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5. 240P Effect of dose intensity (DI) of palbociclib (PAB) and initial body weight dosage (BWD) on progression free survival (PFS): A real-world data analysis in patients with hormone-receptor (HR) positive HER2 negative metastatic breast cancer (MBC)

Author

Penabad, S. Recalde, Fort, E., Otero, S., Lezcano, C., Gil, V.L. Obadia, Sabaté, N., Juher, H. Pla, Falgas, E. Felip, Vila, M. Margeli, Villaro, G. Vinas, Gomez, A.M. Esteve, Rey, M., Simon, S. Pernas, and Fontanals, S.

Published
2023
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6. V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?

Author

Harmanec, P., Božić, H., Koubský, P., Yang, S., Ruždjak, D., Sudar, D., Šlechta, M., Wolf, M., Korčáková, D., Zasche, P., Oplištilová, A., Vršnak, D., Ak, H., Eenens, P., Bakiş, H., Bakiş, V., Otero, S., Chini, R., Demsky, T., Barlow, B.N., Svoboda, P., Jonák, J., Vitovský, K., and Harmanec, A.

Subjects
binaries: spectroscopic, stars: emission-line, Be, stars: fundamental parameters, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics::Solar and Stellar Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics, Solar and Stellar Astrophysics (astro-ph.SR)
Abstract

A reliable determination of the basic physical properties and variability patterns of hot emission-line stars is important for understanding the Be phenomenon and ultimately, the evolutionary stage of Be stars. This study is devoted to one of the most remarkable Be stars, V1294 Aql = HD 184279. We collected and analysed spectroscopic and photometric observations covering a time interval of about 25000 d (68 yr). We present evidence that the object is a single-line 192.9 d spectroscopic binary and estimate that the secondary probably is a hot compact object with a mass of about 1.1-1.2 solar masses. We found and documented very complicated orbital and long-term spectral, light, and colour variations, which must arise from a combination of several distinct variability patterns. Attempts at modelling them are planned for a follow-up study. We place the time behaviour of V1294 Aql into context with variations known for some other systematically studied Be stars and discuss the current ideas about the nature of the Be phenomenon., Comment: 15 pages, 15 figures, accepted for publication in Astronomy and Astrophysics

Published
2022

7. Rethinking the 'one-stop' neck lump clinic: a novel pathway beyond coronavirus disease 2019.

Author

Hariri, A, Jawad, S, Otero, S, Lechner, M, Morley, S, Beale, T, Hughes, J, Stimpson, P, Dwivedi, R, and Vaz, F

Subjects
HEAD & neck cancer, MEDICAL care, UNNECESSARY surgery, CANCER patients, MEDICAL care use, MEDICAL referrals, MEDICAL appointments, COVID-19 pandemic, CANCER patient medical care
Abstract

Objectives: UK guidelines advocate 'one-stop' neck lump assessment for cancer referrals. This paper reports the pilot of a novel pre-clinic ultrasound pathway, presents outcomes, and discusses strengths and limitations in the context of the coronavirus disease 2019 pandemic. Methods: Two-week-wait cancer referral patients with a neck lump were allocated a pre-clinic ultrasound scan followed by a clinic appointment. Demographic, patient journey and outcome data were collected and analysed. Results: Ninety-nine patients underwent ultrasound assessment with or without biopsy on average 8 days following referral. Patients were followed up on average 14.1 days (range, 2–26 days) after initial referral. At the first clinic appointment, 45 patients were discharged, 10 were scheduled for surgery, 12 were diagnosed with cancer, 6 were referred to another specialty and cancer was excluded in 19 patients. Retrospectively, four ultrasounds were performed unnecessarily. Conclusion: Pre-clinic ultrasound scanning is an alternative to the one-stop neck lump pathway. This study demonstrates fewer clinic visits, faster diagnosis and a low proportion of unnecessary scans, whilst minimising face-to-face consultations and aerosol-generating procedures. [ABSTRACT FROM AUTHOR]

Published
2023
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9. PHYSICAL ACTIVITY IN YOUNG CHILEAN WOMEN DURING COVID-19 LOCKDOWN.

Author

Saavedra, E. and Otero, S.

Subjects
PHYSICAL activity, COVID-19 pandemic, CHILEANS
Abstract

Copyright of International Journal of Medicine & Science of Physical Activity & Sport / Revista Internacional de Medicina y Ciencias de la Actividad Física y del Deporte is the property of Revista Internacional de Medicina y Ciencias de la Actividad Fisica y del Deporte and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Published
2022
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20. LHCb silicon tracker performance studies

Author

Kostner, S., Adeva, B., Agari, M., Bauer, C., Baumeister, D., Bay, A., Bernhard, R.P., Bernet, R., Blouw, J., Carron, B., Ermoline, Y., Esperante, D., Frei, R., Gassner, J., Hofmann, W., Jimenez-Otero, S., Knopfle, K.T., Lehner, F., Lochner, S., Lois, C., Needham, M., Perron, A., Pugatch, V., Schmelling, M., Schwingenheuer, B., Siegler, M., Steinkamp, O., Straumann, U., Tran, M.T., Vazques, P., Vollhardt, A., Volyanski, D., and Voss, H.

Subjects
Chemical detectors -- Usage, Chemical detectors -- Analysis, Pitch (Bituminous material) -- Analysis, Silicon diodes -- Analysis, Silicon diodes -- Properties, Business, Electronics, Electronics and electrical industries
Abstract

LHCb is one of the experiments for the Large Hadron Collider at CERN and is dedicated to B-physics and CP-violation measurements. To exploit its physics potential good tracking performance with high efficiency in a high particle density environment close to the beam pipe is required. Silicon strip detectors with large read-out pitch and long strips will be used for the LHCb Inner Tracker behind the magnet and the Trigger Tracker station in front of the magnet. We report here about the design of the Silicon Tracker, test beam results and the electrical tests foreseen during production. Index Terms--Large read-out pitch, long read-out strips, silicon-microstrip detector, silicon tracker, tracking detector.

Published
2006

25. The LHCb Silicon Tracker Project

Author

Agari, M., Bauer, C., Baumeister, D., Blouw, J., Hofmann, W., Knöpfle, K.T., Löchner, S., Schmelling, M., Pugatch, V., Bay, A., Carron, B., Frei, R., Jiminez-Otero, S., Tran, M.-T., Voss, H., Adeva, B., Esperante, D., Lois, C., Vasquez, P., Bernhard, R.P., Bernet, R., Ermoline, Y., Gassner, J., Köstner, S., Lehner, F., Needham, M., Siegler, M., Steinkamp, O., Straumann, U., Vollhardt, A., and Volyanskyy, D.

Published
2006
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28. The LHCb silicon tracker

Author

Adeva, B., Agari, M., Bauer, C., Baumeister, D., Bay, A., Bernhard, R.P., Bernet, R., Blouw, J., Carron, B., Ermoline, Y., Esperante, D., Frei, R., Gassner, J., Hofmann, W., Jimenez-Otero, S., Knöpfle, K.T., Köstner, S., Lehner, F., Löchner, S., Lois, C., Needham, M., Pugatch, V., Schmelling, M., Schwingenheuer, B., Siegler, M., Steinkamp, O., Straumann, U., Tran, M.T., Vazquez, P., Vollhardt, A., Volyanskyy, D., and Voss, H.

Published
2005
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30. Possible evidence for a magnetic dynamo in hot Algols.

Author

Mennickent, R. E., Garcés, J., Djurašević, G., Rojas, G., Schleicher, D., Otero, S., Kosovichev, Alexander, Strassmeier, Klaus, and Jardine, Moira

Abstract

We present the case of hot semi-detached Algols showing photometric cycles longer than the orbital period. The evidence indicating that this long cycle might be due to a magnetic dynamo operating in the rapidly rotating donor star is examined. [ABSTRACT FROM AUTHOR]

Published
2021
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31. The ASAS-SN catalogue of variable stars IX: The spectroscopic properties of Galactic variable stars.

Author

Jayasinghe, T, Kochanek, C S, Stanek, K Z, Shappee, B J, Holoien, T W-S, Thompson, Todd A, Prieto, J L, Dong, Subo, Pawlak, M, Pejcha, O, Pojmanski, G, Otero, S, Hurst, N, and Will, D

Subjects
VARIABLE stars, GIANT stars, ECLIPSING binaries, LIGHT curves, STELLAR rotation, RED giants
Abstract

The All-Sky Automated Survey for Supernovae provides long baseline (∼4 yr) V - band light curves for sources brighter than V≲ 17 mag across the whole sky. We produced V - band light curves for a total of ∼61.5 million sources and systematically searched these sources for variability. We identified ∼426 000 variables, including ∼219 000 new discoveries. Most (⁠|${\sim }74{ per\ cent}$|⁠) of our discoveries are in the Southern hemisphere. Here, we use spectroscopic information from LAMOST, GALAH, RAVE, and APOGEE to study the physical and chemical properties of these variables. We find that metal-poor eclipsing binaries have orbital periods that are shorter than metal-rich systems at fixed temperature. We identified rotational variables on the main-sequence, red giant branch, and the red clump. A substantial fraction (⁠|${\gtrsim }80{ per\ cent}$|⁠) of the rotating giants have large |$v$| rot or large near-ultraviolet excesses also indicative of fast rotation. The rotational variables have unusual abundances suggestive of analysis problems. Semiregular variables tend to be lower metallicity (⁠|$\rm [Fe/H]{\sim }-0.5$|⁠) than most giant stars. We find that the APOGEE DR16 temperatures of oxygen-rich semiregular variables are strongly correlated with the W RP − W JK colour index for |$\rm T_{eff}\lesssim 3800$|  K. Using abundance measurements from APOGEE DR16, we find evidence for Mg and N enrichment in the semiregular variables. We find that the Aluminum abundances of the semiregular variables are strongly correlated with the pulsation period, where the variables with |$\rm P\gtrsim 60$|  d are significantly depleted in Al. [ABSTRACT FROM AUTHOR]

