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1. The Extreme Stellar-Signals Project III. Combining Solar Data from HARPS, HARPS-N, EXPRES, and NEID

Author

Zhao, Lily L., Dumusque, Xavier, Ford, Eric B., Llama, Joe, Mortier, Annelies, Bedell, Megan, Moulla, Khaled Al, Bender, Chad F., Blake, Cullen H., Brewer, John M., Cameron, Andrew Collier, Cosentino, Rosario, Figueira, Pedro, Fischer, Debra A., Ghedina, Adriano, Gonzalez, Manuel, Halverson, Samuel, Kanodia, Shubham, Latham, David W., Lin, Andrea S. J., Curto, Gaspare Lo, Lodi, Marcello, Logsdon, Sarah E., Lovis, Christophe, Mahadevan, Suvrath, Monson, Andrew, Ninan, Joe P., Pepe, Francesco, Roettenbacher, Rachael M., Roy, Arpita, Santos, Nuno C., Schwab, Christian, Stefánsson, Guðmundur, Szymkowiak, Andrew E., Terrien, Ryan C., Udry, Stephane, Weiss, Sam A., Wildi, François, Wildi, Thibault, and Wright, Jason T.

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

We present an analysis of Sun-as-a-star observations from four different high-resolution, stabilized spectrographs -- HARPS, HARPS-N, EXPRES, and NEID. With simultaneous observations of the Sun from four different instruments, we are able to gain insight into the radial velocity precision and accuracy delivered by each of these instruments and isolate instrumental systematics that differ from true astrophysical signals. With solar observations, we can completely characterize the expected Doppler shift contributed by orbiting Solar System bodies and remove them. This results in a data set with measured velocity variations that purely trace flows on the solar surface. Direct comparisons of the radial velocities measured by each instrument show remarkable agreement with residual intra-day scatter of only 15-30 cm/s. This shows that current ultra-stabilized instruments have broken through to a new level of measurement precision that reveals stellar variability with high fidelity and detail. We end by discussing how radial velocities from different instruments can be combined to provide powerful leverage for testing techniques to mitigate stellar signals., Comment: 17 pages, 9 figures, accepted for publication

Published
2023

2. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Author

Jin, Shoko, Trager, Scott C., Dalton, Gavin B., Aguerri, J. Alfonso L., Drew, J. E., Falcón-Barroso, Jesús, Gänsicke, Boris T., Hill, Vanessa, Iovino, Angela, Pieri, Matthew M., Poggianti, Bianca M., Smith, D. J. B., Vallenari, Antonella, Abrams, Don Carlos, Aguado, David S., Antoja, Teresa, Aragón-Salamanca, Alfonso, Ascasibar, Yago, Babusiaux, Carine, Balcells, Marc, Barrena, R., Battaglia, Giuseppina, Belokurov, Vasily, Bensby, Thomas, Bonifacio, Piercarlo, Bragaglia, Angela, Carrasco, Esperanza, Carrera, Ricardo, Cornwell, Daniel J., Domínguez-Palmero, Lilian, Duncan, Kenneth J., Famaey, Benoit, Fariña, Cecilia, Gonzalez, Oscar A., Guest, Steve, Hatch, Nina A., Hess, Kelley M., Hoskin, Matthew J., Irwin, Mike, Knapen, Johan H., Koposov, Sergey E., Kuchner, Ulrike, Laigle, Clotilde, Lewis, Jim, Longhetti, Marcella, Lucatello, Sara, Méndez-Abreu, Jairo, Mercurio, Amata, Molaeinezhad, Alireza, Monguió, Maria, Morrison, Sean, Murphy, David N. A., de Arriba, Luis Peralta, Pérez, Isabel, Pérez-Ràfols, Ignasi, Picó, Sergio, Raddi, Roberto, Romero-Gómez, Mercè, Royer, Frédéric, Siebert, Arnaud, Seabroke, George M., Som, Debopam, Terrett, David, Thomas, Guillaume, Wesson, Roger, Worley, C. Clare, Alfaro, Emilio J., Prieto, Carlos Allende, Alonso-Santiago, Javier, Amos, Nicholas J., Ashley, Richard P., Balaguer-Núñez, Lola, Balbinot, Eduardo, Bellazzini, Michele, Benn, Chris R., Berlanas, Sara R., Bernard, Edouard J., Best, Philip, Bettoni, Daniela, Bianco, Andrea, Bishop, Georgia, Blomqvist, Michael, Boeche, Corrado, Bolzonella, Micol, Bonoli, Silvia, Bosma, Albert, Britavskiy, Nikolay, Busarello, Gianni, Caffau, Elisabetta, Cantat-Gaudin, Tristan, Castro-Ginard, Alfred, Couto, Guilherme, Carbajo-Hijarrubia, Juan, Carter, David, Casamiquela, Laia, Conrado, Ana M., Corcho-Caballero, Pablo, Costantin, Luca, Deason, Alis, de Burgos, Abel, De Grandi, Sabrina, Di Matteo, Paola, Domínguez-Gómez, Jesús, Dorda, Ricardo, Drake, Alyssa, Dutta, Rajeshwari, Erkal, Denis, Feltzing, Sofia, Ferré-Mateu, Anna, Feuillet, Diane, Figueras, Francesca, Fossat, Matteo, Franciosin, Elena, Frasca, Antonio, Fumagalli, Michele, Gallazzi, Anna, García-Benito, Rubén, Fusillo, Nicola Gentile, Gebran, Marwan, Gilbert, James, Gledhill, T. M., Delgado, Rosa M. González, Greimel, Robert, Guarcello, Mario Giuseppe, Guerra, Jose, Gullieuszik, Marco, Haines, Christopher P., Hardcastle, Martin J., Harris, Amy, Haywood, Misha, Helmi, Amina, Hernandez, Nauzet, Herrero, Artemio, Hughes, Sarah, Irsic, Vid, Jablonka, Pascale, Jarvis, Matt J., Jordi, Carme, Kondapally, Rohit, Kordopatis, Georges, Krogager, Jens-Kristian, La Barbera, Francesco, Lam, Man I, Larsen, Søren S., Lemasle, Bertrand, Lewis, Ian J., Lhomé, Emilie, Lind, Karin, Lodi, Marcello, Longobardi, Alessia, Lonoce, Ilaria, Magrin, Laura, Apellániz, Jesús Maíz, Marchal, Olivier, Marco, Amparo, Martin, Nicolas F., Matsuno, Tadafumi, Maurogordato, Sophie, Merluzzi, Paola, Miralda-Escudé, Jordi, Molinari, Emilio, Monari, Giacomo, Morelli, Lorenzo, Mottram, Christopher J., Naylor, Tim, Negueruela, Ignacio, Oñorbe, Jose, Pancino, Elena, Peirani, Sébastien, Peletier, Reynier F., Pozzetti, Lucia, Rainer, Monica, Ramos, Pau, Read, Shaun C., Rossi, Elena Maria, Röttgering, Huub J. A., Rubiño-Martín, Jose Alberto, Montes, Jose Sabater, Juan, José San, Sanna, Nicoletta, Schallig, Ellen, Schiavon, Ricardo P., Schultheis, Mathias, Serra, Paolo, Shimwell, Timothy W., Simón-Díaz, Sergio, Smith, Russell J., Sordo, Rosanna, Sorini, Daniele, Soubiran, Caroline, Starkenburg, Else, Steele, Iain A., Stott, John, Stuik, Remko, Tolstoy, Eline, Tortora, Crescenzo, Tsantaki, Maria, Van der Swaelmen, Mathieu, van Weeren, Reinout J., Vergani, Daniela, Verheijen, Marc A. W., Verro, Kristiina, Vink, Jorick S., Vioque, Miguel, Walcher, C. Jakob, Walton, Nicholas A., Wegg, Christopher, Weijmans, Anne-Marie, Williams, Wendy L., Wilson, Andrew J., Wright, Nicholas J., Xylakis-Dornbusch, Theodora, Youakim, Kris, Zibetti, Stefano, and Zurita, Cristina

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366$-$959\,nm at $R\sim5000$, or two shorter ranges at $R\sim20\,000$. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for $\sim$3 million stars and detailed abundances for $\sim1.5$ million brighter field and open-cluster stars; (ii) survey $\sim0.4$ million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey $\sim400$ neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in $z<0.5$ cluster galaxies; (vi) survey stellar populations and kinematics in $\sim25\,000$ field galaxies at $0.3\lesssim z \lesssim 0.7$; (vii) study the cosmic evolution of accretion and star formation using $>1$ million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at $z>2$. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator., Comment: 41 pages, 27 figures, accepted for publication by MNRAS; updated version including information on individual grants in a revised Acknowledgements section, corrections to the affiliation list, and an updated references list

Published
2022
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3. Five carbon- and nitrogen-bearing species in a hot giant planet's atmosphere

