Team

 

April 2026
Mon Tue Wed Thu Fri Sat Sun
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6 7 8 9 10 11 12
13 14 15 16 17 18 19
20 21 22 23 24 25 26
27 28 29 30
"UNIVERSE+ Online Seminars"

Apr 8, 2026 from 04:00 PM to 05:00 PM (Local Time Germany)

TBA

Apr 9, 2026 from 03:30 PM to 04:00 PM (Local Time Germany)

Registration Deadline – MPCDF Deep Learning Workshop (Extended)

Apr 11, 2026 from 12:00 AM to 01:00 AM (Local Time Germany)

"Fundamentals of Deep Learning"

Apr 14, 2026 from 09:00 AM to 05:00 PM (Local Time Germany)

"CN7 Dust Connector 'Kick Off'"

Apr 16, 2026 from 10:00 AM to 12:00 PM (Local Time Germany)

"From Sand to Silicon – How Modern Microchips Are Made"

Apr 16, 2026 from 12:00 PM to 01:00 PM (Local Time Germany)

"Piercing Deeper Into the Radio Universe - A MeerKAT Perspective"

Apr 16, 2026 from 03:15 PM to 04:15 PM (Local Time Germany)

"What is Life? Perspectives from Biology and Philosophy"

Apr 17, 2026 from 04:15 PM to 05:15 PM (Local Time Germany)

"Antipodal Self-Duality in Planar N=4 and Fishnets"

Apr 21, 2026 from 11:00 AM to 12:00 PM (Local Time Germany)

"A Story of Condensation in Giant Exoplanet Atmospheres"

Apr 21, 2026 from 02:00 PM to 03:00 PM (Local Time Germany)

"A Cosmic Cocktail: From Molecules to Maps"

Apr 21, 2026 from 06:30 PM to 08:30 PM (Local Time Germany)

MPP & MPQ Career Day

Apr 22, 2026

"The Need for High Spectral Resolution in Future Spectroscopic Surveys"

Apr 22, 2026 from 10:00 AM to 11:00 AM (Local Time Germany)

"Intracluster Light as a Dark Matter Tracer in Galaxy Clusters"

Apr 22, 2026 from 11:00 AM to 12:00 PM (Local Time Germany)

"The Radio Properties of Dusty Quasars"

Apr 22, 2026 from 02:30 PM to 03:30 PM (Local Time Germany)

USM Games Night

Apr 22, 2026 from 06:00 PM to 08:00 PM (Local Time Germany)

"The SMBH Factory: Ready, Set, Go"

Apr 23, 2026 from 11:00 AM to 12:00 PM (Local Time Germany)

IMPRS Colloquium

Apr 23, 2026 from 11:00 AM to 01:00 PM (Local Time Germany)

"The First Breath of Rocky Worlds: How Magma Oceans Create Planetary Atmospheres"

Apr 23, 2026 from 12:15 PM to 02:00 PM (Local Time Germany)

"Latest Results from the NIKA2 mm Camera"

Apr 27, 2026 from 11:00 AM to 12:00 PM (Local Time Germany)

"Is There an Ideal Tool to Model Cosmic Reionization?"

Apr 27, 2026 from 03:30 PM to 04:30 PM (Local Time Germany)

"Efficiently Emulating Distribution Functions in Gigaparsec Volumes for Varying Cosmological Parameters"

Apr 28, 2026 from 11:00 AM to 12:00 PM (Local Time Germany)

This event will take place in Room 006.

"Peering Down the Barrel With DESI DR2: 10,000+ Inflows at z < 0.6"

Apr 28, 2026 from 12:00 PM to 12:45 PM (Local Time Germany)

"Novel Forward and Inverse Approaches to Modelling the Observable Universe"

Apr 29, 2026 from 11:00 AM to 12:00 PM (Local Time Germany)

"When is a Quantum Computer Really Quantum?"

Apr 29, 2026 from 01:00 PM to 02:00 PM (Local Time Germany)

"Do Galaxy Mergers Increase Star Formation and Turbulence at Cosmic Noon?"