Published
2021
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32. Circulating metabolic biomarkers of renal function in diabetic and non-diabetic populations

Author

Barrios, C., Zierer, J., Würtz, P., Haller, T., Metspalu, A., Gieger, C., Thorand, B., Meisinger, C., Waldenberger, M., Raitakari, O., Lehtimäki, T., Otero, S., Rodríguez, E., Pedro-Botet, J., Kähönen, M., Ala-Korpela, M., Kastenmüller, G., Spector, T.D., Pascual, J., Menni, C., Research Programs Unit, Diabetes and Obesity Research Program, and University of Helsinki

Subjects
CHRONIC KIDNEY-DISEASE, Male, lcsh:Medicine, Kidney, Kidney Function Tests, Article, Cohort Studies, MELLITUS, MAGNETIC-RESONANCE METABOLOMICS, HDL PHOSPHOLIPID CONTENT, Humans, AMINO-ACIDS, Diabetic Nephropathies, ddc:610, Renal Insufficiency, Chronic, CARDIOVASCULAR EVENTS, lcsh:Science, IN-VIVO, Aged, Aged, 80 and over, CHOLESTEROL EFFLUX CAPACITY, PHENYLALANINE, lcsh:R, Middle Aged, Cross-Sectional Studies, Diabetes Mellitus, Type 2, 3121 General medicine, internal medicine and other clinical medicine, Case-Control Studies, COHORT PROFILE, Female, lcsh:Q, 3111 Biomedicine, Biomarkers, Glomerular Filtration Rate
Abstract

Using targeted NMR spectroscopy of 227 fasting serum metabolic traits, we searched for novel metabolic signatures of renal function in 926 type 2 diabetics (T2D) and 4838 non-diabetic individuals from four independent cohorts. We furthermore investigated longitudinal changes of metabolic measures and renal function and associations with other T2D microvascular complications. 142 traits correlated with glomerular filtration rate (eGFR) after adjusting for confounders and multiple testing: 59 in diabetics, 109 in non-diabetics with 26 overlapping. The amino acids glycine and phenylalanine and the energy metabolites citrate and glycerol were negatively associated with eGFR in all the cohorts, while alanine, valine and pyruvate depicted opposite association in diabetics (positive) and nondiabetics (negative). Moreover, in all cohorts, the triglyceride content of different lipoprotein subclasses showed a negative association with eGFR, while cholesterol, cholesterol esters (CE), and phospholipids in HDL were associated with better renal function. In contrast, phospholipids and CEs in LDL showed positive associations with eGFR only in T2D, while phospholipid content in HDL was positively associated with eGFR both cross-sectionally and longitudinally only in non-diabetics. In conclusion, we provide a wide list of kidney function-associated metabolic traits and identified novel metabolic differences between diabetic and non-diabetic kidney disease.

Published
2018

34. The ASAS-SN catalogue of variable stars – VII. Contact binaries are different above and below the Kraft break.

Author

Jayasinghe, T, Stanek, K Z, Kochanek, C S, Shappee, B J, Pinsonneault, M H, Holoien, T W-S, Thompson, Todd A, Prieto, J L, Pawlak, M, Pejcha, O, Pojmanski, G, Otero, S, Hurst, N, and Will, D

Subjects
LIGHT curves, CATALOGS, ANGULAR momentum (Mechanics), VARIABLE stars, ECLIPSING binaries, SUPERNOVAE
Abstract

We characterize |${\sim } 71\, 200$| W Ursae Majoris (UMa) type (EW) contact binaries, including |${\sim } 12\, 600$| new discoveries, using All-Sky Automated Survey for SuperNovae (ASAN-SN) V -band all-sky light curves along with archival data from Gaia , 2MASS, AllWISE, LAMOST, GALAH, RAVE, and APOGEE. There is a clean break in the EW period–luminosity relation at |$\rm \log (\it P/{\rm d})\,{\simeq }\,{\rm -0.30}$|⁠ , separating the longer period, early-type EW binaries from the shorter period, late-type systems. The two populations are even more cleanly separated in the space of period and effective temperature, by |$T_{\rm eff}=6710\,{\rm K}-1760\,{\rm K}\, \log (P/0.5\,{\rm d})$|⁠. Early-type and late-type EW binaries follow opposite trends in T eff with orbital period. For longer periods, early-type EW binaries are cooler, while late-type systems are hotter. We derive period–luminosity relationships in the WJK , V, Gaia DR2 G, J, H, K s, and W 1 bands for the late-type and early-type EW binaries separated by both period and effective temperature, and by period alone. The dichotomy of contact binaries is almost certainly related to the Kraft break and the related changes in envelope structure, winds, and angular momentum loss. [ABSTRACT FROM AUTHOR]

Published
2020
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35. The ASAS-SN catalogue of variable stars VI: an all-sky sample of δ Scuti stars.

Author

Jayasinghe, T, Stanek, K Z, Kochanek, C S, Vallely, P J, Shappee, B J, Holoien, T W-S, Thompson, Todd A, Prieto, J L, Pejcha, O, Fausnaugh, M, Otero, S, Hurst, N, and Will, D

Subjects
ECLIPSING binaries, VARIABLE stars, CATALOGS, LIGHT curves, STARS
Abstract

We characterize an all-sky catalogue of ∼8400 δ Scuti variables in ASAS-SN, which includes ∼3300 new discoveries. Using distances from Gaia DR2, we derive period–luminosity relationships for both the fundamental mode and overtone pulsators in the WJK , V, Gaia DR2 G, J, H, Ks , and W 1 bands. We find that the overtone pulsators have a dominant overtone mode, with many sources pulsating in the second overtone or higher order modes. The fundamental mode pulsators have metallicity-dependent periods, with log10(P) ∼ −1.1 for |$\rm [Fe/H]\lt -0.3$| and log10(P) ∼ −0.9 for |$\rm [Fe/H]\gt 0$|⁠ , which leads to a period-dependent scale height. Stars with |$P\gt 0.100\, \rm d$| are predominantly located close to the Galactic disc (⁠|$\rm |\mathit{ Z}|\lt 0.5\, kpc$|⁠). The median period at a scale height of |$Z\sim 0\, \rm kpc$| also increases with the Galactocentric radius R , from log10(P) ∼ −0.94 for sources with |$R\gt 9\, \rm kpc$| to log10(P) ∼ −0.85 for sources with |$R\lt 7\, \rm kpc$|⁠ , which is indicative of a radial metallicity gradient. To illustrate potential applications of this all-sky catalogue, we obtained 30 min cadence, image subtraction TESS light curves for a sample of 10 fundamental mode and 10 overtone δ Scuti stars discovered by ASAS-SN. From this sample, we identified two new δ Scuti eclipsing binaries, ASASSN-V J071855.62−434247.3 and ASASSN-V J170344.20−615941.2 with short orbital periods of P orb = 2.6096 and 2.5347 d, respectively. [ABSTRACT FROM AUTHOR]

Published
2020
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36. The ASAS-SN catalogue of variable stars – V. Variables in the Southern hemisphere.

Author

Jayasinghe, T, Stanek, K Z, Kochanek, C S, Shappee, B J, Holoien, T W-S, Thompson, T A, Prieto, J L, Dong, S, Pawlak, M, Pejcha, O, Shields, J V, Pojmanski, G, Otero, S, Hurst, N, Britt, C A, and Will, D

Subjects
VARIABLE stars, PULSATING stars, LIGHT curves, ECLIPSING binaries, LIGHT sources, CATALOGS
Abstract

The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline (∼4 yr) light curves for sources brighter than V ≲ 17 mag across the whole sky. As part of our effort to characterize the variability of all the stellar sources visible in ASAS-SN, we have produced ∼30.1 million V -band light curves for sources in the Southern hemisphere using the APASS DR9 (AAVSO Photometric All-Sky Survey Data Release) catalogue as our input source list. We have systematically searched these sources for variability using a pipeline based on random forest classifiers. We have identified |${\sim } 220\, 000$| variables, including |${\sim } 88\, 300$| new discoveries. In particular, we have discovered |${\sim }48\, 000$| red pulsating variables, |${\sim }23\, 000$| eclipsing binaries, ∼2200 δ-Scuti variables, and |${\sim }10\, 200$| rotational variables. The light curves and characteristics of the variables are all available through the ASAS-SN variable stars data base (https://asas-sn.osu.edu/variables). The pre-computed ASAS-SN V -band light curves for all the ∼30.1 million sources are available through the ASAS-SN photometry data base (https://asas-sn.osu.edu/photometry). This effort will be extended to provide ASAS-SN light curves for sources in the Northern hemisphere and for V  ≲ 17 mag sources across the whole sky that are not included in APASS DR9. [ABSTRACT FROM AUTHOR]

Published
2020
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37. SOFIAS – Herramienta para el análisis de ciclo de vida y la calificación ambiental de edificios

Author

Oregi Isasi, X., Tenorio, J. A., Gazulla, C., Zabalza, I., Cambra, D., Leao, S. O., Mabe, L., Otero, S., and Raigosa, J.

