Astrophysics and Space Science Proceedings

Eduardo de la Fuente, Tomas Oceguera-Becerra, Guillermo García-Torales, José Luis García-Luna, A. U. Abeysekara, A. Aguilar, J. A. Aguilar, S. Aguilar, R. Alfaro, E. Almaraz, C. Álvarez, J. De D. Álvarez-Romero, M. Álvarez, R. Arceo, J. C. Arteaga-Velázquez, C. Badillo, A. Barber, B. M. Baughman, N. Bautista-Elivar, E. Belmont & 30 others E. Benítez, S. Y. Benzvi, D. Berley, A. Bernal, E. Bonamente, J. Braun, R. Caballero-Lopez, I. Cabrera, A. Carramiñana, L. Carrasco, M. Castillo, L. Chambers, R. Conde, P. Condreay, U. Cotti, J. Cotzomi, J. C. D’Olivo, E. De La Fuente, C. de León, S. Delay, D. Delepine, T. Deyoung, L. Diaz, L. Diaz-Cruz, B. L. Dingus, M. A. Duvernois, D. Edmunds, R. W. Ellsworth, B. Fick, J. Martínez-Castro

Research output: Contribution to conferencePaperResearch

Abstract

© Springer-Verlag Berlin Heidelberg 2013. The High Altitude Water Čerenkov observatory is a second generation ground based very high-energy γ-ray detector under construction in Sierra Negra, Puebla, México at an altitude of 4,100m. Higher altitude, improved design and a larger physical size used to reject cosmic ray background, make HAWC 10–20 times more sensitive than its predecessorMilagro. HAWC’s large field of view (~2 sr) and over 90% duty cycle make it ideal to search for several types of TeV astronomical γ-ray sources, diffuse emission, cosmic anisotropy, and transients. Details and status of HAWC at date, and a galactic star formation application are here presented.
Original languageAmerican English
Pages439-446
Number of pages8
DOIs
StatePublished - 1 Jan 2013
Eventconference -
Duration: 1 Jan 2013 → …

Conference

Conferenceconference
Period1/01/13 → …

Fingerprint

aerospace sciences
high altitude
congressional reports
rays
astrophysics
field of view
star formation
cosmic rays
observatories
anisotropy
cycles
detectors
water
energy

