and lower odds of being employed despite being in the labour force. The association between multimorbidity and lower retirement age was found in Australia only. CONCLUSION: Having more NCDs pose significant economic burden to the health system and wider society in Australia and Japan. Targeted policies are critical to improve financial protection, especially for lower income groups who are more likely to have multiple NCDs. These individuals incur both high direct and indirect costs, which lead to a greater risk of impoverishment.
Published: 2020

19. XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission

Author: Abarr, Q., Awaki, H., Baring, M. G., Bose, R., De Geronimo, G., Dowkontt, P., Errando, M., Guarino, V., Hattori, K., Hayashida, K., Imazato, F., Ishida, M., Iyer, N. K., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lisalda, L., Matake, H., Maeda, Y., Matsumoto, H., Mineta, T., Miyazawa, T., Mizuno, T., Okajima, T., Pearce, M., Rauch, B. F., Ryde, F., Shreves, C., Spooner, S., Stana, T. -A., Takahashi, H., Takeo, M., Tamagawa, T., Tamura, K., Tsunemi, H., Uchida, N., Uchida, Y., West, A. T., Wulf, E. A., Yamamoto, R., Abarr, Q., Awaki, H., Baring, M. G., Bose, R., De Geronimo, G., Dowkontt, P., Errando, M., Guarino, V., Hattori, K., Hayashida, K., Imazato, F., Ishida, M., Iyer, N. K., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lisalda, L., Matake, H., Maeda, Y., Matsumoto, H., Mineta, T., Miyazawa, T., Mizuno, T., Okajima, T., Pearce, M., Rauch, B. F., Ryde, F., Shreves, C., Spooner, S., Stana, T. -A., Takahashi, H., Takeo, M., Tamagawa, T., Tamura, K., Tsunemi, H., Uchida, N., Uchida, Y., West, A. T., Wulf, E. A., and Yamamoto, R.
Abstract: XL-Calibur is a hard X-ray (15-80 keV) polarimetry mission operating from a stabilised balloon-borne platform in the stratosphere. It builds on heritage from the X-Calibur mission, which observed the accreting neutron star GX 301-2 from Antarctica, between December 29th 2018 and January 1st 2019. The XL-Calibur design incorporates an X-ray mirror, which focusses X-rays onto a polarimeter comprising a beryllium rod surrounded by Cadmium Zinc Telluride (CZT) detectors. The polarimeter is housed in an anticoincidence shield to mitigate background from particles present in the stratosphere. The mirror and polarimeter-shield assembly are mounted at opposite ends of a 12 m long lightweight truss, which is pointed with arcsecond precision by WASP - the Wallops Arc Second Pointer. The XL-Calibur mission will achieve a substantially improved sensitivity over X-Calibur by using a larger effective area X-ray mirror, reducing background through thinner CZT detectors, and improved anticoincidence shielding. When observing a 1 Crab source for $t_{\rm day}$ days, the Minimum Detectable Polarisation (at 99% confidence level) is $\sim$2$\%\cdot t_{\rm day}^{-1/2}$. The energy resolution at 40 keV is $\sim$5.9 keV. The aim of this paper is to describe the design and performance of the XL-Calibur mission, as well as the foreseen science programme., Comment: 19 pages, 17 figures. Accepted for publication in Astroparticle Physics
Published: 2020
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20. Inorbit Performance of the Hard X-ray Telescope (HXT) on board the Hitomi (ASTRO-H) satellite

Author: Matsumoto, H., Awaki, H., Ishida, M., Furuzawa, A., Yamauchi, S., Maeda, Y., Mitsuishi, I., Haba, Y., Hayashi, T., Iizuka, R., Ishibashi, K., Itoh, M., Kunieda, H., Miyazawa, T., Mori, H., Okajima, T., Sugita, S., Tamura., K., Tawara, Y., Matsumoto, H., Awaki, H., Ishida, M., Furuzawa, A., Yamauchi, S., Maeda, Y., Mitsuishi, I., Haba, Y., Hayashi, T., Iizuka, R., Ishibashi, K., Itoh, M., Kunieda, H., Miyazawa, T., Mori, H., Okajima, T., Sugita, S., Tamura., K., and Tawara, Y.
Abstract: Hitomi (ASTRO-H) carries two Hard X-ray Telescopes (HXTs) that can focus X-rays up to 80 keV. Combined with the Hard X-ray Imagers (HXIs) that detect the focused X-rays, imaging spectroscopy in the high-energy band from 5 keV to 80 keV is made possible. We studied characteristics of HXTs after the launch such as the encircled energy function (EEF) and the effective area using the data of a Crab observation. The half power diameters (HPDs) in the 5--80 keV band evaluated from the EEFs are 1.59 arcmin for HXT-1 and 1.65 arcmin for HXT-2. Those are consistent with the HPDs measured with ground experiments when uncertainties are taken into account. We can conclude that there is no significant change in the characteristics of the HXTs before and after the launch. The off-axis angle of the aim point from the optical axis is evaluated to be less than 0.5 arcmin for both HXT-1 and HXT-2. The best-fit parameters for the Crab spectrum obtained with the HXT-HXI system are consistent with the canonical values., Comment: 13 pages, 5 figures; the acknowledgment was modified
Published: 2018
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21. In-orbit performance of the soft X-ray imaging system aboard Hitomi (ASTRO-H)

Author: Nakajima, H., Maeda, Y., Uchida, H., Tanaka, T., Tsunemi, H., Hayashida, K., Tsuru, T. G., Dotani, T., Nagino, R., Inoue, S., Ozaki, M., Tomida, H., Natsukari, C., Ueda, S., Mori, K., Yamauchi, M., Hatsukade, I., Nishioka, Y., Sakata, M., Beppu, T., Honda, D., Nobukawa, M., Hiraga, J. S., Kohmura, T., Murakami, H., Nobukawa, K. K., Bamba, A., Doty, J. P., Iizuka, R., Sato, T., Kurashima, S., Nakaniwa, N., Asai, R., Ishida, M., Mori, H., Soong, Y., Okajima, T., Serlemitsos, P., Tawara, Y., Mitsuishi, I., Ishibashi, K., Tamura, K., Hayashi, T., Furuzawa, A., Sugita, S., Miyazawa, T., Awaki, H., Miller, E. D., Yamaguchi, H., Nakajima, H., Maeda, Y., Uchida, H., Tanaka, T., Tsunemi, H., Hayashida, K., Tsuru, T. G., Dotani, T., Nagino, R., Inoue, S., Ozaki, M., Tomida, H., Natsukari, C., Ueda, S., Mori, K., Yamauchi, M., Hatsukade, I., Nishioka, Y., Sakata, M., Beppu, T., Honda, D., Nobukawa, M., Hiraga, J. S., Kohmura, T., Murakami, H., Nobukawa, K. K., Bamba, A., Doty, J. P., Iizuka, R., Sato, T., Kurashima, S., Nakaniwa, N., Asai, R., Ishida, M., Mori, H., Soong, Y., Okajima, T., Serlemitsos, P., Tawara, Y., Mitsuishi, I., Ishibashi, K., Tamura, K., Hayashi, T., Furuzawa, A., Sugita, S., Miyazawa, T., Awaki, H., Miller, E. D., and Yamaguchi, H.
Abstract: We describe the in-orbit performance of the soft X-ray imaging system consisting of the Soft X-ray Telescope and the Soft X-ray Imager aboard Hitomi. Verification and calibration of imaging and spectroscopic performance are carried out making the best use of the limited data of less than three weeks. Basic performance including a large field of view of 38'x38' is verified with the first light image of the Perseus cluster of galaxies. Amongst the small number of observed targets, the on-minus-off pulse image for the out-of-time events of the Crab pulsar enables us to measure a half power diameter of the telescope as about 1.3'. The average energy resolution measured with the onboard calibration source events at 5.89 keV is 179 pm 3 eV in full width at half maximum. Light leak and cross talk issues affected the effective exposure time and the effective area, respectively, because all the observations were performed before optimizing an observation schedule and parameters for the dark level calculation. Screening the data affected by these two issues, we measure the background level to be 5.6x10^{-6} counts s^{-1} arcmin^{-2} cm^{-2} in the energy band of 5-12 keV, which is seven times lower than that of the Suzaku XIS-BI., Comment: Accepted for publication in PASJ. 17 pages, 18 figures
Published: 2017
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22. Discovery of Rapidly Moving Partial X-ray Absorbers within gamma Cassiopeiae

Author: Hamaguchi, K., Oskinova, L., Russell, C. M. P., Petre, R., Enoto, T., Morihana, K., Ishida, M., Hamaguchi, K., Oskinova, L., Russell, C. M. P., Petre, R., Enoto, T., Morihana, K., and Ishida, M.
Abstract: Gamma Cassiopeiae is an enigmatic Be star with unusually strong hard X-ray emission. The Suzaku observatory detected six rapid X-ray spectral hardening events called "softness dips" in a ~100 ksec duration observation in 2011. All the softness dip events show symmetric softness ratio variations, and some of them have flat bottoms apparently due to saturation. The softness dip spectra are best described by either ~40% or ~70% partial covering absorption to kT ~12 keV plasma emission by matter with a neutral hydrogen column density of ~2-8e21 cm-2, while the spectrum outside of these dips is almost free of absorption. This result suggests the presence of two distinct X-ray emitting spots in the gamma Cas system, perhaps on a white dwarf companion with dipole mass accretion. The partial covering absorbers may be blobs in the Be stellar wind, the Be disk, or rotating around the white dwarf companion. Weak correlations of the softness ratios to the hard X-ray flux suggest the presence of stable plasmas at kT ~0.9 and 5 keV, which may originate from the Be or white dwarf winds. The formation of a Be star and white dwarf binary system requires mass transfer between two stars; gamma Cas may have experienced such activity in the past., Comment: 16 pages, 5 figures, accepted for publication in Astrophysical Journal
Published: 2016
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23. Development and Validation of a Risk Score for Chronic Kidney Disease in HIV Infection Using Prospective Cohort Data from the D:A:D Study

