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2,964 results on '"Mészáros, P"'

601. The Open Cluster Chemical Analysis and Mapping Survey: Local Galactic Metallicity Gradient with APOGEE using SDSS DR10

Author

Frinchaboy, Peter M., Thompson, Benjamin, Jackson, Kelly M., O'Connell, Julia, Meyer, Brianne, Zasowski, Gail, Majewski, Steven R., Chojnowksi, S. Drew, Johnson, Jennifer A., Prieto, Carlos Allende, Beers, Timothy C., Bizyaev, Dmitry, Brewington, Howard, Cunha, Katia, Ebelke, Garrett, Perez, Ana Elia Garcia, Hearty, Frederick R., Holtzman, Jon, Kinemuchi, Karen, Malanushenko, Elena, Malanushenko, Viktor, Marchante, Moses, Meszaros, Szabolcs, Muna, Demitri, Nidever, David L., Oravetz, Daniel, Pan, Kaike, Schiavon, Ricardo P., Schneider, Donald P., Shetrone, Matthew, Simmons, Audrey, Snedden, Stephanie, Smith, Verne V., and Wilson, John C.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

The Open Cluster Chemical Analysis and Mapping (OCCAM) Survey aims to produce a comprehensive, uniform, infrared-based dataset for hundreds of open clusters, and constrain key Galactic dynamical and chemical parameters from this sample. This first contribution from the OCCAM survey presents analysis of 141 members stars in 28 open clusters with high-resolution metallicities derived from a large uniform sample collected as part of the SDSS-III/Apache Point Observatory Galactic Evolution Experiment (APOGEE). This sample includes the first high-resolution metallicity measurements for 22 open clusters. With this largest ever uniformly observed sample of open cluster stars we investigate the Galactic disk gradients of both [M/H] and [alpha/M]. We find basically no gradient across this range in [alpha/M], but [M/H] does show a gradient for R_{GC} < 10 kpc and a significant flattening beyond R_{GC} = 10 kpc. In particular, whereas fitting a single linear trend yields an [M/H] gradient of -0.09 +/- 0.03$ dex/kpc --- similar to previously measure gradients inside 13 kpc --- by independently fitting inside and outside 10 kpc separately we find a significantly steeper gradient near the Sun (7.9 <= R_{GC} <= 10) than previously found (-0.20 +/- 0.08 dex/kpc) and a nearly flat trend beyond 10 kpc (-0.02 +/- 0.09 dex/kpc)., Comment: 6 pages, 4 figures, ApJ letters, in press

Published
2013
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602. Photon and Neutrino Spectra of Time-Dependent Photospheric Models of Gamma-Ray Bursts

Author

Asano, K. and Mészáros, P.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Phenomenology
Abstract

Thermal photons from the photosphere may be the primary source of the observed prompt emission of gamma-ray bursts (GRBs). In order to produce the observed non-thermal spectra, some kind of dissipation mechanism near the photosphere is required. In this paper we numerically simulate the evolution of the photon spectrum in a relativistically expanding shell with a time-dependent numerical code. We consider two basic models. One is a leptonic model, where a dissipation mechanism heats the thermal electrons maintaining their high temperature. The other model involves a cascade process induced by $pp$($pn$)-collisions which produce high-energy electrons, modify the thermal spectrum, and emit neutrinos. The qualitative properties of the photon spectra are mainly determined by the optical depth at which the dissipation mechanism sets in. Too large optical depths lead to a broad and curved spectrum contradicting the observations, while for optical depths smaller than unity the spectral hardness becomes softer than observed. A significant shift of the spectral peak energy to higher energies due to a large energy injection can lead to an overly broad spectral shape. We show ideal parameter ranges for which these models are able to reproduce the observed spectra. For the $pn$-collision model, the neutrino fluence in the 10-100 GeV range is well above the atmospheric neutrino fluence, but its detection is challenging for presently available detectors., Comment: 21 pages, 13 figures. Accepted for publication in JCAP

Published
2013
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603. Target Selection for the Apache Point Observatory Galactic Evolution Experiment (APOGEE)

Author

Zasowski, G., Johnson, Jennifer A., Frinchaboy, P. M., Majewski, S. R., Nidever, D. L., Pinto, H. J. Rocha, Girardi, L., Andrews, B., Chojnowski, S. D., Cudworth, K. M., Jackson, K., Munn, J., Skrutskie, M. F., Beaton, R. L., Blake, C. H., Covey, K., Deshpande, R., Epstein, C., Fabbian, D., Fleming, S. W., Hernandez, A. Garcia, Herrero, A., Mahadevan, S., Meszaros, Sz., Schultheis, M., Sellgren, K., Terrien, R., van Saders, J., Prieto, C. Allende, Bizyaev, D., Burton, A., Cunha, K., da Costa, L. N., Hasselquist, S., Hearty, F., Holtzman, J., Perez, A. E. Garcia, Maia, M. A. G., O'Connell, R. W., O'Donnell, C., Pinsonneault, M., Santiago, B. X., Schiavon, R. P., Shetrone, M., Smith, V., and Wilson, J. C.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

The Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution infrared spectroscopic survey spanning all Galactic environments (i.e., bulge, disk, and halo), with the principal goal of constraining dynamical and chemical evolution models of the Milky Way. APOGEE takes advantage of the reduced effects of extinction at infrared wavelengths to observe the inner Galaxy and bulge at an unprecedented level of detail. The survey's broad spatial and wavelength coverage enables users of APOGEE data to address numerous Galactic structure and stellar populations issues. In this paper we describe the APOGEE targeting scheme and document its various target classes to provide the necessary background and reference information to analyze samples of APOGEE data with awareness of the imposed selection criteria and resulting sample properties. APOGEE's primary sample consists of ~100,000 red giant stars, selected to minimize observational biases in age and metallicity. We present the methodology and considerations that drive the selection of this sample and evaluate the accuracy, efficiency, and caveats of the selection and sampling algorithms. We also describe additional target classes that contribute to the APOGEE sample, including numerous ancillary science programs, and we outline the targeting data that will be included in the public data releases., Comment: Accepted to AJ. 31 pages, 11 figures

Published
2013
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604. Cosmological Fast Radio Bursts from Binary White Dwarf Mergers

Author

Kashiyama, Kazumi, Ioka, Kunihito, and Mészáros, Peter

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Recently, Thornton et al. reported the detection of four fast radio bursts (FRBs). The dispersion measures indicate that the sources of these FRBs are at cosmological distance. Given the large full sky event rate ~ 10^4 sky^-1 day^-1, the FRBs are a promising target for multi-messenger astronomy. Here we propose double degenerate, binary white-dwarf (WD) mergers as the source of FRBs, which are produced by coherent emission from the polar region of a rapidly rotating, magnetized massive WD formed after the merger. The basic characteristics of the FRBs, such as the energetics, emission duration and event rate, can be consistently explained in this scenario. As a result, we predict that some FRBs can accompany type Ia supernovae (SNe Ia) or X-ray debris disks. Simultaneous detection could test our scenario and probe the progenitors of SNe Ia, and moreover would provide a novel constraint on the cosmological parameters. We strongly encourage future SN and X-ray surveys that follow up FRBs., Comment: 5 pages, 1 figure, published in ApJL (submitted on 07/29/2013)

Published
2013
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605. The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment

