Statistics of galaxy groups in ultraDeep XMM surveys Alexis Finoguenov Max-Planck Institut fuer extraterrestrische Physik University of Maryland, Baltimore.

Slides:

Advertisements

Similar presentations

HI Stacking: Past, Present and Future HI Pathfinder Workshop Perth, February 2-4, 2011 Philip Lah.

Advertisements

1 COSMOS Dark Matter Maps with COSMOS Jason Rhodes (JPL) January 11, 2005 San Diego AAS Meeting For the COSMOS WL team : (Justin Albert, Richard.

Science with FMOS The UDS perspective Omar Almaini (Nottingham) Update on UKIDSS UDS The UDS redshift survey (UDSz) Opportunities with FMOS.

Venice 06 Star Formation in the Cosmic Web Hervé Aussel, AIM Dave Sanders, Mara Salvato, Olivier Ilbert, David Frayer, Jason Surace, Nick Scoville, and.

COSMOS Kyoto meeting May 2005 Obscured AGN in the COSMOS field Andrea Comastri (INAF – Bologna) on behalf of the XMM-COSMOS team.

Swift/BAT Hard X-ray Survey Preliminary results in Markwardt et al ' energy coded color.

Weak lensing mass-selected cluster catalogues Richard Massey (CalTech) with Jason Rhodes (JPL), Alexie Leauthaud (Marseille), Justin Albert (CalTech),

The multiwavelength surveys of the ELAIS-S1 and GOODS fields Fabrizio Fiore & M. Brusa, A. Comastri, C. Feruglio, A. Fontana, A. Grazian, F. La Franca,

Extending α OX Studies to Include the Numerous Low-to- Moderate Luminosity AGNs Aaron Steffen The Pennsylvania State University November 6th, 2006.

Cosmic Shear with HST Jason Rhodes, JPL Galaxies and Structures Through Cosmic Times Venice Italy March 27, 2006 with Richard Massey, Catherine Heymans.

Weak-Lensing selected, X-ray confirmed Clusters and the AGN closest to them Dara Norman NOAO/CTIO 2006 November 6-8 Boston Collaborators: Deep Lens Survey.

Anton Koekemoer AAS 207, Washington DC, 10 January Using COSMOS to Probe the High-Redshift AGN Population Anton Koekemoer (Space Telescope Science.

Growth of Structure Measurement from a Large Cluster Survey using Chandra and XMM-Newton John R. Peterson (Purdue), J. Garrett Jernigan (SSL, Berkeley),

AGN and Quasar Clustering at z= : Results from the DEEP2 + AEGIS Surveys Alison Coil Hubble Fellow University of Arizona Chandra Science Workshop.

I. Balestra, P.T., S. Ettori, P. Rosati, S. Borgani, V. Mainieri, M. Viola, C. Norman Galaxies and Structures through Cosmic Times - Venice, March 2006.

Jason Rhodes, JPL 207 th AAS Meeting, January 10, 2006 Nick Scoville, COSMOS PI COSMOS Lensing Team: Jean-Paul Kneib, Jason Rhodes, Justin Albert, David.

Galaxy groups in the COSMOS Alexis Finoguenov Max-Planck Institut fuer extraterrestrische Physik L. Guzzo, G. Hasinger, N. Scoville, A. Leauthaud, J.P.

SFR and COSMOS Bahram Mobasher + the COSMOS Team.

The spatial clustering of X-ray selected AGN R. Gilli Istituto Nazionale di Astrofisica (INAF) Osservatorio Astronomico di Bologna On behalf of the CDFS.

Tracing Dark and Luminous Matter in COSMOS: Key Astrophysics and Practical Restrictions James Taylor (Caltech) -- Cosmos meeting -- Kyoto, Japan -- May.

Relating Mass and Light in the COSMOS Field J.E. Taylor, R.J. Massey ( California Institute of Technology), J. Rhodes ( Jet Propulsion Laboratory) & the.

Space Density of Heavily-Obscured AGN, Star Formation and Mergers Ezequiel Treister (IfA, Hawaii Ezequiel Treister (IfA, Hawaii) Meg Urry, Priya Natarajan,

Statistics of the Weak-lensing Convergence Field Sheng Wang Brookhaven National Laboratory Columbia University Collaborators: Zoltán Haiman, Morgan May,

The Clustering of AGN Using Photometric Redshifts Elias Koulouridis Antonis Georgakakis National Observatory of Athens.

Image credit: ESO/NASA/ESA/JPL-Caltech Unveiling the astrophysics of high-redshift galaxy evolution.

Cosmology Legacy Survey Jim Dunlop University of Edinburgh + Ian Smail (Durham), Mark Halpern (UBC), Paul van der Werf (Leiden)

X-ray (and multiwavelength) surveys Fabrizio Fiore.

