"Testing Cosmological Models with Galaxy Clusters"

(Structure and some content shamelessly poached from the Ringberg Starbursts workshop 2000)


Schloss Ringberg (Ringberg Castle), Bavaria, Germany

12 - 16 January 2003


email: ringberg03@mpe.mpg.de

URL: www.xray.mpe.mpg.de/ringberg03

This page is an information support service provided by the scientific and local organizing committees. Visitors are referred to the MPE disclaimer/impressum. This page last updated: 23/01/2003


Current Release: 23/01/03: Powerpoint [.ppt], Acrobat [.pdf] and/or Postscript [.ps] files are now appearing in support of contributions...

Thanks to all who attended and helped to make the workshop such a success!


Contents...

Description of the workshop (as it appears in the second announcement)

Scientific Organizing Committee (SOC)

Local Organizing Committee (LOC)

Invited Participants

Venue

Program

Travel Arrangements

Maps

Visas

Accommodation & Meals

Social events

Weather


Description of the Workshop...

The aim of the workshop is a concentrated discussion (i) how X-ray galaxy clusters are best to be used for testing cosmological models in all relevant steps of the observation and modeling, (ii) of the state of the present results, as well as (iii) of the future prospects of observational cosmology with upcoming surveys or surveys to be proposed. Current results on cosmological parameters that are achieved with galaxy clusters studies are very promising and are rivaling the model constraints obtained with CMB and distant supernova observations. This is calling for a higher awareness for accuracy and methodological problems to fully exploit the cosmological potential of cluster observations. The current literature is not reaching a sufficiently good consensus in the methods and results. Thus it is the primary goal of the workshop to improve this situation. In addition the workshop should provide new emphasis on galaxy cluster surveys as an absolutely essential contribution to observational cosmology.

The workshop will therefore consist of very focussed reports contributing to the subject and discussion sessions devoted to working out a consensus on methodology and marking future tasks. The reports and discussions will be divided into 4 different topics:

1) Observations and modeling of the cluster abundance and evolution

2) Measuring the large-scale structure with X-ray clusters

3) Testing cosmological models and future prospects

4) Internal cluster evolution and link between observable and basic cluster parameters

Members of the SOC are assigned to the sessions to compile a focussed set of reports from participants and prepare the discussion sessions. We plan to produce proceedings which should not only contain scripts of the reports but also summaries and recommendations for all 4 main topics worked out by
those responsible for organizing the discussion (asking for help from participants if relevant).

The participation to the workshop is quite limited since we can only accommodate about 50 participants. Therefore participation is by invitation only. We have no funds to support the travel or accommodation costs. Full board loging at the castle is currently 90 EUR per day. But there is also no conference fee!

We plan to have of the order of 30 talks and to be very selective in the sense how the talks are contributing to the discussion of the various topics. But everybody is involved in the discussion sessions where also short contributions are welcome and needed.

...this description is reproduced from the second announcement.

Scientific Organizing Committee (SOC)...

Name Indication (percentage) attendance probability
S. Borgani 100
H. Boehringer 100
R. G. Bower 100
C. A. Collins 100
L. Guzzo 100
A. E. Evrard 100
J. P. Henry 100
T. Ponman 100
P. Rosati 100
P. Schuecker 100
M. White 100

 Local Organizing Committee (LOC)...

Name Indication (percentage) attendance probability
S. Ettori 100
A. Finoguenov 100
M. Giradi 100
P. Lynam 100
K. Matsushita 100
C. Mullis 100
N. Nowak 100
K. Pedersen 100
P. Popesso 100
J. Retzlaff 100
L. Tornatore 100
P. Tozzi 100
R. van der Weygaert 100
M. Zimer 100
Y. Zhang 100

Invited to Participate...

Name Attendance Status
S. Allen 100
M. Arnaud 100
M. Balogh 100
C. Baugh 100
U. Briel 100
S. De Grandi 100
K. Dolag 100
S. Kay 100
R. Kneissl 100
P. Mazzotta 100
C. Miller 100
J. Mohr 100
L. Moscardini 100
A. Ortiz-Gil 100
U. Pen 100
E. Pierpaoli 100
T. Reiprich 100
A. K. Romer 100
M. Schulze 100
R. Sheth 100
V. Springel 70 ?
Y. Suto 100
N. Tormen 100
P. Viana 100
M. Voit 100
X.P. Wu 100

Venue...