Apr 30, 2026 from 10:00 AM to 10:30 AM (Local Time Germany)

"How the Atmosphere Determines the Surface Temperature of a Planet"

Apr 30, 2026 from 02:15 PM to 04:00 PM (Local Time Germany)

"Fast and Differentiable Large-Scale Structure Simulations"

Apr 30, 2026 from 03:30 PM to 04:00 PM (Local Time Germany)

"Foreground Biases in kSZ Velocity Reconstruction: Modelling and Mitigation"

Apr 30, 2026 from 04:00 PM to 04:30 PM (Local Time Germany)

X-ray reprocessing: Through the eclipse spectra of high and low mass X-ray binaries with XMM-NEWTON

Sep 4, 2018 11:00 AM - 12:00 PM (Local Time Germany)
MPE, Room: New Seminar Room, 1.1.18b

The NOAO Data Lab - A science platform for the entire astronomical community

Sep 11, 2018 10:00 AM - 12:00 PM (Local Time Germany)
MPE, Room: New Seminar Room, 1.1.18b

Disk Science - Disks at small and large scales

Sep 12, 2018 09:30 AM - 05:20 PM (Local Time Germany)
MPE, Room: New Seminar Room, 1.1.18b

Illustris TNG Science Workshop 2018

Oct 15, 2018 09:00 AM (Local Time Germany) - Oct 17, 2018 05:30 PM
MPA, Room: Large Seminarroom E.0.11

Insights from high resolution (multi-band) spectroscopy - an application to the ejecta of classical novae

Nov 6, 2018 02:00 PM - 03:00 PM (Local Time Germany)
Boltzmannstraße 2, Garching, Room: Cluster building, seminar room, basement

Exoplanets in Ondrejov - ground based support of space missions

Nov 27, 2018 03:00 PM - 04:00 PM (Local Time Germany)
ESO Headquarters, Garching, Room: ESO library (room 365)

Title1: Detecting dark matter substructures using cold stellar streams Title 2: Ab initio hydrodynamical simulations on galactic scales

Jan 15, 2019 11:00 AM - 12:00 PM (Local Time Germany)
MPA, Room: Large Seminar Room E.0.11.

MPE

Project Office  
Richard Davies Principal Investigator (PI)
Empty
Susanne Dengler Project Assistant
Veronika Hörmann System Engineer Construction, Deputy System Engineer
Angela Kleiser Project Assistant
Sebastian Rabien System Engineer (SE)
Eckhard Sturm Project Manager (PM)
Optical Engineering  
Norbert Geis Optical Design
Michael Hartl System Engineer Optics
Mechanical Engineering  
Andreas Emslander Mechanical Engineer
Hans Gemperlein Mechanical Engineer
Frank Haußmann Mechanical Engineer
Heinrich Huber Mechanical Engineer
Andreas Pflüger Engineering, Procurement
Josef Schubert Head of MPE construction (SE until 2019)

A*

João AlvesUniv. Vienna
Wolfgang KauschUniv. Innsbruck
Kieran LeschinskiUniv. Vienna
Norbert PrzybillaUniv. Innsbruck
Ronny RamlauUniv. Linz
Nadeen SabhaUniv. Innsbruck
Miguel VerdugoUniv. Vienna
Roland WagnerUniv. Linz
Werner ZeilingerUniv. Vienna
Bodo ZieglerUniv. Vienna

ESO

Paola Amico
Naidu Bezawada
Florian Kerber
Pierre-Yves Madec
Suzanne Ramsay
Ulf Seeman

FINCA

Tapio HelinLUT Univ.
Jari KotilainenUniv. Turku
Hanin KuncarayakatiUniv. Turku
Seppo MattilaUniv. Turku

MICADO Test (oben): Überschrift extra, Exceltabelle einkopiert (ab Project Office) und in CMS-Tab-Erweiterung umgewandelt - hier dann auf Reiter “Optionen gehen” und “erste Zeile in Überschrift umwandelnt” (ist hier Project Office)
Achtung! Bei ESO hier nur die erste Spalte eingefügt (ohne die 2. leere, hier keine Funktion angegeben)

So jeden Bereich separat eingefügt, anschl. jede Exceltabelle aus HTML löschen!

Obwohl die einzelnen Excel-Tabellen aus der gleichen Tabelle herauskopiert wurden (gleiche Spaltenbreite) wird es im CMS unterscheidlich breit eingefügt.

Vergleich: Tabelle MPE und Tabelle A* => hier ist die erste Spalte breiter. Das sieht man dann in der Großansicht.

