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1. Assessing the efficacy of a Tier 2 early intervention for transcription skills in Spanish elementary school students

Author

Sara C. De León, Rocío C. Seoane, Eduardo García, and Juan E Jiménez

Subjects
Speech and Hearing, Linguistics and Language, Neuropsychology and Physiological Psychology, Education
Abstract

The main objective of this study was to evaluate the efficacy of a Tier 2 intervention within the context of the Response to Intervention (RtI) model implemented by Spanish first- to second-grade primary school teachers to improve at-risk students’ transcription skills. Teachers were instructed in the administration of a writing curriculum-based measure composed of 5 isolates measures (allographs, dictated words with arbitrary spelling or non-ruled, dictated words with rule-based spelling, dictated nonsense words, and dictated sentences) to identify at-risk students and to monitor their progress; and in the implementation of a systematic and explicit instructional program to improve transcription skills in at-risk students. A total of 164 at-risk students from 12 schools from the Canary Islands participated in the study. Teachers were provided with a support system that included a web-based training program for writing. Implementation fidelity was analyzed using direct observations and self-reports. All students were assessed three times during the academic year. In a hierarchical linear growth modeling procedure, differences in growth rates of transcription skills were compared between students who received the intervention, those who did not, and their typically achieving peers. Additionally, the effects of the intervention in the experimental at-risk group were also analyzed, differentiating between those who left the risk status and those who remained at-risk. Children at-risk in the intervention condition appeared to benefit more in handwriting skills than at-risk children in the control condition, but to a lesser extent in spelling accuracy. Nevertheless, improvements in both transcription skills had only been made in the experimental risk group that had left the risk situation.

Published
2022

2. HAWC Study of the Ultra-high-energy Spectrum of MGRO J1908+06

Author

A. Albert, R. Alfaro, C. Alvarez, J. D. Álvarez, J. R. Angeles Camacho, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, R. Babu, E. Belmont-Moreno, C. Brisbois, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, C. de León, R. Diaz Hernandez, B. L. Dingus, M. A. DuVernois, M. Durocher, J. C. Díaz-Vélez, K. Engel, C. Espinoza, K. L. Fan, K. Fang, M. Fernández Alonso, N. Fraija, D. Garcia, J. A. García-González, F. Garfias, G. Giacinti, H. Goksu, M. M. González, J. A. Goodman, J. P. Harding, J. Hinton, B. Hona, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, A. Jardin-Blicq, V. Joshi, S. Kaufmann, D. Kieda, W. H. Lee, J. Lee, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, V. Marandon, O. Martinez, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, J. A. Morales-Soto, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, M. U. Nisa, R. Noriega-Papaqui, L. Olivera-Nieto, N. Omodei, A. Peisker, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, H. Salazar, F. Salesa Greus, A. Sandoval, M. Schneider, H. Schoorlemmer, J. Serna-Franco, A. J. Smith, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, L. Villaseñor, X. Wang, I. J. Watson, E. Willox, A. Zepeda, H. Zhou, M. Breuhaus, H. Li, and H. Zhang

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, ddc:530, High Energy Physics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report TeV gamma-ray observations of the ultra-high-energy source MGRO J1908+06 using data from the High Altitude Water Cherenkov (HAWC) Observatory. This source is one of the highest-energy known gamma-ray sources, with emission extending past 200 TeV. Modeling suggests that the bulk of the TeV gamma-ray emission is leptonic in nature, driven by the energetic radio-faint pulsar PSR J1907+0602. Depending on what assumptions are included in the model, a hadronic component may also be allowed. Using the results of the modeling, we discuss implications for detection prospects by multi-messenger campaigns., Comment: accepted by ApJ, in press

Published
2022

3. Searching for TeV Dark Matter in Irregular dwarf galaxies with HAWC Observatory

Author

R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, R. Babu, E. Belmont-Moreno, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, O. Chaparro-Amaro, U. Cotti, J. Cotzomi, E. De la Fuente, R. Diaz Hernandez, B. L. Dingus, M. A. DuVernois, M. Durocher, J. C. Díaz-Vélez, C. Espinoza, K. L. Fan, N. Fraija, J. A. García-González, F. Garfias, M. M. González, J. P. Harding, S. Hernández-Cadena, D. Huang, F. Hueyotl-Zahuantitla, A. Iriarte, V. Joshi, S. Kaufmann, D. Kieda, J. Lee, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, J. Martínez-Castro, J. A. Matthews, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, N. Omodei, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, H. Salazar, D. Salazar-Gallegos, A. Sandoval, J. Serna-Franco, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, L. Villaseñor, X. Wang, E. Willox, H. Zhou, C. de León, V. Gammaldi, E. Karukes, and P. Salucci

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

We present the results of dark matter (DM) searches in a sample of 31 dwarf irregular (dIrr) galaxies within the field of view of the HAWC Observatory. dIrr galaxies are DM dominated objects, which astrophysical gamma-ray emission is estimated to be negligible with respect to the secondary gamma-ray flux expected by annihilation or decay of Weakly Interacting Massive Particles (WIMPs). While we do not see any statistically significant DM signal in dIrr galaxies, we present the exclusion limits ($95\%~\text{C.L.}$) for annihilation cross-section and decay lifetime for WIMP candidates with masses between $1$ and $100~\text{TeV}$. Exclusion limits from dIrr galaxies are relevant and complementary to benchmark dwarf Spheroidal (dSph) galaxies. In fact, dIrr galaxies are targets kinematically different from benchmark dSph, preserving the footprints of different evolution histories. We compare the limits from dIrr galaxies to those from ultrafaint and classical dSph galaxies previously observed with HAWC. We find that the contraints are comparable to the limits from classical dSph galaxies and $\thicksim2$ orders of magnitude weaker than the ultrafaint dSph limits., Comment: 22 pages, 11 figures, 3 tables

Published
2023
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4. The High-Altitude Water Cherenkov (HAWC) Observatory in México: The Primary Detector

Author

A.U. Abeysekara, A. Albert, R. Alfaro, C. Alvarez, J.D. Álvarez, M. Araya, J.C. Arteaga-Velázquez, K.P. Arunbabu, D. Avila Rojas, H.A. Ayala Solares, R. Babu, A.S. Barber, A. Becerril, E. Belmont-Moreno, S.Y. BenZvi, O. Blanco, J. Braun, C. Brisbois, K.S. Caballero-Mora, J.I. Cabrera Martínez, T. Capistrán, A. Carramiñana, S. Casanova, M. Castillo, O. Chaparro-Amaro, U. Cotti, J. Cotzomi, S. Coutiño de León, E. de la Fuente, C. de León, T. De Young, R. Diaz Hernandez, B.L. Dingus, M.A. DuVernois, M. Durocher, J.C. Díaz-Vélez, R.W. Ellsworth, K. Engel, C. Espinoza, K.L. Fan, K. Fang, B. Fick, H. Fleischhack, J.L. Flores, N. Fraija, J.A. García-González, G. Garcia-Torales, F. Garfias, G. Giacinti, H. Goksu, M.M. González, A. González-Muñoz, J.A. Goodman, J.P. Harding, E. Hernandez, S. Hernandez, J. Hinton, B. Hona, D. Huang, F. Hueyotl-Zahuantitla, C.M. Hui, T.B. Humensky, P. Hüntemeyer, A. Iriarte, A. Imran, A. Jardin-Blicq, V. Joshi, S. Kaufmann, D. Kieda, G.J. Kunde, A. Lara, R. Lauer, W.H. Lee, D. Lennarz, H. León Vargas, J.T. Linnemann, A.L. Longinotti, G. Luis-Raya, J. Lundeen, K. Malone, V. Marandon, A. Marinelli, O. Martinez, I. Martínez-Castellanos, J. Martínez-Castro, H. Martínez-Huerta, J.A. Matthews, P. Miranda-Romagnoli, T. Montaruli, J.A. Morales-Soto, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, M.U. Nisa, R. Noriega-Papaqui, T. Oceguera-Becerra, L. Olivera-Nieto, N. Omodei, A. Peisker, Y. Pérez Araujo, E.G. Pérez-Pérez, E. Ponce, J. Pretz, C.D. Rho, D. Rosa-González, E. Ruiz-Velasco, H. Salazar, D. Salazar-Gallegos, F. Salesa Greus, A. Sandoval, M. Schneider, H. Schoorlemmer, J. Serna-Franco, G. Sinnis, A.J. Smith, Y. Son, K. Sparks Woodle, R.W. Springer, I. Taboada, A. Tepe, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, T.N. Ukwatta, E. Varela, M. Vargas-Magaña, L. Villaseñor, X. Wang, I.J. Watson, F. Werner, S. Westerhoff, E. Willox, I. Wisher, J. Wood, G.B. Yodh, D. Zaborov, A. Zepeda, and H. Zhou

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Nuclear and High Energy Physics, FOS: Physical sciences, High Energy Physics, Molecular Developmental Biology, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract

The High-Altitude Water Cherenkov (HAWC) observatory is a second-generation continuously operated, wide field-of-view, TeV gamma-ray observatory. The HAWC observatory and its analysis techniques build on experience of the Milagro experiment in using ground-based water Cherenkov detectors for gamma-ray astronomy. HAWC is located on the Sierra Negra volcano in M\'exico at an elevation of 4100 meters above sea level. The completed HAWC observatory principal detector (HAWC) consists of 300 closely spaced water Cherenkov detectors, each equipped with four photomultiplier tubes to provide timing and charge information to reconstruct the extensive air shower energy and arrival direction. The HAWC observatory has been optimized to observe transient and steady emission from sources of gamma rays within an energy range from several hundred GeV to several hundred TeV. However, most of the air showers detected are initiated by cosmic rays, allowing studies of cosmic rays also to be performed. This paper describes the characteristics of the HAWC main array and its hardware., Comment: Accepted for publications in Nuclear Inst. and Methods in Physics Research, A (2023) 168253 ( https://www.sciencedirect.com/science/article/abs/pii/S0168900223002437 ); 39 pages, 14 Figures

Published
2023
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5. HAWC Detection of a TeV Halo Candidate Surrounding a Radio-quiet pulsar

Author

A. Albert, R. Alfaro, J. C. Arteaga-Velázquez, H. A. Ayala Solares, E. Belmont-Moreno, T. Capistrán, A. Carramiñana, S. Casanova, J. Cotzomi, S. Coutiño De León, E. De la Fuente, C. de León, R. Diaz Hernandez, M. A. DuVernois, J. C. Díaz-Vélez, C. Espinoza, K. L. Fan, N. Fraija, K. Fang, J. A. García-González, F. Garfias, A. Jardin-Blicq, M. M. González, J. A. Goodman, J. P. Harding, S. Hernandez, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, V. Joshi, A. Lara, J. Lee, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, J. Martínez-Castro, J. A. Matthews, J. A. Morales-Soto, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, M. U. Nisa, Y. Pérez Araujo, Y. Son, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, A. Sandoval, M. Schneider, J. Serna-Franco, A. J. Smith, R. W. Springer, K. Tollefson, I. Torres, R. Torres-Escobedo, X. Wang, K. Whitaker, E. Willox, H. Zhou, and HEP, INSPIRE

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), formation, water, halo, FOS: Physical sciences, Astronomy and Astrophysics, VHE, observatory, Space and Planetary Science, gamma ray, TeV, spectral, Cherenkov, galaxy, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], HAWC, pulsar
Abstract

Extended very-high-energy (VHE; 0.1–100 TeV) γ-ray emission has been observed around several middle-aged pulsars and referred to as “TeV halos.” Their formation mechanism remains under debate. It is also unknown whether they are ubiquitous or related to a certain subgroup of pulsars. With 2321 days of observation, the High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory detected VHE γ-ray emission at the location of the radio-quiet pulsar PSR J0359+5414 with >6σ significance. By performing likelihood tests with different spectral and spatial models and comparing the TeV spectrum with multiwavelength observations of nearby sources, we show that this excess is consistent with a TeV halo associated with PSR J0359+5414, though future observation of HAWC and multiwavelength follow-ups are needed to confirm this nature. This new halo candidate is located in a noncrowded region in the outer galaxy. It shares similar properties to the other halos but its pulsar is younger and radio-quiet. Our observation implies that TeV halos could commonly exist around pulsars and their formation does not depend on the configuration of the pulsar magnetosphere.

Published
2023

6. Search for Gamma-Ray and Neutrino Coincidences Using HAWC and ANTARES Data

Author

H. A. Ayala Solares, S. Coutu, D. Cowen, D. B. Fox, T. Grégoire, F. McBride, M. Mostafá, K. Murase, S. Wissel, A. Albert, S. Alves, M. André, M. Ardid, S. Ardid, J.-J. Aubert, J. Aublin, B. Baret, S. Basa, B. Belhorma, M. Bendahman, F. Benfenati, V. Bertin, S. Biagi, M. Bissinger, J. Boumaaza, M. Bouta, M. C. Bouwhuis, H. Brânzaş, R. Bruijn, J. Brunner, J. Busto, B. Caiffi, D. Calvo, A. Capone, L. Caramete, J. Carr, V. Carretero, S. Celli, M. Chabab, T. N. Chau, R. Cherkaoui El Moursli, T. Chiarusi, M. Circella, J. A. B. Coelho, A. Coleiro, R. Coniglione, P. Coyle, A. Creusot, A. F. Díaz, G. de Wasseige, B. De Martino, C. Distefano, I. Di Palma, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, T. van Eeden, D. van Eijk, N. El Khayati, A. Enzenhöfer, P. Fermani, G. Ferrara, F. Filippini, L. Fusco, J. García, P. Gay, H. Glotin, R. Gozzini, R. Gracia Ruiz, K. Graf, C. Guidi, S. Hallmann, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, J. Hößl, J. Hofestädt, F. Huang, G. Illuminati, C. W. James, B. Jisse-Jung, M. de Jong, P. de Jong, M. Kadler, O. Kalekin, U. Katz, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, M. Lamoureux, R. Le Breton, D. Lefèvre, E. Leonora, G. Levi, S. Le Stum, D. Lopez-Coto, S. Loucatos, L. Maderer, J. Manczak, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martínez-Mora, K. Melis, P. Migliozzi, A. Moussa, R. Muller, L. Nauta, S. Navas, E. Nezri, B. Ó Fearraigh, A. Păun, G. E. Păvălaş, C. Pellegrino, M. Perrin-Terrin, V. Pestel, P. Piattelli, C. Pieterse, C. Poirè, V. Popa, T. Pradier, N. Randazzo, D. Real, S. Reck, G. Riccobene, A. Romanov, A. Sánchez-Losa, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, J. Schnabel, J. Schumann, F. Schüssler, J. Seneca, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, S. J. Tingay, B. Vallage, V. Van Elewyck, F. Versari, S. Viola, D. Vivolo, J. Wilms, S. Zavatarelli, A. Zegarelli, J. D. Zornoza, J. Zúñiga, C. Alvarez, J. C. Arteaga-Velázquez, R. Babu, E. Belmont-Moreno, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, U. Cotti, O. Chaparro-Amaro, J. Cotzomi, S. Coutiño de León, E. De la Fuente, C. de León, R. Diaz Hernandez, M. A. DuVernois, M. Durocher, J. C. Díaz-Vélez, K. Engel, C. Espinoza, K. L. Fan, M. Fernández Alonso, N. Fraija, J. A. García-González, F. Garfias, M. M. González, J. A. Goodman, J. P. Harding, S. Hernandez, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, V. Joshi, S. Kaufmann, A. Lara, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, I. Martinez-Castellanos, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, J. A. Morales-Soto, E. Moreno, A. Nayerhoda, L. Nellen, M. U. Nisa, R. Noriega-Papaqui, N. Omodei, A. Peisker, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, E. Ruiz-Velasco, H. Salazar, F. Salesa Greus, A. Sandoval, M. Schneider, A. J. Smith, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, E. Varela, X. Wang, K. Whitaker, E. Willox, A. Zepeda, H. Zhou, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AMON Team, ANTARES, HAWC, Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Laboratoire d'Informatique et Systèmes (LIS), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut Universitaire de France (IUF), and Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.)

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Astrofísica, ANTARES, Telescopis, background, water, FOS: Physical sciences, Astronomy and Astrophysics, neutrino: particle source, Astrophysics, neutrino: UHE, IceCube, observatory, neutrino: detector, Space and Planetary Science, gamma ray, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], Cherenkov, Neutrins, Neutrinos, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], HAWC, Telescopes
Abstract

In the quest for high-energy neutrino sources, the Astrophysical Multimessenger Observatory Network has implemented a new search by combining data from the High Altitude Water Cherenkov (HAWC) Observatory and the Astronomy with a Neutrino Telescope and Abyss environmental RESearch (ANTARES) neutrino telescope. Using the same analysis strategy as in a previous detector combination of HAWC and IceCube data, we perform a search for coincidences in HAWC and ANTARES events that are below the threshold for sending public alerts in each individual detector. Data were collected between 2015 July and 2020 February with a live time of 4.39 yr. Over this time period, three coincident events with an estimated false-alarm rate of, The National Science Foundation under grants PHY-1708146, PHY-1806854, The Institute for Gravitation and the Cosmos of the Pennsylvania State University, Centre National de la Recherche Scientifique (CNRS), Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Région Île-de-France (DIM-ACAV), Région Alsace (contrat CPER), Région Provence-Alpes-Côte d’Azur, Département du Var and Ville de La Seyne-sur-Mer, Bundesministerium für Bildung und Forschung (BMBF), Istituto Nazionale di Fisica Nucleare (INFN), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania; Ministerio de Ciencia, Innovación, Investigación y Universidades (MCIU), Programa Estatal de Generación de Conocimiento (refs. PGC2018- 096663-B-C41, -A-C42, B-C43, B-C44, PID2021- 124591NB-C41, C42, C43, (MCIU/FEDER), Generalitat Valenciana, Prometeo (PROMETEO/2020/019), Grisolía (refs. GRISOLIA/2018/119, /2021/192), GenT (refs. /2019/043, /2020/049, /2021/023) programs, Junta de Andalucía (ref. A-FQM-053-UGR18), La Caixa Foundation (ref. LCF/BQ/IN17/11620019), MSC program (ref. 101025085), Spain; Ministry of Higher Education, Scientific Research and Innovation, The Arab Fund for Economic and Social Development, Kuwait, US National Science Foundation (NSF), The US Department of Energy Office of High-Energy Physics, Laboratory Directed Research and Development (LDRD) program of Los Alamos National Laboratory, Consejo Nacional de Ciencia y Tecnología (CONACyT), México, grants 271051, 232656, 260378, 179588, 254964, 258865, 243290, 132197, A1-S-46288, A1- S-22784, Cátedras 873, 1563, 341, 323, Red HAWC, México, DGAPA-UNAM grants IG101320, IN111716-3, IN111419, IA102019, IN110621, IN110521, VIEP-BUAP, PIFI 2012, PROFOCIE 2014, 2015, the University of Wisconsin Alumni Research Foundation, The Institute of Geophysics, Planetary Physics, Signatures at Los Alamos National Laboratory, Polish Science Centre grant, DEC-2017/27/B/ ST9/02272, Coordinación de la Investigación Científica de la Universidad Michoacana; Royal Society—Newton Advanced Fellowship 180385, Generalitat Valenciana, grant CIDEGENT/ 2018/034, The Program Management Unit for Human Resources & Institutional Development, Research and Innovation, NXPO (grant No. B16F630069), Coordinación General Académica e Innovación (CGAI-UdeG), PRODEP-SEP UDGCA- 499; Institute of Cosmic Ray Research (ICRR), University of Tokyo, NASA under award number 80GSFC21M0002

Published
2023

7. Teaching Spanish Spelling in Grades 2–3: A Cross-National Approach

Author

Juan E. Jiménez, Desirée González, Remedios Guzmán, and Sara C. de León

Subjects
Linguistics and Language, Mathematics education, Sample (statistics), Psychology, Spelling, Education, Cross national
Abstract

This study aimed to explore instructional practices used to teach words with irregular spelling patterns by Spanish-speaking teachers in 2nd and 3rd grade of elementary school. A sample of 320 teac...

