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Teaching • The Astrophysics Seminar
Welcome to the homepage of The Astrophysics Seminar (astro894 - 6961), a four credit point elective seminar in the Master of Astrophysics programme at the Argelander Institute for Astronomy, part of the University of Bonn. Students give a talk and answer relevant questions both live and afterward on the Astrosem Blog. Talk topics are based on published papers, as suggested by the supervisors, and students should discuss their topic, and the content of their talk, with their supervisor prior to giving it.

Time and Place
    Mondays, 14-15.30, Room 0.012 (Hoersaal Astronomie/Astronomy Main Lecture Room), AIfA, starting 8th April with an introductory session chaired by Thomas Reiprich. Supervisors will present their topics at this first session, so attendance is crucial! Students should email Rob () stating their choice of date, paper and supervisor.

Purpose
    In science, it is not enough to simply do your research even if you are the best scientist in the world. We all must communicate what we have done, both effectively and efficiently. This seminar is a chance for a student to give a talk on a state-of-the-art subject in astrophysics. Students will learn about oral communication: the art of communicating using your voice with their peers. This is a skill required of any professional scientist, e.g. at conferences, in meetings or when teaching.
    See also the course on Scientific Writing for complementary information about writing skills.

Talks
   The talks are a strict maximum of 30 minutes in length with 15 minutes of questions at the end (total 45 minutes). Speakers should expect to receive and answer questions both immediately following the talk and on the Astrosem blog during the week following their talk (see below).
   This may be the first time that students encounter state of the art scientific literature in the form of research papers. Research papers are not easy to read, and this is one of the hurdles will need to be passed on your way to giving the talk. Supervisors are there to help!
   A research paper typically contains references to other papers. Which of these should followed up will be clarified by talking to with supervisors. Following-up some of the cited literature will teach the speaker how to navigate the minefield that is the scientific literature.

The Audience
   An important skill in giving talks is to know your audience. The Astrosem audience consists mostly of the peers of the speaker: Talks should be aimed at a level that can be understood by all the attending students. That means for most weeks each speaker is a member of the audience. However it is not an opportunity to sleep: there is a question and answer session immediately following the talk and all students are expected to participate. Questions should also be posted on the Astrosem Blog (see below).

Astrosem Blog
    After the seminar, the questions posed and any further questions and/or discussion should be posted on the Astrosem blog http://www.astro.uni-bonn.de/blogs/astrosem/.    To use the blog you need 1) the password given out in the seminar and 2) to register. Please use your real name when you register, we need to know from whom the questions and answers come.

Assessment
    Students should attend all the seminars, give their complete attention and participate fully by asking questions immediately following the talk and by posting questions on the Astrosem blog after the seminar. It is an essential part of training as a professional - scientist or otherwise! - to learn to both respond to and to ask good questions. All students taking the Astrosem are graded on the usual 1-5 system, 1 being the best, based on their talk.
    Students should repeat any questions they ask after the talk on the blog, and the speaker must similarly answer them there also, so that the questions and answers are recorded and that students can engage in lively debate.

Feedback
    Students can provide anonymous feedback at www.astro.uni-bonn.de/lecture-feedback using the password given in the class.

Facilities
    Talks are usually in the format of computer-based slides (e.g. Impress, Keynote, Powerpoint, LaTeX Beamer). If you use the projector you must make sure it functions with your laptop before the talk starts because any time taken fixing the laptop will be taken out of your allocated 30 minutes. It is also up to you to make sure - in advance - that all your text, plots, images, animations etc. are clearly visible. Marks will be deducted for poor presentation because it often impedes good science.

Topics
    The topics (i.e. talk titles) listed below are chosen by the scientific supervisors. You should choose one of them from the list below by contacting the supervisor, usually at the introductory meeting or shortly thereafter. Also, topics other than the ones shown below can be arranged with the supervisors. Note that there are maximum two talks per week - first come first served! Term ends on 19th July, please make sure talks are before 15th July to avoid clashes with exams/revision. Please note that each supervisor is limited to two talks.

Language
    As with all of the Master in Astrophysics, talks must be given in English.

List of Topics and Timetable (Summer 2013)
Title/linkSupervisorDates UnavailableSpeakerSeminar Date
Dust Formation in the Ejecta of Common Envelope Systems Robert Izzard (Herbert Lau presents...) 8/04, 15/04, 27/05 ... ...
Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts Cristiano Porciani 8/04 ... ...
Planck 2013 results. XXII. Constraints on inflation
Planck 2013 results. XXVI. Background geometry and topology of the Universe
Possible indication for non-zero neutrino mass and additional neutrino species from cosmological observations
See also 1212.6154v1
Thomas Reiprich 24/06 ... ...
A Catalog of Ultra-compact High Velocity Clouds from the ALFALFA Survey: Local Group Galaxy Candidates? Nadya Ben Bekhti ... ...
Probing the Extended Gaseous Regions of M31 with Quasar Absorption Lines
Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove Kaustuv moni Basu ... ...
More than meets the eye: magnetars in disguise Thomas Tauris 20/05, 27/05 ... ...
Cross-calibration of Suzaku/XIS and XMM-Newton/EPIC using galaxy clusters Yu-Ying Zhang ... ...
The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics
A Massive, Cooling-Flow-Induced Starburst in the Core of a HighlyLuminous Galaxy Cluster Peter Schneider ... ...
Planck 2013 results. XVI. Cosmological parameters
PHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies Benjamin Magnelli ... ...
Convective-reactive Proton-^12 C Combustion in Sakurai's Object (V4334 Sagittarii) and Implications for the Evolution and Yields from the First Generations of Stars Richard Stancliffe 20/05, 10/06, 17/06, 24/06, 1/07 ... ...
The CO-to-H2 Conversion Factor and Dust-to-Gas Ratio on Kiloparsec Scales in Nearby Galaxies Marcus Albrecht ... ...
Dynamics of Circumstellar Disks in Be Star Binaries Massi Maria ... ...
IRAS 16293: A Magnetic Tale of Two Cores Felipe Alves 15,22,29/04; 20/05; 10,24/06; 8,15/07 ... ...
A phenomenological approach to the evolution of galaxies Pavel Kroupa ... ...
The Most Metal-Poor Stars. IV. The Two Populations With [Fe/H] < -3.0 Herbert Lau ... ...
Nonlinear Evolution of the Radiation-Driven Magneto-Acoustic Instability (RMI) Jonathan Braithwaite ... ...
Spin down of the core rotation in red giants
Detection of a weak surface magnetic field on Sirius A: are all tepid stars magnetic?
... ...
... ...
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