GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat Choice of hot and emission stars for GBO(1/7) Objectives: Preparation phase: to develop and to test.

Slides:



Advertisements
Similar presentations
Choosing a Journal APS Professional Skills Course: Writing and Reviewing for Scientific Journals.
Advertisements

3rd Plenary MeetingRA-2/MWR Cross-Cal & Val Team, ESRIN 12/09/01 Third Plenary ENVISAT RADAR ALTIMETRY CROSS-CALIBRATION and VALIDATION TEAM Meeting Jérôme.
CW5 Berlin 12/2003 COROT planet field observations at INT La Palma H.J. Deeg 1, M. Deleuil 2, C. Moutou 2 1 IAC, Tenerife; 2 LAM Marseille - Observations.
Ranking and priorities | | Michael Hilker Ranking of service mode observations and relative priorities Michael Hilker.
Report from IWG on Environmental and Propulsion Performance Requirements for Light vehicles (EPPR) 70 th GRPE th January 2015 Geneva Chair: Petter.
The JMMC softwares to prepare AMBER observations AMBER Workshop - LAOG - 9 Nov 2004.
Extragalactic science with the Herschel Space Observatory Marc Sauvage CEA/DSM/DAPNIA Service d'Astrophysique UMR AIM.
E-content Generation and Delivery Management for Student Centric Learning CONTROL NUMBER : DE Dr DVLN Somayajulu Professor, PI and Institute.
ORDC Phase 2 Analysis Summary Wholesale Market Subcommittee March 4, 2015 David Thompson.
Photometric follow-up of transiting planet candidates Marton Hidas UNSW.
Measuring the Temperature of Hot Solar Flare Plasma with RHESSI Amir Caspi 1,2, Sam Krucker 2, Robert P. Lin 1,2 1 Department of Physics, University of.
Performance Development Plan (PDP) Training
1. 2 Password Verification Valid? No Create/Add AbstractCheck Status & Print Submitted Abstract (Individual or All) Yes.
GHOST, Brussels, Feb.14th The GHOST in CU8 Coralie Neiner Paris-Meudon Observatory GHOST website:
Revisions If you received the grade: “R” If you received the grade: “R” You must do a revision to receive a grade for lab 2. You must do a revision to.
Observational Astrophysics II: May-June, Observational Astrophysics Part II: Observations (5 p) May/June 2004: Rene´ Liseau Magnus.
RECURSIVE PATTERNS WRITE A START VALUE… THEN WRITE THE PATTERN USING THE WORDS NOW AND NEXT: NEXT = NOW _________.
Ground based observations for Gaia 2001 : need to have reference stars to calibrate AP algorithms for Gaia i.e. stars with well-known APs that will observed.
A spectroscopic survey of the 3CR sample of radio galaxies Authors: Sara Buttiglione (SISSA - Trieste), Alessandro Capetti (INAF – Osservatorio Astronomico.
The monitoring of 8.0
Fuerteventura, Spain – May 25, 2013 Physical parameters of a sample of M dwarfs from high- resolution near-infrared spectra Carlos del Burgo Collaborators:
Consortium Meeting La Palma October PV-Phase & Calibration Plans Sarah Leeks 1 SPIRE Consortium Meeting La Palma, Oct. 1 – PV Phase and.
The excess emission in Classical T Tauri Stars Jorge Filipe S. Gameiro DMA, Faculdade de Ciências Universidade do Porto Centro de Astrofísica da Universidade.
Ground Based Observations for the ESP V-1 1.Existing data and catalogues 2.Planned observations 3.Needed observations 4.Telescopes 5.Questions Sources:
The CoRoT ground-based complementary archive The CoRoT ground-based complementary archive Monica Rainer, Ennio Poretti M. Rosa Panzera, Angelo Mistò INAF.
CW9, ESTEC, Dec AP summary Corot Be star group GEPI, Meudon: Hubert, Floquet, Martayan, Frémat, Neiner Univ. Valencia: Fabregat, Gutiérrez-Soto,
The XMM SSC Bright Source sample * November 2006 Report to the SSC XID R. Della Ceca A. Caccianiga T. Maccacaro P. Severgnini F. Cocchia * on behalf of.
OmegaTranS: are we ready? R.P. Saglia, MPE Planets searches using the Transit method Our current and future surveys: WFI, WTS, PanPlanets, OmegaTrans Follow-ups.
PI Total time #CoIs, team Bob Fosbury 10n (ELT 42m) ~5. Skills: lens modelling, photoionization modelling, massive star SED modelling, practical nebular.
CU5-DU13: Ground-based support observations for Gaia absolute photometric calibration BOLOGNA: C. Cacciari, G. Altavilla, M. Bellazzini, A. Bragaglia,
VISTA Hemisphere Survey Dark Energy Survey VHS & DES Francisco Javier Castander.
XMM 1Norbert Schartel Report From The Project Scientist Presentation for the XMM-Newton Users Group Meeting VI 19 th / 20 th May 2005 Norbert Schartel.
PVPhotFlux PACS Photometer photometric calibration MPIA PACS Commissioning and PV Phase Plan Review 21 st – 22 nd January 2009, MPE Garching Markus Nielbock.
June 6-9, 2006COROT Week 10, Nice PMS Thematic Team Activities since CW9 K. Zwintz (Institute of Astronomy, Univ. Vienna, Austria) & members of the PMS.
The Dust Environment of Main-Belt Comet P/2012 T1 (Pan-STARRS) Moreno, F.(1); Cabrera-Lavers, A.(2,3,4); Vaduvescu, O.(2,5); Licandro, J.(2,3); Pozuelos,
Corot Week 61 Targets selection Be stars Paris-Meudon Observatory: A.-M. Hubert, M. Floquet, C. Neiner Univ. of Valencia: J. Fabregat, J. Gutierrez-Soto,
Il ruolo della spettroscopia a grande campo per Gaia B. Bucciarelli - INAF/Osservatorio Astronomico di Torino S. Randich - INAF /Osservatorio Astrofisico.
Chair : M. Deleuil. 3.5º Main target m v  6 Secondary targets m v < 9 Exoplanet field 2.8º N Focal plane:
GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat Algorithms for CU8 (1/10)
PLAnetary Transits and Oscillations of stars Claude CATALA Observatoire de Paris, LESIA Main Science Requirements.
Variable Star Observation
Atmospheric extinction Suppose that Earth’s atmosphere has mass absorption coefficient  at wavelength. If f 0 is flux of incoming beam above atmosphere,
Natal 2004/11/011st Brazil-CoRoT meeting1 Seismology of Be stars with CoRoT Paris-Meudon Observatory: A.M. Hubert, M. Floquet, C. Neiner* Univ. of Valencia:
Natal 2004/11/011st Brazil-CoRoT meeting1 Seismology of Be stars with CoRoT Paris-Meudon Observatory: A.M. Hubert, M. Floquet, C. Neiner* Univ. of Valencia:
Task 2.4 Crowded Field 3D Spectroscopy : goals: “to implement software tools for accurate background subtraction and spectrophotometry of point sources.
The Doppler follow-up of COROT transit candidates F. Bouchy Laboratoire d’Astrophysique de Marseille Corot Week 8 – 23/27 May 2005.
Application of a Charge Transfer Model to Space Telescope Data Paul Bristow Dec’03
Korea Carbon Footprint Labelling and Its Activities June 2009.
FOUR NEW ECLIPSING CATACLYSMIC VARIABLES FROM THE SDSS John Southworth and Boris Gänsicke Department of Physics, University of Warwick, UK
Advanced Topics in Algorithms SPRING TERM PROJECT Is worth 40% of your final grade Completed project with report is due in week th May,
OSIRIS Solar System Simulator
Teacher Evaluation Timeline
The Hubble Legacy Archive (HLA) Slitless Spectroscopy Project
NEON Observing School 2007 Asiago, Italy Gabriel Szász1
CASE-FOMBS Follow-up of One Million Bright Stars
Spectroscopy surveys of stellar populations
Scientific Investigation
Jean-Baptiste Camille COROT ( )
Guideline prepared by the Veterinary Harmonisation Group
Timothy C. Beers University of Notre Dame
The VIMOS IFU Pipeline Carlo Izzo.
How light from the stars can tell us (almost) everything about them!
Corot Be stars group Be stars: The team:
Observational Prospect of NIREBL
Optical cameras (NIRST- HSC) plus DCS & ROSA
Assignment.
The Hertzsprung-Russell Diagram
observations of Dolidze 25
PFIS Commissioning - SSII
Search and Characterization
Presentation transcript:

GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat Choice of hot and emission stars for GBO(1/7) Objectives: Preparation phase: to develop and to test algorithms During the mission: verification and correction … or for pattern recognition algorithms Magnitude range: Mainly V = 10 – 14 Observations type: Photometry, LR spectroscopy, spectrophotometry HR spectroscopy

GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat Choice of hot and emission stars for GBO(2/7) Present status: 2 pilot programs submitted: (for flux calibration) at La Palma (DOLORES, TNG) PI: C.Cacciari Dates: May or June 2007 at Calar Alto (CAFOS, 2.2-m) PI. C.Jordi Dates: May other submission foreseen in spring 2007

Choice of hot and emission stars for GBO(3/7) GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat What is foreseen: Agreement between ESO and ESA for guaranteed observing time Refer to the minutes of the 1 st GBOG meeting: GAIA-C8-MN-L3AB-CS-002

Choice of hot and emission stars for GBO(4/7) GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat Target lists preparation: (GAIA-C8-MN-L3AB-CS-002) FGK-type stars: C.Soubiran A & M stars: A.Lanzafame Ultra cool dwarf stars: D.Barrado Anomalous abundance stars: V.Straizys Hot and emission line stars: GHOST !

Choice of hot and emission stars for GBO(5/7) Target lists – basic rules: 1. First version: no restriction on the number and hemisphere 2. H-R and L-R observations: same list 3. V = 10 – Favor stars with already existing H-R data. 5. Favor “non-variable” and “non-peculiar” stars. Other rules or suggestions ? GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat Participants ? R. Blomme, J.-C. Bouret, Y. Frémat, F. Martins, Liege additions ?

Choice of hot and emission stars for GBO(6/7) GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat More difficult: observations will mainly help to develop the algorithms and to test the models. … pattern recognition algorithms ? Target lists – what basic rules ? 1. First version: no restriction on the number and hemisphere 2. H-R and L-R observations: same list ????? 3. V = 10 – 14 ????????? 4. Favor stars with already existing H-R data. 5. Favor “non-variable” and “non-peculiar” stars ????

Choice of hot and emission stars for GBO(7/7) GHOST #2: Marseille: Nov 13-14, 2006 – Yves Frémat Participants ? (GAIA-C8-TN-OPM-CM-001-1) Meudon Liège Catala ? Acker ?, ROB ? Hutsemakers (liege), Fabrice ?, de koter Lanzafame ?