Author

Giacobbe, Paolo, Brogi, Matteo, Gandhi, Siddharth, Cubillos, Patricio E., Bonomo, Aldo S., Sozzetti, Alessandro, Fossati, Luca, Guilluy, Gloria, Carleo, Ilaria, Rainer, Monica, Harutyunyan, Avet, Borsa, Francesco, Pino, Lorenzo, Nascimbeni, Valerio, Benatti, Serena, Biazzo, Katia, Bignamini, Andrea, Chubb, Katy L., Claudi, Riccardo, Cosentino, Rosario, Covino, Elvira, Damasso, Mario, Desidera, Silvano, Fiorenzano, Aldo F. M., Ghedina, Adriano, Lanza, Antonino F., Leto, Giuseppe, Maggio, Antonio, Malavolta, Luca, Maldonado, Jesus, Micela, Giuseppina, Molinari, Emilio, Pagano, Isabella, Pedani, Marco, Piotto, Giampaolo, Poretti, Ennio, Scandariato, Gaetano, Yurchenko, Sergei N., Fantinel, Daniela, Galli, Alberto, Lodi, Marcello, Sanna, Nicoletta, and Tozzi, Andrea

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

The atmospheres of gaseous giant exoplanets orbiting close to their parent stars (hot Jupiters) have been probed for nearly two decades. They allow us to investigate the chemical and physical properties of planetary atmospheres under extreme irradiation conditions. Previous observations of hot Jupiters as they transit in front of their host stars have revealed the frequent presence of water vapour and carbon monoxide in their atmospheres; this has been studied in terms of scaled solar composition under the usual assumption of chemical equilibrium. Both molecules as well as hydrogen cyanide were found in the atmosphere of HD 209458b, a well studied hot Jupiter (with equilibrium temperature around 1,500 kelvin), whereas ammonia was tentatively detected there and subsequently refuted. Here we report observations of HD 209458b that indicate the presence of water (H2O), carbon monoxide (CO), hydrogen cyanide (HCN), methane (CH4), ammonia (NH3) and acetylene (C2H2), with statistical significance of 5.3 to 9.9 standard deviations per molecule. Atmospheric models in radiative and chemical equilibrium that account for the detected species indicate a carbon-rich chemistry with a carbon-to-oxygen ratio close to or greater than 1, higher than the solar value (0.55). According to existing models relating the atmospheric chemistry to planet formation and migration scenarios, this would suggest that HD 209458b formed far from its present location and subsequently migrated inwards. Other hot Jupiters may also show a richer chemistry than has been previously found, which would bring into question the frequently made assumption that they have solar-like and oxygen-rich compositions., Comment: As part of the Springer Nature Content Sharing Initiative, it is possible to access a view-only version of this paper by using the following SharedIt link: https://rdcu.be/cifrz

Published
2021
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4. GIARPS: the unique VIS-NIR high precision radial velocity facility in this world

Author

Claudi, Riccardo, Benatti, Serena, Carleo, Ilaria, Ghedina, Adriano, Molinari, Emilio, Oliva, Ernesto, Tozzi, Andrea, Baruffolo, Andrea, Cecconi, Massimo, Cosentino, Rosario, Fantinel, Daniela, Fini, Luca, Ghinassi, Francesca, Gonzalez, Manuel, Gratton, Raffaele, Guerra, Jose, Harutyunyan, Avet, Hernandez, Nauzet, Iuzzolino, Marcella, Lodi, Marcello, Malavolta, Luca, Maldonado, Jesus, Micela, Giusi, Sanna, Nicoletta, Sanjuan, Jose, Scuderi, Salvo, Sozzetti, Alessandro, Ventura, Hector Perez, Diaz, Marcos Hernandez, Galli, Alberto, Gonzalez, Carlos, Riverol, Luis, and Riverol, Carlos

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

GIARPS (GIAno & haRPS) is a project devoted to have on the same focal station of the Telescopio Nazionale Galileo (TNG) both the high resolution spectrographs HARPS-N (VIS) and GIANO (NIR) working simultaneously. This could be considered the first and unique worldwide instrument providing cross-dispersed echelle spectroscopy at a high resolution (R=115,000 in the visual and R=50,000 in the IR) and over in a wide spectral range (0.383 - 2.45 micron) in a single exposure. The science case is very broad, given the versatility of such an instrument and the large wavelength range. A number of outstanding science cases encompassing mainly extra-solar planet science starting from rocky planet search and hot Jupiters, atmosphere characterization can be considered. Furthermore both instrument can measure high precision radial velocity by means the simultaneous thorium technique (HARPS - N) and absorbing cell technique (GIANO) in a single exposure. Other science cases are also possible. Young stars and proto-planetary disks, cool stars and stellar populations, moving minor bodies in the solar system, bursting young stellar objects, cataclysmic variables and X-ray binary transients in our Galaxy, supernovae up to gamma-ray bursts in the very distant and young Universe, can take advantage of the unicity of this facility both in terms of contemporaneous wide wavelength range and high resolution spectroscopy., Comment: 8 pages, 5 figures, SPIE Conference Proceedings

Published
2016
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5. HARPS-N observes the Sun as a star

Author

Dumusque, Xavier, Glenday, Alex, Phillips, David F., Buchschacher, Nicolas, Cameron, Andrew Collier, Cecconi, Massimo, Charbonneau, David, Cosentino, Rosario, Ghedina, Adriano, Latham, David W., Li, Chih-Hao, Lodi, Marcello, Lovis, Christophe, Molinari, Emilio, Pepe, Francesco, Udry, Stephane, Sasselov, Dimitar, Szentgyorgyi, Andrew, and Walsworth, Ronald

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

Radial velocity perturbations induced by stellar surface inhomogeneities including spots, plages and granules currently limit the detection of Earth-twins using Doppler spectroscopy. Such stellar noise is poorly understood for stars other than the Sun because their surface is unresolved. In particular, the effects of stellar surface inhomogeneities on observed stellar radial velocities are extremely difficult to characterize, and thus developing optimal correction techniques to extract true stellar radial velocities is extremely challenging. In this paper, we present preliminary results of a solar telescope built to feed full-disk sunlight into the HARPS-N spectrograph, which is in turn calibrated with an astro-comb. This setup enables long-term observation of the Sun as a star with state-of-the-art sensitivity to radial velocity changes. Over seven days of observing in 2014, we show an average 50\cms radial velocity rms over a few hours of observation. After correcting observed radial velocities for spot and plage perturbations using full-disk photometry of the Sun, we lower by a factor of two the weekly radial velocity rms to 60\cms. The solar telescope is now entering routine operation, and will observe the Sun every clear day for several hours. We will use these radial velocities combined with data from solar satellites to improve our understanding of stellar noise and develop optimal correction methods. If successful, these new methods should enable the detection of Venus over the next two to three years, thus demonstrating the possibility of detecting Earth-twins around other solar-like stars using the radial velocity technique., Comment: 8 pages, 5 figures, accepted to ApJ Letters

Published
2015
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6. Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

Author

Dalton, Gavin, Trager, Scott, Abrams, Don Carlos, Bonifacio, Piercarlo, Aguerri, J. Alfonso L., Middleton, Kevin, Benn, Chris, Dee, Kevin, Sayede, Frederic, Lewis, Ian, Pragt, Johannes, Pico, Sergio, Walton, Nic, Rey, Juerg, Prieto, Carlos Allende, Penate, Jose, Lhome, Emilie, Agocs, Tibor, Alonso, Jose, Terrett, David, Brock, Matthew, Gilbert, James, Ridings, Andy, Guinouard, Isabelle, Verheijen, Marc, Tosh, Ian, Rogers, Kevin, Steele, Iain, Stuik, Remko, Tromp, Neils, Jasko, Attila, Kragt, Jan, Lesman, Dirk, Mottram, Chris, Bates, Stuart, Gribbin, Frank, Rodriguez, Luis Fernando, Delgado, Jose Miguel, Martin, Carlos, Cano, Diego, Navarro, Ramon, Irwin, Mike, Lewis, Jim, Solares, Eduardo Gonzales, Mahony, Neil O, Bianco, Andrea, Zurita, Christina, ter Horst, Rik, Molinari, Emilio, Lodi, Marcello, Guerra, Jose, Vallenari, Antonella, and Baruffolo, Andrea

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We present an overview of and status report on the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT). WEAVE principally targets optical ground-based follow up of upcoming ground-based (LOFAR) and space-based (Gaia) surveys. WEAVE is a multi-object and multi-IFU facility utilizing a new 2-degree prime focus field of view at the WHT, with a buffered pick-and-place positioner system hosting 1000 multi-object (MOS) fibres, 20 integral field units, or a single large IFU for each observation. The fibres are fed to a single spectrograph, with a pair of 8k(spectral) x 6k (spatial) pixel cameras, located within the WHT GHRIL enclosure on the telescope Nasmyth platform, supporting observations at R~5000 over the full 370-1000nm wavelength range in a single exposure, or a high resolution mode with limited coverage in each arm at R~20000. The project is now in the final design and early procurement phase, with commissioning at the telescope expected in 2017., Comment: 11 pages, 11 Figures, Summary of a presentation to Astronomical Telescopes and Instrumentation 2014

Published
2014
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7. DAS: a data management system for instrument tests and operations

Author

Frailis, Marco, Sartor, Stefano, Zacchei, Andrea, Lodi, Marcello, Cirami, Roberto, Pasian, Fabio, Trifoglio, Massimo, Bulgarelli, Andrea, Gianotti, Fulvio, Franceschi, Enrico, Nicastro, Luciano, Conforti, Vito, Zoli, Andrea, Smart, Ricky, Morbidelli, Roberto, and Dadina, Mauro

