The 6th Young Astronomers Meeting at CAMK-PAN

Europe/Warsaw
Lecture Hall (Hybrid)

Lecture Hall (Hybrid)

Bartycka 18 00-716 Warsaw
Description

Recruitment 2024/2025 is open for applications!

Nicolaus Copernicus Astronomical Center invites applications for astronomy and astrophysics PhD studies

For more information: Recruitment

 

Nicolaus Copernicus Astronomical Center Polish Academy of Sciences is a leading astronomical institute in Poland established in 1978.
The main subjects of research include:

  • Stellar astrophysics
  • Binary systems
  • Cosmic distance scale
  • Dense matter and neutron stars
  • Black holes
  • Accretion processes
  • Structure and evolution of active galaxies
  • Gravitational waves
  • Cosmology
  • Dark matter

Astronomers from the Nicolaus Copernicus Astronomical Center are involved in a number of major international observational projects such as H.E.S.S., CTA (observations of ultra high energy photons (TeV) via detection of Cherenkov radiation), Herschel (satellite observations in IR domain), SALT (Southern African Large Telescope), INTEGRAL, Fermi (satellite observations of gamma rays), LIGO-Virgo-KAGRA (detection of gravitational waves). DarkSide collaboraton (Searching for Dark matter), the Araucaria Project (improving the calibration of the cosmic distance scale in the local universe) and Project SOLARIS (search for extrasolar planetary systems), financed in part by the European Research Council (Starting Independent Researcher Grant).

Important information:

  • The meeting will be in a hybrid format (both on-site and on the Zoom platform) and participation is free of charge.
  • The abstracts (poster and talk) should be sent to young.astro.meeting@camk.edu.pl by 1st of March, 2024.
  • Limited on-site participation slots and limited accommodations for participants who want to join in person from outside of Warsaw. Please register by the 1st of March for on-site participation.
  • The registration for Online participants is extended till the 5th of March.
  • Please send an email to young.astro.meeting@camk.edu.pl for the accommodation request.

 


Research at CAMK (Youtube)
Develop your career at CAMK (Youtube) 

    • Registration
    • 1
      Welcome address
      Speaker: Sergen Özdemir
    • 2
      A speech by the director of Nicolaus Copernicus Astronomical Center
      Speaker: Rafał Moderski
    • 3
      A speech by the coordinator of the GeoPlanet doctoral school
      Speaker: Radek Smolec
    • 12:00
      Lunch
    • 4
      Cosmic distances - the royal road to solve the biggest mysteries of the Universe
      Speaker: Grzegorz Pietrzynski (CAMK)
    • 5
      Gravitational waves astronomy with LIGO-Virgo-KAGRA
      Speaker: Michał Bejger (CAMK)
    • 6
      Chaos and Einstein-Rosen Gravitational Waves
      Speaker: Syed Umair Naqvi (Jagiellonian Universtiy)
    • 7
      Stellar mergers and interferometry: high resolution astronomy of colliding stars
      Speaker: Thomas Steinmetz (Nicolaus Copernicus Centre for Astronomy)
    • 15:00
      Coffee break
    • 8
      Uncertainties on the evolutionary tracks of medium mass stars
      Speaker: Oliwia Ziółkowska (CAMK)
    • 9
      Tools for modern scientific computing
      Speaker: Piotr Gawron (CAMK PAN)
    • 10
      ISM removal process in the early-type galaxies under the view of spectral analysis
      Speaker: Oleh Ryzhov
    • 11
      Q & A session
    • 12
      Growing Black Holes in Star Clusters

      Since 2015, more than 80 merging black holes have been discovered through the direct detection of gravitational waves by the LIGO-Virgo-KAGRA collaboration. While these observations provide unprecedented insights into the demographics of black holes, they also raise important questions about the astrophysical origin and formation of these elusive binary systems. One of the formation channels for these observed gravitational wave sources are dynamical interactions in star clusters. A significant fraction of stars are born in clusters where they are closely packed together. In some of these clusters, the density of stars can be up to a million times higher than the density of stars in the solar neighbourhood. In this talk, I will briefly describe how star clusters evolve and how we can evolve them using state-of-the-art computer simulations. I will show how gravitational encounters in these dense stellar environments can be conducive to forming merging binary black holes. Massive and dense star clusters could also be potential sites for forming black holes with masses between ~ 100 to 10,000 times the mass of the Sun. I will also highlight different pathways by which these intermediate-mass black holes can form and grow in the densest star clusters.