The venue for the workshop is the Schloß Ringberg (Ringberg Castle), a turn of the century castle located in the foothills of the Bavarian Alps, and overlooking the Tegernsee. Located about 70 km south of Munich, the Tegernsee is a beautiful lake surrounded by mountains and small resort villages. The peaceful location, meeting schedule, and attendance limit of 65 set by the size of the castle are all conducive to an informal workshop atmosphere offering many opportunities for stimulating discussion. The scientific sessions will begin on Monday, 13 January 2002 at 9 AM, and end on Thursday evening, 16 January 2002 --- although participants are welcome to stay overnight Thursday in the castle and depart on Friday morning if more convenient.
 

Program...

The following preliminary program is in an evolving state and is aimed primarily for the attention of the SOC. The original text version of this program and associated comments was circulated by electronic mail on Friday 22 November 2002. This program was edited further Monday 02 December 2002. Latest version is that of 08 January 2003. Note that the times for talks are full talk times. The time for the discussion is not counted.
 
Sunday January 12...
Arrivals in the Afternoon

 
 
Monday January 13...
MORNING SESSION: 09:00 - 12:30 (135/210 min.) X-ray Cluster Abundance and Evolution
Pat Henry   [pdf] 30 min. X-ray Cluster Abundance & Evolution
Chris Mullis 15 min. Evolution in Cluster Abundance based on the final ROSAT 160 square degree survey
Chris Mullis (for Harald Ebeling) 5 min. The MACS Project
Piero Rosati 30 min. X-ray Cluster Evolution to High Redshift (Discussion)
~~~ C O F F E E ~~~
~~~ 30 min. ~~~
~~~ C O F F E E ~~~
Kathy Romer   [.ppt]   [.pdf] 20 min. ACBAR Distant Cluster Survey (SHARC?)
Thomas Reiprich 15 min. The Local Galaxy Cluster Abundance, systematics in the X-ray luminosity-mass relation, and cosmological constraints
SDSS Cluster Abundance


Chris Miller 20 min. The Spectroscopic SDSS Cluster Survey

~~~ L U N C H ~~~ L U N C H ~~~ L U N C H ~~~

AFTERNOON SESSION: 14:00 - 18:00 (180/240 min.) SDSS Cluster Abundance - continued
Gus Evrard (for Risa Wechsler)   [.ppt]   [.pdf] 15 min. Calibrating the Mass Function of Galaxy Clusters in the SDSS
Large Scale Structure Traced By Clusters
Carlton Baugh 30 min. Using Galaxy Clusters to Probe the Large Scale Structure of the Universe
Peter Schuecker 30 min. Cosmology from the Large Scale Distribution of X-ray Clusters
~~~ C O F F E E ~~~
~~~ 30 min ~~~
~~~ C O F F E E ~~~
Paul Lynam 15 min. BCGs and Cluster Streaming Flows
Rien van der Weygaert 15 min. Local Supercluster Dynamics
Joerg Retzlaff 15 min. Status and Prospects of the XMM-LSS Galaxy Cluster Survey.
Luigi Guzzo 30 min. Special Lecture:
The VIRMOS VLT Deep Survey
Discussion 1: Chair: Chris Collins, Luigi Guzzo, Peter Schuecker 30 min. Discussion on Large Scale Structure Traced by Clusters.

~~~ D I N N E R ~~~ D I N N E R ~~~ D I N N E R ~~~

EVENING SESSION: 20:00 - 21:00 

Discussion Session on Possible Large Survey Programs with CHANDRA and XMM

Discussion on a Proposal of a CHANDRA L.P. (initiative by J. P. Henry)

Discussion on a Proposal of an XMM-Newton L.P. (initiative by H. Boeringer)


