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Jonathan Tedds X-ray Universe 2008 Jonathan Tedds University of Leicester/XMM-Newton SSC/AstroGrid/ EuroVODCA science team [email protected]

AG Xray Granada May08 - Cosmos Home

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Page 1: AG Xray Granada May08 - Cosmos Home

Jonathan Tedds

X-ray Universe 2008

Jonathan Tedds

University of Leicester/XMM-Newton SSC/AstroGrid/EuroVO DCA science team

[email protected]

Page 2: AG Xray Granada May08 - Cosmos Home

Data Archives

Jonathan Tedds

X-ray Universe 2008

Page 3: AG Xray Granada May08 - Cosmos Home

Jonathan Tedds

X-ray Universe 2008

Page 4: AG Xray Granada May08 - Cosmos Home

Jonathan Tedds

X-ray Universe 2008

Page 5: AG Xray Granada May08 - Cosmos Home

Jonathan Tedds

X-ray Universe 2008

Page 6: AG Xray Granada May08 - Cosmos Home

What are Virtual Observatories (VOs)?

“The VO vision can be summed up as the desire to make all archives speak the

same language – all searchable and analyzable by the same tools, all data

sources accessible through a common interface, all data held in distributed

databases that appear as one.”

Jonathan Tedds

X-ray Universe 2008

September 2003

Andy Lawrence (PI AstroGrid)

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Creating a Virtual Observatory - An

International Effort

The International Virtual Observatory Alliance

Agree international standards for any dataset or

Jonathan Tedds

X-ray Universe 2008

Agree international standards for any dataset or

astronomical resource published to the VO

� Allow simultaneous multi archive, multi parameter

correlations

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As a result of the IVOA we have

� A common Resource Metadata

� A common data querying language� Astronomical Data Query Language (ADQL)

Jonathan Tedds

X-ray Universe 2008

� Astronomical Data Query Language (ADQL)

� Based on Structured Query Language (SQL)

� Common table format� Virtual Observatory Table (.vot)

� …and much more in the pipeline

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Advantages of VO data access

� Accessing multiwavelength data easier:

� Do not need to access different interfaces, register once only

Jonathan Tedds

X-ray Universe 2008

Page 10: AG Xray Granada May08 - Cosmos Home

Advantages of VO data access

� Accessing multiwavelength data easier:

� Do not need to access different interfaces, register once only

� Data access from one single entry point

Able to build workflows i.e. pieces of code which run on

Jonathan Tedds

X-ray Universe 2008

� Able to build workflows i.e. pieces of code which run on the server and are reusable

Page 11: AG Xray Granada May08 - Cosmos Home

http://www.astrogrid.org (April 2008 1st public release)

Jonathan Tedds

X-ray Universe 2008

Page 12: AG Xray Granada May08 - Cosmos Home

VO Explorer: public release April 08

� AstroGrid front end, part of VOdesktop

� Resource-centric

� Select a search-space

� Search for resources

� Filter these resources

View selected resources

Jonathan Tedds

X-ray Universe 2008

� View selected resources

� Use the selection

� Invoke it

� Save/Bookmark/Tag it

� Export it

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Access existing X-ray cluster catalogues

� Browse through keyword metadata

Jonathan Tedds

X-ray Universe 2008

� Browse through keyword metadata

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Find

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Description

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�� If data in a simple DB can If data in a simple DB can publish to VO in ~day!publish to VO in ~day!

�� We can help you: June 23We can help you: June 23--27, 27, 2008 2008 data publishingdata publishing workshop workshop at at ESO, ESO, GarchingGarching

content +resources

�� For catalogues, imagesFor catalogues, images, spectra, , spectra, transient & theoretical archivestransient & theoretical archives

�� CensusCensus of European Data of European Data Centres & ArchivesCentres & Archives

�� UK contact: UK contact: [email protected]@star.le.ac.uk

�� See See TeddsTedds et al. poster J16!et al. poster J16!

technicalsystem

operations +support

Page 17: AG Xray Granada May08 - Cosmos Home

Resources!

Select all LEDAS tables!

Jonathan Tedds

X-ray Universe 2008

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Resources!

Search all LEDAS tables by position for CV: WW Cet

Jonathan Tedds

X-ray Universe 2008

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More advanced query: Access all extended 2XMM

X-ray sources

� Make own X-ray cluster candidate catalogue

� Filter large multiwavelength archives remotely:

Jonathan Tedds

X-ray Universe 2008

� Filter large multiwavelength archives remotely:

� Create manageable science subsets

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Resources!

Jonathan Tedds

X-ray Universe 2008

Columns

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Resources!

Filter columns

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Resources!

Query

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Resources!

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Resources!