Subjects
Building construction, LCA software, rating, environmental product declaration, base de datos, NA1-9428, calificación, edificios, building, Architecture, software acv, database, TH1-9745, declaración ambiental de producto
Abstract

This paper describes the development process of a new software tool, called SOFIAS (Software for a Sustainable Architecture), funded by the Spanish Ministry of Economy and Competitivenes. Following CEN/TC 350 standard on environmental assessment of buildings, the tool aims at assisting building professionals on reducing the life-cycle environmental impact through the design of new buildings and the refurbishment of existing ones. In addition, SOFIAS provides a rating system based on the Life Cycle Assessment (LCA) methodology. This paper explains the innovative aspects of this software, the working methodology and the different type of results that can be obtained using SOFIAS., Este artículo describe el proceso de desarrollo de la nueva herramienta informática SOFIAS (Software de Funciones Integradas para una Arquitectura Sostenible), financiado por el Ministerio de Economía y Competitividad del Gobierno de España. En base al estandar de la evaluación ambiental de los edificios definido por el CEN/TC 350, esta nueva herramienta tiene como objetivo ayudar a los técnicos de la construcción en reducir el impacto ambiental durante el ciclo de vida a través del diseño optimizado de nuevos edificios o edificios rehabilitados. De forma paralela, SOFIAS proporciona un nuevo sistema de calificación basado en la metodología del Análisis de Ciclo de Vida (ACV). Este artículo expone los aspectos innovadores de esta herramienta informática, la metodología de trabajo y los diferentes tipos de resultados que se pueden obtener tras su aplicación.

Published
2016
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38. Modeling the Complete Lightcurve of omega CMa

Author

Ghoreyshi, M. R., Carciofi, A. C., Rimulo, L. R., Otero, S., Baade, D., Bjorkman, J. E., Okazaki, A. T., and Rivinius, Th.

Subjects
Astrophysics - Solar and Stellar Astrophysics, FOS: Physical sciences, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics
Abstract

We have used the radiative transfer code HDUST to analyze and interpret the long-term photometric behavior of the Be star omega CMa, considering four complete cycles of disk formation and dissipation. This is the first time in which a full lightcurve of a Be star was investigated and modeled including both disk build-up and dissipation phases. Based on the quite good fit of the observed data we were able to derive the history of stellar mass decretion rates (including long- and short-term changes) during the disk formation and dissipation phases in all four cycles., 4 pages, 4 figures

Published
2015

39. ASAS-SN catalogue of variable stars – II. Uniform classification of 412 000 known variables.

Author

Jayasinghe, T, Stanek, K Z, Kochanek, C S, Shappee, B J, Holoien, T W-S, Thompson, Todd A, Prieto, J L, Dong, Subo, Pawlak, M, Pejcha, O, Shields, J V, Pojmanski, G, Otero, S, Britt, C A, and Will, D

Subjects
LIGHT curves, CLASSIFICATION, CATALOGS, VARIABLE stars, ECLIPSING binaries, SUPERNOVAE
Abstract

The variable stars in the VSX catalogue are derived from a multitude of inhomogeneous data sources and classification tools. This inhomogeneity complicates our understanding of variable star types, statistics, and properties, and it directly affects attempts to build training sets for current (and next) generation all-sky, time-domain surveys. We homogeneously analyse the All-Sky Automated Survey for SuperNovae (ASAS-SN) V -band light curves of |${\sim }412\, 000$| variables from the VSX catalogue. The variables are classified using an updated random forest classifier with an F 1 score of 99.4 per cent and refinement criteria for individual classifications. We have derived periods for |${\sim }52\, 000$| variables in the VSX catalogue that lack a period, and have reclassified |${\sim } 17\, 000$| sources into new broad variability groups with high confidence. We have also reclassified |${\sim } 94\, 000$| known variables with miscellaneous/generic classifications. The light curves, classifications, and a range of properties of the variables are all available through the ASAS-SN Variable Stars Database (https://asas-sn.osu.edu/variables). We also include the V -band light curves for a set of ∼4000 rare variables and transient sources, including cataclysmic variables, symbiotic binaries, and flare stars. [ABSTRACT FROM AUTHOR]

Published
2019
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40. Possible evidence for a magnetic dynamo in hot Algols.

Author

Mennickent, R. E., Garcés, J., Djurašević, G., Rojas, G., Schleicher, D., Otero, S., Kosovichev, Alexander, Strassmeier, Klaus, and Jardine, Moira

Abstract

We present the case of hot semi-detached Algols showing photometric cycles longer than the orbital period. The evidence indicating that this long cycle might be due to a magnetic dynamo operating in the rapidly rotating donor star is examined. [ABSTRACT FROM AUTHOR]

Published
2019
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41. The ASAS-SN catalogue of variable stars III: variables in the southern TESS continuous viewing zone.

Author

Jayasinghe, T, Stanek, K Z, Kochanek, C S, Shappee, B J, Holoien, T W-S, Thompson, Todd A, Prieto, J L, Dong, Subo, Pawlak, M, Pejcha, O, Shields, J V, Pojmanski, G, Otero, S, Hurst, N, Britt, C A, and Will, D

Subjects
LIGHT curves, VARIABLE stars, LIGHT sources, CATALOGS, DATABASES, ECLIPSING binaries
Abstract

The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long-baseline (∼4 yr) light curves for sources brighter than V ≲ 17 mag across the whole sky. The Transiting Exoplanet Survey Satellite (TESS) has started to produce high-quality light curves with a baseline of at least 27 d, eventually for most of the sky. The combination of ASAS-SN and TESS light curves probes both long- and short-term variability in great detail, especially towards the TESS continuous viewing zones (CVZ) at the ecliptic poles. We have produced ∼1.3 million V -band light curves covering a total of |${\sim }1000 \, \rm deg^2$| towards the southern TESS CVZ and have systematically searched these sources for variability. We have identified ∼11 700 variables, including ∼7 000 new discoveries. The light curves and characteristics of the variables are all available through the ASAS-SN variable stars data base (https://asas-sn.osu.edu/variables). We also introduce an online resource to obtain pre-computed ASAS-SN V -band light curves (https://asas-sn.osu.edu/photometry) starting with the light curves of the ∼1.3 million sources studied in this work. This effort will be extended to provide ASAS-SN light curves for ∼50 million sources over the entire sky. [ABSTRACT FROM AUTHOR]

Published
2019
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42. The life cycles of Be viscous decretion discs: The case of ω CMa.

Author

Ghoreyshi, M R, Carciofi, A C, Rímulo, L R, Vieira, R G, Faes, D M, Baade, D, Bjorkman, J E, Otero, S, and Rivinius, Th

Subjects
DISKS (Astrophysics), VISCOSITY, ASTRONOMICAL photometry, MATHEMATICAL models of hydrodynamics, ENERGY dissipation
Abstract

We analysed V-band photometry of the Be star ω CMa, obtained during the last four decades, during which the star went through four complete cycles of disc formation and dissipation. The data were simulated by hydrodynamic models based on a time-dependent implementation of the viscous decretion disc (VDD) paradigm, in which a disc around a fast-spinning Be star is formed by material ejected by the star and driven to progressively larger orbits by means of viscous torques. Our simulations offer a good description of the photometric variability during phases of disc formation and dissipation, which suggests that the VDD model adequately describes the structural evolution of the disc. Furthermore, our analysis allowed us to determine the viscosity α,as well as the net mass and angular momentum (AM) loss rates. We find that α is variable, ranging from 0.1 to 1.0, not only from cycle to cycle but also within a given cycle. Additionally, build-up phases usually have larger values of α than the dissipation phases. Furthermore, during dissipation the outward AM flux is not necessarily zero, meaning that ω CMa does not experience a true quiescence but, instead, switches between a high to a low AM loss rate during which the disc quickly assumes an overall lower density but never zero. We confront the average AM loss rate with predictions from stellar evolution models for fast-rotating stars, and find that our measurements are smaller by more than one order of magnitude. [ABSTRACT FROM AUTHOR]

Published
2018
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43. The ASAS-SN catalogue of variable stars I: <italic>The Serendipitous Survey</italic>.

Author

Jayasinghe, T, Kochanek, C S, Stanek, K Z, Shappee, B J, Holoien, T W-S, Thompson, Toda A, Prieto, J L, Dong, Subo, Pawlak, M, Shields, J V, Pojmanski, G, Otero, S, Britt, C A, and Will, D

Subjects
VARIABLE stars, LIGHT curves, STAR catalogs, SUPERNOVAE, ASTRONOMICAL observations, BINARY stars
Abstract

The All-Sky Automated Survey for Supernovae (ASAS-SN) is the first optical survey to routinely monitor the whole sky with a cadence of ∼2–3  d down to V ≲ 17 mag. ASAS-SN has monitored the whole sky since 2014, collecting ∼100–500 epochs of observations per field. The V-band light curves for candidate variables identified during the search for supernovae are classified using a random forest classifier and visually verified. We present a catalogue of 66 179 bright, new variable stars discovered during our search for supernovae, including 27 479 periodic variables and 38 700 irregular variables. V-band light curves for the ASAS-SN variables are available through the ASAS-SN variable stars data base (https://asas-sn.osu.edu/variables). The data base will begin to include the light curves of known variable stars in the near future along with the results for a systematic, all-sky variability survey. [ABSTRACT FROM AUTHOR]

Published
2018
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44. Switching from tipranavir (TPV) 500/ritonavir (RTV) 200 mg to TPV 500/RTV 100 mg in treatment‐experienced patients (pts) with HIV RNA <50 copies/mL

Author

Casado, Jl, Domingo, P, Rubio, R, Antela, A, Lopez?Ruz, Ma, Castro, A, Portilla, J, Ribera, E, Podzamczer, D, Oteo, Ja, Galindo, J, Otero, S, Lozano, F, Estrada, V, Moltó, J, and Moreno, S

Subjects
Ritonavir -- Testing -- Dosage and administration, HIV infection -- Drug therapy, Health
Abstract

7‐11 November 2010, Tenth International Congress on Drug Therapy in HIV Infection, Glasgow, UK, Background The administration of 200 mg of RTV to boost TPV plasma levels is associated with poor tolerance and toxicity. Some studies have shown that 100 mg of RTV could [...]

