Direct Measurement of the Spectral Structure of Cosmic-Ray Electrons+Positrons in the TeV Region with CALET on the International Space Station.

Detailed measurements of the spectral structure of cosmic-ray electrons and positrons from 10.6 GeV to 7.5 TeV are presented from over 7 years of observations with the CALorimetric Electron Telescope (CALET) on the International Space Station. The instrument, consisting of a charge detector, an imaging calorimeter, and a total absorption calorimeter with a total depth of 30 radiation lengths at normal incidence and a fine shower imaging capability, is optimized to measure the all-electron spectrum well into the TeV region. Because of the excellent energy resolution (a few percent above 10 GeV) and the outstanding e/p separation (10^{5}), CALET provides optimal performance for a detailed search of structures in the energy spectrum. The analysis uses data up to the end of 2022, and the statistics of observed electron candidates has increased more than 3 times since the last publication in 2018. By adopting an updated boosted decision tree analysis, a sufficient proton rejection power up to 7.5 TeV is achieved, with a residual proton contamination less than 10%. The observed energy spectrum becomes gradually harder in the lower energy region from around 30 GeV, consistently with AMS-02, but from 300 to 600 GeV it is considerably softer than the spectra measured by DAMPE and Fermi-LAT. At high energies, the spectrum presents a sharp break around 1 TeV, with a spectral index change from -3.15 to -3.91, and a broken power law fitting the data in the energy range from 30 GeV to 4.8 TeV better than a single power law with 6.9 sigma significance, which is compatible with the DAMPE results. The break is consistent with the expected effects of radiation loss during the propagation from distant sources (except the highest energy bin). We have fitted the spectrum with a model consistent with the positron flux measured by AMS-02 below 1 TeV and interpreted the electron+positron spectrum with possible contributions from pulsars and nearby sources. Above 4.8 TeV, a possible contribution from known nearby supernova remnants, including Vela, is addressed by an event-by-event analysis providing a higher proton-rejection power than a purely statistical analysis.

Erratum: Charge-Sign Dependent Cosmic-Ray Modulation Observed with the Calorimetric Electron Telescope on the International Space Station [Phys. Rev. Lett. 130, 211001 (2023)].

This corrects the article DOI: 10.1103/PhysRevLett.130.211001.

Charge-Sign Dependent Cosmic-Ray Modulation Observed with the Calorimetric Electron Telescope on the International Space Station.

We present the observation of a charge-sign dependent solar modulation of galactic cosmic rays (GCRs) with the Calorimetric Electron Telescope onboard the International Space Station over 6 yr, corresponding to the positive polarity of the solar magnetic field. The observed variation of proton count rate is consistent with the neutron monitor count rate, validating our methods for determining the proton count rate. It is observed by the Calorimetric Electron Telescope that both GCR electron and proton count rates at the same average rigidity vary in anticorrelation with the tilt angle of the heliospheric current sheet, while the amplitude of the variation is significantly larger in the electron count rate than in the proton count rate. We show that this observed charge-sign dependence is reproduced by a numerical "drift model" of the GCR transport in the heliosphere. This is a clear signature of the drift effect on the long-term solar modulation observed with a single detector.

Direct Measurement of the Cosmic-Ray Helium Spectrum from 40 GeV to 250 TeV with the Calorimetric Electron Telescope on the International Space Station.

We present the results of a direct measurement of the cosmic-ray helium spectrum with the CALET instrument in operation on the International Space Station since 2015. The observation period covered by this analysis spans from October 13, 2015, to April 30, 2022 (2392 days). The very wide dynamic range of CALET allowed for the collection of helium data over a large energy interval, from ∼40 GeV to ∼250 TeV, for the first time with a single instrument in low Earth orbit. The measured spectrum shows evidence of a deviation of the flux from a single power law by more than 8σ with a progressive spectral hardening from a few hundred GeV to a few tens of TeV. This result is consistent with the data reported by space instruments including PAMELA, AMS-02, and DAMPE and balloon instruments including CREAM. At higher energy we report the onset of a softening of the helium spectrum around 30 TeV (total kinetic energy). Though affected by large uncertainties in the highest energy bins, the observation of a flux reduction turns out to be consistent with the most recent results of DAMPE. A double broken power law is found to fit simultaneously both spectral features: the hardening (at lower energy) and the softening (at higher energy). A measurement of the proton to helium flux ratio in the energy range from 60 GeV/n to about 60 TeV/n is also presented, using the CALET proton flux recently updated with higher statistics.