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•Python + Perl, IDL scripts…

•Single archive image

search

•Cone search for multiple,

user defined archives

•Sextractor script –

generate catalogue from

images

Jonathan Tedds

X-ray Universe 2008

images

•Montage - mosaic tool

•Taverna

•Graphical interface

•Embed existing code (any

language)

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Command Line Scripting� Connect to the AstroGrid system from command line

� Write your own Python scripts (IDL, perl…to come)

#!/usr/bin/python# Given an input list od objects, queries the 2MASS catalogue returning a # VOTable for each object.

from astrogrid import ConeSearchfrom astrogrid.utils import broadcast, read_votable

# Read input list of ra, decs from VOTablevot=read_votable('sample.vot')id = vot['id']

Jonathan Tedds

X-ray Universe 2008

id = vot['id']ra = map(float, vot['ra'])dec = map(float, vot['dec'])

# We are going to query 2MASS at RoEivorn = 'ivo://wfau.roe.ac.uk/twomass-dsa/cone'cone = ConeSearch(ivorn)

nsrc = len(ra) # Number of sourcesradius=20./3600.0 # Search radius in degrees

print 'Starting Query: %d objects' % nsrc

for i in range(nsrc):res = cone.execute(ra[i], dec[i], radius)# Uncomment the following line if you want to send the output to TOPCAT# broadcast(res)print 'Writing 2mass_%s.vot' % id[i]open('2mass_%s.vot' % id[i], 'w').write(res)

Page 27: AG Xray Granada May08 - Cosmos Home

e.g. correlation with SDSS� Select SDSS galaxies within 1 arcmin of 411 X-ray positions

� photometry (ugriz), photometric redshifts

� spectra, spectroscopic redshifts

� colour thumbnail images

Jonathan Tedds

X-ray Universe 2008

colour thumbnail images

� Visual inspection of images, spectroscopic and photoscopic redshifts

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Correlation with SDSS

Jonathan Tedds

X-ray Universe 2008

Spectroscopic z = 0.223 (Lamer+, in prep)

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The VO is already in use…

� Using VO tools to investigate distant radio starburst hosting obscured AGN in the HDF(N) region

� Richards et al., A&A, 472, 805 (2007)

� Albus 1: a very bright White Dwarf candidate

� Caballero & Solano, ApJ, 665, L151 (2007) � Caballero & Solano, ApJ, 665, L151 (2007)

� Flare productivity of newly-emerged paired and isolated solar active regions

� Dalla et al., A&A, 468, 1103 (2007)

� Radio-loud Narrow-Line Type 1 Quasars

� Komossa et al., AJ, 132, 531 (2006)

� Luminous AGB stars in nearby galaxies: a study using VO tools

� Salmantza et al., A&A, 447, 89 (2006)

Page 30: AG Xray Granada May08 - Cosmos Home

Advantages of VO data access

� Accessing multiwavelength data easier:

� Do not need to access different interfaces, register once only

� Data access from one single entry point

Able to build workflows i.e. pieces of code which run on

Jonathan Tedds

X-ray Universe 2008

� Able to build workflows i.e. pieces of code which run on the server and are reusable

� Tools to analyse the returned data

� Different tools which share standards on how to interoperate

Page 31: AG Xray Granada May08 - Cosmos Home

X-Ray Upper Limit Server: Clive Page/XMM-SSC + Duncan Law-Green /LEDAS

ALADIN image here

Raw & processed archive data

FITS HDS JPG

ALADIN image hereMeasure counts within circle and fitted

Background + set detection LH threshold

⇒ Empirical upper-limit to flux

according to algorithm of Carrera+ 07

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ALADIN image here

Raw & processed archive data

Catalogue Fluxes

FITS HDS JPG

X-Ray Upper Limit Server

ALADIN image here

Page 33: AG Xray Granada May08 - Cosmos Home

X-Ray Upper Limit Server

ALADIN image here

Raw & processed archive data

Catalogue Fluxes

Generated Fluxes

FITS HDS JPG

ALADIN image here

Page 34: AG Xray Granada May08 - Cosmos Home

X-Ray Upper Limit Server

ALADIN image here

Raw & processed archive data

Catalogue Fluxes

Generated Fluxes

FITS HDS JPG

ALADIN image here

Flux limits

Page 35: AG Xray Granada May08 - Cosmos Home

X-Ray Upper Limit Server

ALADIN image here

Raw & processed archive data

Catalogue Fluxes

Generated Fluxes

FITS HDS JPG

ALADIN image here

Flux limits

Automation (workflow)

Generated spectra/time series, thumbnail images

Page 36: AG Xray Granada May08 - Cosmos Home

X-Ray Upper Limit Server

ALADIN image here

Raw & processed archive data

Catalogue Fluxes

Generated Fluxes

FITS HDS JPG

ALADIN image here

Flux limits

Automation (workflow)

Generated spectra/time series, thumbnail images

e.g. upper limits for SDSS optically selected

BAL QSOs (Cottis, Goad et al)

Page 37: AG Xray Granada May08 - Cosmos Home

http://www.astrogrid.org (April 2008 1st public release)

Jonathan Tedds

X-ray Universe 2008