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In this paper we present attenuation formulas for horizontal Peak Ground Accelerations (PGA) and horizontal Spectral Accelerations (SA) for subduction interface earthquakes recording in the Chilean

CHIRON2

CHIRON is a highly stable cross-dispersed echelle spectrometer deployed at CTIO 1.5m telescope. It is fed by fiber and intended primarily for precise radial velocities.

Reflection seismic images and amplitude ratio modelling of the Chilean

The aim of this paper is to obtain an integrative image of the continental crust and the plate interface in southern Chile, to quantitatively study their petrophysical properties, such as

Three-dimensional electrical resistivity image of the South-Central

The new 3-D conductivity image of the South-Central Chilean subduction zone basically confirms former 2-D inversion models along three profiles and complete the previous results.

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In this context, the development of attenuation relations for the earthquakes that occurs in this specific subduction zone is an important input in the seismic hazard assessment of Chile, and eventually for

FAQ for CHIRON on the CTIO/SMARTS 1

3.3 Is there a program to calculate when a star can be observed at the 1.5m with CHIRON on a given night, and for how long it can be observed on various nights throughout the year?

Ground motion prediction equations for the

Intraslab earthquakes show a steeper attenuation slope than that of interface ones, which is consistent with other GMPE results derived from worldwide subduction zones data. Moreover, the Chilean

Chile (SUBTEL)

Subsecretaría de Telecomunicaciones (SUBTEL) of Chile issued Resolution 1807 on October 22, 2020. This Resolution modifies the Resolution 1985 "On fixed technical standards for SRD".

CHIRON | NOIRLab Science

CHIRON is a highly stable cross-dispersed echelle spectrometer at the SMARTS-GSU 1.5-meter telescope. It is fed by fiber and intended primarily for precise radial velocities.

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