Mini-courses

Thor’s Helmet - Thor’s Helmet is a rare example of a Wolf-Rayet star. Around 40 times the mass of our Sun, this type of star is young and extremely bright. It generates a wind that blasts outwards from the star at millions of kilometres per hour. Because Wolf-Rayet stars burn so brightly and shed so much material, scientists think they represent a brief stage before the star explodes as a supernova.

Credit: Jean-Charles Cuillandre

An introduction to Astrophysics

Frédéric Courbin

The main objective of this mini-course is to introduce the students to the concepts and tools of the modern Astrophysics.The course starts presenting the Kepler's laws and the Virial theorem.
Then the topics of radiation, matter and black body will be presented. With this basis there will be foreforward presented the concepts of magnitudes and spectrum and the Doppler-Fizeau effect. Next the topic of interestellar medium, tides and Roche limit will be studied. Then  topics continue with Comets, planets and their atmospheres, stellar formation, galaxies and the  Milky Way. The course will end with some of the most interesting topics nowadays: dark matter, cosmological distances and gravitational lensing.

 

Pleiades - The Seven Sisters, also known as the Pleiades star cluster, seem to float on a bed of feathers in this infrared image from the Spitzer Space Telescope. Clouds of dust sweep around the stars, wrapping them in a cushiony veil. The Pleiades, located in the Taurus constellation (the bull), are the subject of many legends and writings in cultures around the globe.

Credit: NASA/JPL-Caltech/J. Stauffer

An introduction to basic descriptive statistical concepts applied to modern Astronomy

Jaime Muñoz and Alejandro García

The main objective of this mini-course is to show basic statistical concepts and how these can be applied to handled astronomy data sets. Participants will learn or review concepts
such as statistic variable types, data descriptive analysis including graphical data analysis, location and scale measures, skewness, kurtosis. On each session participants not only are going to learn the concepts theoretically but also, they will have a workshop to practice the concepts explained in class using R Statistical software. We hope that at the end of the mini-course, participants must be able to make a descriptive analysis of the data and have learned basic concepts of R software to do so.
Topics: Variable Types: Quantitative and qualitative, levels of measurement. Graphical data analysis: Bar graphs, Pie charts, Line charts, Histograms, Box plots, Quantile graphs. Locations and Scale Measure: Mean, Trimmed Mean, Median, Range, Variance, Median Absolute Deviation, Interquartil range. Distribution data shape measures: Skewness, Homogenity, Kurtosis. Quantile-Quantile graphs: Interpretation.  Example of statistical modeling (presentation of the use of a linear model).

 

NGC 253 -One of the brightest galaxies beyond our local group, NGC 253 is also one of the dustiest. In addition to its spiral dust lanes, ones running perpendicular to the galaxy’s plane indicate intense star formation, making it a good example of a starburst galaxy.

Credit: R. Jay GaBany.

 

The fundamentals of Astrometry: Key concepts, procedures and applications

Katherine Vieira

We will cover the basics of Astrometry that anyone working on a Astronomy/Astrophysics subject should know, to have a comprehensive professional profile, necessary and
looked after, whether you do research, teaching or outreach. How we assign coordinates to celestial objects involves defining and realizing the appropiate reference systems, considering the effects that change the position of such objects along time introduce errors in their measurement. Such reference systems are materialised by astrometric catalogs used by the astronomical community at large. We will also explore various key Astrophysical problems answered  - sometimes only - by Astrometry.

The application period has ended

  • Antennae Galaxies
    Antennae Galaxies

    Credit: NASA/ESA/ Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration

  • Thor’s Helmet
    Thor’s Helmet

    Credit: image made in visible light by Jean-Charles Cuillandre for the Canada-France-hawaii Telescope Corporation

  • Carina Nebula
    Carina Nebula

    Credit: image made in visible light by N. Smith (UC Berkeley) and the NASA/ESA Hubble Heritage Team

  • Hercules Cluster of Galaxies
    Hercules Cluster of Galaxies

    Credit: Canada-France-Hawaii Telescope / Coelum / J.-C. Cuillandre & G. Anselmi

  • Horsehead Nebula
    Horsehead Nebula

    Credit: T.A.Rector (NOAO/AURA/NSF) and Hubble Heritage Team (STScI / AURA / NASA).

  • Hubble Ultra Deep Field
    Hubble Ultra Deep Field

    Credit: image made in visible and infrered light by S. Beckwith for the NASA/ESA Hudf Team

  • Lunar Eclipse
    Lunar Eclipse

    Credit: Akira Fujii / Ciel et Espace

  • Pleiades
    Pleiades

    Credit: NASA/JPL-Caltech/J. Stauffer (SSC/Caltech)

  • NGC 253
    NGC 253

    Credit: R. Jay GaBany

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