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R. González-Riestra P.M. Rodríguez-Pascual XMM-Newton Science Operations Centre ESAC Astronomical Spectroscopy and the Virtual Observatory, March 21 st 2007, ESAC X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

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Astronomical Spectroscopy and the Virtual Observatory, March 21 st 2007, ESAC. X-ray high resolution spectra in the VO: the case of XMM-Newton RGS. R. Gonz á lez-Riestra P.M. Rodr í guez-Pascual XMM-Newton Science Operations Centre ESAC. Not calibrated - PowerPoint PPT Presentation

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Page 1: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

R. González-Riestra

P.M. Rodríguez-Pascual

XMM-Newton Science Operations Centre

ESAC

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

X-ray high resolution spectra in the VO:the case of XMM-Newton RGS

Page 2: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

Can X-Ray spectra be included in the VO ?

• Not calibrated • Response matrices are not invertible• Fluxes are model dependent

• In some cases response matrices are nearly diagonal• Calibrated data - useful for some purposes, when detailed spectral analysis is not required - can be provided • Example: XMM-Newton RGS spectra

NO

YES

Page 3: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

• Operates in parallel with the EPIC cameras and the Optical Monitor

• Provides X-ray high resolution (R = 100 - 500) spectroscopy in the spectral range 6 - 39 Å

• Extracted spectra can be corrected for the effective area and provided in physical units (Flux vs. Wavelength): RGS fluxed spectra

RGS: The XMM-Newton Reflection Grating Spectrometer

Page 4: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

• Currently RGS data are not uniformly processed (different versions of SW and of Calibration Files)

• Fluxed spectra are not produced in the standard pipeline processing

Database containing:

• ~ 4600 RGS fluxed spectra uniformly processed

• Plus some ‘added value’ items relevant to the interpretation of the data

• Tool for data browsing and evaluation

Browsing interface for RGS Data

Page 5: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

a Browsing interface for RGS Data

Search by:• Object name • Coordinates• Observing date• Observation Id

Additional search criteria:• Type of object• Quality• Hydrogen Column• Redshift• Exposure time

Optional output fields:• Simbad name• Simbad Type• Simbad Coordinates• Observing date• Exposure time• Quality• Hydrogen Column• Redshift

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

Page 6: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

a Browsing interface for RGS Data

XM

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Simbad query by object or by coordinates

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sample selection plotting options

Page 7: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

a Browsing interface for RGS Data

Single Spectrum Plot

Page 8: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Multiple Spectra Plot

Average Spectrum Plot

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

a Browsing interface for RGS Data• For a single object • For a class of objects• For an user-defined sample

Page 9: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

a Browsing interface for RGS Data

Page 10: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

a Browsing interface for RGS Data

Page 11: X-ray high resolution spectra in the VO: the case of XMM-Newton RGS

Astronomical Spectroscopy and the Virtual Observatory, March 21st 2007, ESAC

A wish list for a visualization tool for spectra

• Data sets uniformly processed and calibrated

• Estimation of the quality of the data

• Basic plotting and display tools (rebinning, smoothing ...)

• Comparison of spectra and images, if applicable

• Ability to build sub-samples of data with specific characteristics (date of observation, redshift...)

• Access to additional information (object classification, parameters pertinent to the specific dataset, publications…) of relevance for the interpretation of the data