Observation of Spectral Structures in the Flux of Cosmic-Ray Protons from 50 GeV to 60 TeV with the Calorimetric Electron Telescope on the International Space Station.

A precise measurement of the cosmic-ray proton spectrum with the Calorimetric Electron Telescope (CALET) is presented in the energy interval from 50 GeV to 60 TeV, and the observation of a softening of the spectrum above 10 TeV is reported. The analysis is based on the data collected during ∼6.2 years of smooth operations aboard the International Space Station and covers a broader energy range with respect to the previous proton flux measurement by CALET, with an increase of the available statistics by a factor of ∼2.2. Above a few hundred GeV we confirm our previous observation of a progressive spectral hardening with a higher significance (more than 20 sigma). In the multi-TeV region we observe a second spectral feature with a softening around 10 TeV and a spectral index change from -2.6 to -2.9 consistently, within the errors, with the shape of the spectrum reported by DAMPE. We apply a simultaneous fit of the proton differential spectrum which well reproduces the gradual change of the spectral index encompassing the lower energy power-law regime and the two spectral features observed at higher energies.

Cosmic-Ray Boron Flux Measured from 8.4 GeV/n to 3.8 TeV/n with the Calorimetric Electron Telescope on the International Space Station.

We present the measurement of the energy dependence of the boron flux in cosmic rays and its ratio to the carbon flux in an energy interval from 8.4 GeV/n to 3.8 TeV/n based on the data collected by the Calorimetric Electron Telescope (CALET) during ∼6.4 yr of operation on the International Space Station. An update of the energy spectrum of carbon is also presented with an increase in statistics over our previous measurement. The observed boron flux shows a spectral hardening at the same transition energy E_{0}∼200 GeV/n of the C spectrum, though B and C fluxes have different energy dependences. The spectral index of the B spectrum is found to be γ=-3.047±0.024 in the interval 25

Direct Measurement of the Nickel Spectrum in Cosmic Rays in the Energy Range from 8.8 GeV/n to 240 GeV/n with CALET on the International Space Station.

The relative abundance of cosmic ray nickel nuclei with respect to iron is by far larger than for all other transiron elements; therefore it provides a favorable opportunity for a low background measurement of its spectrum. Since nickel, as well as iron, is one of the most stable nuclei, the nickel energy spectrum and its relative abundance with respect to iron provide important information to estimate the abundances at the cosmic ray source and to model the Galactic propagation of heavy nuclei. However, only a few direct measurements of cosmic-ray nickel at energy larger than ∼3 GeV/n are available at present in the literature, and they are affected by strong limitations in both energy reach and statistics. In this Letter, we present a measurement of the differential energy spectrum of nickel in the energy range from 8.8 to 240 GeV/n, carried out with unprecedented precision by the Calorimetric Electron Telescope (CALET) in operation on the International Space Station since 2015. The CALET instrument can identify individual nuclear species via a measurement of their electric charge with a dynamic range extending far beyond iron (up to atomic number Z=40). The particle's energy is measured by a homogeneous calorimeter (1.2 proton interaction lengths, 27 radiation lengths) preceded by a thin imaging section (3 radiation lengths) providing tracking and energy sampling. This Letter follows our previous measurement of the iron spectrum [1O. Adriani et al. (CALET Collaboration), Phys. Rev. Lett. 126, 241101 (2021).PRLTAO0031-900710.1103/PhysRevLett.126.241101], and it extends our investigation on the energy dependence of the spectral index of heavy elements. It reports the analysis of nickel data collected from November 2015 to May 2021 and a detailed assessment of the systematic uncertainties. In the region from 20 to 240 GeV/n our present data are compatible within the errors with a single power law with spectral index -2.51±0.07.

Measurement of the Iron Spectrum in Cosmic Rays from 10 GeV/n to 2.0 TeV/n with the Calorimetric Electron Telescope on the International Space Station.