Author

Ahn, Christopher P., Alexandroff, Rachael, Prieto, Carlos Allende, Anders, Friedrich, Anderson, Scott F., Anderton, Timothy, Andrews, Brett H., Aubourg, Éric, Bailey, Stephen, Bastien, Fabienne A., Bautista, Julian E., Beers, Timothy C., Beifiori, Alessandra, Bender, Chad F., Berlind, Andreas A., Beutler, Florian, Bhardwaj, Vaishali, Bird, Jonathan C., Bizyaev, Dmitry, Blake, Cullen H., Blanton, Michael R., Blomqvist, Michael, Bochanski, John J., Bolton, Adam S., Borde, Arnaud, Bovy, Jo, Bradley, Alaina Shelden, Brandt, W. N., Brauer, Dorothée, Brinkmann, J., Brownstein, Joel R., Busca, Nicolás G., Carithers, William, Carlberg, Joleen K., Carnero, Aurelio R., Carr, Michael A., Chiappini, Cristina, Chojnowski, S. Drew, Chuang, Chia-Hsun, Comparat, Johan, Crepp, Justin R., Cristiani, Stefano, Croft, Rupert A. C., Cuesta, Antonio J., Cunha, Katia, da Costa, Luiz N., Dawson, Kyle S., De Lee, Nathan, Dean, Janice D. R., Delubac, Timothée, Deshpande, Rohit, Dhital, Saurav, Ealet, Anne, Ebelke, Garrett L., Edmondson, Edward M., Eisenstein, Daniel J., Epstein, Courtney R., Escoffier, Stephanie, Esposito, Massimiliano, Evans, Michael L., Fabbian, D., Fan, Xiaohui, Favole, Ginevra, Castellá, Bruno Femenía, Alvar, Emma Fernández, Feuillet, Diane, Ak, Nurten Filiz, Finley, Hayley, Fleming, Scott W., Font-Ribera, Andreu, Frinchaboy, Peter M., Galbraith-Frew, J. G., García-Hernández, D. A., Pérez, Ana E. García, Ge, Jian, Génova-Santos, R., Gillespie, Bruce A., Girardi, Léo, Hernández, Jonay I. González, Gott III, J. Richard, Gunn, James E., Guo, Hong, Halverson, Samuel, Harding, Paul, Harris, David W., Hasselquist, Sten, Hawley, Suzanne L., Hayden, Michael, Hearty, Frederick R., Davó, Artemio Herrero, Ho, Shirley, Hogg, David W., Holtzman, Jon A., Honscheid, Klaus, Huehnerhoff, Joseph, Ivans, Inese I., Jackson, Kelly M., Jiang, Peng, Johnson, Jennifer A., Kirkby, David, Kinemuchi, K., Klaene, Mark A., Kneib, Jean-Paul, Koesterke, Lars, Lan, Ting-Wen, Lang, Dustin, Goff, Jean-Marc Le, Lee, Khee-Gan, Lee, Young Sun, Long, Daniel C., Loomis, Craig P., Lucatello, Sara, Lupton, Robert H., Ma, Bo, Mack III, Claude E., Mahadevan, Suvrath, Maia, Marcio A. G., Majewski, Steven R., Malanushenko, Elena, Malanushenko, Viktor, Manchado, A., Manera, Marc, Maraston, Claudia, Margala, Daniel, Martell, Sarah L., Masters, Karen L., McBride, Cameron K., McGreer, Ian D., McMahon, Richard G., Ménard, Brice, Mészáros, Sz., Miralda-Escudé, Jordi, Miyatake, Hironao, Montero-Dorta, Antonio D., Montesano, Francesco, More, Surhud, Morrison, Heather L., Muna, Demitri, Munn, Jeffrey A., Myers, Adam D., Nguyen, Duy Cuong, Nichol, Robert C., Nidever, David L., Noterdaeme, Pasquier, Nuza, Sebastián E., O'Connell, Julia E., O'Connell, Robert W., O'Connell, Ross, Olmstead, Matthew D., Oravetz, Daniel J., Owen, Russell, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Pan, Kaike, Parejko, John K., Pâris, Isabelle, Pepper, Joshua, Percival, Will J., Pérez-Ràfols, Ignasi, Perottoni, Hélio Dotto, Petitjean, Patrick, Pieri, Matthew M., Pinsonneault, M. H., Prada, Francisco, Price-Whelan, Adrian M., Raddick, M. Jordan, Rahman, Mubdi, Rebolo, Rafael, Reid, Beth A., Richards, Jonathan C., Riffel, Rogério, Robin, Annie C., Rocha-Pinto, H. J., Rockosi, Constance M., Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Roy, Arpita, Rubiño-Martin, J. A., Sabiu, Cristiano G., Sánchez, Ariel G., Santiago, Basílio, Sayres, Conor, Schiavon, Ricardo P., Schlegel, David J., Schlesinger, Katharine J., Schmidt, Sarah J., Schneider, Donald P., Schultheis, Mathias, Sellgren, Kris, Seo, Hee-Jong, Shen, Yue, Shetrone, Matthew, Shu, Yiping, Simmons, Audrey E., Skrutskie, M. F., Slosar, Anže, Smith, Verne V., Snedden, Stephanie A., Sobeck, Jennifer S., Sobreira, Flavia, Stassun, Keivan G., Steinmetz, Matthias, Strauss, Michael A., Streblyanska, Alina, Suzuki, Nao, Swanson, Molly E. C., Terrien, Ryan C., Thakar, Aniruddha R., Thomas, Daniel, Thompson, Benjamin A., Tinker, Jeremy L., Tojeiro, Rita, Troup, Nicholas W., Vandenberg, Jan, Magaña, Mariana Vargas, Viel, Matteo, Vogt, Nicole P., Wake, David A., Weaver, Benjamin A., Weinberg, David H., Weiner, Benjamin J., White, Martin, White, Simon D. M., Wilson, John C., Wisniewski, John P., Wood-Vasey, W. M., Yèche, Christophe, York, Donald G., Zamora, O., Zasowski, Gail, Zehavi, Idit, Zheng, Zheng, and Zhu, Guangtun

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

The Sloan Digital Sky Survey (SDSS) has been in operation since 2000 April. This paper presents the tenth public data release (DR10) from its current incarnation, SDSS-III. This data release includes the first spectroscopic data from the Apache Point Observatory Galaxy Evolution Experiment (APOGEE), along with spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS) taken through 2012 July. The APOGEE instrument is a near-infrared R~22,500 300-fiber spectrograph covering 1.514--1.696 microns. The APOGEE survey is studying the chemical abundances and radial velocities of roughly 100,000 red giant star candidates in the bulge, bar, disk, and halo of the Milky Way. DR10 includes 178,397 spectra of 57,454 stars, each typically observed three or more times, from APOGEE. Derived quantities from these spectra (radial velocities, effective temperatures, surface gravities, and metallicities) are also included.DR10 also roughly doubles the number of BOSS spectra over those included in the ninth data release. DR10 includes a total of 1,507,954 BOSS spectra, comprising 927,844 galaxy spectra; 182,009 quasar spectra; and 159,327 stellar spectra, selected over 6373.2 square degrees., Comment: 15 figures; 1 table. Accepted to ApJS. DR10 is available at http://www.sdss3.org/dr10 v3 fixed 3 diacritic markings in the arXiv HTML listing of the author names

Published
2013
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606. How to decompose a permutation into a pair of labeled Dyck paths by playing a game

Author

Billera, Louis J., Levine, Lionel, and Meszaros, Karola

Subjects
Mathematics - Combinatorics, Computer Science - Computer Science and Game Theory, Mathematics - Probability, 05A05, 05A15, 91A10
Abstract

We give a bijection between permutations of length 2n and certain pairs of Dyck paths with labels on the down steps. The bijection arises from a game in which two players alternate selecting from a set of 2n items: the permutation encodes the players' preference ordering of the items, and the Dyck paths encode the order in which items are selected under optimal play. We enumerate permutations by certain statistics, AA inversions and BB inversions, which have natural interpretations in terms of the game. We give new proofs of classical identities such as \sum_p \prod_{i=1}^n q^{h_i -1} [h_i]_q = [1]_q [3]_q ... [2n-1]_q where the sum is over all Dyck paths p of length 2n, and the h_i are the heights of the down steps of p., Comment: 9 pages, 1 figure

Published
2013

607. The Fly's Eye Camera System -- an instrument design for large \'etendue time-domain survey

Author

Pál, András, Mészáros, László, Csépány, Gergely, Jaskó, Attila, Schlaffer, Ferenc, Vida, Krisztián, Mező, György, Döbrentei, László, Farkas, Ernő, Kiss, Csaba, Oláh, Katalin, and Regály, Zsolt

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

In this paper we briefly summarize the design concepts of the Fly's Eye Camera System, a proposed high resolution all-sky monitoring device which intends to perform high cadence time domain astronomy in multiple optical passbands while still accomplish a high \'etendue. Fundings have already been accepted by the Hungarian Academy of Sciences in order to design and build a Fly's Eye device unit. Beyond the technical details and the actual scientific goals, this paper also discusses the possibilities and yields of a network operation involving ~10 sites distributed geographically in a nearly homogeneous manner. Currently, we expect to finalize the mount assembly -- that performs the sidereal tracking during the exposures -- until the end of 2012 and to have a working prototype with a reduced number of individual cameras sometimes in the spring or summer of 2013., Comment: Accepted for publication in AN, 4.05 pages. Website of the project: http://flyseye.net/

Published
2013
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608. A curious relation between the flat cosmological model and the elliptic integral of the first kind

Author

Meszaros, A. and Ripa, J.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The dependence of the luminosity distance on the redshift has a key importance in the cosmology. This dependence can well be given by standard functions for the zero cosmological constant. The purpose of this article is to present such a relation also for the non-zero cosmological constant, if the universe is spatially flat. A definite integral is used. The integration ends in the elliptic integral of the first kind. The result shows that no numerical integration is needed for the non-zero cosmological constant, if the universe is spatially flat., Comment: Accepted for publication in Astronomy & Astrophysics. 2 pages

Published
2013
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609. Observation of the cosmic-ray shadow of the Moon with IceCube

Author

IceCube Collaboration, Aartsen, M. G., Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Bertrand, D., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohaichuk, S., Bohm, C., Bose, D., Böser, S., Botner, O., Brayeur, L., Bretz, H. -P., Brown, A. M., Bruijn, R., Brunner, J., Carson, M., Casey, J., Casier, M., Chirkin, D., Christov, A., Christy, B., Clark, K., Clevermann, F., Coenders, S., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., De Ridder, S., Desiati, P., de With, M., DeYoung, T., Díaz-Vélez, J. C., Dunkman, M., Eagan, R., Eberhardt, B., Eisch, J., Ellsworth, R. W., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Goodman, J. A., Góra, D., Grandmont, D. T., Grant, D., Groß, A., Ha, C., Ismail, A. Haj, Hallen, P., Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Jagielski, K., Japaridze, G. S., Jero, K., Jlelati, O., Kaminsky, B., Kappes, A., Karg, T., Karle, A., Kelley, J. L., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Krings, K., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Landsman, H., Larson, M. J., Lesiak-Bzdak, M., Leuermann, M., Leute, J., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pfendner, C., Pieloth, D., Pinat, E., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rameez, M., Rawlins, K., Redl, P., Reimann, R., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Sestayo, Y., Seunarine, S., Sheremata, C., Smith, M. W. E., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Tepe, A., Ter-Antonyan, S., Tešić, G., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Waldenmaier, T., Wallraff, M., Wasserman, R., Weaver, Ch., Wellons, M., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., and Zoll, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report on the observation of a significant deficit of cosmic rays from the direction of the Moon with the IceCube detector. The study of this "Moon shadow" is used to characterize the angular resolution and absolute pointing capabilities of the detector. The detection is based on data taken in two periods before the completion of the detector: between April 2008 and May 2009, when IceCube operated in a partial configuration with 40 detector strings deployed in the South Pole ice, and between May 2009 and May 2010 when the detector operated with 59 strings. Using two independent analysis methods, the Moon shadow has been observed to high significance (> 6 sigma) in both detector configurations. The observed location of the shadow center is within 0.2 degrees of its expected position when geomagnetic deflection effects are taken into account. This measurement validates the directional reconstruction capabilities of IceCube., Comment: Submitted to Physical Review D