Published
2021

8. Reading Curriculum-Based Measures for Universal Screening in Monolingual Spanish First Graders

Author

Sara C. de León, Juan E. Jiménez, and Nuria Gutiérrez

Subjects
Response to intervention, media_common.quotation_subject, 05 social sciences, 050301 education, Research findings, behavioral disciplines and activities, Education, Developmental psychology, Reading (process), Developmental and Educational Psychology, 0501 psychology and cognitive sciences, Psychology, 0503 education, Curriculum, 050104 developmental & child psychology, media_common
Abstract

Research findings: Universal screening is the first stage in identifying students at risk for reading difficulties within a Response to Intervention model. However, there is a lack of validated scr...

Published
2021

9. Study of the Very High Energy Emission of M87 through its Broadband Spectral Energy Distribution

Author

R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, E. Belmont-Moreno, T. Capistrán, A. Carramiñana, S. Casanova, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, C. de León, R. Diaz Hernandez, M. A. DuVernois, M. Durocher, J. C. Díaz-Vélez, C. Espinoza, K. L. Fan, M. Fernández Alonso, N. Fraija, J. A. García-González, F. Garfias, M. M. González, J. A. Goodman, J. P. Harding, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, V. Joshi, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, R. Noriega-Papaqui, N. Omodei, A. Peisker, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, H. Salazar, D. Salazar-Gallegos, F. Salesa Greus, A. Sandoval, J. Serna-Franco, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, F. Ureña-Mena, L. Villaseñor, X. Wang, E. Willox, and A. Zepeda

Subjects
Space and Planetary Science, Astronomy and Astrophysics, ddc:530
Abstract

The radio galaxy M87 is the central dominant galaxy of the Virgo Cluster. Very high-energy (VHE, ≳0.1 TeV) emission from M87 has been detected by imaging air Cherenkov telescopes. Recently, marginal evidence for VHE long-term emission has also been observed by the High Altitude Water Cherenkov Observatory, a gamma-ray and cosmic-ray detector array located in Puebla, Mexico. The mechanism that produces VHE emission in M87 remains unclear. This emission originates in its prominent jet, which has been spatially resolved from radio to X-rays. In this paper, we construct a spectral energy distribution from radio to gamma rays that is representative of the nonflaring activity of the source, and in order to explain the observed emission, we fit it with a lepto-hadronic emission model. We found that this model is able to explain nonflaring VHE emission of M87 as well as an orphan flare reported in 2005.

Published
2022

10. Identification of Spanish third graders at risk of math problems: Usefulness of number sense based screening measures

Author

Juan E. Jiménez, Eduardo García, Sara C. de León, and Nuria Gutiérrez

Subjects
Identification (information), Curriculum-based measurement, Receiver operating characteristic, education, Multilevel model, Statistics, Developmental and Educational Psychology, Sample (statistics), Number sense, At-risk students, Reliability (statistics), Education, Mathematics
Abstract

This study aimed to explore the utility of a math curriculum-based measurement (M-CBM) to identify Spanish-speaking students at risk of math failure in third grade. The M-CBM includes a set of number sense based single and composite screening for third graders. The study's sample included 236 Spanish third-graders from the Canary Islands tested in the fall, winter, and spring. Reliability and validity of all measures were explored, finding adequate indexes. Receiver operating characteristics (ROC) and Hierarchical linear modeling analyses were conducted for both single and composite measures. All the measures revealed an area under the ROC curve values at or above 0.84, the composite measures ranging from 0.86 to 0.94. When comparing the single and composite measures, the latter revealed a higher classification accuracy for identifying students at risk in third grade than quantity discrimination, missing number, and multi-digit computation measures, but not for single-digit computation and place value measures. Finally, significant differences were found between at-risk and non-risk students learning growth throughout the school year.

Published
2021

11. Analyzing the role of fidelity of RTI Tier 2 reading intervention in Spanish kindergarten and first grade students

Author

Juan E. Jiménez, Sara C. de León, and Nuria Gutiérrez

Subjects
Medical education, Academic year, Response to intervention, media_common.quotation_subject, education, 05 social sciences, Multilevel model, 050301 education, Fidelity, 050105 experimental psychology, Education, Speech and Hearing, Intervention (counseling), Tier 2 network, Reading (process), 0501 psychology and cognitive sciences, Psychology, 0503 education, At-risk students, media_common
Abstract

This study examined the role of fidelity in the reading outcomes within a Tier 2 intervention implemented by Spanish kindergarten and first grade school teachers. For this purpose, differences in reading performance growth were analyzed among at-risk students who received a Tier 2 intervention with high fidelity, at-risk students who received the same intervention with medium fidelity, and an at-risk control group that did not receive a Tier 2 intervention. Implementation fidelity was analyzed using direct observations and self-reports. All students were assessed three times during the academic year. Hierarchical linear modeling analyses were conducted to explore differences in growth rate. The at-risk children in the intervention condition showed a higher growth compared to at-risk children in the control condition, and specifically when the intervention was delivered with a high degree of fidelity.

Published
2021

12. Assessing the Efficacy of Tier 2 Mathematics Intervention for Spanish Primary School Students

Author

Nuria Gutiérrez, Sara C. de León, Juan E. Jiménez, and Juan Andrés Hernández-Cabrera

Subjects
Sociology and Political Science, Response to intervention, media_common.quotation_subject, education, 05 social sciences, Control (management), 050301 education, Fidelity, Context (language use), behavioral disciplines and activities, Education, Elementary mathematics, Intervention (counseling), Tier 2 network, mental disorders, ComputingMilieux_COMPUTERSANDEDUCATION, Developmental and Educational Psychology, Mathematics education, 0501 psychology and cognitive sciences, 0503 education, Curriculum, 050104 developmental & child psychology, media_common
Abstract

This study explored the efficacy of a Tier 2 intervention within the context of the Response to Intervention (RtI) model implemented by Spanish first- to third-grade primary school teachers to improve at-risk students’ early math skills. Teachers were instructed in the administration of a math curriculum-based measure composed of 5 isolated measures (quantity discrimination, missing number, single-digit computation, multidigit computation, and place value) to identify at-risk students and to monitor their progress; and in the implementation of a systematic and explicit instructional program to improve basic math skills in at-risk students. Implementation fidelity was analyzed using direct observations and self-reports. The intervention was conducted with adequate fidelity and had a significant positive impact on all grades. Significant differences were found between experimental and control students at risk of math failure in the improvement rate of quantity discrimination, missing number, and place value in all grades. Experimental at-risk students showed a monthly improvement, assessed using a combination of screening and progress monitoring measures. In conclusion, Spanish first to third graders at risk of math failure benefited from a Tier 2 intervention based on basic math skills, implemented by in-service teachers.

Published
2021

13. Structure of biomimetic apatite grown on hydroxyapatite (HA)

Author

D.A. Sánchez-Téllez, Marco Antonio Alvarez-Perez, Nancy Vargas-Becerril, L. Zarazúa-Villalobos, C. de León-Escobedo, D.M. González-García, and Lucía Téllez-Jurado

Subjects
010302 applied physics, Materials science, Scanning electron microscope, Process Chemistry and Technology, Simulated body fluid, 02 engineering and technology, engineering.material, 021001 nanoscience & nanotechnology, 01 natural sciences, Apatite, Nanocrystalline material, Surfaces, Coatings and Films, Electronic, Optical and Magnetic Materials, Crystallinity, Coating, Chemical engineering, Transmission electron microscopy, visual_art, 0103 physical sciences, Materials Chemistry, Ceramics and Composites, engineering, visual_art.visual_art_medium, Hydroxyapatites, 0210 nano-technology
Abstract

Nanocrystalline hydroxyapatite (HA) is the bone mineral phase in vertebrate animals. When bones suffer illness or injuries, natural hydroxyapatite reconstructs and remodels its structure. It has been demonstrated that synthetic hydroxyapatite materials emulate bone properties and enhance bone-bonding ability through a biomimetic apatite coating, obtained when bioactive materials are immersed in a physiological-like media. In this research, the biomimetic apatite structure deposited in three synthetic hydroxyapatites (HAs: HAMS, HAUB, and HAUT), after being immersed in a simulated body fluid (SBF), is studied. The synthetic HAs are obtained by co-precipitation, using three different stirring methods: magnetic stirring (HAMS), ultrasonic bath (HAUB), and ultrasonic tip (HAUT). The synthetic HAs are characterized by X-Ray Diffraction (X-RD), High-Resolution Scanning Electron Microscopy (HR-SEM), Energy Dispersive X-ray (EDX) microanalysis and Transmission Electron Microscopy (TEM) before and after SBF assays. The crystal sizes of synthetic HAs are 12.567 nm, 15.188 nm, and 17.903 nm for HAMS, HAUB, and HAUT, respectively. Additionally, HAs have values between 0.940 and 0.942 nm for a-cell parameter, and values between 0.688 and 0.689 nm for c-cell parameter. After 28 days of immersion in Simulated Body Fluid (SBF), the materials show poor crystalline-fine films of biomimetic apatite covering their surfaces. These biomimetic apatite films have values between 0.946 and 0.969 nm for the a-cell parameter and values between 0.698 and 0.710 nm for the c-cell parameter. Hence, crystallinity, crystal size, and morphology of synthetic HAs are dependent on the stirring method used during the synthesis process, which affects the structural characteristics of the biomimetic apatite layers deposited on the synthetic HAs surfaces.

Published
2020

14. Gamma/Hadron Separation with the HAWC Observatory

Author

R. Alfaro, C. Alvarez, J.D. Álvarez, J.R. Angeles Camacho, J.C. Arteaga-Velázquez, D. Avila Rojas, H.A. Ayala Solares, R. Babu, E. Belmont-Moreno, C. Brisbois, K.S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, O. Chaparro-Amaro, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, C. de León, R. Diaz Hernandez, B.L. Dingus, M.A. DuVernois, M. Durocher, J.C. Díaz-Vélez, R.W. Ellsworth, K. Engel, C. Espinoza, K.L. Fan, M. Fernández Alonso, N. Fraija, D. Garcia, J.A. García-González, F. Garfias, M.M. González, J.A. Goodman, J.P. Harding, S. Hernandez, B. Hona, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, A. Jardin-Blicq, V. Joshi, S. Kaufmann, G.J. Kunde, A. Lara, W.H. Lee, J. Lee, H. León Vargas, J.T. Linnemann, G. Luis-Raya, J. Lundeen, K. Malone, V. Marandon, O. Martinez, J. Martínez-Castro, J.A. Matthews, P. Miranda-Romagnoli, J.A. Morales-Soto, A. Nayerhoda, L. Nellen, M.U. Nisa, R. Noriega-Papaqui, L. Olivera-Nieto, N. Omodei, A. Peisker, Y. Pérez Araujo, E.G. Pérez-Pérez, C.D. Rho, D. Rosa-González, E. Ruiz-Velasco, H. Salazar, F. Salesa Greus, A. Sandoval, P.M. Saz Parkinson, J. Serna-Franco, A.J. Smith, R.W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, L. Villaseñor, X. Wang, I.J. Watson, F. Werner, E. Willox, J. Wood, A. Zepeda, and H. Zhou

Subjects
HAWC - Abteilung Hinton, High Energy Astrophysical Phenomena (astro-ph.HE), Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Instrumentation
Abstract

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory observes atmospheric showers produced by incident gamma rays and cosmic rays with energy from 300 GeV to more than 100 TeV. A crucial phase in analyzing gamma-ray sources using ground-based gamma-ray detectors like HAWC is to identify the showers produced by gamma rays or hadrons. The HAWC observatory records roughly 25,000 events per second, with hadrons representing the vast majority ($>99.9\%$) of these events. The standard gamma/hadron separation technique in HAWC uses a simple rectangular cut involving only two parameters. This work describes the implementation of more sophisticated gamma/hadron separation techniques, via machine learning methods (boosted decision trees and neural networks), and summarizes the resulting improvements in gamma/hadron separation obtained in HAWC., 35 pages, 9 figures, published in Nuclear Instruments and Methods in Physics Research Section A

Published
2022

15. Effects of <scp>web‐based</scp> training on Spanish <scp>pre‐service</scp> and <scp>in‐service</scp> teacher knowledge and implicit beliefs on learning to write

Author

Eduardo García, Juan E. Jiménez, Sara C. de León, and Rocío C. Seoane

Subjects
Service (business), Medical education, business.industry, Knowledge level, Professional development, Training (civil), Spelling, Computer Science Applications, Education, Pre service, Handwriting, Web application, business, Psychology
Published
2020

16. Universal Screening for Writing Risk in Spanish-Speaking First Graders

Author

Juan E. Jiménez, Sara C. de León, and Verónica Gil

Subjects
Predictive validity, Linguistics and Language, education, 05 social sciences, 050301 education, Early detection, Spanish speaking, Spelling, Education, Nonverbal communication, Curriculum-based measurement, Handwriting, Mathematics education, 0501 psychology and cognitive sciences, Psychology, 0503 education, At-risk students, 050104 developmental & child psychology
Abstract

The main objective of this study was to analyze what writing measures, or combination of measures, would be most appropriate for early detection of students at risk of presenting future difficultie...

Published
2020

17. Universal Screening in Mathematics for Spanish Students in First Grade

Author

Juan E. Jiménez, Sara C. de León, Nuria Gutiérrez, Verónica Gil, and Eduardo García

Subjects
Predictive validity, Measure (data warehouse), Receiver operating characteristic, 05 social sciences, Multilevel model, 050109 social psychology, Context (language use), Education, Behavioral Neuroscience, General Health Professions, Learning disability, medicine, Mathematics education, 0501 psychology and cognitive sciences, medicine.symptom, Psychology, Curriculum, Reliability (statistics), 050104 developmental & child psychology
Abstract

The main purpose of this study was to validate the curriculum-based measure Indicadores de Progreso de Aprendizaje en Matemáticas (IPAM [Indicators of Basic Early Math Skills]) in a local, Spanish-speaking context. This tool has been designed to identify first-grade students at risk for mathematics learning disabilities. The IPAM includes five measures (i.e., quantity discrimination, multi-digit computation, missing number, single-digit computation, and place value), which were analyzed as single measures and as part of a composite measure. In this study, 176 first graders were administered the curriculum-based measurement IPAM at the beginning, middle, and end of the school year. The results showed that the composite measure of the IPAM was the best indicator of risk status. Reliability and concurrent and predictive validity results were adequate. Furthermore, receiver operating curve analysis and hierarchical linear model supported the capacity of the IPAM to correctly identify students’ risk status and growth rate during first grade.

Published
2020

18. Confirmatory factor analysis of the indicators of basic early math skills

Author

Sara C. de León, Juan E. Jiménez, and Juan Andrés Hernández-Cabrera

Subjects
Predictive validity, Factorial, 05 social sciences, Concurrent validity, 050109 social psychology, Number sense, 050105 experimental psychology, Confirmatory factor analysis, Discriminant, Goodness of fit, Statistics, 0501 psychology and cognitive sciences, Measurement invariance, Psychology, General Psychology
Abstract

A study was conducted to analyze the factorial structure and measurement invariance of the Curriculum-Based Measurement (CBM) Indicadores de Progreso de Aprendizaje en Matematicas (IPAM [Indicators of Basic Early Math Skills]), in 2nd grade Spanish students. The model proposed is a one-factor model in which the five IPAM tasks (i.e., number comparison, missing number, single-digit computation, multi-digit computation, and place value) serve as observable indicators for a single underlying factor (i.e., number sense). The IPAM, composed of three parallel forms (i.e., A, B, and C), was administered to 252 Spanish second graders, three times throughout the school year (i.e., fall, winter, and spring). Consequently, the goodness of fit of the proposed model was analyzed for each measurement time. Furthermore, longitudinal measurement invariance was explored to analyze whether the measurement model would remain stable throughout the three-time points of measurement. Discriminant, predictive, and concurrent validity were also tested. The results support that the number sense latent factor explains the common variance of the observable indicators throughout the school year. Each latent factor was found highly related to the next. Moreover, the IPAM showed adequate indices for discriminant, concurrent and predictive validity. We conclude that the IPAM is an appropriate measure to assess number sense competence in second grade.

Published
2020

19. $γ$-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC

Author

Albert, A., Alfaro, R., Alvarez, C., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Babu, R., Belmont-Moreno, E., Blochwitz, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Chaparro-Amaro, O., Cotti, U., Cotzomi, J., de León, E. De la Fuente. C. de León. S. Coutiño, Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Durocher, M., Díaz-Vélez, J. C., Engel, K., Espinoza, C., Fan, K. L., Fang, K., Fraija, N., García-González, J. A., Garfias, F., González, M. M., Goodman, J. A., Harding, J. P., Hernandez, S., Hinton, J., Huang, D., Hueyotl-Zahuantitla, F., Hüntemeyer, P., Iriarte, A., Joshi, V., Lara, A., Lee, W. H., Linnemann, J. T., Longinotti, A. L., Luis-Raya, G., Lundeen, J., Malone, K., Marandon, V., Martinez, O., Martínez-Castro, J., Matthews, J. A., Miranda-Romagnoli, P., Morales-Soto, J. A., Moreno, E., Mostafá, M., Nayerhoda, A., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Omodei, N., Peisker, A., Araujo, Y. Pérez, Pérez-Pérez, E. G., Rho, C. D., Rosa-González, D., Ruiz-Velasco, E., Salazar-Gallegos, D., Greus, F. Salesa, Serna-Franco, A. Sandoval. J., Smith, A. J., Son, Y., Springer, R. W., Tibolla, O., Tollefson, K., Torres, I., Torres-Escobedo, R., Turner, R., Ureña-Mena, F., Villaseñor, L., Wang, X., Willox, E., Zhou, A. Zepeda. H., Chomiuk, L., Aydi, E., Li, K. L., Metzger, B. D., and Vurm, I.

