24–26 May 2017
Rayong Marriott Resort & Spa
Asia/Bangkok timezone

Session

A10: Astronomy II

25 May 2017, 11:00
Ballroom 2

Ballroom 2

Conveners

A10: Astronomy II

  • Peera Pongkitiwanichakul (Mahidol University)
  • Maneenate Wechakama (Kasetsart University)

Presentation materials

There are no materials yet.

  1. Ms Khemsinan Gunsriwiwat (Chiang Mai University)
    25/05/2017, 11:00
    Astronomy, Astrophysics, and Cosmology
    Oral

    AS Eridani is a 2.664152 day, semi-detached Algol type binary system. Gamarova, Mkrtichian & Kusakin (2000) discovered a short-period 24 min pulsation in a primary mass-accreting component. The oscillation spectrum has been investigated by Mkrtichian et al. (2004), they suggested that AS Eri is a promising pulsating star for further detailed investigations.
    We started a new campaign of...

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  2. Mr Narenrit Thananusak
    25/05/2017, 11:15
    Astronomy, Astrophysics, and Cosmology
    Oral

    We present the technique for selecting high redshift quasar candidates, $z \approx 6 – 11$, suitable for studying the Epoch of Reionization (EoR). Such technique is important for deep and resource-intensive spectroscopic follow-up to confirm the final identification of the sources as well as studying the Inter Galactic Medium (IGM) and its environment. We employ deep optical and near-infrared...

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  3. Sakdithut Jitpienka (The Institute for Fundamental Study, Naresuan University)
    25/05/2017, 11:30
    Astronomy, Astrophysics, and Cosmology
    Oral

    We study non-Gaussianities in primordial perturbations by using the Delta-N approach to avoid the complexity of solving differential equations for non-linear perturbations directly. we have shown, for the case of the double massive inflation with the arbitrary constant metric in the field space, even the mass of two scalar fields are equal, the non-Gaussianity parameter may not vanish....

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  4. Mr Stharporn Sapa
    25/05/2017, 11:45
    Astronomy, Astrophysics, and Cosmology
    Oral

    We consider a cosmological model where the coupling between dark energy and dark matter is motivated by disformal transformation. We consider the case where conformal coefficient depends only on scalar field while disformal coefficient depends both on the scalar field and its kinetic energy. We found that there exist new two classes of fixed point when disformal coefficient depend on both...

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  5. Sean Chen (Andor Technology Ltd., 7 Millennium Way, Springvale Business Park, Belfast, BT12 7AL, United Kingdom )
    25/05/2017, 12:00
    Astronomy, Astrophysics, and Cosmology
    Oral

    Andor is a global leader in the development and manufacturing of high performance scientific imaging cameras, spectroscopy solutions and microscopy systems to match your application needs in research and OEM.
    The prsentation will brief introduce camera technologies, including Electron Multiplying CCD (EMCCD) cameras, Scientific CMOS (SCMOS) cameras, CCD cameras and Intensified cameras .We...

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