Author: Mocroft, A., Lundgren, J. D., Ross, M., Law, M., Reiss, P., Kirk, O., Smith, C., Wentworth, D., Neuhaus, J., Fux, C. A., Moranne, O., Morlat, P., Johnson, M. A., Ryom, L., Powderly, B., Shortman, N., Moecklinghoff, C., Reilly, G., Franquet, X., Sabin, C. A., Phillips, A., Weber, R., Pradier, C., d'Arminio Monforte, A., Dabis, F., El-Sadr, W. M., De Wit, S., Kamara, D., Tverland, J., Mansfeld, M., Nielsen, J., Raben, D., Salbol Brandt, R., Rickenbach, M., Fanti, I., Krum, E., Hillebregt, M., Geffard, S., Sundstrom, A., Delforge, M., Fontas, E., Torres, F., Mcmanus, H., Wright, S., Kjaer, J., Sjol, A., Meidahl, P., Helweg-Larsen, J., Schmidt Iversen, J., Kesselring, A. M., Friis-Moller, N., Kowalska, J., Sabin, C., Bruyand, M., Kamara, D. A., Bower, M., Fatkenheuer, G., Donald, A., Grulich, A., Prins, J. M., Kuijpers, T. W., Scherpbier, H. J., van der Meer, J. T. M., Wit, F. W. M. N., Godfried, M. H., van der Poll, T., Nellen, F. J. B., Geerlings, S. E., van Vugt, M., Pajkrt, D., Bos, J. C., Wiersinga, W. J., van der Valk, M., Goorhuis, A., Hovius, J. W., van Eden, J., Henderiks, A., van Hes, A. M. H., Mutschelknauss, M., Nobel, H. E., Pijnappel, F. J. J., Westerman, A. M., Jurriaans, S., Back, N. K. T., Zaaijer, H. L., Berkhout, B., Cornelissen, M. T. E., Schinkel, C. J., Thomas, X. V., van den Berge, M., Stegeman, A., Baas, S., Hage de Looff, L., Versteeg, D., Pronk, M. J. H., Ammerlaan, H. S. M., Korsten-Vorstermans, E. M. H. M., de Munnik, E. S., Jansz, A. R., Tjhie, J., Wegdam, M. C. A., Deiman, B., Scharnhorst, V., van der Plas, A., Weijsenfeld, A. M., van der Ende, M. E., de Vries-Sluijs, T. E. M. S., C. M. van Gorp, E., Schurink, C. A. M., Nouwen, J. L., Verbon, A., Rijnders, B. J. A., Bax, H. I., Hassing, R. J., van der Feltz, M., Bassant, N., van Beek, J. E. A., Vriesde, M., van Zonneveld, L. M., de Oude-Lubbers, A., van den Berg-Cameron, H. J., Bruinsma-Broekman, F. B., de Groot, J., de Zeeuw- de Man, M., Broekhoven-Kruijne, M. J., Schutten, M., Osterhaus, A. D. M. E., Boucher, C. A. B., Driessen, G. J. A., van Rossum, A. M. C., van der Knaap, L. C., Visser, E., Branger, J., H. M. Duijf-van de Ven C., J., Schippers, E. F., van Nieuwkoop, C., Brimicombe, R. W., van IJperen, J. M., van der Hut, G., Franck, P. F. H., van Eeden, A., Brokking, W., Groot, M., Damen, M., Kwa, I. S., Groeneveld, P. H. P., Bouwhuis, J. W., van den Berg, J. F., van Hulzen, A. G. W., van der Bliek, G. L., Bor, P. C. J., Bloembergen, P., Wolfhagen, M. J. H. M., Ruijs, G. J. H. M., van Lelyveld, S. F. L., Soetekouw, R., Hulshoff, N., van der Prijt, L. M. M., Schoemaker, M., Bermon, N., van der Reijden, W. A., Jansen, R., Herpers, B. L., Veenendaal, D., Kroon, F. P., Arend, S. M., de Boer, M. G. J., Bauer, M. P., Jolink, H., Vollaard, A. M., Dorama, W., Moons, C., Claas, E. C. J., Kroes, A. C. M., den Hollander, J. G., Pogany, K., Kastelijns, M., Smit, J. V., Smit, E., Bezemer, M., van Niekerk, T., Pontesilli, O., Lowe, S. H., Oude Lashof, A., Posthouwer, D., Ackens, R. P., Schippers, J., Vergoossen, R., Weijenberg Maes, B., Savelkoul, P. H. M., Loo, I. H., Weijer, S., El Moussaoui, R., Heitmuller, M., Kortmann, W., van Twillert, G., Cohen Stuart, J. W. T., Diederen, B. M. W., Pronk, D., van Truijen-Oud, F. A., Leyten, E. M. S., Gelinck, L. B. S., van Hartingsveld, A., Meerkerk, C., Wildenbeest, G. S., Mutsaers, J. A. E. M., Jansen, C. L., van Vonderen, M. G. A., van Houte, D. P. F., Dijkstra, K., Faber, S., Weel, J., Kootstra, G. J., Delsing, C. E., van der Burg-van de Plas, M., Heins, H., Lucas, E., Brinkman, K., Frissen, P. H. J., Blok, W. L., Schouten, W. E. M., Bosma, A. S., Brouwer, C. J., Geerders, G. F., Hoeksema, K., Kleene, M. J., van der Meche, I. B., Toonen, A. J. M., Wijnands, S., van Ogtrop, M. L., Koopmans, P. P., Keuter, M., van der Ven, A. J. A. M., ter Hofstede, H. J. M., Dofferhoff, A. S. 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J., Munjishvili, L., Kruijne, E., Tuk, B., Bonnet, F., Dupon, M., Chene, G., Breilh, D., Fleury, H., Malvy, D., Mercie, P., Pellegrin, I., Neau, D., Bouchet, S., Gaborieau, V., Lacoste, D., Tchamgoue, S., Thiebaut, R., Lawson-Ayayi, S., Wittkop, L., Bernard, N., Hessamfar, M., Vandenhende, M. A., Dauchy, F. A., Dutronc, H., Longy-Boursier, M., Duffau, P., Roger Schmeltz, J., Pistone, T., Receveur, M. C., Cazanave, C., Ochoa, A., Vareil, M. O., Pellegrin, J. L., Viallard, J. F., Greib, C., Lazaro, E., Lafon, M. E., Reigadas, S., Trimoulet, P., Molimard, M., Titier, K., Moreau, J. F., Haramburu, F., Miremont-Salame, G., Dupont, A., Gerard, Y., Caunegre, L., Andre, K., Bonnal, F., Farbos, S., Gemain, M. C., Ceccaldi, J., De Witte, S., Courtault, C., Monlun, E., Lataste, P., Meraud, J. P., Chossat, I., Blaizeau, M. 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R., Sampson, J., Baxter, J., Cozzi-Lepri, A., Grint, D., Podlekareva, D., Peters, L., Reekie, J., Fischer, A. H., Losso, M., Elias, C., Vetter, N., Zangerle, R., Karpov, I., Vassilenko, A., Mitsura, V. M., Suetnov, O., Colebunders, R., Vandekerckhove, L., Hadziosmanovic, V., Kostov, K., Begovac, J., Machala, L., Jilich, D., Sedlacek, D., Kronborg, G., Benfield, T., Larsen, M., Gerstoft, J., Katzenstein, T., Hansen, A. -B. E., Skinhoj, P., Pedersen, C., Ostergaard, L., Zilmer, K., Smidt, J., Ristola, M., Katlama, C., Viard, J. -P., Girard, P. -M., Livrozet, J. M., Vanhems, P., Rockstroh, J., Schmidt, R., van Lunzen, J., Degen, O., Stellbrink, H. J., Staszewski, S., Bickel, M., Kosmidis, J., Gargalianos, P., Xylomenos, G., Perdios, J., Panos, G., Filandras, A., Karabatsaki, E., Sambatakou, H., Banhegyi, D., Mulcahy, F., Yust, I., Turner, D., Burke, M., Pollack, S., Hassoun, G., Maayan, S., Vella, S., Esposito, R., Mazeu, I., Mussini, C., Arici, C., Pristera, R., Mazzotta, F., Gabbuti, A., Vullo, V., Lichtner, M., Chirianni, A., Montesarchio, E., Gargiulo, M., Antonucci, G., Testa, A., Narciso, P., Vlassi, C., Zaccarelli, M., Lazzarin, A., Castagna, A., Gianotti, N., Galli, M., Ridolfo, A., Rozentale, B., Zeltina, I., Chaplinskas, S., Hemmer, R., Staub, T., Ormaasen, V., Maeland, A., Bruun, J., Knysz, B., Gasiorowski, J., Horban, A., Bakowska, E., Grzeszczuk, A., Flisiak, R., Boron-Kaczmarska, A., Pynka, M., Parczewski, M., Beniowski, M., Mularska, E., Trocha, H., Jablonowska, E., Malolepsza, E., Wojcik, K., Antunes, F., Doroana, M., Caldeira, L., Mansinho, K., Maltez, F., Duiculescu, D., Rakhmanova, A., Zakharova, N., Buzunova, S., Jevtovic, D., Mokras, M., Stanekova, D., Tomazic, J., Gonzalez-Lahoz, J., Soriano, V., Labarga, P., Medrano, J., Moreno, S., Rodriguez, J. 