Published
2013
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610. Sub-PeV Neutrinos from TeV Unidentified Sources in the Galaxy

Author

Fox, D. B., Kashiyama, K., and Meszaros, P.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract

The IceCube collaboration discovery of 28 high-energy neutrinos over the energy range 30 TeV <~ E_nu <~ 1 PeV, a 4.3-sigma excess over expected backgrounds, represents the first high-confidence detection of cosmic neutrinos at these energies. In light of this discovery, we explore the possibility that some of the Sub-PeV cosmic neutrinos might originate in our Galaxy's TeV unidentified (TeV UnID) sources. While typically resolved at TeV energies, these sources lack prominent radio or X-ray counterparts, and so have been considered promising sites for hadron acceleration within our Galaxy. Modeling the TeV UnID sources as Galactic hypernova remnants, we predict Sub-PeV neutrino fluxes and spectra consistent with their contributing a minority of n_nu <~ 2 of the observed events. This is consistent with our analysis of the spatial distribution of the Sub-PeV neutrinos and TeV UnID sources, which finds that a best-fit of one, and maximum of 3.8 (at 90%-confidence), of the ~16 non-atmospheric Sub-PeV neutrinos may originate in TeV UnID sources, with the remaining 75% to 95% of events being drawn from an isotropic background. If our scenario is correct, we expect excess Sub-PeV neutrinos to accumulate along the Galactic plane, within |l| <~ 30 deg of the Galactic center and in the Cygnus region, as observations by IceCube and other high-energy neutrino facilities go forward. Our scenario also has implications for radio, X-ray, and TeV observations of the TeV UnID sources., Comment: Submitted to ApJ. 17 pages, 2 figures. v3: Revised analysis, conclusions; further references v2: Corrected typos, added references

Published
2013
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611. On the neutrino non-detection of GRB 130427A

Author

Gao, Shan, Kashiyama, Kazumi, and Meszaros, Peter

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Phenomenology
Abstract

The recent gamma-ray burst GRB 130427A has an isotropic electromagnetic energy $E^{iso}\sim10^{54}$ erg, suggesting an ample supply of target photons for photo-hadronic interactions, which at its low redshift of $z\sim0.34$ would appear to make it a promising candidate for neutrino detection. However, the IceCube collaboration has reported a null result based on a search during the prompt emission phase. We show that this neutrino non-detection can provide valuable information about this GRB's key physical parameters such as the emission radius $R_{d}$, the bulk Lorentz factor $\Gamma$ and the energy fraction converted into cosmic rays $\epsilon_{p}$. The results are discussed both in a model-independent way and in the specific scenarios of an internal shock model (IS), a baryonic photospheric model (BPH) and magnetic photospheric model (MPH). We find that the constraints are most stringent for the magnetic photospheric model considered, but the constraints on the internal shock and the baryonic photosphere models are fairly modest., Comment: 5 pages, 4 figures, version accepted for publication in ApJ(Lett)

Published
2013
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612. First observation of PeV-energy neutrinos with IceCube

Author

IceCube Collaboration, Aartsen, M. G., Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Bertrand, D., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohaichuk, S., Bohm, C., Bose, D., Böser, S., Botner, O., Brayeur, L., Bretz, H. -P., Brown, A. M., Bruijn, R., Brunner, J., Carson, M., Casey, J., Casier, M., Chirkin, D., Christov, A., Christy, B., Clark, K., Clevermann, F., Coenders, S., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., De Ridder, S., Desiati, P., de With, M., DeYoung, T., Díaz-Vélez, J. C., Dunkman, M., Eagan, R., Eberhardt, B., Eisch, J., Ellsworth, R. W., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Goodman, J. A., Góra, D., Grant, D., Groß, A., Gurtner, M., Ha, C., Ismail, A. Haj, Hallen, P., Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Jagielski, K., Japaridze, G. S., Jero, K., Jlelati, O., Kaminsky, B., Kappes, A., Karg, T., Karle, A., Kelley, J. L., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Krings, K., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Landsman, H., Larson, M. J., Lesiak-Bzdak, M., Leuermann, M., Leute, J., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pfendner, C., Pieloth, D., Pinat, E., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rameez, M., Rawlins, K., Redl, P., Reimann, R., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Sestayo, Y., Seunarine, S., Sheremata, C., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tešić, G., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Waldenmaier, T., Wallraff, M., Wasserman, R., Weaver, Ch., Wellons, M., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., Zilles, A., and Zoll, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract

We report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04 $\pm$ 0.16 and 1.14 $\pm$ 0.17 PeV, respectively, the highest neutrino energies observed so far. These events are consistent with fully contained particle showers induced by neutral-current $\nu_{e,\mu,\tau}$ ($\bar\nu_{e,\mu,\tau}$) or charged-current $\nu_{e}$ ($\bar\nu_{e}$) interactions within the IceCube detector. The events were discovered in a search for ultra-high energy neutrinos using data corresponding to 615.9 days effective livetime. The expected number of atmospheric background is $0.082 \pm 0.004 \text{(stat)}^{+0.041}_{-0.057} \text{(syst)}$. The probability to observe two or more candidate events under the atmospheric background-only hypothesis is $2.9\times10^{-3}$ ($2.8\sigma$) taking into account the uncertainty on the expected number of background events. These two events could be a first indication of an astrophysical neutrino flux, the moderate significance, however, does not permit a definitive conclusion at this time., Comment: 7 pages, 5 figures, 1 table, accepted for publication in Physical Review Letters

Published
2013
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613. Neutron-Proton-Converter Acceleration Mechanism at Subphotospheres of Relativistic Outflows

Author

Kashiyama, Kazumi, Murase, Kohta, and Mészáros, Peter

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Phenomenology
Abstract

We study a type of particle acceleration that operates via neutron-proton conversion in inelastic nuclear collisions. This mechanism can be expected for relativistic shocks at subphotospheres if relativistic outflows contain neutrons. Using a test-particle approximation, we numerically calculate the energy spectrum and the efficiency of accelerated particles, and show that a good energy fraction of the nucleons can be accelerated. This mechanism may especially be relevant if the shock is radiation-mediated, and it would enhance the detectability of GeV-TeV neutrinos., Comment: 5 pages, 3 figures, published in PRL (submitted on 04/06/2013)

Published
2013
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614. Dependence of the optical brightness on the gamma and X-ray properties of GRBs

Author

Balázs, L. G., Bagoly, Z., Horvath, I., Kóbori, J., Szécsi, D., and Mészáros, A.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The Swift satellite made a real break through with measuring simultaneously the gamma X-ray and optical data of GRBs, effectively. Although, the satellite measures the gamma, X-ray and optical properties almost in the same time a significant fractions of GRBs remain undetected in the optical domain. In a large number of cases only an upper bound is obtained. Survival analysis is a tool for studying samples where a part of the cases has only an upper (lower) limit. The obtained survival function may depend on some other variables. The Cox regression is a way to study these dependencies. We studied the dependence of the optical brightness (obtained by the UVOT) on the gamma and X-ray properties, measured by the BAT and XRT on board of the Swift satellite. We showed that the gamma peak flux has the greatest impact on the afterglow's optical brightness while the gamma photon index and the X-ray flux do not. This effect probably originates in the energetics of the jet launched from the central engine of the GRB which triggers the afterglow., Comment: 2012 Fermi Symposium proceedings - eConf C121028

Published
2013

615. Advantage in the discrete Voronoi game

Author

Gerbner, Dániel, Mészáros, Viola, Pálvölgyi, Dömötör, Pokrovskiy, Alexey, and Rote, Günter

Subjects
Mathematics - Combinatorics, Computer Science - Discrete Mathematics
Abstract

We study the discrete Voronoi game, where two players alternately claim vertices of a graph for t rounds. In the end, the remaining vertices are divided such that each player receives the vertices that are closer to his or her claimed vertices. We prove that there are graphs for which the second player gets almost all vertices in this game, but this is not possible for bounded-degree graphs. For trees, the first player can get at least one quarter of the vertices, and we give examples where she can get only little more than one third of them. We make some general observations, relating the result with many rounds to the result for the one-round game on the same graph.