Published
2010
Full Text
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45. Spectroscopic Observations of \delta Sco Through the 2011 Periastron Passage

Author

Rivinius, Th., Štefl, S., Baade, D., Carciofi, A. C., Otero, S., Miroshnichenko, A. S., and Manset, N.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We present prelimiary results from a coordinated spectroscopic campaign in 2011, centered on the \delta Sco periastron passage in July. Data have mostly been obtained with the FEROS/2.2 m at La Silla and ESPaDOnS/CFHT at Mauna Kea echelle instruments. Main results include the absence of tidally induced disturbance to the main \beta Cephei pulsation mode and the absence of tidally triggered mass-ejection at time of periastron proper. The observed (as far as yet analyzed) variations are compatible with the picture of a disk that is disturbed on its outer radius, with the disturbance propagating inwards after the periastron., Comment: Presented in "Circumstellar Dynamics at High Resolution", Foz do Igua\c{c}u, Brazil, February 27 - March 02, to appear in 2012, ASP Conf. Series 464, in press

Published
2012

46. Salmonella Montevideo infections associated with salami products made with contaminated imported black and red pepper--United States, July 2009-April 2010

Author

Julian, E., MacDonald, K., Marsden-Haug, N., Saathoff-Huber, L., Bonavolante, R., Otero, S., Nosari, J., Austin, C., Von Stein, D., Garvey, A., Kline, G., Lord, C., Groepper, R., Kissler, B., Parish, M., Elder, D., Pringle, J., Besser, J., Brown, S., Cooper, K., Sodha, S., Williams, I., Behravesh, C.Barton, and Gieraltowski, L. Bettencourt

Subjects
United States. Food and Drug Administration, Salmonella food poisoning -- Health aspects, Infection -- Health aspects, Salmonella -- Health aspects, Health
Abstract

In August and September 2009, PulseNet, the national molecular subtyping network for foodborne disease surveillance, detected a multistate cluster of Salmonella Montevideo infections with an indistinguishable pulse-field gel electrophoresis (PFGE) [...]

Published
2010

47. Muon Detection Based on a Hadronic Calorimeter

Author

Ciodaro, T, Abolins, M, Abreu, R, Achenbach, R, Adragna, P, Aharrouche, M, Aielli, G, Al-Shabibi, A, Aleksandrov, I, Alexandrov, E, Aloisio, A, Alviggi, M G, Amorim, A, Amram, N, Andrei, V, Anduaga, X, Angelaszek, D, Anjos, N, Annovi, A, Antonelli, S, Anulli, F, Apolle, R, Aracena, I, Ask, S, Åsman, B, Avolio, G, Baak, M, Backes, M, Backlund, S, Badescu, E, Baines, J, Ballestrero, S, Banerjee, S, Bansil, H S, Barnett, B M, Bartoldus, R, Bartsch, V, Batraneanu, S, Battaglia, A, Bauss, B, Beauchemin, P, Beck, H P, Bee, C, Begel, M, Behera, P K, Bell, P, Bell, W H, Bellagamba, L, Bellomo, M, Ben Ami, S, Bendel, M, Benhammou, Y, Benslama, K, Berge, D, Bernius, C, Berry, T, Bianco, M, Biglietti, M, Blair, R E, Bogaerts, A, Bohm, C, Boisvert, V, Bold, T, Bondioli, M, Borer, C, Boscherini, D, Bosman, M, Bossini, E, Boveia, A, Bracinik, J, Brandt, A G, Brawn, I P, Brelier, B, Brenner, R, Bressler, S, Brock, R, Brooks, W K, Brown, G, Brunet, S, Bruni, A, Bruni, G, Bucci, F, Buda, S, Burckhart-Chromek, D, Buscher, V, Buttinger, W, Calvet, S, Camarri, P, Campanelli, M, Canale, V, Canelli, F, Capasso, L, Caprini, M, Caracinha, D, Caramarcu, C, Cardarelli, R, Carlino, G, Casadei, D, Casado, M P, Cattani, G, Cerri, A, Cerrito, L, Chapleau, B, Childers, J T, Chiodini, G, Christidi, I, Ciapetti, G, Cimino, D, Ciobotaru, M, Coccaro, A, Cogan, J, Collins, N J, Conde Muino, P, Conidi, C, Conventi, F, Corradi, M, Corso-Radu, A, Coura Torres, R, Cranmer, K, Crescioli, F, Crone, G, Crupi, R, Cuenca Almenar, C, Cummings, J T, Curtis, C J, Czyczula, Z, Dam, M, Damazio, D, Dao, V, Darlea, G L, Davis, A O, De Asmundis, R, De Pedis, D, De Santo, A, de Seixas, J M, Degenhardt, J, Della Pietra, M, Della Volpe, D, Demers, S, Demirkoz, B, Di Ciaccio, A, Di Mattia, A, Di Nardo, R, Di Simone, A, Diaz, M A, Dietzsch, T A, Dionisi, C, Dobson, E, Dobson, M, dos Anjos, A, Dotti, A, Dova, M T, Drake, G, Dufour, M-A, Dumitru, I, Eckweiler, S, Ehrenfeld, W, Eifert, T, Eisenhandler, E, Ellis, K V, Ellis, N, Emeliyanov, D, Enoque Ferreira de Lima, D, Ermoline, Y, Ernst, J, Etzion, E, Falciano, S, Farrington, S, Farthouat, P, Faulkner , P J W, Fedorko, W, Fellmann, D, Feng, E, Ferrag, S, Ferrari, R, Ferrer, M L, Fiorini, L, Fischer, G, Flowerdew, M J, Fonseca Martin, T, Francis, D, Fratina, S, French, S T, Front, D, Fukunaga, C, Gadomski, S, Garelli, N, Garitaonandia Elejabarrieta, H, Gaudio, G, Gee, C N P, George, S, Giagu, S, Giannetti, P, Gillman, A R, Giorgi, M, Giunta, M, Giusti, P, Goebel, M, Gonçalo, R, Gonzalez