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, High Energy Physics::Experiment
Abstract

This paper reports on the $γ$-ray properties of the 2018 Galactic nova V392 Per, spanning photon energies $\sim$0.1 GeV to 100 TeV by combining observations from the Fermi Gamma-ray Space Telescope and the HAWC Observatory. In one of the most rapidly evolving $γ$-ray signals yet observed for a nova, GeV $γ$ rays with a power law spectrum with index $Γ= 2.0 \pm 0.1$ were detected over eight days following V392 Per's optical maximum. HAWC observations constrain the TeV $γ$-ray signal during this time and also before and after. We observe no statistically significant evidence of TeV $γ$-ray emission from V392 Per, but present flux limits. Tests of the extension of the Fermi/LAT spectrum to energies above 5 TeV are disfavored by 2 standard deviations (95\%) or more. We fit V392 Per's GeV $γ$ rays with hadronic acceleration models, incorporating optical observations, and compare the calculations with HAWC limits., 18 pages, 14 figures; revised for referee comments; section 5 revised

Published
2022
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20. Probing the extragalactic mid-infrared background with HAWC

Author

A. Albert, R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, R. Babu, E. Belmont-Moreno, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, O. Chaparro-Amaro, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, R. Diaz Hernandez, M. A. DuVernois, M. Durocher, J. C. Díaz-Vélez, K. Engel, C. Espinoza, K. L. Fan, M. Fernández Alonso, N. Fraija, J. A. García-González, F. Garfias, M. M. González, J. A. Goodman, J. P. Harding, S. Hernandez, D. Huang, F. Hueyotl-Zahuantitla, P. Hntemeyer, A. Iriarte, A. Jardin-Blicq, V. Joshi, D. Kieda, W. H. Lee, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, M. U. Nisa, R. Noriega-Papaqui, N. Omodei, A. Peisker, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, H. Salazar, D. Salazar-Gallegos, F. Salesa Greus, A. Sandoval, J. Serna-Franco, A. J. Smith, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, L. Villaseñor, X. Wang, T. Weisgarber, E. Willox, H. Zhou, and C. de León

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, ddc:520, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics
Abstract

The extragalactic background light (EBL) contains all the radiation emitted by nuclear and accretion processes in stars and compact objects since the epoch of recombination. Measuring the EBL density directly is challenging, especially in the near- to far-infrared waveband, mainly due to the zodiacal light foreground. Instead, gamma-ray astronomy offers the possibility to indirectly set limits on the EBL by studying the effects of gamma-ray absorption in the very high energy (VHE:$>$100 GeV) spectra of distant blazars. The High Altitude Water Cherenkov gamma ray observatory (HAWC) is one of the few instruments sensitive to gamma rays with energies above 10 TeV. This offers the opportunity to probe the EBL in the near/mid IR region: $\lambda$ = 1 $\mu$m - 100 $\mu$m. In this study, we fit physically motivated emission models to Fermi Large Area Telescope (LAT) GeV data to extrapolate the intrinsic TeV spectra of blazars. We then simulate a large number of absorbed spectra for different randomly generated EBL model shapes and calculate Bayesian credible bands in the EBL intensity space by comparing and testing the agreement between the absorbed spectra and HAWC extragalactic observations of two blazars. The resulting bands are in agreement with current EBL lower and upper limits, showing a downward trend towards higher wavelength values $\lambda>10\, \mu$m also observed in previous measurements., Comment: Submitted to ApJ

Published
2022
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21. Detailed Analysis of the TeV γ-Ray Sources 3HWC J1928+178, 3HWC J1930+188, and the New Source HAWC J1932+192

Author

A. Albert, R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, R. Babu, E. Belmont-Moreno, C. Brisbois, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, O. Chaparro-Amaro, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, C. de León, R. Diaz Hernandez, J. C. Díaz-Vélez, B. L. Dingus, M. A. DuVernois, M. Durocher, K. Engel, C. Espinoza, K. L. Fan, M. Fernández Alonso, N. Fraija, J. A. García-González, F. Garfias, H. Goksu, M. M. González, J. A. Goodman, J. P. Harding, S. Hernandez, J. Hinton, B. Hona, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, A. Jardin-Blicq, V. Joshi, S. Kaufmann, D. Kieda, W. H. Lee, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, R. López-Coto, K. Malone, V. Marandon, O. Martinez, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, J. A. Morales-Soto, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, M. U. Nisa, R. Noriega-Papaqui, L. Olivera-Nieto, N. Omodei, A. Peisker, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, E. Ruiz-Velasco, H. Salazar, D. Salazar-Gallegos, F. Salesa Greus, A. Sandoval, M. Schneider, J. Serna-Franco, A. J. Smith, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, L. Villaseñor, X. Wang, F. Werner, E. Willox, and H. Zhou

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

The latest High Altitude Water Cherenkov (HAWC) point-like source catalog up to 56 TeV reported the detection of two sources in the region of the Galactic plane at galactic longitude 52° < ℓ < 55°, 3HWC J1930+188 and 3HWC J1928+178. The first one is associated with a known TeV source, the supernova remnant SNR G054.1+00.3. It was discovered by one of the currently operating Imaging Atmospheric Cherenkov Telescope (IACT), the Very Energetic Radiation Imaging Telescope Array System (VERITAS), detected by the High Energy Stereoscopic System (H.E.S.S), and identified as a composite SNR. However, the source 3HWC J1928+178, discovered by HAWC and coincident with the pulsar PSR J1928+1746, was not detected by any IACT despite their long exposure on the region, until a recent new analysis of H.E.S.S. data was able to confirm it. Moreover, no X-ray counterpart has been detected from this pulsar. We present a multicomponent fit of this region using the latest HAWC data. This reveals an additional new source, HAWC J1932+192, which is potentially associated with the pulsar PSR J1932+1916, whose γ-ray emission could come from the acceleration of particles in its pulsar wind nebula. In the case of 3HWC J1928+178, several possible explanations are explored, in an attempt to unveil the origins of the very-high-energy γ-ray emission.

Published
2023

23. Multimedia Battery for Assessment of Cognitive and Basic Skills in Mathematics (BM-PROMA)

Author

Isaac Marco, Cristina Rodríguez, Juan E. Jiménez, and Sara C. de León

Subjects
Protocol (science), Structure (mathematical logic), General Immunology and Microbiology, Multimedia, Learning Disabilities, Process (engineering), General Chemical Engineering, General Neuroscience, education, Primary education, Cognition, computer.software_genre, medicine.disease, General Biochemistry, Genetics and Molecular Biology, Basic skills, Dyscalculia, medicine, Humans, Learning, Child, computer, Mathematics, Grade level
Abstract

Learning mathematics is a complex process that requires the development of multiple domain-general and domain-specific skills. It is therefore not unexpected that many children struggle to stay at grade level, and this becomes especially difficult when several abilities from both domains are impaired, as in the case of mathematical learning disabilities (MLD). Surprisingly, although MLD is one of the most common neurodevelopmental disorders affecting schoolchildren, most of the diagnostic instruments available do not include assessment of domain-general and domain-specific skills. Furthermore, very few are computerized. To the best of our knowledge, there is no tool with these features for Spanish-speaking children. The purpose of this study was to describe the protocol for the diagnosis of Spanish MLD children using the BM-PROMA multimedia battery. BM-PROMA facilitates the evaluation of both skill domains, and the 12 tasks included for this purpose are empirically evidence-based. The strong internal consistency of BM-PROMA and its multidimensional internal structure are demonstrated. BM-PROMA proves to be an appropriate tool for diagnosing children with MLD during primary education. It provides a broad cognitive profile for the child, which will be relevant not only for diagnosis but also for individualized instructional planning.

Published
2021

24. TeV Emission of Galactic Plane Sources with HAWC and H.E.S.S

Author

Nicola Omodei, Sebastian Panny, A. Sandoval, Q. Piel, S. Raab, Arturo Iriarte, Kirsty Feijen, R. D. Parsons, Michael Newbold, J. Zorn, Michael Schneider, Fernando Garfias, D. Huber, Christo Venter, Jacek Niemiec, Arnaud Mares, Frank M. Rieger, Thomas Weisgarber, A. Dmytriiev, Olaf Reimer, A. Zech, E. Ruiz-Velasco, Thomas Bylund, Y. A. Gallant, David Sánchez, R. López-Coto, Jorge Cotzomi, Jacques Muller, H. León Vargas, Alison Peisker, Justine Devin, Thomas Murach, P. Morris, Harm Schoorlemmer, Jonathan Mackey, Andrea Albert, Samuel Zouari, Pascal Vincent, M. Zacharias, Stefan Ohm, S. Pita, Tadayuki Takahashi, Gilgamesh Luis-Raya, A. Yusafzai, Andreas Quirrenbach, Samuel Timothy Spencer, Stefano Gabici, Regis Terrier, Victor Doroshenko, L. Nellen, Włodek Kluźniak, R. Noriega-Papaqui, E. Kasai, C. Moore, L. Oakes, J. Bolmont, Michal Ostrowski, J.-P. Lenain, Pooja Surajbali, William H. Lee, L. Olivera-Nieto, E. Moulin, Tomasz Bulik, Rhiannon Turner, Lente Dreyer, O. Martinez, Stefan Klepser, Alessandro Montanari, D. J. van der Walt, Fernando Ureña-Mena, J. P. Harding, César Alvarez, Michael DuVernois, A.M. Taylor, J. C. Arteaga-Velézquez, Connor Duffy, Davit Zargaryan, R. J. White, Stefan Funk, Alicja Wierzcholska, Dmitriy Kostunin, J. Damascene Mbarubucyeye, R. Rauth, Maria Magdalena González, Kristi Engel, A. Galván-Gámez, Christoph Deil, Krzysztof Katarzynski, F. Eichhorn, Mohanraj Senniappan, E. Moreno, Michael Punch, Axel Donath, B. Hona, A. W. Chen, S. Steinmassl, Sami Caroff, Domenico Tiziani, D. Malyshev, Catherine Boisson, M. Panter, Mora Durocher, U. Katz, Pedro Miranda-Romagnoli, C. Arcaro, H. Zhou, Michael Backes, S. Coutiño de León, Ernesto Belmont-Moreno, M. de Bony de Lavergne, R. Brose, Petra Hüntemeyer, C. Levy, Francois Brun, R. J. Tuffs, B. Bi, Andreas Specovius, Joachim Hahn, K. P. Arunbabu, Riaan Steenkamp, Gavin Rowell, P. Reichherzer, James E. M. Watson, M. Bryan, E. de Oña Wilhelmi, Łukasz Stawarz, C. van Rensburg, Pierre Brun, Brenda Dingus, V. Marandon, J. A. Morales-Soto, M. Büchele, H. Prokoph, C. De León, A. Marcowith, V. Baghmanyan, J. Schäfer, Nu. Komin, Tim Holch, Q. Remy, H. M. Schutte, Isak Delberth Davids, A. Fiasson, Jean-Pierre Ernenwein, Hassan Abdalla, S. Hernandez, Jim Hinton, V. Sahakian, E. De la Fuente, F. Werner, Mischa Breuhaus, Luis Villaseñor, Yu Wun Wong, Hambeleleni Ndiyavala, D. Avila Rojas, G. Lamanna, K. S. Caballero-Mora, Roberta Zanin, G. Emery, Halim Ashkar, Fabian Leuschner, Heiko Salzmann, A. S. Seyffert, Kwok Lung Fan, M. Hörbe, T. Tavernier, Nissim Illich Fraija, P. T. O'Brien, Johannes Veh, S. Sailer, Dmitry Khangulyan, Gilles Maurin, S. J. Fegan, A. Djannati-Ataï, D. Jankowsky, J. Dyks, Celine Armand, M. Füßling, R. Marx, Dieter Horns, M. Tluczykont, F. Ait Benkhali, J. F. Glicenstein, M. U. Nisa, Marek Jamrozy, Clemens Hoischen, A. A. Zdziarski, A. Jardin-Blicq, E. O. Angüner, R. Diaz Hernandez, N. Shafi, Natalia Żywucka, M. de Naurois, Andrea Santangelo, K. Malone, Gwenael Giacinti, L. Sun, M.-H. Grondin, D. Garcia, M. Seglar-Arroyo, B. Khélifi, A. J. Smith, T. Capistrán, B. van Soelen, G. Hermann, Anna Barnacka, D. Gottschall, Anne Lemiere, B. Rudak, Markus Böttcher, K. Tollefson, Jhilik Majumdar, Helene Sol, T. Chand, C. Brisbois, Andreas Zmija, Tom Armstrong, Elijah Willox, Carlo Romoli, Alison Mitchell, R. Torres-Escobedo, Atreyee Sinha, Manuel Meyer, I. Martinez-Castellanos, Zorawar Wadiasingh, A. Priyana Noel, V. Barbosa Martins, C. van Eldik, M. Lemoine-Goumard, M. Tsirou, Michael Kreter, Anna Lia Longinotti, F. Schüssler, Dezhi Huang, Jose Andres Garcia-Gonzalez, Werner Hofmann, Monica Barnard, Juan Carlos Diaz-Velez, V. Poireau, Jimmy N.S. Shapopi, K. Nakashima, José Serna-Franco, G. Peron, Garret Cotter, Jacco Vink, A. Carraminana, Umberto Cotti, Jim Davies, M. A. Kastendieck, Thomas Lohse, K. Kosack, Paolo Marchegiani, Konrad Bernlöhr, Heinrich J. Völk, Sabrina Casanova, Catalina Espinoza, M. Renaud, D. Berge, G. Vasileiadis, F. Salesa Greus, I. Jung-Richardt, Kleopas Shiningayamwe, Gilles Fontaine, J. T. Linnemann, Lenka Tomankova, M. Mostafá, G. Fichet de Clairfontaine, R. Konno, Gianluca Giavitto, V. Joshi, B. Peyaud, G. Pühlhofer, J. A. Goodman, H. Odaka, A. Reimer, R. W. Ellsworth, R. W. Springer, M. Curyło, F. Hueyotl-Zahuantitla, E. G. Pérez-Pérez, Y. Pérez Araujo, A. Nayerhoda, Christian Stegmann, Stefan Wagner, Yasunobu Uchiyama, David Kieda, L. Mohrmann, Misao Sasaki, Markus Holler, Felix Jankowsky, Felix Aharonian, D. Glawion, Jesús Martínez-Castro, Segev BenZvi, Constantin Steppa, L. Giunti, D. A. Prokhorov, Ullrich Schwanke, L. Rinchiuso, J. A. Matthews, Ibrahim Torres, Rachel Simoni, A. Carosi, K. Egberts, S. Chandra, Ruben Alfaro, Sabrina Einecke, Iryna Lypova, Daniel Rosa-Gonzalez, Yvonne Becherini, M. Fernández Alonso, L. Dirson, G. Martí-Devesa, C. Trichard, Sylvia Zhu, P. J. Meintjes, J. H. E. Thiersen, Marion Spir-Jacob, Maria Haupt, C. D. Rho, Rafal Moderski, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Gravitation and Astroparticle Physics Amsterdam, High Energy Astrophys. & Astropart. Phys (API, FNWI), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Collaboration, H.E.S.S., and Collaboration, HAWC

Subjects
High-energy astronomy, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, IACT, Field of view, 030226 pharmacology & pharmacy, 01 natural sciences, 03 medical and health sciences, 0302 clinical medicine, Observatory, 0103 physical sciences, High Energy Stereoscopic System, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, media_common, Physics, [PHYS]Physics [physics], Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, Galactic plane, Space and Planetary Science, Sky, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], High energy astrophysics
Abstract

International audience; The High Altitude Water Cherenkov (HAWC) observatory and the High Energy Stereoscopic System (H.E.S.S.) are two leading instruments in the ground-based very-high-energy γ-ray domain. HAWC employs the water Cherenkov detection (WCD) technique, while H.E.S.S. is an array of Imaging Atmospheric Cherenkov Telescopes (IACTs). The two facilities therefore differ in multiple aspects, including their observation strategy, the size of their field of view, and their angular resolution, leading to different analysis approaches. Until now, it has been unclear if the results of observations by both types of instruments are consistent: several of the recently discovered HAWC sources have been followed up by IACTs, resulting in a confirmed detection only in a minority of cases. With this paper, we go further and try to resolve the tensions between previous results by performing a new analysis of the H.E.S.S. Galactic plane survey data, applying an analysis technique comparable between H.E.S.S. and HAWC. Events above 1 TeV are selected for both data sets, the point-spread function of H.E.S.S. is broadened to approach that of HAWC, and a similar background estimation method is used. This is the first detailed comparison of the Galactic plane observed by both instruments. H.E.S.S. can confirm the γ-ray emission of four HAWC sources among seven previously undetected by IACTs, while the three others have measured fluxes below the sensitivity of the H.E.S.S. data set. Remaining differences in the overall γ-ray flux can be explained by the systematic uncertainties. Therefore, we confirm a consistent view of the γ-ray sky between WCD and IACT techniques.

