The 3XMM catalogue. Natalie Webb. Institut de Recherche en Astrophysique et Planétologie Toulouse, France

Similar documents
The Survey Science Centre report to the XMM Newton Users Group

A Library of the X-ray Universe: Generating the XMM-Newton Source Catalogues

Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift

Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift

XMM-Newton Calibration

High-energy astrophysics data provision at Leicester Julian Osborne. Open Universe ASI: Tor Vergata April 2017 JO

Natalie Webb & Mathieu Servillat, Sean Farrell, Didier Barret. Centre d Etude Spatiale des Rayonnements Toulouse, France

Tidal disruption events from the first XMM-Newton Slew Survey

The XMM-Newton serendipitous survey

Coronal geometry at low mass- accretion rates from XMM and NuSTAR spectra. Felix Fürst Caltech for the NuSTAR AGN physics and binaries teams

HLX-1: unsolved puzzles

XMM-Newton Observations of Unidentified Gamma-Ray Objects

XMM-Newton Optical-UV Monitor: introduction and calibration status OM instrument and calibration

CONTENTS AIM OF THE PROJECT. INTRODUCTION: AGNs, XMM-Newton, ROSAT. TECHNIQUES: IDL, SQL, Catalogues RESULTS SUMMARY DESIRED OUTPUTS QUESTIONS

Analysis of extended sources with the EPIC cameras

Luminous Galaxy Clusters from the XMM Archive Possibilites and Limitations

The quest for Type 2 quasars: What are the X-ray observations of optically selected QSOs2 telling us?

The Bright Side of the X-ray Sky The XMM-Newton Bright Survey. R. Della Ceca. INAF Osservatorio Astronomico di Brera,Milan

ROSAT Roentgen Satellite. Chandra X-ray Observatory

Few good reasons to hold the meeting in Cervia

X ray Survey Results on AGN Physics and Evolution Niel Brandt

Cosmological Constraints from the XMM Cluster Survey (XCS) Martin Sahlén, for the XMM Cluster Survey Collaboration The Oskar Klein Centre for

Investigating Ultraluminous X-ray Sources through multi-wavelength variability, broadband spectra, and theoretical modelling

Radio Detections During Two State Transitions of the Intermediate Mass Black Hole HLX-1

The Extragalactic Gamma-Ray View of AGILE and Fermi

arxiv: v1 [astro-ph] 28 Nov 2008

Results from the Chandra Deep Field North

PDF hosted at the Radboud Repository of the Radboud University Nijmegen

A new catalogue of ultraluminous X-ray sources (and more!)

PoS(INTEGRAL 2010)131

Optical studies of an ultraluminous X-ray source: NGC1313 X-2

Chandra was launched aboard Space Shuttle Columbia on July 23, 1999!!!

4U E. Bozzo. M. Falanga, A. Papitto, L. Stella, R. Perna, D. Lazzati G. Israel, S. Campana, V. Mangano, T. Di Salvo, L.

The Compton Spectrometer and Imager A balloon- borne gamma- ray spectrometer, polarimeter, and imager

The Hamburg/RASS Catalogue of Optical Identifications of ROSAT-BSC X-ray Sources

BAR. Chandra Acis Timing Brera And Rome astronomical observatories

The BAT AGN Survey - Progress Report J. Tueller, C. Markwardt, L. Winter and R. Mushotzky Goddard Space Flight Center

X-ray Astronomy F R O M V - R O CKETS TO AT HENA MISSION. Thanassis Akylas

Chapter 0 Introduction X-RAY BINARIES

PoS(Extremesky 2011)009

X-ray Observations of Nearby Galaxies

Science and source catalogs with JEM-X. Niels Jørgen Westergaard National Space Institute, Technical University of Denmark

The History of Active Galaxies A.Barger, P. Capak, L. Cowie, RFM, A. Steffen, and Y. Yang

High Redshift Universe

Surveys for high-redshift (z>6) AGN with AXIS (cf. Athena) James Aird. University of Cambridge (-> University of Leicester)

Ultraluminous X-ray Sources in Nearby Galaxies

GAME: GRB and All-Sky Monitor Experiment

Background Picture: Millennium Simulation (MPA); Spectrum-Roentgen-Gamma satellite (P. Predehl 2011)

Multi epoch variability of αox in the CDFS

Exploring Fermi-LAT Extended GeV Emission with Stacking Analysis

Spitzer Space Telescope Calibration Strategy: The Use of Asteroids

Rajib Ganguly (University of Michigan-Flint)