Silva, L, Göringer, C, Gorini, B, Gorini, E, Grabowska-Bold, I, Green, B, Groll, M, Guida, A, Guler, H, Haas, S, Hadavand, H, Hadley, D R, Haller, J, Hamilton, A, Hanke, P, Hansen, J R, Hasegawa, S, Hasegawa, Y, Hauser, R, Hayakawa, T, Hayden, D, Head, S, Heim, S, Hellman, S, Henke, M, Hershenhorn, A, Hidvégi, A, Hillert, S, Hillier, S J, Hirayama, S, Hod, N, Hoffmann, D, Hong, T M, Hryn'ova, T, Huston, J, Iacobucci, G, Igonkina, O, Ikeno, M, Ilchenko, Y, Ishikawa, A, Ishino, M, Iwasaki, H, Izzo, V, Jez, P, Jimenez Otero, S, Johansen, M, Johns, K, Jones, G, Joos, M, Kadlecik, P, Kajomovitz, E, Kanaya, N, Kanega, F, Kanno, T, Kapliy, A, Kaushik, V, Kawagoe, K, Kawamoto, T, Kazarov, A, Kehoe, R, Kessoku, K, Khomich, A, Khoriauli, G, Kieft, G, Kirk, J, Klemetti, M, Klofver, P, Klous, S, Kluge, E-E, Kobayashi, T, Koeneke, K, Koletsou, I, Koll, J D, Kolos, S, Kono, T, Konoplich, R, Konstantinidis, N, Korcyl, K, Kordas, K, Kotov, V, Kowalewski, R V, Krasznahorkay, A, Kraus, J, Kreisel, A, Kubota, T, Kugel, A, Kunkle, J, Kurashige, H, Kuze, M, Kwee, R, Laforge, B, Landon, M, Lane, J, Lankford, A J, Laranjeira Lima, S M, Larner, A, Leahu, L, Lehmann Miotto, G, Lei, X, Lellouch, D, Levinson, L, Li, S, Liberti, B, Lilley, J N, Linnemann, J T, Lipeles, E, Lohse, T, Losada, M, Lowe, A, Luci, C, Luminari, L, Lundberg, J, Lupu, N, Machado Miguéns, J, Mackeprang, R, Maettig, S, Magnoni, L, Maiani, C, Maltrana, D, Mangeard, P-S, Männer, R, Mapelli, L, Marchese, F, Marino, C, Martin, B, Martin, B T, Martin, T, Martyniuk, A, Marzano, F, Masik, J, Mastrandrea, P, Matsushita, T, McCarn, A, Mechnich, J, Medinnis, M, Meier, K, Melachrinos, C, Mendoza Nava, L M, Merola, L, Messina, A, Meyer, C P, Middleton, R P, Mikenberg, G, Mills, C M, Mincer, A, Mineev, M, Misiejuk, A, Moa, T, Moenig, K, Monk, J, Monticelli, F, Mora Herrera, C, Morettini, P, Morris, J D, Müller, F, Munwes, Y, Murillo Garcia, R, Nagano, K, Nagasaka, Y, Navarro, G A, Negri, A, Nelson, S, Nemethy, P, Neubauer, M S, Neusiedl, A, Newman, P, Nisati, A, Nomoto, H, Nozaki, M, Nozicka, M, Nurse, E, Ochando, C, Ochi, A, Oda, S, Oh, A, Ohm, C, Okumura, Y, Olivito, D, Omachi, C, Osculati, B, Oshita, H, Ospanov, R, Owen, M A, Özcan, V E, Ozone, K, Padilla, C, Panes, B, Panikashvili, N, Paramonov, A, Parodi, F, Pasqualucci, E, Pastore, F, Patricelli, S, Pauly, T, Perera, V J O, Perez, E, Petcu, M, Petersen, B A, Petersen, J, Petrolo, E, Phan, A, Piegaia, R, Pilkington, A, Pinder, A, Poddar, S, Polini, A, Pope, B G, Potter, C T, Primavera, M, Prokoshin, F, Ptacek, E, Qian, W, Quinonez, F, Rajagopalan, S, Ramos Dos Santos Neves, R, Reinherz-Aronis, E, Reinsch, A, Renkel, P, Rescigno, M, Rieke, S, Riu, I, Robertson, S H, Robinson, M, Rodriguez, D, Roich, A, Romeo, G, Romero, R, Roos, L, Ruiz Martinez, A, Ryabov, Y, Ryan, P, Saavedra, A, Safai Tehrani, F, Sakamoto, H, Salamanna, G, Salamon, A, Saland, J, Salnikov, A, Salvatore, F, Sankey, D P C, Santamarina, C, Santonico, R, Sarkisyan-Grinbaum, E, Sasaki, O, Savu, D, Scannicchio, D A, Schäfer, U, Scharf, V L, Scheirich, D, Schiavi, C, Schlereth, J, Schmitt, K, Schroder, C, Schroer, N, Schultz-Coulon, H-C, Schwienhorst, R, Sekhniaidze, G, Sfyrla, A, Shamim, M, Sherman, D, Shimojima, M, Shochet, M, Shooltz, D, Sidoti, A, Silbert, O, Silverstein, S, Sinev, N, Siragusa, G, Sivoklokov, S, Sjoen, R, Sjölin, J, Slagle, K, Sloper, J E, Smith, B C, Soffer, A, Soloviev, I, Spagnolo, S, Spiwoks, R, Staley, R J, Stamen, R, Stancu, S, Steinberg, P, Stelzer, J, Stockton, M C, Straessner, A, Strauss, E A, Strom, D, Su, D, Sugaya, Y, Sugimoto, T, Sushkov, S, Sutton, M R, Suzuki, Y, Taffard, A, Taiblum, N, Takahashi, Y, Takeda, H, Takeshita, T, Tamsett, M, Tan, C L A, Tanaka, S, Tapprogge, S, Tarem, S, Tarem, Z, Taylor, C, Teixeira-Dias, P, Thomas, J P, Thompson, P D, Thomson, M A, Tokushuku, K, Tollefson, K, Tomoto, M, Topfel, C, Torrence, E, Touchard, F, Traynor, D, Tremblet, L, Tricoli, A, Tripiana, M, Triplett, N, True, P, Tsiakiris, M, Tsuno, S, Tuggle, J, Ünel, G, Urquijo, P, Urrejola, P, Usai, G, Vachon, B, Vallecorsa, S, Valsan, L, Vandelli, W, Vari, R, Vaz Gil Lopes, L, Veneziano, S, Ventura, A, Venturi, N, Vercesi, V, Vermeulen, J C, Volpi, G, Vorwerk, V, Wagner, P, Wang, M, Warburton, A, Watkins, P M, Watson, A T, Watson, M, Weber, P, Weidberg, A R, Wengler, T, Werner, P, Werth, M, Wessels, M, White, M, Whiteson, D, Wickens, F J, Wiedenmann, W, Wielers, M, Winklmeier, F, Woods, K S, Wu, S-L, Wu, X, Xaplanteris Karampatsos, L, Xella, S, Yakovlev, A, Yamazaki, Y, Yang, U, Yasu, Y, Yuan, L, Zaitsev, A, Zanello, L, Zhang, H, Zhang, J, Zhao, L, Zobernig, H, and zur Nedden, M