Published
2021

25. HAWC as a Ground-Based Space-Weather Observatory

Author

A. Zepeda, K. P. Arunbabu, S. Hernandez, J. A. Goodman, Ernesto Belmont-Moreno, R. W. Springer, O. Tibolla, E. Moreno, Juan Carlos Diaz-Velez, J. R. Angeles Camacho, Jose Andres Garcia-Gonzalez, Gerd Joachim Kunde, L. Nellen, D. Garcia, E. G. Pérez-Pérez, V. Baghmanyan, K. Malone, C. Alvarez, Karen S. Caballero-Mora, J. A. Morales-Soto, E. Tabachnick, Dezhi Huang, Catalina Espinoza, E. De la Fuente, D. Avila Rojas, Gilgamesh Luis-Raya, Jesús Martínez-Castro, Luis Villaseñor, Segev BenZvi, Pedro Miranda-Romagnoli, Alison Peisker, John Matthews, A. Sandoval, James M. Ryan, J. C. Arteaga-Velázquez, Umberto Cotti, Binita Hona, Michael Newbold, C. De León, P. Colin-Farias, Ibrahim Torres, Jorge Cotzomi, Nissim Illich Fraija, A. Galván-Gámez, R. Torres-Escobedo, Brenda Dingus, Daniel Rosa-Gonzalez, Fernando Garfias, Tomás Capistrán, H. León Vargas, M. J. F. Rosenberg, Y. Pérez Araujo, Maria Magdalena González, J. P. Harding, A. Nayerhoda, Chang Dong Rho, Hongyan Zhou, Filiberto Hueyotl-Zahuantitla, Simone Dichiara, Arturo Iriarte, Chad Brisbois, Michael DuVernois, Anna Lia Longinotti, Humberto Ibarguen Salazar, V. Joshi, K. Tollefson, R. Noriega-Papaqui, S. Coutiño de León, Alejandro Lara, and O. Martinez

Subjects
Physics, Photomultiplier, 010504 meteorology & atmospheric sciences, Physics::Instrumentation and Detectors, Detector, Gamma ray, Astronomy and Astrophysics, Cosmic ray, Space weather, 01 natural sciences, Space and Planetary Science, Observatory, 0103 physical sciences, 010303 astronomy & astrophysics, Energy (signal processing), Cherenkov radiation, 0105 earth and related environmental sciences, Remote sensing
Abstract

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is located close to the equator (latitude $18^{\circ }$ N), at an altitude of 4100 m above sea level. HAWC has 295 water Cherenkov detectors (WCD), each containing four photomultiplier tubes (PMT). The main purpose of HAWC is the determination of the energy and arrival direction of very high energy gamma rays produced by energetic processes in the universe, HAWC also has a scaler system which counts the arrival of secondary particles to the detector. In this work we show that the scaler system of HAWC is an ideal instrument for solar modulation and space-weather studies due to its large area and high sensitivity. In order to prepare the scaler system for low energy heliospheric studies, we model and correct the efficiency variation of each PMT of the array, which result in a capability to measure variations $> 0.01\%$ with high accuracy. Using the singular value decomposition method, we correct the rate deviations of all PMTs of the array, due to changes in efficiency, gain and operational voltage. We isolate and remove the atmospheric modulations of the PMTs count rates measured by the TDC-scaler data acquisition system. In particular, the atmospheric pressure at the HAWC site exhibits an oscillating behavior with a period of ∼12 hours and we make use of this periodic property to estimate the pressure coefficients for the HAWC TDC-scaler system. These corrections performed on the TDC-scaler system make the HAWC TDC-scaler system an ideal instrument for solar modulation and space-weather studies. As examples of this capability, we present the preliminary analysis of the solar modulation of cosmic rays at three time scales observed by HAWC, with an unprecedented accuracy.

Published
2021

26. HAWC Search for High-Mass Microquasars

Author

Ernesto Belmont-Moreno, Elijah Willox, J. A. Goodman, Dezhi Huang, Jorge Cotzomi, Mora Durocher, Petra Hüntemeyer, J. P. Harding, R. W. Springer, A. Carraminana, K. Malone, A. J. Smith, J. C. Arteaga-Velázquez, H. Zhou, Joe Lundeen, C. D. Rho, F. Salesa Greus, R. W. Ellsworth, C. De León, K. P. Arunbabu, A. L. Longinotti, David Kieda, B. Hona, Alison Peisker, L. Nellen, E. Moreno, Fernando Ureña-Mena, Umberto Cotti, R. Torres-Escobedo, C. Brisbois, Sabrina Casanova, R. Diaz Hernandez, Maria Magdalena González, S. Hernandez, Nissim Illich Fraija, Karen S. Caballero-Mora, Michael Newbold, Rhiannon Turner, Fernando Garfias, Michael DuVernois, Thomas Weisgarber, Catalina Espinoza, A. Sandoval, Jose Andres Garcia-Gonzalez, Filiberto Hueyotl-Zahuantitla, Jesús Martínez-Castro, Michael Schneider, H. A. Ayala Solares, Ke Fang, Y. J. Roh, Andrea Albert, T. Capistrán, O. Martinez, Ian James Watson, Miguel Mostafa, Gilgamesh Luis-Raya, V. Baghmanyan, V. Joshi, José Serna-Franco, Alejandro Lara, J. T. Linnemann, R. Noriega-Papaqui, William H. Lee, L. Olivera-Nieto, J. S. H. Lee, A. Galván-Gámez, Brenda Dingus, K. Tollefson, Ruben Alfaro, Pedro Miranda-Romagnoli, Daniel Rosa-Gonzalez, John Matthews, J. A. Morales-Soto, Luis Villaseñor, Kwok Lung Fan, H. León Vargas, A. Jardin-Blicq, Ibrahim Torres, M. U. Nisa, Juan Carlos Diaz-Velez, C. Alvarez, Nicola Omodei, Arturo Iriarte, Y. Pérez Araujo, A. Nayerhoda, Segev BenZvi, E. De la Fuente, D. Avila Rojas, and J. R. Angeles Camacho

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, High mass, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

Microquasars with high-mass companion stars are promising very-high-energy (VHE; 0.1-100 TeV) gamma-ray emitters, but their behaviors above 10 TeV are poorly known. Using the High Altitude Water Cherenkov (HAWC) observatory, we search for excess gamma-ray emission coincident with the positions of known high-mass microquasars (HMMQs). No significant emission is observed for LS 5039, Cygnus X-1, Cygnus X-3, and SS 433 with 1,523 days of HAWC data. We set the most stringent limit above 10 TeV obtained to date on each individual source. Under the assumption that HMMQs produce gamma rays via a common mechanism, we have performed source-stacking searches, considering two different scenarios: I) gamma-ray luminosity is a fraction $\epsilon_\gamma$ of the microquasar jet luminosity, and II) very-high-energy gamma rays are produced by relativistic electrons up-scattering the radiation field of the companion star in a magnetic field $B$. We obtain $\epsilon_\gamma < 5.4\times 10^{-6}$ for scenario I, which tightly constrains models that suggest observable high-energy neutrino emission by HMMQs. In the case of scenario II, the non-detection of VHE gamma rays yields a strong magnetic field, which challenges synchrotron radiation as the dominant mechanism of the microquasar emission between 10 keV and 10 MeV., Comment: Accepted for publication in ApJL

Published
2021

27. Evidence that Ultra-High-Energy Gamma Rays are a Universal Feature Near Powerful Pulsars

Author

R. Diaz Hernandez, Pedro Miranda-Romagnoli, J. A. Goodman, J. R. Angeles Camacho, Michael Newbold, Karen S. Caballero-Mora, Catalina Espinoza, John Matthews, Fernando Garfias, Jesús Martínez-Castro, H. A. Ayala Solares, Andrea Albert, Segev BenZvi, C. D. Rho, Thomas Weisgarber, Nicola Omodei, Dezhi Huang, Nissim Illich Fraija, E. Ruiz-Velasco, R. Torres-Escobedo, Ibrahim Torres, Arturo Iriarte, H. León Vargas, A. Carraminana, Joe Lundeen, R. W. Ellsworth, Meghan Tanner, C. De León, A. Sandoval, O. Martinez, K. Malone, J. C. Arteaga-Velázquez, Ernesto Belmont-Moreno, R. W. Springer, Michael Schneider, Alison Peisker, H. Zhou, E. G. Pérez-Pérez, K. P. Arunbabu, A. L. Longinotti, Kristi Engel, Harm Schoorlemmer, B. Hona, A. Jardin-Blicq, Elijah Willox, J. D. Álvarez, J. A. Morales-Soto, T. Capistrán, A. J. Smith, David Kieda, Humberto Ibarguen Salazar, Y. Pérez Araujo, J. P. Harding, Gwenael Giacinti, Gilgamesh Luis-Raya, L. Nellen, A. Nayerhoda, R. Noriega-Papaqui, Juan Carlos Diaz-Velez, S. Hernandez, Ruben Alfaro, William H. Lee, L. Olivera-Nieto, M. Fernández Alonso, C. Alvarez, Y. J. Roh, Miguel Mostafa, Daniel Rosa-Gonzalez, José Serna-Franco, Luis Villaseñor, Umberto Cotti, E. De la Fuente, Sabrina Casanova, D. Avila Rojas, V. Joshi, F. Salesa Greus, S. Coutiño de León, M. U. Nisa, Jorge Cotzomi, Alejandro Lara, J. T. Linnemann, Rhiannon Turner, Maria Magdalena González, Michael DuVernois, Kwok Lung Fan, Filiberto Hueyotl-Zahuantitla, J. S. H. Lee, E. Moreno, A. Galván-Gámez, Brenda Dingus, V. Marandon, K. Tollefson, C. Brisbois, V. Baghmanyan, Mora Durocher, Petra Hüntemeyer, Pooja Surajbali, Fernando Ureña-Mena, and Jose Andres Garcia-Gonzalez

Subjects
Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), High energy, High-energy astronomy, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Pulsar, Space and Planetary Science, Feature (computer vision), Astrophysics - High Energy Astrophysical Phenomena
Abstract

The highest-energy known gamma-ray sources are all located within 0.5 degrees of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; $>$ 56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory, we present a joint-likelihood analysis of ten extremely powerful pulsars to search for UHE gamma-ray emission correlated with these locations. We report a significant detection ($>$ 3$��$), indicating that UHE gamma-ray emission is a generic feature of powerful pulsars. We discuss the emission mechanisms of the gamma rays and the implications of this result. The individual environment that each pulsar is found in appears to play a role in the amount of emission., accepted by ApJL

Published
2021

28. Analysis of Physicochemical and Nutritional Properties of Rambutan (Nephelium Lappaceum L.) Fruit

Author

José Sandoval-Cortés, José Juan Buenrostro-Figueroa, Cristian Hernández-Hernández, José C. De León-Medina, Cristóbal N. Aguilar, Juan A. Ascacio-Valdés, Leonardo Sepúlveda, and Adriana C. Flores-Gallegos

Subjects
Rambutan, biology, Starch, JAMS, Pulp (paper), Raw material, engineering.material, biology.organism_classification, Southeast asia, chemistry.chemical_compound, chemistry, engineering, Nephelium, Cultivar, Food science
Abstract

Rambutan is an exotic fruit native to Southeast Asia. It is composed of peel, pulp, and seed; the pulp is the only edible part of the fruit. The cultivars of rambutan have been expanded in many parts of the world, and its consumption is principally fresh but also is processed in the industry in the production of juices, jams, or jellies, resulting in the peel and the seed as byproducts with potential applications in the industry due to their physicochemical properties, especially the seed. The peel has been reported as an interesting 96source of bioactive compounds and a source of lignocellulosic material that can be used for applications such as bionanocomposites. Rambutan seed is the part of the fruit where most physicochemical properties are reported and is considered for its high amount of fat and starch. The physicochemical properties of rambutan seed fat and starch can be compared with other commercial raw materials used widely in the industry, like cocoa butter or corn starch. So, rambutan seed seems to be a potential new source to be used as a raw material in the pharmaceutical, cosmetic, and food industries.

Published
2021

30. Long-term spectra of the blazars Mrk 421 and Mrk 501 at TeV energies seen by HAWC

Author

A. Albert, R. Alfaro, C. Alvarez, J. R. Angeles Camacho, J. C. Arteaga-Velázquez, K. P. Arunbabu, D. Avila Rojas, H. A. Ayala Solares, V. Baghmanyan, E. Belmont-Moreno, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, R. Diaz Hernandez, M. A. DuVernois, M. Durocher, J. C. Díaz-Vélez, K. Engel, C. Espinoza, K. L. Fan, M. Fernández Alonso, N. Fraija, D. Garcia, J. A. García-González, F. Garfias, M. M. González, J. A. Goodman, J. P. Harding, B. Hona, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, V. Joshi, A. Lara, W. H. Lee, J. Lee, H. León Vargas, J. T. Linneman, A. L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, R. Noriega-Papaqui, A. Peisker, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, H. Salazar, F. Salesa Greus, A. Sandoval, M. Schneider, J. Serna-Franco, A. J. Smith, R. W. Springer, K. Tollefson, I. Torres, R. Torres-Escobedo, F. Ureña-Mena, L. Villaseñor, X. Wang, T. Weisgarber, E. Willox, H. Zhou, and C. de León

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, ddc:530, High Energy Physics::Experiment, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

The High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory surveys the very high energy sky in the 300 GeV to $>100$ TeV energy range. HAWC has detected two blazars above $11\sigma$, Markarian 421 (Mrk 421) and Markarian 501 (Mrk 501). The observations are comprised of data taken in the period between June 2015 and July 2018, resulting in a $\sim 1038$ days of exposure. In this work we report the time-averaged spectral analysis for both sources above 0.5 TeV. Taking into account the flux attenuation due to the extragalactic background light (EBL), the intrinsic spectrum of Mrk 421 is described by a power law with an exponential energy cut-off with index $\alpha=2.26\pm(0.12)_{stat}(_{-0.2}^{+0.17})_{sys}$ and energy cut-off $E_c=5.1\pm(1.6)_{stat}(_{-2.5}^{+1.4})_{sys}$ TeV, while the intrinsic spectrum of Mrk 501 is better described by a simple power law with index $\alpha=2.61\pm(0.11)_{stat}(_{-0.07}^{+0.01})_{sys}$. The maximum energies at which the Mrk 421 and Mrk 501 signals are detected are 9 and 12 TeV, respectively. This makes these some of the highest energy detections to date for spectra averaged over years-long timescales. Since the observation of gamma radiation from blazars provides information about the physical processes that take place in their relativistic jets, it is important to study the broad-band spectral energy distribution (SED) of these objects. To this purpose, contemporaneous data in the gamma-ray band to X-ray range, and literature data in the radio to UV range, were used to build time-averaged SEDs that were modeled within a synchrotron self-Compton leptonic scenario., Comment: 16 pages, 5 tables, 9 figures

Published
2021
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31. Probing the Sea of Cosmic Rays by Measuring Gamma-Ray Emission from Passive Giant Molecular Clouds with HAWC

Author

Segev BenZvi, C. Alvarez, S. Coutiño de León, A. Sandoval, Alejandro Lara, Pooja Surajbali, S. Hernandez, E. De la Fuente, Fernando Ureña-Mena, D. Avila Rojas, R. Diaz Hernandez, Andrea Albert, Michael Schneider, K. Malone, Fernando Garfias, H. Zhou, E. Ruiz-Velasco, C. Brisbois, K. P. Arunbabu, Mora Durocher, Petra Hüntemeyer, A. L. Longinotti, O. Martinez, J. S. H. Lee, D. Garcia, H. León Vargas, J. A. Morales-Soto, A. Galván-Gámez, Nicola Omodei, J. A. Goodman, Meghan Tanner, Arturo Iriarte, Brenda Dingus, Y. Pérez Araujo, J. C. Arteaga-Velázquez, Michael Newbold, Alison Peisker, A. Nayerhoda, Juan Carlos Diaz-Velez, Luis Villaseñor, Jose Andres Garcia-Gonzalez, J. R. Angeles Camacho, Ernesto Belmont-Moreno, E. Moreno, Miguel Mostafa, B. Hona, Kwok Lung Fan, Umberto Cotti, K. Tollefson, Kristi Engel, Nissim Illich Fraija, J. P. Harding, T. Weisgarber, Maria Magdalena González, V. Joshi, Sabrina Casanova, M. U. Nisa, J. A. Matthews, Karen S. Caballero-Mora, Ibrahim Torres, V. Baghmanyan, Elijah Willox, Jorge Cotzomi, Catalina Espinoza, José Serna-Franco, Gilgamesh Luis-Raya, Filiberto Hueyotl-Zahuantitla, Jesús Martínez-Castro, H. A. Ayala Solares, Ruben Alfaro, C. D. Rho, R. Noriega-Papaqui, Dezhi Huang, Pedro Miranda-Romagnoli, J. T. Linnemann, William H. Lee, Daniel Rosa-Gonzalez, T. Capistrán, M. Fernández Alonso, R. Torres-Escobedo, A. J. Smith, R. W. Springer, L. Nellen, E. G. Pérez-Pérez, David Kieda, C. De León, F. Salesa Greus, Rhiannon Turner, Michael DuVernois, A. Carraminana, Joe Lundeen, and R. W. Ellsworth

Subjects
Physics, High Energy Astrophysical Phenomena (astro-ph.HE), High-energy astronomy, Molecular cloud, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Space and Planetary Science, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics
Abstract

The study of high-energy gamma rays from passive Giant Molecular Clouds (GMCs) in our Galaxy is an indirect way to characterize and probe the paradigm of the "sea" of cosmic rays in distant parts of the Galaxy. By using data from the High Altitude Water Cherenkov (HAWC) observatory, we measure the gamma-ray flux above 1 TeV of a set of these clouds to test the paradigm. We selected high-galactic latitude clouds that are in HAWC's field-of-view and which are within 1~kpc distance from the Sun. We find no significant excess emission in the cloud regions, nor when we perform a stacked log-likelihood analysis of GMCs. Using a Bayesian approach, we calculate 95\% credible intervals upper limits of the gamma-ray flux and estimate limits on the cosmic-ray energy density of these regions. These are the first limits to constrain gamma-ray emission in the multi-TeV energy range ($>$1 TeV) using passive high-galactic latitude GMCs. Assuming that the main gamma-ray production mechanism is due to proton-proton interaction, the upper limits are consistent with a cosmic-ray flux and energy density similar to that measured at Earth., 6 figures, 6 tables

Published
2021
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32. Piloting the Response to Intervention Model in the Canary Islands: Prevention of Reading and Math Learning Disabilities

Author

Sara C. de León, Nuria Gutiérrez, and Juan E. Jiménez

Subjects
Linguistics and Language, Response to intervention, media_common.quotation_subject, Fidelity, Context (language use), Language and Linguistics, Intervention (counseling), Reading (process), Tier 2 network, Mathematics education, medicine, Humans, 0501 psychology and cognitive sciences, Students, General Psychology, media_common, Academic year, Learning Disabilities, 05 social sciences, 050301 education, Reading, Spain, Learning disability, medicine.symptom, Psychology, 0503 education, Mathematics, 050104 developmental & child psychology
Abstract

The main objective of this study was to examine the effectiveness of an intervention implemented by elementary school teachers within the context of the Response to Intervention (RtI) model. For this purpose, a Tier 2 or secondary intervention was implemented by Spanish-speaking teachers in grades K-3 after receiving training to implement RtI components with fidelity. A total of 1,923 at-risk students were assigned to treatment (in reading,n= 542; in math,n= 483) or control (in reading,n= 406; in math,n= 492). Teachers were provided with a support system that included two web-based training programs for reading (i.e.,Letraprogram) and math (i.e.,Primateprogram). Implementation fidelity was analyzed using direct observations and self-reports. All students were assessed three times during the academic year. A hierarchical linear growth modeling was conducted, and differences in the growth rate of reading and math performance were analyzed between at-risk students who have received the intervention and those who have not received it. Children at-risk in the intervention condition appeared to benefit more than at-risk children in the control condition. Moreover, findings indicate that the earlier the intervention, the greater the percentage of students who leave the situation of risk of learning difficulties in reading and math.

