Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Álvarez JD"'
Autor:
Jiménez-Zarazúa O, Vélez-Ramírez LN, Alcocer-León M, Utrilla-Álvarez JD, Martínez-Rivera MA, Flores-Saldaña GA, Mondragón JD
Publikováno v:
Journal of Clinical Tuberculosis and Other Mycobacterial Diseases, Vol 16, Iss , Pp - (2019)
Conditions, where the patient's immune system is compromised are the main risk factor for mucormycosis. Approximately 23% of the world's population is estimated to have a latent Mycobacterium tuberculosis infection and more than 10 million new cases
Externí odkaz:
https://doaj.org/article/7acb1761fbfe48a6b3d996fc62b8a61c
Autor:
María Alcocer-León, Utrilla-Álvarez Jd, María Andrea Martínez-Rivera, Jaime D Mondragón, Lourdes N Vélez-Ramírez, Flores-Saldaña Ga, Omar Jiménez-Zarazúa
Publikováno v:
Journal of Clinical Tuberculosis and Other Mycobacterial Diseases, 16:100105. De Tijdstroom/Elsevier
Journal of Clinical Tuberculosis and Other Mycobacterial Diseases
Journal of Clinical Tuberculosis and Other Mycobacterial Diseases, Vol 16, Iss, Pp-(2019)
Journal of Clinical Tuberculosis and Other Mycobacterial Diseases
Journal of Clinical Tuberculosis and Other Mycobacterial Diseases, Vol 16, Iss, Pp-(2019)
Conditions, where the patient's immune system is compromised are the main risk factor for mucormycosis. Approximately 23% of the world's population is estimated to have a latent Mycobacterium tuberculosis infection and more than 10 million new cases
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b48d756a34f377b4992a36b63b406aaf
https://research.rug.nl/en/publications/0d6d5999-5adf-42f0-b9e5-8027056115f1
https://research.rug.nl/en/publications/0d6d5999-5adf-42f0-b9e5-8027056115f1
Autor:
Abeysekara, AU, Albert, A, Alfaro, R, Alvarez, C, Álvarez, JD, Arceo, R, Arteaga-Velázquez, JC, Solares, HAA, Barber, AS, Bautista-Elivar, N, Becerril, A, Belmont-Moreno, E, Benzvi, SY, Berley, D, Braun, J, Brisbois, C, Caballero-Mora, KS, Capistrán, T, Carramiñana, A, Casanova, S, Castillo, M, Cotti, U, Cotzomi, J, León, SCD, Fuente, EDL, León, CD, Deyoung, T, Dingus, BL, Duvernois, MA, Díaz-Vélez, JC, Ellsworth, RW, Fiorino, DW, Fraija, N, García-González, JA, Gerhardt, M, Munöz, AG, González, MM, Goodman, JA, Hampel-Arias, Z, Harding, JP, Hernandez, S, Hernandez-Almada, A, Hinton, J, Hui, CM, Hüntemeyer, P, Iriarte, A, Jardin-Blicq, A, Joshi, V, Kaufmann, S, Kieda, D, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, Vargas, HL, Linnemann, JT, Longinotti, AL, Raya, GL, Luna-García, R, López-Coto, R, Malone, K, Marinelli, SS, Martinez, O, Martinez-Castellanos, I, Martínez-Castro, J, Martínez-Huerta, H, Matthews, JA, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Nisa, MU, Noriega-Papaqui, R, Pelayo, R, Pretz, J, Pérez-Pérez, EG, Ren, Z, Rho, CD, Rivière, C, Rosa-González, D, Rosenberg, M, Ruiz-Velasco, E, Salazar, H, Greus, FS, Sandoval, A, Schneider, M, Schoorlemmer, H, Sinnis, G, Smith, AJ, Springer, RW, Surajbali, P, Taboada, I, Tibolla, O, Tollefson, K, Torres, I, Ukwatta, TN, Villaseñor, L, Weisgarber, T, Westerhoff, S
Publikováno v:
Abeysekara, AU; Albert, A; Alfaro, R; Alvarez, C; Álvarez, JD; Arceo, R; et al.(2017). Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory. Astrophysical Journal, 843(1). doi: 10.3847/1538-4357/aa7555. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/0f97m85c