Subjects
Physics::Instrumentation and Detectors, Physics::Accelerator Physics, High Energy Physics::Experiment, Detectors and Experimental Techniques
Abstract

The ATLAS Tile hadronic calorimeter (TileCal) provides highly-segmented energy measurements of incoming particles. The information from TileCal's last segmentation layer can assist in muon tagging and it is being considered for a near future upgrade of the level-one trigger, mainly for rejecting triggers due to cavern background at the barrel region. A muon receiver for the TileCal muon signals is being designed in order to interface with the ATLAS level-one trigger. This paper addresses the preliminary studies concerning the muon discrimination capability for the muon receiver. Monte Carlo simulations for single muons from the interaction point were used to study the effectiveness of hadronic calorimeter information on muon detection.

Published
2010

48. The ATLAS Trigger/DAQ Authorlist, version 4.0

Author

Abolins, M, Abreu, R, Achenbach, R, Adragna, P, Aharrouche, M, Aielli, G, Al-Shabibi, A, Aleksandrov, I, Alexandrov, E, Aloisio, A, Alviggi, M G, Amorim, A, Amram, N, Andrei, V, Anduaga, X, Angelaszek, D, Anjos, N, Annovi, A, Antonelli, S, Anulli, F, Apolle, R, Aracena, I, Ask, S, Åsman, B, Avolio, G, Baak, M, Backes, M, Backlund, S, Badescu, E, Baines, J, Ballestrero, S, Banerjee, S, Bansil, H S, Barnett, B M, Bartoldus, R, Bartsch, V, Batraneanu, S, Battaglia, A, Bauss, B, Beauchemin, P, Beck, H P, Bee, C, Behera, P K, Bell, P, Bell, W H, Bellagamba, L, Bellomo, M, Ben Ami, S, Bendel, M, Benhammou, Y, Benslama, K, Berge, D, Bernius, C, Berry, T, Bianco, M, Biglietti, M, Blair, R E, Bogaerts, A, Bohm, C, Boisvert, V, Bold, T, Bondioli, M, Borer, C, Boscherini, D, Bosman, M, Bossini, E, Boveia, A, Bracinik, J, Brandt, A G, Brawn, I P, Brelier, B, Brenner, R, Bressler, S, Brock, R, Brooks, W K, Brown, G, Brunet, S, Bruni, A, Bruni, G, Bucci, F, Buda, S, Burckhart-Chromek, D, Buscher, V, Buttinger, W, Calvet, S, Camarri, P, Campanelli, M, Canale, V, Canelli, F, Capasso, L, Caprini, M, Caracinha, D, Caramarcu, C, Cardarelli, R, Carlino, G, Casadei, D, Casado, M P, Cattani, G, Cerri, A, Cerrito, L, Chapleau, B, Childers, J T, Chiodini, G, Christidi, I, Ciapetti, G, Cimino, D, Ciobotaru, M, Coccaro, A, Cogan, J, Collins, N J, Conde Muino, P, Conidi, C, Conventi, F, Corradi, M, Corso-Radu, A, Coura Torres, R, Cranmer, K, Crescioli, F, Crone, G, Crupi, R, Cuenca Almenar, C, Cummings, J T, Curtis, C J, Czyczula, Z, Dam, M, Damazio, D, Dao, V, Darlea, G L, Davis, A O, De Asmundis, R, De Pedis, D, De Santo, A, de Seixas, J M, Degenhardt, J, Della Pietra, M, Della Volpe, D, Demers, S, Demirkoz, B, Di Ciaccio, A, Di Mattia, A, Di Nardo, R, Di Simone, A, Diaz, M A, Dietzsch, T A, Dionisi, C, Dobson, E, Dobson, M, dos Anjos, A, Dotti, A, Dova, M T, Drake, G, Dufour, M-A, Dumitru, I, Eckweiler, S, Ehrenfeld, W, Eifert, T, Eisenhandler, E, Ellis, K V, Ellis, N, Emeliyanov, D, Enoque Ferreira de Lima, D, Ermoline, Y, Ernst, J, Etzion, E, Falciano, S, Farrington, S, Farthouat, P, Faulkner, P J W, Fedorko, W, Fellmann, D, Feng, E, Ferrag, S, Ferrari, R, Ferrer, M L, Fiorini, L, Fischer, G, Flowerdew, M J, Föhlisch, F, Fonseca Martin, T, Francis, D, Fratina, S, French, S T, Front, D, Fukunaga, C, Gadomski, S, Garelli, N, Garitaonandia Elejabarrieta, H, Gaudio, G, Gee, C N P, George, S, Giagu, S, Giannetti, P, Gillman, A R, Giorgi, M, Giunta, M, Giusti, P, Goebel, M, Gonçalo, R, Gonzalez Silva, L, Göringer, C, Gorini, B, Gorini, E, Grabowska-Bold, I, Green, B, Groll, M, Guida, A, Guler, H, Haas, S, Hadavand, H, Hadley, D R, Haller, J, Hamilton, A, Hanke, P, Hansen, J R, Hasegawa, S, Hasegawa, Y, Hauser, R, Hayakawa, T, Hayden, D, Head, S, Heim, S, Hellman, S, Henke, M, Hershenhorn, A, Hidvégi, A, Hillert, S, Hillier, S J, Hirayama, S, Hod, N, Hoffmann, D, Hryn'ova, T, Huston, J, Iacobucci, G, Igonkina, O, Ikeno, M, Ilchenko, Y, Ishikawa, A, Ishino, M, Iwasaki, H, Izzo, V, Jez, P, Jimenez Otero, S, Johansen, M, Johns, K, Joos, M, Kadlecik, P, Kajomovitz, E, Kanaya, N, Kanega, F, Kanno, T, Kapliy, A, Kaushik, V, Kawagoe, K, Kawamoto, T, Kazarov, A, Kehoe, R, Kessoku, K, Khomich, A, Khoriauli, G, Kieft, G, Kirk, J, Klemetti, M, Klofver, P, Klous, S, Kluge, E-E, Kobayashi, T, Koeneke, K, Koletsou, I, Koll, J D, Kolos, S, Kono, T, Konoplich, R, Konstantinidis, N, Korcyl, K, Kordas, K, Kotov, V, Kowalewski, R V, Krasznahorkay, A, Kraus, J, Kreisel, A, Kubota, T, Kugel, A, Kurashige, H, Kuze, M, Kwee, R, Laforge, B, Landon, M, Lane, J, Lankford, A J, Laranjeira Lima, S M, Larner, A, Leahu, L, Lehmann Miotto, G, Lei, X, Lellouch, D, Levinson, L, Li, S, Liberti, B, Lilley, J N, Linnemann, J T, Lohse, T, Losada, M, Lowe, A, Luci, C, Luminari, L, Lundberg, J, Lupu, N, Machado Miguéns, J, Mackeprang, R, Maettig, S, Magnoni, L, Maiani, C, Maltrana, D, Mangeard, P-S, Männer, R, Mapelli, L, Marchese, F, Marino, C, Martin, B, Martin, B T, Martin, T, Martyniuk, A, Marzano, F, Masik, J, Mastrandrea, P, Matsushita, T, McCarn, A, Mechnich, J, Medinnis, M, Meier, K, Melachrinos, C, Mendoza Nava, L M, Merola, L, Messina, A, Meyer, C P, Middleton, R P, Mikenberg, G, Mincer, A, Mineev, M, Misiejuk, A, Moa, T, Moenig, K, Monk, J, Monticelli, F, Mora Herrera, C, Morettini, P, Morris, J D, Müller, F, Munwes, Y, Murillo Garcia, R, Nagano, K, Nagasaka, Y, Navarro, G A, Negri, A, Nelson, S, Nemethy, P, Neubauer, M S, Neusiedl, A, Newman, P, Nisati, A, Nomoto, H, Nozaki, M, Nozicka, M, Nurse, E, Ochando, C, Ochi, A, Oda, S, Oh, A, Ohm, C, Okumura, Y, Olvito, D, Omachi, C, Osculati, B, Oshita, H, Owen, M A, Özcan, V E, Ozone, K, Padilla, C, Panes, B, Panikashvili, N, Paramonov, A, Parodi, F, Pasqualucci, E, Pastore, F, Patricelli, S, Pauly, T, Perera, V J O, Perez, E, Petcu, M, Petersen, B, Petersen, J, Petrolo, E, Phan, A, Piegaia, R, Pilkington, A, Pinder, A, Poddar, S, Polini, A, Pope, B G, Potter, C T, Primavera, M, Prokoshin, F, Ptacek, E, Qian, W, Quinonez, F, Rajagopalan, S, Ramos Dos Santos Neves, R, Reinherz-Aronis, E, Reinsch, A, Renkel, P, Rescigno, M, Rieke, S, Riu, I, Robertson, S H, Robinson, M, Rodriguez, D, Roich, A, Romeo, G, Romero, R, Roos, L, Rühr, F, Ruiz Martinez, A, Ryabov, Y, Ryan, P, Saavedra, A, Sakamoto, H, Salamanna, G, Salamon, A, Saland, J, Salnikov, A, Salvatore, F, Sankey, D P C, Santamarina, C, Santonico, R, Sarkisyan-Grinbaum, E, Sasaki, O, Savu, D, Scannicchio, D A, Schäfer, U, Scharf, V L, Scheirich, D, Schiavi, C, Schlereth, J, Schmitt, K, Schroder, C, Schroer, N, Schultz-Coulon, H-C, Schwienhorst, R, Sekhniaidze, G, Sfyrla, A, Shamim, M, Sherman, D, Shimojima, M, Shochet, M, Shooltz, D, Sidoti, A, Silbert, O, Silverstein, S, Sinev, N, Siragusa, G, Sivoklokov, S, Sjoen, R, Sjölin, J, Slagle, K, Sloper, J E, Soffer, A, Soloviev, I, Spagnolo, S, Spiwoks, R, Staley, R J, Stamen, R, Stancu, S, Steinberg, P, Stelzer, J, Stockton, M C, Straessner, A, Strauss, E A, Strom, D, Su, D, Sugaya, Y, Sugimoto, T, Sushkov, S, Sutton, M R, Suzuki, Y, Taffard, A, Taiblum, N, Takahashi, Y, Takeda, H, Takeshita, T, Tamsett, M, Tan, C L A, Tanaka, S, Tapprogge, S, Tarem, S, Tarem, Z, Taylor, C, Teixeira-Dias, P, Thomas, J P, Thompson, P D, Thomson, M A, Tokushuku, K, Tollefson, K, Tomoto, M, Topfel, C, Torrence, E, Touchard, F, Traynor, D, Tremblet, L, Tricoli, A, Tripiana, M, Triplett, N, True, P, Tsiakiris, J, Tsuno, S, Tuggle, J, Ünel, G, Urquijo, P, Urrejola, P, Usai, G, Vachon, B, Vallecorsa, S, Valsan, L, Vandelli, W, Vari, R, Vaz Gil Lopes, L, Veneziano, S, Ventura, A, Venturi, N, Vercesi, V, Vermeulen, J C, Volpi, G, Vorwerk, V, Wang, M, Warburton, A, Watkins, P M, Watson, A T, Watson, M, Weber, P, Weidberg, A R, Wengler, T, Werner, P, Werth, M, Wessels, M, White, M, Whiteson, D, Wickens, F J, Wiedenmann, W, Wielers, M, Winklmeier, F, Woods, K S, Wu, S-L, Wu, X, Xaplanteris Karampatsos, L, Xella, S, Yakovlev, A, Yamazaki, Y, Yang, U, Yasu, Y, Yuan, L, Zaitsev, A, Zanello, L, Zhang, H, Zhang, J, Zhao, L, Zobernig, H, and zur Nedden, M