Published
2021

33. Spectrum and morphology of the very-high-energy source HAWC J2019+368

Author

R. W. Springer, C. D. Rho, E. G. Pérez-Pérez, Alison Peisker, A. J. Smith, J. A. Morales-Soto, E. Moreno, Sabrina Casanova, V. Joshi, Dezhi Huang, Rhiannon Turner, Michael DuVernois, L. Nellen, A. Carraminana, T. Capistrán, Joe Lundeen, J. P. Harding, Gwenael Giacinti, Jorge Cotzomi, J. C. Arteaga-Velázquez, Karen S. Caballero-Mora, Nicola Omodei, Jose Andres Garcia-Gonzalez, S. Coutiño de León, T. Weisgarber, V. Baghmanyan, Catalina Espinoza, J. A. Goodman, D. Garcia, Nissim Illich Fraija, H. Zhou, A. Jardin-Blicq, Jesús Martínez-Castro, H. A. Ayala Solares, K. P. Arunbabu, A. L. Longinotti, A. Sandoval, Ernesto Belmont-Moreno, Humberto Ibarguen Salazar, O. Martinez, Jim Hinton, Andrea Albert, Michael Schneider, P. Huentemeyer, Miguel Mostafa, C. Brisbois, Harm Schoorlemmer, M. U. Nisa, R. Noriega-Papaqui, Binita Hona, Elijah Willox, Pooja Surajbali, Brenda Dingus, William H. Lee, L. Olivera-Nieto, Michael Newbold, José Serna-Franco, R. Diaz Hernandez, Fernando Ureña-Mena, Pedro Miranda-Romagnoli, R. López-Coto, K. Tollefson, Y. Pérez Araujo, E. Ruiz-Velasco, A. Nayerhoda, J. T. Linnemann, F. Salesa Greus, Ibrahim Torres, Mora Durocher, H. León Vargas, C. Alvarez, Maria Magdalena González, E. De la Fuente, C. De León, D. Avila Rojas, Filiberto Hueyotl-Zahuantitla, Gilgamesh Luis-Raya, K. Malone, John Matthews, Ruben Alfaro, Daniel Rosa-Gonzalez, and Kristi Engel

Subjects
Energy dependent, Physics, High energy, Nebula, 010504 meteorology & atmospheric sciences, media_common.quotation_subject, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Pulsar wind nebula, Pulsar, Space and Planetary Science, Sky, 0103 physical sciences, Supernova remnant, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, media_common
Abstract

The MGRO J2019+37 region is one of the brightest sources in the sky at TeV energies. It was detected in the second HAWC catalog as 2HWC J2019+367 and here we present a detailed study of this region using data from HAWC. This analysis resolves the region into two sources: HAWC J2019+368 and HAWC J2016+371. We associate HAWC J2016+371 with the evolved supernova remnant CTB 87, although its low significance in this analysis prevents a detailed study at this time. An investigation of the morphology (including possible energy-dependent morphology) and spectrum for HAWC J2019+368 is the focus of this work. We associate HAWC J2019+368 with PSR J2021+3651 and its X-ray pulsar wind nebula, the Dragonfly nebula. Modeling the spectrum measured by HAWC and Suzaku reveals a ∼7 kyr pulsar and nebula system producing the observed emission at X-ray and γ-ray energies.

Published
2021

34. Heterogeneous contributions of change in population distribution of body mass index to change in obesity and underweight

Author

Iurilli, M.L.C. Zhou, B. Bennett, J.E. Carrillo-Larco, R.M. Sophiea, M.K. Rodriguez-Martinez, A. Bixby, H. Solomon, B.D. Taddei, C. Danaei, G. Di Cesare, M. Stevens, G.A. Riley, L.M. Savin, S. Cowan, M.J. Bovet, P. Damasceno, A. Chirita-Emandi, A. Hayes, A.J. Ikeda, N. Jackson, R.T. Khang, Y.-H. Laxmaiah, A. Liu, J. Miranda, J.J. Saidi, O. Sebert, S. Sorić, M. Starc, G. Gregg, E.W. Abarca-Gómez, L. Abdeen, Z.A. Abdrakhmanova, S. Ghaffar, S.A. Rahim, H.F.A. Abu-Rmeileh, N.M. Garba, J.A. Acosta-Cazares, B. Adams, R.J. Aekplakorn, W. Afsana, K. Afzal, S. Agdeppa, I.A. Aghazadeh-Attari, J. Aguilar-Salinas, C.A. Agyemang, C. Ahmad, M.H. Ahmad, N.A. Ahmadi, A. Ahmadi, N. Ahmed, S.H. Ahrens, W. Aitmurzaeva, G. Ajlouni, K. Al-Hazzaa, H.M. Al-Lahou, B. Al-Raddadi, R. Alarouj, M. AlBuhairan, F. AlDhukair, S. Ali, M.M. Alkandari, A. Alkerwi, A. Allin, K. Alvarez-Pedrerol, M. Aly, E. Amarapurkar, D.N. Amiri, P. Amougou, N. Amouyel, P. Andersen, L.B. Anderssen, S.A. Ängquist, L. Anjana, R.M. Ansari-Moghaddam, A. Aounallah-Skhiri, H. Araújo, J. Ariansen, I. Aris, T. Arku, R.E. Arlappa, N. Aryal, K.K. Aspelund, T. Assah, F.K. Assunção, M.C.F. Aung, M.S. Auvinen, J. Mária Avdicová Avi, S. Azevedo, A. Azimi-Nezhad, M. Azizi, F. Azmin, M. Babu, B.V. Bæksgaard Jørgensen, M. Baharudin, A. Bahijri, S. Baker, J.L. Balakrishna, N. Bamoshmoosh, M. Banach, M. Bandosz, P. Banegas, J.R. Baran, J. Barbagallo, C.M. Barceló, A. Barkat, A. Barros, A.J.D. Barros, M.V.G. Basit, A. Bastos, J.L.D. Bata, I. Batieha, A.M. Batista, R.L. Battakova, Z. Batyrbek, A. Baur, L.A. Beaglehole, R. Bel-Serrat, S. Belavendra, A. Romdhane, H.B. Benedics, J. Benet, M. Bergh, I.H. Berkinbayev, S. Bernabe-Ortiz, A. Bernotiene, G. Bettiol, H. Bezerra, J. Bhagyalaxmi, A. Bharadwaj, S. Bhargava, S.K. Bhutta, Z.A. Bi, H. Bi, Y. Bia, D. Lele, E.C.B. Bikbov, M.M. Bista, B. Bjelica, D.J. Bjerregaard, P. Bjertness, E. Bjertness, M.B. Björkelund, C. Bloch, K.V. Blokstra, A. Bo, S. Bobak, M. Boddy, L.M. Boehm, B.O. Boeing, H. Boggia, J.G. Bogova, E. Boissonnet, C.P. Bojesen, S.E. Bonaccio, M. Bongard, V. Bonilla-Vargas, A. Bopp, M. Borghs, H. Braeckevelt, L. Braeckman, L. Bragt, M.C.E. Brajkovich, I. Branca, F. Breckenkamp, J. Breda, J. Brenner, H. Brewster, L.M. Brian, G.R. Brinduse, L. Brophy, S. Bruno, G. Bueno-de-Mesquita, H.B. Bugge, A. Buoncristiano, M. Burazeri, G. Burns, C. de León, A.C. Cacciottolo, J. Cai, H. Cama, T. Cameron, C. Camolas, J. Can, G. Candido, A.P.C. Cañete, F. Capanzana, M.V. Capková, N. Capuano, E. Capuano, V. Cardol, M. Cardoso, V.C. Carlsson, A.C. Carmuega, E. Carvalho, J. Casajús, J.A. Casanueva, F.F. Celikcan, E. Censi, L. Cervantes-Loaiza, M. Cesar, J.A. Chamukuttan, S. Chan, A.W. Chan, Q. Chaturvedi, H.K. Chaturvedi, N. Rahim, N.C.A. Chee, M.L. Chen, C.-J. Chen, F. Chen, H. Chen, S. Chen, Z. Cheng, C.-Y. Cheraghian, B. Chetrit, A. Chikova-Iscener, E. Chiolero, A. Chiou, S.-T. Chirlaque, M.-D. Cho, B. Christensen, K. Christofaro, D.G. Chudek, J. Cifkova, R. Cilia, M. Cinteza, E. Claessens, F. Clarke, J. Clays, E. Cohen, E. Concin, H. Confortin, S.C. Cooper, C. Coppinger, T.C. Corpeleijn, E. Costanzo, S. Cottel, D. Cowell, C. Craig, C.L. Crampin, A.C. Crujeiras, A.B. Csilla, S. Cucu, A.M. Cui, L. Cureau, F.V. Czenczek-Lewandowska, E. D’Arrigo, G. d’Orsi, E. Dacica, L. Dal Re Saavedra, M.A. Dallongeville, J. Damsgaard, C.T. Dankner, R. Dantoft, T.M. Dasgupta, P. Dastgiri, S. Dauchet, L. Davletov, K. De Backer, G. De Bacquer, D. de Gaetano, G. De Henauw, S. de Oliveira, P.D. De Ridder, D. De Ridder, K. de Rooij, S.R. De Smedt, D. Deepa, M. Deev, A.D. DeGennaro, V., Jr Dehghan, A. Delisle, H. Delpeuch, F. Demarest, S. Dennison, E. Dereń, K. Deschamps, V. Dhimal, M. Di Castelnuovo, A.F. Dias-da-Costa, J.S. Díaz-Sánchez, M.E. Diaz, A. Dika, Z. Djalalinia, S. Djordjic, V. Do, H.T.P. Dobson, A.J. Donati, M.B. Donfrancesco, C. Donoso, S.P. Döring, A. Dorobantu, M. Dorosty, A.R. Doua, K. Dragano, N. Drygas, W. Duan, J.L. Duante, C.A. Duboz, P. Duda, R.B. Duleva, V. Dulskiene, V. Dumith, S.C. Dushpanova, A. Dzerve, V. Dziankowska-Zaborszczyk, E. Eddie, R. Eftekhar, E. Egbagbe, E.E. Eggertsen, R. Eghtesad, S. Eiben, G. Ekelund, U. El-Khateeb, M. Ati, J.E. Eldemire-Shearer, D. Eliasen, M. Elliott, P. Engle-Stone, R. Enguerran, M. Erasmus, R.T. Erbel, R. Erem, C. Eriksen, L. Eriksson, J.G. Escobedo-de la Peña, J. Eslami, S. Esmaeili, A. Evans, A. Faeh, D. Fakhretdinova, A.A. Fall, C.H. Faramarzi, E. Farjam, M. Sant’Angelo, V.F. Farzadfar, F. Fattahi, M.R. Fawwad, A. Felix-Redondo, F.J. Ferguson, T.S. Fernandes, R.A. Fernández-Bergés, D. Ferrante, D. Ferrao, T. Ferrari, M. Ferrario, M.M. Ferreccio, C. Ferrer, E. Ferrieres, J. Figueiró, T.H. Fijalkowska, A. Fink, G. Fischer, K. Foo, L.H. Forsner, M. Fouad, H.M. Francis, D.K. Maria do Carmo Franco Frikke-Schmidt, R. Frontera, G. Fuchs, F.D. Fuchs, S.C. Fujiati, I.I. Fujita, Y. Fumihiko, M. Furusawa, T. Gaciong, Z. Gafencu, M. Galbarczyk, A. Galenkamp, H. Galeone, D. Galfo, M. Galvano, F. Gao, J. Garcia-de-la-Hera, M. García-Solano, M. Gareta, D. Garnett, S.P. Gaspoz, J.-M. Gasull, M. Gaya, A.C.A. Gaya, A.R. Gazzinelli, A. Gehring, U. Geiger, H. Geleijnse, J.M. Ghanbari, A. Ghasemi, E. Gheorghe-Fronea, O.-F. Giampaoli, S. Gianfagna, F. Gill, T.K. Giovannelli, J. Gironella, G. Giwercman, A. Gkiouras, K. Godos, J. Gogen, S. Goldberg, M. Goldsmith, R.A. Goltzman, D. Gómez, S.F. Gomula, A. da Silva, B.G.C. Gonçalves, H. Gonzalez-Chica, D.A. Gonzalez-Gross, M. González-Leon, M. González-Rivas, J.P. González-Villalpando, C. González-Villalpando, M.-E. Gonzalez, A.R. Gottrand, F. Graça, A.P. Graff-Iversen, S. Grafnetter, D. Grajda, A. Grammatikopoulou, M.G. Gregor, R.D. Grodzicki, T. Grøholt, E.K. Grøntved, A. Grosso, G. Gruden, G. Gu, D. Gualdi-Russo, E. Guallar-Castillón, P. Gualtieri, A. Gudmundsson, E.F. Gudnason, V. Guerrero, R. Guessous, I. Guimaraes, A.L. Gulliford, M.C. Gunnlaugsdottir, J. Gunter, M.J. Guo, X.-H. Guo, Y. Gupta, P.C. Gupta, R. Gureje, O. Gurzkowska, B. Gutiérrez-González, E. Gutierrez, L. Gutzwiller, F. Ha, S. Hadaegh, F. Hadjigeorgiou, C.A. Haghshenas, R. Hakimi, H. Halkjær, J. Hambleton, I.R. Hamzeh, B. Hange, D. Hanif, A.A.M. Hantunen, S. Hao, J. Kumar, R.H. Hashemi-Shahri, S.M. Hassapidou, M. Hata, J. Haugsgjerd, T. He, J. He, Y. He, Y. Heidinger-Felso, R. Heinen, M. Hejgaard, T. Hendriks, M.E. dos Santos Henrique, R. Henriques, A. Cadena, L.H. Herrala, S. Herrera, V.M. Herter-Aeberli, I. Heshmat, R. Hill, A.G. Ho, S.Y. Ho, S.C. Hobbs, M. Holdsworth, M. Homayounfar, R. Homs, C. Hopman, W.M. Horimoto, A.R.V.R. Hormiga, C.M. Horta, B.L. Houti, L. Howitt, C. Htay, T.T. Htet, A.S. Htike, M.M.T. Hu, Y. Huerta, J.M. Huhtaniemi, I.T. Huiart, L. Petrescu, C.H. Huisman, M. Husseini, A. Huu, C.N. Huybrechts, I. Hwalla, N. Hyska, J. Iacoviello, L. Ibarluzea, J.M. Ibrahim, M.M. Wong, N.I. Ikram, M.A. Iotova, V. Irazola, V.E. Ishida, T. Islam, M. Islam, S.M.S. Iwasaki, M. Jacobs, J.M. Jaddou, H.Y. Jafar, T. James, K. Jamil, K.M. Jamrozik, K. Janszky, I. Janus, E. Jarani, J. Jarvelin, M.-R. Jasienska, G. Jelakovic, A. Jelakovic, B. Jennings, G. Jha, A.K. Jiang, C.Q. Jimenez, R.O. Jöckel, K.-H. Joffres, M. Johansson, M. Jokelainen, J.J. Jonas, J.B. Jonnagaddala, J. Jørgensen, T. Joshi, P. Joukar, F. Jovic, D.P. Jóźwiak, J.J. Juolevi, A. Jurak, G. Simina, I.J. Juresa, V. Kaaks, R. Kaducu, F.O. Kafatos, A. Kajantie, E.O. Kalmatayeva, Z. Kalter-Leibovici, O. Kameli, Y. Kampmann, F.B. Kanala, K.R. Kannan, S. Kapantais, E. Karakosta, A. Kårhus, L.L. Karki, K.B. Katibeh, M. Katz, J. Katzmarzyk, P.T. Kauhanen, J. Kaur, P. Kavousi, M. Kazakbaeva, G.M. Keil, U. Boker, L.K. Keinänen-Kiukaanniemi, S. Kelishadi, R. Kelleher, C. Kemper, H.C.G. Kengne, A.P. Keramati, M. Kerimkulova, A. Kersting, M. Key, T. Khader, Y.S. Khalili, D. Khaw, K.-T. Kheiri, B. Kheradmand, M. Khosravi, A. Khouw, I.M.S.L. Kiechl-Kohlendorfer, U. Kiechl, S. Killewo, J. Kim, D.W. Kim, H.C. Kim, J. Kindblom, J.M. Klakk, H. Klimek, M. Klimont, J. Klumbiene, J. Knoflach, M. Koirala, B. Kolle, E. Kolsteren, P. König, J. Korpelainen, R. Korrovits, P. Korzycka, M. Kos, J. Koskinen, S. Kouda, K. Kovacs, V.A. Kowlessur, S. Koziel, S. Kratenova, J. Kratzer, W. Kriemler, S. Kristensen, P.L. Krokstad, S. Kromhout, D. Kruger, H.S. Kubinova, R. Kuciene, R. Kujala, U.M. Kujundzic, E. Kulaga, Z. Kumar, R.K. Kunešová, M. Kurjata, P. Kusuma, Y.S. Kuulasmaa, K. Kyobutungi, C. La, Q.N. Laamiri, F.Z. Laatikainen, T. Lachat, C. Laid, Y. Lam, T.H. Lambrinou, C.-P. Landais, E. Lanska, V. Lappas, G. Larijani, B. Latt, T.S. Lauria, L. Lazo-Porras, M. Le Coroller, G. Bao, K.L.N. Le Port, A. Le, T.D. Lee, J. Lee, J. Lee, P.H. Lehmann, N. Lehtimäki, T. Lemogoum, D. Levitt, N.S. Li, Y. Liivak, M. Lilly, C.L. Lim, W.-Y. Lima-Costa, M.F. Lin, H.-H. Lin, X. Lin, Y.-T. Lind, L. Linneberg, A. Lissner, L. Litwin, M. Liu, L. Lo, W.-C. Loit, H.-M. Long, K.Q. Lopes, L. Lopes, O. Lopez-Garcia, E. Lopez, T. Lotufo, P.A. Lozano, J.E. Lukrafka, J.L. Luksiene, D. Lundqvist, A. Lundqvist, R. Lunet, N. Lunogelo, C. Lustigová, M. Łuszczki, E. Ma, G. Ma, J. Ma, X. Machado-Coelho, G.L.L. Machado-Rodrigues, A.M. Macieira, L.M. Madar, A.A. Maggi, S. Magliano, D.J. Magnacca, S. Magriplis, E. Mahasampath, G. Maire, B. Majer, M. Makdisse, M. Mäki, P. Malekzadeh, F. Malekzadeh, R. Malhotra, R. Rao, K.M. Malyutina, S.K. Maniego, L.V. Manios, Y. Mann, J.I. Mansour-Ghanaei, F. Manzato, E. Margozzini, P. Markaki, A. Markey, O. Ioannidou, E.M. Marques-Vidal, P. Marques, L.P. Marrugat, J. Martin-Prevel, Y. Martin, R. Martorell, R. Martos, E. Maruszczak, K. Marventano, S. Mascarenhas, L.P. Masoodi, S.R. Mathiesen, E.B. Mathur, P. Matijasevich, A. Matsha, T.E. Mavrogianni, C. Mazur, A. Mbanya, J.C.N. McFarlane, S.R. McGarvey, S.T. McKee, M. McLachlan, S. McLean, R.M. McLean, S.B. McNulty, B.A. Benchekor, S.M. Medzioniene, J. Mehdipour, P. Mehlig, K. Mehrparvar, A.H. Meirhaeghe, A. Meisfjord, J. Meisinger, C. Menezes, A.M.B. Menon, G.R. Mensink, G.B.M. Menzano, M.T. Mereke, A. Meshram, I.I. Metspalu, A. Meyer, H.E. Mi, J. Michaelsen, K.F. Michels, N. Mikkel, K. Milkowska, K. Miller, J.C. Minderico, C.S. Mini, G.K. Miquel, J.F. Mirjalili, M.R. Mirkopoulou, D. Mirrakhimov, E. Mišigoj-Durakovic, M. Mistretta, A. Mocanu, V. Modesti, P.A. Moghaddam, S.S. Mohajer, B. Mohamed, M.K. Mohamed, S.F. Mohammad, K. Mohammadi, Z. Mohammadifard, N. Mohammadpourhodki, R. Mohan, V. Mohanna, S. Yusoff, M.F.M. Mohebbi, I. Mohebi, F. Moitry, M. Molbo, D. Møllehave, L.T. Møller, N.C. Molnár, D. Momenan, A. Mondo, C.K. Monroy-Valle, M. Monterrubio-Flores, E. Monyeki, K.D.K. Moon, J.S. Moosazadeh, M. Moreira, L.B. Morejon, A. Moreno, L.A. Morgan, K. Morin, S.N. Mortensen, E.L. Moschonis, G. Mossakowska, M. Mostafa, A. Mota-Pinto, A. Mota, J. Motlagh, M.E. Motta, J. Moura-dos-Santos, M.A. Mridha, M.K. Msyamboza, K.P. Mu, T.T. Muc, M. Mugoša, B. Muiesan, M.L. Mukhtorova, P. Müller-Nurasyid, M. Murphy, N. Mursu, J. Murtagh, E.M. Musa, K.I. Milanovic, S.M. Musil, V. Mustafa, N. Nabipour, I. Naderimagham, S. Nagel, G. Naidu, B.M. Najafi, F. Nakamura, H. Námešná, J. Nang, E.E.K. Nangia, V.B. Nankap, M. Narake, S. Nardone, P. Nauck, M. Neal, W.A. Nejatizadeh, A. Nekkantti, C. Nelis, K. Nelis, L. Nenko, I. Neovius, M. Nervi, F. Nguyen, C.T. Nguyen, N.D. Nguyen, Q.N. Nieto-Martínez, R.E. Nikitin, Y.P. Ning, G. Ninomiya, T. Nishtar, S. Noale, M. Noboa, O.A. Nogueira, H. Norat, T. Nordendahl, M. Nordestgaard, B.G. Noto, D. Nowak-Szczepanska, N. Al Nsour, M. Nuhoglu, I. Nurk, E. O’Neill, T.W. O’Reilly, D. Obreja, G. Ochimana, C. Ochoa-Avilés, A.M. Oda, E. Oh, K. Ohara, K. Ohlsson, C. Ohtsuka, R. Olafsson, O. Olinto, M.T.A. Oliveira, I.O. Omar, M.A. Onat, A. Ong, S.K. Ono, L.M. Ordunez, P. Ornelas, R. Ortiz, A.P. Ortiz, P.J. Osler, M. Osmond, C. Ostojic, S.M. Ostovar, A. Otero, J.A. Overvad, K. Owusu-Dabo, E. Paccaud, F.M. Padez, C. Pagkalos, I. Pahomova, E. de Paiva, K.M. Pajak, A. Palli, D. Palloni, A. Palmieri, L. Pan, W.-H. Panda-Jonas, S. Pandey, A. Panza, F. Papandreou, D. Park, S.-W. Park, S. Parnell, W.R. Parsaeian, M. Pascanu, I.M. Pasquet, P. Patel, N.D. Pecin, I. Pednekar, M.S. Peer, N. Pei, G. Peixoto, S.V. Peltonen, M. Pereira, A.C. Peres, M.A. Pérez-Farinós, N. Pérez, C.M. Peterkova, V. Peters, A. Petersmann, A. Petkeviciene, J. Petrauskiene, A. Pettenuzzo, E. Peykari, N. Pham, S.T. Pichardo, R.N. Pierannunzio, D. Pigeot, I. Pikhart, H. Pilav, A. Pilotto, L. Pistelli, F. Pitakaka, F. Piwonska, A. Pizarro, A.N. Plans-Rubió, P. Poh, B.K. Pohlabeln, H. Pop, R.M. Popovic, S.R. Porta, M. Posch, G. Poudyal, A. Poulimeneas, D. Pouraram, H. Pourfarzi, F. Pourshams, A. Poustchi, H. Pradeepa, R. Price, A.J. Price, J.F. Providencia, R. Puder, J.J. Pudule, I. Puhakka, S.E. Puiu, M. Punab, M. Qasrawi, R.F. Qorbani, M. Bao, T.Q. Radic, I. Radisauskas, R. Rahimikazerooni, S. Rahman, M. Rahman, M. Raitakari, O. Raj, M. Rakhimova, E. Rakhmatulloev, S. Rakovac, I. Rao, S.R. Ramachandran, A. Ramke, J. Ramos, E. Ramos, R. Rampal, L. Rampal, S. Rarra, V. Rascon-Pacheco, R.A. Rasmussen, M. Rech, C.R. Redon, J. Reganit, P.F.M. Regecová, V. Revilla, L. Rezaianzadeh, A. Ribas-Barba, L. Ribeiro, R. Riboli, E. Richter, A. Rigo, F. Rinaldo, N. de Wit, T.F.R. Rito, A. Ritti-Dias, R.M. Rivera, J.A. Robitaille, C. Roccaldo, R. Rodrigues, D. Rodríguez-Artalejo, F. del Cristo Rodriguez-Perez, M. Rodríguez-Villamizar, L.A. Roggenbuck, U. Rojas-Martinez, R. Rojroongwasinkul, N. Romaguera, D. Romeo, E.L. Rosario, R.V. Rosengren, A. Rouse, I. Roy, J.G.R. Rubinstein, A. Rühli, F.J. Ruidavets, J.-B. Ruiz-Betancourt, B.S. Ruiz-Castell, M. Moreno, E.R. Rusakova, I.A. Jonsson, K.R. Russo, P. Rust, P. Rutkowski, M. Sabanayagam, C. Sacchini, E. Sachdev, H.S. Sadjadi, A. Safarpour, A.R. Safiri, S. Saki, N. Salanave, B. Martinez, E.S. Salmerón, D. Salomaa, V. Salonen, J.T. Salvetti, M. Samoutian, M. Sánchez-Abanto, J. Sans, S. Marina, L.S. Santos, D.A. Santos, I.S. Santos, L.C. Santos, M.P. Santos, O. Santos, R. Sanz, S.S. Saramies, J.L. Sardinha, L.B. Sarrafzadegan, N. Sathish, T. Saum, K.-U. Savva, S. Savy, M. Sawada, N. Sbaraini, M. Scazufca, M. Schaan, B.D. Rosario, A.S. Schargrodsky, H. Schienkiewitz, A. Schipf, S. Schmidt, C.O. Schmidt, I.M. Schnohr, P. Schöttker, B. Schramm, S. Schramm, S. Schröder, H. Schultsz, C. Schutte, A.E. Sein, A.A. Selamat, R. Sember, V. Sen, A. Senbanjo, I.O. Sepanlou, S.G. Sequera, V. Serra-Majem, L. Servais, J. Ševcíková, L. Shalnova, S.A. Shamah-Levy, T. Shamshirgaran, M. Shanthirani, C.S. Sharafkhah, M. Sharma, S.K. Shaw, J.E. Shayanrad, A. Shayesteh, A.A. Shengelia, L. Shi, Z. Shibuya, K. Shimizu-Furusawa, H. Shin, D.W. Shirani, M. Shiri, R. Shrestha, N. Si-Ramlee, K. Siani, A. Siantar, R. Sibai, A.M. Silva, A.M. Silva, D.A.S. Simon, M. Simons, J. Simons, L.A. Sjöberg, A. Sjöström, M. Skodje, G. Slowikowska-Hilczer, J. Slusarczyk, P. Smeeth, L. So, H.-K. Soares, F.C. Sobek, G. Sobngwi, E. Sodemann, M. Söderberg, S. Soekatri, M.Y.E. Soemantri, A. Sofat, R. Solfrizzi, V. Somi, M.H. Sonestedt, E. Song, Y. Sørensen, T.I.A. Sørgjerd, E.P. Jérome, C.S. Soto-Rojas, V.E. Soumaré, A. Sovic, S. Sparboe-Nilsen, B. Sparrenberger, K. Spinelli, A. Spiroski, I. Staessen, J.A. Stamm, H. Stathopoulou, M.G. Staub, K. Stavreski, B. Steene-Johannessen, J. Stehle, P. Stein, A.D. Stergiou, G.S. Stessman, J. Stevanovic, R. Stieber, J. Stöckl, D. Stocks, T. Stokwiszewski, J. Stoyanova, E. Stratton, G. Stronks, K. Strufaldi, M.W. Sturua, L. Suárez-Medina, S. Suka, M. Sun, C.-A. Sundström, J. Sung, Y.-T. Sunyer, J. Suriyawongpaisal, P. Swinburn, B.A. Sy, R.G. Syddall, H.E. Sylva, R.C. Szklo, M. Szponar, L. Tai, E.S. Tammesoo, M.-L. Tamosiunas, A. Tan, E.J. Tang, X. Tanrygulyyeva, M. Tanser, F. Tao, Y. Tarawneh, M.R. Tarp, J. Tarqui-Mamani, C.B. Braunerová, R.T. Taylor, A. Taylor, J. Tchibindat, F. Tebar, W.R. Tell, G.S. Tello, T. Tham, Y.C. Thankappan, K.R. Theobald, H. Theodoridis, X. Thijs, L. Thomas, N. Thuesen, B.H. Tichá, L. Timmermans, E.J. Tjonneland, A. Tolonen, H.K. Tolstrup, J.S. Topbas, M. Topór-Madry, R. Torheim, L.E. Tormo, M.J. Tornaritis, M.J. Torrent, M. Torres-Collado, L. Toselli, S. Touloumi, G. Traissac, P. Tran, T.T.-H. Trichopoulos, D. Trichopoulou, A. Trinh, D.T.H. Trivedi, A. Tshepo, L. Tsigga, M. Tsugane, S. Tuliakova, A.M. Tulloch-Reid, M.K. Tullu, F. Tuomainen, T.-P. Tuomilehto, J. Turley, M.L. Twig, G. Tynelius, P. Tzotzas, T. Tzourio, C. Ueda, P. Ugel, E. Ukoli, F.A.M. Ulmer, H. Unal, B. Usupova, Z. Uusitalo, H.M.T. Uysal, N. Vaitkeviciute, J. Valdivia, G. Vale, S. Valvi, D. van Dam, R.M. Van der Heyden, J. van der Schouw, Y.T. Van Herck, K. Van Minh, H. Van Schoor, N.M. van Valkengoed, I.G.M. Vanderschueren, D. Vanuzzo, D. Varbo, A. Varela-Moreiras, G. Varona-Pérez, P. Vasan, S.K. Vega, T. Veidebaum, T. Velasquez-Melendez, G. Velika, B. Veronesi, G. Verschuren, W.M.M. Victora, C.G. Viegi, G. Viet, L. Villalpando, S. Vineis, P. Vioque, J. Virtanen, J.K. Visser, M. Visvikis-Siest, S. Viswanathan, B. Vladulescu, M. Vlasoff, T. Vocanec, D. Vollenweider, P. Völzke, H. Voutilainen, A. Voutilainen, S. Vrijheid, M. Vrijkotte, T.G.M. Wade, A.N. Wagner, A. Waldhör, T. Walton, J. Wambiya, E.O.A. Bebakar, A.M.W. Mohamud, W.N.W. de Souza Wanderley Júnior, R. Wang, M.-D. Wang, N. Wang, Q. Wang, X. Wang, Y.X. Wang, Y.-W. Wannamethee, S.G. Wareham, N. Weber, A. Wedderkopp, N. Weerasekera, D. Weghuber, D. Wei, W. Weres, A. Werner, B. Whincup, P.H. Widhalm, K. Widyahening, I.S. Wiecek, A. Wilks, R.J. Willeit, J. Willeit, P. Williams, J. Wilsgaard, T. Wojtyniak, B. Wong-McClure, R.A. Wong, A. Wong, J.E. Wong, T.Y. Woo, J. Woodward, M. Wu, F.C. Wu, J. Wu, L.J. Wu, S. Xu, H. Xu, L. Yaacob, N.A. Yamborisut, U. Yan, W. Yang, L. Yang, X. Yang, Y. Yardim, N. Yaseri, M. Yasuharu, T. Ye, X. Yiallouros, P.K. Yoosefi, M. Yoshihara, A. You, Q.S. You, S.-L. Younger-Coleman, N.O. Yusof, S.M. Yusoff, A.F. Zaccagni, L. Zafiropulos, V. Zainuddin, A.A. Zakavi, S.R. Zamani, F. Zambon, S. Zampelas, A. Zamrazilová, H. Zapata, M.E. Zargar, A.H. Zaw, K.K. Zdrojewski, T. Zejglicova, K. Vrkic, T.Z. Zeng, Y. Zhang, L. Zhang, Z.-Y. Zhao, D. Zhao, M.-H. Zhao, W. Zhen, S. Zheng, W. Zheng, Y. Zholdin, B. Zhou, M. Zhu, D. Zins, M. Zitt, E. Zocalo, Y. Cisneros, J.Z. Zuziak, M. Ezzati, M. Filippi, S. NCD Risk Factor Collaboration (NCD-RisC)

