The existence of hot Jupiters is still not well understood. Two main channels are thought to be responsible for their current location: a smooth planet migration through the proto-planetary disk or ...the circularization of an initial high eccentric orbit by tidal dissipation leading to a strong decrease of the semimajor axis. Different formation scenarios result in different observable effects, such as orbital parameters (obliquity/eccentricity), or frequency of planets at different stellar ages. In the context of the GAPS Young-Objects project, we are carrying out a radial velocity survey with the aim to search and characterize young hot-Jupiter planets. Our purpose is to put constraints on evolutionary models and establish statistical properties, such as the frequency of these planets from a homogeneous sample. Since young stars are in general magnetically very active, we performed multi-band (visible and near-infrared) spectroscopy with simultaneous GIANO-B + HARPS-N (GIARPS) observing mode at TNG. This helps to deal with stellar activity and distinguish the nature of radial velocity variations: stellar activity will introduce a wavelength-dependent radial velocity amplitude, whereas a Keplerian signal is achromatic. As a pilot study, we present here the cases of two already claimed hot Jupiters orbiting young stars: HD285507 b and AD Leo b. Our analysis of simultaneous high-precision GIARPS spectroscopic data confirms the Keplerian nature of HD285507's radial velocities variation and refines the orbital parameters of the hot Jupiter, obtaining an eccentricity consistent with a circular orbit. On the other hand, our analysis does not confirm the signal previously attributed to a planet orbiting AD Leo. This demonstrates the power of the multi-band spectroscopic technique when observing active stars.
This document is a paper of multidisciplinary academic opinion of 27 professors and researchers of the Autonomous University of Nayarit, Mexico. In the manuscript, the pandemic of the COVID-19 ...disease is approached from different perspectives, with the aim to approach this great problem that has paralyzed humanity in the beginning of the year 2020 in an interdisciplinary form (thus many of the research problems should be approached), on the other hand, with the aim to prove all the academic potential that Mexican public universities hold to respond to society. Professors of history, biology, medicine, biomedicine, nutrition, social sciences, law, psychology, economy, tourism, political sciences, education, communication media, engineering, technological innovation, and intellectual property take part in this paper. This document represents a groundbreaking exercise in the Autonomous University of Nayarit and performing multidisciplinary work is, perhaps, one of the major lesson and message that the pandemic of COVID-19 will leave us.
GIARPS (GIAno \& haRPS) is a project devoted to have on the same focal station of the Telescopio Nazionale Galileo (TNG) both high resolution spectrographs, HARPS-N (VIS) and GIANO-B (NIR), working ...simultaneously. This could be considered the first and unique worldwide instrument providing cross-dispersed echelle spectroscopy at a resolution of 50,000 in the NIR range and 115,000 in the VIS and over in a wide spectral range (\(0.383 - 2.45\ \mu\)m) in a single exposure. The science case is very broad, given the versatility of such an instrument and its large wavelength range. A number of outstanding science cases encompassing mainly extra-solar planet science starting from rocky planets search and hot Jupiters to atmosphere characterization can be considered. Furthermore both instruments can measure high precision radial velocities by means the simultaneous thorium technique (HARPS-N) and absorbing cell technique (GIANO-B) in a single exposure. Other science cases are also possible. GIARPS, as a brand new observing mode of the TNG started after the moving of GIANO-A (fiber fed spectrograph) from Nasmyth-A to Nasmyth-B where it was re-born as GIANO-B (no more fiber feed spectrograph). The official Commissioning finished on March 2017 and then it was offered to the community. Despite the work is not finished yet. In this paper we describe the preliminary scientific results obtained with GIANO-B and GIARPS observing mode with data taken during commissioning and first open time observations.
LOCNES (LOw-Cost NIR Extended Solar telescope) is a solar telescope installed at the TNG (Telescopio Nazionale Galileo). It feeds the light of the Sun into the NIR spectrograph GIANO-B through a 40-m ...patch of optical fibers. LOCNES has been designed to obtain high signal-to-noise ratio spectra of the Sun as a star with an accurate wavelength calibration through molecular-band cells. This is an entirely new area of investigation that will provide timely results to improve the search of telluric planets with NIR spectrographs such as iSHELL, CARMENES, and GIANO-B. We will extract several disc-integrated activity indicators and average magnetic field measurements for the Sun in the NIR. Eventually, they will be correlated with both the RV of the Sun-as-a -star and the resolved images of the solar disc in visible and NIR. Such an approach will allow for a better understanding of the origin of activity-induced RV variations in the two spectral domains and will help in improving the techniques for their corrections. In this paper, we outline the science drivers for the LOCNES project and its first commissioning results.
ABSTRACT The COVID-19 pandemic has caused a decrease in tourism activity. This has caused huge losses to the tourism industry, so different approaches have been devised for economic reactivation. ...This article aims to provide a novel strategy for mass molecular monitoring of clinically healthy individuals, and also including potentially asymptomatic carriers of SARS-CoV-2, who traveled to a tourist resort The monitoring consisted of collecting individual saliva samples (n=120) and conforming groups of 10 samples, thus setting 12 individual pools, which were analyzed by qRT-PCR. Obtained data showed that all the samples analyzed were negative, thus confirming that no individuals were infected with SARS-CoV-2 before and during the travel. The proposed molecular protocol allowed the analysis of massive saliva samples and detect individual infected persons (negative or positive). protocol for evaluate massive event, thus promoting the economic activation of the tourism industry.