The Calorimetric Electron Telescope (CALET), in operation on the International Space Station since 2015, collected a large sample of cosmic-ray iron over a wide energy interval. In this Letter a measurement of the iron spectrum is presented in the range of kinetic energy per nucleon from 10 GeV/n to 2.0 TeV/n allowing the inclusion of iron in the list of elements studied with unprecedented precision by space-borne instruments. The measurement is based on observations carried out from January 2016 to May 2020. The CALET instrument can identify individual nuclear species via a measurement of their electric charge with a dynamic range extending far beyond iron (up to atomic number Z=40). The energy is measured by a homogeneous calorimeter with a total equivalent thickness of 1.2 proton interaction lengths preceded by a thin (3 radiation lengths) imaging section providing tracking and energy sampling. The analysis of the data and the detailed assessment of systematic uncertainties are described and results are compared with the findings of previous experiments. The observed differential spectrum is consistent within the errors with previous experiments. In the region from 50 GeV/n to 2 TeV/n our present data are compatible with a single power law with spectral index -2.60±0.03.

Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10 GeV/n to 2.2 TeV/n with the Calorimetric Electron Telescope on the International Space Station.

In this paper, we present the measurement of the energy spectra of carbon and oxygen in cosmic rays based on observations with the Calorimetric Electron Telescope on the International Space Station from October 2015 to October 2019. Analysis, including the detailed assessment of systematic uncertainties, and results are reported. The energy spectra are measured in kinetic energy per nucleon from 10 GeV/n to 2.2 TeV/n with an all-calorimetric instrument with a total thickness corresponding to 1.3 nuclear interaction length. The observed carbon and oxygen fluxes show a spectral index change of ∼0.15 around 200 GeV/n established with a significance >3σ. They have the same energy dependence with a constant C/O flux ratio 0.911±0.006 above 25 GeV/n. The spectral hardening is consistent with that measured by AMS-02, but the absolute normalization of the flux is about 27% lower, though in agreement with observations from previous experiments including the PAMELA spectrometer and the calorimetric balloon-borne experiment CREAM.

Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space Station.

In this paper, we present the analysis and results of a direct measurement of the cosmic-ray proton spectrum with the CALET instrument onboard the International Space Station, including the detailed assessment of systematic uncertainties. The observation period used in this analysis is from October 13, 2015 to August 31, 2018 (1054 days). We have achieved the very wide energy range necessary to carry out measurements of the spectrum from 50 GeV to 10 TeV covering, for the first time in space, with a single instrument the whole energy interval previously investigated in most cases in separate subranges by magnetic spectrometers (BESS-TeV, PAMELA, and AMS-02) and calorimetric instruments (ATIC, CREAM, and NUCLEON). The observed spectrum is consistent with AMS-02 but extends to nearly an order of magnitude higher energy, showing a very smooth transition of the power-law spectral index from -2.81±0.03 (50-500 GeV) neglecting solar modulation effects (or -2.87±0.06 including solar modulation effects in the lower energy region) to -2.56±0.04 (1-10 TeV), thereby confirming the existence of spectral hardening and providing evidence of a deviation from a single power law by more than 3σ.

Extended Measurement of the Cosmic-Ray Electron and Positron Spectrum from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope on the International Space Station.

Extended results on the cosmic-ray electron + positron spectrum from 11 GeV to 4.8 TeV are presented based on observations with the Calorimetric Electron Telescope (CALET) on the International Space Station utilizing the data up to November 2017. The analysis uses the full detector acceptance at high energies, approximately doubling the statistics compared to the previous result. CALET is an all-calorimetric instrument with a total thickness of 30 X_{0} at normal incidence and fine imaging capability, designed to achieve large proton rejection and excellent energy resolution well into the TeV energy region. The observed energy spectrum in the region below 1 TeV shows good agreement with Alpha Magnetic Spectrometer (AMS-02) data. In the energy region below ∼300 GeV, CALET's spectral index is found to be consistent with the AMS-02, Fermi Large Area Telescope (Fermi-LAT), and Dark Matter Particle Explorer (DAMPE), while from 300 to 600 GeV the spectrum is significantly softer than the spectra from the latter two experiments. The absolute flux of CALET is consistent with other experiments at around a few tens of GeV. However, it is lower than those of DAMPE and Fermi-LAT with the difference increasing up to several hundred GeV. The observed energy spectrum above ∼1 TeV suggests a flux suppression consistent within the errors with the results of DAMPE, while CALET does not observe any significant evidence for a narrow spectral feature in the energy region around 1.4 TeV. Our measured all-electron flux, including statistical errors and a detailed breakdown of the systematic errors, is tabulated in the Supplemental Material in order to allow more refined spectral analyses based on our data.