VERITAS detection of VHE emission from the optically bright quasar OJ 287

The Palermo Swift-BAT Hard X-ray Catalogue

PoS(extremesky2009)018

arxiv:astro-ph/ v1 21 Mar 2003

Galaxy Clusters with Swift/BAT

GDR1 photometry. CU5/DPCI team

Chandra: the Next Decade

VISTA HEMISPHERE SURVEY DATA RELEASE 1

AGILE GRBs: detections and upper limits

RGS CALIBRATION STATUS

ESASky, ESA s new open-science portal for ESA space astronomy missions

Search for galaxies in interaction/merging in a sample of hard X- Ray selected objects

SUPPLEMENTARY INFORMATION

Introduction to SDSS -instruments, survey strategy, etc

RLW paper titles:

Optical short-time variability properties of AGN

THE SUNYAEV-ZELDOVICH EFFECT

ACIS ( , ) Total e e e e-10 4.

WORKSHOP ULXs AND THEIR ENVIRONMENT June 13th 16th, 2016 Strasbourg, France

V5116 Sgr (Nova Sgr 2005b): an eclipsing supersoft postoutburst nova?

Extended Chandra Multi-Wavelength Project (ChaMPx): Source Catalog and Applications

Comets observed with XMM-Newton

X-raying galactic feedback in nearby disk galaxies. Q. Daniel Wang University of Massachusetts

arxiv: v1 [astro-ph] 29 Nov 2007

A caleidoscopic view of Active Galactic Nuclei

Searching for black holes in nearby galaxies with Simbol-X

X-ray emission properties vary with spin-down age. Crab-like pulsars (< 10 4 yrs)

Science Olympiad Astronomy Event Division C. Supervisor: JoDee Baker.

Monitoring nearly 4000 nearby stellar systems with the OVRO-LWA in search of radio exoplanets

Future X-rayX Spectroscopy Missions. Jan-Willem den Herder

X-raying High-Redshift AGNs and the First Black Holes: From Chandra to Lynx

S. Basa, Laboratoire d Astrophysique de Marseille, France

CHARACTERIZATION OF AGN VARIABILITY IN THE OPTICAL AND NIR REGIMES

Hard X-ray AGN and the Cosmic X-ray Background

XMM-Newton - Chandra Synergy: Maximizing their Future Science Impact over the Next Decade

arxiv: v1 [astro-ph.ga] 31 Mar 2014

PACS spectroscopy Data Analysis

Relativistic jets from XRBs with LOFAR. Stéphane Corbel (University Paris 7 & CEA Saclay)

RX J and RX J : recent results and status

A Decade of Short-duration Gamma-ray Burst Afterglows

Recent Observations of Supernova Remnants

Soft X-ray Emission Lines in Active Galactic Nuclei. Mat Page

SUPPLEMENTARY INFORMATION

GOODS/FORS2 Final Data Release: Version 3.0

Modern Image Processing Techniques in Astronomical Sky Surveys

Bringing Real-time Astronomical Observations into the Classroom

A Multiwavelength Study of the Gamma-ray Binaries 1FGL J and LMC P3

Nearby Galaxy Clusters with UVIT/Astrosat

Transcription:

The 3XMM catalogue Institut de Recherche en Astrophysique et Planétologie Toulouse, France and for the XMM Newton Survey Science Centre (SSC) 1

XMM Newton Survey Science Centre (SSC) The XMM Newton Survey Science Centre was selected by ESA to ensure that the scientific community can exploit XMM Newton data Responsibilities : Development of science analysis software (SAS) Pipeline processing of all XMM Newton observations. Follow up/identification of the XMM Newton serendipitous sky the XID Programme Compilation of the Serendipitous Source Catalogue. 2

3XMM DR7 3 February 2000 15 December 2016 made public 1st June 2017! 727790 detections, some sources up to 59 times Rosen, Webb 499266 unique sources et al. (2016) 162045 sources with spectra and lightcurves 11220 extended sources Cross correlation with many catalogues Covers 1032 sq. deg of sky 3

3XMM DR7 A source chosen at random from those with >40 pointings In 3XMM DR7, the median flux : ~ 1.9 10 14 erg cm 2 s 1 (0.2 12.0 kev) ~23% sources fluxes <1 10 14 erg cm 2 s 1 (0.2 12.0 kev) ~ 6 10 15 erg cm 2 s 1 (0.2 2.0 kev) ~ 8 10 15 erg cm 2 s 1 (2.0 12.0 kev) 5631 sources variable (χ2 < 1 10 5) 4

