Status of the treatments and deliveries

Slides:



Advertisements
Similar presentations
Rate Rhythm P-R Interval QRS Duration P-QRS Ratio Treatment Causes.
Advertisements

First CoRoT International Symposium – Paris – France.
N HD mv SpT Vsini com F2.0 V 10.9 sol-puls (Mosser et al 04) A4.0IV Am A d Scu A2.0 Ap
2009/02/03Meunier et al., Symposium CoRoT EXODAT: Exo-Planet Information System : Evolutions J.-C. Meunier †, M. Deleuil †, C. Moutou †, H. Deeg,
E. Michel COROT, field eval E. Michel COROT, field eval Fields evaluation – CW10 Long Run LR2C RA=18:39:03 ( °) DEC= (6.27 °) ROT=
Annie BAGLIN, CNRS, Observatoire de Paris, SC25th September 24th 2007 Drift or not drift Why a drift of the orbital plane along the right ascension axis.
Oversampling mode Roi Alonso, Pierre-Yves Chabaud Christian Surace, Raphael Cautain, P. Barge.
CCD Imaging of Variable Stars Kimberly Anderson Joshua Smith December 3, 2002.
Thanks to Henrietta Swan Leavitt, Harvard CfA November 5th Hommage to Henrietta Leavitt from the CoRoT Team Annie BAGLIN, Merième CHADID,
Logarithms and The Distance Modulus. Logarithms and Exponents 10 2 = = 1000 Question asked: If you multiply a number by itself a number of times.
Properties of binary systems found in the CoRoT exoplanet search J.M. Almenara, H. Deeg, CoRoT Detection WG, CoRoT Ground-Based Follow-Up WG, Planets in.
Observation of the photocentre position variations with CoRoT - Scientific motivations and expected performance C. Moutou (LAM) – H. Deeg (IAC) – M. Ollivier.
Spectroscopy. Spectroscopy and Star Fingerprints LT: To understand how spectral lines can identify elements in a star. Terms: Spectroscopy – branch of.
PLANET Codes  MTAC. Confirm Reports Delivery vs. Service Goal –Released - October 19 th –Speed – Less than 1 minute; no time-outs –Data – 90 days –Separate.
1Corot Science Week, Berlin, December 2003 Inside the COROT machine Overview of global loop for COROT operations Description of COROT Subsystems.
Trans-Neptunian Objects (TNOs) are the witnesses of the early Solar System and can provide astronomers much valuable knowledge about their formation and.
GROUND BASED OBSERVATIONS of the targets in the SEISMO field Ennio Poretti – INAF-OAB.
PHYS 205 Multiple Star Systems PHYS 205 Binary systems Question: Why are the binaries important?? Answer: They allow us to measure the mass of other.
SKY BACKGROUND CALIBRATION and CORRECTION José Eduardo Costa.
1 Annie BAGLIN, CNRS, Observatoire de Paris, 2005, CW9 AP Short runs in the Anticentre Phase B till March 30th Priorities among AP None yet in the centre……
Measurement of the photocentre position variations with CoRoT - further investigations M. Ollivier (IAS)
Second Grade Word List Second Grade Sight Words. 224.
2nd CoRoT Brazil Workshop Ubatuba, November The scientific Programme Less than one year from launch !
Determinants of Aggregate Demand Aggregate Demand is the total amount of G&S demanded(purchased) by the CONSUMER, BUSINESS, and GOVERNMENT and NET EXPORTS.
E. Michel COROT fields evaluation CW9 12/05 ESTEC E. Michel COROT fields evaluation CW9 12/05 ESTEC Field evaluation: Initial runs.
Looking for exoplanets
Economic Growth in Macroeconomic Models
Validation of N1 Light Curves
Simple Keynesian Model
Shapes of Aggregate Supply
Figure 4 from Characterization of CoRoT Target Fields With Berlin Exoplanet Search Telescope. II. Identification of Periodic Variable Stars in the LRc2.
Observation scheduling
COROT, COnvection, ROtation & Transits exoplanétaires
SHORT-RUN ECONOMIC FLUCTUATIONS
Aggregate Demand and Aggregate Supply
Quick Start Guide for Visual Studio 2010
Supply Shocks AS/AD Model Analysis.
Fabio de Oliveira Fialho Michel Auvergne
Aggregate Demand and Aggregate Supply.
Growth Policy: Why Economic Growth Rates Differ
LRAS & Full Potential Output
Unit 3: Aggregate Demand and Supply and Fiscal Policy
Inflation and Unemployment and the Phillips Curve
Social Research Methods Nonreactive Research and Secondary Analysis
Award Log Number: Award Title PI: Name, Institution, State
Aggregate Supply & Demand Model Part 2
مديريت موثر جلسات Running a Meeting that Works
Reconciling the Models
Some graphs to lecture 8, ch 19 and 20 in IAM.
Update on Status of LIGO
Изразеното в настоящата презентация мнение обвързва единствено автора и не представлява официално становище на Комисията за финансов надзор Данил Джоргов.
The Road to Quality Improvement in HER2-Positive Breast Cancer
Current DAPS Status Observations
Supply Shocks AS/AD Model Analysis.
Shifting Aggregate Supply
The Additional Programme
SHORT-RUN ECONOMIC FLUCTUATIONS
Overall Project RAG Status:
Overall Project RAG Status:
SOME IMPLICATIONS FOR FUTURE CoRoT POINTINGS
Some preliminary results from the exochannel
Unit 3: Aggregate Demand and Supply and Fiscal Policy
AS/AD Model: from the short run to the long run Or… the economic shifty-shift AP/IB Economics.
(A) Absolute and (B) change from baseline in 6 min walk distance over time for all patients and by Down syndrome status. (A) Absolute and (B) change from.
Award Log Number: Award Title PI: Name, Institution, State
25th Scientific Committee
QUESTION #1 1b) Both Prices & Wages are sticky in the short run which causes QTY supply to rise as inflation Examples Price Level ↑ => nominal prices.
Business Cycle Chapter 9 - Witte Short-run booms and busts See Data
Conclusions 1 Building the observing programme
The Scientific Method.
Presentation transcript:

Status of the treatments and deliveries Sylviane Chaintreuil

Status and planning LRc07 20 06/04/2011 28/06/2011 84 82 Run code Run nb Begins (data) Ends (data) Duration seismo data Duration exo data Released LRc07 20 06/04/2011 28/06/2011 84 82 S : 04/04/2012 E : 17/01/2012 SRc03 21 01/07/2011 05/07/2011 5 Planned 22/05/12 Planned 10/05/12 LRc08 22 06/07/2011 30/09/2011 88 86 E : 13/03/2012 SRa04 23 28/11/2011 56 53 Planned 03/05/12 SRa05 24 29/11/2011 09/01/2012 41 39 E : 24/02/2012 LRa06 25 10/01/2012 29/03/2012 80 78 LRc09 28 10/04/2012 S.Ch. - CoRoT SC43 - 18/04/2012

Re-processing in progress Line of sight and light curves are re-produced Some runs were asked for : LRa03, LRa04, LRa05, LRc03 Other runs will follow S.Ch. - CoRoT SC43 - 18/04/2012

Re-observations Stars must be well identified before the observation It is not possible to change the CorotID when the observation has begun The instrument was not designed to have absolute measurements It is very difficult to compare absolute intensities between two observations S.Ch. - CoRoT SC43 - 18/04/2012