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IVOA Newsletter - June 2025

Created: June 02, 2025 - 09:00 UTC

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The International Virtual Observatory Alliance (IVOA) was formed in June 2002 with a mission to facilitate the international coordination and collaboration necessary for the development and deployment of the tools, systems and organizational structures necessary to enable the international utilization of astronomical archives as an integrated and interoperating virtual observatory. The IVOA now comprises 20 VO programs from Argentina, Armenia, Australia, Brazil, Canada, Chile, China, Europe, France, Germany, Hungary, India, Italy, Japan, Russia, South Africa, Spain, Ukraine, the United Kingdom, and the United States and an inter-governmental organization (ESA). Membership is open to other national and international programs according to the IVOA Guidelines for Participation. You can read more about the IVOA and what we do at https://ivoa.net/about/.

What is the VO?

The Virtual Observatory (VO) aims to provide a research environment that will open up new possibilities for scientific research based on data discovery, efficient data access, and interoperability. The vision is of global astronomy archives connected via the VO to form a multiwavelength digital sky that can be searched, visualized, and analyzed in new and innovative ways. VO projects worldwide working toward this vision are already providing science capabilities with new tools and services. This newsletter, aimed at astronomers, highlights VO tools and technologies for doing astronomy research, recent papers, and upcoming events.


IVOA NEWS

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IVOA Interoperability meeting – Malta, November 2024

Simon O’Toole

The Northern Fall Interoperability meeting was held on 15-17 November in Valletta, Malta, after the ADASS meeting. As with all IVOA meetings since the COVID pandemic, it was a hybrid meeting, with a large number of attendees in person (113 in person, 49 online). Sessions were recorded and posted online. There were many great discussions and some big decisions were made, outlined below.

High Energy Interest Group

A new Interest Group focussed on High Energy Astrophysics (HEIG) was formally approved at the Malta Interop. This had followed over a year of planning and many discussions and a session at the May 2024 Interop in Sydney. The chair of the Interest Group is Bruno Khelifi from CNRS, and the vice chair is Janet Evans from CfA.

The HEIG held a joint plenary session with the Time Domain Interest Group where we heard about multi-messenger astronomy and the transient nature of high energy astrophysics. This session led to a renewed focus on the VOEvent standard, and a splinter session organised to discuss the path moving forward.

Protocol Transitioning Tiger Team

The Protocol Transitioning Tiger Team (P3T) held its final session in Malta with a lot of great work by the team to move IVOA standards into the OpenAPI framework. Initial work around UWS was presented by Josh Fraustro and further discussions around more complex standards took place. The team presented a set of potential next steps, and the transition to OpenAPI will now be the responsibility of the working groups.

Highlights

There were plenty of other highlights from this Interop, including, but definitely not limited to, the following:


The Virtual Observatory is evolving and adapting to the needs of the community and in particular next generation facilities such as the Vera Rubin Observatory and the SKA. The Malta Interop was a great example of this. Special thanks go to Alessio Magro and his team at the University of Malta for hosting us in such a beautiful part of the world!


Members of the astronomical community are welcome to get involved in the IVOA. See the links below for ways to participate:

Name URL Description
IVOA Website https://www.ivoa.net/ Place to start
IVOA Wiki pages https://wiki.ivoa.net/ Collaboration area
Main Mailing List interop ‘at’ ivoa.net IVOA community list
All Mailing Lists https://www.ivoa.net/members/ Identifies email lists for all WG/IG, CSP & Exec.
Slack https://ivoa.slack.com/ Collaboration slack channel
Github https://github.com/ivoa Collaboration development/new ideas
Github https://github.com/ivoa-std Standard document development


Some recent papers about VO-enabled science

The Initial Mass Function Based on the Full-sky 20 pc Census of ∼3600 Stars and Brown Dwarfs

Kirkpatrick, J. Davy et al.

The Astrophysical Journal Supplement Series, Volume 271, 55

A complete accounting of nearby objects—from the highest-mass white dwarf progenitors down to low-mass brown dwarfs—is now possible, thanks to an almost complete set of trigonometric parallax determinations from Gaia, ground-based surveys, and Spitzer follow-up. We create a census of objects within a Sun-centered sphere of 20 pc radius and check published literature to decompose each binary or higher-order system into its separate components. The result is a volume-limited census of ∼3600 individual star formation products useful in measuring the initial mass function across the stellar (<8M⊙) and substellar (≳5M Jup) regimes. Comparing our resulting initial mass function to previous measurements shows good agreement above 0.8M⊙ and a divergence at lower masses. Our 20 pc space densities are best fit with a quadripartite power law, ξ(M)=dN/dM∝M−α , with long-established values of α = 2.3 at high masses (0.55 < M < 8.00M⊙), and α = 1.3 at intermediate masses (0.22 < M < 0.55M⊙), but at lower masses, we find α = 0.25 for 0.05 < M < 0.22M⊙, and α = 0.6 for 0.01 < M < 0.05M⊙. This implies that the rate of production as a function of decreasing mass diminishes in the low-mass star/high-mass brown dwarf regime before increasing again in the low-mass brown dwarf regime. Correcting for completeness, we find a star to brown dwarf number ratio of, currently, 4:1, and an average mass per object of 0.41 M⊙.

DOI: 10.3847/1538-4365/ad24e2

Refereed Publications

The full list of refereed publications from April 2022 to June 2025 can be found at the following list, curated by the Spanish Virtual Observatory.

All ADS links mentioning the “virtual observatory” in the abstract.

All refereed publications mentioning the “virtual observatory” in the abstract.


VO calendar

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