Energy Spectrum of Cosmic-Ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station.

First results of a cosmic-ray electron and positron spectrum from 10 GeV to 3 TeV is presented based upon observations with the CALET instrument on the International Space Station starting in October, 2015. Nearly a half million electron and positron events are included in the analysis. CALET is an all-calorimetric instrument with total vertical thickness of 30 X_{0} and a fine imaging capability designed to achieve a large proton rejection and excellent energy resolution well into the TeV energy region. The observed energy spectrum over 30 GeV can be fit with a single power law with a spectral index of -3.152±0.016 (stat+syst). Possible structure observed above 100 GeV requires further investigation with increased statistics and refined data analysis.

[Gastric bypass in the surgical treatment of the morbid obesity and super obesity: comparative study]. / Bypass gástrico en el tratamiento de la obesidad mórbida y la superobesidad: estudio comparativo.

INTRODUCTION: Gastric Bypass (GB) constitutes the surgical treatment of election of morbid obesity (BMI < 50) at the present time, however doubts exist about its effectiveness in super obesity patients (BMI > 50). OBJECTIVE: The purpose of this work is one of to analyze the results of loss of weight of the first 52 open GB of our series, and to compare the losses of weight in morbid obesity (MO) and super obesity (SO), to determine if the superobese patient looses enough weight with this technique or if it would be more indicated another technique more malabsorptive, like some authors recommend. MATERIALS AND METHOD: Retrospective study of the first 52 patients operated of open GB pathway. The weight loss of 32 patients' with MO are compared with the weight loss of 20 patients with super obesity after five year follow-up. The parameters analyzed are: age, sex, height, initial weight, current weight, initial BMI, current BMI, % BMI lost, % overweight lost, incidence of incisional hernia, acceptable oral tolerance and metabolic alterations. The malabsorptive procedure associated in patients with super obesity was a 200 cm Roux-en-Y and a patients with BMI between 40 and 50 was a 150 cm Roux-en-Y. The results are compared by means of the X2 and Mann Whitney statistical test. RESULTS: The age, the sex and the stature are homogeneous in the two groups. In the group of MO the initial weight was of 121.5 kg; initial BMI, 45; current BMI; 28.9, the median loss of weight in 5 years was of 48 kg; the percentage loss of the excess of BMI is of 80% and the percentage loss of the excess of weight is of 74.6%. In the group of SO the initial weight was of 142.,7 kg; initial BMI, 54.9; current BMI, 34.,9; the median loss of weight in 5 years was of 54 kg; the percentage loss of the excess of BMI was of 65,3% and the percentage loss of the excess of weight was of 63.2%. The analysis of the results ponders shows that it exists statistically significant differences (P < 0.05) among the two groups, however the rate of success, according to the classic parameter of loss of more than 50% of the excess of weight, was superior to 90% in both groups. The results of the study about the presence of incisional postoperative hernia, alimentary tolerance and metabolic alterations, indicate that it doesn't exist differences statistically significant between both groups. CONCLUSIONS: GB is an effective surgical technique in patients with morbid obesity and with super obesity, provided that in these patients is realized a procedure more malabsorptive. There are not differences between both groups, in morbidity, improvement in the associate disease, alimentary tolerance and necessity of nutritional supplements.

Colovesical fistula complicating diverticular disease: one-stage resection.

