Talks

NameTitleTime
ALLIK Mohamed LamineContribution of Amateur Astronomers from Bejaia to the Observation of Stellar Occultation by Asteroids in Algeria10 min
BABA AISSA DjounaiThe observation of quadruple-chords stellar occultation on February 18th, 2025 by the trans- Neptunian object (468861) 2013 LU28 in the far southern of Algeria on February 18, 202520 min
BOUDIBA Ghoulam Imad Eddine Exploring the Shape and Size of the Trojan (4709) Ennomos from multiple events stellar Occultation20 min
EBERLE Andreas
GÄHRKEN Bernd, KATTENTIDT Björn Grazing Occultation of Maia at April 1. 202525 min
GÄHRKEN BerndOccultation by Psyche in Algeria at Okt. 8. 202525 min
GUHL Konrad, SCHAFFER FrankImprovment
in VAMOR process
20 min
GUTEKUNST MartinOptimal exposure time regarding the detectability of big dips (>1.5mag)20 min
GUTEKUNST MartinOptimal exposure time regarding the detectability of small dips (<1.5mag)20 min
KATTENTIDT Björn Grazing lunar occultation on 1. May 2025 near Regensburg using 3 different optical systems by comparison30 min
MARTINEZ PatrickESOP 45 in Toulouse
NIKOŁAJUK MarekEclipsing X-ray binaries25 min
PERŁA Julia, MARCINIAK AnnaExpanding Results from Asteroid Shape Modelling Driven by Archival Stellar Occultation Data15 min
PRATT AlexLunar occultations of double stars15 min
SAOULI AdnaneScientific Achievements of Suhail Astronomy Association in Laghouat in Observing Stellar Occultations by Asteroids in Algeria10 min
SCHNABEL CarlesSpanish TSE 2026 from the edges15 min
STOLZEN PeterObservation of the partial solar eclipse on March 29, 2025 on La Palma15 min
VELASCO EnriqueOLED Project – Lunar occultations of double stars30 min
WILAND Janusz47 years of my occultation observations30 min
ZAWILSKI MarekHistorical occultation phenomena observed from the Greater Poland region20 min

Posters

NameTitle
Ellington ChadTrials and tribulations of trying to see PHESAT25 events (??)
Haymes Tim
O’Connell MichaelRemote Observations of Stellar Occultations
Marciniak Anna, Durech Josef, Choukroun Antoine, Perła JuliaAsteroid sizes determined with stellar occultations