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Computer Science - Databases
Abstract

The Data Access System (DAS) is a metadata and data management software system, providing a reusable solution for the storage of data acquired both from telescopes and auxiliary data sources during the instrument development phases and operations. It is part of the Customizable Instrument WorkStation system (CIWS-FW), a framework for the storage, processing and quick-look at the data acquired from scientific instruments. The DAS provides a data access layer mainly targeted to software applications: quick-look displays, pre-processing pipelines and scientific workflows. It is logically organized in three main components: an intuitive and compact Data Definition Language (DAS DDL) in XML format, aimed for user-defined data types; an Application Programming Interface (DAS API), automatically adding classes and methods supporting the DDL data types, and providing an object-oriented query language; a data management component, which maps the metadata of the DDL data types in a relational Data Base Management System (DBMS), and stores the data in a shared (network) file system. With the DAS DDL, developers define the data model for a particular project, specifying for each data type the metadata attributes, the data format and layout (if applicable), and named references to related or aggregated data types. Together with the DDL user-defined data types, the DAS API acts as the only interface to store, query and retrieve the metadata and data in the DAS system, providing both an abstract interface and a data model specific one in C, C++ and Python. The mapping of metadata in the back-end database is automatic and supports several relational DBMSs, including MySQL, Oracle and PostgreSQL., Comment: Accepted for pubblication on ADASS Conference Series

Published
2014

8. CIWS-FW: a Customizable InstrumentWorkstation Software Framework for instrument-independent data handling

Author

Conforti, Vito, Trifoglio, Massimo, Bulgarelli, Andrea, Gianotti, Fulvio, Franceschi, Enrico, Nicastro, Luciano, Zoli, Andrea, Dadina, Mauro, Smart, Ricky, Morbidelli, Roberto, Frailis, Marco, Sartor, Stefano, Zacchei, Andrea, Lodi, Marcello, Cirami, Roberto, and Pasian, Fabio

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The CIWS-FW is aimed at providing a common and standard solution for the storage, processing and quick look at the data acquired from scientific instruments for astrophysics. The target system is the instrument workstation either in the context of the Electrical Ground Support Equipment for space-borne experiments, or in the context of the data acquisition system for instrumentation. The CIWS-FW core includes software developed by team members for previous experiments and provides new components and tools that improve the software reusability, configurability and extensibility attributes. The CIWS-FW mainly consists of two packages: the data processing system and the data access system. The former provides the software components and libraries to support the data acquisition, transformation, display and storage in near real time of either a data packet stream and/or a sequence of data files generated by the instrument. The latter is a meta-data and data management system, providing a reusable solution for the archiving and retrieval of the acquired data. A built-in operator GUI allows to control and configure the IW. In addition, the framework provides mechanisms for system error and logging handling. A web portal provides the access to the CIWS-FW documentation, software repository and bug tracking tools for CIWS-FW developers. We will describe the CIWS-FW architecture and summarize the project status., Comment: Accepted for pubblication on ADASS Conference Series

Published
2014

9. The magnetically quiet solar surface dominates HARPS-N solar RVs during low activity.

Author

Lakeland, Ben S, Naylor, Tim, Haywood, Raphaëlle D, Meunier, Nadège, Rescigno, Federica, Dalal, Shweta, Mortier, Annelies, Thompson, Samantha J, Cameron, Andrew Collier, Dumusque, Xavier, López-Morales, Mercedes, Pepe, Francesco, Rice, Ken, Sozzetti, Alessandro, Udry, Stéphane, Ford, Eric, Ghedina, Adriano, and Lodi, Marcello

Subjects
SOLAR surface, SOLAR oscillations, SOLAR cycle, HELIOSEISMOLOGY, SOLAR granulation
Abstract

Using images from the Helioseismic and Magnetic Imager aboard the Solar Dynamics Observatory , we extract the radial velocity (RV) signal arising from the suppression of convective blueshift and from bright faculae and dark sunspots transiting the rotating solar disc. We remove these rotationally modulated magnetic-activity contributions from simultaneous RVs observed by the HARPS-N (High Accuracy Radial velocity Planet Searcher for the Northern hemisphere) solar feed to produce an RV time series arising from the magnetically quiet solar surface (the 'inactive-region RVs'). We find that the level of variability in the inactive-region RVs remains constant over the almost 7-yr baseline and shows no correlation with well-known activity indicators. With an root-mean-square scatter of roughly 1 |${\rm m\, s}^{-1}$|⁠ , the inactive-region RV time series dominates the total RV variability budget during the decline of solar cycle 24. Finally, we compare the variability amplitude and time-scale of the inactive-region RVs with simulations of supergranulation. We find consistency between the inactive-region RV and simulated time series, indicating that supergranulation is a significant contribution to the overall solar RV variability, and may be the main source of variability towards solar minimum. This work highlights supergranulation as a key barrier to detecting Earth twins. [ABSTRACT FROM AUTHOR]

Published
2024
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10. The Extreme Stellar-signals Project. III. Combining Solar Data from HARPS, HARPS-N, EXPRES, and NEID

Author

Zhao, Lily L., primary, Dumusque, Xavier, additional, Ford, Eric B., additional, Llama, Joe, additional, Mortier, Annelies, additional, Bedell, Megan, additional, Al Moulla, Khaled, additional, Bender, Chad F., additional, Blake, Cullen H., additional, Brewer, John M., additional, Collier Cameron, Andrew, additional, Cosentino, Rosario, additional, Figueira, Pedro, additional, Fischer, Debra A., additional, Ghedina, Adriano, additional, Gonzalez, Manuel, additional, Halverson, Samuel, additional, Kanodia, Shubham, additional, Latham, David W., additional, Lin, Andrea S. J., additional, Lo Curto, Gaspare, additional, Lodi, Marcello, additional, Logsdon, Sarah E., additional, Lovis, Christophe, additional, Mahadevan, Suvrath, additional, Monson, Andrew, additional, Ninan, Joe P., additional, Pepe, Francesco, additional, Roettenbacher, Rachael M., additional, Roy, Arpita, additional, Santos, Nuno C., additional, Schwab, Christian, additional, Stefánsson, Guđmundur, additional, Szymkowiak, Andrew E., additional, Terrien, Ryan C., additional, Udry, Stephane, additional, Weiss, Sam A., additional, Wildi, François, additional, Wildi, Thibault, additional, and Wright, Jason T., additional

Published
2023
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11. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Author