Colonic diverticular disease is common in developed countries, and its prevalence increases with age. Most affected individuals remain asymptomatic throughout their lives, and relatively few patients require surgical intervention for obstructive or inflammatory complications. Colovesical fistula is the most common type (65%) of fistula associated with colonic diverticular disease. Primary resection of sigmoid colon with colorectal anastomosis performed as a one-stage procedure is its definitive treatment and can be performed safely--as simple closure, using an omental flap, or through resection and closure of bladder defect--in 90% of the patients. We report our experience with four patients suffering from colovesical fistula who were treated with primary resection of sigmoid colon and colorectal anastomosis performed as a one-step procedure. In our experience, diverting colostomy or Hartmann intervention is not recommended because of the lack of fistula definitive resolution and the possibility of additional complications.

[Bochdalek's hernia in an adult with stomach volvulus and extrapulmonary sequestration]. / Hernia de Bochdalek del adulto con volvulación gástrica y secuestro extrapulmonar.

We report a case of Bochdalek's hernia with volvulus of the stomach and extrapulmonary sequestration in an adult. A 27-year-old woman presented acute respiratory failure, pain in the left side of the chest and recurrent vomiting of sudden onset. Upon examination there was pain in the left hypochondrium that was not tolerated in decubitus position. A chest film showed an "arch" at the base on the left side and an upper gastrointestinal series revealed volvulus of the stomach. After a left thoracotomy, the stomach, spleen and greater omentum were found displaced into the thoracic cavity. After the viscera were confined to the abdomen, the hernia was repaired and the pulmonary sequestration was removed. Two years later, the patient was asymptomatic and a chest film was normal.

Bypass gástrico en el tratamiento de la obesidad mórbida y la superobesidad: estudio comparativo / Gastric bypass in the surgical treatment of the mobid obesity and super obesity: comparative study

Introducción: El Bypass Gástrico (BG) constituye en la actualidad el tratamiento quirúrgico de elección de la obesidad mórbida (IMC 50). Objetivo: El objetivo de éste trabajo es el de analizar los resultados de pérdida de peso de los primeros 52 Bypass Gástricos abiertos consecutivos de nuestra serie y comparar las pérdidas de peso en obesos mórbidos (OM) y superobesos (SO), para determinar si los pacientes superobesos pierden suficiente peso con nuestra técnica o por el contrario sería más recomendable otra técnica más malaobsortiva, como recomiendan algunos autores. Materiales y método: Estudio retrospectivo de los primeros 52 pacientes intervenidos de BG por vía abierta. Se comparan las pérdidas de peso de 32 pacientes con OM y 20 con SO a 60 meses de seguimiento. Los parámetros analizados son edad, sexo, talla, peso inicial, peso actual, IMC inicial, IMC actual, % del IMC perdido, % del sobrepeso perdido (% SPP), incidencia de hernia incisional, tolerancia alimentaría y alteraciones metabólicas. El componente malabsortivo asociado a los pacientes SO era una Y de Roux de 150 a 200 cm de pie de asa y en los pacientes con OM el pie de asa estaba entre 100 y 150 cm. Los resultados se comparan mediante el test estadístico del chi2 para porcentajes y la U de Mann Whitney para medias numéricas. Resultados: Los grupos son homogéneos en cuanto a edad media, sexo y talla. En el grupo de OM el peso inicial es de 121,5 kg, IMC inicial 45, IMC actual 28,9, la pérdida media de peso a 5 años es de 48 kg; la pérdida porcentual del exceso de IMC es del 80% y la pérdida porcentual del exceso de peso es del 74,6%. En el grupo de SO el peso inicial es de 142,7 kg, IMC inicial 54,9, IMC actual 34,9, la pérdida media de peso a 5 años es de 54 kg; la pérdida porcentual del exceso de IMC es del 65,3% y la pérdida porcentual del exceso de peso es del 63,2%. Las diferencias en cuanto a resultados ponderales resultan estadísticamente significativas en los dos grupos (P < 0,05), sin embargo la tasa de éxitos, según el parámetro clásico de pérdida de más del 50% del exceso de peso, es superior al 90% en ambos grupos. Los resultados del estudio sobre la presencia de hernia incisional postoperatoria, tolerancia alimentaria y alteraciones metabólicas, indican que no existen diferencias estadísticamente significativas entre los dos grupos. Conclusiones: El BG es una técnica eficaz en el tratamiento quirúrgico de la obesidad tanto en el paciente con obesidad mórbida, como en el paciente con superobesidad, siempre que se aplique en estos últimos un mayor grado de malabsorción. No existe diferencia en la morbilidad, mejoría de la enfermedad asociada, tolerancia a la ingesta y en la necesidad de suplementos nutricionales entre los grupos