3XMM DR7 data proposed 332 columns of information including : Identifiers/coordinates Observation date/time and observing mode Exposure /background info Band 8 Flux Extent 0.2 12.0 kev Counts/fluxes/rates Band 9 = 2+3+4 0.5 4.5 kev Hardness ratios (HR) Maximum likelihood Band 1 Quality flags 0.2 0.5 Band 2 Variability kev HRi = Bandi+1 Bandi Bandi+1 + Bandi 0.5 1.0 kev Band 3 1.0 2.0 Band 4 kev 2.0 4.5 kev Band 5 4.5 12.0 kev Energy

3XMM DR7 data quality Astrometry Cross match with latest version of SDSS quasars catalogue Comparison between 2XMM DR3 and 3XMM DR7 6

3XMM DR7 relative size 800000 X-ray detections 700000 600000 500000 400000 300000 200000 100000 0 UHURU (1971) HEAO-1 (1979) ROSAT 2RXS (2016) Swift 1SXPS (2014) Chandra CSC 2.0 (2017) XMM 3XMM-DR7 (2017) X-ray missions/catalogues 7

3XMM DR7 uses The catalogue is excellent for : Quick access to data products (fluxes, spectra, images, etc) Finding new objects Population studies Cross correlation for multi wavelength studies 8

Accreting compact objects 2 magnetic cataclysmic variables (CVs) (Webb et al., submitted) 2.15 hr period 1.6 hr period credit: M. A. Garlickk 9

Accreting compact objects 2 more magnetic CVs (Lin, Webb & Barret, 2014) 10

Extreme tidal disruption event Lin et al. (2017) See also poster by Sébastien Soler J20 for other examples 11

HLX 1 12

HLX 1 13

HLX 1 2XMM J011028.1 460421 (HLX 1, Farrell, Webb et al., Nature, 2009) ~8 from nucleus of ESO 243 49 (z=0.0224, ~95 Mpc) Associated with ESO 243 49 => Lx=1.1x1042 erg s 1 (0.2 10.0 kev, Wiersema et al. 2010) Spectral analysis + modelling => black hole with mass ~ 104 M For more information on HLX 1 see poster F04 14

Stacked catalogue New stacked source detection tasks in SAS to provide a standardised source detection method for overlapping observations more convenient handling of multiple pointings for the users optimize stacked source parameters basis of a stacked catalogue of repeatedly observed sources Images stacked with emldetect Source detection using edetect_stack #OBS #grps 2 204 3 40 4 10 5 8 4 6 9,10,12 1 each Proto catalogue: 736 observations, 278 stacks, 25,500 detections 15

SUSS 3.0 Field of view coincides with 3XMM FOV 6,880,116 detections 4,751,899 unique sources 867,022 have multiple entries Visible (U, B and V) and UV (UVW1, UVM2 and UVW2) Detections down to AB magnitude: UVW2~ 23.0 UVM2~ 24.1 UVW1~ 24.8 U~ 25.2 B~ 24.0 V~ 23.4 (Page et al. 2012) FWHM ('') 1.98 1.8 2.0 1.55 1.39 1.38 16

4XMM 3XMM DR8 planned for first half of 2018 4XMM anticipated for 2019 full re reduction of all data (~10500 obs.) with improved software and improved calibration to include : variability between observations in catalogue added variability analysis improved source flagging sky exposure for population studies... 17

Summary Wide range of rare objects found in 3XMM catalogue New incremental version planned for 2018 (DR8) New major version, 4XMM DR9 planned for 2019 Access the catalogue : XMM Newton SSC webpages :http://xmmssc.irap.omp.eu But also at : XSA at ESA's XMM Newton SOC : http://xmm.esac.esa.int/xsa/ XCAT DB at : http://xcatdb.unistra.fr/3xmmdr7 The IRAP catalogue server XSA : http://xmm catalog.irap.omp.eu/ Browse at HEASARC NASA GSFC : http://heasarc.gsfc.nasa.gov/db perl/w3browse/w3browse.pl LEDAS at : http://www.ledas.ac.uk/ ESA sky : http://sky.esa.int/ 18

Backup slides 2XMM J011028.1 460421 ~8 from nucleus of ESO 243 49 (z=0.0224, ~95 Mpc) Backup slides 19

20