The above picture was extracted from the paper: Density structure of prestellar cores seen in absorption with ISOCAM", A. Bacmann et al., presented at "The Universe as seen by ISO" conference, held in Paris, 20-23 October 1998. |
|
ISO observations spatially resolved a variety of objects ranging from planets, circumstellar envelopes, and galaxies, to structures with larger angular sizes like comet trails, interstellar clouds, and star forming regions. It is also possible to investigate the properties of the zodiacal, galactic, and extra- galactic backgrounds since ISO measured the absolute brightness level of the infrared sky.
The analysis of extended sources presents new challenges compared to the analysis of point sources. In most cases, expertise is required in surface brightness calibration, map construction, and source flux extraction to arrive at reliable results and interpretation. Comparison of results with data from other experiments is often highly desirable.
This workshop aims at bringing together scientists, who are working on programmes in which extended emission is important, to exchange results and experiences. Spectroscopy on extended sources is included. We invite participants to give presentations concentrating on the scientific case of their project.
The registration form can be found here and the deadline for abstracts is: August 1, 1999
Registration - until 14:00
19:30 Bus leaves for San Lorenzo de El Escorial
09:00 Bus leaves from San Lorenzo de El Escorial
18:30 Bus leaves for San Lorenzo de El Escorial
09:00 Bus leaves from San Lorenzo de El Escorial
Social Event:
09:00 Bus leaves from San Lorenzo de El Escorial
14:30 Bus leaves from VILSPA
Final Programme
(as of 1st September)
Except for the introduction presented by F. Boulanger (35+10 min), all
scientific presentations will last 20 minutes plus 10 min discussion at
most.
Tuesday 14th September
14:00 - 14:05
Welcome from VILSPA Station Director
V. Claros
14:05 - 14:15
Workshop opening by ISO Project Scientist
M.F. Kessler
14:15 - 15:00
Review: Extended source emission - what has been achieved among infrared instruments
F. Boulanger 1
15:00 - 15:30
ISO, IRAS and COBE/DIRBE surface brightness calibration
K. Lehtinen
15:30 - 16:00
ISO Beamprofiles: Towards extended source calibration
A. Salama
16:00 - 16:30
16:30 - 17:00
The ISO point spread function and CAM beamprofiles
K. Okumura
17:00 - 17:30
ISO LWS Beam Profile and Fringing
C. Lloyd
18:00 - 19:30
Welcome drink and buffet at VILSPA
1reading contribution from J.-L. Puget
Wednesday 15th September
09:30 - 10:00
Aperture photometry with PHT
T. Mueller 2
10:00 - 10:30
Map coadding and simulation techniques with ISOPHOT Interactive Analysis (PIA)
C. Gabriel
10:30 - 11:00
New ISOCAM data reduction techniques for raster imaging of extended emission
M.-A. Miville-Deschenes
11:00 - 11:30
11:30 - 12:00
Object detection and deconvolution: a combined approach
J.-L. Starck
12:00 - 12:30
LWS parallel mode: usage and first results + demonstration
T. Lim
12:45 - 13:00
Workshop Picture and guided tours of the station
13:00 - 14:00
14:00 - 14:30
ISO Observations of the Offset in the Center of Symmetry of the Zodiacal Cloud with respect to the Sun
E. Holmes
14:30 - 15:00
ISOCAM Observations of the Nucleus of Comet Hale-Bopp and of four Short-Period Comets
P. Lamy
15:00 - 15:30
First Maps of Comet Hale-Bopp at 60 and 175 Micron
S. Peschke
15:30 - 16:00
16:00 - 16:30
ISOPHOT Mapping of Vega-type Circumstellar Dust
S. Fajardo Acosta
16:30 - 17:00
Extended IR emission at proximity of Red Giants
T. Le Bertre
17:00 - 17:30
Circumstellar dust around Post-AGB stars
A. Speck
17:30 - 18:00
The ISOGAL Survey
P. Hennebelle
2presented by B. Schulz
Thursday 16th September
09:30 - 10:00
Spectroscopic observations extended emission with ISOCAM
F. Boulanger
10:00 - 10:30
ISOCAM mapping of Galactic cirrus
M.-A. Miville-Deschenes
10:30 - 11:00
Cirrus spectra of low surface brightness regions based on ISOPHOT maps
M. Juvela
11:00 - 11:30
11:30 - 12:00
Far-Infrared Properties of small Scale Cirrus Structure
R.J. Laureijs
12:00 - 12:30
Extended galactic emission and colour variations in the submillimeter range: PRONAOS results
C. Meny
12:30 - 13:00
Large atomic oxygen abundance towards the molecular clouds L1689N and W49N from ISO-LWS observations
E. Caux
13:00 - 14:00
14:00 - 14:30
Far-infrared ISOPHOT observations of globules
K. Lehtinen
14:30 - 15:00
Infrared emission in high mass star forming regions
J. Cernicharo
15:00 - 15:30
ISOCAM Survey of Molecular Cloud: Small Scale Structures and Color Variations of the Emission
A. Abergel
15:30 - 16:00
16:00 - 16:30
FIR mapping of the dwarf irregular galaxy UGCA 86
M. Braun
16:30 - 17:00
Star Formation in a Magnitude-Limited Sample of Spiral Galaxies
G.J. Bendo
17:00 - 17:30
ISO observations of spirals: Modeling the FIR emission
S. Bianchi
17:30 - 18:00
Extended FIR emission in Seyfert galaxies
J. Rodriguez Espinosa
18:00 Excursion to the Deep Space Network station in Robledo de Chavela
21:00 Workshop dinner in San Lorenzo de El Escorial
Friday 17th September
09:30 - 10:00
The Abell 2163 spectrum from infrared to millimeter wavelengths
E. Pointecouteau
10:00 - 10:30
The FIRBACK far-infrared cosmological survey with ISO
H. Dole
10:30 - 11:00
BOOMERANG observations of the CBR
P. DeBernardis
11:00 - 11:30
11:30 - 12:00
Extended foreground emission with Planck
J. Tauber
12:00 - 12:30
Prospects of observing extended emission with FIRST
G. Pilbratt
12:30 - 13:00
Lessons learned for future work: new perspectives from this workshop
13:00
Closing