Introduction: Gastric Bypass (GB) constitutes the surgical treatment of election of morbid obesity (BMI 50). Objective: The purpose of this work is one of to analyze the results of loss of weight of the first 52 open GB of our series, and to compare the losses of weight in morbid obesity (MO) and super obesity (SO), to determine if the superobese patient looses enough weight with this technique or if it would be more indicated another technique more malabsorptive, like some authors recommend. Materials and method: Retrospective study of the first 52 patients operated of open GB pathway. The weight loss of 32 patients’ with MO are compared with the weight loss of 20 patients with super obesity after five year follow-up. The parameters analyzed are: age, sex, height, initial weight, current weight, initial BMI, current BMI, % BMI lost, % overweight lost, incidence of incisional hernia, acceptable oral tolerance and metabolic alterations. The mal absorptive procedure associated in patients with super obesity was a 200 cm Roux-en-Y and a patients with BMI between 40 and 50 was a 150 cm Roux-en-Y. The results are compared by means of the X2 and Mann Whitney statistical test. Results: The age, the sex and the stature are homogeneous in the two groups. In the group of MO the initial weight was of 121,5 kg; initial BMI, 45; current BMI; 28,9, the median loss of weight in 5 years was of 48 kg; the percentage loss of the excess of BMI is of 80% and the percentage loss of the excess of weight is of 74,6%. In the group of SO the initial weight was of 142,7 kg; initial BMI, 54,9; current BMI, 34,9; the median loss of weight in 5 years was of 54 kg; the percentage loss of the excess of BMI was of 65,3% and the percentage loss of the excess of weight was of 63,2%.The analysis of the results ponders shows that it exists statistically significant differences (P < 0,05) among the two groups, however the rate of success, according to the classic parameter of loss of more than 50% of the excess of weight, was superior to 90% in both groups. The results of the study about the presence of incisional postoperative hernia, alimentary tolerance and metabolic alterations, indicate that it doesn’t exist differences statistically significant between both groups. Conclusions: GB is an effective surgical technique in patients with morbid obesity and with super obesity, provided that in these patients is realized a procedure more malabsorptive. There are not differences between both groups, in morbidity, improvement in the associate disease, alimentary tolerance and necessity of nutritional supplements

Sarcoma de células claras gigante de muslo: cuadro clínico, diagnóstico y tratamiento / Thigh giant clear cell sarcoma: clinical aspect, diagnosis and treatment

El sarcoma de células claras de tendones y aponeurosis,es una tumoración infrecuente que afecta principalmentea las extremidades inferiores de adultos jóvenes. Presentamos un caso de una paciente de 72 años de edad, que debutó con una tumoración no dolorosa en la raíz delmuslo izquierdo de dos años de evolución. La resonanciamagnética y la citología por aspiración orientaron el diagnóstico. Tras descartar diseminación a distancia se realizó extirpación en bloque de toda la tumoración. El estudio anatomopatológico de la pieza quirúrgica confirmó la presencia de un sarcoma de células claras. La paciente recibió radioterapia y quimioterapia postoperatoria y se encuentra libre de enfermedad seis meses después

Clear cell sarcoma of tendons and aponeuroses is a rareagressive soft tissue tumour that usually appears in the lower extremities of young adults and frequently producesmelanin. We report the case of a previously healthy 72-year- old- woman with clear cell sarcoma of the left thigh who presented with a large painless mass of 2 year´s duration. MR imaging showed the tumour to be of high signal intensity on fast spin-echo and STIR images. The fine needle aspiration showed abundant melanin pigments. There was no evidence of metastatic disease. We performed resection with complete removal of the tumour. Histologic diagnosis was compatible with clear cell sarcoma. The patient received adjuvant chemotherapy and radiotherapy. She is free of disease at 6 months of follow-up