Subjects
nutritional and metabolic diseases, sense organs, skin and connective tissue diseases
Abstract

From 1985 to 2016, the prevalence of underweight decreased, and that of obesity and severe obesity increased, in most regions, with significant variation in the magnitude of these changes across regions. We investigated how much change in mean body mass index (BMI) explains changes in the prevalence of underweight, obesity, and severe obesity in different regions using data from 2896 population-based studies with 187 million participants. Changes in the prevalence of underweight and total obesity, and to a lesser extent severe obesity, are largely driven by shifts in the distribution of BMI, with smaller contributions from changes in the shape of the distribution. In East and Southeast Asia and sub-Saharan Africa, the underweight tail of the BMI distribution was left behind as the distribution shifted. There is a need for policies that address all forms of malnutrition by making healthy foods accessible and affordable, while restricting unhealthy foods through fiscal and regulatory restrictions. © Copyright.

Published
2021

36. Responding to Human Influence: Southern Sea Lion Males Adapt to Harbor Habitats

Author

Joaquín C. M. Gana, Marta C. De León, Sergio Morón, Diego Rodríguez, Pablo Denuncio, María Agustina Mandiola, Julián Bastida, Gisela Giardino, and Ricardo Bastida

Subjects
Fishery, Geography, Habitat, biology, Fishing, Seasonal breeder, %22">Fish , Otaria flavescens, biology.organism_classification, Sea lion
Abstract

Male-only hauling grounds occur in close association to breeding colonies in several otariids. The occasional use of human-built infrastructure by these groups is also common. We observed permanent male aggregations of southern sea lions, Otaria flavescens, in urban contexts, such as two of the main fishing harbors in Argentina and investigated how they changed over 35 years. These haul-outs are located approximately 700 km from Uruguayan and northern Patagonian breeding grounds. Males in urban colonies have functional connections with both populations. A predictable pattern of dispersion during the breeding season, returning for winter, indicate site fidelity. Harbor habitats present ever changing stimuli, threats and challenges to habituated sea lions. Sequential, rapid and spontaneous changes in the location of the aggregations may be a response to quick learning and socially transmitted knowledge. Food provision via consumption of fish offal—complemented with natural foraging—provide support to these aggregations over prolonged periods. The presence of hundreds of sea lions in harbors represents a management challenge. Fidelity to resting areas and rapid habituation to human presence makes it difficult to design strategies that can deter sea lions from intensive use of critical sectors of port activity. Interaction with fishing gear results in frequent entanglements. The risk of transmission of diseases from and to dogs and other domestic animals is a major potential problem for individuals in unnatural aggregations.