How to start an AGN: the role of host galaxy environment Rachel Gilmour (ESO Chile & IfA, Edinburgh) Philip Best (Edinburgh), Omar Almaini & Meghan Gray.

X-ray Surveys with Space Observatory Khyung Hee University Kim MinBae Park Jisook.

Cosmic scaffolding and the growth of structure Richard Massey (CalTech ) with Jason Rhodes (JPL), David Bacon (Edinburgh), Joel Berg é (Saclay), Richard.

Black Hole Growth and Galaxy Evolution Meg Urry Yale University.

XMM-Newton surveys of X-ray galaxy groups Alexis Finoguenov MPE/UMBC+ S.Giodini, V.Allevato, M. Tanaka, A. Leauthaud, O. Ilbert, N.Cappelluti, J.Silverman,

Galaxy groups Michael Balogh Department of Physics and Astronomy University of Waterloo.

ORELSE in the Radio : AGN and Starbursts in High-Redshift Structures The Observations of Redshift Evolution in Large Scale Environments Survey Lori Lubin.

Francisco Javier Castander Serentill Institut d’Estudis Espacials de Catalunya (IEEC) Institut de Ciències de l’Espai (ICE/CSIC) Barcelona Exploiting the.

Testing the Shear Ratio Test: (More) Cosmology from Lensing in the COSMOS Field James Taylor University of Waterloo (Waterloo, Ontario, Canada) DUEL Edinburgh,

Properties of the point-like sources in the XMM-LSS field Olga Melnyk and XMM-LSS collaboration N. Clerc, L. Chiappetti, A. Elyiv, P.Gandhi, E.Gosset,

X-ray clues on the nature of sub-mm galaxies I.Georgantopoulos INAF/OABO A Comastri INAF/OABO E. Rovilos MPE.

MMT Science Symposium1 “false-color” keV X-ray image of the Bootes field Thousands of AGNs in the 9.3 square degree Bootes field * X-ray and infrared.

Initial Results from the Chandra Shallow X-ray Survey in the NDWFS in Boötes S. Murray, C. Jones, W. Forman, A. Kenter, A. Vikhlinin, P. Green, D. Fabricant,

The Evolution of AGN Obscuration

Full strength of (weak) Cluster lensing

Wide Field Astronomy from Space Steven Beckwith Space Telescope Science Institute January 9, 2002.

Revealing X-ray obscured Quasars in SWIRE sources with extreme MIR/O Giorgio Lanzuisi Fabrizio Fiore Enrico Piconcelli Chiara Feruglio Cristian Vignali.

Baryon content of galaxy groups Ming Sun (University of Virginia) ‏ M. Voit, M. Donahue (MSU) A. Vikhlinin, W. Forman, C. Jones (CfA) N. Sehgal (KIPAC)

On the evolution of Cool Core Clusters Joana Santos (INAF-Trieste) Piero Rosati (ESO), Paolo Tozzi (INAF-Trieste), Hans Boehringer (MPE), Stefano Ettori.

The NuSTAR Extragalactic Survey: A 1 st Look at the Distant High-Energy X-ray Background D.R. Ballantyne (Georgia Tech) on behalf of M. Ajello, D. Alexander,

USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS AT 1

Andrii Elyiv and XMM-LSS collaboration The correlation function analysis of AGN in the XMM-LSS survey.

Probing Cosmology with Weak Lensing Effects Zuhui Fan Dept. of Astronomy, Peking University.

Luminous Red Galaxies in the SDSS Daniel Eisenstein ( University of Arizona) with Blanton, Hogg, Nichol, Tegmark, Wake, Zehavi, Zheng, and the rest of.

EROSITA + group meeting, Ringberg, February 2008 z>3 QSOs in XMM-COSMOS: lessons for eROSITA Marcella Brusa (MPE) with help from: A. Comastri M. Salvato,

The XMM Cluster Survey: Project summary and Cosmology Forecasts Kathy Romer University of Sussex.

ENVIRONMENTALPROPERTIES ENVIRONMENTAL PROPERTIES OF z~[1-3] AGN AND OF z~[1-3] AGN AND STARFORMING GALAXIES: STARFORMING GALAXIES: THE Spitzer VIEW ON.

Robust identification of distant Compton-thick AGNs IR AGN Optical AGN Need for deep optical-mid-IR spectroscopy: multiple lines of evidence for intrinsic.

The Black Hole-Galaxy Evolution Connection Ezequiel Treister Einstein Fellow IfA, Hawaii IfA, Hawaii Credit: ESO/NASA, the AVO project and Paolo Padovani.

