Differences between revisions 4 and 5
Revision 4 as of 2013-07-30 09:32:57
Size: 3710
Comment:
Revision 5 as of 2013-07-30 10:01:19
Size: 3700
Comment:
Deletions are marked like this. Additions are marked like this.
Line 60: Line 60:
        * longterm (given availability of suitable developer/maintainer): make available functionality of Frank's SMC DB system in SkyQuery/Millenium/TAP, tailor for eROSITA...         * longterm (given availability of suitable developer/maintainer): port functionality of Frank's SMC DB system to SkyQuery/Millenium/TAP, tailor for eROSITA...

Notes on discussion

Vadim Burwitz (MPE)/ Jan Robrade (Hamburg) - Stellar Working Group

  • Even shallow surveys are adequate, because these tend to be bright
  • Need coverage over the galactic plane
  • Typically one direction-- look at optical star catalog and find the eROSITA counterpart
  • a challenge is stars tend to have companions, and these cannot be easily separated in the X-ray
  • Nearby- so proper motions must be available for the optical catalogs...
  • Stellar scientists will generate new lists and need to upload those into Frank's tool to allow for cross-correlations with other catalogs.

Arne Rau (MPE) and Axel Schwope (AIP) - compact objects working group

  • Type 1 sources: known X-ray emitters (famous but a minority of sources)
  • Type 2 sources: standard multi-wavelength catalogs... position, flux, morphology and variability information needed
  • Most are galactic sources (also LMC and SMC), but not true for all....
  • Variability - on different timescales-- typically shorter timescales than AGN
  • Lack of a counterpart is also important information
  • Proper motions would be key way to separate CV and AGN-- otherwise only Spectra can do this
    • o Galaxy extent also useful for AGN... (but not QSO's)
  • