Field content and target identification

Slides:



Advertisements
Similar presentations
CAHA, 5 Feb 2005XMM-Newton Surveys Xavier Barcons.
Advertisements

Astrometry and EPIC flux cross-calibration in 2XMMp/2XMM Silvia Mateos R. Saxton, S. Sembay and the XMM-Newton Survey Science Centre.
Tracing cosmic accretion through the XMM-Newton Medium Survey (XMS) Xavier Barcons On behalf of the AXIS/XMS/SSC team.
X-ray spectral variability of seven LINER nuclei with XMM-Newton and Chandra data Author: Hernandez-Garcia, L; Gonzalez-Martin, O; Marquez, I; Masegosa.
A Large Catalogue of Ultraluminous X-ray Source Candidates in Nearby Galaxies Madrid: 2010 DOM WALTON IoA, Cambridge, UK In collaboration with Jeanette.
Variability: who cares? or…. Photometric redshift for XMM-COSMOS sources M.Salvato, G. Hasinger, O. Ilbert, G. Zamorani, M.Brusa + COSMOS collaboration.
Probing the X-ray Universe: Analysis of faint sources with XMM-Newton G. Hasinger, X. Barcons, J. Bergeron, H. Brunner, A. C. Fabian, A. Finoguenov, H.
Planck Satellite Revisited Anne Lähteenmäki Metsähovi Radio Observatory Helsinki University of Technology TKK.
Ringberg Meeting, Apr 05 2dF Spectroscopic Identification of a Southern XMM-Newton Serendipitous Sample Jonathan Tedds (Leicester), Mat Page (MSSL) & XMM-Newton.
Obscured and unobscured growth of Super-massive Black Holes Francisco J. Carrera, X. Barcons, J. Bussons, J. Ebrero, M. Ceballos, A. Corral (IFCA, CSIC-UC,
COSMOS Team Meeting, Kyoto, 23 May 2005 C-COSMOS The Chandra Cycle 7 COSMOS Proposal Martin Elvis (PI) & 32 others.
Science Requirements Impacting AO Architecture Claire Max Architecture Meeting July
The XMM-Newton hard band wide angle Survey Nicoletta Carangelo and Silvano Molendi (IASF-MI(CNR)) Epic Consortium Meeting Palazzo Steri, Palermo,
Review of 2XMMp data products Anja Schröder, Univ of Leicester, UK John Pye, Univ of Leicester, UK.
July 16, 2004P. Padovani, NEON Archive School Science with Multi- Archival Data Paolo Padovani (ST-ECF/ESO) Astrophysical Virtual Observatory Science Manager.
July 16, 2004P. Padovani, NEON Archive School Science with multi-wavelength Archival Data Paolo Padovani (ESO) Virtual Observatory Systems Department &
Obscured AGN and XRB models Andrea Comastri (INAF-OABologna-Italy) Roberto Gilli (INAF-OABologna-Italy) F. Fiore (INAF-OARoma-Italy) G. Hasinger (MPE-Garching-
The X-ray source population of M 31 and M 33 Wolfgang Pietsch Max Planck Institut für extraterrestrische Physik.
Spectral Energy Distributions of 2XMM-selected AGN & VO-tools Rodrigo Gil-Merino Instituto de Física de Cantabria (CSIC-UC) Santander, Spain MAVO workshop,
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.
11 July 20036dF workshop1 Radio sources in the 6dFGS Tom Mauch & Elaine Sadler University of Sydney ‘Main survey’ science: Faint end of radio luminosity.
X-ray emission properties of BLAGN in the XMM-2dF Wide Angle Survey S. Mateos, M.G. Watson, J. A. Tedds and the XMM-Newton Survey Science Centre Department.
X-ray sky survey of bright, serendipitous sources with 2XMMi at the AIP Speaker: Alexander Kolodzig Origin: Humboldt-Uni Berlin, Germany Institute:AIP.
XMM slew survey Richard Saxton 1, Andy Read 2, Pili Esquej 3, Michael Freyberg 3, Bruno Altieri 1 1. ESAC 2. University of Leicester 3. MPE XMM slew survey.
Update on the XMM Slew Survey Richard Saxton 1, M. Pilar Esquej 1 Andy Read 2, Michael Freyberg 3, Bruno Altieri 1, 1 ESAC 2 University of Leicester, U.K.
The X-ray source population studies in nearby galaxies Wolfgang Pietsch Max Planck Institut für extraterrestrische Physik.
Progress report on LSS Catalogue web site and database  (2) which database tables ? on which sky area ? who can access them ?  (3) what path did X-ray,
New XMM-Newton deep Survey in the Lockman Hole Vincenzo Mainieri MPE Workshop on AGN Surveys, Puebla, June 23- July 11, 2003 Guenther Hasinger Hans Boehringer.
Seeking type 2 QSO amongst bright X-ray selected EXOs Agnese Del Moro University of Leicester, UK In collaboration with: M.G. Watson (UoL), S. Mateos (UoL),
Average Fe Kα emission from distant AGN
JWST FGS Guide Star Studies
The XMM-Newton Slew Survey
EVALUATION OF THE XMM NEWTON CROSS CALIBRATION ARCHIVE
The Hubble Legacy Archive (HLA) Slitless Spectroscopy Project
High Resolution X-Ray Spectra A DIAGNOSTIC TOOL OF THE HOT UNIVERSE
Periodicity Search in X-ray data of RX J
Neutral Hydrogen in Galaxy Groups
MedDRA and Ontology Discussion of Strategy
X-ray Surveys Lockman Hole Team Giacconi (JHU) Gunn (Princeton)
Yuichi Terashima (Ehime U.)
Fermi & ASDC Elisabetta Cavazzuti on behalf ASDC Team Fermi Meeting
CCA schemes for the 120MHz spectrum in China
DIFFUSE RADIO SOURCES in GROUPS and POOR CLUSTERS
The Space Density of Compton Thick AGN
The Variable Source Content of the The Variable Source Content of the
Re-engineering the French Business Register ( )
Andrea Comastri (INAF- Oss. Astr. Bologna)
A 325 MHz Radio Survey of M31 Yosi Gelfand (CfA) Joseph Lazio (NRL) Bryan Gaensler (CfA) Using the VLA A-array, we imaged 405 radio sources.
Source catalogue generation
Humble Hubble Team 18 – Derek Pesyna Abstract
The INTEGRAL NLSy1 FRANCESCA PANESSA The X-ray Universe 2011
XMM-NEWTON reveals a dipping black-hole X-ray binary in NGC 55
Quasi-periodic pulsations in stellar flares observed with XMM-Newton
Hard X-ray observations of Extremely Red Objects
The XMM-Newton long look of NGC 1365:
XMM-Newton slew sources A quick analysis
How to classify a Gamma -ray source as a Blazar
Text Categorization Rong Jin.
Nam08, belfast apr 1-4, 2008 martin still, christopher brindle, mat page, vladimir yershov, alice breeveld, houri ziaeepour (ucl-mssl) simon rosen (leicester)
Identification of PHLOTE Students
Risolvere il Background X al suo picco
The spectral properties of Galactic X-ray sources at faint fluxes
Black Holes in the Deepest Extragalactic X-ray Surveys
A.Malizia, L. Bassani , M. Molina
The merger-AGN connection since z~1: causal or circumstantial?
Reporting QA Measures to EBAS – and a Word on Flagging
A handbook on validation methodology. Metrics.
GK1 Highlights Automatic and Unbiased Emotional screening System, based on LVA Voice Analysis technology Designed for quick identification of “crime in.
X-ray high resolution spectra in the VO: the case of XMM-Newton RGS
CCA schemes for the 120MHz spectrum in China
Presentation transcript:

Field content and target identification 20th Survey Science Centre Consortium meeting Field content and target identification Ann-Marie Stobbart Anja Schroeder, Mike Watson and the XMM-Newton Survey Science Centre

2XMMp: selecting observations 2XMMp contains a subset of the total number of observations to be included in the final 2XMM catalogue. Subset selected via visual screening of each observation + sources + automatic flags  Quick field identifications based on the number of ‘spurious’ detections i.e. those NOT automatically flagged as spurious 14th November 2006 Ann-Marie Stobbart

2XMMp: selecting observations Observations classified into one of four quality flags (OBSFLAG=0-3)  ‘Good’ observations (OBSFLAG=0-2) included i.e. those with no or few obvious spurious detections (83% public observations with EPIC data) 14th November 2006 Ann-Marie Stobbart

Observation classes: OBSFLAG=0 52% : no obvious spurious detections (may include one or two non-obvious ones) 14th November 2006 Ann-Marie Stobbart

Observation classes: OBSFLAG=1 30% : one or more spurious detections (but usually < 8 ) 14th November 2006 Ann-Marie Stobbart

Observation classes: OBSFLAG=2 0.9% : class 1 + missed detections in a group of very densely positioned sources 14th November 2006 Ann-Marie Stobbart

Observation classes: OBSFLAG=3 17% : not accepted for inclusion in the catalogue 14th November 2006 Ann-Marie Stobbart

Field identification 2XMMp screening effectively independent of target itself 2XMM  Serendipitous catalogue Aim for 2XMM is to classify XMM-Newton fields by the type of target within them But, is the target: a single object ? a whole field ? extended ? 14th November 2006 Ann-Marie Stobbart

Field identification 5 proposed field classifications: Point source Extended source Small extended Large extended Field (e.g. The Lockman Hole) Not detected (e.g. OM calibration field) Unknown 14th November 2006 Ann-Marie Stobbart

Field ID : Large extended SIMBAD PROPOSAL NED RA_PNT DEC_PNT XSA NGC 55 (WEST): 0028740101 : X-ray background and surveys 14th November 2006 Ann-Marie Stobbart

Field ID : Large extended SIMBAD PROPOSAL NED RA_PNT DEC_PNT XSA NGC 4258: 0059140401 : AGN, QSOs, BL-Lacs and XRB 14th November 2006 Ann-Marie Stobbart

Target identification Aim to flag the target of the observation Difficulties, e.g. for galaxies  no source to flag unambiguously Simplest solution  flag the targets from the ‘point source’ field classification 14th November 2006 Ann-Marie Stobbart

Summary 2XMMp screening: quick field identifications  83% public observations included Aim for 2XMM: field and target identifications  work in progress Difficulties: Finding a position that best identifies the target in order to classify the field finding an unambiguous target position in order to flag the target 14th November 2006 Ann-Marie Stobbart