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L., Michelet, C., Michon, C., Mole, M., Netzer, E., Pialoux, G., Poizot-Martin, I., Raffi, F., Ratajczak, M., Ravaux, I., Reynes, J., Salmon-Ceron, D., Sebire, M., Simon, A., Tegna, L., Tisne-Dessus, D., Tramoni, C., Viard, J. P., Vidal, M., Viet-Peaucelle, C., Weiss, L., Zeng, A., Zucman, D., Adam, A., Arasteh, K., Behrens, G., Bergmann, F., Bittner, D., Bogner, J., Brockmeyer, N., Darrelmann, N., Deja, M., Doerler, M., Esser, S., Faetkenheuer, G., Fenske, S., Gajetzki, S., Goebel, F., Gorriahn, D., Harrer, E., Harrer, T., Hartl, H., Hartmann, M., Heesch, S., Jakob, W., Jager, H., Klinker, H., Kremer, G., Ludwig, C., Mantzsch, K., Mauss, S., Meurer, A., Niedermeier, A., Pittack, N., Plettenberg, A., Potthoff, A., Probst, M., Rittweger, M., Ross, B., Rotty, J., Rund, E., Ruzicka, T., Schmidt, R. T., Schmutz, G., Schnaitmann, E., Schuster, D., Sehr, T., Spaeth, B., Stephan, C., Stockey, T., Stoehr, A., Trein, A., Vaeth, T., Vogel, M., Wasmuth, J., Wengenroth, C., Winzer, R., Wolf, E., Reidy, D. L., Cohen, Y., Drora, G., Eliezer, I., Godo, O., Kedem, E., Magen, E., Mamorsky, M., Sthoeger, Z., Vered, H., Aiuti, F., Bechi, M., Bergamasco, A., Bertelli, D., Bruno, R., Butini, L., Cagliuso, M., Carosi, G., Casari, S., Chrysoula, V., Cologni, G., Conti, V., Corpolongo, A., D'Offizi, G., Gaiottino, F., Di Pietro, M., Filice, G., Francesco, M., Gianelli, E., Graziella, C., Magenta, L., Martellotta, F., Maserati, R., Murdaca, G., Nardini, G., Nozza, S., Puppo, F., Pogliaghi, M., Ripamonti, D., Ronchetti, C., Rusconi, V., Sacchi, P., Silvia, N., Suter, F., Tambussi, G., Uglietti, A., Vechi, M., Vergani, B., Vichi, F., Vitiello, P., Iwamoto, A., Kikuchi, Y., Miyazaki, N., Mori, M., Nakamura, T., Odawara, T., Oka, S., Shirasaka, T., Tabata, M., Takano, M., Ueta, C., Watanabe, D., Yamamoto, Y., Erradey, I., Himmich, H., Marhoum El Filali, K., Blok, W., van Boxtel, R., Brinkman H Doevelaar, K., Grijsen, M., Juttmann, J., Ligthart, S., van der Meulen, P., Lange, J., Schrijnders-Gudde, L., Septer-Bijleveld, E., Sprenger, H., Vermeulen, J., ten Kate, R., van de Ven, B., Kvale, D., Inglot, M., Rymer, W., Szymczak, A., Aldir, M., Baptista, C., da Conceicao Vera, J., Raquel A dos Santos, C., Valadas, E., Vaz Pinto, I., Chia, E., Foo, E., Karim, F., Lim, P. L., Panchalingam, A., Quek, A., Alcazar-Caballero, R., Arribas, J., Arrizabalaga, J., de Barron, X., Blanco, F., Bouza, E., Calvo, S., Carbonero, L., Carpena, I., Castro, M., Cortes, L., del Toro, M., Elias, M., Espinosa, J., Estrada, V., Fernandez-Cruz, E., Fernandez, P., Freud, H., Garcia, A., Garcia, G., Garrido, R., Gijon, P., Gonzalez- Garcia, J., Gil, I., Gonzalez, A., Lopez Grosso, P., Guzman, E., Iribarren, J., Jimenez, M., Juega, J., Lopez, J., Lozano, F., Martin-Carbonero, L., Mata, R., Menasalvas, A., Mirelles, C., de Miguel Prieto, J., Montes, M., Moreno, A., Moreno, J., Moreno, V., Munoz, R., Ocampo, A., Ortega, E., Ortiz, L., Padilla, B., Parras, A., Paster, A., Pedreira, J., Pena, J., Perea, R., Portas, B., Pulido, F., Rebollar, M., de Rivera, J., Roca, V., Rodriguez- Arrondo, F., Rubio, R., Santos, J., Sanz, J., Sebastian, G., Segovia, M., Tamargo, L., Viciana, P., von Wichmann, M., Bratt, G., Hollander, A., Olov Pehrson, P., Petz, I., Sandstrom, E., Sonnerborg, A., Gurtner, V., Ampunpong, U., Auchieng, C., Bowonwatanuwong, C., Chanchai, P., Chetchotisakd, P., Chuenyan, T., Duncombe, C., Horsakulthai, M., Kantipong, P., Laohajinda, K., Phanuphak, P., Pongsurachet, V., Pradapmook, S., Ruxruntham, K., Seekaew, S., Sonjai, A., Suwanagool, S., Techasathit, W., Ubolyam, S., Wankoon, J., Alexander, I., Dockrell, D., Easterbrook, P., Edwards, B., Evans, E., Fox, R., Gazzard, B., Gilleran, G., Hand, J., Heald, L., Higgs, C., Jebakumar, S., Jendrulek, I., Johnson, S., Kinghorn, G., Kuldanek, K., Maw, R., Mckernan, S., Mclean, L., Morris, S., O'Farrell, S., Ong, E., Peters, B., Stroud, C., Wansbrough-Jones, M., White, D., Williams, I., Wiselka, M., Yee, T., Adams, S., Allegra, D., Andrews, L., Aneja, B., Anstead, G., Artz, R., Bailowitz, J., Banks, S., Baum, J., Benator, D., Black, D., Boh, D., Bonam, T., Brito, M., Brockelman, J., Bruzzese, V., Burnside, A., Cafaro, V., Casey, K., Cason, L., Childress, G., Clark, C. L., Clifford, D., Climo, M., Couey, P., Cuervo, H., Deeks, S., Dennis, M., Diaz-Linares, M., Dickerson, D., Diez, M., Di Puppo, J., Dodson, P., Dupre, D., Elion, R., Elliott, K., El-Sadr, W., Estes, M., Fabre, J., Farrough, M., Flamm, J., Follansbee, S., Foster, C., Frank, C., Franz, J., Frechette, G., Freidland, G., Frische, J., Fuentes, L., Funk, C., Geisler, C., Genther, K., Giles, M., Goetz, M., Gonzalez, M., Graeber, C., Graziano, F., Grice, D., Hahn, B., Hamilton, C., Hassler, S., Henson, A., Hopper, S., John, M., Johnson, L., Johnson, R., Jones, R., Kahn, J., Klimas, N., Kolber, M., Koletar, S., Labriola, A., Larsen, R., Lasseter, F., Lederman, M., Ling, T., Lusch, T., Macarthur, R., Machado, C., Makohon, L., Mandelke, J., Mannheimer, S., Martinez, M., Martinez, N., Mass, M., Masur, H., Mcgregor, D., Mcintyre, D., Mckee, J., Mcmullen, D., Mettinger, M., Middleton, S., Mieras, J., Mildvan, D., Miller, P., Miller, T., Mitchell, V., Mitsuyasu, R., Moanna, A., Mogridge, C., Moran, F., Murphy, R., Nahass, R., Nixon, D., O'Brien, S., Ojeda, J., Okhuysen, P., Olson, M., Osterberger, J., Owen, W., Pablovich, S. S., Patel, S., Pierone, G., Poblete, R., Potter, A., Preston, E., Rappoport, C., Regevik, N., Reyelt, M., Riney, L., Rodriguez-Barradas, M., Rodriguez, M., Rodriguez, J., Roland, R., Rosmarin-DeStefano, C., Rossen, W., Rouff, J., Saag, M., Santiago, S., Sarria, J., Wirtz, S., Schmidt, U., Scott, C., Sheridan, A., Shin, A., Shrader, S., Slowinski, D., Smith, K., Spotkov, J., Sprague, C., States, D., Suh, C., Sullivan, J., Summers, K., Sweeton, B., Tan, V., Tanner, T., Temesgen, Z., Thomas, D., Thompson, M., Tobin, C., Toro, N., Towner, W., Upton, K., Uy, J., Valenti, S., van der Horst, C., Vita, J., Voell, J., Walker, J., Walton, T., Wason, K., Watson, V., Wellons, A., Weise, J., White, M., Whitman, T., Williams, B., Williams, N., Windham, J., Witt, M., Workowski, K., Wortmann, G., Wright, T., Zelasky, C., Zwickl, B., Finley, E., Dietz, D., Chesson, C., Vjecha, M., Schmetter, B., Grue, L., Willoughby, M., Demers, A., Dragsted, U. B., Jensen, K. B., Jansson, P. O., Jensen, B. G., Benfield, T. L., Darbyshire, J. H., Babiker, A. G., Fleck, S. L., Collaco-Moraes, Y., Wyzydrag, L., Drummond, F. M., Connor, S. A., Satchell, C. S., Gunn, S., Delfino, M. A., Merlin, K., Mcginley, C., Neaton, J. D., George, M., Grund, B., Hogan, C., Miller, C., Roediger, M. P., Thackeray, L., Campbell, C., Lahart, C., Perlman, D., Rein, M., Dersimonian, R., Brody, B. A., Daar, E. S., Dubler, N. N., Fleming, T. R., Freeman, D. J., Kahn, J. P., Kim, K. M., Medoff, G., Modlin, J. F., Moellering, R., Murray, B. E., Robb, M. L., Scharfstein, D. O., Sugarman, J., Tsiatis, A., Tuazon, C., Zoloth, L., Belloso, W. H., Losso, M. H., Benetucci, J. A., Bogdanowicz, E. P., Cahn, P. E., Casiro, A. D., Cassetti, I., Contarelli, J. M., Corral, J. A., Crinejo, A., David, D. O., Ishida, M. T., Laplume, H. E., Lasala, M. B., Lupo, S. H., Masciottra, F., Michaan, M., Ruggieri, L., Salazar, E., Allworth, A. M., Anderson, J. S. C., Armishaw, J., Barnes, K., Chiam, A., Chuah, J. C. P., Curry, M. C., Dever, R. L., Donohue, W. A., Doong, N. C., Dwyer, D. E., Dyer, J., Eu, B., Ferguson, V. W., French, M. A. H., Garsia, R. J., Hudson, J. H., Jeganathan, S., Konecny, P., Mccormack, C. L., Mcmurchie, M., Moore, R. J., Moussa, M. B., Piper, M., Read, T., Roney, J. J., Shaw, D. R., Silvers, J., Smith, D. J., Street, A. C., Vale, R. J., Wendt, N. A., Wood, H., Youds, D. W., Zillman, J., Tozeau, V., de Roo, A., Leonard, P., Lynen, L., Moutschen, M., Pereira, L. C., Souza, T. N. L., Schechter, M., Zajdenverg, R., Almeida, M. M. T. B., Araujo, F., Bahia, F., Brites, C., Caseiro, M. M., Casseb, J., Etzel, A., Falco, G. G., Filho, E. C. J., Flint, S. R., Gonzales, C. R., Madruga, J. V. R., Passos, L. N., Reuter, T., Sidi, L. C., Toscano, A. L. C., Cherban, E., Conway, B., Dufour, C., Foster, A., Haase, D., Haldane, H., Klein, M., Lessard, B., Martel, A., Martel, C., Paradis, E., Schlech, W., Schmidt, S., Thompson, B., Vezina, S., Wolff