Published
2013
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616. Measurement of South Pole ice transparency with the IceCube LED calibration system

Author

IceCube Collaboration, Aartsen, M. G., Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Bertrand, D., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohaichuk, S., Bohm, C., Bose, D., Böser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Buitink, S., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clark, K., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., De Ridder, S., Desiati, P., de With, M., DeYoung, T., Díaz-Vélez, J. C., Dunkman, M., Eagan, R., Eberhardt, B., Eisch, J., Ellsworth, R. W., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Goodman, J. A., Góra, D., Grant, D., Groß, A., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jero, K., Jlelati, O., Kaminsky, B., Kappes, A., Karg, T., Karle, A., Kelley, J. L., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Landsman, H., Larson, M. J., Lesiak-Bzdak, M., Leute, J., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pfendner, C., Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönherr, L., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Sheremata, C., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Waldenmaier, T., Wallraff, M., Wasserman, R., Weaver, Ch., Wellons, M., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., Zilles, A., and Zoll, M.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract

The IceCube Neutrino Observatory, approximately 1 km^3 in size, is now complete with 86 strings deployed in the Antarctic ice. IceCube detects the Cherenkov radiation emitted by charged particles passing through or created in the ice. To realize the full potential of the detector, the properties of light propagation in the ice in and around the detector must be well understood. This report presents a new method of fitting the model of light propagation in the ice to a data set of in-situ light source events collected with IceCube. The resulting set of derived parameters, namely the measured values of scattering and absorption coefficients vs. depth, is presented and a comparison of IceCube data with simulations based on the new model is shown.

Published
2013
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617. On the Interpolation of Model Atmospheres and High-Resolution Synthetic Stellar Spectra

Author

Mészáros, Sz. and Prieto, C. Allende

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We present tests carried out on optical and infrared stellar spectra to evaluate the accuracy of different types of interpolation. Both model atmospheres and continuum normalized fluxes were interpolated. In the first case we used linear interpolation, and in the second linear, cubic spline, cubic-Bezier and quadratic-Bezier methods. We generated 400 ATLAS9 model atmospheres with random values of the atmospheric parameters for these tests, spanning between -2.5 and +0.5 in [Fe/H], from 4500 to 6250 K in effective temperature, and 1.5 to 4.5 dex in surface gravity. Synthesized spectra were created from these model atmospheres, and compared with spectra derived by interpolation. We found that the most accurate interpolation algorithm among those considered in flux space is cubic-Bezier, closely followed by quadratic-Bezier and cubic splines. Linear interpolation of model atmospheres results in errors about a factor of two larger than linear interpolation of fluxes, and about a factor of four larger than high order flux interpolations., Comment: 14 pages, 5 figures, 1 table, accepted to MNRAS

Published
2013
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618. Subphotospheric Neutrinos from Gamma-Ray Bursts: The Role of Neutrons

Author

Murase, Kohta, Kashiyama, Kazumi, and Meszaros, Peter

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Extragalactic Astrophysics, High Energy Physics - Phenomenology
Abstract

Relativistic outflows with neutrons inevitably lead to inelastic collisions, and resulting subphotospheric gamma rays may explain prompt emission of gamma-ray bursts. In this model, hadronuclear, quasithermal neutrinos in the 10-100 GeV range should be generated, and they may even have a high-energy tail by neutron-proton-converter or shock acceleration mechanisms. We demonstrate the importance of dedicated searches with DeepCore+IceCube, though such analyses have not been performed. Successful detections enable us to discriminate among prompt emission mechanisms, probe the jet composition, and see roles of relativistic neutrons as well as effects of cosmic-ray acceleration., Comment: 5 pages, 4 figures, published in PRL (submitted on 01/17/2013)

Published
2013
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619. Very Metal-poor Stars in the Outer Galactic Bulge Found by the Apogee Survey

Author

Pérez, Ana E. García, Cunha, Katia, Shetrone, Matthew, Majewski, Steven R., Johnson, Jennifer A., Smith, Verne V., Schiavon, Ricardo P., Holtzman, Jon, Nidever, David, Zasowski, Gail, Prieto, Carlos Allende, Beers, Timothy C., Bizyaev, Dmitry, Ebelke, Garrett, Eisenstein, Daniel J., Frinchaboy, Peter M., Girardi, Léo, Hearty, Fred R., Malanushenko, Elena, Malanushenko, Viktor, Meszaros, Szabolcs, O'Connel, Robert W., Oravetz, Daniel, Pan, Kaike, Robin, Annie C., Schneider, Donald P., Schultheis, Mathias, Skrutskie, Michael F., Simmonsand, Audrey, and Wilson, John C.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

Despite its importance for understanding the nature of early stellar generations and for constraining Galactic bulge formation models, at present little is known about the metal-poor stellar content of the central Milky Way. This is a consequence of the great distances involved and intervening dust obscuration, which challenge optical studies. However, the Apache Point Observatory Galactic Evolution Experiment (APOGEE), a wide-area, multifiber, high-resolution spectroscopic survey within Sloan Digital Sky Survey III (SDSS-III), is exploring the chemistry of all Galactic stellar populations at infrared wavelengths, with particular emphasis on the disk and the bulge. An automated spectral analysis of data on 2,403 giant stars in twelve fields in the bulge obtained during APOGEE commissioning yielded five stars with low metallicity([Fe/H]$\le-1.7$), including two that are very metal-poor [Fe/H]$\sim-2.1$ by bulge standards. Luminosity-based distance estimates place the five stars within the outer bulge, where other 1,246 of the analyzed stars may reside. A manual reanalysis of the spectra verifies the low metallicities, and finds these stars to be enhanced in the $\alpha$-elements O, Mg, and Si without significant $\alpha$-pattern differences with other local halo or metal-weak thick-disk stars of similar metallicity, or even with other more metal-rich bulge stars. While neither the kinematics nor chemistry of these stars can yet definitively determine which, if any, are truly bulge members, rather than denizens of other populations co-located with the bulge, the newly-identified stars reveal that the chemistry of metal-poor stars in the central Galaxy resembles that of metal-weak thick-disk stars at similar metallicity., Comment: 6 pages, 3 figures, 2 tables

Published
2013
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620. Exploring the circumstellar environment of the young eruptive star V2492 Cyg

Author

Kóspál, Á., Ábrahám, P., Acosta-Pulido, J. A., Morales, M. J. Arévalo, Balog, Z., Carnerero, M. I., Szegedi-Elek, E., Farkas, A., Henning, Th., Kelemen, J., Kovács, T., Kun, M., Marton, G., Mészáros, Sz., Moór, A., Pál, A., Sárneczky, K., Szakáts, R., Szalai, N., Szing, A., Tóth, I., Turner, N. J., and Vida, K.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

Context. V2492 Cyg is a young eruptive star that went into outburst in 2010. The near-infrared color changes observed since the outburst peak suggest that the source belongs to a newly defined sub-class of young eruptive stars, where time-dependent accretion and variable line-of-sight extinction play a combined role in the flux changes. Aims. In order to learn about the origin of the light variations and to explore the circumstellar and interstellar environment of V2492 Cyg, we monitored the source at ten different wavelengths, between 0.55 \mu m and 2.2 \mu m from the ground and between 3.6 \mu m and 160 \mu m from space. Methods. We analyze the light curves and study the color-color diagrams via comparison with the standard reddening path. We examine the structure of the molecular cloud hosting V2492 Cyg by computing temperature and optical depth maps from the far-infrared data. Results. We find that the shapes of the light curves at different wavelengths are strictly self-similar and that the observed variability is related to a single physical process, most likely variable extinction. We suggest that the central source is episodically occulted by a dense dust cloud in the inner disk, and, based on the invariability of the far-infrared fluxes, we propose that it is a long-lived rather than a transient structure. In some respects, V2492 Cyg can be regarded as a young, embedded analog of UX Orionis-type stars. Conclusions. The example of V2492 Cyg demonstrates that the light variations of young eruptive stars are not exclusively related to changing accretion. The variability provided information on an azimuthally asymmetric structural element in the inner disk. Such an asymmetric density distribution in the terrestrial zone may also have consequences for the initial conditions of planet formation., Comment: 9 pages, 7 figures, 2 online tables, accepted for publication in A&A

Published
2013
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621. A profilozás könnyűségéről és nehézségéről – egy perspektivikus megközelítés

Author

József Haller, Attila Petőfi, and Kristóf Mészáros

Subjects
bűnözői profilalkotás, profilozási eljárások, célok, felhasználók, Political institutions and public administration (General), JF20-2112
Abstract

Folyó év őszén a Nemzeti Közszolgálati Egyetem (NKE) Rendészettudományi Kar Kriminálpszichológia Tanszéke és Kutatóműhelye egy konferenciát szervezett, amely a bűnözői profilalkotás témája köré szerveződött. A konferencia előadói részben a kérdéskör elméleti szakemberei közül verbuválódtak, részben azok közül a gyakorlati – nyomozati – szakemberek köréből, akik egy profilalkotási folyamatnak a megrendelői és egyben haszonélvezői lehetnének. A konferencia célja egy olyan párbeszéd kezdeményezése volt, amely párbeszéd nélkül a résztvevők egyöntetű véleménye szerint a magyar profilozási tevékenység nem újítható meg. A Belügyi Szemle jelen és következő lapszámában publikálja az előadások tanulmánnyá konvertált változatait. Ebben a tanulmányban tág perspektívában vizsgáljuk meg a kérdést, mintegy alapot teremtve a következő, részletkérdéseket kifejtő tanulmányok számára.