Jin, Shoko, primary, Trager, Scott C, additional, Dalton, Gavin B, additional, Aguerri, J Alfonso L, additional, Drew, J E, additional, Falcón-Barroso, Jesús, additional, Gänsicke, Boris T, additional, Hill, Vanessa, additional, Iovino, Angela, additional, Pieri, Matthew M, additional, Poggianti, Bianca M, additional, Smith, D J B, additional, Vallenari, Antonella, additional, Abrams, Don Carlos, additional, Aguado, David S, additional, Antoja, Teresa, additional, Aragón-Salamanca, Alfonso, additional, Ascasibar, Yago, additional, Babusiaux, Carine, additional, Balcells, Marc, additional, Barrena, R, additional, Battaglia, Giuseppina, additional, Belokurov, Vasily, additional, Bensby, Thomas, additional, Bonifacio, Piercarlo, additional, Bragaglia, Angela, additional, Carrasco, Esperanza, additional, Carrera, Ricardo, additional, Cornwell, Daniel J, additional, Domínguez-Palmero, Lilian, additional, Duncan, Kenneth J, additional, Famaey, Benoit, additional, Fari na, Cecilia, additional, Gonzalez, Oscar A, additional, Guest, Steve, additional, Hatch, Nina A, additional, Hess, Kelley M, additional, Hoskin, Matthew J, additional, Irwin, Mike, additional, Knapen, Johan H, additional, Koposov, Sergey E, additional, Kuchner, Ulrike, additional, Laigle, Clotilde, additional, Lewis, Jim, additional, Longhetti, Marcella, additional, Lucatello, Sara, additional, Méndez-Abreu, Jairo, additional, Mercurio, Amata, additional, Molaeinezhad, Alireza, additional, Monguió, Maria, additional, Morrison, Sean, additional, Murphy, David N A, additional, de Arriba, Luis Peralta, additional, Pérez, Isabel, additional, Pérez-Ràfols, Ignasi, additional, Picó, Sergio, additional, Raddi, Roberto, additional, Romero-Gómez, Mercè, additional, Royer, Frédéric, additional, Siebert, Arnaud, additional, Seabroke, George M, additional, Som, Debopam, additional, Terrett, David, additional, Thomas, Guillaume, additional, Wesson, Roger, additional, Worley, C Clare, additional, Alfaro, Emilio J, additional, Prieto, Carlos Allende, additional, Alonso-Santiago, Javier, additional, Amos, Nicholas J, additional, Ashley, Richard P, additional, Balaguer-Nú nez, Lola, additional, Balbinot, Eduardo, additional, Bellazzini, Michele, additional, Benn, Chris R, additional, Berlanas, Sara R, additional, Bernard, Edouard J, additional, Best, Philip, additional, Bettoni, Daniela, additional, Bianco, Andrea, additional, Bishop, Georgia, additional, Blomqvist, Michael, additional, Boeche, Corrado, additional, Bolzonella, Micol, additional, Bonoli, Silvia, additional, Bosma, Albert, additional, Britavskiy, Nikolay, additional, Busarello, Gianni, additional, Caffau, Elisabetta, additional, Cantat-Gaudin, Tristan, additional, Castro-Ginard, Alfred, additional, Couto, Guilherme, additional, Carbajo-Hijarrubia, Juan, additional, Carter, David, additional, Casamiquela, Laia, additional, Conrado, Ana M, additional, Corcho-Caballero, Pablo, additional, Costantin, Luca, additional, Deason, Alis, additional, de Burgos, Abel, additional, De Grandi, Sabrina, additional, Di Matteo, Paola, additional, Domínguez-Gómez, Jesús, additional, Dorda, Ricardo, additional, Drake, Alyssa, additional, Dutta, Rajeshwari, additional, Erkal, Denis, additional, Feltzing, Sofia, additional, Ferré-Mateu, Anna, additional, Feuillet, Diane, additional, Figueras, Francesca, additional, Fossati, Matteo, additional, Franciosini, Elena, additional, Frasca, Antonio, additional, Fumagalli, Michele, additional, Gallazzi, Anna, additional, García-Benito, Rubén, additional, Fusillo, Nicola Gentile, additional, Gebran, Marwan, additional, Gilbert, James, additional, Gledhill, T M, additional, Delgado, Rosa M González, additional, Greimel, Robert, additional, Guarcello, Mario Giuseppe, additional, Guerra, Jose, additional, Gullieuszik, Marco, additional, Haines, Christopher P, additional, Hardcastle, Martin J, additional, Harris, Amy, additional, Haywood, Misha, additional, Helmi, Amina, additional, Hernandez, Nauzet, additional, Herrero, Artemio, additional, Hughes, Sarah, additional, Irsic, Vid, additional, Jablonka, Pascale, additional, Jarvis, Matt J, additional, Jordi, Carme, additional, Kondapally, Rohit, additional, Kordopatis, Georges, additional, Krogager, Jens-Kristian, additional, Barbera, Francesco La, additional, Lam, Man I, additional, Larsen, Søren S, additional, Lemasle, Bertrand, additional, Lewis, Ian J, additional, Lhomé, Emilie, additional, Lind, Karin, additional, Lodi, Marcello, additional, Longobardi, Alessia, additional, Lonoce, Ilaria, additional, Magrini, Laura, additional, Apellániz, Jesús Maíz, additional, Marchal, Olivier, additional, Marco, Amparo, additional, Martin, Nicolas F, additional, Matsuno, Tadafumi, additional, Maurogordato, Sophie, additional, Merluzzi, Paola, additional, Miralda-Escudé, Jordi, additional, Molinari, Emilio, additional, Monari, Giacomo, additional, Morelli, Lorenzo, additional, Mottram, Christopher J, additional, Naylor, Tim, additional, Negueruela, Ignacio, additional, Onorbe, Jose, additional, Pancino, Elena, additional, Peirani, Sébastien, additional, Peletier, Reynier F, additional, Pozzetti, Lucia, additional, Rainer, Monica, additional, Ramos, Pau, additional, Read, Shaun C, additional, Rossi, Elena Maria, additional, Röttgering, Huub J A, additional, Rubi no-Martín, Jose Alberto, additional, Montes, Jose Sabater, additional, Juan, José San, additional, Sanna, Nicoletta, additional, Schallig, Ellen, additional, Schiavon, Ricardo P, additional, Schultheis, Mathias, additional, Serra, Paolo, additional, Shimwell, Timothy W, additional, Simón-Díaz, Sergio, additional, Smith, Russell J, additional, Sordo, Rosanna, additional, Sorini, Daniele, additional, Soubiran, Caroline, additional, Starkenburg, Else, additional, Steele, Iain A, additional, Stott, John, additional, Stuik, Remko, additional, Tolstoy, Eline, additional, Tortora, Crescenzo, additional, Tsantaki, Maria, additional, Van der Swaelmen, Mathieu, additional, van Weeren, Reinout J, additional, Vergani, Daniela, additional, Verheijen, Marc A W, additional, Verro, Kristiina, additional, Vink, Jorick S, additional, Vioque, Miguel, additional, Walcher, C Jakob, additional, Walton, Nicholas A, additional, Wegg, Christopher, additional, Weijmans, Anne-Marie, additional, Williams, Wendy L, additional, Wilson, Andrew J, additional, Wright, Nicholas J, additional, Xylakis-Dornbusch, Theodora, additional, Youakim, Kris, additional, Zibetti, Stefano, additional, and Zurita, Cristina, additional

Published
2023
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13. SiFAP4XP : time domain polarimetry with silicon photometers at the TNG

Author

Ghedina, Adriano, primary, Ambrosino, Filippo, additional, Cecconi, Massimo, additional, Gonzalez, Manuel D., additional, Riverol, Luis, additional, Hernandez Díaz, Marcos, additional, Pérez Ventura, Héctor, additional, San Juan, José Juan, additional, Guerra, Jose, additional, Lodi, Marcello, additional, Hernandez, Nauzet, additional, De Benedetto, Marco, additional, Papitto, Alessandro, additional, Leone, Francesco, additional, Meddi, Franco, additional, and Poretti, Ennio, additional

Published
2022
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14. ASTRI Mini-Array on-site Information and Communication Technology infrastructure

Author

Gianotti, Fulvio, primary, Lodi, Marcello, additional, Conforti, Vito, additional, Tacchini, Alessandro, additional, Bulgarelli, Andrea A., additional, Bruno, Pietro Giuseppe, additional, Costa, Alessandro, additional, De Rosa, Adriano, additional, Gallozzi, Stefano, additional, Germani, Stefano, additional, Incardona, Federico, additional, Leto, Giuseppe, additional, Lucarelli, Fabrizio, additional, Malaspina, Giuseppe, additional, Munari, Kevin, additional, Parmiggiani, Nicolò, additional, Pastore, Valerio, additional, Russo, Federico, additional, Scuderi, Salvo, additional, and Tosti, Gino, additional

Published
2022
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15. GIANO: An Ultra-Stable IR Echelle Spectrometer for the TNG Telescope

Author

Oliva, Ernesto, Origlia, Livia, Maiolino, Roberto, Gennari, Sandro, Biliotti, Valdemaro, Rossetti, Emanuel, Baffa, Carlo, Leone, Franco, Montegriffo, Paolo, Lolli, Marco, D’Amato, Francesco, Bruno, Pietro, Scuderi, Salvatore, Ghinassi, Francesca, Gonzalez, Manuel, Lodi, Marcello, Falcini, Gilberto, Giani, Elisabetha, Marcucci, Gianni, Sozzi, Mauro, Käufl, Hans Ulrich, editor, Siebenmorgen, Ralf, editor, and Moorwood, Alan F. M., editor

Published
2005
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16. Five carbon- and nitrogen-bearing species in a hot giant planet’s atmosphere

Author

Giacobbe, Paolo, primary, Brogi, Matteo, additional, Gandhi, Siddharth, additional, Cubillos, Patricio E., additional, Bonomo, Aldo S., additional, Sozzetti, Alessandro, additional, Fossati, Luca, additional, Guilluy, Gloria, additional, Carleo, Ilaria, additional, Rainer, Monica, additional, Harutyunyan, Avet, additional, Borsa, Francesco, additional, Pino, Lorenzo, additional, Nascimbeni, Valerio, additional, Benatti, Serena, additional, Biazzo, Katia, additional, Bignamini, Andrea, additional, Chubb, Katy L., additional, Claudi, Riccardo, additional, Cosentino, Rosario, additional, Covino, Elvira, additional, Damasso, Mario, additional, Desidera, Silvano, additional, Fiorenzano, Aldo F. M., additional, Ghedina, Adriano, additional, Lanza, Antonino F., additional, Leto, Giuseppe, additional, Maggio, Antonio, additional, Malavolta, Luca, additional, Maldonado, Jesus, additional, Micela, Giuseppina, additional, Molinari, Emilio, additional, Pagano, Isabella, additional, Pedani, Marco, additional, Piotto, Giampaolo, additional, Poretti, Ennio, additional, Scandariato, Gaetano, additional, Yurchenko, Sergei N., additional, Fantinel, Daniela, additional, Galli, Alberto, additional, Lodi, Marcello, additional, Sanna, Nicoletta, additional, and Tozzi, Andrea, additional

Published
2021
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17. Integration and early testing of WEAVE: the next-generation spectroscopy facility for the William Herschel Telescope