Reyes, M. J., Northland, R., Hergens, L., Loftheim, I. R., Raukas, M., Justinen, J., Landman, R., Abel, S., Abgrall, S., Amat, K., Auperin, L., Barruet, R., Benalycherif, A., Benammar, N., Bentata, M., Besnier, J. M., Blanc, M., Cabie, A., Chavannet, P., Dargere, S., de la Tribonniere, X., Debord, T., Decaux, N., Delgado, J., Frixon-Marin, V., Genet, C., Gerard, L., Gilquin, J., Jeantils, V., Kouadio, H., Leclercq, P., Lelievre, J. -D., Michon, C. P., Nau, P., Pacanowski, J., Piketty, C., Salmon, D., Schmit, J. L., Serini, M. A., Tassi, S., Touam, F., Verdon, R., Weinbreck, P., Yazdanpanah, Y., Yeni, P., Bitsch, S., Bogner, J. R., Goebel, F. D., Lehmann, C., Lennemann, T., Potthof, A., Wasmuth, J. C., Wiedemeyer, K., Hatzakis, A., Touloumi, G., Antoniadou, A., Daikos, G. L., Dimitrakaki, A., Gargalianos-Kakolyris, P., Giannaris, M., Karafoulidou, A., Katsambas, A., Katsarou, O., Kontos, A. N., Kordossis, T., Lazanas, M. K., Panagopoulos, P., Paparizos, V., Papastamopoulos, V., Petrikkos, G., Skoutelis, A., Tsogas, N., Bergin, C. J., Mooka, B., Mamorksy, M. G., Agmon-Levin, N., Karplus, R., Shahar, E., Biglino, A., De Gioanni, M., Montroni, M., Raise, E., Honda, M., Ishisaka, M., Caplinskas, S., Uzdaviniene, V., Schmit, J. C., Mills, G. D., Blackmore, T., Masters, J. A., Morgan, J., Pithie, A., Brunn, J., Ormasssen, V., La Rosa, A., Guerra, O., Espichan, M., Gutierrez, L., Mendo, F., Salazar, R., Knytz, B., Kwiatkowski, J., Castro, R. S., Horta, A., Miranda, A. C., Pinto, I. V., Vera, J., Vinogradova, E., Yakovlev, A., Wood, R., Orrel, C., Arnaiz, J. A., Carrillo, R., Dalmau, D., Jordano, Q., Knobel, H., Larrousse, M., Moreno, J. S., Oretaga, E., Pena, J. N., Spycher, R., Bottone, S., Christen, A., Franc, C., Furrer, H. J., Gayet-Ageron, A., Genne, D., Hochstrasser, S., Moens, C., Nuesch, R., Ruxrungtham, K., Pumpradit, W., Dangthongdee, S., Kiertiburanakul, S., Klinbuayaem, V., Mootsikapun, P., Nonenoy, S., Piyavong, B., Prasithsirikul, W., Raksakulkarn, P., Gazzard, B. G., Ainsworth, J. G., Angus, B. J., Barber, T. J., Brook, M. G., Care, C. D., Chadwick, D. R., Chikohora, M., Churchill, D. R., Cornforth, D., Dockrell, D. H., Easterbrook, P. J., Fox, P. A., Gomez, P. A., Gompels, M. M., Harris, G. M., Herman, S., Jackson, A. G. A., Jebakumar, S. P. R., Kinghorn, G. R., Kuldanek, K. A., Larbalestier, N., Lumsden, M., Maher, T., Mantell, J., Muromba, L., Orkin, C. M., Palfreeman, A. J., Peters, B. S., Peto, T. E. A., Portsmouth, S. D., Rajamanoharan, S., Ronan, A., Schwenk, A., Slinn, M. A., Stroud, C. J., Thomas, R. C., Wansbrough-Jones, M. H., Whiles, H. J., White, D. J., Williams, E., Williams, I. G., Acosta, E. A., Adamski, A., Antoniskis, D., Aragon, D. R., Barnett, B. J., Baroni, C., Barron, M., Baxter, J. D., Beers, D., Beilke, M., Bemenderfer, D., Bernard, A., Besch, C. L., Bessesen, M. T., Bethel, J. T., Blue, S., Blum, J. D., Boarden, S., Bolan, R. K., Borgman, J. B., Brar, I., Braxton, B. K., Bredeek, U. F., Brennan, R., Britt, D. E., Bulgin-Coleman, D., Bullock, D. E., Campbell, B., Caras, S., Carroll, J., Casey, K. K., Chiang, F., Cindrich, R. B., Clark, C., Cohen, C., Coley, J., Condoluci, D. V., Contreras, R., Corser, J., Cozzolino, J., Daley, L., Dandridge, D., D'Antuono, V., Darcourt Rizo Patron, J. G., Dehovitz, J. A., Dejesus, E., Desjardin, J., Dietrich, C., Dolce, E., Erickson, D., Faber, L. L., Falbo, J., Farrough, M. J., Farthing, C. F., Ferrell-Gonzalez, P., Flynn, H., Frank, M., Freeman, K. F., French, N., Fujita, N., Gahagan, L., Gilson, I., Goetz, M. B., Goodwin, E., Guity, C. K., Gulick, P., Gunderson, E. R., Hale, C. M., Hannah, K., Henderson, H., Hennessey, K., Henry, W. K., Higgins, D. T., Hodder, S. L., Horowitz, H. W., Howe-Pittman, M., Hubbard, J., Hudson, R., Hunter, H., Hutelmyer, C., Insignares, M. T., Jackson, L., Jenny, L., Johnson, D. L., Johnson, G., Johnson, J., Kaatz, J., Kaczmarski, J., Kagan, S., Kantor, C., Kempner, T., Kieckhaus, K., Kimmel, N., Klaus, B. M., Koeppe, J. R., Koirala, J., Kopka, J., Kostman, J. R., Kozal, M. J., Kumar, A., Lampiris, H., Lamprecht, C., Lattanzi, K. M., Lee, J., Leggett, J., Long, C., Loquere, A., Loveless, K., Lucasti, C. J., Macveigh, M., Makohon, L. H., Markowitz, N. P., Marks, C., Martorell, C., Mcfeaters, E., Mcgee, B., Mcintyre, D. M., Mcmanus, E., Melecio, L. G., Melton, D., Mercado, S., Merrifield, E., Mieras, J. A., Mogyoros, M., Moran, F. M., Murphy, K., Mutic, S., Nadeem, I., Nadler, J. P., Ognjan, A., O'Hearn, M., O'Keefe, K., Okhuysen, P. C., Oldfield, E., Olson, D., Orenstein, R., Ortiz, R., Parpart, F., Pastore-Lange, V., Paul, S., Pavlatos, A., Pearce, D. D., Pelz, R., Peterson, S., Pitrak, D., Powers, S. L., Pujet, H. C., Raaum, J. W., Ravishankar, J., Reeder, J., Reilly, N. A., Reyelt, C., Riddell, J., Rimland, D., Robinson, M. L., Rodriguez, A. E., Rodriguez-Barradas, M. C., Rodriguez Derouen, V., Rosmarin, C., Rossen, W. L., Rouff, J. R., Sampson, J. H., Sands, M., Savini, C., Schrader, S., Schulte, M. M., Scott, R., Seedhom, H., Sension, M., Sheble-Hall, A., Shuter, J., Slater, L. N., Slotten, R., Smith, M., Snap, S., States, D. M., Stringer, G., Summers, K. K., Swanson, K., Sweeton, I. B., Szabo, S., Telzak, E. E., Thompson, M. A., Thompson, S., Ting Hong Bong, C., Vaccaro, A., Vasco, L. M., Vecino, I., Verlinghieri, G. K., Visnegarwala, F., Wade, B. H., Weis, S. E., Weise, J. A., Weissman, S., Wilkin, A. M., Witter, J. H., Wojtusic, L., Wright, T. J., Yeh, V., Young, B., Zeana, C., Zeh, J., Savio, E., Vacarezza, M., and Cauda R. (ORCID:0000-0002-1498-4229)
Abstract: Chronic kidney disease (CKD) is a major health issue for HIV-positive individuals, associated with increased morbidity and mortality. Development and implementation of a risk score model for CKD would allow comparison of the risks and benefits of adding potentially nephrotoxic antiretrovirals to a treatment regimen and would identify those at greatest risk of CKD. The aims of this study were to develop a simple, externally validated, and widely applicable long-term risk score model for CKD in HIV-positive individuals that can guide decision making in clinical practice. A total of 17,954 HIV-positive individuals from the Data Collection on Adverse Events of Anti-HIV Drugs (D:A:D) study with ≥3 estimated glomerular filtration rate (eGFR) values after 1 January 2004 were included. Baseline was defined as the first eGFR > 60 ml/min/1.73 m2 after 1 January 2004; individuals with exposure to tenofovir, atazanavir, atazanavir/ritonavir, lopinavir/ritonavir, other boosted protease inhibitors before baseline were excluded. CKD was defined as confirmed (>3 mo apart) eGFR ≤ 60 ml/min/1.73 m2. Poisson regression was used to develop a risk score, externally validated on two independent cohorts. In the D:A:D study, 641 individuals developed CKD during 103,185 person-years of follow-up (PYFU; incidence 6.2/1,000 PYFU, 95% CI 5.7–6.7; median follow-up 6.1 y, range 0.3–9.1 y). Older age, intravenous drug use, hepatitis C coinfection, lower baseline eGFR, female gender, lower CD4 count nadir, hypertension, diabetes, and cardiovascular disease (CVD) predicted CKD. The adjusted incidence rate ratios of these nine categorical variables were scaled and summed to create the risk score. The median risk score at baseline was −2 (interquartile range –4 to 2). There was a 1:393 chance of developing CKD in the next 5 y in the low risk group (risk score < 0, 33 events), rising to 1:47 and 1:6 in the medium (risk score 0–4, 103 events) and high risk groups (risk score ≥ 5, 505 events)
Published: 2015