Published
2021
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622. Nanoanyagok humánbiztonsági kockázatot jelentő tulajdonságainak bemutatása és csoportosítása

Author

Eszter Járdán and Renáta Zákányiné Mészáros

Subjects
nanoanyag, humánbiztonság, egészségi kockázat, Technology, Industries. Land use. Labor, HD28-9999
Abstract

A nanoanyagok egyedi tulajdonságaik révén egyre szélesebb körű felhasználásnak örvendenek, amelyeknek köszönhetően számos iparág tevékenységében fellelhetők, térhódításuk továbbra is növekvő tendenciát mutat. Az ipari felhasználásuk az utóbbi néhány évtizedben lett számottevő. Ezen robbanásszerű fejlődés következtében hiányos ismeretekkel rendelkezünk az anyagok élő szervezetekre, valamint az emberi egészségre gyakorolt pontos hatásmechanizmusát illetően mind rövid-, mind pedig hosszútávon. A nanoanyagok számos különböző megjelenési formájukból, változatos fizikai és kémiai tulajdonságaikból adódóan különböző módokon juthatnak be az élő szervezetekbe, majd tovább a véráramba, a nyirokrendszerbe elérve az egyes szerveket és ott különböző egészségkárosító hatásokat előidézve súlyos megbetegedéseket okozhatnak. Hazánkban és az Európai Unióban jogi szabályozások tekintetében az érintett tématerület lefedettsége kezdetlegesnek mondható. Az anyagoknak való kitettség kockázatának vizsgálatához szintén nem áll rendelkezésünkre, olyan összefoglaló anyag, amely részletesen kitérne az egyes kockázati tényezőkre, vizsgálandó paraméterekre. Munkánk során célunk volt egy olyan szempontrendszer kialakítása, amely figyelembe veszi a nanoanyagok használata, illetve a velük való érintkezés során felmerülő kockázatokat az anyagok egyes tulajdonságai alapján - legyen az fizikai, kémiai vagy biológiai- , amely szempontrendszer a későbbiekben megfelelő kiindulási alapot biztosíthat a munkavédelmi kockázatértékelések elkészítése alkalmával, ezáltal biztonságosabbá téve az ezen anyagokkal való munkavégzést, a munkát végzők és a munkavégzés hatókörében jelenlévők számára egyaránt.

Published
2021
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623. Nanomagnetit-bentonit vizes közegű diszperz rendszereinek zeta-potenciáljának vizsgálata

Author

Ákos Pintér-Móricz and Renáta Zákányiné Mészáros

Subjects
nanomagnetit, bentonit, zeta-potenciál, Technology, Industries. Land use. Labor, HD28-9999
Abstract

Napjaink tudományos, ipari kihívásai között jelentős szerepet kap a különböző típusú nanoanyagok stabilitásának kérdésköre, melynek kapcsán ezen anyagok és azok elegyeinek diszperz részecskék felületi, elektromos felületi tulajdonságaira és aggregálódásának mértékére gyakorolt hatásának vizsgálata kulcsfontosságú. A bentonitot és különböző nanoanyagokkal képzett kompozitját gyakran alkalmazzák például a környezetvédelemben szennyvíztisztításra, mivel a nagy fajlagos felületük miatt kiváló szorpciós tulajdonságokkal bírnak. A bentonit fúróiszap adalékanyagként történő alkalmazására vonatkozóan számos publikáció fellelhető a szakirodalomban. Használatával csökkenthető a fluidumveszteség a fúrás során, növeli a fluidum filtrációját, javítja a reológiai tulajdonságokat és a formációkárosodás is csökkenthető. A kutatások során célszerű lehet különböző típusú nanorészecskék és azok elegyeinek zeta-potenciáljának vizsgálata és elemzése különböző pH értékeknél és sótartalomnál. Kísérleteink során laboratóriumi eljárás során szintetizált nanomagnetit (NM), kationcserélt mádi bentonit (Be), valamint ezen nanorészecskék elegyeinek elektromos felületi tulajdonságait vizsgálatuk. Vizsgáltunk különböző összetételű elegyeket (9:1, 7:3, 1:1, 3:7, 1:9) különböző töménységű (0.1 M – 0.0001 M) kálium-klorid oldatban. A meghatározott zeta-potenciál értékek segítségével kiválóan jellemezhető a felületen történő részecskemegkötődés, azaz a felületi töltések változása. A fenti rendszerek viselkedését a teljes pH tartományban figyelemmel követtük, amely során a kolloidikai stabilitás szempontjából értékes adatokat nyertünk. A stabilitás kapcsán gyakorlati szempontból többféle kívánalom felmerülhet, vannak olyan alkalmazási területek, ahol a kolloidikai szempontból stabil rendszer előnyös, bizonyos esetekben pedig a stabil rendszer megszüntetése a cél. Az általunk végzett vizsgálatok a stabilitás és annak jellemzése szempontjából kiemelt jelentőséggel bírnak

Published
2021
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624. Carbon Footprint Analysis of a Laboratory Plate Heat Exchanger Control

Author

Michaela Horváthová, Juraj Oravec, Monika Bakošová, and Alajos Mészáros

Subjects
Chemical engineering, TP155-156, Computer engineering. Computer hardware, TK7885-7895
Abstract

More than 100 countries worldwide have pledged carbon neutrality by 2050 to reduce the negative environmental impacts of carbon emissions. To reach this goal, every part of the industry must prepare to transform and take precautions. Heat exchangers are one of the most common parts of industrial production. The industrial operation of heat exchangers still offers lots of opportunities to minimize their carbon footprints. This goal can be achieved by their optimized operation. This work investigates the operation of a laboratory plate heat exchanger controlled by a proportional-integral-derivative (PID) controller and by an optimization-based model predictive controller (MPC). The analysis is performed using both, the simulations, and the laboratory experiments. The carbon footprint and energy consumption of the heat exchanger are analysed and compared. The paper investigates whether the optimization-based approach subject to the constraints on manipulated variables and controlled variables, considering economic criteria, simultaneously, reduces the carbon footprint of a laboratory heat exchanger control.

Published
2021
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625. Fuzzy Control Design for Energy Efficient Heat Exchanger Network

Author

Anna Vasickaninová, Monika Bakošová, and Alajos Mészáros

Subjects
Chemical engineering, TP155-156, Computer engineering. Computer hardware, TK7885-7895
Abstract

Increasing energy efficiency and decreasing power consumption play a substantial role in the modern industrial and technological world. Consequently, there are enhanced requirements on all production processes and especially on energy intensive processes. Heat exchangers (HEs) and heat exchanger networks (HENs) are very energy intensive processes and only their optimal operation assures efficient heat recovery. Advanced optimization and advanced control are tools for assuring the energetic efficacy of HEs or HENs. Between them, fuzzy logic control represents the advanced control strategy that has many applications in industry and advantages as it can be used for control of strongly non-linear processes and processes that are difficult to control because of asymmetric dynamics or uncertainties. The type-1 and type-2 fuzzy logic controllers (FLCs) designed for a small heat exchanger network (HEN) are compared in this paper using simulation results with the PI and PID controllers tuned by conventional methods. The controlled HEN was a combination of two heat exchangers in series and one in parallel to them. The best controller was the type-2 fuzzy logic controller (FLC). This controller assured the most efficient operation of HEN measured by the smallest coolant consumption. The coolant consumption increased exploiting the type-1 FLC by 2 %, the PI controller by 3 %, and the PID controller by 5 %.

Published
2021
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626. A kriminalisztika hipotézisei

Author

Bence Mészáros

Subjects
verzió, kriminalisztikai alapkérdések, verziók felállítása, gondolati rekonstrukció, Political institutions and public administration (General), JF20-2112
Abstract

A tanulmány a kriminalisztikában alkalmazott hipotézis, az úgynevezett verzió fogalmát, a kriminalisztikai alapkérdésekhez való viszonyát, valamint a verziók fajtáit mutatja be. A szerző a verzió felállításának folyamatát egy tágan értelmezett gondolati rekonstrukciónak tekinti, és felhívja a figyelmet az annak során érvényesülő legfontosabb alapelvre, a realitás elvére. Kitér a verziók felállítása és értékelése kapcsán gyakran hivatkozott Occam-borotvája filozófiai megközelítés alkalmazhatóságára is. A verziók versengésének bemutatását követően az egy kiválasztott verzióhoz ragaszkodás – mint tipikus nyomozási hiba – okait és hátrányos következményeit elemzi a szerző.

Published
2021
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627. We Should've Made a Revolution: A Critical Rhapsody of the Hungarian Education System's Catching-Up Revolutions since 1989

Author

Tóth, Tamás, Mészáros, György, and Marton, András

Abstract

From the perspective of the world-systems theory and post-colonial studies, the 1989 transition in Hungary was a part of the re-integration of former Soviet countries into an inferior position in the world system. The political-economic transition was in no sense a revolution, but a replacement of dictatorial/totalitarian state capitalism with neoliberal global capitalism. In this paper we will analyze how Hungary's semi-peripheral "catching-up revolution" consisted of stabilizing the neoliberal hegemony in education. As a result, one of the most decentralized, diverse, vertically, and horizontally stratified, and hence extremely selective education systems emerged from the gloomy Central-East European semi-periphery with exemplary diligence in conserving and reproducing social inequalities. Some 27 years after the transition, the teaching staff from Herman Ottó High School in Budapest wrote a public letter analyzing the problems of public education and criticizing the Hungarian government's interventions, which led to one of the country's biggest movements since the political-economic transition in 1989. To understand the conditions that led to these situations, wherein education under siege triggered the biggest protests since 1989, we will first describe how the Hungarian education system was affected by the political-economic transition. Second, we will point to a rupture in the post-socialist history of Hungary, namely the neoconservative interventions of Hungary's post-fascist, far-right government which has been in power since 2010. And lastly, we will try to place the teacher's movement (and, briefly, the pro-Central European University protests) in this post-socialist rhapsody by showing how they interweave with Hungary's forever lasting semi-peripheral catching-up revolution. In our conclusion we will try to propose a strategy drawing on Immanuel Wallerstein's idea of an anti-systemic Rainbow Coalition, by which new social and anti-systemic movements could organize their resistance more effectively.

