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The importance of archival science increases significantly for astrophysical observatories as they mature and their archive holdings grow in size and complexity. Further enhancing the science return of archival data requires engaging a larger audience than the mission reference community, mostly because of the growth of interest in multi-wavelength and transient/time variability research. Such a goal, though, can be difficult to achieve. In this paper I will describe a different approach to this question that, while minimizing technological friction and leveraging existing services, makes archival observations more accessible and increases our capability to proactively engage astronomers on potentially interesting archival records. Inspired by this strategy, the Chandra Data Archive team is working on two specific experimental projects that will hopefully demonstrate their potential while contributing to the maximization of the scientific return of the Chandra mission.
In this article I present IEAD, a new interface for astronomical science databases. It is based on a powerful, yet simple, syntax designed to completely abstract the user from the structure of the underlying database. The programming language chosen
The future of astronomy is inextricably entwined with the care and feeding of astronomical data products. Community standards such as FITS and NDF have been instrumental in the success of numerous astronomy projects. Their very success challenges us
In this article we wonder what the next 100 years will bring for women in astronomy in the UK. After this year of looking back and celebrating 100 years of women in the Royal Astronomical Society (RAS), we now ask: what might the future hold? Extrapo
The U.S. Virtual Astronomical Observatory was a software infrastructure and development project designed both to begin the establishment of an operational Virtual Observatory (VO) and to provide the U.S. coordination with the international VO effort.
This white paper advocates for the creation of a community-wide program to maintain precise mid-transit times of exoplanets that would likely be targeted by future platforms. Given the sheer number of targets that will require careful monitoring betw