Clustering properties of normal and active galaxies at z~3 Harold Francke, PUC Postdoctoral Fellow (Leopoldo Infante) Thesis Adv.: Eric Gawiser (Rutgers),

The History of Active Galaxies A.Barger, P. Capak, L. Cowie, RFM, A. Steffen, and Y. Yang Active Galaxies (AKA quasars, Seyfert galaxies etc) are radiating.

6dF Workshop, May MASS Selected AGN with 6dF Paul Francis (ANU) Roc Cutri, Brant Nelson, David Kirkpatrick (IPAC/CALTECH) M. Skrutskie (U. Virginia)

A synthesis model for AGN evolution: unveiling SMBH growth with (past and future) X- ray surveys Ringberg Meeting, 2/2008 Andrea Merloni Max-Planck Institut.

Weak Lensing and X-Ray Observations of a Complete X-Ray Flux-Limited Sample of Distant Galaxy Clusters Thomas Reiprich Danny Hudson Oxana Nenestyan Emmy.

Hiroyasu Tajima Stanford Linear Accelerator Center Kavli Institute for Particle Astrophysics and Cosmology October 26, 2006 GLAST lunch Particle Acceleration.

Multiwavelength AGN Number Counts in the GOODS fields Ezequiel Treister (Yale/U. de Chile) Meg Urry (Yale) And the GOODS AGN Team.

CTIO Camera Mtg - Dec ‘03 Studies of Dark Energy with Galaxy Clusters Joe Mohr Department of Astronomy Department of Physics University of Illinois.

COSMIC MAGNIFICATION the other weak lensing signal Jes Ford UBC graduate student In collaboration with: Ludovic Van Waerbeke COSMOS 2010 Jes Ford Jason.

Z = 1.22 Red-Sequence Selected Clusters at 1 < z < 2 in the Spitzer SWIRE Survey Supervisor: Howard Yee Collaborators: Gillian Wilson Mark Lacy Henk Hoekstra.

LoCuSS: An XMM survey of X-ray groups being accreted by massive clusters Chris Haines (INAF - OA Brera, Milano) Alexis Finoguenov (Helsinki,

Exdended sources in ECDF-S

Black Holes in the Deepest Extragalactic X-ray Surveys

Cluster Cosmology in Deep Fields

Presentation transcript:

Statistics of galaxy groups in ultraDeep XMM surveys Alexis Finoguenov Max-Planck Institut fuer extraterrestrische Physik University of Maryland, Baltimore County & COSMOS, eCDFS, UDS/SXDF teams

Alexis FinoguenovStatistics of galaxy groups2

Alexis FinoguenovStatistics of galaxy groups3 COSMOSCOSMOS

Alexis FinoguenovStatistics of galaxy groups4 Challenges due to XMM PSF Incomplete candidate list Verified against Chandra clusters False detection Proper threshold ratio for point vs extended source AGN flux removal Profits from having Chandra coverage

Alexis FinoguenovStatistics of galaxy groups5 CDF S+N original

Alexis FinoguenovStatistics of galaxy groups6 CDF S+N restored

Alexis FinoguenovStatistics of galaxy groups7 CDF S+N diffuse

Alexis FinoguenovStatistics of galaxy groups8 CDFS: X-ray scaling relations

Alexis FinoguenovStatistics of galaxy groups9 COSMOS: scaling using weak lensing Credit: Alexie Leauthaud + COSMOS weak lensing team

Alexis FinoguenovStatistics of galaxy groups10 Group statistics: COSMOS & CDFS Self-consistent evidence for no evolution in Lx function!

Alexis FinoguenovStatistics of galaxy groups11 Survey strategies to detect evolution fx required area Lxz evol z off survey 1.e-15>12.e43> UDS/DUX ultraVISTA 1.e-14>105.e43> XMM-LSS XCS 1.e-13>2002.e44> d 1.e-12>10k1.e45> RASS

Alexis FinoguenovStatistics of galaxy groups12 Strategy of high-z cluster detection 1

Alexis FinoguenovStatistics of galaxy groups13 The UKIDSS Ultra-Deep Survey 0.77 sq degrees K=23, H=24, J=25 (5 , Vega, point source) Year 1: K=21.8, J=23.0 (86 hours) EDR: K=20.6, J=21.7 (12 hours) 0.88 deg. Almaini et al. 2006

Alexis FinoguenovStatistics of galaxy groups14 UDSUDS

Alexis FinoguenovStatistics of galaxy groups15 z=1.408 cluster

Alexis FinoguenovStatistics of galaxy groups16 Conclusions Deep surveys are dominated by clusters with non-evolving luminosity function X-ray spectroscopy, stacked weak lensing and clustering could all be used to yield the total mass Deep X-ray surveys extended over an area >1 square degree access cosmological parameters at z=1.5