24. ASTRO-H White Paper - Older Supernova Remnants and Pulsar Wind Nebulae

Author: Long, K. S., Bamba, A., Aharonian, F., Foster, A., Funk, S., Hiraga, J., Hughes, J., Ishida, M., Katsuda, S., Matsumoto, H., Mori, K., Nakajima, H., Nakamori, T., Ozaki, M., Safi-Harb, S., Sawada, M., Tamagawa, T., Tamura, K., Tanaka, T., Tsunemi, H., Uchida, H., Uchiyama, Y., Yamauchi, S., Long, K. S., Bamba, A., Aharonian, F., Foster, A., Funk, S., Hiraga, J., Hughes, J., Ishida, M., Katsuda, S., Matsumoto, H., Mori, K., Nakajima, H., Nakamori, T., Ozaki, M., Safi-Harb, S., Sawada, M., Tamagawa, T., Tamura, K., Tanaka, T., Tsunemi, H., Uchida, H., Uchiyama, Y., and Yamauchi, S.
Abstract: Most supernova remnants (SNRs) are old, in the sense that their structure has been profoundly modified by their interaction with the surrounding interstellar medium (ISM). Old SNRs are very heterogenous in terms of their appearance, reflecting differences in their evolutionary state, the environments in which SNe explode and in the explosion products. Some old SNRs are seen primarily as a result of a strong shock wave interacting with the ISM. Others, the so-called mixed-morphology SNRs, show central concentrations of emission, which may still show evidence of emission from the ejecta. Yet others, the pulsar wind nebulae (PWNe), are seen primarily as a result of emission powered by a pulsar; these SNRs often lack the detectable thermal emission from the primary shock. The underlying goal in all studies of old SNRs is to understand these differences, in terms of the SNe that created them, the nature of the ISM into which they are expanding, and the fundamental physical processes that govern their evolution. Here we identify three areas of study where ASTRO-H can make important contributions. These are constraining abundances and physical processes in mature limb-brightened SNRs, understanding the puzzling nature of mixed-morphology SNRs, and exploring the nature of PWNe. The Soft X-ray Spectrometer (SXS) on-board ASTRO-H will, as a result of its high spectral resolution, be the primary tool for addressing problems associated with old SNRs, supported by hard X-ray observations with the Hard X-ray Imager (HXI) to obtain broad band X-ray coverage., Comment: 25 pages, 17 figures, ASTRO-H White Paper
Published: 2014

25. ASTRO-H White Paper - White Dwarf

Author: Mukai, K., Yuasa, T., Harayama, A., Hayashi, T., Ishida, M., Long, K. S., Terada, Y., Tsujimoto, M., Mukai, K., Yuasa, T., Harayama, A., Hayashi, T., Ishida, M., Long, K. S., Terada, Y., and Tsujimoto, M.
Abstract: Interacting binaries in which a white dwarf accretes material from a companion --- cataclysmic variables (CVs) in which the mass loss is via Roche-lobe overflow, and symbiotic stars in which the white dwarf captures the wind of a late type giant --- are relatively commonplace. They display a wide range of behaviors in the optical, X-rays, and other wavelengths, which still often baffles observers and theorists alike. They are likely to be a significant contributor to the Galactic ridge X-ray emission, and the possibility that some CVs or symbiotic stars may be the progenitors of some of the Type Ia supernovae deserves serious consideration. Furthermore, these binaries serve as excellent laboratories in which to study physics of X-ray emission from high density plasma, accretion physics, reflection, and particle acceleration. ASTRO-H is well-matched to the study of X-ray emission from many of these objects. In particular, the excellent spectral resolution of the SXS will enable dynamical studies of the X-ray emitting plasma. We also discuss the possibility of identifying an accreting, near-Chandrasekhar-mass white dwarf by measuring the gravitational redshift of the 6.4 keV line., Comment: 25 pages, 20 figures, ASTRO-H White Paper
Published: 2014

26. ASTRO-H White Paper - Young Supernova Remnants

Author: Hughes, J. P., Safi-Harb, S., Bamba, A., Katsuda, S., Leutenegger, M., Long, K. S., Maeda, Y., Mori, K., Nakajima, H., Sawada, M., Tanaka, T., Uchida, H., Yamaguchi, H., Aharonian, F., Funk, S., Hiraga, J., Ishida, M., Koyama, K., Matsumoto, H., Nobukawa, M., Ozaki, M., Tamagawa, T., Tsunemi, H., Tomida, H., Uchiyama, Y., Uno, S., Hughes, J. P., Safi-Harb, S., Bamba, A., Katsuda, S., Leutenegger, M., Long, K. S., Maeda, Y., Mori, K., Nakajima, H., Sawada, M., Tanaka, T., Uchida, H., Yamaguchi, H., Aharonian, F., Funk, S., Hiraga, J., Ishida, M., Koyama, K., Matsumoto, H., Nobukawa, M., Ozaki, M., Tamagawa, T., Tsunemi, H., Tomida, H., Uchiyama, Y., and Uno, S.
Abstract: Thanks to the unprecedented spectral resolution and sensitivity of the Soft X-ray Spectrometer (SXS) to soft thermal X-ray emission, ASTRO-H will open a new discovery window for understanding young, ejecta-dominated, supernova remnants (SNRs). In particular we study how ASTRO-H observations will address, comprehensively, three key topics in SNR research: (1) using abundance measurements to unveil SNR progenitors, (2) using spatial and velocity distribution of the ejecta to understand supernova explosion mechanisms, (3) revealing the link between the thermal plasma state of SNRs and the efficiency of their particle acceleration., Comment: 38 pages, 19 figures, ASTRO-H White Paper
Published: 2014

27. The PHEMU09 catalogue and astrometric results of the observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter made in 2009