Published
2021

37. Evidence of 200 TeV photons from HAWC J1825-134

Author

R. Noriega-Papaqui, J. R. Angeles Camacho, Gerd J. Kunde, Luis Villaseñor, C. Brisbois, K. Tollefson, J. T. Linnemann, Catalina Espinoza, D. Garcia, F. Serna, Nicola Omodei, A. Iriarte, H. A. Ayala Solares, Lukas Nellen, I. Torres, E. Belmont-Moreno, Gwenael Giacinti, A. Sandoval, B. Hona, Segev BenZvi, J. C. Díaz-Vélez, Vincent Marandon, H. Fleischhack, Michael Schneider, J. Lundeen, Mehr Nisa, K. Engel, Vardan Baghmanyan, F. Salesa Greus, Nissim Fraija, K. P. Arunbabu, A. L. Longinotti, M. Mostafá, J. A. Goodman, M. Durocher, A. Jardin-Blicq, C. De León, Andrea Albert, M. Newbold, U. Cotti, Brenda Dingus, J. P. Harding, J. Martínez-Castro, Alejandro Lara, A. Peisker, E. Moreno, Amid Nayerhoda, Daniel Rosa-Gonzalez, Michael DuVernois, A. Carramiñana, Y. Pérez Araujo, H. León Vargas, R. Diaz Hernandez, E. Willox, P. Miranda-Romagnoli, John Matthews, A. Galván-Gámez, E. De la Fuente, D. Avila Rojas, Oscar Martinez, G. Luis-Raya, Sabrina Casanova, V. Joshi, J.C. Arteaga-Velázquez, P. Hüntemeyer, W. H. Lee, Ke Fang, R. Torres-Escobedo, T. Capistrán, J. Cotzomi, F. Ureña-Mena, F. Garfias, Maria Magdalena González, Hongyan Zhou, Filiberto Hueyotl-Zahuantitla, Ruben Alfaro, C. D. Rho, R. W. Springer, H. Salazar, C. Alvarez, D. Huang, K. Malone, E. G. Pérez-Pérez, and Jose Andres Garcia-Gonzalez

Subjects
Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Photon, 010504 meteorology & atmospheric sciences, Proton, Molecular cloud, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Radiation, 7. Clean energy, 01 natural sciences, Galaxy, 13. Climate action, Space and Planetary Science, Observatory, 0103 physical sciences, Physics::Accelerator Physics, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, Cherenkov radiation, 0105 earth and related environmental sciences
Abstract

The Earth is bombarded by ultra-relativistic particles, known as cosmic rays (CRs). CRs with energies up to a few PeV (=10$^{15}$ eV), the knee in the particle spectrum, are believed to have a Galactic origin. One or more factories of PeV CRs, or PeVatrons, must thus be active within our Galaxy. The direct detection of PeV protons from their sources is not possible since they are deflected in the Galactic magnetic fields. Hundred TeV $\gamma$-rays from decaying $\pi^0$, produced when PeV CRs collide with the ambient gas, can provide the decisive evidence of proton acceleration up to the knee. Here we report the discovery by the High Altitude Water Cherenkov (HAWC) observatory of the $\gamma$-ray source, HAWC~J1825-134, whose energy spectrum extends well beyond 200 TeV without a break or cutoff. The source is found to be coincident with a giant molecular cloud. The ambient gas density is as high as 700 protons/cm$^3$. While the nature of this extreme accelerator remains unclear, CRs accelerated to energies of several PeV colliding with the ambient gas likely produce the observed radiation., Comment: Accepted for publication in ApJL

Published
2020

38. A survey of active galaxies at TeV photon energies with the HAWC gamma-ray observatory

Author

Andrea Albert, Fernando Garfias, Kristi Engel, K. Tollefson, A. Zepeda, E. Ruiz-Velasco, H. León Vargas, Segev BenZvi, Binita Hona, H. Zhou, K. P. Arunbabu, J. A. Morales-Soto, C. Brisbois, Karen S. Caballero-Mora, Jose Andres Garcia-Gonzalez, Ernesto Belmont-Moreno, Pedro Miranda-Romagnoli, Catalina Espinoza, S. Coutiño de León, J. R. Angeles Camacho, Jesús Martínez-Castro, F. Salesa Greus, H. A. Ayala Solares, A. Carraminana, Luis Villaseñor, Daniel Rosa-Gonzalez, E. Moreno, Alejandro Lara, R. W. Springer, Joe Lundeen, C. De León, Alison Peisker, Kwok Lung Fan, E. G. Pérez-Pérez, O. Martinez, J. C. Arteaga-Velázquez, Elijah Willox, Gerd Joachim Kunde, Henrike Fleischhack, Fernando Ureña-Mena, John Matthews, Harm Schoorlemmer, Ibrahim Torres, R. Torres-Escobedo, Gilgamesh Luis-Raya, David Kieda, V. Baghmanyan, R. Noriega-Papaqui, William H. Lee, L. Olivera-Nieto, I. Martinez-Castellanos, C. D. Rho, Mora Durocher, Petra Hüntemeyer, A. Sandoval, A. J. Smith, M. U. Nisa, K. Malone, Michael Schneider, Jorge Cotzomi, S. Hernandez, J. A. Goodman, Michael DuVernois, A. Jardin-Blicq, Nissim Illich Fraija, Dezhi Huang, D. Garcia, J. P. Harding, T. Weisgarber, A. Nayerhoda, Arturo Iriarte, Michael Newbold, Juan Carlos Diaz-Velez, J. T. Linnemann, Tomás Capistrán, C. Alvarez, E. De la Fuente, D. Avila Rojas, A. Galván-Gámez, Brenda Dingus, Anna Lia Longinotti, Humberto Ibarguen Salazar, Umberto Cotti, Maria Magdalena González, Miguel Mostafa, Sabrina Casanova, M. Fernández Alonso, V. Joshi, Filiberto Hueyotl-Zahuantitla, and L. Nellen

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Active galactic nucleus, Radio galaxy, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Extragalactic background light, Space and Planetary Science, Observatory, Sky, Blazar, Astrophysics - High Energy Astrophysical Phenomena, Cherenkov radiation, media_common
Abstract

The High Altitude Water Cherenkov Gamma-Ray Observatory (HAWC) continuously detects TeV photons and particles within its large field-of-view, accumulating every day a deeper exposure of two thirds of the sky. We analyzed 1523~days of HAWC live data acquired over four and a half years, in a follow-up analysis of {138} nearby ($z, Comment: The HAWC survey of Fermi 3FHL AGNs: 30 pages, 13 figures. Submitted to the Astrophysical Journal

Published
2020

39. Universal Screening for Prevention of Reading, Writing, and Math Disabilities in Spanish

Author

Juan E. Jiménez, Nuria Gutiérrez, and Sara C. de León

Subjects
Male, Response to intervention, media_common.quotation_subject, General Chemical Engineering, Writing, Alphabetic principle, General Biochemistry, Genetics and Molecular Biology, Fluency, Phonological awareness, Reading (process), Mathematics education, medicine, Humans, Child, Students, media_common, Language, General Immunology and Microbiology, Learning Disabilities, General Neuroscience, Teaching, Spelling, Curriculum-based measurement, Reading, Learning disability, Female, medicine.symptom, Mathematics
Abstract

The purpose of this study was to describe a Spanish protocol that includes reading, writing, and math Curriculum-Based Measures (CBMs) aimed at early detection of students at risk of presenting learning disabilities (LD). Early identification of LD is a critical component of the Response to Intervention (RtI) model. In early grades, the screening of foundational skills mentioned above can provide a data-based guideline for identifying students requiring a more intensive response-based intervention before starting elementary school. We designed different CBMs based on indicators of basic early reading, writing, and math skills [Indicadores de Progreso de Aprendizaje en Lectura, Escritura y Matematicas, IPAL, IPAE, and IPAM respectively] that aim to fulfill the twofold objective of universal screening and evaluation of the Spanish students’ progress. For reading, IPAL includes alphabetic principle, phonological awareness, concepts about print, and riddles in kindergarten. In first and second grades, IPAL includes alphabetic principle, nonsense words fluency, maze sentences, and oral reading fluency. In addition, it includes phonemic segmentation for first grade and prosody for second grade. For writing, IPAE includes copying letters, writing allographs, dictated letters, dictated words with arbitrary spelling, dictated words with rule-based spelling, dictated nonsense words, dictated sentences, writing sentences, and writing a story for first-third grades. Finally, for math, IPAM includes number comparison, missing number, number identification, quantity array, and counting aloud for kindergarten, and number comparison, multi-digit computation, missing number, single-digit computation, and place value for first-third grades.

Published
2020

40. 3HWC: The Third HAWC Catalog of Very-High-Energy Gamma-ray Sources

Author

Michael Newbold, O. Martinez, Segev BenZvi, F. Serna, Pooja Surajbali, Gus Sinnis, Fernando Garfias, S. Hernandez, A. Zepeda, Fernando Ureña-Mena, E. Ruiz-Velasco, H. Zhou, Y. Pérez Araujo, Nicola Omodei, Arturo Iriarte, A. Nayerhoda, L. Diaz-Cruz, K. P. Arunbabu, A. L. Longinotti, R. Diaz Hernandez, Mora Durocher, Petra Hüntemeyer, A. Sandoval, H. León Vargas, J. A. Morales-Soto, Michael Schneider, A. Jardin-Blicq, J. C. Arteaga-Velázquez, Harm Schoorlemmer, B. Hona, Gilgamesh Luis-Raya, K. Malone, T. N. Ukwatta, R. Noriega-Papaqui, Andrea Albert, Tomás Capistrán, Kwok Lung Fan, Humberto Ibarguen Salazar, William H. Lee, L. Olivera-Nieto, V. Baghmanyan, Alison Peisker, C. Brisbois, Henrike Fleischhack, A. Carraminana, Jose Andres Garcia-Gonzalez, C. Rivière, Mehr Nisa, Miguel Mostafa, D. Garcia, Joe Lundeen, Juan Carlos Diaz-Velez, John Matthews, R. López-Coto, J. P. Harding, R. W. Ellsworth, S. Coutiño de León, T. Weisgarber, V. Joshi, J. R. Angeles Camacho, Alejandro Lara, A. J. Smith, Ibrahim Torres, L. Nellen, J. D. Álvarez, Ke Fang, Ruben Alfaro, K. Tollefson, F. Salesa Greus, Daniel Rosa-Gonzalez, M. Fernández Alonso, C. Alvarez, Kristi Engel, Michael DuVernois, C. De León, E. De la Fuente, J. T. Linnemann, F. Werner, D. Avila Rojas, J. A. Goodman, Pedro Miranda-Romagnoli, Dezhi Huang, A. Galván-Gámez, Brenda Dingus, V. Marandon, Karen S. Caballero-Mora, Catalina Espinoza, Jesús Martínez-Castro, H. A. Ayala Solares, Gwenael Giacinti, I. Martinez-Castellanos, R. Torres-Escobedo, E. Moreno, R. W. Springer, E. G. Pérez-Pérez, David Kieda, Umberto Cotti, Sabrina Casanova, Ernesto Belmont-Moreno, Nissim Illich Fraija, Jim Hinton, Maria Magdalena González, Elijah Willox, Z. Ren, Filiberto Hueyotl-Zahuantitla, and C. D. Rho

Subjects
Physics, High Energy Astrophysical Phenomena (astro-ph.HE), High energy, High-energy astronomy, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Gamma-ray astronomy, Astrophysics::Cosmology and Extragalactic Astrophysics, Pulsar, Space and Planetary Science, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics
Abstract

We present a new catalog of TeV gamma-ray sources using 1523 days of data from the High Altitude Water Cherenkov (HAWC) observatory. The catalog represents the most sensitive survey of the Northern gamma-ray sky at energies above several TeV, with three times the exposure compared to the previous HAWC catalog, 2HWC. We report 65 sources detected at $\geq$ 5 sigma significance, along with the positions and spectral fits for each source. The catalog contains eight sources that have no counterpart in the 2HWC catalog, but are within $1^\circ$ of previously detected TeV emitters, and twenty sources that are more than $1^\circ$ away from any previously detected TeV source. Of these twenty new sources, fourteen have a potential counterpart in the fourth \textit{Fermi} Large Area Telescope catalog of gamma-ray sources. We also explore potential associations of 3HWC sources with pulsars in the ATNF pulsar catalog and supernova remnants in the Galactic supernova remnant catalog., 20 pages, 11 figures. Matches the version published in The Astrophysical Journal. See accompanying data release at https://data.hawc-observatory.org/datasets/3hwc-survey/index.php

Published
2020

41. Analyzing the role of fidelity of RTI Tier 2 reading intervention in Spanish kindergarten and first grade students

Author

Juan E, Jiménez, Nuria, Gutiérrez, and Sara C, de León

Subjects
Dyslexia, Male, Schools, Reading, Spain, Child, Preschool, Early Intervention, Educational, Humans, Female, Self Report, Child, Students
Abstract

This study examined the role of fidelity in the reading outcomes within a Tier 2 intervention implemented by Spanish kindergarten and first grade school teachers. For this purpose, differences in reading performance growth were analyzed among at-risk students who received a Tier 2 intervention with high fidelity, at-risk students who received the same intervention with medium fidelity, and an at-risk control group that did not receive a Tier 2 intervention. Implementation fidelity was analyzed using direct observations and self-reports. All students were assessed three times during the academic year. Hierarchical linear modeling analyses were conducted to explore differences in growth rate. The at-risk children in the intervention condition showed a higher growth compared to at-risk children in the control condition, and specifically when the intervention was delivered with a high degree of fidelity.

Published
2020

42. HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron

Author

E. Moreno, P. Hüntemeyer, R. Torres-Escobedo, Armelle Jardin-Blicq, R. Noriega-Papaqui, J. T. Linnemann, E. G. Pérez-Pérez, Karen S. Caballero-Mora, J. A. Goodman, J. R. Angeles Camacho, K. Tollefson, Catalina Espinoza, H. León Vargas, H. A. Ayala Solares, J. A. Morales-Soto, Segev BenZvi, A. Galván-Gámez, Luis Villaseñor, Sabrina Casanova, V. Joshi, K. Malone, K. P. Arunbabu, Kwok Lung Fan, D. Garcia, S. Hernandez, U. Cotti, Arnulfo Zepeda, E. De la Fuente, S. S. Marinelli, D. Avila Rojas, E. Belmont-Moreno, Mehr Nisa, Nicola Omodei, H. Schoorlemmer, Andrea Albert, J. P. Harding, F. Garfias, M. Newbold, A. Iriarte, J. D. Álvarez, E. Tabachnick, P. Surajbali, Meghan Tanner, A. J. Smith, B. Hona, C. De León, M. Fernández Alonso, T. Capistrán, P. Miranda-Romagnoli, A. Sandoval, G. Luis-Raya, R. W. Ellsworth, Michael Schneider, Jose Andres Garcia-Gonzalez, E. Ruiz-Velasco, S. Coutiño de León, C. Brisbois, M. Mostafá, Y. Pérez Araujo, J. C. Díaz-Vélez, R. W. Springer, Daniel Rosa-Gonzalez, Amid Nayerhoda, T. Weisgarber, Brenda Dingus, Maria Magdalena González, Nissim Fraija, G. Sinnis, Ke Fang, H. Salazar, Lukas Nellen, Hongyan Zhou, J.C. Arteaga-Velázquez, Michael DuVernois, A. Carramiñana, I. Torres, Gwenael Giacinti, F. Ureña-Mena, Filiberto Hueyotl-Zahuantitla, J. Serna Franco, I. Martinez-Castellanos, C. Alvarez, K. Engel, Ruben Alfaro, C. D. Rho, F. Salesa Greus, A. L. Longinotti, W. H. Lee, A. Peisker, L. Diaz-Cruz, D. Huang, J. Cotzomi, J. Martínez-Castro, O. Tibolla, Henrike Fleischhack, J. Hinton, J. Lundeen, Vardan Baghmanyan, John Matthews, Oscar Martinez, and HAWC Collaboration

Subjects
HAWC - Abteilung Hinton, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Hydrogen compounds, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Lower limit, Galaxy, Space and Planetary Science, Observatory, 0103 physical sciences, Supernova remnant, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences
Abstract

We present the detection of VHE gamma-ray emission above 100 TeV from HAWC J2227+610 with the HAWC observatory. Combining our observations with previously published results by VERITAS, we interpret the gamma-ray emission from HAWC J2227+610 as emission from protons with a lower limit in their cutoff energy of 800 TeV. The most likely source of the protons is the associated supernova remnant G106.3+2.7, making it a good candidate for a Galactic PeVatron. However, a purely leptonic origin of the observed emission cannot be excluded at this time., Accepted for publication by ApJL

Published
2020

43. An Analysis and Comparison of Three Theoretical Models of the Reading-Writing Relationships in Spanish-Speaking Children

Author

Juan Andrés Hernández-Cabrera, Eduardo García, Juan E. Jiménez, Francisco Naranjo, and Sara C. de León

Subjects
education.field_of_study, media_common.quotation_subject, Population, Theoretical models, Nature based, Spanish speaking, Structural equation modeling, Linguistics, Reading (process), Learning to read, education, Psychology, Orthography, media_common
Abstract

In this chapter we present a comparison and evaluation of three alternative theoretical models of the reading-writing relationship through structural equation modeling of a Spanish-speaking school population: (a) a reading-writing model which postulates that reading has a direct influence on writing); (b) a writing-reading model which postulates that reading is influenced by writing and; (c) an interactive model which postulates that both skills are influenced reciprocally. Previous studies have been conducted in a language with opaque orthography as English. English, being an opaque language, has many inconsistencies in the grapheme-phoneme correspondences and vice versa; however, the Spanish is a language more regular and consistent. Therefore, the explanatory models on the relationship between reading and writing in languages with opaque orthography should not be extrapolated directly to languages with transparent orthography. So far, we have no studies of this nature in our language. Taking into account our findings, the chapter concludes by suggesting that the flow of information between reading and writing may be of a more universal nature based in the alphabetic systems.

Published
2020

44. HAWC and Fermi-LAT Detection of Extended Emission from the Unidentified Source 2HWC J2006+341

Author

E. Moreno, Nissim Illich Fraija, Nicola Omodei, Pedro Miranda-Romagnoli, Alison Peisker, Arturo Iriarte, L. Nellen, Henrike Fleischhack, Fernando Ureña-Mena, C. Alvarez, Andrea Albert, F. Salesa Greus, Mora Durocher, Petra Hüntemeyer, A. Zepeda, D. Garcia, R. W. Springer, Mehr Nisa, C. Brisbois, H. Zhou, Miguel Mostafa, E. G. Pérez-Pérez, E. De la Fuente, John Matthews, D. Avila Rojas, K. P. Arunbabu, Michael DuVernois, Ibrahim Torres, V. Joshi, A. Galván-Gámez, C. De León, Jose Andres Garcia-Gonzalez, R. Torres-Escobedo, R. Diaz Hernandez, K. Malone, Miguel Araya, A. Carraminana, V. Baghmanyan, Brenda Dingus, Karen S. Caballero-Mora, Catalina Espinoza, R. López-Coto, Anna Lia Longinotti, Jesús Martínez-Castro, Joe Lundeen, H. A. Ayala Solares, K. Tollefson, O. Martinez, A. Jardin-Blicq, Ruben Alfaro, Gilgamesh Luis-Raya, Juan Carlos Diaz-Velez, J. R. Angeles Camacho, Umberto Cotti, Daniel Rosa-Gonzalez, Sabrina Casanova, R. Noriega-Papaqui, J. T. Linnemann, Dezhi Huang, J. C. Arteaga-Velázquez, B. Hona, J. A. Goodman, Fernando Garfias, Maria Magdalena González, Ernesto Belmont-Moreno, Filiberto Hueyotl-Zahuantitla, H. León Vargas, A. Sandoval, Michael Schneider, Elijah Willox, J. P. Harding, C. D. Rho, T. Weisgarber, and Luis Villaseñor

Subjects
Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Interstellar medium, Space and Planetary Science, 0103 physical sciences, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, Fermi Gamma-ray Space Telescope
Abstract

The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best described by an extended source with a soft spectrum. At GeV energies, an extended source is significantly detected in Fermi-LAT data. The matching locations, sizes and spectra suggest that both gamma-ray detections correspond to the same source. Different scenarios for the origin of the emission are considered and we rule out an association to the pulsar PSR J2004+3429 due to extreme energetics required, if located at a distance of 10.8 kpc., Comment: 12 pages, 2 figures. To appear in ApJL

Published
2020
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45. Constraining the local burst rate density of primordial black holes with HAWC

