EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 (Nearby) Active galaxies Task manager : Pierre FERRUIT (CRAL)

Slides:



Advertisements
Similar presentations
Multi-long-slit Spectroscopy for Kinematic Studies. I. Implementation and Demonstration Rene A. M. Walterbos, Jiehae Choi, Sophia Cisneros, Maria T. Patterson,
Advertisements

European Southern Observatory European Southern Observatory © ESO 2005 Page 1 AO Department Leiden, April 26th 2005 MUSE M ulti U nit S pectroscopic E.
A detailed 2D spectroscopic study of the Central Region of NGC 5253 Ana Monreal Ibero (1) José Vílchez (1), Jeremy Walsh (2), Casiana Muñoz-Tuñón (3) (1)
Extremely Large Telescopes and Surveys Mark Dickinson, NOAO.
PCA Tomography and its application to nearby galactic nuclei João Steiner IAG - Universidade de São Paulo +R. B. Menezes, T. V. Ricci +F. Ferrari (UNIPAMPA)
The ubiquitous UV murmurs of sleeping supermassive BHs Dani Maoz With: Neil Nagar, Heino Falcke, Andrew Wilson.
Spitzer Reveals Activities of Supermassive Black Holes in Elliptical Galaxies Qiusheng Gu Nanjing University in collaboration with J.-S. Huang (CfA), G.
Mrk334: is a connection between nucleus activity and merging of a companion? Smirnova A.A., Moiseev A.V., Afanasiev V.L. Special Astrophysical Observatory.
Science Group: Status, Plans, and Issues Claire Max Liz McGrath August 19, 2008.
EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 Deconvolution of 3D data cubes Task manager : Pierre Ferruit (CRAL)
Eddington limited starbursts in the central 10pc of AGN Richard Davies, Reinhard Genzel, Linda Tacconi, Francisco Mueller Sánchez, Susanne Friedrich Max.
M77 (NGC 1068) By: Ryan Desautels. Messier 77 A Brief History A Brief History General Information General Information Galactic Information Galactic Information.
Molecular Hydrogen in the outer filaments surrounding NGC 1275 Nina Hatch CS Crawford, RM Johnstone, AC Fabian IOA, Cambridge.
The Dwarf Starburst Galaxy NGC 1705 : New H II Region Element Abundances & Reddening Variations Near the Center NGC 1705 is a nearby dwarf starburst galaxy.
ULTRALUMINOUS INFRARED GALAXIES: 2D KINEMATICS AND STAR FORMATION L. COLINA, IEM/CSIC S. ARRIBAS, STSCI & CSIC D. CLEMENTS, IMPERIAL COLLEGE A. MONREAL,
The Narrow-Line Region and Ionization Cone Lei Xu.
Stellar and Gas Kinematics in the Core and Bar Regions of M100 Emma L. Allard, Johan H. Knapen, University of Hertfordshire, UK Reynier F. Peletier, University.
Mid-IR High Ionization Lines in Starbursts Lei Hao Spitzer IRS Team Cornell University.
Active Galactic Nuclei (or AGN) Seyfert galaxies have very small (unresolved), extremely powerful centers! The strength of the emission lines vary on timescales.
EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 Emission-line fitting Task manager : Pierre FERRUIT (CRAL)
The Milky Way and Other Galaxies Science A-36 12/4/2007.
Quasars and Other Active Galaxies
Andrew Humphrey INAOE Submitted to MNRAS Letters with M. Villar-Martín, S.F. Sánchez, A. Martínez-Sansigre, R. González Delgado, E. Pérez, C. Tadhunter,
1 BDRv3 - November 26, Markus Kissler-Patig E-ELT Programme 1 E-ELT Science Case Markus Kissler-Patig.
Molecular Gas and Dust in SMGs in COSMOS Left panel is the COSMOS field with overlays of single-dish mm surveys. Right panel is a 0.3 sq degree map at.
Observational signatures of gas flows toward the center of galaxies Thaisa Storchi Bergmann Instituto de Física, UFRGS, Brazil Collaborators: Barbosa,
IFU observations of the high-z Universe Constraints on feedback from deep field observations with SAURON and VIMOS Joris Gerssen.
A spectroscopic survey of the 3CR sample of radio galaxies Authors: Sara Buttiglione (SISSA - Trieste), Alessandro Capetti (INAF – Osservatorio Astronomico.
INTEGRAL FIELD SPECTROSCOPY AT THE VLT STAR (CLUSTER) FORMATION IN 3D : INTEGRAL FIELD SPECTROSCOPY AT THE VLT Markus Kissler-Patig (Instrument Scientist.
Euro3D RTN Kick-off Meeting IAC, Tenerife July 2-4, Introduction of FP5: „Improving the Human Research Potential and the Socio-economic Knowledge.
THE HST VIEW OF LINERS AND OTHER LOCAL AGN MARCO CHIABERGE CNR - Istituto di Radioastronomia - Bologna Alessandro Capetti (INAF-OATo) Duccio Macchetto.
