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To investigate this process numerical aggregates of particles bonded by cohesive forces would be generated and their resulting fragmentation, sticking or disruption on impact with a target studied. Velocity, Density with a time delay will be displayed. The most recent spectroscopic results are the end-product of laboratory attempts to create accurate linelists of methane coefficients.

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It carries three high throughput X-ray telescopes with an unprecedented effective area. Statistical methods, including possibly data mining, will be used to distinguish between real variability and measurement noise. Programming in common web application development languages and frameworks e.

Whilst their detection can be made in various wavelengths, the only true confirmation of cluster comes from the presence of Bremsstrahlung emission. But there are further types of transient or strongly time variable sources not yet covered by these monitor tools, e. The enormous amounts of matter and energy thus injected may affect the evolution of the central black hole and the galaxy in a process called cosmic feedback. If time permits we will then use the system to look for unusual ultraviolet and X-ray variability in a sample of galaxies.

This code requires complex configuration and is very tied to Gaia data model. Linux at system administration level. In spite of their potential importance, the origin, location, and impact of these winds are still a matter of debate and a hot topic in modern extragalactic astrophysics.

The project can be divided in different parts. In fact, scientific observations from archives are more likely to be used if the descriptions and the metadata clearly point the scientific users to the data they need. Their large bolometric output is powerful enough to drive ionized winds into the interstellar medium of the host galaxy and even into the intergalactic medium. As these stars evolve they accrete their surrounding gas and eventually form a protoplanetary disk around them. These four systems shall be executed in a daily base fed-up with orbital information gathered in the database.

Apply additional layers of information e. The current state of the art is AgisLab. It ensures access to scientific products for decades to the public and the science community. The simulator will allow the execution of additional tasks, which can be considered as auxiliary tasks supporting the overall Science Planning processes. The trainee will receive support regarding astrometry and Python.

Version control systems e. More advanced web interfaces and alert mechanisms via mobile phones should also be investigated. This project is a great way to learn about X-ray astrophysics and the analysis methods commonly used.

The student will also have access to a reference simulator to validate the prototype. Some programming skills will be helpful e. Good level of English, both spoken and written, is required. The two active galaxies to be studied have been recently observed and the full scientific potential of these observations has not been fully exploited yet.

They have proven to be helpful for the scientific comunity, on occasion triggering observations with targeted telescopes. This project has a high outreach potential, and the outcome of this work may be presented in a scientific publication. The confirmation of a cluster detection is typically done by eye, a slow and inefficient process. Training on methods and approaches will be provided by the tutors. Depending on performance and the outcome of the analysis, co-authorship of a paper in a refereed astronomy journal.

There are two related topics of investigation, either of which could be considered, depending on the strength of the applicant. Computing network engineering principles. Furthermore, the hard X-ray spectrum revealed direct evidence for its magnetic field, through the study of so-called cyclotron resonant scattering features. Once this is achieved, the map will be combined with complementary data such as protoplanetary disk and stellar properties e. The output of the project will be exhibited to the public through various forms e.

Version control systems e