 
Tuesday January 14
MORNING SESSION: 09:00 - 12:30 (140/210 min.) Galaxy Clusters in Cosmological Simulations
Gus Evrard   [.ppt]   [.pdf] 30 min. Cluster and LSS simulations
Martin White   [.pdf] 30 min. Finding Galaxy Clusters in Simualtions and Reality
Testing Cosmological Models with Cluster Observations
Elena Pierpaoli   [.ppt]   [.pdf] 20 min. Systematics in the Determination sigma_8/Omega_m fromX-ray Cluster Abundance.
~~~ C O F F E E ~~~ 
30 min.
~~~ C O F F E E ~~~
Hans Boehringer  25 min. Modelling the REFLEX Cluster Abundance
Steve Allen 20 min. Cosmological Constraints from X-ray and Lensing Observations of Galaxy Clusters
Steffano Ettori 15 min. Constraining the Cosmological Parameters with the Gas Mass Fraction in Local and z > 0.7 Galaxy Clusters

~~~ L U N C H ~~~ L U N C H ~~~ L U N C H ~~~

AFTERNOON SESSION: 14:00 - 18:00 (180/240 min.) Theory of Cosmological Model Tests with Clusters

Yasushi Suto   [.ppt]   [.pdf] 30 min. Reliability of Galaxy Clusters as Cosmological Probes
Joe Mohr   [.pdf] 30 min. Prospects for Studying Dark Energy with Cluster Surveys: The Importance of Cluster Structural Evolution
Discussion 2: Chair: Gus Evrard, Martin White 30 min. Clusters in Simulations
~~~ C O F F E E ~~~ 30 min. ~~~ C O F F E E ~~~
Discussion 3: Chair: Piero Rosati, Pat Henry, Peter Scheucker 45 min. Galaxy Cluster Surveys
Discussion 4: Stefano Borgani, Hans Boehringer, Gus Evrard 45 min. Testing Cosmological Models with Galaxy Clusters 

~~~ D I N N E R ~~~ D I N N E R ~~~ D I N N E R ~~~

(POSSIBLE) EVENING SESSION: 20:00 - 21:00

Further definition of the CHANDRA and XMM-Newton Proposals

Possibility for other special discussion sessions


 
 
 
 
Wednesday January 15...
MORNING SESSSION: 09:00 - 12:30 (165/210 min.) S-Z Effect Observations of Clusters
Rueduger Kneissl 25 min. Expectations for cosmological constraints from future Sunyaev-Zel'dovich cluster surveys
Cluster X-ray Observations I: Temperature structure and metallicity
Monique Arnaud 25 min. Structural and scaling properties of X-ray clusters from XMM observations
~~~ C O F F E E ~~~
~~~ 30 min ~~~
~~~ C O F F E E ~~~
Paolo Tozzi 15 min. Thermodynamical properties of the ICM at high redshift
Pasquale Mazzottta 15 min. Cold Fronts and Hydrodynamic Instabilities in clusters: the Chandra view
Sabrina De Grandi   [.ppt]   [.pdf] 15 min. On the Iron Content In Nearby Galaxy Clusters
Cluster X-ray Observations II: Groups and Entropy Structure
Trevor Ponman 25 min. Scaling and Entropy in Groups and Clusters
Alexis Finoguenov 15 min.
Further Cluster Studies
Marisa Giradi 15 min. Cluster Mass Determination from Optical Data
Kyoko Matsushita   [.ppt] 15 min. Gravitational Mass Profile of Elliptical Galaxies at the Center of Clusters.

~~~ LU N C H ~~~ L U N C H ~~~ L U N C H  ~~~
 

~~~ FREE AFTERNOON ~~~

 
 
 
Thursday January 16...
MORNING SESSION: 09:00 - 12:30 (170/210 min.) Cluster ICM Structure Theory - continued
Marc Voit   [.ppt]   [.pdf] 30 min. Intracluster Entropy
Richard Bower 30 min. TBD
Xiang-Ping Wu   [.ppt]   [.pdf] 20 min. Non-gravitational Effect and the soft X-ray background
Michael Balogh   [.ppt]   [.pdf] 20 min. Evidence for non-gravtiational heating from SZ observations
~~~ C O F F E E ~~~
~~~ C O F F E E ~~~
~~~ C O F F E E ~~~
Scott Kay   [.ppt] 20 min Cooling and Feedback in X-ray Groups and Clusters
Stefano Borgani   [.ps] 30 min. TBD
Lauro Moscardini 20 min. Modelling the ICM and the Dark Matter Distribution in High Resolution Simulations