© 2017. The American Astronomical Society. All rights reserved. The Crab Nebula is the brightest TeV gamma-ray source in the sky and has been used for the past 25 years as a reference source in TeV astronomy, for calibration and verification of new
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::a5f337a2baf7f74459799d8d5588b7bc
http://www.escholarship.org/uc/item/0f97m85c
http://www.escholarship.org/uc/item/0f97m85c
Autor:
Abeysekara, AU, Alfaro, R, Alvarez, C, Álvarez, JD, Arceo, R, Arteaga-Velázquez, JC, Solares, HA Ayala, Barber, AS, Baughman, BM, Bautista-Elivar, N, Reyes, AD Becerril, Belmont, E, BenZvi, SY, Bernal, A, Braun, J, Caballero-Mora, KS, Capistrán, T, Carramiñana, A, Casanova, S, Castillo, M, Cotti, U, Cotzomi, J, de León, S Coutińo, de la Fuente, E, De León, C, DeYoung, T, Hernandez, R Diaz, Dingus, BL, DuVernois, MA, Ellsworth, RW, Enriquez-Rivera, O, Fiorino, DW, Fraija, N, Garfias, F, González, MM, Goodman, JA, Gussert, M, Hampel-Arias, Z, Harding, JP, Hernandez, S, Hüntemeyer, P, Hui, CM, Imran, A, Iriarte, A, Karn, P, Kieda, D, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, Vargas, H León, Linnemann, JT, Longo, M, Raya, G Luis, Malone, K, Marinelli, A, Marinelli, SS, Martinez, H, Martinez, O, Martínez-Castro, J, Matthews, JA, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Noriega-Papaqui, R, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Ren, Z, Rivière, C, Rosa-González, D, Salazar, H, Greus, F Salesa, Sandoval, A, Schneider, M, Sinnis, G, Smith, AJ, Woodle, K Sparks, Springer, RW, Taboada, I, Tibolla, O, Tollefson, K, Torres, I, Ukwatta, TN, Villaseñor, L, Vrabel, K, Weisgarber, T, Westerhoff, S, Wisher, IG, Wood, J, Yapici, T, Yodh, GB, Younk, PW, Zaborov, D, Zepeda, A, Zhou, H
Publikováno v:
Astrophysical Journal, vol 817, iss 1
The Astrophysical Journal, vol 817, iss 1
The Astrophysical Journal, vol 817, iss 1
A survey of the inner Galaxy region of Galactic longitude l ∈[+15,+50] and latitude b ∈ [-4, +4] is performed using one-third of the High Altitude Water Cherenkov Observatory, operated during ts construction phase. To address the ambiguities aris
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4704814bdfd45552da353ec8664560a2
https://escholarship.org/uc/item/1pw9z9sc
https://escholarship.org/uc/item/1pw9z9sc
Autor:
Abdo, AA, Abeysekara, AU, Alfaro, R, Allen, BT, Alvarez, C, Álvarez, JD, Arceo, R, Arteaga-Velázquez, JC, Aune, T, Ayala Solares, HA, Barber, AS, Baughman, BM, Bautista-Elivar, N, Becerra Gonzalez, J, Belmont, E, Benzvi, SY, Berley, D, Bonilla Rosales, M, Braun, J, Caballero-Lopez, RA, Caballero-Mora, KS, Carramiñana, A, Castillo, M, Christopher, GE, Cotti, U, Cotzomi, J, De La Fuente, E, De León, C, Deyoung, T, Diaz Hernandez, R, Diaz-Cruz, L, Díaz-Vélez, JC, Dingus, BL, Duvernois, MA, Ellsworth, RW, Fiorino, DW, Fraija, N, Galindo, A, Garfias, F, González, MM, Goodman, JA, Grabski, V, Gussert, M, Hampel-Arias, Z, Harding, JP, Hays, E, Hoffman, CM, Hui, CM, Hüntemeyer, P, Imran, A, Iriarte, A, Karn, P, Kieda, D, Kolterman, BE, Kunde, GJ, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, León Vargas, H, Linares, EC, Linnemann, JT, Longo, M, Luna-Garcia, R, Macgibbon, JH, Marinelli, A, Marinelli, SS, Martinez, H, Martinez, O, Martínez-Castro, J, Matthews, JAJ, McEnery, J, Mendoza Torres, E, Mincer, AI, Miranda-Romagnoli, P, Moreno, E, Morgan, T, Mostafá, M, Nellen, L, Nemethy, P, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, T, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Rivière, C, Rosa-González, D, Ruiz-Velasco, E, Ryan, J, Salazar, H, Salesa, F, Sandoval, A, Saz Parkinson, PM, Schneider, M, Silich, S, Sinnis, G, Smith, AJ, Stump, D