Hot gas in galaxy pairs Olga Melnyk. It is known that the dark matter is concentrated in individual haloes of galaxies and is located in the volume of.
Nearby and distant galaxies from ORM and CAHA: the next decade Patricia Sánchez-Blázquez (Universidad Autónoma de Madrid)
Central Engine of AGN Xi’ian October 2006 Black Hole Mass Measurements with Adaptive Optic Assisted 3D-Spectroscopy Courtesy ESO Guia Pastorini Osservatorio.
Do YSOs host a wide-angled wind? - NIR imaging spectroscopy of H 2 emission - 3. Spectro-Imaging using Gemini-NIFS Subaru UM, 1/30/2008 Hiro Takami (ASIAA)
PI Total time #CoIs, team Bob Fosbury 10n (ELT 42m) ~5. Skills: lens modelling, photoionization modelling, massive star SED modelling, practical nebular.
Imaging Molecular Gas in a Nearby Starburst Galaxy NGC 3256, a nearby luminous infrared galaxy, as imaged by the SMA. (Left) Integrated CO(2-1) intensity.
Viewing the Universe. 8Astronomers gather information about objects throughout the universe by detecting various kinds of energy given off by these objects.
Observations of the Large Magellanic Cloud with Fermi Jürgen Knödlseder (Centre d’Etude Spatiale des Rayonnements) On behalf of the Fermi/LAT collaboration.
Dr Katherine Inskip Montse Villar-Martín (IAA Granada) Clive Tadhunter, Joanna Holt, Dan Dicken (Sheffield) Raffaella Morganti (ASTRON) Friday 20 th October.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
Active Galaxies and Supermassive Black Holes Chapter 17.
Nebulae Associated with Ultraluminous X-ray Sources P. Abolmasov, Special Astrophysical Observatory.
Quasars and Other Active Galaxies
Junfeng Wang, G. Fabbiano, G. Risaliti, M. Elvis, M. Karovska, A. Zezas (Harvard-CfA/SAO), C. G. Mundell (Liverpool John Moores University, UK), G. Dumas,
UW SALT Science Update SALT Science Day November 2012.
Probing the nuclear emission structure in the LINER F with the VLTI by Konstantina & Jürgen Abstract: LINER bear an AGN with unusual properties.
A bestiary of QSO/host interactions Y. Letawe 1, P. Magain 1, G. Letawe 1, F. Courbin 2, D. Hutsemékers 1 1 Institut d’Astrophysique.
Crowded Field Spectroscopy CASTLES Crowded Field Spectroscopy B
Radio Galaxies part 4. Apart from the radio the thin accretion disk around the AGN produces optical, UV, X-ray radiation The optical spectrum emitted.
Mapping CO in the Outer Parts of UV Disks CO Detection Beyond the Optical Radius Miroslava Dessauges Observatoire de Genève, Switzerland Françoise Combes.
David R. Law Hubble Fellow, UCLA The Physical Structure of Galaxies at z ~ John McDonald, CFHT Galaxies in the Distant Universe: Ringberg Castle.
Properties of the NLR from Spatially Resolved Spectroscopy Nicola Bennert University of California Riverside Collaborators: Bruno Jungwiert, Stefanie Komossa,
Describing 3D Datasets Igor Chilingarian (CRAL Observatoire de Lyon/Sternberg Astronomical Institute of the Moscow State University) IVOA DM & DAL WG –
UNIVERSIDAD COMPLUTENSE DE MADRID Grupo UCM de Astrofísica Instrumental y eXtragaláctica PRESENTADO POR: Raffaella Anna Marino COLABORADORES: A. Gil de.
Competitive Science with the WHT for Nearby Unresolved Galaxies Reynier Peletier Kapteyn Astronomical Institute Groningen.
Task 2.4 Crowded Field 3D Spectroscopy : goals: “to implement software tools for accurate background subtraction and spectrophotometry of point sources.
Sample expanded template for one theme: Physics of Galaxy Evolution Mark Dickinson.
High Redshift Galaxies/Galaxy Surveys ALMA Community Day April 18, 2011 Neal A. Miller University of Maryland.
Spatially Resolved Spectroscopy ASTR 3010 Lecture 17 Textbook Ch. 11.
Outflows in nearby AGN and their relation with radio jets Thaisa Storchi Bergmann Instituto de Física, UFRGS, Porto Alegre, RS, Brazil Leiden Conference.
The Science Case Hubble Space Telescope CELT+AO HDF.
3D spectroscopy at Paris Obs. (GEPI)
The upgraded HET Hobby-Eberly Telescope Dark Energy Experiment.
Resolving the black hole - nuclear cluster - spheroid connection
MODELS OF EMISSION LINE PROFILES AND SPECTRAL ENERGY DISTRIBUTIONS
Integral Field Spectroscopy
Unusual sites of GRBs in their host galaxies Lise Christensen
The extended HeIIλ4686 emission in the extremely metal-poor galaxy SBS E seen with MUSE C. Kehrig 2018.
Presentation transcript:

EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 (Nearby) Active galaxies Task manager : Pierre FERRUIT (CRAL)

EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 Nearby Active galaxies Goal : conduct one or two scientific programs on nearby active galaxies Goal : conduct one or two scientific programs on nearby active galaxies Careful selection of the scientific goals Careful selection of the scientific goals Well focused program(s) that can produce significant results & publications within ~2 years Well focused program(s) that can produce significant results & publications within ~2 years Involve the post-doc(s), encourage collaborative work between the Euro 3D community Involve the post-doc(s), encourage collaborative work between the Euro 3D community Take advantage of 3D instruments available to the Euro 3D community Take advantage of 3D instruments available to the Euro 3D community Real goal : observe NGC 1068 with every available 3D spectrograph Real goal : observe NGC 1068 with every available 3D spectrograph

EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 Nearby Active galaxies Some possible topics : Some possible topics : The quest for inflow signatures The quest for inflow signatures Little work done so far in 3D (mainly by the Integral group) Little work done so far in 3D (mainly by the Integral group) Compare stellar & gaseous kinematics in the central kpc Compare stellar & gaseous kinematics in the central kpc VIMOS IFU, SPIFFI… VIMOS IFU, SPIFFI… Stellar populations in Seyfert galaxies Stellar populations in Seyfert galaxies History of Seyfert galaxies. Are they different ? Seyfert 1 / 2 ? History of Seyfert galaxies. Are they different ? Seyfert 1 / 2 ? Mainly long-slit work done so far (2 major groups in the world) Mainly long-slit work done so far (2 major groups in the world) IFU with extensive spectral coverage, mounted on a large telescope IFU with extensive spectral coverage, mounted on a large telescope Excitation conditions of ionized gas in Seyfert galaxies with compact radio emission Excitation conditions of ionized gas in Seyfert galaxies with compact radio emission Get rid of the shocks, study photoionization by the active nucleus alone Get rid of the shocks, study photoionization by the active nucleus alone Line ratio diagnostics, spatially resolved information Line ratio diagnostics, spatially resolved information IFU with extensive spectral coverage, mounted on a large telescope IFU with extensive spectral coverage, mounted on a large telescope Others… Others…

EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 Nearby active galaxies Definition of the scientific goals Selection of the best suited instrument(s) Ask for telescope time Get the telescope time Reduce the data Analyse the data / model the object Write the paper Try to initiate the work in september Apply for time as soon as possible Start before the post-doc arrives ?

EURO 3D – Kick Off Meeting – IAC 2-3-4/07/2002 MPE ESO ? LEI ? PAR ? IAC ? CAM ?