Author

E. G. Pérez-Pérez, U. Cotti, S. Hernandez, A. J. Smith, T. Capistrán, J.C. Arteaga-Velázquez, K. Malone, W. H. Lee, J. Cotzomi, E. Tabachnick, R. Noriega-Papaqui, E. Belmont-Moreno, A. Iriarte, Joe Lundeen, B. Hona, S. S. Marinelli, Lukas Nellen, Hao Zhou, Alejandro Lara, G. Sinnis, Michael DuVernois, F. Garfias, I. Torres, A. Carramiñana, K. Tollefson, J. Martínez-Castro, Mehr Nisa, C. D. Rho, J. C. Díaz-Vélez, Nissim Fraija, O. Tibolla, C. De León, I. Martinez-Castellanos, E. De la Fuente, Karen S. Caballero-Mora, G. Luis-Raya, R. W. Ellsworth, H. Fleischhack, R. López-Coto, K. Engel, F. Salesa Greus, C. Brisbois, Jose Andres Garcia-Gonzalez, R. W. Springer, A. Galván-Gámez, Sabrina Casanova, H. Martínez-Huerta, V. Joshi, Brenda Dingus, Catalina Espinoza, John N. Wood, H. Salazar, Segev BenZvi, C. Alvarez, Vardan Baghmanyan, A. L. Longinotti, Alison Peisker, John Matthews, K. P. Arunbabu, Oscar Martinez, D. Avila Rojas, H. A. Ayala Solares, Daniel Rosa-Gonzalez, Amid Nayerhoda, Andrea Albert, M. Newbold, M. J. F. Rosenberg, Meghan Tanner, P. Miranda-Romagnoli, P. Hüntemeyer, R. Torres-Escobedo, J. P. Harding, C. Rivière, J. T. Linnemann, Maria Magdalena González, A. Sandoval, J. A. Goodman, Michael Schneider, H. León Vargas, Dezhi Huang, J. A. Morales-Soto, M. Mostafá, Filiberto Hueyotl-Zahuantitla, T. Weisgarber, Arnulfo Zepeda, Ruben Alfaro, and E. Moreno

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Solar mass, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Gamma ray, FOS: Physical sciences, Astronomy and Astrophysics, Primordial black hole, Astrophysics, Universe, High Energy Physics - Experiment, 85-05, Black hole, High Energy Physics - Experiment (hep-ex), RAIOS GAMA, Observatory, Astrophysics - High Energy Astrophysical Phenomena, Cherenkov radiation, Hawking radiation, media_common
Abstract

Primordial Black Holes (PBHs) may have been created by density fluctuations in the early Universe and could be as massive as $> 10^9$ solar masses or as small as the Planck mass. It has been postulated that a black hole has a temperature inversely-proportional to its mass and will thermally emit all species of fundamental particles via Hawking Radiation. PBHs with initial masses of $\sim 5 \times 10^{14}$ g (approximately one gigaton) should be expiring today with bursts of high-energy gamma radiation in the GeV--TeV energy range. The High Altitude Water Cherenkov (HAWC) Observatory is sensitive to gamma rays with energies of $\sim$300 GeV to past 100 TeV, which corresponds to the high end of the PBH burst spectrum. With its large instantaneous field-of-view of $\sim 2$ sr and a duty cycle over 95%, the HAWC Observatory is well suited to perform an all-sky search for PBH bursts. We conducted a search using 959 days of HAWC data and exclude the local PBH burst rate density above $3400~\mathrm{pc^{-3}~yr^{-1}}$ at 99% confidence, the strongest limit on the local PBH burst rate density from any existing electromagnetic measurement., Corresponding authors: K.L. Engel & A. Peisker. 13 pages, 5 figures

Published
2020

46. Assessing Foundational Reading Skills in Kindergarten: A Curriculum-Based Measurement in Spanish

Author

Nuria Gutiérrez, Sara C. de León, Juan E. Jiménez, and Rocío C. Seoane

Subjects
Male, Health (social science), Response to intervention, media_common.quotation_subject, education, 050109 social psychology, Logistic regression, Education, Dyslexia, Predictive Value of Tests, Reading (process), Humans, 0501 psychology and cognitive sciences, Longitudinal Studies, Child, Curriculum, media_common, Medical education, Psycholinguistics, Receiver operating characteristic, Phonemic awareness, 05 social sciences, 050301 education, Comprehension, Curriculum-based measurement, Reading, Spain, Child, Preschool, General Health Professions, Female, Educational Measurement, Psychology, 0503 education
Abstract

Early identification of learning difficulties is a critical component of the Response to Intervention (RtI) model. In kindergarten, the screening of foundational reading skills can provide a data-based guideline for identifying students requiring a more intensive response-based intervention before starting elementary school. This study examines the classification accuracy and best predictors of a set of Spanish curriculum-based measures administered during kindergarten. The study’s sample included 189 students tested in the fall, winter, and spring. Receiver operating characteristic (ROC) analysis was conducted. The composite score of the curriculum-based measurement (CBM) revealed area under the ROC curve (AUC) values of 0.83, 0.97, and 0.94 in the fall, winter, and spring, respectively. Phonemic awareness and letter-sound knowledge were the only isolated measures that demonstrated excellent AUC values throughout kindergarten. Logistic regression models showed that, when entered simultaneously, all measures were significant predictors of reading risk at some moment of the school year.

Published
2019

47. Data acquisition architecture and online processing system for the HAWC gamma-ray observatory

Author

Jorge Cotzomi, P. Karn, Fernando Garfias, M. Longo Proper, Anushka Udara Abeysekara, Petra Hüntemeyer, Thomas Weisgarber, J. P. Harding, T. Yapici, F. Salesa Greus, Alberto Carramiñana, A. Imran, Ruben Alfaro, H. León Vargas, Daniel Rosa-Gonzalez, T. N. Ukwatta, Varlen Grabski, R. Arceo, Pedro Miranda-Romagnoli, M. Bonilla Rosales, Michael Newbold, A. J. Smith, O. Martinez, Michael DuVernois, Nissim Illich Fraija, James E. Braun, E. De la Fuente, R. Noriega-Papaqui, R. A. Caballero-Lopez, J. C. Arteaga-Velázquez, Gerd Joachim Kunde, D. Berley, N. Bautista-Elivar, James M. Ryan, A. Sandoval, G. Sinnis, J. Becerra González, L. Nellen, William H. Lee, J. Pretz, S. S. Marinelli, E. Mendoza Torres, James W. Wood, Kelly Malone, C. M. Hui, Hao Zhou, C. De León, Umberto Cotti, H. Martínez-Huerta, Julie McEnery, Michael Schneider, I. G. Wisher, Edna Ruiz-Velasco, R. W. Springer, E. G. Pérez-Pérez, Tyce DeYoung, P. A. Toale, I. Taboada, K. Sparks Woodle, C. Alvarez, Rodrigo Pelayo, E. C. Linares, J. A.J. Matthews, A. Marinelli, A. Zepeda, David Kieda, S. Westerhoff, F. E. Sanchez, M. Castillo, Humberto Ibarguen Salazar, Juan Carlos Diaz-Velez, P. W. Younk, D. W. Fiorino, Dirk Lennarz, E. Moreno, J. D. Álvarez, Maria Magdalena González, Arturo Iriarte, T. Oceguera-Becerra, R. J. Lauer, A. Galindo, Karen S. Caballero-Mora, Jesús Martínez-Castro, H. A. Ayala Solares, K. Tollefson, Alejandro Lara, Z. Hampel-Arias, R. Diaz Hernandez, Ibrahim Torres, D. Zaborov, J. T. Linnemann, G. B. Yodh, A. S. Barber, R. W. Ellsworth, S. Silich, B. M. Baughman, C. Rivière, L. Villaseñor, J. A. Goodman, Ernesto Belmont-Moreno, Miguel Mostafa, Segev BenZvi, J. Diaz-Cruz, M. Gussert, B. Patricelli, Brenda Dingus, and R. Luna-Garcia

Subjects
Physics, Nuclear and High Energy Physics, business.industry, Gigabit Ethernet, Electrical engineering, FOS: Physical sciences, Dead time, 01 natural sciences, Data processing system, Time-to-digital converter, Air shower, Data acquisition, Observatory, 0103 physical sciences, Custom software, Astrophysics - Instrumentation and Methods for Astrophysics, 010306 general physics, business, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Instrumentation, Computer hardware
Abstract

The High Altitude Water Cherenkov observatory (HAWC) is an air shower array devised for TeV gamma-ray astronomy. HAWC is located at an altitude of 4100 m a.s.l. in Sierra Negra, Mexico. HAWC consists of 300 Water Cherenkov Detectors, each instrumented with 4 photomultiplier tubes (PMTs). HAWC re-uses the Front-End Boards from the Milagro experiment to receive the PMT signals. These boards are used in combination with Time to Digital Converters (TDCs) to record the time and the amount of light in each PMT hit (light flash). A set of VME TDC modules (128 channels each) is operated in a continuous (dead time free) mode. The TDCs are read out via the VME bus by Single-Board Computers (SBCs), which in turn are connected to a gigabit Ethernet network. The complete system produces ~ 500 MB/s of raw data. A high-throughput data processing system has been designed and built to enable real-time data analysis. The system relies on off-the-shelf hardware components, an open-source software technology for data transfers (ZeroMQ) and a custom software framework for data analysis (AERIE). Multiple trigger and reconstruction algorithms can be combined and run on blocks of data in a parallel fashion, producing a set of output data streams which can be analyzed in real time with minimal latency (< 5 s). This paper provides an overview of the hardware set-up and an in-depth description of the software design, covering both the TDC data acquisition system and the real-time data processing system. The performance of these systems is also discussed., 14 pages, 3 figures, submitted to Nucl. Instrum. Meth. A

Published
2018

48. Author Correction: HAWC observations of the acceleration of very-high-energy cosmic rays in the Cygnus Cocoon

Author

A. Jardin-Blicq, J. A. Morales-Soto, Juan Carlos Diaz-Velez, A. Sandoval, Mora Durocher, D. Garcia, C. Alvarez, E. De la Fuente, F. Werner, D. Avila Rojas, F. Serna, J. R. Angeles Camacho, Kwok Lung Fan, Petra Hüntemeyer, J. C. Arteaga-Velázquez, Michael Schneider, R. Diaz Hernandez, S. Hernandez, Nicola Omodei, Arturo Iriarte, K. Tollefson, B. Hona, Gilgamesh Luis-Raya, C. De León, V. Baghmanyan, E. Moreno, C. Brisbois, Umberto Cotti, Maria Magdalena González, Kristi Engel, Nissim Illich Fraija, Sabrina Casanova, Fernando Garfias, A. Zepeda, Harm Schoorlemmer, Pooja Surajbali, J. A. Matthews, E. Ruiz-Velasco, Humberto Ibarguen Salazar, H. Zhou, Fernando Ureña-Mena, Alison Peisker, Z. Ren, Ibrahim Torres, R. Noriega-Papaqui, Filiberto Hueyotl-Zahuantitla, K. P. Arunbabu, Ruben Alfaro, A. L. Longinotti, H. León Vargas, J. P. Harding, Henrike Fleischhack, William H. Lee, L. Olivera-Nieto, O. Martinez, T. Weisgarber, Daniel Rosa-Gonzalez, Miguel Mostafa, Michael DuVernois, Anushka Udara Abeysekara, Roger Blandford, S. Coutiño de León, R. W. Springer, Jose Andres Garcia-Gonzalez, Michael Newbold, Alejandro Lara, K. Malone, E. G. Pérez-Pérez, V. Joshi, J. D. Álvarez, E. Belmont-Moreno, A. J. Smith, Ke Fang, C. D. Rho, T. Capistrán, David Kieda, L. Nellen, F. Salesa Greus, A. Carraminana, Joe Lundeen, R. W. Ellsworth, Jim Hinton, Elijah Willox, J. A. Goodman, Dezhi Huang, Pedro Miranda-Romagnoli, M. U. Nisa, A. Galván-Gámez, Brenda Dingus, J. T. Linnemann, Y. Pérez Araujo, A. Nayerhoda, Segev BenZvi, Gwenael Giacinti, I. Martinez-Castellanos, Andrea Albert, R. Torres-Escobedo, Karen S. Caballero-Mora, Catalina Espinoza, Jesús Martínez-Castro, and H. A. Ayala Solares

Subjects
Physics, Acceleration, Astronomy and Astrophysics, Astrophysics, Ultra-high-energy cosmic ray
Published
2021

49. Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC

Author

J. C. Arteaga-Velázquez, Karen S. Caballero-Mora, S. Hernandez, A. Carraminana, Maria Magdalena González, Z. Ren, Filiberto Hueyotl-Zahuantitla, Dezhi Huang, Catalina Espinoza, J. Pretz, Joe Lundeen, Miguel Mostafa, Gilgamesh Luis-Raya, John Matthews, Jesús Martínez-Castro, R. W. Ellsworth, H. A. Ayala Solares, J. A. Morales-Soto, Tomás Capistrán, S. S. Marinelli, C. Brisbois, Haocheng Zhang, V. Joshi, Luis Villaseñor, Ruben Alfaro, C. Rivière, R. W. Springer, Ibrahim Torres, Anushka Udara Abeysekara, Fernando Garfias, Michael Newbold, Daniel Rosa-Gonzalez, E. G. Pérez-Pérez, A. Nayerhoda, Thomas Weisgarber, A. Galván-Gámez, S. Coutiño de León, E. Ruiz-Velasco, S. Kaufmann, Hao Zhou, Segev BenZvi, J. A. Goodman, Alejandro Lara, Chang Dong Rho, Alison Peisker, Pedro Miranda-Romagnoli, H. León Vargas, E. Moreno, Kristi Engel, Umberto Cotti, Ernesto Belmont-Moreno, K. P. Arunbabu, David Kieda, Jim Hinton, J C Díaz-Vélez, Brenda Dingus, R. López-Coto, Andrea Albert, Henrike Fleischhack, Sabrina Casanova, A. Sandoval, Jorge Cotzomi, R. Torres-Escobedo, Arturo Iriarte, Anna Lia Longinotti, Kelly Malone, Meghan Tanner, Michael Schneider, Harm Schoorlemmer, E. Tabachnick, Nissim Illich Fraija, R. Noriega-Papaqui, M. U. Nisa, O. Tibolla, J. T. Linnemann, William H. Lee, D. Garcia, J. P. Harding, Binita Hona, O. Martinez, I. Martinez-Castellanos, K. Tollefson, Pooja Surajbali, Gus Sinnis, J. Wood, J. R. Angeles Camacho, T. Yapici, H. Martínez-Huerta, Jose Andres Garcia-Gonzalez, Petra Hüntemeyer, E. De la Fuente, D. Avila Rojas, A. J. Smith, L. Nellen, V. Baghmanyan, C. De León, Armelle Jardin-Blicq, Michael DuVernois, F. Salesa Greus, M. J. F. Rosenberg, Simone Dichiara, and HAWC Collaboration

Subjects
Physics, HAWC - Abteilung Hinton, High Energy Astrophysical Phenomena (astro-ph.HE), Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, General Physics and Astronomy, Flux, Astronomy, FOS: Physical sciences, ASTROFÍSICA, Effects of high altitude on humans, 01 natural sciences, Spectral line, Observatory, 0103 physical sciences, 010306 general physics, Astrophysics - High Energy Astrophysical Phenomena, Cherenkov radiation
Abstract

We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov (HAWC) Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV. Nine sources are observed above 56 TeV, all of which are likely Galactic in origin. Three sources continue emitting past 100 TeV, making this the highest-energy gamma-ray source catalog to date. We report the integral flux of each of these objects. We also report spectra for three highest-energy sources and discuss the possibility that they are PeVatrons., Accepted by Physical Review Letters

Published
2019

50. Constraints on Lorentz invariance violation from HAWC observations of gamma rays above 100 TeV

Author

Maria Magdalena González, Filiberto Hueyotl-Zahuantitla, J. A. Morales-Soto, Gilgamesh Luis-Raya, C. De León, O. Tibolla, G. B. Yodh, Chang Dong Rho, Michael Newbold, H. Martínez-Huerta, Alison Peisker, Pooja Surajbali, Anna Lia Longinotti, Gus Sinnis, V. Baghmanyan, Ibrahim Torres, A. Nayerhoda, A. Sandoval, K. Tollefson, J. R. Angeles Camacho, A. Zepeda, A. J. Smith, Hao Zhou, Henrike Fleischhack, F. Salesa Greus, E. Moreno, Ernesto Belmont-Moreno, A. Carraminana, M. J. F. Rosenberg, Michael Schneider, Joe Lundeen, L. Nellen, S. Hernandez, Humberto Ibarguen Salazar, K. P. Arunbabu, R. López-Coto, Petra Hüntemeyer, Binita Hona, Nicola Omodei, S. Coutiño de León, R. W. Ellsworth, Chad Brisbois, Michael DuVernois, Arturo Iriarte, D. Garcia, Kristi Engel, Alejandro Lara, Andrea Albert, C. Alvarez, K. Malone, R. Torres-Escobedo, M. U. Nisa, V. Joshi, Segev BenZvi, C. Rivière, Meghan Tanner, John Matthews, Harm Schoorlemmer, E. Tabachnick, Pedro Miranda-Romagnoli, R. Noriega-Papaqui, J. A. Goodman, E. De la Fuente, D. Avila Rojas, Jose Andres Garcia-Gonzalez, William H. Lee, Nissim Illich Fraija, Dezhi Huang, Karen S. Caballero-Mora, J. P. Harding, Catalina Espinoza, Ruben Alfaro, Tomás Capistrán, Jesús Martínez-Castro, H. A. Ayala Solares, Daniel Rosa-Gonzalez, S. S. Marinelli, R. W. Springer, Jorge Cotzomi, A. Galván-Gámez, E. G. Pérez-Pérez, Brenda Dingus, Juan Carlos Diaz-Velez, I. Martinez-Castellanos, Umberto Cotti, Sabrina Casanova, J. T. Linnemann, Fernando Garfias, Thomas Weisgarber, E. Ruiz-Velasco, H. León Vargas, and J. C. Arteaga-Velázquez

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Photon, Planck energy, Superluminal motion, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, General Physics and Astronomy, ASTROFÍSICA, Astrophysics, Lorentz covariance, 01 natural sciences, symbols.namesake, Orders of magnitude (time), Observatory, 0103 physical sciences, symbols, 010306 general physics, Astrophysics - High Energy Astrophysical Phenomena, Cherenkov radiation
Abstract

Due to the high energies and long distances to the sources, astrophysical observations provide a unique opportunity to test possible signatures of Lorentz invariance violation (LIV). Superluminal LIV enables the decay of photons at high energy. The High Altitude Water Cherenkov (HAWC) Observatory is among the most sensitive gamma-ray instruments currently operating above 10 TeV. HAWC finds evidence of 100 TeV photon emission from at least four astrophysical sources. These observations exclude, for the strongest of the limits set, the LIV energy scale to $2.2\times10^{31}$ eV, over 1800 times the Planck energy and an improvement of 1 to 2 orders of magnitude over previous limits., Accepted for publication in Physical Review Letters

Published
2019

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