Primordial Black Holes (PBHs) are gravitationally collapsed objects that may have been created by density fluctuations in the early universe and could have arbitrarily small masses down to the Planck scale. Hawking showed that due to quantum effects,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::7635674c960c14a4e33ad860b8038ba6
https://escholarship.org/uc/item/8cm6c2w1
https://escholarship.org/uc/item/8cm6c2w1
Autor:
Abeysekara, AU, Alfaro, R, Alvarez, C, Álvarez, JD, Arceo, R, Arteaga-Velázquez, JC, Solares, HAA, Barber, AS, Baughman, BM, Bautista-Elivar, N, Benzvi, SY, Rosales, MB, Braun, J, Caballero-Mora, KS, Carramiñana, A, Castillo, M, Cotti, U, Cotzomi, J, De La Fuente, E, De León, C, Deyoung, T, Hernandez, RD, Dingus, BL, Duvernois, MA, Ellsworth, RW, Fiorino, DW, Fraija, N, Galindo, A, Garfias, F, González, MM, Goodman, JA, Gussert, M, Hampel-Arias, Z, Harding, JP, Hüntemeyer, P, Hui, CM, Imran, A, Iriarte, A, Karn, P, Kieda, D, Kunde, GJ, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, Vargas, HL, Linnemann, JT, Longo, M, Luna-García, R, Malone, K, Marinelli, A, Marinelli, SS, Martinez, H, Martinez, O, Martínez-Castro, J, Matthews, JAJ, Torres, EM, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, TO, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Rivière, C, Rosa-González, D, Salazar, H, Greus, FS, Sandoval, A, Schneider, M, Sinnis, G, Smith, AJ, Woodle, KS, Springer, RW, Taboada, I, Tollefson, K, Torres, I, Ukwatta, TN, Villaseñor, L, Weisgarber, T, Westerhoff, S, Wisher, IG, Wood, J, Yodh, GB, Younk, PW
Publikováno v:
Abeysekara, AU; Alfaro, R; Alvarez, C; Álvarez, JD; Arceo, R; Arteaga-Velázquez, JC; et al.(2015). Search for gamma-rays from the unusually bright GRB 130427a with the hawc gamma-ray observatory. Astrophysical Journal, 800(2). doi: 10.1088/0004-637X/800/2/78. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/39h1v03d
© 2015. The American Astronomical Society. All rights reserved.. The first limits on the prompt emission from the long gamma-ray burst (GRB) 130427A in the >100 GeV energy band are reported. GRB 130427A was the most powerful burst ever detected with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::4e373ab50ed817fd050a4ba40ef21eaa
http://www.escholarship.org/uc/item/39h1v03d
http://www.escholarship.org/uc/item/39h1v03d
Autor:
Abeysekara, AU, Alfaro, R, Alvarez, C, Álvarez, JD, Ángeles, F, Arceo, R, Arteaga-Velázquez, JC, Avila-Aroche, A, Solares, HA Ayala, Badillo, C, Barber, AS, Baughman, BM, Bautista-Elivar, N, Gonzalez, J Becerra, Belmont, E, Benítez, E, BenZvi, SY, Berley, D, Bernal, A, Rosales, M Bonilla, Braun, J, Caballero-Lopez, RA, Caballero-Mora, KS, Cabrera, I, Carramiñana, A, Castañeda-Martínez, L, Castillo, M, Cotti, U, Cotzomi, J, de la Fuente, E, De León, C, DeYoung, T, Diaz-Azuara, A, Diaz-Cruz, L, Hernandez, R Diaz, Díaz-Vélez, JC, Dingus, BL, Dultzin, D, DuVernois, MA, Ellsworth, RW, Fernandez, A, Fiorino, DW, Fraija, N, Galindo, A, García-Torales, G, Garfias, F, González, A, González, LX, González, MM, Goodman, JA, Grabski, V, Gussert, M, Guzmán-Cerón, C, Hampel-Arias, Z, Harding, JP, Hernández-Cervantes, L, Hui, CM, Hüntemeyer, P, Imran, A, Iriarte, A, Karn, P, Kieda, D, Kunde, GJ, Langarica, R, Lara, A, Lara, G, Lauer, RJ, Lee, WH, Lennarz, D, Vargas, H León, Linares, EC, Linnemann, JT, Longo, M, Luna-Garcia, R, Marinelli, A, Martínez, LA, Martínez, H, Martínez, O, Martínez-Castro, J, Martos, M, Matthews, JAJ, McEnery, J, Torres, E Mendoza, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nava, J, Nellen, L, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, T, Page, DP, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Ramírez, I, Rentería, A, Rivière, C, Rosa-González, D
