Key Points Question Did human mobility patterns change during stay-at-home orders and were the mobility changes associated with the coronavirus disease 2019 (COVID-19) curve? Findings This cross-sectional study using anonymous location data from more than 45 million mobile phones found that median travel distance decreased and stay-at-home time increased across the nation, although there was geographic variation. State-specific empirical doubling time of total COVID-19 cases increased (ie, the spread reduced) significantly after stay-at-home orders were put in place. Meaning These findings suggest that stay-at-home social distancing mandates were associated with the reduced spread of COVID-19 when they were followed.

We present the results of a model-based search for continuous gravitational waves from the low-mass X-ray binary Scorpius X-1 using LIGO detector data from the third observing run of Advanced LIGO and Advanced Virgo. This is a semicoherent search that uses details of the signal model to coherently combine data separated by less than a specified coherence time, which can be adjusted to balance sensitivity with computing cost. The search covered a range of gravitational-wave frequencies from 25 to 1600 Hz, as well as ranges in orbital speed, frequency, and phase determined from observational constraints. No significant detection candidates were found, and upper limits were set as a function of frequency. The most stringent limits, between 100 and 200 Hz, correspond to an amplitude h 0 of about 10−25 when marginalized isotropically over the unknown inclination angle of the neutron star’s rotation axis, or less than 4 × 10−26 assuming the optimal orientation. The sensitivity of this search is now probing amplitudes predicted by models of torque balance equilibrium. For the usual conservative model assuming accretion at the surface of the neutron star, our isotropically marginalized upper limits are close to the predicted amplitude from about 70 to 100 Hz; the limits assuming that the neutron star spin is aligned with the most likely orbital angular momentum are below the conservative torque balance predictions from 40 to 200 Hz. Assuming a broader range of accretion models, our direct limits on gravitational-wave amplitude delve into the relevant parameter space over a wide range of frequencies, to 500 Hz or more.

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Con el objeto de describir la relación entre las variables climáticas y las respuestas fisiológicas, 20 ovejas fueron asignadas a: Con Sombra (CS): sombra artificial (12:00 - 14:00 h) en corral con techo de malla sombra (70%); Sin Sombra (SS): sin ofrecimiento de sombra. Se determinó radiación solar (RS; W/m2), temperatura ambiental (°C), humedad relativa (%), temperatura de globo negro (TGN; °C) e índice de temperatura-humedad (ITH; unidades), temperatura superficial (TS; °C; termómetro infrarrojo), temperatura corporal (TC; °C; termómetro digital), frecuencia respiratoria (FR; mov/min; observación directa) y coeficiente de tolerancia al calor (CTC; unidades) (PROC MIXED; SAS).Adicionalmente, los datos fueron analizados por componentes principales (InfoStat/E, 2008).CS presenta una menor TS (35,9) en comparación con SS (38,9; P ≤ 0,01); igual ocurre en TC (P ≤ 0,01). La FR en CS (112,3) fue superior a SS (139,6; P ≤ 0,01). El CTC fue mayor en SS (7,8) vs. CS (5,8; P ≤ 0,01), indicando mejor bienestar térmico en CS. La TS en lomo, cadera y/o costado presenta alta relación con TC. TGN > 42,8 y de RS > 529,1 podrían indicar reducciones del bienestar térmico. Basado en la TC y FR, el punto de quiebre del ITH en ovinos es > 80.