Context. Stellar activity is currently challenging the detection of young planets via the radial velocity (RV) technique. Aims. We attempt to definitively discriminate the nature of the RV variations ...for the young active K5 star BD+20 1790, for which visible (VIS) RV measurements show divergent results on the existence of a substellar companion. Methods. We compare VIS data with high precision RVs in the near infrared (NIR) range by using the GIANO - B and IGRINS spectrographs. In addition, we present for the first time simultaneous VIS-NIR observations obtained with GIARPS (GIANO - B and HARPS - N) at Telescopio Nazionale Galileo (TNG). Orbital RVs are achromatic, so the RV amplitude does not change at different wavelengths, while stellar activity induces wavelength-dependent RV variations, which are significantly reduced in the NIR range with respect to the VIS. Results. The NIR radial velocity measurements from GIANO - B and IGRINS show an average amplitude of about one quarter with respect to previously published VIS data, as expected when the RV jitter is due to stellar activity. Coeval multi-band photometry surprisingly shows larger amplitudes in the NIR range, explainable with a mixture of cool and hot spots in the same active region. Conclusions. In this work, the claimed massive planet around BD+20 1790 is ruled out by our data. We exploited the crucial role of multi- wavelength spectroscopy when observing young active stars: thanks to facilities like GIARPS that provide simultaneous observations, this method can reach its maximum potential.
Since 2012, thanks to the installation of the high resolution echelle spectrograph in the optical range HARPS-N, the Italian telescope TNG (La Palma) became one of the key facilities for the study of ...the extrasolar planets. In 2014 TNG also offered GIANO to the scientific community, providing a near-infrared (NIR) cross-dispersed echelle spectroscopy covering 0.97 - 2.45 micron at a resolution of 50,000. GIANO, although designed for direct light-feed from the telescope at the Nasmyth-B focus, was provisionally mounted on the rotating building and connected via fibers to only available interface at the Nasmyth-A focal plane. The synergy between these two instruments is particularly appealing for a wide range of science cases, especially for the search for exoplanets around young and active stars and the characterisation of their atmosphere. Through the funding scheme "WOW" (a Way to Others Worlds), the Italian National Institute for Astrophysics (INAF) proposed to position GIANO at the focal station for which it was originally designed and the simultaneous use of these spectrographs with the aim to achieve high-resolution spectroscopy in a wide wavelength range (0.383-2.45 micron) obtained in a single exposure, giving rise to the project called GIARPS (GIANO-B & HARPS-N). Because of its characteristics GIARPS can be considered the first and unique worldwide instrument providing not only high resolution in a large wavelength band, but also a high precision radial velocity measurement both in the visible and in the NIR arm, since in the next future GIANO-B will be equipped with gas absorption cells.
In Mexico, beef for human consumption comes from federal-inspection type (TIF, tipo inspección federal) or non-TIF slaughterhouses. The latter do not comply with all national quality and hygiene ...standards established by the Ministry of Agriculture and Rural Development (SADER, Secretaría de Agricultura y Desarrollo Rural), while TIF beef is certified by the National Service of Health, Safety, and Food Quality (SENASICA, Servicio Nacional de Sanidad, Inocuidad y Calidad Agroalimentaria), which reports to SADER. In this work the presence of Salmonella spp. was analyzed in TIF and non-TIF beef commercialized in supermarkets, as well as non-TIF beef commercialized in local butchers in Tepic, Nayarit (Mexico). Salmonella spp. was detected using qPCR, and the results indicate its presence in the three types of beef analyzed. Although a smaller proportion of contaminated samples and a lower degree of contamination were detected in it, TIF beef is not free from the presence of this pathogen and thus cannot be considered an innocuous product.
The COVID-19 pandemic has caused a decrease in tourism activity. This has caused huge losses to the tourism industry, so different approaches have been devised for economic reactivation. This article ...aims to provide a novel strategy for mass molecular monitoring of clinically healthy individuals, and also including potentially asymptomatic carriers of SARS-CoV-2, who traveled to a tourist resort The monitoring consisted of collecting individual saliva samples (n=120) and conforming groups of 10 samples, thus setting 12 individual pools, which were analyzed by qRT-PCR. Obtained data showed that all the samples analyzed were negative, thus confirming that no individuals were infected with SARS-CoV-2 before and during the travel. The proposed molecular protocol allowed the analysis of massive saliva samples and detect individual infected persons (negative or positive). protocol for evaluate massive event, thus promoting the economic activation of the tourism industry.
Son of X-Shooter (SOXS) will be a high-efficiency spectrograph with a mean
Resolution-Slit product of $\sim 4500$ over the entire band capable of
simultaneously observing the complete spectral range ...350-2000 nm. It consists
of three scientific arms (the UV-VIS Spectrograph, the NIR Spectrograph, and
the Acquisition Camera) connected by the Common Path system to the NTT, and the
Calibration Unit. The Common Path is the backbone of the instrument and the
interface to the NTT Nasmyth focus flange. The instrument project went through
the Final Design Review in 2018 and is currently in Assembly Integration and
test (AIT) Phase. This paper outlines the observing modes of SOXS and the
efficiency of each subsystem and the laboratory test plan to evaluate it.
