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The achievement of microarcsecond relative astrometry in the near-infrared, with ground-based extremely large telescopes (ELTs) requires an extremely careful calibration strategy. In this paper we address the removal of optical distortions originating from the ELT's first light instrument MICADO and its adaptive optics system MAORY by means of a Warm Astrometric calibration Mask (WAM). The results of the test campaign on small spatial scales (1.5 mm) of a prototype mask has confirmed the manufacturing precision down to ∼50 nm/1 mm scale, leading to a relative precision of δ ∼ 5 10−5. The assessed manufacturing precision indicates that an astrometric relative precision of δ ∼ 5 10 − 5 = 50 as 1 ″ , corresponding to the MICADO astrometric requirement, is in principle achievable, reaching microarcsecond near-infrared astrometry on an ELT. The impact of ∼20 nm, (peak to valley) error residuals on position of the pinholes of the mask is tolerable at a calibration level as confirmed by ray tracing simulations of realistic MICADO distortion patterns affected by mid spatial frequencies (MSFs) residuals. Here we demonstrate that the MICADO astrometric precision of 50 as over 1″ field of view is also achievable in the presence of a MSFs pattern and manufacturing errors of the WAM, found by fitting the distorted WAM pattern seen through the instrument with a 10th order Legendre polynomial.

A novel panoramic stereo imaging system is proposed in this paper. The system is able to carry out a 360° stereoscopic vision, useful for rover autonomous-driving, and capture simultaneously a high-resolution stereo scene. The core of the concept is a novel \"bifocal panoramic lens\" (BPL) based on hyper hemispheric model (Pernechele et al. 2016). This BPL is able to record a panoramic field of view (FoV) and, simultaneously, an area (belonging to the panoramic FoV) with a given degree of magnification by using a unique image sensor. This strategy makes possible to avoid rotational mechanisms. Using two BPLs settled in a vertical baseline (system called PANROVER) allows the monitoring of the surrounding environment in stereoscopic (3D) mode and, simultaneously, capturing an high-resolution stereoscopic images to analyse scientific cases, making it a new paradigm in the planetary rovers framework.Differently from the majority of the Mars systems which are based on rotational mechanisms for the acquisition of the panoramic images (mosaicked on ground), the PANROVER does not contain any moving components and can rescue a hi-rate stereo images of the context panorama.Scope of this work is the geometric calibration of the panoramic acquisition system by the omnidirectional calibration methods (Scaramuzza et al. 2006) based on Zhang calibration grid. The procedures are applied in order to obtain well rectified synchronized stereo images to be available for 3D reconstruction. We applied a Zhang chess boards based approach even during STC/SIMBIO-SYS stereo camera calibration (Simioni et al. 2014, 2017). In this case the target of the calibration will be the stereo heads (the BPLs) of the PANROVER with the scope of extracting the intrinsic parameters of the optical systems. Differently by previous pipelines, using the same data bench the estimate of the extrinsic parameters is performed.

Dual-mirror Schwarzschild-Couder (SC) telescopes are based on highly aspherical optics, and they represent a novel design in the world of very high energy astrophysics. This work addresses the realization and the qualification of the secondary mirror for an SC telescope, named ASTRI, developed in the context of the Cherenkov Telescope Array Observatory. The discussion surveys the overall development from the early design concept to the final acceptance optical tests.

The achievement of microarcsecond relative astrometry in the near-infrared, with ground-based extremely large telescopes (ELTs) requires an extremely careful calibration strategy. In this paper we address the removal of optical distortions originating from the ELT’s first light instrument MICADO and its adaptive optics system MAORY by means of a Warm Astrometric calibration Mask (WAM). The results of the test campaign on small spatial scales (1.5 mm) of a prototype mask has confirmed the manufacturing precision down to ∼50 nm/1 mm scale, leading to a relative precision of δσ ∼ 5 · 10−5. The assessed manufacturing precision indicates that an astrometric relative precision of δ σ ~ 5 ⋅ 10 − 5 = 50 μ as 1 ′ ′ , corresponding to the MICADO astrometric requirement, is in principle achievable, reaching microarcsecond near-infrared astrometry on an ELT. The impact of ∼20 nm, (peak to valley) error residuals on position of the pinholes of the mask is tolerable at a calibration level as confirmed by ray tracing simulations of realistic MICADO distortion patterns affected by mid spatial frequencies (MSFs) residuals. Here we demonstrate that the MICADO astrometric precision of 50 μas over 1″ field of view is also achievable in the presence of a MSFs pattern and manufacturing errors of the WAM, found by fitting the distorted WAM pattern seen through the instrument with a 10th order Legendre polynomial.