Published
2018
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628. Gamma photometric redshifts for long gamma-ray bursts

Author

Bagoly, Z., Csabai, I., Mészáros, A., Mészáros, P., Horváth, I., Balázs, L. G., and Vavrek, R.

Subjects
Astrophysics
Abstract

It is known that the soft tail of the gamma-ray bursts' spectra show excesses from the exact power-law dependence. In this article we show that this departure can be detected in the peak flux ratios of different BATSE DISCSC energy channels. This effect allows to estimate the redshift of the bright long gamma-ray bursts in the BATSE Catalog. A verification of these redshifts is obtained for the 8 GRB which have both BATSE DISCSC data and measured optical spectroscopic redshifts. There is good correlation between the measured and esti redshifts, and the average error is $\Delta z \approx 0.33$. The method is similar to the photometric redshift estimation of galaxies in the optical range, hence it can be called as "gamma photometric redshift estimation". The estimated redshifts for the long bright gamma-ray bursts are up to $z \simeq 4$. For the the faint long bursts - which should be up to $z \simeq 20$ - the redshifts cannot be determined unambiguously with this method., Comment: accepted in A&A, 7 pages incl. 7 figures

Published
2002
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635. Metal Coordination and Biological Screening of a Schiff Base Derived from 8-Hydroxyquinoline and Benzothiazole

Author

Nádia Ribeiro, Pedro F. Farinha, Jacinta O. Pinho, Hugo Luiz, János P. Mészáros, Adelino M. Galvão, João Costa Pessoa, Éva A. Enyedy, Catarina Pinto Reis, Isabel Correia, and Maria Manuela Gaspar

Subjects
metal complexes, hydrazone, proton dissociation constants, albumin binding, colorectal cancer, in vitro studies, Pharmacy and materia medica, RS1-441
Abstract

Designing new metallodrugs for anticancer therapy is a driving force in the scientific community. Aiming to contribute to this field, we hereby report the development of a Schiff base (H2L) derived from the condensation of 2-carbaldehyde-8-hydroxyquinoline with 2-hydrazinobenzothiazole and its complexation with transition metal ions. All compounds were characterised by analytical and spectroscopic techniques, which disclosed their structure: [Cu(HL)Cl], [Cu(HL)2], [Ni(HL)(acetate)], [Ni(HL)2], [Ru(HL)Cl(DMSO)], [VO(HL)2] and [Fe(HL)2Cl(H2O)]. Different binding modes were proposed, showing the ligand’s coordination versatility. The ligand proton dissociation constants were determined, and the tested compounds showed high lipophilicity and light sensitivity. The stability of all complexes in aqueous media and their ability to bind to albumin were screened. Based on an antiproliferative in vitro screening, [Ni(HL)(acetate)] and [Ru(HL)Cl(DMSO)] were selected for further studies aiming to investigate their mechanisms of action and therapeutic potential towards colon cancer. The complexes displayed IC50 < 21 μM towards murine (CT-26) and human (HCT-116) colon cancer cell lines. Importantly, both complexes exhibited superior antiproliferative properties compared to the clinically approved 5-fluorouracil. [Ni(HL)(acetate)] induced cell cycle arrest in S phase in CT-26 cells. For [Ru(HL)Cl(DMSO)] this effect was observed in both colon cancer cell lines. Additionally, both compounds significantly inhibited cell migration particularly in the human colon cancer cell line, HCT-116. Overall, the therapeutic potential of both metal complexes was demonstrated.

Published
2022
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636. Effects of Hydroxypropyl-Beta-Cyclodextrin on Cultured Brain Endothelial Cells

Author

Szilvia Veszelka, Mária Mészáros, Gergő Porkoláb, Ágnes Rusznyák, Katalin Szászné Réti-Nagy, Mária A. Deli, Miklós Vecsernyés, Ildikó Bácskay, Judit Váradi, and Ferenc Fenyvesi

Subjects
blood–brain barrier, 2-hydroxypropyl-beta-cyclodextrin, endocytosis, Niemann–Pick disease, type C, Organic chemistry, QD241-441
Abstract

The application of 2-hydroxypropyl-beta-cyclodextrin (HPBCD) in the treatment of the rare cholesterol and lipid storage disorder Niemann–Pick disease type C opened new perspectives in the development of an efficient therapy. Even if the systemic administration of HPBCD was found to be effective, its low permeability across the blood–brain barrier (BBB) limited the positive neurological effects. Nevertheless, the cellular interactions of HPBCD with brain capillary endothelial cells have not been investigated in detail. In this study, the cytotoxicity, permeability, and cellular internalization of HPBCD on primary rat and immortalized human (hCMEC/D3) brain capillary endothelial cells were investigated. HPBCD shows no cytotoxicity on endothelial cells up to 100 µM, measured by impedance kinetics. Using a fluorescent derivative of HPBCD (FITC-HPBCD) the permeability measurements reveal that on an in vitro triple co-culture BBB model, FITC-HPBCD has low permeability, 0.50 × 10−6 cm/s, while on hCMEC/D3 cell layers, the permeability is higher, 1.86 × 10−5 cm/s. FITC-HPBCD enters brain capillary endothelial cells, is detected in cytoplasmic vesicles and rarely localized in lysosomes. The cellular internalization of HPBCD at the BBB can help to develop new strategies for improved HPBCD effects after systemic administration.

Published
2022
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637. A Novel Tandem-Tag Purification Strategy for Challenging Disordered Proteins

Author

Attila Mészáros, Kevin Muwonge, Steven Janvier, Junaid Ahmed, and Peter Tompa

Subjects
intrinsically disordered proteins (IDPs), protein purification, affinity chromatography, Tau, androgen receptor (AF1), Microbiology, QR1-502
Abstract

Intrinsically disordered proteins (IDPs) lack well-defined 3D structures and can only be described as ensembles of different conformations. This high degree of flexibility allows them to interact promiscuously and makes them capable of fulfilling unique and versatile regulatory roles in cellular processes. These functional benefits make IDPs widespread in nature, existing in every living organism from bacteria and fungi to plants and animals. Due to their open and exposed structural state, IDPs are much more prone to proteolytic degradation than their globular counterparts. Therefore, the purification of recombinant IDPs requires extra care and caution, such as maintaining low temperature throughout the purification, the use of protease inhibitor cocktails and fast workflow. Even so, in the case of long IDP targets, the appearance of truncated by-products often seems unavoidable. The separation of these unwanted proteins can be very challenging due to their similarity to the parent target protein. Here, we describe a tandem-tag purification method that offers a remedy to this problem. It contains only common affinity-chromatography steps (HisTrap and Heparin) to ensure low cost, easy access and scaling-up for possible industrial use. The effectiveness of the method is demonstrated with four examples, Tau-441 and two of its fragments and the transactivation domain (AF1) of androgen receptor.

Published
2022
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638. Measurement of the Atmospheric $\nu_e$ flux in IceCube

Author

IceCube Collaboration, Aartsen, M. G., Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beattie, K., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohaichuk, S., Bohm, C., Bose1, D., Boser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Buitink, S., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clark, K., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., De Ridder, S., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., DeYoung, T., Diaz-Velez, J. C., Dreyer, J., Dumm, J. P., Dunkman, M., Eagan, R., Eberhardt, B., Eisch, J., Ellsworth, R. W., Engdegard, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Golup, G., Goodman, J. A., Gora, D., Grant, D., Gross, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jlelati, O., Kappes, A., Karg, T., Karle, A., Kiryluk, J., Kislat, F., Klas, J., Klein, S. R., Kohne, J. -H., Kohnen, G., Kolanoski, H., Kopke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Landsman, H., Larson, M. J., Lauer, R., Lesiak-Bzdak, M., Lunemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Meszaros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Panknin, S., Paul, L., Pepper, J. A., Heros, C. Perez de los, Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Radel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schoneberg, S., Schonherr, L., Schonwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Sheremata, C., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stoss, A., Strahler, E. A., Strom, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge1, M., Vraeghe, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Wasserman, R., Weaver, Ch., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., Zilles, A., and Zoll, M.

