Pith. sign in

REVIEW

Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1901.08040 v3 pith:3FXN6KSA submitted 2019-01-23 astro-ph.IM astro-ph.HE

Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

The Pierre Auger Collaboration: A. Aab , P. Abreu , M. Aglietta , I.F.M. Albuquerque , J.M. Albury , I. Allekotte , A. Almela , J. Alvarez Castillo
show 383 more authors
J. Alvarez-Mu\~niz G.A. Anastasi L. Anchordoqui B. Andrada S. Andringa C. Aramo H. Asorey P. Assis G. Avila A.M. Badescu A. Bakalova A. Balaceanu F. Barbato R.J. Barreira Luz S. Baur K.H. Becker J.A. Bellido C. Berat M.E. Bertaina X. Bertou P.L. Biermann J. Biteau S.G. Blaess A. Blanco J. Blazek C. Bleve M. Boh\'a\v{c}ov\'a D. Boncioli C. Bonifazi N. Borodai A.M. Botti J. Brack T. Bretz A. Bridgeman F.L. Briechle P. Buchholz A. Bueno S. Buitink M. Buscemi K.S. Caballero-Mora L. Caccianiga L. Calcagni A. Cancio F. Canfora J.M. Carceller R. Caruso A. Castellina F. Catalani G. Cataldi L. Cazon M. Cerda J.A. Chinellato J. Chudoba L. Chytka R.W. Clay A.C. Cobos Cerutti R. Colalillo A. Coleman M.R. Coluccia R. Concei\c{c}\~ao A. Condorelli G. Consolati F. Contreras F. Convenga M.J. Cooper S. Coutu C.E. Covault B. Daniel S. Dasso K. Daumiller B.R. Dawson J.A. Day R.M. de Almeida S.J. de Jong G. De Mauro J.R.T. de Mello Neto I. De Mitri J. de Oliveira F.O. de Oliveira Salles V. de Souza J. Debatin M. del R\'io O. Deligny N. Dhital M.L. D\'iaz Castro F. Diogo C. Dobrigkeit J.C. D'Olivo Q. Dorosti R.C. dos Anjos M.T. Dova A. Dundovic J. Ebr R. Engel M. Erdmann C.O. Escobar A. Etchegoyen H. Falcke J. Farmer G. Farrar A.C. Fauth N. Fazzini F. Feldbusch F. Fenu L.P. Ferreyro J.M. Figueira A. Filip\v{c}i\v{c} M.M. Freire T. Fujii A. Fuster B. Garc\'ia H. Gemmeke A. Gherghel-Lascu P.L. Ghia U. Giaccari M. Giammarchi M. Giller D. G{\l}as J. Glombitza F. Gobbi G. Golup M. G\'omez Berisso P.F. G\'omez Vitale J.P. Gongora N. Gonz\'alez I. Goos D. G\'ora A. Gorgi M. Gottowik T.D. Grubb F. Guarino G.P. Guedes E. Guido R. Halliday M.R. Hampel P. Hansen D. Harari T.A. Harrison V.M. Harvey A. Haungs T. Hebbeker D. Heck P. Heimann G.C. Hill C. Hojvat E.M. Holt P. Homola J.R. H\"orandel P. Horvath M. Hrabovsk\'y T. Huege J. Hulsman A. Insolia P.G. Isar I. Jandt J.A. Johnsen M. Josebachuili J. Jurysek A. K\"a\"ap\"a K.H. Kampert B. Keilhauer N. Kemmerich J. Kemp H.O. Klages M. Kleifges J. Kleinfeller R. Krause D. Kuempel G. Kukec Mezek A. Kuotb Awad B.L. Lago D. LaHurd R.G. Lang R. Legumina M.A. Leigui de Oliveira V. Lenok A. Letessier-Selvon I. Lhenry-Yvon O.C. Lippmann D. Lo Presti L. Lopes R. L\'opez A. L\'opez Casado R. Lorek Q. Luce A. Lucero M. Malacari G. Mancarella D. Mandat B.C. Manning P. Mantsch A.G. Mariazzi I.C. Mari\c{s} G. Marsella D. Martello H. Martinez O. Mart\'inez Bravo M. Mastrodicasa H.J. Mathes S. Mathys J. Matthews G. Matthiae E. Mayotte P.O. Mazur G. Medina-Tanco D. Melo A. Menshikov K.