Author: Arlot, J. -E., Emelyanov, N., Varfolomeev, M. I., Amossé, A., Arena, C., Assafin, M., Barbieri, L., Bolzoni, S., Bragas-Ribas, F., Camargo, J. I. B., Casarramona, F., Casas, R., Christou, A., Colas, F., Collard, A., Combe, S., Constantinescu, M., Dangl, G., De, Cat, P., Degenhardt, S., Delcroix, M., Dias-Oliveira, A., Dourneau, G., Douvris, A., Druon, C., Ellington, C. K., Estraviz, G., Farissier, P., Farmakopoulos, A., Garlitz, J., Gault, D., George, T., Gorda, S. Y., Grismore, J., Guo, D. F., Herald, D., Ida, M., Ishida, M., Ivanov, A. V., Klemt, B., Koshkin, N., Le, Campion, J. F., Liakos, A., Liao, S. L., Li, S. N., Loader, B., Lopresti, C., Lo, Savio, E., Marchini, A., Marino, G., Masi, G., Massallé, A., Maulella, R., Mcfarland, J., Miyashita, K., Napoli, C., Noyelles, B., Pauwels, T., Pavlov, H., Peng, Q. Y., Perelló, C., Priban, V., Prost, J., Razemon, S., Rousselle, J. P., Rovira, J., Ruisi, R., Ruocco, N., Salvaggio, F., Sbarufatti, G., Shakun, L., Scheck, A., Sciuto, C., Da, Silva, Neto, D. N., V, Sinyaeva, N., Sofia, A., Sonka, A., Talbot, J., Tang, Z. H., Tejfel, V. G., Thuillot, W., Tigani, K., Timerson, B., Tontodonati, E., Tsamis, V., Unwin, M., Venable, R., Vieira-Martins, R., Vilar, J., Vingerhoets, P., Watanabe, H., Yin, H. X., Yu, Y., Zambelli, R., Arlot, J. -E., Emelyanov, N., Varfolomeev, M. I., Amossé, A., Arena, C., Assafin, M., Barbieri, L., Bolzoni, S., Bragas-Ribas, F., Camargo, J. I. B., Casarramona, F., Casas, R., Christou, A., Colas, F., Collard, A., Combe, S., Constantinescu, M., Dangl, G., De, Cat, P., Degenhardt, S., Delcroix, M., Dias-Oliveira, A., Dourneau, G., Douvris, A., Druon, C., Ellington, C. K., Estraviz, G., Farissier, P., Farmakopoulos, A., Garlitz, J., Gault, D., George, T., Gorda, S. Y., Grismore, J., Guo, D. F., Herald, D., Ida, M., Ishida, M., Ivanov, A. V., Klemt, B., Koshkin, N., Le, Campion, J. F., Liakos, A., Liao, S. L., Li, S. N., Loader, B., Lopresti, C., Lo, Savio, E., Marchini, A., Marino, G., Masi, G., Massallé, A., Maulella, R., Mcfarland, J., Miyashita, K., Napoli, C., Noyelles, B., Pauwels, T., Pavlov, H., Peng, Q. Y., Perelló, C., Priban, V., Prost, J., Razemon, S., Rousselle, J. P., Rovira, J., Ruisi, R., Ruocco, N., Salvaggio, F., Sbarufatti, G., Shakun, L., Scheck, A., Sciuto, C., Da, Silva, Neto, D. N., V, Sinyaeva, N., Sofia, A., Sonka, A., Talbot, J., Tang, Z. H., Tejfel, V. G., Thuillot, W., Tigani, K., Timerson, B., Tontodonati, E., Tsamis, V., Unwin, M., Venable, R., Vieira-Martins, R., Vilar, J., Vingerhoets, P., Watanabe, H., Yin, H. X., Yu, Y., and Zambelli, R.
Abstract: Context. In 2009, the Sun and the Earth passed through the equatorial plane of Jupiter and therefore the orbital planes of its main satellites. It was the equinox on Jupiter. This occurrence made mutual occultations and eclipses between the satellites possible. Experience has shown that the observations of such events provide accurate astrometric data able to bring new information on the dynamics of the Galilean satellites. Observations are made under the form of photometric measurements, but need to be made through the organization of a worldwide observation campaign maximizing the number and the quality of the data obtained. Aims. This work focuses on processing the complete database of photometric observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter made during the international campaign in 2009. The final goal is to derive new accurate astrometric data. Methods. We used an accurate photometric model of mutual events adequate with the accuracy of the observation. Our original method was applied to derive astrometric data from photometric observations of mutual occultations and eclipses of the Galilean satellites of Jupiter. Results. We processed the 457 lightcurves obtained during the international campaign of photometric observations of the Galilean satellites of Jupiter in 2009. Compared with the theory, for successful observations, the r.m.s. of O-C residuals are equal to 45.8 mas and 81.1 mas in right ascension and declination, respectively; the mean O-C residuals are equal to -2 mas and -9 mas in right ascension and declination, respectively, for mutual occultations; and -6 mas and +1 mas in right ascension and declination, respectively, for mutual eclipses. © ESO, 2014.
Published: 2014

28. Modeling Dipolar Post-Shock Accretion Columns for Various Specific Accretion Rate Intermediate Polars

Author: Hayashi, T., Ishida, M., Hayashi, T., and Ishida, M.
Abstract: We model the post-shock accretion column (PSAC) for intermediate polars (IPs), with parameterizing specific accretion rate between 0.0001 and 100 g cm-2 s-1 and metal abundance between 0.1 and 2 times of solar abundance, and taking into account the gravitational potential and non-equipartition between ions, electrons and ionization degree. We assume the cylinder and dipole as geometry of the PSAC. The PSAC becomes higher against the white dwarf (WD) radius for lower specific accretion rate and more massive WD, and may be comparable to the WD radius. The consideration of the dipolar geometry significantly reduces the density and temperature over the whole PSAC comparing with the cylindrical case when the specific accretion rate is lower than a threshold which the PSAC height reachs 0.2 RWD with and is decreased by the more massive white dwarf. We calculate the spectra of the cylindrical and dipolar PSACs with the wide range of the specific accretion rate. Although the spectra soften as the specific accretion rate decreases for the both geometrical assumptions under the specific accretion rate threshold, the softening is more speedy for the dipolar PSAC. The fact means that the both geometrical assumptions lead the different WD masses for each other when their spectra are applied to the IPs hosting the low accretion or a massive WD. Although the ionization non-equilibrium are also involved for the spectral calculation, the effects are trivial because the radiation from ionization non-equilibrium plasma is a few percent of the whole at most., Comment: submitted to MNRAS, 11 pages, 10 figures
Published: 2013

29. Searching for Stoponium along with the Higgs boson

Author: Barger, V., Ishida, M., Keung, W. -Y., Barger, V., Ishida, M., and Keung, W. -Y.
Abstract: Stoponium, a bound state of top squark and its antiparticle in a supersymmetric model, may be found in the ongoing Higgs searches at the LHC. Its WW and ZZ detection ratios relative to the Standard Model Higgs boson can be more than unity from WW* threshold to the two Higgs threshold. The gamma gamma channel is equally promising. Some regions of the stoponium mass below 150 GeV are already being probed by the ATLAS and CMS experiments., Comment: 10 pages 5 figures
Published: 2011
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30. X-ray observation of AM Herculis in a very low state with Suzaku

Author: Terada, Y., Ishida, M., Bamba, A., Mukai, K., Hayashi, T., Harayama, A., Terada, Y., Ishida, M., Bamba, A., Mukai, K., Hayashi, T., and Harayama, A.
Abstract: The X-ray observation of AM Her in a very low state was performed with {\it Suzaku} in October 2008. One flare event with a time scale of $\sim$ 3700 sec was detected at the X-ray luminosity of $6.0 \times 10^{29} {\rm ~erg ~sec}^{-1}$ in the 0.5 -- 10 keV band assuming at a distance of 91 pc. The X-ray spectrum is represented by a thermal plasma emission model with a temperature of $8.67_{-1.14}^{+1.31}$ keV. During the quiescence out of the flare interval, {\it Suzaku} also detected significant X-rays at a luminosity of $1.7 \times 10^{29} {\rm ~erg ~sec}^{-1}$ in the 0.5 -- 10 keV band, showing a clear spin modulation at a period of 0.1289273(2) days at BJD 2454771.581. The X-ray spectra in the quiescence were represented by a MEKAL + Power Law (PL) model or a single CEMEKL model, which are also supported by phase-resolved analyses. A correlation between the temperature and the volume emission measure was found together with historical X-ray measurements of AM Her in various states. In order to account for a possible non-thermal emission from AM Her, particle acceleration mechanisms in the AM Her system are also discussed, including a new proposal of a shock acceleration process on the top of the accretion column., Comment: 16 pages, 9 figures, 4 tables, Accepted for publication in Astrophysical Journal
Published: 2010
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31. Test rig for micro gear and experimental analysis on the meshing condition and failure characteristics of steel micro involute gear and metallic glass one

Author: 90335191, Niza, M. E., Komori, M., Nomura, T., Yamaji, I., Nishiyama, N., Ishida, M., Shimizu, Y., 90335191, Niza, M. E., Komori, M., Nomura, T., Yamaji, I., Nishiyama, N., Ishida, M., and Shimizu, Y.
Published: 2010