Author

Dalton, Gavin, primary, Trager, Scott C., additional, Abrams, Don Carlos, additional, Bonifacio, Piercarlo, additional, Aguerri, Alfonso, additional, Vallenari, Antonella, additional, Bishop, Georgia, additional, Middleton, Kevin, additional, Benn, Chris, additional, Dee, Kevin, additional, Mignot, Shan, additional, Lewis, Ian J., additional, Pragt, Johannes, additional, Pico, Sergio, additional, Walton, Nicholas, additional, Rey, Juerg, additional, Allende, Carlos, additional, Lhomé, Emilie, additional, Balcells, Marc, additional, Terrett, David, additional, Brock, Matthew, additional, Ridings, Andy, additional, Skvarč, Jure, additional, Verheijen, Marc, additional, Steele, Iain, additional, Stuik, Remko, additional, Kroes, Gabby, additional, Tromp, Neils, additional, Kragt, Jan, additional, Lesman, Dirk, additional, Mottram, Chris, additional, Bates, Stuart, additional, Gribbin, Frank, additional, Burgal, Jose Alonso, additional, Herreros, José Miguel, additional, Delgado, José Miguel, additional, Martin, Carlos, additional, Cano, Diego, additional, Navarro, Ramon, additional, Irwin, Mike J., additional, Peralta, Luis, additional, O'Mahoney, Neil, additional, Bianco, Andrea, additional, Moleinezhad, Alireza, additional, ter Horst, Rik, additional, Molinari, Emilio, additional, Lodi, Marcello, additional, Guerra, José, additional, Baruffalo, Andrea, additional, Carrasco, Esperanza, additional, Farcas, Szigfrid, additional, Schallig, Ellen, additional, Hughes, Sarah, additional, Hill, Vanessa, additional, Smith, Dan J., additional, Drew, Janet, additional, Poggianti, Bianca, additional, Iovino, Angela, additional, Pieri, Mat, additional, Jin, Shoko, additional, Dominguez, Lillian, additional, Farina, Cecilia, additional, Martin, Adrian, additional, Worley, Clare, additional, Murphy, David, additional, Guest, Steve, additional, Morris, Huw, additional, Elswijk, Eddy, additional, de Haan, Menno, additional, Hanenburg, Hiddo, additional, Salasnich, Bernardo, additional, Mayya, Divakara, additional, Izazaga-Perez, Rafael, additional, Gafton, Emanuel, additional, Caffau, Elisabetta, additional, Horville, David, additional, Paz Chinchon, Francisco, additional, Falcon-Barosso, Jesus, additional, Gänsicke, Boris, additional, San Juan, Jose, additional, and Hernandez, Nauzet, additional

Published
2020
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18. LOCNES: A solar telescope to study the Sun-as-a-star activity in the near infrared

Author

Claudi, Riccardo U., primary, Ghedina, Adriano, additional, Pace, Emanuele, additional, Di Giorgio, Anna Maria, additional, D'Orazi, Valentina, additional, Gallorini, Lorenzo, additional, Lanza, Antonino F., additional, Liù, Scigè J., additional, Rainer, Monica, additional, Tozzi, Andrea, additional, Carleo, Ilaria, additional, Maldonado Prado, Jesus, additional, Micela, Giuseppina, additional, Molinari, Emilio, additional, Poretti, Ennio, additional, Phillips, David, additional, Tripodo, G., additional, Cecconi, Massimo, additional, Galli, Alberto, additional, Gonzalez, Manuel, additional, Guerra Padilla, V., additional, Guerra, Jose, additional, Harutyunyan, Avet, additional, Hernandez, Nauzet, additional, Hernandez Diaz, Marcos, additional, Lodi, Marcello, additional, Pérez Ventura, Héctor, additional, Riverol, Luis, additional, Riverol, Carlos, additional, and San Juan Gómez, José J., additional

Published
2020
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19. Telescopio Nazionale Galileo control system upgrade, new milestone achieved: azimuth axis completed

Author

Gonzalez, Manuel, primary, Pérez Ventura, Héctor, additional, Hernandez Diaz, Marcos, additional, Schipani, Pietro, additional, Ghedina, Adriano, additional, San Juan Gómez, José J., additional, Hernandez, Nauzet, additional, Guerra, Jose, additional, Lodi, Marcello, additional, Riverol Rodríguez, Angel Luis, additional, Riverol, Carlos, additional, Gonzalez, Carlos, additional, Galli, Alberto, additional, Colapietro, Mirko, additional, and Savarese, Salvatore, additional

Published
2020
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20. Importância do acompanhamento da doença granulomatosa crônica / Importance of monitoring chronic granulomatous disease

Author

Leão, João Marcos de Castro Possato, Lodi, Marcello Melaragno, Libera, Pedro Henrique Della, Leite, Luiz Fernando Bacarini, Mosca, Tainá, and Forte, Wilma Carvalho Neves

Abstract

A Doença Granulomatosa Crônica (DGC) é uma Imunodeficiência Primária (IDP) em que há disfunção no processo de digestão por fagócitos, causando maior suscetibilidade a infecções por microrganismos catalase-positivos, em especial Staphylococcus aureus, o que leva a abscessos de repetição e necessidade de antibiótico profilático. Apresentamos caso de criança com abscessos de repetição desde os três meses de idade. Aos dois anos foi encaminhada a Setor especializado em IDPs, onde foi feito o diagnóstico de DGC. Passou a receber antibiótico profilático e não apresentou infecções nos dois anos subsequentes. A famí­lia abandonou o acompanhamento quando o paciente tinha quatro anos, procurando profissional próximo í residência. Foi suspenso o antibiótico, recebendo apenas em iní­cio de infecções e passou bem nos quatros anos seguintes. Aos oito anos, novamente procurou o Setor, apresentando abscessos em arco costal e coluna vertebral, além de osteomielite. Após quatro meses de internação, houve regressão do quadro infeccioso, mas restaram sequelas graves e dificuldade de locomoção, levando í necessidade de cadeira de rodas. Ressaltamos que a DGC deve ser lembrada por profissionais da saúde para que possa ser feito o diagnóstico precoce e o devido acompanhamento, permitindo uma melhor qualidade de vida ao paciente.Descritores: Doença granulomatosa crônica, Sí­ndromes de imunodeficiência, Nitroazul de tetrazólio, Antibioticoprofilaxia, Abscesso, Recidiva, Fagocitose

Published
2018

21. Construction progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

Author

Benn, Chris, primary, Dee, Kevin, primary, Sayède, Frédéric N., primary, Lewis, Ian J., primary, Pragt, Johan, primary, Picó, Sergio, primary, Walton, Nicholas A., primary, Rey, Jeurg, primary, Allende Prieto, Carlos, primary, Lhomé, Émilie, primary, Terrett, David, primary, Brock, Matthew, primary, Gilbert, James, primary, Ridings, Andy, primary, Verheijen, Marc, primary, Tosh, Ian, primary, Steele, Iain A., primary, Stuik, Remko, primary, Kroes, Gabby, primary, Burgal, José Alonso, primary, Tromp, Neils, primary, Kragt, Jan, primary, Lesman, Dirk, primary, Mottram, Chris, primary, Bates, Stuart, primary, Gribbin, Frank, primary, Mayya, Divakara, primary, Dalton, Gavin B., primary, Trager, Scott C., primary, Abrams, Don Carlos, primary, Aguerri, Jose Alfonso, primary, Bonifacio, Piercarlo, primary, Vallenari, Antonella, primary, Carrasco Licea, Esperanza E., primary, Middleton, Kevin, primary, Jin, Shoko, primary, Herreros, José Miguel, primary, Delgado, Jose Miguel, primary, Martin, Carlos, primary, Cano Infantes, Diego, primary, Navarro, Ramón, primary, Irwin, Mike J., primary, Lewis, James, primary, Gonzales, Eduardo, primary, O'Mahony, Neil, primary, Bianco, Andrea, primary, Zurita, Christina, primary, ter Horst, Rik, primary, Molinari, Emilio, primary, Lodi, Marcello, primary, Guerra, Jose, primary, Baruffolo, Andrea, primary, Salasnich, Bernardo, primary, Farkas, Szigfrid, primary, Schallig, Ellen, primary, Hill, Vanessa, primary, Smith, Dan, primary, Drew, Janet, primary, Poggianti, Bianca, primary, Pieri, Matthew, primary, Domínquez, Lilian, primary, Fariña, Cecilia, primary, Martin, Adrian, primary, Worley, Clare, primary, Murphy, David, primary, Hidalgo, Andrea, primary, Mignot, Shan B., primary, Bishop, Georgia, primary, Guest, Steve, primary, Elswijk, Eddy, primary, de Haan, Menno, primary, Hanenburg, Hiddo, primary, Izazaga-Pérez, Rafael, primary, and Peralta de Arriba, Luis, primary

Published
2018
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22. GIANO-B online data reduction software at the TNG

Author

Harutyunyan, Avet, primary, Rainer, Monica, primary, Hernandez, Nauzet, primary, Oliva, Ernesto, primary, Guerra, Jose, primary, Lodi, Marcello, primary, San Juan Gómez, José, primary, Bignamini, Andrea, primary, Ghedina, Adriano, primary, Ghinassi Luschi, Francesca, primary, Molinari, Emilio, primary, Benatti, Serena, primary, Carleo, Ilaria, primary, Claudi, Riccardo U., primary, Micela, Giuseppina, primary, Tozzi, Andrea, primary, Baffa, Carlo, primary, Baruffolo, Andrea, primary, Biliotti, Valdemaro, primary, Buchschacher, Nicolas, primary, Cecconi, Massimo, primary, Cosentino, Rosario, primary, Falcini, Gilberto, primary, Fantinel, Daniela, primary, Fini, Luca, primary, Galli, Alberto, primary, Giani, Elisabetta, primary, Gonzalez, Carlos, primary, Gonzalez-Alvarez, Esther, primary, Gonzalez, Manuel, primary, Gratton, Raffaele, primary, Hernandez Diaz, Marcos, primary, Iuzzolino, Marcella, primary, Malavolta, Luca, primary, Maldonado, Jesus, primary, Origlia, Livia, primary, Poretti, Ennio, primary, Perez Ventura, Hector, primary, Puglisi, Alfio, primary, Riverol, Carlos, primary, Riverol, Luis, primary, Sanna, Nicoletta, primary, Scuderi, Salvatore, primary, Seeman, Ulf, primary, Sozzetti, Alessandro, primary, and Sozzi, Mauro, primary

