8:00 |
Breakfast |
9:00 |
Prof. Jσzef
Maslowski (Director of the Astronomical Observatory of the
Jagiellonian University) Welcome address |
9:15 |
Heiko Hafok The new KOSMA 3m radio telescope |
9:30 |
Eduardo Gonzalez-Solares Radio sources in ELAIS
areas |
9:45 |
Yury Romanchev Radiophysical complexes for
cosmic investigations based on Ukrainian radio telescope URAN-3 |
10:00 |
Leszek Blaszkiewicz The
present status of spectral observations in Torun Radio Astronomy Observatory |
10:15 |
Aznaur Botashev Observations of the sample
sources from PMN catalogue on RATAN-600 radio telescope |
10:30 |
Svetlana Veselkova VLBI S/X Cryoreceivers
Research Results |
10:45 |
Vladimir Frolov S2 VLBI-correlator TISS-1M
software |
11:00 |
Coffee |
11:30 |
Wendy Lane Preliminary results of a Westerbork
Survey for moderate redshift HI 21 cm absorption in MgII selected systems |
11:45 |
Noelle Daly Mapping solar wind structure with
interplanetary scintillation |
12:00 |
Vincent de Heij On unravelling the kinematic
structure of Galactic infrared cirrus |
12:15 |
Csaba Kiss Multiwavelength studies of
Khavtassi 15 |
12:30 |
Vincent Minier Methanol survey of the Northern
Galactic plane |
12:45 |
Karl Joulain - Chemistry in dissipative structures
of interstellar turbulence |
13:00 |
Lunch |
15:00 17:00 |
Visit to the Jagiellonian University,
meeting with the university authorities, visit to the Jagiellonian University Museum (Collegium
Maius) |
17:00 - 19:30 |
Visit to the Astronomical Observatory |
19:30 |
Dinner |
8:00 |
Breakfast |
9:00 |
Prof. Richard Wielebinski - The
development of radio astronomy from metre to sub-millimetre wavelengths (invited lecture) |
9:45 |
Indra Bains - Continuum
observations of young planetary nebulae |
10:00 |
Sona Ehlerovα Numerical simulations of expanding shells |
10:15 |
Tomasz Kobak Cosmic ray acceleration in a 3D
magnetic field reconnection volume with turbulence |
10:30 |
Ruslan Shalashov To the question of solving
reverse problems in multifrequent polarimetric studies of interstellar medium |
10:45 |
Ramachandran Rajagopalan Modelling scattering in
the interstellar medium - distances to pulsars |
11:00 |
Coffee |
11:45 |
Kirill Semenkov Simulation of interstellar
scattering effects from compact radio sources |
12:00 |
Tatyana Kaltman 3-dimensional
modelling of solar microwave radio sources of slowly varying component |
12:15 |
Vera Medar Radio observations of the
Coronal Holes with the RATAN-600 radio telescope |
12:30 |
Carla Buemi Radio emission from closed
binary systems |
12:45 |
Sarah Watson MERLIN observations of symbiotic
novae |
13:00 |
Lunch |
14:20 |
Fabrice Herpin On the origin of the
high velocity SiO maser emission from late-type stars |
14:35 |
Volodymyr Koshovy The restoration of
the large scale image of Cas A in decametre waveband |
14:50 |
Bryan Jacoby, Wojciech Lewandowski
and Malgorzata Redmerska Timing and scintillation observations of
pulsars with the TCfA 32-m radio telescope |
15:15 |
Artem Dzura The observations of
methanol quasi-maser emission from star-forming regions at 95 GHz |
15:30 |
Alexander Rodin Astronomical time
scale based on the orbital motion of pulsar in binary system |
16:00 |
Bus departure for city centre |
17:00 18:30 |
Prof. Aleksander
Wolszczan Planety wokσl
innych slonc (Planets of other suns), public
lecture in Polska Akademia Umiejetnosci,
ul. Slawkowska (in Polish) |
19:00 |
Dinner |
8:00 |
Breakfast |
9:00 |
Prof. Aleksander Wolszczan
Applications of pulsar timing (invited lecture) |
9:45 |
Olaf Maron Why is Geminga pulsar radio
quiet at higher frequencies? |
10:00 |
Oleg Malov Observations of Geminga as a radio pulsar |
10:15 |
Alastair McD. Stirling Cygnus X-1, more interesting
than we thought? |
10:30 |
Jόrgen Zweigle CO synthesis images of
a dense torus in the Butterfly nebula M 2-9 |
10:45 |
Carmen Sαnchez Contreras The
asymmetric bipolar flow and the rich molecular content of the protoplanetary nebula
OH231.8+4.2 |
11:00 |
Coffee |
11:30 |
Linda Schmidtobreick UV-Photometry of
dark clouds in The Milky Way |
11:45 |
Victoria Morozova Statistical
properties of interstellar HI clouds |
12:00 |
Bόlent Uyaniker The local magnetic
field in the Milky Way based on 21 cm polarisation mapping |
12:15 |
Thomas Fritz HI synthesis observations
of dwarf galaxies in the Centaurus Group |
12:30 |
Fabian Walter The violent interstellar
medium of the dwarf galaxy IC 2574 |
12:45 |
Robert Rohde Dynamo induced magnetic
fields in spiral galaxies |
13:00 |
Lunch |
14:30 |
Stephen Curran Confirmation of the
molecular ring structure in the Circinus galaxy |
14:45 |
Ilse van Bemmel Nature of the
Far-Infrared Emission in 3C47, 3C207 and 3C334 |
15:00 |
Julia Hutchison The Magnetic Field
Structure of the Jet in Quasar 4C71.07 |
15:15 |
Pekka Heinamaki Black hole ejections
from galaxy nuclei |
15:30 |
Coffee |
16:00 |
Bus departure for city centre |
17:00 18:30 |
Prof. Richard
Wielebinski Niewidzialny Wszechswiat,
czyli co i jak widza radioastronomowie (The invisible
Universe - what does radio astronomy contribute to our knowledge of the Universe), public
lecture in Polska Akademia
Umiejetnosci, ul. Slawkowska (in Polish) |
19:00 |
Conference dinner (in
the city centre) |
8:00 |
Breakfast |
9:00 |
Prof. Marek Urbanik Radio
emission from normal galaxies a key to understand the cosmic magnetism (invited lecture) |
9:45 |
Jacek Niezgoda What Are The Gigahertz
Peaked-Spectrum Radio Sources? |
10:00 |
Marco Pedani Search for ultra steep
spectrum radio sources from a new low-frequency survey |
10:15 |
Izabela Owsianik First detection of
hotspot advance speed in a Compact Symmetric Objects |
10:30 |
Michael Thierbach X-ray properties of
three clusters of galaxies and their implications for the Sunyaev-Zeldovich effect |
10:45 |
Dmitry Krivitsky Quasars in a merger
model: comparison with the observed luminosity function |
11:00 |
Coffee |
11:30 |
Keith Baxter A new model for galactic structure
based upon Percolating Star Formation |
11:45 |
Bong Won Sohn Polarisation properties of radio
galaxies: First sample - 5 low luminosity radio galaxies and 2 giant radio galaxies |
12:00 |
Marek Jamrozy Cosmological evolution
of extragalactic radio sources |
12:15 |
Youri Dabrowski Invisible clusters and
CMB decrements |
12:30 |
Marek Gierlinski Why X-rays are better than radio waves |
13:00 |
Lunch |
15:00 18:30 |
Trip to Wieliczka Salt Mine Museum |
19:00 |
Dinner |
20:00 20:10 |
Krzysztof Chyzy Closing remarks |