32. Suzaku X-Ray Imaging and Spectroscopy of Cassiopeia A

Author: Maeda, Y., Uchiyama, Y., Bamba, A., Kosugi, H., Tsunemi, H., Helder, E. A., Vink, J., Kodaka, N., Terada, Y., Fukazawa, Y., Hiraga, J., Hughes, J. P., Kokubun, M., Kouzu, T., Matsumoto, H., Miyata, E., Nakamura, R., Okada, S., Someya, K., Tamagawa, T., Tamura, K., Totsuka, K., Tsuboi, Y., Ezoe, Y., Holt, S. S., Ishida, M., Kamae, T., Petre, R., Takahashi, T., Maeda, Y., Uchiyama, Y., Bamba, A., Kosugi, H., Tsunemi, H., Helder, E. A., Vink, J., Kodaka, N., Terada, Y., Fukazawa, Y., Hiraga, J., Hughes, J. P., Kokubun, M., Kouzu, T., Matsumoto, H., Miyata, E., Nakamura, R., Okada, S., Someya, K., Tamagawa, T., Tamura, K., Totsuka, K., Tsuboi, Y., Ezoe, Y., Holt, S. S., Ishida, M., Kamae, T., Petre, R., and Takahashi, T.
Abstract: Suzaku X-ray observations of a young supernova remnant, Cassiopeia A, were carried out. K-shell transition lines from highly ionized ions of various elements were detected, including Chromium (Cr-Kalpha at 5.61 keV). The X-ray continuum spectra were modeled in the 3.4--40 keV band, summed over the entire remnant, and were fitted with a simplest combination of the thermal bremsstrahlung and the non-thermal cut-off power-law models. The spectral fits with this assumption indicate that the continuum emission is likely to be dominated by the non-thermal emission with a cut-off energy at > 1 keV. The thermal-to-nonthermal fraction of the continuum flux in the 4-10 keV band is best estimated as ~0.1. Non-thermal-dominated continuum images in the 4--14 keV band were made. The peak of the non-thermal X-rays appears at the western part. The peak position of the TeV gamma-rays measured with HEGRA and MAGIC is also shifted at the western part with the 1-sigma confidence. Since the location of the X-ray continuum emission was known to be presumably identified with the reverse shock region, the possible keV-TeV correlations give a hint that the accelerated multi-TeV hadrons in Cassiopeia A are dominated by heavy elements in the reverse shock region., Comment: Publ. Astron. Soc. Japan 61, pp.1217-1228 (2009)
Published: 2009
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33. Broad-band properties of the hard X-ray cataclysmic variables IGR J00234+6141 and 1RXS J213344.1+510725

Author: Anzolin, G., de Martino, D., Falanga, M., Mukai, K., Bonnet-Bidaud, J. -M., Mouchet, M., Terada, Y., Ishida, M., Anzolin, G., de Martino, D., Falanga, M., Mukai, K., Bonnet-Bidaud, J. -M., Mouchet, M., Terada, Y., and Ishida, M.
Abstract: A significant number of cataclysmic variables were detected as hard X-ray sources in the INTEGRAL survey, most of them of the magnetic intermediate polar type. We present a detailed X-ray broad-band study of two new sources, IGR J00234+6141 and 1RXS J213344.1+510725, that allow us to classify them as secure members of the intermediate polar class. Timing and spectral analysis of IGR J00234+6141 are based on a XMM-Newton observation and INTEGRAL publicly available data. For 1RXS J213344.1+510725 we use XMM-Newton and Suzaku observations at different epochs, as well as INTEGRAL publicly available data. We determine a spin period of 561.64 +/- 0.56 s for the white dwarf in IGR J00234+6141. The X-ray pulses are observed up to about 2 keV. From XMM-Newton and Suzaku observations of 1RXS J213344.1+510725, we find a rotational period of 570.862 +/- 0.034 s. The observations span three epochs where the pulsation is observed to change at different energies both in amplitude and shape. In both objects, the spectral analysis spanned over a wide energy range, from 0.3 to 100 keV, shows the presence of multiple emission components absorbed by dense material. The X-ray spectrum of IGR J00234+6141 is consistent with a multi-temperature plasma with a maximum temperature of about 50 keV. In 1RXS J213344.1+510725, multiple optically thin components are inferred, as well as an optically thick (blackbody) soft X-ray emission with a temperature of about 100 eV. This latter adds 1RXS J213344.1+510725 to the growing group of soft X-ray intermediate polars. (abridged), Comment: 12 pages, 8 figures, 5 tables. Accepted for publication in A&A
Published: 2009
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34. Prototype of real-time tumor-tracking system without implanted fiducial marker for proton therapy

Author: Terunuma, T, Sakae, T, Ishida, M, Sato, M, Yasuoka, K, Kumada, H, Okumura, T, Tsuboi, K, Sakurai, H, Terunuma, T, Sakae, T, Ishida, M, Sato, M, Yasuoka, K, Kumada, H, Okumura, T, Tsuboi, K, and Sakurai, H
Published: 2009

35. The NeXT Mission

Author: Takahashi, T., Kelley, R., Mitsuda, K., Kunieda, H., Petre, R., White, N., Dotani, T., Fujimoto, R., Fukazawa, Y., Hayashida, K., Ishida, M., Ishisaki, Y., Kokubun, M., Makishima, K., Koyama, K., Madejski, G. M., Mori, K., Mushotzky, R., Nakazawa, K., Ogasaka, Y., Ohashi, T., Ozaki, M., Tajima, H., Tashiro, M., Terada, Y., Tsunemi, H., Tsuru, T. G., Ueda, Y., Yamasaki, N., Watanabe, S., team, the NeXT, Takahashi, T., Kelley, R., Mitsuda, K., Kunieda, H., Petre, R., White, N., Dotani, T., Fujimoto, R., Fukazawa, Y., Hayashida, K., Ishida, M., Ishisaki, Y., Kokubun, M., Makishima, K., Koyama, K., Madejski, G. M., Mori, K., Mushotzky, R., Nakazawa, K., Ogasaka, Y., Ohashi, T., Ozaki, M., Tajima, H., Tashiro, M., Terada, Y., Tsunemi, H., Tsuru, T. G., Ueda, Y., Yamasaki, N., Watanabe, S., and team, the NeXT
Abstract: The NeXT (New exploration X-ray Telescope), the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2013. NeXT is a combination of wide band X-ray spectroscopy (3 - 80 keV) provided by multi-layer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3 - 10 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope and a non-focusing soft gamma-ray detector. With these instruments, NeXT covers very wide energy range from 0.3 keV to 600 keV. The micro-calorimeter system will be developed by international collaboration lead by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of Delta E ~ 7 eV by the micro-calorimeter will enable a wide variety of important science themes to be pursued., Comment: 14 pages, 10 figures, Proceedings of the SPIE meeting, "Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray 2008", Marseille (2008)
Published: 2008
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36. DIOS: the Diffuse Intergalactic Oxygen Surveyor

Author: Ohashi, T., Ishida, M., Sasaki, S., Ishisaki, Y., Mitsuda, K., Yamasaki, N. Y., Fujimoto, R., Takei, Y., Tawara, Y., Furuzawa, A., Suto, Y., Yoshikawa, K., Kawahara, H., Kawai, N., Tsuru, T. G., Matsushita, K., Kitayama, T., Ohashi, T., Ishida, M., Sasaki, S., Ishisaki, Y., Mitsuda, K., Yamasaki, N. Y., Fujimoto, R., Takei, Y., Tawara, Y., Furuzawa, A., Suto, Y., Yoshikawa, K., Kawahara, H., Kawai, N., Tsuru, T. G., Matsushita, K., and Kitayama, T.
Abstract: We present our proposal for a small X-ray mission DIOS (Diffuse Intergalactic Oxygen Surveyor), consisting of a 4-stage X-ray telescope and an array of TES microcalorimeters, cooled with mechanical coolers, with a total weight of about 400 kg. The mission will perform survey observations of warm-hot intergalactic medium using OVII and OVIII emission lines, with the energy coverage up to 1.5 keV. The wide field of view of about 50' diameter, superior energy resolution close to 2 eV FWHM, and very low background will together enable us a wide range of science for diffuse X-ray sources. We briefly describe the design of the satellite, performance of the subsystems and the expected results., Comment: 9 pages, 11 figures, a proceedings of SPIE "Astronomical Telescopes and Instrumentation" 2006
Published: 2006
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37. XMM-Newton Observation of IC 310 in the Outer Region of the Perseus Cluster of Galaxies

Author: Sato, K., Furusho, T., Yamasaki, N. Y., Ishida, M., Matsushita, K., Ohashi, T., Sato, K., Furusho, T., Yamasaki, N. Y., Ishida, M., Matsushita, K., and Ohashi, T.
Abstract: We present results from an XMM-Newton observation of the head-tail radio galaxy IC 310 located in the southwest region of the Perseus cluster. The spectrum is well-fitted by an absorbed power-law model with a photon index of $2.50 \pm 0.02$ with no significant absorption excess. The X-ray image shows a point-like emission at IC 310 without any signs of a structure correlated with the radio halo tail. The temperature of the intracluster medium surrounding IC 310 declines as a function of distance from the cluster center, from $ kT \sim 6$ keV in the northeast corner of the field of view to about 3 keV in the southwest region. Although we do not find any sharp edges in the surface brightness profile, a brightness excess over a smooth $\beta$ model by about 20% is seen. The temperature also rises by about 10% in the same region. This indicates that the IC 310 region is a subcluster probably infalling into the Perseus cluster, and the gas in front of IC 310 towards the Perseus cluster is likely to be compressed by the large-scale motion, which supports the view that the IC 310 system is undergoing a merger., Comment: 7 pages, 8 figures (including color), accepted for publication in PASJ
Published: 2005
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38. Theoretical fine spectroscopy with SAC-CI method: Outer- and inner-valence ionization spectra of CO and N-2