VAMOS1 was a prototype detector built in 2011 at an altitude of 4100 m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and data acquisition system of the HAWC observatory. HAWC is an air-sho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3335fdf79d04381828855c87a33b0e23
https://escholarship.org/uc/item/2h19n7r9
https://escholarship.org/uc/item/2h19n7r9
Autor:
Abeysekara, AU, Alfaro, R, Alvarez, C, Álvarez, JD, Arceo, R, Arteaga-Velázquez, JC, Ayala Solares, HA, Barber, AS, Baughman, BM, Bautista-Elivar, N, Becerra Gonzalez, J, Belmont, E, Benzvi, SY, Berley, D, Bonilla Rosales, M, Braun, J, Caballero-Lopez, RA, Caballero-Mora, KS, Carramiñana, A, Castillo, M, Cotti, U, Cotzomi, J, De La Fuente, E, De León, C, Deyoung, T, Diaz Hernandez, R, Diaz-Cruz, L, Díaz-Vélez, JC, Dingus, BL, Duvernois, MA, Ellsworth, RW, Fiorino, DW, Fraija, N, Galindo, A, Garfias, F, González, MM, Goodman, JA, Grabski, V, Gussert, M, Hampel-Arias, Z, Harding, JP, Hui, CM, Hüntemeyer, P, Imran, A, Iriarte, A, Karn, P, Kieda, D, Kunde, GJ, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, León Vargas, H, Linares, EC, Linnemann, JT, Longo, M, Luna-Garcia, R, Marinelli, A, Martinez, H, Martinez, O, Martínez-Castro, J, Matthews, JAJ, McEnery, J, Mendoza Torres, E, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, T, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Rivière, C, Rosa-González, D, Ryan, J, Salazar, H, Salesa, F, Sanchez, FE, Sandoval, A, Schneider, M, Silich, S, Sinnis, G, Smith, AJ, Sparks Woodle, K, Springer, RW, Taboada, I, Toale, PA, Tollefson, K, Torres, I, Ukwatta, TN
Publikováno v:
Abeysekara, AU; Alfaro, R; Alvarez, C; Álvarez, JD; Arceo, R; Arteaga-Velázquez, JC; et al.(2014). Sensitivity of HAWC to high-mass dark matter annihilations. Physical Review D-Particles, Fields, Gravitation and Cosmology, 90(12). doi: 10.1103/PhysRevD.90.122002. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/21n0435g
© 2014 American Physical Society. The High Altitude Water Cherenkov (HAWC) observatory is a wide field-of-view detector sensitive to gamma rays of 100 GeV to a few hundred TeV. Located in central Mexico at 19° North latitude and 4100 m above sea le
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::24670d08139e8684cd6a33b8542a5b06
http://www.escholarship.org/uc/item/21n0435g
http://www.escholarship.org/uc/item/21n0435g
Autor:
Abeysekara, AU, Alfaro, R, Alvarez, C, Álvarez, JD, Arceo, R, Arteaga-Velázquez, JC, Solares, HAA, Barber, AS, Baughman, BM, Bautista-Elivar, N, Belmont, E, BenZvi, SY, Berley, D, Rosales, MB, Braun, J, Caballero-Mora, KS, Carramiñana, A, Castillo, M, Cotti, U, Cotzomi, J, De La Fuente, E, De