~~~ L U N C H ~~~ L U N C H ~~~ L U N C H ~~~

AFTERNOON SESSION: 14:00 - 18:00 (140/240 min.)
Ue-Li Pen   [.ppt]   [.pdf] 30 min. Special Lecture:
Sigma_8 and Omega_m from weak Lensing
Discussion 5: Chair: Trevor Ponman, Richard Bower, Stefano Borgani 60 min. Problems in our knowledge of the cluster structure relevent for Cosmological Model Testing.
Future Prospects of Cosmological Studies with Clusters
Pedro Viana 20 min. XCS: Current Status and Future Prospects
~~~ C O F F E E ~~~
~~~ 30 min. ~~~ ~~~ C O F F E E ~~~
All
60 min.
Summary Discussion

~~~ END OF MEETING ~~~


 
 
 
Posters...
Amelia Ortiz-Gil   [.pdf] The LX-sigma relation in REFLEX

 
 
 
 

Notes on the discussion sessions:

Here we have prepared a list of major questions to help you to prepare for the discussion sessions. The questions are only meant as a guide and should not be seen as exclusive. We need to discuss everything that is related to the topic of the conference: what do we need to know to use clusters for the test of cosmological models, how precisely do we know it, what can we do to improve our knowledge.

Discussion 1 (30min) Discussion 0n Large-Scale Structure Traced by Clusters

  - What is the current status of the LSS measurements ?

  - Do clusters selected in different wavelength ranges trace the same
    structures ?

  - What are the merits of different statistics to assess the LSS,
    what is exactly probed by the different means ?

  - What are the major uncertainties in the statistical estimates and
    how are they controlled ?

  - What are the necessary corrections to go from
    observations to the dark matter power spectrum ?

 - How are different statistics best combined ?

  - Can we reproduce the mass/X-ray luminosity dependent biasing, can
    we test the biasing ?

 Discussion 2 (30min) Clusters in Simulations

  - What can we learn from simulations, how accurately are the tests
    based on current simulations, how far can we go with semi-analytic models ?

  - What is the correct recipe to interpret the observational data in
    terms of cluster mass selected tracer samples ?

  - How much do we have to worry about the effect of different cluster
    finding algorithms ?

 Discussion 3 (45min) Galaxy Cluster Surveys

  - How do we define clusters in the X-rays (optical), what is the
    influence of the definition on the selection function, how well do
    we understand the selection function ?

  - What is the current status of the cluster abundance measurements,
    for the X-ray luminosity function, for the temperature function,
    for other means of selection ?

  - What do we know about cluster evolution in X-rays ?

  - How do we relate measured selection parameters to cluster mass,
    and what is the influence of this relation on the results ?

  - Do we have to worry when we combined the results of different surveys
    in e.g. studying selection effects if different cluster sampling and
    flux measuring methods have been used ?

The Future of Cluster Surveys

  -  What cluster surveys are planned for the future ?

  -  What prospects has a future X-ray cluster survey mission ?

  -  What are the prospects of non-X-ray cluster surveys  (in
     particular Sloan, SZ) ?

 Discussion 4 (45min) Testing cosmological models with galaxy clusters

  - What are the most important statistical and systematic
    uncertainties and what should we do to minimize them ?

  - What are the requirements for a representative sample ?

  - What is the strength of clusters as cosmological probes and how
    do they compete with or complement other cosmological measurements ?

  - What is the range of cosmological models/parameters to be tested ?

 Discussion 5  (60min) Problems in our knowledge of the cluster structure relevant for cosmological model testing

  -  What is the relation of scaling relations and internal structure ?

  -  What can we learn from the "scatter" in the cluster scaling relation ?

  -  How can we model cluster structure evolution with preheating and
     cooling models ?

  -  How reliable are cluster mass measurements and the models of
     cluster mass profiles ?

  -  Is the influence of cluster mergers a large uncertainty ?

  -  Can the structure of individual clusters be related to their
     evolutionary history ?

  -  How and why are cluster properties related to the galaxy contents ?
 
 

Travel Arrangements...

