IPARCOS seminars, colloquia and journal club. 2018
List of IPARCOS seminars and colloquia:
- IPARCOSastro-seminars coordinated by Enrica Bellocchi, Patricia Sánchez Blazquez, Armado Gil de Paz and David Montes.
- IPARCOSFT-seminar coordinated by Felipe Llanes.
- IPARCOS colloquiums coordinated by Luis J. Garay.
- IPARCOS NUC-seminars cordinated by
- IPARCOS Journal Club cordinated by Clara Peset
- see IPARCOS YouTube channel
| Announc. | Date/Time | Place | Type | Title |
Speaker / Institution |
Available at |
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December 10th 2018, 15h:30 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Supermassive Black Holes and its effects on galaxy evolution |
UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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November 29th 2018, 15h:30 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Eclipsing binaries: mass transfer and starspots |
Shinjirou Kouzuma |
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November 15th 2018, 15h:30 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Discovery of a new planet around one of the closest stars through CARMENES data: Barnard's star b |
David Montes UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group
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November 7th 2018, 15h:30 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Discussion about paper: |
Various Speakers UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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October 24th 2018, 15h:30 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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weekly astro-meeting |
Various Speakers UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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October 15th 2018, 15h:30 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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The MOSAIC project.
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UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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October 1th 2018, 15h:00 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Discussion about paper: |
Various Speakers UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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September 24th 2018, 15h:00 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Discussion about how outflows in galaxies work, related with SNe feedback, AGN feedback and other effects you can think on. The main question is: Is it the fountain effect consistent with observations and simulations? |
Various Speakers UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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June 26th 2018, 15h:00 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Spatially-resolved analysis of the Star Formation Rate: insights on the activation and quenching mechanisms in bulges and disks
Abstract: To examine the relative role of the processes that can trigger and quench star formation on different spatial scales, it is essential to isolate the basic stellar structures that shaped galaxies (spiral arms, bars, bulges, etc.). Thus, we have combined a 2D multi-component photometric decomposition with CALIFA IFS data in a representative sample of 220 nearby galaxies. This allows us to determine the stellar mass and SFR from each of these components. Based on these parameters, the Star Formation Main Sequence of galaxies is explored. The main finding is that not only more massive galaxies but also more massive star-forming disks and earlier-type spiral disks have undergone efficient suppression of their star formation. We evaluate which mechanisms might be responsible for this quenching process. In particular, we analyze the presence of AGNs as a possible internal cause of star formation shutdown. The sSFR–M∗ relation for both disks and bulges is analyzed, finding that type-2 AGNs play a role damping the sSFR in bulges and less efficiently in disks. We emphasize the importance of the spatially-resolved analysis to provide an in-depth understanding of the processes that govern star formation. |
UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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June 21th 2018, 15h:00 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Applying deep learning techniques to analyzing weak lensing data Summary: Weak lensing (WL) measurements allow us to reconstruct the evolution of the matter density field, unlocking a wealth of cosmological information. As a result, many experiments such as Euclid, WFIRST or LSST will include extensive WL measurements as part of their scientific program. I will discuss our efforts to extract as much cosmological information from these upcoming datasets as possible. In particular, I will show as a proof of concept how neural networks can extract information from simulated WL maps beyond two-point statistics and some non-Gaussian observables. |
José Manuel Zorrilla Matilla Department of Astronomy in the Columbia University |
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June 11th 2018, 15h:00 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Estudio del medio circumgaláctico en galaxias simuladas |
UPARCOS, Univ. UCM, Dtpo. FTA, GUAIX Group |
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June 4th 2018, 15h:00 |
Seminar room of theoretical physics (4rd floor) |
IPARCOS astro-seminars
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Star-forming galaxies at low-redshift in the SHARDS survey: physical and morphological properties. |
Alejandro Lumbreras-Calle (IAC) |
Seminarios de miembros de IPARCOS en el ciclo "Hablemos de Física"
| Announc. | Date/Time | Place | Type | Title |
Speaker / Institution |
Available at |
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04 octubre 2018 13:30 |
Aula Magna |
IPARCOS astro-seminars |
Toda la luz del Universo |
Alberto Domínguez UPARCOS, Univ. UCM, Dtpo. FTA, EMFTEL Group
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* Seminars organized by the differente research groups:
- - Seminarios del Máster en Astrofísica: "Temas Avanzados en Astrofísica"
- - Seminarios de especialización - Doctorado en Astrofísica
- - Seminarios y Defensas de Tesis Doctorales - Doctorado en Astrofísica
- Seminarios de Física Teorica
- - Ciclo de seminarios De Madrid al Cosmos (organizado conjuntamente por el Grupo de Teorías Efectivas en Física Moderna de la UCM y el Grupo de Gravitación y Cosmología del Instituto de Estructura de la Materia (IEM-CSIC))
| Seminario | |
Deep learning as a tool for scientific data analysis: Introduction and hands-on sessionDaniel Nieto (GAE-UCM) Date: 17/05/2018 Location: Room 19, second floor RSVP here (for a headcount): https://goo.gl/forms/YkvoLrmBjRKnM2qo1 Abstract: It's been a while since we have had computers learn fromsci entific datasets to help squeezing the most out of our experimentsand astrophysical observatories. Nowadays, the "deep learning"revolution that is uplifting artificial intelligence to its next level is also permeating into the analysis of data from instruments as different as the LHC and LIGO, thus having an impact on fields from cosmology to particle physics. In this seminar we intend to a) present a brief introduction to deep learning for non-experts and give a quick overview on how various experiments and observatories are already exploiting this machine learning technique, and b) walk the attendants through a tutorial where they will learn the basics of how to build a simple deep-learning model and how to train it on their own laptops. |
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24 de octubre de 2017 - SEMINARIO Departamento de Física Atómica, Molecular y Nuclear, FAMN, Físicas, UCMTítulo: "Physical properties of Gamma-Ray Blazars" Conferenciante: Vaidehi S. Paliya, Clemson University, SC, USA Hora: 15:00 h |
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