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Workshop Laboratorio Spettroscopia INAF

Jun 10 – 11, 2019
Europe/Rome timezone

Contribution List

28 / 28
16. Aims and organization of the national laboratories at INAF
Adriano Fontana
6/10/19, 11:30 AM
17. Towards a new INAF laboratory for spectroscopy
Germano Sacco, Marco Scodeggio
6/10/19, 11:45 AM
20. MOONS GTO GALACTIC Survey and Labs
Livia Origlia
6/10/19, 12:00 PM

In this talk I will briefly review the main features of the MOONS GTO Galactic Survey, including data treatment. I will also pose some questions for discussion concerning Labs.
18. WEAVE and 4MOST Galactic Surveys
Sara Lucatello
6/10/19, 12:30 PM
19. A 4MOST survey of young stars in the solar neighbourhood: the role of the laboratory
Germano Sacco
6/10/19, 12:50 PM
42. WEAVE-STePS - Lessons learned
Angela Iovino
6/10/19, 2:10 PM

In this talk we will present what are the tools that we think are needed to prepare efficiently science exploitation of forthcoming spectrsocopic extragalactic large surveys.
We will discuss our experience of planning for the forthcoming WEAVE-StePS survey, highlighting the advantages offered by the availability of simple tools that enable realistic simulations of the whole process from...
22. MOONS extragalactic surveys
Bianca Garilli
6/10/19, 2:30 PM
23. Lessons for the Future from High-Resolution Surveys
Stefano Cristiani
6/10/19, 3:00 PM

High-resolution spectroscopy traditionally has been one of the first fields in which the standardizationof the data and the implementation of an end-to-end concept of the instrumentation has taken place. The HIRES @ Keck and UVES and, more recently, ESPRESSO @ VLT are paramount
recent examples in this sense (e.g. KODIAK, Popler).
This overview talk will try to extract the lessons derived from...
24. Spectroscopic characterisation of sub-stellar objects
Valentina D'Orazi
6/10/19, 3:20 PM
27. Spectroscopic pipelines from VLT/VIMOS to the LBT instruments and beyond
Marco Scodeggio
6/10/19, 4:00 PM
28. QSFit: Automatic analysis of AGN optical spectra
Giorgio Calderone
6/10/19, 4:30 PM

The QSFit package allows to perform automatic analysis of optical/UV AGN spectra. The software is very easy to use (it just requires the input FITS file) and provides estimates of: emission line luminosities, widths and velocity offsets; host galaxy luminosities; iron lines luminosities at optical and UV wavelengths; Balmer continuum luminosities; continuum slopes and luminosities at several...
29. Present and Future of stellar spectroscopy
Raffaele Gratton
6/10/19, 4:50 PM
30. Measuring gas-phase metallicities in distant galaxies
Filippo Mannucci
6/10/19, 5:20 PM
32. Methodological challenges in the spectroscopic estimates of stellar population parameters from low to high redshift
Stefano Zibetti
6/11/19, 9:10 AM
33. INTRIGOSS: A library of High Resolution synthetic spectra for FGK stars
Mariagrazia Franchini
6/11/19, 9:30 AM
34. The Italian Astronomical Archive (IA2): status of the services and future perspectives
Elisa Londero
6/11/19, 10:00 AM
35. Large-scale spectroscopic surveys management
Paolo Frazetti
6/11/19, 10:20 AM
36. Expandable Management of Astrophysical Catalogues: the case of CLASH-VLT data
Giuseppe Riccio
6/11/19, 10:40 AM
43. The ICT Office at INAF: todays activity and future plans.
Anna Di Giorgio
6/11/19, 11:00 AM

The ICT office of the Science Directorate of INAF has the primary role to support INAF researchers
in scientific and technological activities related to Information Technology (IT) at large.
IT is playing a crucial role in present and future scientific activities. New challenges in astronomy
require the use of modern ICT tools and frameworks such as efficient large storage systems,
distributed...
37. Astroinformatics and Astrophysics, a virtuous synergy in the Big Data era
Massimo Brescia
6/11/19, 11:40 AM
38. Data processing for high-resolution spectroscopy: today and tomorrow
Guido Cupani
6/11/19, 12:10 PM

INAF has a long tradition in the treatment of spectroscopical data. The Astronomical Observatory of Trieste (OATs), in particular, has always been at the forefront of the field, both validating the state-of-the-art software (e.g. the VLT UVES and X-shooter pipelines) and implementing new solutions
for the analysis of near-UV to near-IR medium-to-high resolution quasar spectra.
In this talk, I...
39. SyNaLoTA, a web infrastructure for astrophysical data analysis and exploration
Giuseppe Riccio
6/11/19, 12:30 PM

On top of modern large astrophysical data repositories, a fast, flexible, portable and efficient system for data analysis and exploration is required. We present SyNaLoTA (Systems from Naples for Long Term Analysis), a web based infrastructure, specialized in monitoring, analysis and visualization
of scientific data. Initially designed and under development for the ESA Euclid Mission...
40. Is this lab properly aimed? Optimizing data quality and analysis by focusing on the design, calibration and maintenance of the spectrometers.
Ernesto Oliva
6/11/19, 12:50 PM

The analysis of data is too often considered as a task that must inevitably accept and correct the problems related to the instrumentation.
Many FTEs are therefore dedicated to developing tools and tricks to mitigate these problems; and when these FTEs are not available the data are poorly used or not used at all.
In most cases, the instrumental problems can be solved using far less efforts...
41. Open discussion on aims, organization and future actions for the laboratory
Adriano Fontana, Germano Sacco, Marco Scodeggio
6/11/19, 2:10 PM
31. Methodological challenges in the spectroscopic estimates of stellar population parameters from low to high redshift
Stefano Zibetti
26. Spectroscopic pipelines from VLT/VIMOS to the LBT instruments and beyond
Marco Scodeggio

Starting from the work with the ESO/VLT VIMOS spectrograph, we have developed a spectroscopic
pipeline that has been used to reduce data from many spectroscopic surveys (VVDS, zCOSMOS,
VIPERS, VANDELS). This software was then used to create the pipelines used by the LBT Data
Reduction Center, to reduce spectroscopic data obtained with the LUCI and MODS instruments at
LBT, and we are preparing...
25. The ICT Office at INAF: todays activity and future plans.
Giuliano Taffoni
21. WEAVE Extragalactic Survey
Angela Iovino
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