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Found 11 papers, 2 papers with code
Improving Earth-like planet detection in radial velocity using deep learning
By injecting simulated planetary signals at the spectral level, we demonstrate that our machine learning algorithm can achieve, for HD128621 and HD10700, a detection threshold of 0. 5 m/s in semi-amplitude for planets with periods ranging from 10 to 300 days.
Development status of the UV-VIS detector system of SOXS for the ESO-NTT telescope
The first tests of the detector system with the UV-VIS camera will be shown.
Instrumentation and Methods for Astrophysics
Design and development of the SOXS calibration unit
The calibration unit will employ seven calibration lamps: a quartz-tungsten-halogen and a deuterium lamp for the flat-field correction, a ThAr lamp and four pencil-style rare-gas lamps for the wavelength calibration.
Instrumentation and Methods for Astrophysics
Development status of the SOXS instrument control software
SOXS (Son Of X-Shooter) is a forthcoming instrument for ESO-NTT, mainly dedicated to the spectroscopic study of transient events and is currently starting the AIT (Assembly, Integration, and Test) phase.
Instrumentation and Methods for Astrophysics
Progress on the UV-VIS arm of SOXS
We present our progress on the UV-VIS arm of Son Of X-Shooter (SOXS), a new spectrograph for the NTT.
Instrumentation and Methods for Astrophysics
SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment
SOXS (Son Of X-Shooter) is the new medium resolution wide-band spectrograph to be installed at the 3. 6m New Technology Telescope (NTT) in La Silla.
Instrumentation and Methods for Astrophysics
The AIV strategy of the Common Path of Son of X-Shooter
Son Of X-Shooter (SOXS) is a double-armed (UV-VIS, NIR) spectrograph designed to be mounted at the ESO-NTT in La Silla, now in its Assembly Integration and Verification (AIV) phase.
Instrumentation and Methods for Astrophysics
The SOXS Data-Reduction Pipeline
The SOXS is a dual-arm spectrograph (UV-VIS & NIR) and AC due to mounted on the ESO 3. 6m NTT in La Silla.
Instrumentation and Methods for Astrophysics
The SOXS scheduler for remote operation at LaSilla:Concept and design
In this paper we present the SOXS Scheduler, a web-based application aimed at optimising remote observations at the NTT-ESO in the context of scientific topics of both the SOXS Consortium and regular ESO proposals. This paper will give details of how detected transients from various surveys are inserted, prioritised, and selected for observations with SOXS at the NTT while keeping the correct sharing between GTO time (for the SOXSConsortium) and the regularly approved observing time from ESO proposals.
Instrumentation and Methods for Astrophysics
Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks
We trained our machine learning models on both simulated data (generated with the SOAP 2. 0 software; Dumusque et al. 2014) and observations of the Sun from the HARPS-N Solar Telescope (Dumusque et al. 2015; Phillips et al. 2016; Collier Cameron et al. 2019).
Architecture of the SOXS instrument control software
We illustrate the control network, the instrument functions and detectors to be controlled, the overall design of SOXS Instrument Software (INS) and its main components.
Instrumentation and Methods for Astrophysics