Published
2018
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23. Introducing GOFIO: a DRS for the GIANO-B near-infrared spectrograph

Author

Harutyunyan, Avet, primary, Carleo, Ilaria, primary, Oliva, Ernesto, primary, Benatti, Serena, primary, Micela, Giuseppina, primary, Ghinassi Luschi, Francesca, primary, Iuzzolino, Marcella, primary, Lodi, Marcello, primary, Malavolta, Luca, primary, Maldonado, Jesus, primary, Origlia, Livia, primary, Puglisi, Alfio, primary, San Juan Gómez, José, primary, Scuderi, Salvatore, primary, Seeman, Ulf, primary, Sozzetti, Alessandro, primary, Sozzi, Mauro, primary, Pérez Ventura, Héctor, primary, Hernandez Diaz, Marcos, primary, Galli, Alberto, primary, Gonzalez, Carlos, primary, Riverol, Luis, primary, Riverol, Carlos, primary, Rainer, Monica, primary, Bignamini, Andrea, primary, Claudi, Riccardo U., primary, Gonzalez-Alvarez, Esther, primary, Sanna, Nicoletta, primary, Ghedina, Adriano, primary, Molinari, Emilio, primary, Tozzi, Andrea, primary, Baffa, Carlo, primary, Baruffolo, Andrea, primary, Buchschacher, Nicolas, primary, Cecconi, Massimo, primary, Cosentino, Rosario, primary, Falcini, Gilberto, primary, Fantinel, Daniela, primary, Fini, Luca, primary, Giani, Elisabetta, primary, Gonzalez, Manuel, primary, Guerra, Jose, primary, Hernandez, Nauzet, primary, and Gratton, Raffaele, primary

Published
2018
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24. GIARPS: commissioning and first scientific results

Author

Claudi, Riccardo U., primary, Benatti, Serena, primary, Carleo, Ilaria, primary, Ghedina, Adriano, primary, Guerra, Jose, primary, Ghinassi Luschi, Francesca, primary, Harutyunyan, Avet, primary, Micela, Giuseppina, primary, Molinari, Emilio, primary, Oliva, Ernesto, primary, Rainer, Monica, primary, Tozzi, Andrea, primary, Baffa, Carlo, primary, Baruffolo, Andrea, primary, Buchschacher, Nicolas, primary, Cecconi, Massimo, primary, Cosentino, Rosario, primary, Falcini, Gilberto, primary, Fantinel, Daniela, primary, Fini, Luca, primary, Giani, Elisabetta, primary, Gonzalez-Alvarez, Esther, primary, Gonzalez, Manuel, primary, Gratton, Raffaele, primary, Hernandez, Nauzet, primary, Iuzzolino, Marcella, primary, Lodi, Marcello, primary, Malavolta, Luca, primary, Maldonado, Jesus, primary, Origlia, Livia, primary, Puglisi, Alfio, primary, Sanna, Nicoletta, primary, San Juan Gómez, José, primary, Scuderi, Salvatore, primary, Seemann, Ulf, primary, Sozzetti, Alessandro, primary, Sozzi, Mauro, primary, Pérez Ventura, Héctor, primary, Hernandez Diaz, Marcos, primary, Galli, Alberto, primary, Gonzalez, Carlos, primary, Riverol, Luis, primary, Riverol, Carlos, primary, and Biliotti, V., primary

Published
2018
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25. Final design and progress of WEAVE

Author

Dalton, Gavin, Trager, Scott, Abrams, Don Carlos, Bonifacio, Piercarlo, Aguerri, J. Alfonso L., Middleton, Kevin, Benn, Chris, Dee, Kevin, Sayède, Frédéric, Lewis, Ian, Pragt, Johannes, Pico, Sergio, Walton, Nic, Rey, Jeurg, Allende Prieto, Carlos, Peñate, José, Lhome, Emilie, Agócs, Tibor, Alonso, José, Terrett, David, Brock, Matthew, Gilbert, James, Schallig, Ellen, Ridings, Andy, Guinouard, Isabelle, Verheijen, Marc, Tosh, Ian, Rogers, Kevin, Lee, Martin, Steele, Iain, Stuik, Remko, Tromp, Niels, Jaskó, Attila, Carrasco, Esperanza, Farcas, Szigfrid, Kragt, Jan, Lesman, Dirk, Kroes, Gabby, Mottram, Chris, Bates, Stuart, Rodriguez, Luis Fernando, Gribbin, Frank, Delgado, José Miguel, Herreros, José Miguel, Martin, Carlos, Cano, Diego, Navarro, Ramon, Irwin, Mike, Lewis, Jim, Gonzalez Solares, Eduardo, Murphy, David, Worley, Clare, Bassom, Richard, O'Mahoney, Neil, Bianco, Andrea, Zurita, Christina, ter Horst, Rik, Molinari, Emilio, Lodi, Marcello, Guerra, José, Martin, Adrian, Vallenari, Antonella, Salasnich, Bernardo, Baruffolo, Andrea, Jin, Shoko, Hill, Vanessa, Smith, Dan, Drew, Janet, Poggianti, Bianca, Pieri, Mat, Dominquez Palmero, Lillian, Farina, Cecilia, Evans, Christopher J, Simard, Luc, Takami, Hideki, Astronomy, STFC Rutherford Appleton Laboratory, Kapteyn Astronomical Institute, University of Groningen, Isaac Newton Group of Telescopes (Spain), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Physique stellaire et galactique, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Instituto de Astrofísica de Canarias (IAC), Univ. of Oxford (United Kingdom), Netherlands Institute for Radio Astronomy (ASTRON), Institute of Astronomy, Madingley Road, Liverpool John Moores University, Konkoly Observatory, Research Center for Astronomy and Earth Sciences, Instituto Nacional de Astrofísica Óptica y Electrónica (INAOE), Osservatorio Astronomico di Cagliari, Astrochemistry Group (INAF), INAF/TNG Fundación Galileo Galilei - Rambla José Ana Fernández Pérez, 7, Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), University of Hertfordshire [Hatfield] (UH), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), ITA, GBR, FRA, ESP, MEX, and NLD

Subjects
Physics, Pixel, business.industry, Field of view, First light, LOFAR, 01 natural sciences, law.invention, 010309 optics, Telescope, Optics, law, 0103 physical sciences, William Herschel Telescope, Aerospace engineering, business, Spectroscopy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, Spectrograph
Abstract

We present the Final Design of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), together with a status update on the details of manufacturing, integration and the overall project schedule now that all the major fabrication contracts are in place. We also present a summary of the current planning behind the 5-year initial phase of survey operations. WEAVE will provide optical ground-based follow up of ground-based (LOFAR) and space-based (Gaia) surveys. WEAVE is a multi-object and multi-IFU facility utilizing a new 2-degree prime focus field of view at the WHT, with a buffered pick-and-place positioner system hosting 1000 multi-object (MOS) fibres, 20 integral field units, or a single large IFU for each observation. The fibres are fed to a single (dual-beam) spectrograph, with total of 16k spectral pixels, located within the WHT GHRIL enclosure on the telescope Nasmyth platform, supporting observations at R~5000 over the full 370-1000nm wavelength range in a single exposure, or a high resolution mode with limited coverage in each arm at R~20000. The project is now in the manufacturing and integration phase with first light expected for early of 2018.

Published
2016

26. GIANO-B Online Data Reduction Software at the TNG.

Author

Harutyunyan, Avet, Rainer, Monica, Hernandez, Nauzet, Oliva, Ernesto, Guerra, Jose, Lodi, Marcello, Juan, Jose San, Bignamini, Andrea, Ghedina, Adriano, Ghinassi, Francesca, Molinari, Emilio, Benatti, Serena, Carleo, Ilaria, Claudi, Riccardo, Micela, Giuseppina, Tozzi, Andrea, Baffa, Carlo, Baruffolo, Andrea, Biliotti, Valdemaro, and Buchschacher, Nicolas

Published
2018
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27. CIWS-FW: a Customizable Instrument Workstation Software Framework for instrument-independent data handling

Author

CONFORTI, Vito, TRIFOGLIO, MASSIMO, BULGARELLI, ANDREA, GIANOTTI, FULVIO, FRANCESCHI, ENRICO, NICASTRO, LUCIANO, Zoli, Andrea, DADINA, MAURO, Smart, Ricky, MORBIDELLI, Roberto, Frailis , Marco, SARTOR, Stefano, ZACCHEI, Andrea, Lodi, Marcello, CIRAMI, ROBERTO, PASIAN, Fabio, and ITA

Abstract

The CIWS-FW is aimed at providing a common and standard solution for the storage, processing and quick look at the data acquired from scientific instruments for astrophysics. The target system is the instrument workstation either in the context of the Electrical Ground Support Equipment for space-borne experiments, or in the context of the data acquisition system for instrumentation. The CIWS-FW core includes software developed by team members for previous experiments and provides new components and tools that improve the software reusability, configurability and extensibility attributes. The CIWS-FW mainly consists of two packages: the data processing system and the data access system. The former provides the software components and libraries to support the data acquisition, transformation, display and storage in near real time of either a data packet stream and/or a sequence of data files generated by the instrument. The latter is a meta-data and data management system, providing a reusable solution for the archiving and retrieval of the acquired data. A built-in operator GUI allows to control and configure the IW. In addition, the framework provides mechanisms for system error and logging handling. A web portal provides the access to the CIWS-FW documentation, software repository and bug tracking tools for CIWS-FW developers. We will describe the CIWS-FW architecture and summarize the project status.