Subjects
High Energy Physics - Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of operation of IceCube's DeepCore low energy extension. Techniques to identify neutrinos interacting within the DeepCore volume and veto muons originating outside the detector are demonstrated. A sample of 1029 events is observed in 281 days of data, of which 496 $\pm$ 66(stat.) $\pm$ 88(syst.) are estimated to be cascade events, including both electron neutrino and neutral current events. The rest of the sample includes residual backgrounds due to atmospheric muons and charged current interactions of atmospheric muon neutrinos. The flux of the atmospheric electron neutrinos is consistent with models of atmospheric neutrinos in this energy range. This constitutes the first observation of electron neutrinos and neutral current interactions in a very large volume neutrino telescope optimized for the TeV energy range., Comment: 7 pages, 4 figures (accepted by PRL)

Published
2012
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639. Chemical Abundances in Field Red Giants from High-Resolution H-Band Spectra using the APOGEE Spectral Linelist

Author

Smith, Verne V., Cunha, Katia, Shetrone, Matthew D., Meszaros, Szabolcs, Prieto, Carlos Allende, Bizyaev, Dmitry, Perez, Ana Garcia, Majewski, Steven R., Schiavon, Ricardo, Holtzman, Jon, and Johnson, Jennifer A.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

High-resolution H-band spectra of five bright field K, M, and MS giants, obtained from the archives of the Kitt Peak National Observatory (KPNO) Fourier Transform Spectrometer (FTS), are analyzed to determine chemical abundances of 16 elements. The abundances were derived via spectrum synthesis using the detailed linelist prepared for the SDSS III Apache Point Galactic Evolution Experiment (APOGEE), which is a high-resolution near-infrared spectroscopic survey to derive detailed chemical abundance distributions and precise radial velocities for 100,000 red giants sampling all Galactic stellar populations. Measured chemical abundances include the cosmochemically important isotopes 12C, 13C, 14N, and 16O, along with Mg, Al, Si, K, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, and Cu. A comparison of the abundances derived here with published values for these stars reveals consistent results to ~0.1 dex. The APOGEE spectral region and linelist is, thus, well-suited for probing both Galactic chemical evolution, as well as internal nucleosynthesis and mixing in populations of red giants using high-resolution spectroscopy., Comment: Accepted for publication in The Astrophysical Journal. 42 pages, 12 figures

Published
2012
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640. Search for dark matter annihilations in the Sun with the 79-string IceCube detector

Author

IceCube collaboration, Aartsen, M. G., Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beattie, K., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohaichuk, S., Bohm, C., Bose1, D., Böser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Buitink, S., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clark, K., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., De Ridder, S., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., DeYoung, T., Díaz-Vélez, J. C., Dreyer, J., Dumm, J. P., Dunkman, M., Eagan, R., Eberhardt, B., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Goodman, J. A., Góra, D., Grant, D., Groß, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jlelati, O., Kappes, A., Karg, T., Karle, A., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Landsman, H., Larson, M. J., Lauer, R., Lesiak-Bzdak, M., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Panknin, S., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönherr, L., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Sheremata, C., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stöß, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge1, M., Vraeghe, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Wasserman, R., Weaver, Ch., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., Zilles, A., and Zoll, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

We have performed a search for muon neutrinos from dark matter annihilation in the center of the Sun with the 79-string configuration of the IceCube neutrino telescope. For the first time, the DeepCore sub-array is included in the analysis, lowering the energy threshold and extending the search to the austral summer. The 317 days of data collected between June 2010 and May 2011 are consistent with the expected background from atmospheric muons and neutrinos. Upper limits are therefore set on the dark matter annihilation rate, with conversions to limits on spin-dependent and spin-independent WIMP-proton cross-sections for WIMP masses in the range 20 - 5000 GeV. These are the most stringent spin-dependent WIMP-proton cross-sections limits to date above 35 GeV., Comment: 7 pages, 3 figues

Published
2012
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641. The Astrophysical Multimessenger Observatory Network (AMON)

Author

Smith, M. W. E., Fox, D. B., Cowen, D. F., Mészáros, P., Tešić, G., Fixelle, J., Bartos, I., Sommers, P., Ashtekar, Abhay, Babu, G. Jogesh, Barthelmy, S. D., Coutu, S., DeYoung, T., Falcone, A. D., Finn, L. S., Gao, Shan, Hashemi, B., Homeier, A., Márka, S., Owen, B. J., and Taboada, I.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract

We summarize the science opportunity, design elements, current and projected partner observatories, and anticipated science returns of the Astrophysical Multimessenger Observatory Network (AMON). AMON will link multiple current and future high-energy, multimessenger, and follow-up observatories together into a single network, enabling near real-time coincidence searches for multimessenger astrophysical transients and their electromagnetic counterparts. Candidate and high-confidence multimessenger transient events will be identified, characterized, and distributed as AMON alerts within the network and to interested external observers, leading to follow-up observations across the electromagnetic spectrum. In this way, AMON aims to evoke the discovery of multimessenger transients from within observatory subthreshold data streams and facilitate the exploitation of these transients for purposes of astronomy and fundamental physics. As a central hub of global multimessenger science, AMON will also enable cross-collaboration analyses of archival datasets in search of rare or exotic astrophysical phenomena., Comment: 32 pages, 4 figures

Published
2012
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642. Shattering-extremal set systems of small VC-dimension

Author

Mészáros, Tamás and Rónyai, Lajos

Subjects
Mathematics - Combinatorics, 05D05, 05C05, 05E40
Abstract

We say that a set system $\mathcal{F}\subseteq 2^{[n]}$ shatters a given set $S\subseteq [n]$ if $2^S={F \cap S : F \in \mathcal{F}}$. The Sauer inequality states that in general, a set system $\mathcal{F}$ shatters at least $|\mathcal{F}|$ sets. Here we concentrate on the case of equality. A set system is called shattering-extremal if it shatters exactly $|\mathcal{F}|$ sets. We characterize shattering extremal set systems of Vapnik-Chervonenkis dimension 1 in terms of their inclusion graphs. Also from the perspective of extremality, we relate set systems of bounded Vapnik-Chervonenkis dimension to their projections., Comment: 17 pages

Published
2012

643. High-energy neutrino and gamma-ray transients from trans-relativistic supernova shock breakouts

Author

Kashiyama, Kazumi, Murase, Kohta, Horiuchi, Shunsaku, Gao, Shan, and Mészáros, Peter

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Relativistic shocks that accompany supernovae (SNe) produce X-ray burst emissions as they break out in the dense circumstellar medium around the progenitors. This phenomenon is sometimes associated with peculiar low-luminosity gamma-ray bursts (LL GRBs). Here, we investigate the high energy neutrino and gamma-ray counterparts of such a class of SNe. Just beyond the shock breakout radius, particle acceleration in the collisionless shock starts to operate in the presence of breakout photons. We show that protons may be accelerated to sufficiently high energies and produce high energy neutrinos and gamma rays via the photomeson interaction. These neutrinos and gamma rays may be detectable from 10 Mpc away by IceCube/KM3Net as multi-TeV transients almost simultaneously with the X-ray burst emission, and even from 100 Mpc away with follow-up observations by CTA using a wide-field sky monitor like Swift as a trigger. A statistical technique using a stacking approach could also be possible for the detection, with the aid of the SN optical/infrared counterparts. Such multi-messenger observations offer the possibility to probe the transition of relativistic shocks from radiation-mediated to collisionless ones, and would also constrain the mechanisms of particle acceleration and emission in LL GRBs., Comment: 5 pages, 3 figures, accepted for publication to ApJL

Published
2012
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644. Search for Galactic PeV Gamma Rays with the IceCube Neutrino Observatory

Author

IceCube collaboration, Aartsen, M. G., Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beattie, K., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohaichuk, S., Bohm, C., Bose1, D., Böser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Buitink, S., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clark, K., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., De Ridder, S., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., DeYoung, T., Díaz-Vélez, J. C., Dreyer, J., Dumm, J. P., Dunkman, M., Eagan, R., Eberhardt, B., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Goodman, J. A., Góra, D., Grant, D., Groß, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jlelati, O., Kappes, A., Karg, T., Karle, A., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Landsman, H., Larson, M. J., Lauer, R., Lesiak-Bzdak, M., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Panknin, S., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönherr, L., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Sheremata, C., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stöß, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge1, M., Vraeghe, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Wasserman, R., Weaver, Ch., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., Zilles, A., and Zoll, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Gamma-ray induced air showers are notable for their lack of muons, compared to hadronic showers. Hence, air shower arrays with large underground muon detectors can select a sample greatly enriched in photon showers by rejecting showers containing muons. IceCube is sensitive to muons with energies above ~500 GeV at the surface, which provides an efficient veto system for hadronic air showers with energies above 1 PeV. One year of data from the 40-string IceCube configuration was used to perform a search for point sources and a Galactic diffuse signal. No sources were found, resulting in a 90% C.L. upper limit on the ratio of gamma rays to cosmic rays of 1.2 x 10^(-3)for the flux coming from the Galactic Plane region (-80 deg < l < -30 deg; -10 deg < b < 5 deg) in the energy range 1.2 - 6.0 PeV. In the same energy range, point source fluxes with E^(-2) spectra have been excluded at a level of (E/TeV)^2 d\Phi/dE ~ 10^(-12)-10^(-11) cm^2/s/TeV depending on source declination. The complete IceCube detector will have a better sensitivity, due to the larger detector size, improved reconstruction and vetoing techniques. Preliminary data from the nearly-final IceCube detector configuration has been used to estimate the 5 year sensitivity of the full detector. It is found to be more than an order of magnitude better, allowing the search for PeV extensions of known TeV gamma-ray emitters., Comment: submitted to PRD, 15 pages, 15 figures