Author: Ehara, M, Ishida, M, Nakatsuji, H, Ehara, M, Ishida, M, and Nakatsuji, H
Published: 2005

39. Locating the Warm-Hot Intergalactic Medium in the Simulated Local Universe

Author: Yoshikawa, K., Dolag, K., Suto, Y., Sasaki, S., Yamasaki, N. Y., Ohashi, T., Mitsuda, K., Tawara, Y., Fujimoto, R., Furusho, T., Furuzawa, A., Ishida, M., Ishisaki, Y., Takei, Y., Yoshikawa, K., Dolag, K., Suto, Y., Sasaki, S., Yamasaki, N. Y., Ohashi, T., Mitsuda, K., Tawara, Y., Fujimoto, R., Furusho, T., Furuzawa, A., Ishida, M., Ishisaki, Y., and Takei, Y.
Abstract: We present an analysis of mock spectral observation of warm-hot intergalactic medium (WHIM) using a constrained simulation of the local universe. The simulated map of oxygen emission lines from local WHIM reproduces well the observed structures traced by galaxies in the real local universe. We further attempt to perform mock observations of outer parts of simulated Coma cluster and A3627 adopting the expected performance of DIOS (Diffuse Intergalactic Oxygen Surveyor), which is proposed as a dedicated soft X-ray mission to search for cosmic missing baryons. We find that WHIMs surrounding nearby clusters are detectable with a typical exposure time of a day, and thus constitute realistic and promising targets for DIOS. We also find that an X-ray emitting clump in front of Coma cluster, recently reported in the XMM-Newton observation, has a counterpart in the simulated local universe, and its observed spectrum can be well reproduced in the simulated local universe if the gas temperature is set to the observationally estimated value., Comment: 25 pages, 3 tables, 16 figures. Accepted for publication in PASJ. High resolution PS/PDF files are available at http://www-utap.phys.s.u-tokyo.ac.jp/~kohji/research/x-ray/index.html
Published: 2004
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40. Future Japanese missions for the study of warm-hot intergalactic medium

Author: Ohashi, T., Ishida, M., Sasaki, S., Ishisaki, Y., Mitsuda, K., Yamasaki, N. Y., Fujimoto, R., Furusho, T., Kunieda, H., Tawara, Y., Furuzawa, A., Suto, Y., Yoshikawa, K., Ohashi, T., Ishida, M., Sasaki, S., Ishisaki, Y., Mitsuda, K., Yamasaki, N. Y., Fujimoto, R., Furusho, T., Kunieda, H., Tawara, Y., Furuzawa, A., Suto, Y., and Yoshikawa, K.
Abstract: We present our proposal for a small X-ray mission DIOS (Diffuse Intergalactic Oxygen Surveyor) to perform survey observations of warm-hot intergalactic medium using OVII and OVIII emission lines. This will be proposed to a small satellite program planned by ISAS/JAXA in Japan for a launch in 2008. The instrument consists of an array of TES microcalorimeters with an energy resolution 2 eV, cooled by mechanical coolers. The X-ray telescope will employ 4-stage reflection mirrors with a focal length as short as 70 cm and an angular resolution 2'. In addition to DIOS, we briefly describe the NeXT (New X-ray Telescope) mission, which is a larger Japanese X-ray observatory to be launched in 2010 and plans to explore non-thermal processes in the universe., Comment: 6 pages, 9 figures. To appear in the proceedings of "Modelling the Intergalactic and Intracluster Media", Vulcano Island, October 1-4, 2003
Published: 2004

41. Analytical energy gradient of the symmetry-adapted-cluster configuration-interaction general-R method for singlet to septet ground and excited states

Author: Ishida, M, Toyota, K, Ehara, M, Frisch, MJ, Nakatsuji, H, Ishida, M, Toyota, K, Ehara, M, Frisch, MJ, and Nakatsuji, H
Published: 2004

42. Energetics of the electron transfer from bacteriopheophytin to ubiquinone in the photosynthetic reaction center of Rhodopseudomonas viridis: Theoretical study

Author: Hasegawa, JY, Ishida, M, Nakatsuji, H, Lu, ZY, Liu, HY, Yang, WT, Hasegawa, JY, Ishida, M, Nakatsuji, H, Lu, ZY, Liu, HY, and Yang, WT
Published: 2003

43. Singularity-free analytical energy gradients for the SAC/SAC-CI method: coupled perturbed minimum orbital-deformation (CPMOD) approach

Author: Toyota, K, Ishida, M, Ehara, M, Frisch, MJ, Nakatsuji, H, Toyota, K, Ishida, M, Ehara, M, Frisch, MJ, and Nakatsuji, H
Published: 2003

44. Fine theoretical spectroscopy using symmetry adapted cluster-configuration interaction general-R method: Outer- and inner-valence ionization spectra of CS2 and OCS

Author: Ehara, M, Ishida, M, Nakatsuji, H, Ehara, M, Ishida, M, and Nakatsuji, H
Published: 2002

45. Outer- and inner-valence ionization spectra of NH3, PH3, and AsH3: symmetry-adapted cluster configuration interaction general-R study

Author: Ishida, M, Ehara, M, Nakatsuji, H, Ishida, M, Ehara, M, and Nakatsuji, H
Published: 2002

46. X-Ray Beaming due to Resonance Scattering in the Accretion Column of Magnetic Cataclysmic Variables

Author: Terada, Yukikatsu., Ishida, M., Makishima, K., Imanari, T., Fujimoto, R., Matsuzaki, K., Kaneda, H., Terada, Yukikatsu., Ishida, M., Makishima, K., Imanari, T., Fujimoto, R., Matsuzaki, K., and Kaneda, H.
Abstract: Extremely strong ionized Fe emission lines, with the equivalent width reaching about 4000 eV, were discovered with ASCA from a few Galactic compact objects, including AX J2315-0592, RX J1802.1+1804 and AX J1842.8-0423. These objects are thought to be binary systems containing magnetized white dwarfs (WDs). A possible interpretation of the strong Fe-K line is the line-photon collimation in the WD accretion column, due to resonance scattering of line photons. The collimation occurs when the accretion column has a flat shape, and the effect is augmented by the vertical velocity gradient there, which reduces the resonant trapping of resonant photons along the magnetic field lines. This effect was quantitatively confirmed with Monte-Carlo simulations. Furthermore, with ASCA observations of the polar V834 Centauri, this collimation effect was clearly detected as a rotational modulation of the equivalent width of the Fe-K emission line. Extremely strong emission lines mentioned above can be explained by our interpretation consistently. Combing this effect with other X-ray information, the geometry and plasma parameters in the accretion column were determined., Comment: 16 pages, Postscript, 32 figures, and 4 tables; accepted for MNRAS (Monthly Notices of The Royal Astronomical Society) on July 24, 2001
Published: 2001
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47. Analytical energy gradients of the excited, ionized and electron-attached states calculated by the SAC-CI general-R method

Author: Ishida, M, Toyota, K, Ehara, M, Nakatsuji, H, Ishida, M, Toyota, K, Ehara, M, and Nakatsuji, H
Published: 2001

48. Analytical energy gradient of high-spin multiplet state calculated by the SAC-CI method

Author: Ishida, M, Toyota, K, Ehara, M, Nakatsuji, H, Ishida, M, Toyota, K, Ehara, M, and Nakatsuji, H
Published: 2001

49. Theoretical study on the outer- and inner-valence ionization spectra of H2O, H2S and H2Se using the SAC-Cl general-R method

Author: Ehara, M, Ishida, M, Nakatsuji, H, Ehara, M, Ishida, M, and Nakatsuji, H
Published: 2001

50. Temperature Map of the Virgo Cluster of Galaxies Observed with ASCA

Author: Shibata, R., Matsushita, K., Yamasaki, N. Y., Ohashi, T., Ishida, M., Kikuchi, K., Boehringer, H., Matsumoto, H., Shibata, R., Matsushita, K., Yamasaki, N. Y., Ohashi, T., Ishida, M., Kikuchi, K., Boehringer, H., and Matsumoto, H.
Abstract: The temperature distribution of the intracluster medium (ICM) in the Virgo cluster of galaxies has been derived from extensive mapping observations with ASCA covering an area of 19 deg^2. In the spectral analysis, the inner region within a radius of ~60' from M87 is characterized by an ICM temperature of kT \~2.5 keV with little variation. On the other hand, the outer regions indicate significant variation of the temperature with an amplitude of about 1 keV. The temperature map was produced from the hardness ratio (H.R.) values with a resolution of about 5'. Besides the previously reported hot region with kT > 4 keV between M87 and M49, several hot regions with kT = 3-4 keV are detected in the cluster outskirts. The auto-correlation function for the H.R. variation shows that the temperature variation is correlated within a size of about 300 kpc, suggesting that gas blobs falling in the Virgo cluster have a typical size of groups of galaxies. A correlation with the velocity dispersion of member galaxies shows that only the north-west region indicates an unusually large beta_spec value of 2-4. The upper limit for extended non-thermal emission in the Virgo cluster is obtained to be L_X ~9 x 10^41 ergs/s in the 2 - 10 keV band. We discuss that these features consistently indicate that the Virgo cluster is in a relatively early stage of the cluster evolution., Comment: 37 pages, including 12 Postscript figures, accepted for publication in ApJ
Published: 2000
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