Published
2014

28. Relazione Scientifica del Progetto TECNO- INAF 2010 – CIWS (CRA 1.05.01.15.04)

Author

TRIFOGLIO, MASSIMO, BULGARELLI, ANDREA, CAPPI, MASSIMO, CONFORTI, Vito, DADINA, MAURO, FRANCESCHI, ENRICO, GIANOTTI, Fulvio, NICASTRO, FABRIZIO, Zoli, Andrea, MORBIDELLI, Roberto, SMART, Richard Laurence, CIRAMI, Roberto, DI MARCANTONIO, Paolo, FRAILIS, Marco, PASIAN, Fabio, SARTOR, Stefano, VUERLI, Claudio, ZACCHEI, Andrea, LODI, Marcello, ITA, and Trifoglio, Massimo

Abstract

Progetto TECNO- INAF 2010 – CIWS Il fiorire di progetti astronomici ed il contemporaneo sviluppo di strumentazione sempre piu' progredita ha, negli ultimi decenni, imposto lo sviluppo di tecniche di archiviazione e utilizzazione dei dati acquisiti sempre più complesse. Tale necessità ha avuto il costo di dirottare importanti risorse di intelligenza e tempo verso lo sviluppo di tecnologie atte a soddisfare queste esigenze. La lunga tempistica (tipicamente decennale) e il dislocamento spaziale dei centri di sviluppo dei programmi e della strumentazione astronomica, ha, fino ad oggi, reso complicato razionalizzare la fase del processo relativo alla creazione e fornitura di workstation scientifiche relative agli strumenti, nonostante le molteplici analogia fra tutti (o quasi) gli strumenti per l'astronomia. Partendo dalle premesse sopra presentate è nato il progetto CIWS (Customizable Instrument Workstation Software) che può permettere una notevole semplificazione per lo sviluppo di workstation scientifiche per i progetti futuri. Il CIWS, infatti, ha riguardato la progettazione e lo sviluppo di software per l’archiviazione e la visualizzazione on-line e off-line di dati acquisiti da strumentazione scientifica posta sia in telescopi di terra che a bordo e di telescopi spaziali. Lo scenario di riferimento è quello della Instrument Workstation che fornisce supporto al team di sviluppo dello strumento durante la fase di integrazione, verifica e calibrazione e al team operativo dell’Osservatorio o del Segmento di Terra, durante le successive fasi di collaudo e operativa. Come indicato nel nome, la configurabilità è la caratteristica fondamentale del progetto. A questa sono state dedicate molte risorse sia in fase di definizione dei requisiti e di progettazione sia in fase di realizzazione. Il framework ottenuto (CIWS-FW) consente allo sviluppatore di modellare molti aspetti caratteristici dello strumento mediante file di configurazione. Altre funzionalità specifiche richieste per il trattamento dei dati dello strumento possono essere realizzate dallo sviluppatore utilizzando moduli di base (templates) e librerie offerte dal CIWS-FW.

Published
2014

29. WAS: the data archive for the WEAVE spectrograph

Author

Guerra, Jose, additional, Molinari, Emilio, additional, Lodi, Marcello, additional, Martin, Adrian, additional, Dalton, Gavin B., additional, Trager, Scott C., additional, Jin, Shoko, additional, Abrams, Don Carlos, additional, Bonifacio, Piercarlo, additional, López Aguerri, Jose Alfonso, additional, Vallenari, Antonella, additional, Carrasco Licea, Esperanza E., additional, and Middleton, Kevin F., additional

Published
2016
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31. An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus

Author

Phillips, David F., additional, Glenday, Alex G., additional, Dumusque, Xavier, additional, Buchschacher, Nicolas, additional, Cameron, Andrew Collier, additional, Cecconi, Massimo, additional, Charbonneau, David, additional, Cosentino, Rosario, additional, Ghedina, Adriano, additional, Haywood, Raphäelle, additional, Latham, David W., additional, Li, Chih-Hao, additional, Lodi, Marcello, additional, Lovis, Christophe, additional, Molinari, Emilio, additional, Pepe, Francesco, additional, Sasselov, Dimitar, additional, Szentgyorgyi, Andrew, additional, Udry, Stephane, additional, and Walsworth, Ronald L., additional

Published
2016
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32. HARPS-N OBSERVES THE SUN AS A STAR

Author

Dumusque, Xavier, primary, Glenday, Alex, additional, Phillips, David F., additional, Buchschacher, Nicolas, additional, Cameron, Andrew Collier, additional, Cecconi, Massimo, additional, Charbonneau, David, additional, Cosentino, Rosario, additional, Ghedina, Adriano, additional, Latham, David W., additional, Li, Chih-Hao, additional, Lodi, Marcello, additional, Lovis, Christophe, additional, Molinari, Emilio, additional, Pepe, Francesco, additional, Udry, Stéphane, additional, Sasselov, Dimitar, additional, Szentgyorgyi, Andrew, additional, and Walsworth, Ronald, additional

Published
2015
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35. GIANO: An Ultra-Stable IR Echelle Spectrometer for the TNG Telescope

Author

Oliva, Ernesto, primary, Origlia, Livia, additional, Maiolino, Roberto, additional, Gennari, Sandro, additional, Biliotti, Valdemaro, additional, Rossetti, Emanuel, additional, Baffa, Carlo, additional, Leone, Franco, additional, Montegriffo, Paolo, additional, Lolli, Marco, additional, D’Amato, Francesco, additional, Bruno, Pietro, additional, Scuderi, Salvatore, additional, Ghinassi, Francesca, additional, Gonzalez, Manuel, additional, Lodi, Marcello, additional, Falcini, Gilberto, additional, Giani, Elisabetha, additional, Marcucci, Gianni, additional, and Sozzi, Mauro, additional

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37. WEAVE core processing system

Author

Walton, Nicholas A., additional, Irwin, Mike, additional, Lewis, James R., additional, Gonzalez-Solares, Eduardo, additional, Dalton, Gavin, additional, Trager, Scott, additional, Aguerri, J. Alfonso L., additional, Allende Prieto, Carlos, additional, Benn, Chris R., additional, Abrams, Don Carlos, additional, Picó, Sergio, additional, Middleton, Kevin, additional, Lodi, Marcello, additional, and Bonifacio, Piercarlo, additional

Published
2014
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38. Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

Author

Dalton, Gavin, additional, Trager, Scott, additional, Abrams, Don Carlos, additional, Bonifacio, Piercarlo, additional, López Aguerri, J. Alfonso, additional, Middleton, Kevin, additional, Benn, Chris, additional, Dee, Kevin, additional, Sayède, Frédéric, additional, Lewis, Ian, additional, Pragt, Johan, additional, Pico, Sergio, additional, Walton, Nic, additional, Rey, Juerg, additional, Allende Prieto, Carlos, additional, Peñate, José, additional, Lhome, Emilie, additional, Agócs, Tibor, additional, Alonso, José, additional, Terrett, David, additional, Brock, Matthew, additional, Gilbert, James, additional, Ridings, Andy, additional, Guinouard, Isabelle, additional, Verheijen, Mark, additional, Tosh, Ian, additional, Rogers, Kevin, additional, Steele, Iain, additional, Stuik, Remko, additional, Tromp, Neils, additional, Jasko, Attila, additional, Kragt, Jan, additional, Lesman, Dirk, additional, Mottram, Chris, additional, Bates, Stuart, additional, Gribbin, Frank, additional, Rodriguez, Luis Fernando, additional, Delgado, José M., additional, Martin, Carlos, additional, Cano, Diego, additional, Navarro, Ramón, additional, Irwin, Mike, additional, Lewis, Jim, additional, Gonzalez Solares, Eduardo, additional, O'Mahony, Neil, additional, Bianco, Andrea, additional, Zurita, Christina, additional, ter Horst, Rik, additional, Molinari, Emilio, additional, Lodi, Marcello, additional, Guerra, José, additional, Vallenari, Antonella, additional, and Baruffolo, Andrea, additional

Published
2014
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39. Construction progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