Published
2012
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645. Magnetically and Baryonically Dominated Photospheric Gamma-Ray Burst Model Fits to Fermi LAT Observations

Author

Veres, Péter, Zhang, Bin-Bin, and Mészáros, Péter

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We consider gamma-ray burst models where the radiation is dominated by a photospheric region providing the MeV Band spectrum, and an external shock region responsible for the GeV radiation via inverse Compton scattering. We parametrize the initial dynamics through an acceleration law Gamma \propto r^\mu, with \mu between 1/3 and 1 to represent the range between an extreme magnetically dominated and a baryonically dominated regime. We compare these models to several bright Fermi LAT bursts, and show that both the time integrated and the time resolved spectra, where available, can be well described by these models. We discuss the parameters which result from these fits, and discuss the relative merits and shortcomings of the two models., Comment: 8 pages, 14 figures, corrected version, accepted by ApJ

Published
2012
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646. Observation of Cosmic Ray Anisotropy with the IceTop Air Shower Array

Author

IceCube Collaboration, Aartsen, M. G., Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beattie, K., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohaichuk, S., Bohm, C., Bose, D., Böser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clark, K., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cru., Danninger, M., Daughhetee, J., Davis, J. C., Clercq, C. D., Ridder, S. D., Descamps, F., Desiati, P., Vries-Uiterweerd, G. d., DeYoung, T., Díaz-Vélez, J. C., Dreyer, J., Dumm, J. P., Dunkman, M., Eagan, R., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Goodman, J. A., Góra, D., Grant, D., Groß, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Ha., Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jlelati, O., Kappes, A., Karg, T., Karle, A., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Landsman, H., Larson, M. J., Lauer, R., Lesiak-Bzdak, M., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Panknin, S., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rothmaier, F., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönherr, L., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Sheremata, C., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., Drift, D. va. de., Eijndhoven, N. va., Overloop, A. Va., Santen, J. va., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Wasserman, R., Weaver, Ch., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., Zilles, A., and Zoll, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report on the observation of anisotropy in the arrival direction distribution of cosmic rays at PeV energies. The analysis is based on data taken between 2009 and 2012 with the IceTop air shower array at the South Pole. IceTop, an integral part of the IceCube detector, is sensitive to cosmic rays between 100 TeV and 1 EeV. With the current size of the IceTop data set, searches for anisotropy at the 10^-3 level can, for the first time, be extended to PeV energies. We divide the data set into two parts with median energies of 400 TeV and 2 PeV, respectively. In the low energy band, we observe a strong deficit with an angular size of about 30 degrees and an amplitude of (-1.58 +/- 0.46 (stat) +/- 0.52 (sys)) x 10^(-3) at a location consistent with previous observations of cosmic rays with the IceCube neutrino detector. The study of the high energy band shows that the anisotropy persists to PeV energies and increases in amplitude to (-3.11 +/- 0.38 (stat) +/- 0.96 (sys)) x 10^(-3)., Comment: Accepted for publication in ApJ. Supplemental information available in the source file of the paper

Published
2012
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647. Search for Neutrinos from Annihilating Dark Matter in the Direction of the Galactic Center with the 40-String IceCube Neutrino Observatory

Author

The IceCube collaboration, Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beattie, K., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bose, D., Böser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Buitink, S., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., Descamps, F., Desiati, P., Uiterweerd, G. de Vries, DeYoung, T., Díaz-Vélez, J. C., Dreyer, J., Dumm, J. P., Dunkman, M., Eagan, R., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Goodman, J. A., Góra, D., Grant, D., Groß, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Hülß, J. -P., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jlelati, O., Kappes, A., Karg, T., Karle, A., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Laihem, K., Landsman, H., Larson, M. J., Lauer, R., Lesiak-Bzdak, M., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Naumann, U., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Panknin, S., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rothmaier, F., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönherr, L., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Wasserman, R., Weaver, Ch., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zilles, A., and Zoll, M.

Subjects
High Energy Physics - Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract

A search for muon neutrinos from dark matter annihilations in the Galactic Center region has been performed with the 40-string configuration of the IceCube Neutrino Observatory using data collected in 367 days of live-time starting in April 2008. The observed fluxes were consistent with the atmospheric background expectations. Upper limits on the self-annihilation cross-section are obtained for dark matter particle masses ranging from 100 GeV to 10 TeV. In the case of decaying dark matter, lower limits on the lifetime have been determined for masses between 200 GeV and 20 TeV., Comment: 11 pages, 13 figures. An error in the limit calculation code has been corrected, which lead to too constraining limits. This error impacted figures 9, 10, 11, 12 and 13

Published
2012

648. Searches for high-energy neutrino emission in the Galaxy with the combined IceCube-AMANDA detector

Author

IceCube collaboration, Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beattie, K., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bose, D., Böser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Buitink, S., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., Descamps, F., Desiati, P., Uiterweerd, G. de Vries, DeYoung, T., Díaz-Vélez, J. C., Dreyer, J., Dumm, J. P., Dunkman, M., Eagan, R., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Goodman, J. A., Góra, D., Grant, D., Groß, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jlelati, O., Kappes, A., Karg, T., Karle, A., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Laihem, K., Landsman, H., Larson, M. J., Lauer, R., Lesiak-Bzdak, M., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Naumann, U., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Panknin, S., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rothmaier, F., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönherr, L., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van der Drift, D., van Eijndhoven, N., Van Overloop, A., van Santen, J., Vehring, M., Voge, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Wasserman, R., Weaver, Ch., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zilles, A., and Zoll, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report on searches for neutrino sources at energies above 200 GeV in the Northern sky of the galactic plane, using the data collected by the South Pole neutrino telescopes IceCube and AMANDA. The galactic region considered here includes the Local Arm towards the Cygnus region and our closest approach to the Perseus Arm. The data have been collected between 2007 and 2009 when AMANDA was an integrated part of IceCube, which was still under construction and operated with 22-strings (2007-8) and 40-strings (2008-9) of optical modules deployed in the ice. By combining the larger IceCube detector with the lower energy threshold of the more compact AMANDA detector, we obtain an improved sensitivity at energies below $\sim$10 TeV with respect to previous searches. The analyses presented here are: a scan for point sources within the galactic plane; a search optimized for multiple and extended sources in the Cygnus region, which might be below the sensitivity of the point source scan; and studies of seven pre-selected neutrino source candidates. For one of them, Cygnus X-3, a time-dependent search for neutrinos in coincidence with observed radio and X-ray flares has been performed. No evidence of a signal is found, and upper limits are reported for each of the searches. We investigate neutrino spectra proportional to E$^{-2}$ and E$^{-3}$ to cover the entire range of possible spectra. The soft E$^{-3}$ spectrum results in an energy distribution similar to a source with cut-off below $\sim$50 TeV. For the considered region of the galactic plane, the 90% confidence level muon neutrino flux upper limits are in the range E$^3$dN/dE$\sim 5.4 - 19.5 \times 10^{-11} \rm{TeV^{2} cm^{-2} s^{-1}}$ for point-like neutrino sources in the energy region [180.0 GeV - 20.5 TeV]. These represent the most stringent upper limits for soft-spectra neutrino sources within the Galaxy reported to date.

Published
2012
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649. Schur times Schubert via the Fomin-Kirillov algebra

Author

Meszaros, Karola, Panova, Greta, and Postnikov, Alexander

Subjects
Mathematics - Combinatorics, 05E15, 05E05, 05E40, 14N35
Abstract

We study multiplication of any Schubert polynomial $\mathfrak{S}_w$ by a Schur polynomial $s_\lambda$ (the Schubert polynomial of a Grassmannian permutation) and the expansion of this product in the ring of Schubert polynomials. We derive explicit nonnegative combinatorial expressions for the expansion coefficients for certain special partitions $\lambda$, including hooks and the 2x2 box. We also prove combinatorially the existence of such nonnegative expansion when the Young diagram of $\lambda$ is a hook plus a box at the (2,2) corner. We achieve this by evaluating Schubert polynomials at the Dunkl elements of the Fomin-Kirillov algebra and proving special cases of the nonnegativity conjecture of Fomin and Kirillov. This approach works in the more general setup of the (small) quantum cohomology ring of the complex flag manifold and the corresponding (3-point) Gromov-Witten invariants. We provide an algebro-combinatorial proof of the nonnegativity of the Gromov-Witten invariants in these cases, and present combinatorial expressions for these coefficients.

Published
2012

650. High Energy Neutrinos from Dissipative Photospheric Models of Gamma Ray Bursts

Author

Gao, Shan, Asano, Katsuaki, and Meszaros, Peter

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We calculate the high energy neutrino spectrum from gamma-ray bursts where the emission arises in a dissipative jet photosphere determined by either baryonically or magnetically dominated dynamics, and compare these neutrino spectra to those obtained in conventional internal shock models. We also calculate the diffuse neutrino spectra based on these models, which appear compatible with the current IceCube 40+59 constraints. While a re-analysis based on the models discussed here and the data from the full array would be needed, it appears that only those models with the most extreme parameters are close to being constrained at present. A multi-year operation of the full IceCube and perhaps a next generation of large volume neutrino detectors may be required in order to distinguish between the various models discussed., Comment: 12 pages, 7 figures

Published
2012
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