Serbian virtual observatory

Abstract

The work on SerVO -Serbian virtual observatory (http://servo.aob.rs/~darko) started in 2008, with aims 1) To establish SerVO and join the EuroVO -European Virtual Observatory and IVOA -Inetrnational Virtual Observatory Alliance; 2) To create SerVO data Center for digitalization and archiving in VO format photo-plates from Belgrade Astronomical Observatory and other astronomical results obtained by the staff; 3) To develop the tools for visualization of data; 3) To develop together with Observatoire de Paris, STARK-B -database containing as the first step Stark widths and shifts of spectral lines, determined within the semiclassical perturbation approach by two of us (MSD-SSB) and to create a mirror site in Belgrade; 4) To make a mirror site for DSED (Darthmouth Stellar Evolution Database) in which development took part one of us (DJ). An additional aim is the creation of VAMDC (Virtual Atomic and Molecular Data Center) AOB (Astronomical Observatory of Belgrade) Node, and a recent objective is the collaboration with the Large Synoptic Telescope (LSST) project.In this contribution SerVO project is reviewed within the context of e-science in AstronomyAstroinformatics.

Stark broadening of B I spectral lines

“…Stark widths and shifts for B I spectral lines presented here will be included in the STARK-B database (Sahal-Bréchot 2010; Sahal-Bréchot, Dimitrijević & Moreau 2012;Sahal-Bréchot et al 2015a,b), which enters in [VAMDC - (Dubernet et al 2010;Rixon et al 2011;Dubernet et al 2016;Albert et al 2020)]. A link to STARK-B is also in the Serbian Virtual Observatory [SerVO, http:servo.aob.rs, Jevremović et al (2009), Jevremović et al (2012)].…”

Stark broadening of Zn II spectral lines

“…Stark widths and shifts for Zn II spectral lines will also be implemented in the STARK-B data base (Sahal-Bréchot et al 2010;Sahal-Bréchot, Dimitrijević & Moreau 2012, 2015aSahal-Bréchot et al 2015b), which is a part of Virtual Atomic and Molecular Data Center (VAMDC) (Dubernet et al 2010;Rixon et al 2011;Dubernet et al 2016;Albert et al 2020). We note as well that a link to STARK-B is in the Serbian Virtual Observatory (SerVO, http:servo.aob.rs) (Jevremović et al 2009;Jevremović et al 2012).…”

Stark broadening of Zr iv spectral lines in the atmospheres of chemically peculiar stars

“…The STARK-B data base is devoted to diagnostics, modelling and investigations of stellar atmospheres, diagnostics of laboratory plasmas, and investigation, analysis and modelling of laser produce, inertial fusion plasma and plasma technologies. There is a link to STARK-B in the Serbian Virtual Observatory's website (SerVO, http://servo.aob.rs, Jevremović et al 2009Jevremović et al , 2012.…”