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33 papers · 2 filters
The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library
D. S. Aguado, Romina Ahumada, Andres Almeida +230
Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years o…
Statistical analysis of probability density functions for photometric redshifts through the KiDS-ESO-DR3 galaxies
Valeria Amaro, Stefano Cavuoti, Massimo Brescia +8
Despite the high accuracy of photometric redshifts (zphot) derived using Machine Learning (ML) methods, the quantification of errors through reliable and accurate Probability Densi…
Absolute reflectance of a concave mirror used for astro-particle physics experiments
Razmik Mirzoyan, Cornelia Arcaro, Hanna Kellermann +1
The absolute reflectance of a reflector and its point spread function are the key parameters of a telescope for measuring light flux. Typically, one is using low-cost technologies…
A 3.9 km baseline intensity interferometry photon counting experiment
Giampiero Naletto, Luca Zampieri, Cesare Barbieri +6
In the last years we have operated two very similar ultrafast photon counting photometers (Iqueye and Aqueye+) on different telescopes. The absolute time accuracy in time tagging t…
Timing analysis and pulse profile of the Vela pulsar in the optical band from Iqueye observations
A. Spolon, L. Zampieri, A. Burtovoi +5
The Vela pulsar is among a number of pulsars which show detectable optical pulsations. We performed optical observations of this pulsar in January and December 2009 with the Iqueye…
The VIS detector system of SOXS
Rosario Cosentino, Matteo Aliverti, Salvatore Scuderi +46
SOXS will be a unique spectroscopic facility for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (8…