Travel to Schloß Ringberg: Participants are requested to travel from Munich, into the Bavarian pre-alps by rail to Tegernsee, from where we plan to have a mini-bus to ferry participants from the railway station at Tegernsee to Ringberg Castle on Sunday and Monday. Similar arrangements will be made for the return connections from Thursday afternoon and Friday morning. The trip by rail from Munich to Tegernsee will take about one and a half hours. The minibus shuttle between Tegernsee and Ringberg will take ~20 minutes. Earliest possible arrival at the castle is 15:00 on Sunday 12 January. For this reason we shall request that all participants forward details of their flights and anticpated rail connections to Tegernsee in an ASCII form to be submitted by e-mail with the subject title "ringberg form"to: ringberg03@mpe.mpg.de

Arriving in Bavaria by air: The Munich Franz-Josef Strauss Airport (MUC) lies approximately 17 km and 30 km north-east of Garching and Munich, respectively. Most major carriers offer service to Munich, although often with stopovers involved on the more distant (North American, for example) routes. There are many cheap fares available if you shop around, and these will normally require staying over one Saturday night. For participants arriving in the area already on Friday or Saturday the LOC can recommend and attempt to arrange for hotel accommodations in Munich.

Arriving in Bavaria by train and airport train transfers: Munich's main train station (Muenchen Hauptbahnhof, map here) can be reached from anywhere within Europe. From here, there are good public transportation connections to all of Munich. There are even railway connections to Tegernsee, in the vicinity of Schloß Ringberg.

Train connections between:

1) Munich Airport (Flughafen Muenchen) and Munich main train station (Muenchen Hauptbahnhof, abbreviated as Muenchen Hbf), using the S1 or S8 metro (.pdf file) lines;
2) Munich main train station (Muenchen Hauptbahnhof, abbreviated as Muenchen Hbf) and Tegernsee, using the BOB trains;
3) Munich Airport (Flughafen Muenchen) and Tegernsee (with one change at Donnersburgerbruecke from S1 or S8 metro (.pdf file) lines to the BOB train).

can be investigated using the German railways (Deutsche Bahn, DB) web-based travel service. When using the English version of this service, the entries to use are: "Munich Airport", "Munich" (for the main train station) and "Tegernsee".

Alternatively, we have text files of:

Timetable for outbound trains from Munich main train station (Muenchen Hbf.) to Tegernsee for Sunday afternoon and evening 12 January 2003;
Timetable for return trains from Tegernsee to Munich main train station (Muenchen Hbf.) for Thursday evening 16 January 2003;
Timetable for return trains from Tegernsee to Munich main train station (Muenchen Hbf.) for Friday morning 17 January 2003.

Note that in all cases, you will need to buy the appropriate ticket for your journey at the airport ticket desk (Fahrscheine) before descending to the platform and boarding the train. Further details regarding travel to Ringberg from Munich airport (in particular about navigating through Munich central train station) are available in the Arriving at Schloss Ringberg page, however we reproduce some useful maps below for convenience.

Airport bus transfers: Alternatively, and possibly more useful for those who plan to spend some days in downtown Munich before or after the Ringberg workshop, there is a "Lufthansa Airport Bus" coach service which collects passengers outside terminal A  (every 20 minutes between 06:17 and 21:37, daily); terminal D (every 20 minutes between 06:25 and 21:45, daily) and the central area, Z (every 20 minutes between 06:20 and 21:40, daily) of Munich Airport. This service goes direct to Munich main train station in circa 45 minutes, stopping once en route at Nordfriedhof U6 metro station in the Schwabing district, North of Munich. Return journeys operate at simlar frequency. Adult single: 9 Euro. Adult return 14.50 Euro.

Arriving in Bavaria by car:

WARNING: Those intending to drive to Tegernsee are recommended to have winter tyres fitted (and if possible to carry snow chains). In particular, drivers of rented vehicles should request that winter tyres are fitted to the vehicle and inform the renting company that you plan to drive in the Tegernsee area. The Bavarian Police ran a pre-Christmas campaign of random spot-checks on vehicles in this area. While most of the main routes are kept clear, snow is lying in the Tegernsee area and fresh snow falls almost daily. The most trecherous part of the journey is likely to be the final ascent of the forest road from the main road in Tegernsee to the Castle. It is here that you should exercise extreme caution and be aware that vehicles may be descending. If you have problems getting up to the castle due to snow or ice (it should not be too bad, but be cautious) you can also leave your car at the parking lot at the bottom. Drive in about 50 m into the private castle road and you will find a space to your right. Walking up could take up to 20 min, not necessarily recommended with luggage. Inform us that you are there and the shuttle will pick you up as soon as possible. Don't forget to note down the cellular phone number.