Léon, C, DeYoung, T, Hernandez, RD, Díaz-Vélez, JC, Dingus, BL, DuVernois, MA, Ellsworth, RW, Fiorino, DW, Fraija, N, Galindo, A, Garfias, F, González, MM, Goodman, JA, Gussert, M, Hampel-Arias, Z, Harding, JP, Hüntemeyer, P, Hui, CM, Imran, A, Iriarte, A, Karn, P, Kieda, D, Kunde, GJ, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, Vargas, HL, Linnemann, JT, Longo, M, Luna-García, R, Malone, K, Marinelli, A, Marinelli, SS, Martinez, H, Martinez, O, Martínez-Castro, J, Matthews, JAJ, McEnery, J, Torres, EM, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, T, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Rivìre, C, Rosa-González, D, Ruiz-Velasco, E, Ryan, J, Salazar, H, Greus, FS, Sandoval, A, Schneider, M, Sinnis, G, Smith, AJ, Sparks Woodle, K, Springer, RW, Taboada, I, Toale, PA, Tollefson, K, Torres, I, Ukwatta, TN, Villaseñor, L
Publikováno v:
Abeysekara, AU; Alfaro, R; Alvarez, C; Álvarez, JD; Arceo, R; Arteaga-Velázquez, JC; et al.(2014). Observation of small-scale anisotropy in the arrival direction distribution of TeV cosmic rays with HAWC. Astrophysical Journal, 796(2). doi: 10.1088/0004-637X/796/2/108. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/48x1w7zw
© 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A. The High-Altitude Water Cherenkov (HAWC) Observatory is sensitive to gamma rays and charged cosmic rays at TeV energies. The detector is still under construction,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::375e6063c388c431b80f711bfba9df0e
http://www.escholarship.org/uc/item/48x1w7zw
http://www.escholarship.org/uc/item/48x1w7zw
Autor:
Abeysekara, AU, Alfaro, R, Alvarez, C, Álvarez, JD, Arceo, R, Arteaga-Velázquez, JC, Ayala Solares, HA, Barber, AS, Baughman, BM, Bautista-Elivar, N, Belmont, E, Benzvi, SY, Berley, D, Bonilla Rosales, M, Braun, J, Caballero-Lopez, RA, Carramiñana, A, Castillo, M, Cotti, U, Cotzomi, J, De La Fuente, E, De León, C, Deyoung, T, Diaz Hernandez, R, Diaz-Velez, JC, Dingus, BL, Duvernois, MA, Ellsworth, RW, Fernandez, A, Fiorino, DW, Fraija, N, Galindo, A, Garcia-Luna, JL, Garcia-Torales, G, Garfias, F, González, LX, González, MM, Goodman, JA, Grabski, V, Gussert, M, Hampel-Arias, Z, Hui, CM, Hüntemeyer, P, Imran, A, Iriarte, A, Karn, P, Kieda, D, Kunde, GJ, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, León Vargas, H, Linares, EC, Linnemann, JT, Longo, M, Luna-García, R, Marinelli, A, Martinez, O, Martínez-Castro, J, Matthews, JAJ, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nava, J, Nellen, L, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, T, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Rivière, C, Ryan, J, Rosa-González, D, Salazar, H, Salesa, F, Sandoval, A, Santos, E, Schneider, M, Silich, S, Sinnis, G, Smith, AJ, Sparks, K, Springer, RW, Taboada, I, Toale, PA, Tollefson, K, Torres, I, Ukwatta, TN, Villaseñor, L, Weisgarber, T, Westerhoff, S, Wisher, IG, Wood, J, Yodh, GB
Publikováno v:
Abeysekara, AU; Alfaro, R; Alvarez, C; Álvarez, JD; Arceo, R; Arteaga-Velázquez, JC; et al.(2013). Sensitivity of the high altitude water Cherenkov detector to sources of multi-TeV gamma rays. Astroparticle Physics, 50-52, 26-32. doi: 10.1016/j.astropartphys.2013.08.002. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/8gh6s1vp
The High Altitude Water Cherenkov (HAWC) observatory is an array of large water Cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band between 100 GeV and 100 TeV. The observatory will be used to measure high-energy p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::26858f06531403bf21d4e46fe09fbdfb
http://www.escholarship.org/uc/item/8gh6s1vp
http://www.escholarship.org/uc/item/8gh6s1vp