SOXS (Son Of X-Shooter) is the new ESO instrument that is going to be installed on the 3.58-m New Technology Telescope at the La Silla Observatory. SOXS is a single object spectrograph offering a wide simultaneous spectral coverage from U- to H-band. Although such an instrument may have potentially a large variety of applications, the consortium designed it with a clear science case: it is going to provide the spectroscopic counterparts to the ongoing and upcoming imaging surveys, becoming one of the main follow-up instruments in the Southern hemisphere for the classification and characterization of transients. The NTT+SOXS system is specialized to observe all transients and variable sources discovered by imaging surveys with a flexible schedule maintained by the consortium, based on a remote scheduler which will interface with the observatory software infrastructure. SOXS is realized timely to be highly synergic with transients discovery machines like the Vera C. Rubin Observatory. The instrument has been integrated and tested in Italy, collecting and assembling subsystems coming from all partners spread over six countries in three continents. The first preparatory activities in Chile have been completed at the telescope. This article gives an updated status of the project before the shipping of the instrument to Chile.

SOXS (Son Of X-Shooter) will be the new medium-resolution (R 4500 for 1 slit), high-efficiency, wide-band spectrograph for the ESO NTT at La Silla Observatory, Chile. It will be dedicated to the follow-up of any kind of transient events, ensuring fast time, high efficiency, and availability. It consists of a central structure (common path) that supports two spectrographs optimized for the UV-Visible and a Near-Infrared range. Attached to the common path is the Acquisition and Guiding Camera system (AC), equipped with a filter wheel that can provide science-grade imaging and moderate high-speed photometry. The AC Unit was integrated and aligned during the summer months of 2022 and has since been mounted in the NTTs telescope simulator. This work gives an update on the Acquisition Camera Unit status, describes the Image Quality Tests that were performed, and discusses the AC Optical Performance.

Food producing and processing industries face with several challenges regarding food illumination (e.g., providing a high quality light experience and color rendering while facilitating inspections) and using Ultraviolet (UV) light for sanitizing, disinfection or germicidal treatments both in food production lines and for the food itself directly or through tools (i.e., used in packaging and processing). The paper describes the development of an innovative product, called RLTProFood (remote LED light technology for processing and producing food), that was designed for giving a customized LED-based lighting system able to deliver different source light from visible to UV according the benefits required by customers. Currently developed in two main configurations (e.g., LED visible light and UV LED light), the product has its main application in the context of processing and producing fresh and possibly organic food especially fruits and vegetables.

The Son Of X-Shooter (SOXS) is a single object spectrograph offering simultaneous spectral coverage in UV-VIS (350-850 nm) and NIR (800-2000 nm) wavelength regimes with an average of R close to 4500 for a 1 slit. SOXS also has imaging capabilities in the visible wavelength regime. It is designed and optimized to observe all kinds of transients and variable sources. The final destination of SOXS is the Nasmyth platform of the ESO NTT at La Silla, Chile. The SOXS consortium has a relatively large geographic spread, and therefore the Assembly Integration and Verification (AIV) of this medium-class instrument follows a modular approach. Each of the five main sub-systems of SOXS, namely the Common Path, the Calibration Unit, the Acquisition Camera, the UV-VIS Spectrograph, and the NIR Spectrograph, are undergoing (or undergone) internal alignment and testing in the respective consortium institutes. INAF-Osservatorio Astronomico di Padova delivers the Common Path sub-system, the backbone of the entire instrument. We report the Common Path internal alignment starting from the assembly of the individual components to the final testing of the optical quality, and the efficiency of the complete sub-system.

SOXS (Son Of X-Shooter) is a single object spectrograph offering a simultaneous spectral coverage from U- to H-band, built by an international consortium for the 3.58-m ESO New Technology Telescope at the La Silla Observatory. It is designed to observe all kind of transients and variable sources discovered by different surveys with a highly flexible schedule maintained by the consortium, based on the Target of Opportunity concept. SOXS is going to be a fundamental spectroscopic partner for any kind of imaging survey, becoming one of the premier transient follow-up instruments in the Southern hemisphere. This paper gives an updated status of the project, when the instrument is in the advanced phase of integration and testing in Europe, prior to the activities in Chile.

The Son Of X-Shooter (SOXS) is a two-channel spectrograph along with imaging capabilities, characterized by a wide spectral coverage (350nm to 2000nm), designed for the NTT telescope at the La Silla Observatory. Its main scientific goal is the spectroscopic follow-up of transients and variable objects. The UV-VIS arm, of the Common Path sub-system, is characterized by the presence of a powered Atmospheric Dispersion Corrector composed (ADC) by two counter-rotating quadruplets, two prisms, and two lenses each. The presence of powered optics in both the optical groups represents an additional challenge in the alignment procedures. We present the characteristics of the ADC, the analysis after receiving the optics from the manufacturer, the emerging issues, the alignment strategies we followed, and the final results of the ADC in dispersion and optical quality.