Schloß Ringberg is located about 70 km SE of Munich. For those interested in driving directly to the castle on Sunday,  12 January the LOC can send out detailed maps and instructions in advance of the workshop. Most major car rental companies have branches at the Munich Airport. Cars usually need to be reserved in advance, and rates are often more favorable if the cars are booked by an overseas travel agent. There is ample parking at the castle, and at the hotels in Kreuth and Rottach-Egern near the castle. For those staying in Munich either before or after the workshop, note that parking can be a problem there and is often quite expensive as well. For those who wish to drive their own cars, maps of the Munich and Tegernsee areas are provided below.
 

Maps...

Map 1: Munich area to Tegernsee area by road...

Map 2: Location of Schloss Ringberg in Tegernsee area...


Visas...

For those participants from countries requiring a visa to enter Germany, it is best to start the application procedure several months before the workshop. Please check with your local German Consulate or travel agent for information about required travel documents.

Accommodation & Meals...

During the workshop, many participants will be lodged at Ringberg Castle. The castle has 34 bedrooms, 7 of which can be used as doubles. Since, at full capacity, the castle can lodge only 40 people, it will be necessary for some participants to stay in hotels in the nearby villages of Rottach-Egern and Kreuth. The cost for the 5 night stay at the Castle including all meals except Sunday and Wednesday dinner will be about Euro 450 per person. For participants and accompanying persons staying in hotels, it may be possible to take lunch and dinner at the castle for a cost of about Euro 10 per meal. However, there is a maximum limit of 65 people imposed by the dining room at Ringberg, so that it may not be possible to accommodate all accompanying persons for all meals. Special dietary requests are happily accommodated provided advance notice is given. If you have any requests (e.g. vegetarian meals) please indicate this on the ASCII form.

The LOC will make arrangements for lodging during the conference for all participants and their accompanying persons, as desired. We will do our best to adhere to everyone's wishes. Due to the limited recreational facilities up at Schloß Ringberg, those travelling with accompanying persons and/or families will may be lodged in hotels in the villages below the Castle. The room rates in the village hotels range from about Euro 70 to Euro 110 per night for the cheapest single and the most expensive double, respectively, including breakfast. Daily transportation from the village hotels to the castle (about a 10-15 minute drive) will be provided by the LOC.

For participants wishing to stay in Bavaria before/after the Ringberg workshop, the LOC can recommend and attempt to assist with booking accommodation. Please do not hesitate to contact us with any requests. Unfortunately, we cannot make reservations for extended side trips. Room rates for hotels in the Munich/Garching area range from Euro 90-220 for singles or doubles.

Credit cards are now accepted at most hotels including Ringberg Castle. We will notify you if there are exceptions to this. Participants should indicate all their lodging preferences on the ASCII form.

Social Events...

  1. Possibly an excursion in the Alps for interested participants and their guests on the free afternoon, depending on the weather. However, it should be emphasized that the weather is not particularly inviting for hiking in January, and those interested in hiking should bring appropriate cold and wet weather gear. If you like to go hiking on the Wednesday afternoon (we will probably guide two tours) please bring your hiking boots and light winter gear. There will be some but probably little snow. An alternative may be a visit to Tegernsee village or an excursion to a place of local interest, depending on the weather.

Weather...


Bavarian weather in the winter is usually crisp with daytime highs around 3° C (??° F) and nighttime lows near -10° C (??° F). Of course, this being central Europe, one should always be prepared for rapid weather changes and rain, especially for the outing in the mountains.


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