Cite this

de la Fuente, E., Oceguera-Becerra, T., García-Torales, G., García-Luna, J. L., Abeysekara, A. U., Aguilar, A., ... Martínez-Castro, J. (2013). Astrophysics and Space Science Proceedings. 439-446. Paper presented at conference, . https://doi.org/10.1007/978-3-642-35410-6_32
de la Fuente, Eduardo ; Oceguera-Becerra, Tomas ; García-Torales, Guillermo ; García-Luna, José Luis ; Abeysekara, A. U. ; Aguilar, A. ; Aguilar, J. A. ; Aguilar, S. ; Alfaro, R. ; Almaraz, E. ; Álvarez, C. ; Álvarez-Romero, J. De D. ; Álvarez, M. ; Arceo, R. ; Arteaga-Velázquez, J. C. ; Badillo, C. ; Barber, A. ; Baughman, B. M. ; Bautista-Elivar, N. ; Belmont, E. ; Benítez, E. ; Benzvi, S. Y. ; Berley, D. ; Bernal, A. ; Bonamente, E. ; Braun, J. ; Caballero-Lopez, R. ; Cabrera, I. ; Carramiñana, A. ; Carrasco, L. ; Castillo, M. ; Chambers, L. ; Conde, R. ; Condreay, P. ; Cotti, U. ; Cotzomi, J. ; D’Olivo, J. C. ; De La Fuente, E. ; de León, C. ; Delay, S. ; Delepine, D. ; Deyoung, T. ; Diaz, L. ; Diaz-Cruz, L. ; Dingus, B. L. ; Duvernois, M. A. ; Edmunds, D. ; Ellsworth, R. W. ; Fick, B. ; Martínez-Castro, J. / Astrophysics and Space Science Proceedings. Paper presented at conference, .8 p.
@conference{7c71ea24c5ff4fba9c923069eca4ffd1,
title = "Astrophysics and Space Science Proceedings",
abstract = "{\circledC} Springer-Verlag Berlin Heidelberg 2013. The High Altitude Water Čerenkov observatory is a second generation ground based very high-energy γ-ray detector under construction in Sierra Negra, Puebla, M{\'e}xico at an altitude of 4,100m. Higher altitude, improved design and a larger physical size used to reject cosmic ray background, make HAWC 10–20 times more sensitive than its predecessorMilagro. HAWC’s large field of view (~2 sr) and over 90{\%} duty cycle make it ideal to search for several types of TeV astronomical γ-ray sources, diffuse emission, cosmic anisotropy, and transients. Details and status of HAWC at date, and a galactic star formation application are here presented.",
author = "{de la Fuente}, Eduardo and Tomas Oceguera-Becerra and Guillermo Garc{\'i}a-Torales and Garc{\'i}a-Luna, {Jos{\'e} Luis} and Abeysekara, {A. U.} and A. Aguilar and Aguilar, {J. A.} and S. Aguilar and R. Alfaro and E. Almaraz and C. {\'A}lvarez and {\'A}lvarez-Romero, {J. De D.} and M. {\'A}lvarez and R. Arceo and Arteaga-Vel{\'a}zquez, {J. C.} and C. Badillo and A. Barber and Baughman, {B. M.} and N. Bautista-Elivar and E. Belmont and E. Ben{\'i}tez and Benzvi, {S. Y.} and D. Berley and A. Bernal and E. Bonamente and J. Braun and R. Caballero-Lopez and I. Cabrera and A. Carrami{\~n}ana and L. Carrasco and M. Castillo and L. Chambers and R. Conde and P. Condreay and U. Cotti and J. Cotzomi and D’Olivo, {J. C.} and {De La Fuente}, E. and {de Le{\'o}n}, C. and S. Delay and D. Delepine and T. Deyoung and L. Diaz and L. Diaz-Cruz and Dingus, {B. L.} and Duvernois, {M. A.} and D. Edmunds and Ellsworth, {R. W.} and B. Fick and J. Mart{\'i}nez-Castro",
year = "2013",
month = "1",
day = "1",
doi = "10.1007/978-3-642-35410-6_32",
language = "American English",
pages = "439--446",
note = "conference ; Conference date: 01-01-2013",

}

de la Fuente, E, Oceguera-Becerra, T, García-Torales, G, García-Luna, JL, Abeysekara, AU, Aguilar, A, Aguilar, JA, Aguilar, S, Alfaro, R, Almaraz, E, Álvarez, C, Álvarez-Romero, JDD, Álvarez, M, Arceo, R, Arteaga-Velázquez, JC, Badillo, C, Barber, A, Baughman, BM, Bautista-Elivar, N, Belmont, E, Benítez, E, Benzvi, SY, Berley, D, Bernal, A, Bonamente, E, Braun, J, Caballero-Lopez, R, Cabrera, I, Carramiñana, A, Carrasco, L, Castillo, M, Chambers, L, Conde, R, Condreay, P, Cotti, U, Cotzomi, J, D’Olivo, JC, De La Fuente, E, de León, C, Delay, S, Delepine, D, Deyoung, T, Diaz, L, Diaz-Cruz, L, Dingus, BL, Duvernois, MA, Edmunds, D, Ellsworth, RW, Fick, B & Martínez-Castro, J 2013, 'Astrophysics and Space Science Proceedings' Paper presented at conference, 1/01/13, pp. 439-446. https://doi.org/10.1007/978-3-642-35410-6_32

Astrophysics and Space Science Proceedings. / de la Fuente, Eduardo; Oceguera-Becerra, Tomas; García-Torales, Guillermo; García-Luna, José Luis; Abeysekara, A. U.; Aguilar, A.; Aguilar, J. A.; Aguilar, S.; Alfaro, R.; Almaraz, E.; Álvarez, C.; Álvarez-Romero, J. De D.; Álvarez, M.; Arceo, R.; Arteaga-Velázquez, J. C.; Badillo, C.; Barber, A.; Baughman, B. M.; Bautista-Elivar, N.; Belmont, E.; Benítez, E.; Benzvi, S. Y.; Berley, D.; Bernal, A.; Bonamente, E.; Braun, J.; Caballero-Lopez, R.; Cabrera, I.; Carramiñana, A.; Carrasco, L.; Castillo, M.; Chambers, L.; Conde, R.; Condreay, P.; Cotti, U.; Cotzomi, J.; D’Olivo, J. C.; De La Fuente, E.; de León, C.; Delay, S.; Delepine, D.; Deyoung, T.; Diaz, L.; Diaz-Cruz, L.; Dingus, B. L.; Duvernois, M. A.; Edmunds, D.; Ellsworth, R. W.; Fick, B.; Martínez-Castro, J.