Subjects
Detectors and Experimental Techniques
Abstract

This is the ATLAS Trigger/DAQ Authorlist, version 4.0, 06 May 2010

Published
2010

49. The ATLAS Trigger/DAQ Authorlist, version 3.0

Author

Abolins, M, Abreu, R, Achenbach, R, Adorisio, C, Adragna, P, Aharrouche, M, Aielli, G, Al-Shabibi, A, Aleksandrov, I, Alexandre, G, Alexandrov, E, Aloisio, A, Alviggi, M G, Amorim, A, Amram, N, Anderson, K, Andrei, V, Anduaga, X, Anjos, N, Antonelli, S, Anulli, F, Aracena, I, Ask, S, Åsman, B, Avolio, G, Baak, M, Backlund, S, Badescu, E, Baines, J, Banerjee, S, Barnett, B M, Bartoldus, R, Batraneanu, S, Battaglia, A, Bauss, B, Beauchemin, P, Beck, H P, Bee, C, Behera, P, Bell, P, Bell, W H, Bellagamba, L, Bellomo, M, Ben Ami, S, Bendel, M, Benhammou, Ya, Benslama, K, Berge, D, Berger, N, Bernius, C, Berry, T, Bianco, M, Biau, C, Biglietti, M, Bizjak, I, Blair, R E, Boeser, S, Bogaerts, A, Böhm, C, Boisvert, V, Bold, T, Bondioli, M, Booth, J R A, Borer, C, Boscherini, D, Bosman, M, Boveia, A, Boyd, J, Bracinik, J, Brawn, I P, Brelier, B, Bressler, S, Brock, R, Brooks, W K, Brunet, S, Bruni, A, Bruni, G, Bucci, F, Buda, S, Burckhart-Chromek, D, Buttar, C, Camarri, P, Campanelli, M, Canale, V, Canelli, F, Capasso, L, Caprini, M, Caracinha, D, Caramarcu, C, Cardarelli, R, Carlino, G, Casadei, D, Casado, M P, Cataldi, G, Cattani, G, Cerri, A, Charlton, D G, Childers, J T, Chiodini, G, Ciapetti, G, Cimino, D, Ciobotaru, M, Coccaro, A, Collins, N J, Conde-Muíño, P, Conventi, F, Corradi, M, Corso-Radu, A, Costa, M J, Coura Torres, R, Cranmer, K, Crone, G, Crupi, R, Cuenca-Almenar, C, Curtis, C J, Czyczula, Z, Dam, M, Damazio, D, Darlea, G L, Davis, A O, De Asmundis, R, De Pedis, D, De Santo, A, De Seixas, J M, Degenhardt, J, Della Pietra, M, Della Volpe, D, Delsart, P-A, Demers, S, Demirkoz, B, Di Ciaccio, A, Di Mattia, A, Di Nardo, R, Di Simone, A, Díaz, M A, Dionisi, C, Djilkibaev, R, Dobson, E, Dobson, M, Dos Anjos, A, Dotti, A, Dova, M T, Drake, G, Dufour, M-A, Eckweiler, S, Ehrenfeld, W, Eifert, T, Eisenhandler, E F, Ellis, Nick, Emeliyanov, D, Enoque Ferreira de Lima, D, Ermoline, Y, Eschrich, I, Etzion, E, Falciano, S, Farrington, S, Farthouat, P, Faulkner, P J W, Fedorko, A, Fedorko, I, Feng, E, Ferland, J, Ferrag, S, Ferrari, R, Ferrer, M L, Fiorini, L, Fischer, G, Flowerdew, M, Föhlisch, F, Fonseca-Martin, T, Francis, D, Fratina, S, Fukunaga, C, Gadomski, S, Gallacher, M P, Garitaonandia Elejabarrieta, H, Gaudio, G, Gee, C N P, George, S, Giagu, S, Gillman, A R, Giusti, P, Goebel, M, Gonçalo, R, Gonzalez Pinto, F, Gonzalez Silva, L, Göringer, C, Gorini, B, Gorini, E, Grabowska-Bold, I, Grancagnolo, S, Green, B, Groll, M, Guida, A, Güler, H, Haas, S, Hadavand, H, Hadley, D R, Haller, J, Hamilton, A, Hanke, P, Hansen, J R, Hasagawa, S, Hasegawa, Y, Hauser, R, Hayakawa, T, Head, S, Heijboer, A, Heim, S, Hellman, S, Hershenhorn, A, Hidvégi, A, Hillier, S J, Hirayama, S, Hod, N, Hoffmann, D, Hori, T, Hrynóva, T, Huston, J, Iacobucci, G, Idarraga, J, Iengo, P, Igonkina, O, Ikeno, M, Ilchenko, Y, Ishikawa, A, Ishino, M, Iwasaki, H, Izzo, V, Jain, V, Jez, P, Jiménez-Otero, S, Johansen, M, Johns, K, Jones, G, Joos, M, Kadosaka, T, Kajomovitz, E, Kalinowski, A, Kama, S, Kanaya, N, Kanega, F, Kapliy, A, Kaushik, V, Kawagoe, K, Kawamoto, T, Kazarov, A, Kehoe, R, Kessoku, K, Khoriauli, G, Kieft, G, Kirk, J, Kiyamura, H, Klementti, M, Klofver, P, Klous, S, Kluge, E-E, Kobayashi, T, Koeneke, K, Kolos, S, Kono, T, Konoplich, R, Konstantinidis, N, Korcyl, K, Kordas, K, Kotov, V, Kowalewski, R V, Krasznahorkay, A, Kreisel, A, Kubota, T, Kugel, A, Kurashige, H, Kwee, R, Landon, M, Lane, J, Lankford, A J, Leahu, L, Leahu, M, Ledroit, F, Lehmann-Miotto, G, Lei, X, Lellouch, D, Lendermann, V, Levinson, L, Li, S, Liberti, B, Lilley, J N, Lim, H, Linnemann, J T, Lohse, T, Losada, M, Lowe, A, Luci, C, Luminari, L, Lundberg, J, Lupu, N, Machado Miguéns, J, Mackeprang, R, Maettig, S, Mahboubi, K, Mahout, G, Maltrana, D, Mamuzic, J, Männer, R, Mapelli, L, Marchese, F, Marino, C, Martin, B, Martin, B T, Martyniuk, A, Marzano, F, Masik, J, Matsushita, T, McCarn, A, McPherson, R, Medinnis, M, Meier, K, Melachrinos, C, Merola, L, Messina, A, Middleton, R P, Mikenberg, G, Mincer, A, Mineev, M, Misiejuk, A, Moa, T, Mönig, K, Monticelli, F, Mora Herrera, C, Moreno, D, Morettini, P, Morris, J D, Müller, F, Murillo Garcia, R, Nagano, K, Nagasaka, Y, Nakatsuka, H, Navarro, G A, Negri, A, Némethy, P, Neubauer, M S, Neusiedl, A, Nisati, A, Niwa, T, Nomoto, H, Nozaki, M, Nozicka, M, Nurse, E, Ochi, A, Oda, S, Oh, A, Ohm, C, Okumura, Y, Oltmann, B, Olvito, D, Omachi, C, Osculati, B, Oshita, H, Osuna, C, Owen, M A, Özcan, E, Ozone, K, Padilla, C, Panes, B, Panikashvili, N, Parodi, F, Pasqualucci, E, Pastore, F, Patricelli, S, Pauly, T, Perantoni, M, Perera, V J O, Pérez, E, Pérez-Réale, V, Perrino, R, Pessoa Lima Junior, H, Petcu, M, Petersen, B, Petersen, J, Petrolo, E, Piegaia, R, Pinzon, G, Policicchio, A, Polini, A, Pope, B G, Potter, C, Prieur, D P F, Primavera, M, Prokoshin, F, Qian, W, Quinonez, F, Rajagopalan, S, Ramos Dos Santos Neves, R, Reinherz, E, Reinsch, A, Renkel, P, Rescigno, M, Rieke, S, Risler, C, Riu, I, Robertson, S, Roda, C, Rodríguez, D, Rogriquez, Y, Roich, A, Romeo, G, Romero, R, Rosati, S, Rühr, F, Ruiz-Martinez, A, Ryabov, Yu, Ryan, P, Saavedra, A, Sakamoto, H, Salamon, A, Salnikov, A, Salvatore, D, Salvatore, F, Sandaker, H, Sankey, D P C, Santamarina, C, Santonico, R, Sarkisyan-Grinbaum, E, Sasaki, O, Savu, D, Scannicchio, D A, Schäfer, U, Schiavi, C, Schlereth, J L, Schmitt, K, Schooltz, D, Schroer, N, Schultz-Coulon, H-C, Schwienhorst, R, Segura, E, Sekhniaidze, G, Sfyrla, A, Sherman, D, Shimojima, M, Shochet, M, Sidoti, A, Silverstein, D, Silverstein, S, Sinev, N, Siragusa, G, Sivoklokov, S, Sjoen, R, Sjölin, J, Slagle, K, Sloper, J E, Smizanska, M, Soffer, A, Soloviev, I, Spagnolo, S, Spiwoks, R, Staley, R J, Stamen, R, Stancu, S, Steinberg, P, Stelzer, J, Stockton, M C, Stradling, A, Strässner, A, Strom, D, Su, D, Sugaya, Y, Sugimoto, T, Sushkov, S, Sutton, M, Suzuki, Y, Szymocha, T, Taffard, A, Takahashi, Y, Takeda, H, Takeshita, T, Tamsett, M, Tan, C L A, Tanaka, S, Tapprogge, S, Tarem, S, Tarem, Z, Taylor, C, Taylor, R P, Teixeira-Dias, P, Thomas, J P, Thompson, P D, Tokushuku, K, Tollefson, K, Tomoto, M, Topfel, C, Torrence, E, Touchard, F, Tremblet, L, Tripiana, M, Triplett, N, Tsulaia, V, Tsuno, S, Tuggle, J, Ünel, G, Urquijo, P, Urrejola, P, Usai, G, Vachon, B, Vandelli, W, Vari, R, Vaz-Gil-Lopes, L, Veneziano, S, Ventura, A, Vercesi, V, Vermeulen, J C, Vorwerk, V, Wang, M, Watkins, P M, Watson, A T, Weber, P, Weidberg, T, Wengler, T, Werner, P, Werth, M, Wessels, M, White, M, Whiteson, D, Wickens, F J, Wiedenmann, W, Wielers, M, Wildt, M, Winklmeier, F, Wu, S-L, Wu, X, Xaplanteris Karampatsos, L, Xella, S, Yakovlev, A, Yamazaki, Y, Yang, U, Yasu, Y, Zaitsev, A, Zanello, L, Zema, F, Zhang, J, Zhao, L, Zobernig, H, and Zur Nedden, M

