Corrigendum to ‘Measurement of the neutron background at the Canfranc Underground Laboratory LSC’ [Astroparticle Physics 42 (2013)1–6](Measurement of the neutron background at the Canfranc Underground Laboratory LSC (2013)42 (1–6), (S0927650512002046), (10.1016/j.astropartphys.2012.11.007))

D. Jordan, J. L. Tain, A. Algora, J. Agramunt, C. Domingo-Pardo, M. B. Gomez-Hornillos, R. Caballero-Folch, G. Cortés, D. Cano-Ott, E. Mendoza, I. Bandac, A. Bettini, L. M. Fraile, C. Domingo

Research output: Comment/debate

Abstract

The authors regret to report that there is an error in the conversion of Monte Carlo simulations into detector versus neutron energy response, described in Section 4 and shown in Fig. 5 in the original paper. This detector response matrix should be multiplied by a factor of 1/4. As a consequence, the neutron flux Φ per bin in Table 4 and figures 6 and 7 must be multiplied by 4. Thus the integrated neutron background flux in Hall A of LSC becomes Φ Hall A = (1.38 ± 0.14)× 10 −5 cm −2 s −1 . The authors would like to thank Marcel Grieger and Daniel Bemmerer who pointed out a possible mistake in our results. The authors would like to apologise for any inconvenience caused.

Original languageEnglish
JournalAstroparticle Physics
DOIs
Publication statusPublished - jan. 1 2019

Fingerprint

neutrons
physics
neutron counters
flux (rate)
detectors
matrices
simulation
energy

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Cite this

Corrigendum to ‘Measurement of the neutron background at the Canfranc Underground Laboratory LSC’ [Astroparticle Physics 42 (2013)1–6](Measurement of the neutron background at the Canfranc Underground Laboratory LSC (2013)42 (1–6), (S0927650512002046), (10.1016/j.astropartphys.2012.11.007)). / Jordan, D.; Tain, J. L.; Algora, A.; Agramunt, J.; Domingo-Pardo, C.; Gomez-Hornillos, M. B.; Caballero-Folch, R.; Cortés, G.; Cano-Ott, D.; Mendoza, E.; Bandac, I.; Bettini, A.; Fraile, L. M.; Domingo, C.

In: Astroparticle Physics, 01.01.2019.

Research output: Comment/debate

Jordan, D. ; Tain, J. L. ; Algora, A. ; Agramunt, J. ; Domingo-Pardo, C. ; Gomez-Hornillos, M. B. ; Caballero-Folch, R. ; Cortés, G. ; Cano-Ott, D. ; Mendoza, E. ; Bandac, I. ; Bettini, A. ; Fraile, L. M. ; Domingo, C. / Corrigendum to ‘Measurement of the neutron background at the Canfranc Underground Laboratory LSC’ [Astroparticle Physics 42 (2013)1–6](Measurement of the neutron background at the Canfranc Underground Laboratory LSC (2013)42 (1–6), (S0927650512002046), (10.1016/j.astropartphys.2012.11.007)). In: Astroparticle Physics. 2019.
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title = "Corrigendum to ‘Measurement of the neutron background at the Canfranc Underground Laboratory LSC’ [Astroparticle Physics 42 (2013)1–6](Measurement of the neutron background at the Canfranc Underground Laboratory LSC (2013)42 (1–6), (S0927650512002046), (10.1016/j.astropartphys.2012.11.007))",
abstract = "The authors regret to report that there is an error in the conversion of Monte Carlo simulations into detector versus neutron energy response, described in Section 4 and shown in Fig. 5 in the original paper. This detector response matrix should be multiplied by a factor of 1/4. As a consequence, the neutron flux Φ per bin in Table 4 and figures 6 and 7 must be multiplied by 4. Thus the integrated neutron background flux in Hall A of LSC becomes Φ Hall A = (1.38 ± 0.14)× 10 −5 cm −2 s −1 . The authors would like to thank Marcel Grieger and Daniel Bemmerer who pointed out a possible mistake in our results. The authors would like to apologise for any inconvenience caused.",
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AU - Jordan, D.

AU - Tain, J. L.

AU - Algora, A.

AU - Agramunt, J.

AU - Domingo-Pardo, C.

AU - Gomez-Hornillos, M. B.

AU - Caballero-Folch, R.

AU - Cortés, G.

AU - Cano-Ott, D.

AU - Mendoza, E.

AU - Bandac, I.

AU - Bettini, A.

AU - Fraile, L. M.

AU - Domingo, C.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - The authors regret to report that there is an error in the conversion of Monte Carlo simulations into detector versus neutron energy response, described in Section 4 and shown in Fig. 5 in the original paper. This detector response matrix should be multiplied by a factor of 1/4. As a consequence, the neutron flux Φ per bin in Table 4 and figures 6 and 7 must be multiplied by 4. Thus the integrated neutron background flux in Hall A of LSC becomes Φ Hall A = (1.38 ± 0.14)× 10 −5 cm −2 s −1 . The authors would like to thank Marcel Grieger and Daniel Bemmerer who pointed out a possible mistake in our results. The authors would like to apologise for any inconvenience caused.

AB - The authors regret to report that there is an error in the conversion of Monte Carlo simulations into detector versus neutron energy response, described in Section 4 and shown in Fig. 5 in the original paper. This detector response matrix should be multiplied by a factor of 1/4. As a consequence, the neutron flux Φ per bin in Table 4 and figures 6 and 7 must be multiplied by 4. Thus the integrated neutron background flux in Hall A of LSC becomes Φ Hall A = (1.38 ± 0.14)× 10 −5 cm −2 s −1 . The authors would like to thank Marcel Grieger and Daniel Bemmerer who pointed out a possible mistake in our results. The authors would like to apologise for any inconvenience caused.

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