2013. 439-446 Paper presented at conference, .

Research output: Contribution to conferencePaperResearch

TY - CONF

T1 - Astrophysics and Space Science Proceedings

AU - de la Fuente, Eduardo

AU - Oceguera-Becerra, Tomas

AU - García-Torales, Guillermo

AU - García-Luna, José Luis

AU - Abeysekara, A. U.

AU - Aguilar, A.

AU - Aguilar, J. A.

AU - Aguilar, S.

AU - Alfaro, R.

AU - Almaraz, E.

AU - Álvarez, C.

AU - Álvarez-Romero, J. De D.

AU - Álvarez, M.

AU - Arceo, R.

AU - Arteaga-Velázquez, J. C.

AU - Badillo, C.

AU - Barber, A.

AU - Baughman, B. M.

AU - Bautista-Elivar, N.

AU - Belmont, E.

AU - Benítez, E.

AU - Benzvi, S. Y.

AU - Berley, D.

AU - Bernal, A.

AU - Bonamente, E.

AU - Braun, J.

AU - Caballero-Lopez, R.

AU - Cabrera, I.

AU - Carramiñana, A.

AU - Carrasco, L.

AU - Castillo, M.

AU - Chambers, L.

AU - Conde, R.

AU - Condreay, P.

AU - Cotti, U.

AU - Cotzomi, J.

AU - D’Olivo, J. C.

AU - De La Fuente, E.

AU - de León, C.

AU - Delay, S.

AU - Delepine, D.

AU - Deyoung, T.

AU - Diaz, L.

AU - Diaz-Cruz, L.

AU - Dingus, B. L.

AU - Duvernois, M. A.

AU - Edmunds, D.

AU - Ellsworth, R. W.

AU - Fick, B.

AU - Martínez-Castro, J.

PY - 2013/1/1

Y1 - 2013/1/1

N2 - © Springer-Verlag Berlin Heidelberg 2013. The High Altitude Water Čerenkov observatory is a second generation ground based very high-energy γ-ray detector under construction in Sierra Negra, Puebla, México at an altitude of 4,100m. Higher altitude, improved design and a larger physical size used to reject cosmic ray background, make HAWC 10–20 times more sensitive than its predecessorMilagro. HAWC’s large field of view (~2 sr) and over 90% duty cycle make it ideal to search for several types of TeV astronomical γ-ray sources, diffuse emission, cosmic anisotropy, and transients. Details and status of HAWC at date, and a galactic star formation application are here presented.

AB - © Springer-Verlag Berlin Heidelberg 2013. The High Altitude Water Čerenkov observatory is a second generation ground based very high-energy γ-ray detector under construction in Sierra Negra, Puebla, México at an altitude of 4,100m. Higher altitude, improved design and a larger physical size used to reject cosmic ray background, make HAWC 10–20 times more sensitive than its predecessorMilagro. HAWC’s large field of view (~2 sr) and over 90% duty cycle make it ideal to search for several types of TeV astronomical γ-ray sources, diffuse emission, cosmic anisotropy, and transients. Details and status of HAWC at date, and a galactic star formation application are here presented.

U2 - 10.1007/978-3-642-35410-6_32

DO - 10.1007/978-3-642-35410-6_32

M3 - Paper

SP - 439

EP - 446

ER -

de la Fuente E, Oceguera-Becerra T, García-Torales G, García-Luna JL, Abeysekara AU, Aguilar A et al. Astrophysics and Space Science Proceedings. 2013. Paper presented at conference, . https://doi.org/10.1007/978-3-642-35410-6_32