Jun 20 – 24, 2022
APC laboratory, Université Paris Cité
Europe/Paris timezone

Session

Time Domain Astrophysics

Jun 21, 2022, 11:25 AM
Buffon Amphitheater (APC laboratory, Université Paris Cité)

Buffon Amphitheater

APC laboratory, Université Paris Cité

Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris

Presentation materials

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  1. Konstantin Malanchev (University of Illinois at Urbana-Champaign)
    6/21/22, 11:25 AM
    Time Domain Astrophysics
    Talk
  2. Helen Qu (University of Pennsylvania)
    6/21/22, 11:45 AM
    Time Domain Astrophysics
    Talk
  3. Prof. Victoria Ashley Villar (Penn State university)
    6/21/22, 2:15 PM
    Time Domain Astrophysics
  4. Paula Sanchez Saez (European Southern Observatory (ESO))
    6/21/22, 3:15 PM
    Time Domain Astrophysics
    Talk
  5. Emille Ishida (Universit ́e Clermont Auvergne, CNRS/IN2P3, LPC)
    6/21/22, 3:35 PM
    Talk
  6. Helen Qu (University of Pennsylvania)
    Time Domain Astrophysics
    Talk

    The use of type Ia supernovae (SNe Ia) as standardizable candles led to the Nobel Prize-winning discovery of the accelerating expansion of the universe and cemented their role in the quest to understand the nature of dark energy. Accurate cosmological parameter estimation requires a sample of pure SNe Ia with minimal non-Ia contamination, but supernova type confirmation using spectroscopy is...

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  7. Dr Emille Ishida (CNRS/LPC-Clermont)
    Time Domain Astrophysics
    Talk

    In order to explore the potential of adaptive learning techniques to big data sets, the SNAD team used Active Anomaly Detection (AAD) as a tool to search for new supernova (SN) candidates in the photometric data from the first 9.4 months of the Zwicky Transient Facility (ZTF) survey – between 2018 March 17 and December 31 (58194 ≤ MJD ≤ 58483). We analyzed 70 ZTF fields with high galactic...

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  8. Paula Sanchez Saez (European Southern Observatory (ESO))
    Time Domain Astrophysics
    Talk

    The classic classification scheme for Active Galactic Nuclei (AGNs) was recently challenged by the discovery of the so-called changing-state (changing-look) AGNs (CSAGNs). The physical mechanism behind this phenomenon is still a matter of open debate and the samples are too small and of serendipitous nature to provide robust answers. In order to tackle this problem, we need to design methods...

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  9. Dr Konstantin Malanchev (University of Illinois at Urbana-Champaign)
    Time Domain Astrophysics
    Talk

    Modern large scale astronomical surveys scan wide areas of the sky following a predetermined cadence. As a result, their data sets contain records of both, known and unknown (or not yet observationally confirmed) astrophysical phenomena. Such datasets hold an immense potential for discovery, however, their volume and complexity makes successfully identifying such events a far from trivial...

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