      Speaker: Abbas Askar (Nicolaus Copernicus Astronomical Center, Warsaw, Poland)
    • 13
      CHemical Survey analysis System (CHESS): Similarity Analysis on clusters
      Speaker: John Eduard Martínez Fernández (CAMK-PAN)
    • 14
      Classical Cepheids: Laboratories of Stellar Astrophysics
      Speaker: Felipe Espinoza (CAMK)
    • 11:00
      Coffee break
    • 15
      Athena X-ray telescope and observations of accreting compact objects
      Speaker: Agata Rozanska (CAMK PAN)
    • 16
      The DarkSide program for dark matter searches
      Speaker: Clea Sunny (CAMK PAN)
    • 17
      Searching for Life: The Speculoos Mission
      Speaker: Daniel Grana Ramos
    • 12:10
      Lunch
    • 18
      Ultra Luminous X-ray sources: Numerical simulations of accreting neutron stars
      Speaker: Fatemeh Kayanikhoo (Nicolaus Copernicus Astronomical Center)
    • 19
      Are black hole accretion disks puffy?
      Speaker: Bhupendra Mishra (CAMK)
    • 20
      Numerical simulations of accretion disks and auroras on exoplanets
      Speaker: Miljenko Čemeljić (CAMK & SU & ASIAA)
    • 21
      Numerical simulations of relativistic jets from black holes
      Speaker: Krzysztof Nalewajko (Nicolaus Copernicus Astronomical Center, PAS, Warsaw, Poland)
    • 14:50
      Coffee break
    • 22
      Prof. Belczyński's science
      Speaker: Tomasz Bulik (Obserwatorium Astronomiczne UW)
    • 23
      Multiwavelength Analysis of AFGL 5157 Star Forming Region
      Speaker: Fatima Saiyed
    • 24
      Studying High-Mass Star Forming Regions: Dust Continuum Emission
      Speaker: Mohna Rebecca
    • 25
      Modelling star spots of YSOs using TESS light curves
      Speaker: Nikhil Yadav
    • 26
      Navigating the PhD experience at CAMK, Warsaw
      Speaker: Gonzalo Rojas García (Nicolaus Copernicus Astronomical Centre, PAN)
    • 27
      CAMK Life in Torun
      Speaker: Thomas Steinmetz (Nicolaus Copernicus Centre for Astronomy)
    • 28
      Navigating the Universe: challenges in the standard model of cosmology
      Speaker: Chandra Shekhar Saraf
    • 12:00
      Lunch
    • 29
      KM3NeT: neutrino astronomy and more
      Speaker: Piotr Kalaczyński (AstroCeNT)
    • 30
      Numerical Study of New Dark Force of Dark Matter
      Speaker: Ami Patel
    • 31
      International Astronomy and Astrophysics Competition
      Speaker: Biswaraj Palit (CAMK PAN)
    • 14:20
      Coffee break
    • 32
      Novel detector concepts for future Dark Matter experiments
      Speaker: André Cortez (CAMK PAN)
    • 33
      Never seen before - Gaia binaries and the challenges for the binary evolution models
      Speaker: Iwona Kotko (Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences)
    • 34
      Multi-wavelength Follow ups of Changing-Look and X-ray-Flaring AGN detected using the eROSITA X-ray telescope
      Speaker: Alex Markowitz (CAMK-PAN)
    • 35
      Theoretical Spectral Analysis of Polycyclic Aromatic Hydrocarbons to Investigate Interstellar Dust Features
      Speaker: Venkata Lakshmi Karri
    • 36
      Conclusion
      Speaker: Oliwia Ziółkowska (CAMK)