-D. Merenda S. Michal M.I. Micheletti L. Middendorf L. Miramonti B. Mitrica D. Mockler S. Mollerach F. Montanet C. Morello G. Morlino M. Mostaf\'a A.L. M\"uller M.A. Muller S. M\"uller R. Mussa L. Nellen P.H. Nguyen M. Niculescu-Oglinzanu M. Niechciol D. Nitz D. Nosek V. Novotny L. No\v{z}ka A Nucita L.A. N\'u\~nez A. Olinto M. Palatka J. Pallotta M.P. Panetta P. Papenbreer G. Parente A. Parra M. Pech F. Pedreira J. P\k{e}kala R. Pelayo J. Pe\~na-Rodriguez L.A.S. Pereira M. Perlin L. Perrone C. Peters S. Petrera J. Phuntsok T. Pierog M. Pimenta V. Pirronello M. Platino J. Poh B. Pont C. Porowski R.R. Prado P. Privitera M. Prouza A. Puyleart S. Querchfeld S. Quinn R. Ramos-Pollan J. Rautenberg D. Ravignani M. Reininghaus J. Ridky F. Riehn M. Risse P. Ristori V. Rizi W. Rodrigues de Carvalho J. Rodriguez Rojo M.J. Roncoroni M. Roth E. Roulet A.C. Rovero P. Ruehl S.J. Saffi A. Saftoiu F. Salamida H. Salazar G. Salina J.D. Sanabria Gomez F. S\'anchez E.M. Santos E. Santos F. Sarazin R. Sarmento C. Sarmiento-Cano R. Sato P. Savina M. Schauer V. Scherini H. Schieler M. Schimassek M. Schimp F. Schl\"uter D. Schmidt O. Scholten P. Schov\'anek F.G. Schr\"oder S. Schr\"oder J. Schumacher S.J. Sciutto M. Scornavacche R.C. Shellard G. Sigl G. Silli O. Sima R. \v{S}m\'ida G.R. Snow P. Sommers J.F. Soriano J. Souchard R. Squartini D. Stanca S. Stani\v{c} J. Stasielak P. Stassi M. Stolpovskiy A. Streich F. Suarez M. Su\'arez-Dur\'an T. Sudholz T. Suomij\"arvi A.D. Supanitsky J. \v{S}up\'ik Z. Szadkowski A. Taboada O.A. Taborda A. Tapia C. Timmermans C.J. Todero Peixoto B. Tom\'e G. Torralba Elipe A. Travaini P. Travnicek M. Trini M. Tueros R. Ulrich M. Unger M. Urban J.F. Vald\'es Galicia I. Vali\~no L. Valore P. van Bodegom A.M. van den Berg A. van Vliet E. Varela B. Vargas C\'ardenas D. Veberi\v{c} C. Ventura I.D. Vergara Quispe V. Verzi J. Vicha L. Villase\~nor J. Vink S. Vorobiov H. Wahlberg A.A. Watson M. Weber A. Weindl M. Wiede\'nski L. Wiencke H. Wilczy\'nski T. Winchen M. Wirtz D. Wittkowski B. Wundheiler L. Yang A. Yushkov E. Zas D. Zavrtanik M. Zavrtanik L. Zehrer A. Zepeda B. Zimmermann M. Ziolkowski Z. Zong F. Zuccarello
This is my paper
classification astro-ph.IM astro-ph.HE
keywords energyestimationobservatoryaugerinvisiblemassmethodmuon
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The determination of the primary energy of extensive air showers using the fluorescence detection technique requires an estimation of the energy carried away by particles that do not deposit all their energy in the atmosphere. This estimation is typically made using Monte Carlo simulations and thus depends on the assumed primary particle mass and on model predictions for neutrino and muon production. In this work we present a new method to obtain the invisible energy from events detected by the Pierre Auger Observatory. The method uses measurements of the muon number at ground level, and it allows us to reduce significantly the systematic uncertainties related to the mass composition and the high energy hadronic interaction models, and consequently to improve the estimation of the energy scale of the Observatory.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.