RESUMEN
The SuperCam instrument suite provides the Mars 2020 rover, Perseverance, with a number of versatile remote-sensing techniques that can be used at long distance as well as within the robotic-arm workspace. These include laser-induced breakdown spectroscopy (LIBS), remote time-resolved Raman and luminescence spectroscopies, and visible and infrared (VISIR; separately referred to as VIS and IR) reflectance spectroscopy. A remote micro-imager (RMI) provides high-resolution color context imaging, and a microphone can be used as a stand-alone tool for environmental studies or to determine physical properties of rocks and soils from shock waves of laser-produced plasmas. SuperCam is built in three parts: The mast unit (MU), consisting of the laser, telescope, RMI, IR spectrometer, and associated electronics, is described in a companion paper. The on-board calibration targets are described in another companion paper. Here we describe SuperCam's body unit (BU) and testing of the integrated instrument. The BU, mounted inside the rover body, receives light from the MU via a 5.8 m optical fiber. The light is split into three wavelength bands by a demultiplexer, and is routed via fiber bundles to three optical spectrometers, two of which (UV and violet; 245-340 and 385-465 nm) are crossed Czerny-Turner reflection spectrometers, nearly identical to their counterparts on ChemCam. The third is a high-efficiency transmission spectrometer containing an optical intensifier capable of gating exposures to 100 ns or longer, with variable delay times relative to the laser pulse. This spectrometer covers 535-853 nm ( 105 - 7070 cm - 1 Raman shift relative to the 532 nm green laser beam) with 12 cm - 1 full-width at half-maximum peak resolution in the Raman fingerprint region. The BU electronics boards interface with the rover and control the instrument, returning data to the rover. Thermal systems maintain a warm temperature during cruise to Mars to avoid contamination on the optics, and cool the detectors during operations on Mars. Results obtained with the integrated instrument demonstrate its capabilities for LIBS, for which a library of 332 standards was developed. Examples of Raman and VISIR spectroscopy are shown, demonstrating clear mineral identification with both techniques. Luminescence spectra demonstrate the utility of having both spectral and temporal dimensions. Finally, RMI and microphone tests on the rover demonstrate the capabilities of these subsystems as well.
RESUMEN
Ectodermal dysplasia with immune deficiency (EDI) is caused by alterations in NEMO (nuclear factor [NF]-kappaB essential modulator). Most genetic mutations are located in exon 10 and affect the C-terminal zinc finger domain. However, the biochemical mechanism by which they cause immune dysfunction remains undetermined. In this report, we investigated the effect of a cysteine-to-arginine mutation (C417R) found in the NEMO zinc finger domain on dendritic cell (DC) function. Following CD40 stimulation of DCs prepared from 2 unrelated patients with the NEMO C417R mutation, we found NEMO ubiquitination was absent, and this was associated with preserved RelA but absent c-Rel activity. As a consequence, CD40 stimulated EDI DCs failed to synthesize the c-Rel-dependent cytokine interleukin-12, had impaired up-regulation of costimulatory molecules, and failed to support allogeneic lymphocyte proliferation in vitro. In contrast, EDI DCs stimulated with the TLR4 ligand lipopolysaccharide (LPS) showed normal downstream NF-kappaB activity, DC maturation, and NEMO ubiquitination. These findings show for the first time how mutations in the zinc finger domain of NEMO can lead to pathway specific defects in NEMO ubiquitination and thus immune deficiency.