Author

Evans, Christopher J., Simard, Luc, Takami, Hideki, Dalton, Gavin, Trager, Scott, Abrams, Don Carlos, Bonifacio, Piercarlo, Aguerri, J. Alfonso L., Vallenari, Antonella, Middleton, Kevin, Benn, Chris, Dee, Kevin, Sayède, Frédéric, Lewis, Ian, Pragt, Johannes, Picó, Sergio, Walton, Nicholas, Rey, Jeurg, Allende, Carlos, Lhomé, Émilie, Terrett, David, Brock, Matthew, Gilbert, James, Ridings, Andy, Verheijen, Marc, Tosh, Ian, Steele, Iain, Stuik, Remko, Kroes, Gabby, Tromp, Neils, Kragt, Jan, Lesman, Dirk, Mottram, Chris, Bates, Stuart, Gribbin, Frank, Burgal, José Alonso, Herreros, Jose Miguel, Delgado, Jose Miguel, Martin, Carlos, Cano, Diego, Navarro, Ramón, Irwin, Mike, Lewis, James, Gonzales Solares, Eduardo, O'Mahony, Neil, Bianco, Andrea, Zurita, Christina, ter Horst, Rik, Molinari, Emilio, Lodi, Marcello, Guerra, José, Baruffolo, Andrea, Carrasco, Esperanza, Farkas, Szigfrid, Schallig, Ellen, Hill, Vanessa, Smith, Dan, Drew, Janet, Poggianti, Bianca, Pieri, Mat, Jin, Shoko, Dominquez Palmero, Lilian, Fariña, Cecilia, Martin, Adrian, Worley, Clare, Murphy, David, Hidalgo, Andrea, Mignot, Shan, Bishop, Georgia, Guest, Steve, Elswijk, Eddy, de Haan, Menno, Hanenburg, Hiddo, Salasnich, Bernardo, Mayya, Divakara, and Izazaga-Pérez, Rafael

Published
2018
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40. Harps-N: the new planet hunter at TNG

Author

Cosentino, Rosario, primary, Lovis, Christophe, additional, Pepe, Francesco, additional, Collier Cameron, Andrew, additional, Latham, David W., additional, Molinari, Emilio, additional, Udry, Stephane, additional, Bezawada, Naidu, additional, Black, Martin, additional, Born, Andy, additional, Buchschacher, Nicolas, additional, Charbonneau, Dave, additional, Figueira, Pedro, additional, Fleury, Michel, additional, Galli, Alberto, additional, Gallie, Angus, additional, Gao, Xiaofeng, additional, Ghedina, Adriano, additional, Gonzalez, Carlos, additional, Gonzalez, Manuel, additional, Guerra, Jose, additional, Henry, David, additional, Horne, Keith, additional, Hughes, Ian, additional, Kelly, Dennis, additional, Lodi, Marcello, additional, Lunney, David, additional, Maire, Charles, additional, Mayor, Michel, additional, Micela, Giusi, additional, Ordway, Mark P., additional, Peacock, John, additional, Phillips, David, additional, Piotto, Giampaolo, additional, Pollacco, Don, additional, Queloz, Didier, additional, Rice, Ken, additional, Riverol, Carlos, additional, Riverol, Luis, additional, San Juan, Jose, additional, Sasselov, Dimitar, additional, Segransan, Damien, additional, Sozzetti, Alessandro, additional, Sosnowska, Danuta, additional, Stobie, Brian, additional, Szentgyorgyi, Andrew, additional, Vick, Andy, additional, and Weber, Luc, additional

Published
2012
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42. An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus

Author

Phillips, David F., Glenday, Alex, Dumusque, Xavier, Buchschacher, Nicolas, Cameron, Andrew Collier, Cecconi, Massimo, Charbonneau, David, Cosentino, Rosario, Ghedina, Adriano, Haywood, Raphaelle D., Latham, David Winslow, Li, Chih-Hao, Lodi, Marcello, Lovis, Christophe, Molinari, Emilio, Pepe, Francesco, Sasselov, Dimitar D., Szentgyorgyi, Andrew H., Udry, Stephane, and Walsworth, Ronald Lee

Abstract

We recently demonstrated sub-m/s sensitivity in measuring the radial velocity (RV) between the Earth and Sun using a simple solar telescope feeding the HARPS-N spectrograph at the Italian National Telescope, which is calibrated with a green astro-comb. We are using the solar telescope to characterize the effects of stellar (solar) RV jitter due to activity on the solar surface with the goal of detecting the solar RV signal from Venus, thereby demonstrating the sensitivity of these instruments to detect true Earth-twin exoplanets., Physics

Published
2016
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43. GIANO: an ultrastable IR echelle spectrometer optimized for high-precision radial velocity measurements and for high-throughput low-resolution spectroscopy

Author

Oliva, Ernesto, primary, Origlia, Livia, additional, Maiolino, Roberto, additional, Gennari, Sandro, additional, Biliotti, Valdemaro, additional, Rossetti, Emanuel, additional, Baffa, Carlo, additional, Leone, F., additional, Montegriffo, Paolo, additional, Lolli, Marco, additional, D'Amato, Francesco, additional, Bruno, Pietro, additional, Scuderi, Salvatore, additional, Ghinassi, Francesca, additional, Gonzalez, Manuel, additional, Lodi, Marcello, additional, Falcini, Gilberto, additional, Giani, Elisabetta, additional, Marcucci, Gianni, additional, and Sozzi, Mauro, additional

Published
2004
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44. GIANO: An Ultra-Stable IR Echelle Spectrometer for the TNG Telescope.

Author

Käufl, Hans Ulrich, Siebenmorgen, Ralf, Moorwood, Alan F. M., Oliva, Ernesto, Origlia, Livia, Maiolino, Roberto, Gennari, Sandro, Biliotti, Valdemaro, Rossetti, Emanuel, Baffa, Carlo, Leone, Franco, Montegriffo, Paolo, Lolli, Marco, D'Amato, Francesco, Bruno, Pietro, Scuderi, Salvatore, Ghinassi, Francesca, Gonzalez, Manuel, Lodi, Marcello, and Falcini, Gilberto

Abstract

GIANO is an IR cross-dispersed echelle spectrometer designed to achieve high throughput, high resolving power, wide band coverage and high accuracy radial velocity measurements. It also includes polarimetric capabilities and a low resolution mode that make it a very versatile, common user instrument which will be permanently mounted and available at one of the Nasmyth foci of the Telescopio Nazionale Galileo (TNG) located at Roque de Los Muchachos Observatory (ORM), La Palma, Spain. This project was selected by INAF as the top priority instrument among those proposed within the Second Generation Instrumentation Plan of the TNG. More information on this project can be found at the web page http://www.bo.astro.it/giano. [ABSTRACT FROM AUTHOR]

Published
2005
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46. An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus

Author

Navarro, Ramón, Burge, James H., Phillips, David F., Glenday, Alex G., Dumusque, Xavier, Buchschacher, Nicolas, Cameron, Andrew Collier, Cecconi, Massimo, Charbonneau, David, Cosentino, Rosario, Ghedina, Adriano, Haywood, Raphäelle, Latham, David W., Li, Chih-Hao, Lodi, Marcello, Lovis, Christophe, Molinari, Emilio, Pepe, Francesco, Sasselov, Dimitar, Szentgyorgyi, Andrew, Udry, Stephane, and Walsworth, Ronald L.

Published
2016
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47. Final design and progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

Author

Evans, Christopher J., Simard, Luc, Takami, Hideki, Dalton, Gavin, Trager, Scott, Abrams, Don Carlos, Bonifacio, Piercarlo, Aguerri, J. Alfonso L., Middleton, Kevin, Benn, Chris, Dee, Kevin, Sayède, Frédéric, Lewis, Ian, Pragt, Johannes, Pico, Sergio, Walton, Nic, Rey, Jeurg, Allende Prieto, Carlos, Peñate, José, Lhome, Emilie, Agócs, Tibor, Alonso, José, Terrett, David, Brock, Matthew, Gilbert, James, Schallig, Ellen, Ridings, Andy, Guinouard, Isabelle, Verheijen, Marc, Tosh, Ian, Rogers, Kevin, Lee, Martin, Steele, Iain, Stuik, Remko, Tromp, Niels, Jaskó, Attila, Carrasco, Esperanza, Farcas, Szigfrid, Kragt, Jan, Lesman, Dirk, Kroes, Gabby, Mottram, Chris, Bates, Stuart, Rodriguez, Luis Fernando, Gribbin, Frank, Delgado, José Miguel, Herreros, José Miguel, Martin, Carlos, Cano, Diego, Navarro, Ramon, Irwin, Mike, Lewis, Jim, Gonzalez Solares, Eduardo, Murphy, David, Worley, Clare, Bassom, Richard, O'Mahoney, Neil, Bianco, Andrea, Zurita, Christina, ter Horst, Rik, Molinari, Emilio, Lodi, Marcello, Guerra, José, Martin, Adrian, Vallenari, Antonella, Salasnich, Bernardo, Baruffolo, Andrea, Jin, Shoko, Hill, Vanessa, Smith, Dan, Drew, Janet, Poggianti, Bianca, Pieri, Mat, Dominquez Palmero, Lillian, and Farina, Cecilia

Published
2016
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49. WAS: the data archive for the WEAVE spectrograph

Author

Chiozzi, Gianluca, Guzman, Juan C., Guerra, Jose, Molinari, Emilio, Lodi, Marcello, Martin, Adrian, Dalton, Gavin B., Trager, Scott C., Jin, Shoko, Abrams, Don Carlos, Bonifacio, Piercarlo, López Aguerri, Jose Alfonso, Vallenari, Antonella, Carrasco Licea, Esperanza E., and Middleton, Kevin F.

Published
2016
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