Subjects
Detectors and Experimental Techniques
Abstract

This is the ATLAS Trigger/DAQ Authorlist, version 3.0, 11 September 2009

Published
2009

50. The ATLAS Trigger/DAQ Authorlist, version 2.0

Author

Abolins, M, Abreu, R, Achenbach, R, Adorisio, C, Adragna, P, Aharrouche, M, Aielli, G, Al-Shabibi, A, Aleksandrov, I, Alexandre, G, Alexandrov, E, Aloisio, A, Alviggi, M G, Amorim, A, Amram, N, Anderson, K, Andrei, V, Anduaga, X, Anjos, N, Antonelli, S, Anulli, F, Aracena, I, Ask, S, Åsman, B, Avolio, G, Baak, M, Backlund, S, Badescu, E, Baines, J, Banerjee, S, Barnett, B M, Bartoldus, R, Batraneanu, S, Battaglia, A, Bauss, B, Beauchemin, P, Beck, H P, Bee, C, Behera, P, Bell, P, Bell, W H, Bellagamba, L, Bellomo, M, Ben Ami, S, Bendel, M, Benhammou, Ya, Benslama, K, Berge, D, Berger, N, Bernius, C, Berry, T, Bianco, M, Biau, C, Biglietti, M, Bizjak, I, Blair, R E, Boeser, S, Bogaerts, A, Böhm, C, Boisvert, V, Bold, T, Bondioli, M, Booth, J R A, Borer, C, Boscherini, D, Bosman, M, Boyd, J, Bracinik, J, Brawn, I P, Brelier, B, Bressler, S, Brock, R, Brooks, W K, Brunet, S, Bruni, A, Bruni, G, Bucci, F, Buda, S, Burckhart-Chromek, D, Buttar, C, Camarri, P, Campanelli, M, Canale, V, Canepa, A, Capasso, L, Caprini, M, Caracinha, D, Caramarcu, C, Cardarelli, R, Carlino, G, Casadei, D, Casado, M P, Cataldi, G, Cerri, A, Charlton, D G, Childers, J T, Chiodini, G, Ciapetti, G, Cimino, D, Ciobotaru, M, Coccaro, A, Collins, N J, Conde-Muíño, P, Conventi, F, Corradi, M, Corso-Radu, A, Costa, M J, Coura Torres, R, Cranmer, K, Crone, G, Crupi, R, Cuenca-Almenar, C, Curtis, C J, Czyczula, Z, Dam, M, Damazio, D, Darlea, G L, Davis, A O, De Pedis, D, De Santo, A, De Seixas, J M, DeAsmundis, R, Degenhardt, J, Della Volpe, D, DellaPietra, M, Delsart, P-A, Demers, S, Demirkoz, B, Di Mattia, A, Di Nardo, R, Díaz, M A, Di Ciaccio, A, Dionisi, C, Djilkibaev, R, Dobson, E, Dobson, M, Dogaru, M, Dos Anjos, A, Dotti, A, Dova, M T, Drake, G, Dufour, M-A, Eckweiler, S, Ehrenfeld, W, Eifert, T, Eisenhandler, E F, Ellis, Nick, Emeliyanov, D, Enoque Ferreira de Lima, D, Ermoline, Y, Eschrich, I, Etzion, E, Falciano, S, Farthouat, P, Faulkner, P J W, Fedorko, A, Fedorko, I, Feng, E, Ferland, J, Ferrag, S, Ferrari, R, Ferrer, M L, Fiorini, L, Fischer, G, Flacher, H, Fleckner, J E, Flowerdew, M, Föhlisch, F, Fonseca-Martin, T, Francis, D, Fratina, S, Fukunaga, C, Gadomski, S, Gallacher, M P, Garitaonandia Elejabarrieta, H, Gaudio, G, Gee, C N P, George, S, Ghete, V M, Giagu, S, Gillman, A R, Giusti, P, Goebel, M, Gonçalo, R, Gonzalez Pinto, F, Gonzalez Silva, L, Göringer, C, Gorini, B, Gorini, E, Grabowska-Bold, I, Grancagnolo, S, Green, B, Groll, M, Guida, A, Güler, H, Haas, S, Hadavand, H, Hadley, D R, Haller, J, Hamilton, A, Hanke, P, Hansen, J R, Hasagawa, S, Hasegawa, Y, Hauschild, M, Hauser, R, Hayakawa, T, Head, S, Heijboer, A, Heim, S, Hellman, S, Hershenhorn, A, Hidvégi, A, Hillier, S J, Hirayama, S, Hod, N, Hori, T, Hrynóva, T, Hughes-Jones, R, Huston, J, Iacobucci, G, Idarraga, J, Iengo, P, Igonkina, O, Ikeno, M, Ilchenko, Y, Ishikawa, A, Ishino, M, Iwasaki, H, Izzo, V, Jain, V, Jez, P, Jiménez-Otero, S, Johansen, M, Johns, K, Jones, G, Joos, M, Kadosaka, T, Kajomovitz, E, Kalinowski, A, Kama, S, Kanaya, N, Kanega, F, Kaushik, V, Kawagoe, K, Kawamoto, T, Kazarov, A, Kehoe, R, Kessoku, K, Khoriauli, G, Kieft, G, Kirk, J, Kiyamura, H, Klementti, M, Klofver, P, Klous, S, Kluge, E-E, Kobayashi, T, Koeneke, K, Kolos, S, Kono, T, Konoplich, R, Konstantinidis, N, Korcyl, K, Kordas, K, Kotov, V, Kowalewski, R V, Krasznahorkay, A, Kreisel, A, Kubota, T, Kugel, A, Kurashige, H, Kwee, R, Landon, M, Lane, J, Lankford, A J, Leahu, L, Leahu, M, LeCompte, T, Ledroit, F, Lehmann-Miotto, G, Lei, X, Lellouch, D, Lendermann, V, Levinson, L, Li, S, Liberti, B, Lilley, J N, Lim, H, Linnemann, J T, Lohse, T, Losada, M, Lowe, A, Luci, C, Luminari, L, Lundberg, J, Lupu, N, Machado Miguéns, J, Mackeprang, R, Maettig, S, Mahboubi, K, Mahout, G, Maltrana, D, Mamuzic, J, Männer, R, Mapelli, L, Marchese, F, Marino, C, Martin, B, Martin, B T, Martyniuk, A, Marzano, F, Masik, J, Matsushita, T, McMahon, T, McPherson, R, Medinnis, M, Meessen, C, Meier, K, Meirosu, C, Merola, L, Messina, A, Middleton, R P, Mikenberg, G, Mincer, A, Mineev, M, Misiejuk, A, Moa, T, Mönig, K, Monticelli, F, Mora Herrera, C, Moreno, D, Morettini, P, Morris, J D, Müller, F, Murillo Garcia, R, Nagano, K, Nagasaka, Y, Nakatsuka, H, Navarro, G A, Negri, A, Némethy, P, Neusiedl, A, Nisati, A, Niwa, T, Nomoto, H, Nozaki, M, Nozicka, M, Nurse, E, Ochi, A, Oda, S, Ohm, C, Okumura, Y, Oltmann, B, Olvito, D, Omachi, C, Osculati, B, Oshita, H, Osuna, C, Owen, M A, Özcan, E, Ozone, K, Padilla, C, Panes, B, Panikashvili, N, Parodi, F, Pasqualucci, E, Pastore, F, Patricelli, S, Pauly, T, Perantoni, M, Perera, V J O, Pérez, E, Pérez-Réale, V, Perrino, R, Pessoa Lima Junior, H, Petcu, M, Petersen, B, Petersen, J, Petrolo, E, Piegaia, R, Pilcher, J E, Pinzon, G, Policicchio, A, Polini, A, Pope, B G, Potter, C, Prieur, D P F, Primavera, M, Prokoshin, F, Qian, W, Quinonez, F, Rajagopalan, S, Ramos Dos Santos Neves, R, Reinherz, E, Reinsch, A, Renkel, P, Rescigno, M, Rieke, S, Risler, C, Riu, I, Robertson, S, Roda, C, Rodríguez, D, Rogriquez, Y, Roich, A, Romeo, G, Romero, R, Rosati, S, Rühr, F, Ruiz-Martinez, A, Ryabov, Yu, Ryan, P, Saavedra, A, Sakamoto, H, Salamon, A, Salnikov, A, Salvatore, D, Salvatore, F, Sandaker, H, Sankey, D P C, Santamarina, C, Santonico, R, Sarkisyan-Grinbaum, E, Sasaki, O, Savu, D, Scannicchio, D, Schäfer, U, Schiavi, C, Schlereth, J L, Schmitt, K, Schmitt, S, Scholtes, I, Schooltz, D, Schroer, N, Schultz-Coulon, H-C, Schwienhorst, R, Scott, W, Segura, E, Sekhniaidze, G, Sfyrla, A, Sherman, D, Shimojima, M, Sidoti, A, Silverstein, D, Silverstein, S, Sinev, N, Siragusa, G, Sivoklokov, S, Sjoen, R, Sjölin, J, Slagle, K, Sloper, J E, Smizanska, M, Soffer, A, Soloviev, I, Spagnolo, S, Spiwoks, R, Staley, R J, Stamen, R, Stancu, S, Steinberg, P, Stelzer, J, Stockton, M C, Stradling, A, Strässner, A, Strom, D, Su, D, Sugaya, Y, Sugimoto, T, Sushkov, S, Sutton, M, Suzuki, Y, Szymocha, T, Taffard, A, Takahashi, Y, Takeda, H, Takeshita, T, Tamsett, M, Tan, C L A, Tanaka, S, Tapprogge, S, Tarem, S, Tarem, Z, Taylor, C, Taylor, R P, Teixeira-Dias, P, Thomas, J P, Thompson, P D, Tokushuku, K, Tollefson, K, Tomoto, M, Topfel, C, Torrence, E, Touchard, F, Tremblet, L, Tripiana, M, Triplett, N, Tsulaia, V, Tsuno, S, Ünel, G, Urquijo, P, Urrejola, P, Usai, G, Vachon, B, Vandelli, W, Vari, R, Vaz-Gil-Lopes, L, Veneziano, S, Ventura, A, Vercesi, V, Vermeulen, J C, Von Der Schmitt, J, Vorwerk, V, Wang, M, Watkins, P M, Watson, A T, Weber, P, Weidberg, T, Wengler, T, Werner, P, Werth, M, Wessels, M, Wheeler-Ellis, S, White, M, Whiteson, D, Wickens, F J, Wiedenmann, W, Wielers, M, Wildt, M, Wilkens, H, Winklmeier, F, Wu, S-L, Wu, X, Xaplanteris Karampatsos, L, Xella, S, Yakovlev, A, Yamazaki, Y, Yang, U, Yasu, Y, Young, C, Zaitsev, A, Zanello, L, Zema, F, Zhang, J, Zhao, L, Zobernig, H, and Zur Nedden, M

Subjects
Detectors and Experimental Techniques
Abstract

This is the ATLAS Trigger/DAQ Authorlist, version 2.0, 31 July 2009

Published
2009

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