 

 

ZZZZZZZZZZZZZZZ

Tabellen unten - sind nur im HTML zu ändern/keine CMS-Tabellen-Erweiterung

MPE
Project Office
Richard Davies Principal Investigator (PI)
Optical Engineering
Norbert Geis Optical Design

 

Name
Type
Groups involved
ATHENA
Instrument for Satellite
High-Energy Astrophysics
ARGOS
Instrument for Telescope
Infrared/Submillimeter Astronomy
ERIS
Instrument for Telescope
Infrared/Submillimeter Astronomy
MICADO
Instrument for Telescope
Infrared/Submillimeter Astronomy

 

Tab1 (unten) : Mechanik/Teslab-Integr/Testlab/Ausstattung => TVK1 / bereits geändert

Allgemein:

Aufnehmbares Volumen (L x B x H):

1450 x 500 x 590 (in mm)

Elektrische Durchführung:

Durchführungen auf Anfrage

Thermaldaten:

Minimaltemperatur:

-50° C

Maximaltemperatur:

+80° C

Temperaturregelung:

Hand- oder Programmbetrieb

Temperatur-Änderungsgeschwindigkeit:

0 - 120 K/h

Temperaturaufzeichnung:

Hybridschreiber mit 19 frei zur Verfügung
stehenden Temperaturmesskanälen und
4 frei zur Verfügung stehenden
Spannungsmesskanälen.

Vakuumdaten:

Vorpumpen:

Wälz- und Hubkolbenpumpe

Hochvakuumpumpe:

Turbomolekularpumpe

Enddruck (leerer Rezipient)

4,0 E - 7 mbar bei 20° C nach 3 Tagen
Pumpzeit

Partialdruckmessung:

Massenspektrometer
bis Masse 100 amu

 

Tab2: Mechanik/Teslab-Integr/Testlab/Ausstattung => TVK2

Allgemein:

Aufnehmbares Volumen (Ø x H):

800 x 1200 (in mm)

Elektrische Durchführung:

Durchführungen auf Anfrage

Thermaldaten:

Minimaltemperatur:

Raumtemperatur (keine Kühlung möglich)

Maximaltemperatur:

+90° C

Temperaturregelung:

Hand- oder Programmbetrieb

Temperatur-Änderungsgeschwindigkeit:

0 - 120 K/h

Temperaturaufzeichnung:

Hybridschreiber mit 10 frei zur Verfügung
stehenden Temperaturmesskanälen und
9 frei zur Verfügung stehenden
Spannungsmesskanälen.

Vakuumdaten:

Vorpumpen:

Spiralvakuumpumpe

Hochvakuumpumpe:

Turbomolekularpumpe

Enddruck (leerer Rezipient)

6,0 E - 7 mbar bei 20° C nach 2 Tagen
Pumpzeit

Partialdruckmessung:

Massenspektrometer
bis Masse 63 amu

Adsorptionsmessung:

TQCM mit 1,96xE-9 g/cm²Hz

 

 

Test: Team-Tabelle für MICADO

 

ElswijkEddyNOVAASTRON
Empty   
KwastSanderNOVAASTRON
JanssenAnnemiekeNOVAASTRON
KunstPeterNOVAASTRON
NavarroRamonNOVAASTRON
PeterzonJan RinzeNOVAASTRON
RompRickNOVAASTRON

 

KravcarHelmutUSMUSM
Lang-BardlFlorianUSMUSM
MonnaAnnaUSMUSM
RichterJosefUSMUSM
SchlichterJörg-UweUSMUSM
ThomasJensUSMMPE
WegnerMichaelUSMUSM
KravcarHelmutUSMUSM
BauerHeinrichUSMUSM
MonnaAnnaUSMUSM
RichterJosefUSMUSM
SchlichterJörg-UweUSMUSM
ThomasJensUSMMPE
WegnerMichaelUSMUSM

 

 

     
 HartlMichaelMPEMPE
 HaußmannFrankMPEMPE
 HörmannVeronikaMPEMPE
 HuberHeinrichMPEMPE
 KampfDirkMPEKTO
 KravchenkoKaterynaMPEMPE
 NeumeierLuisMPEMPE
     
     

 

 

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Alex Agudo Berbel

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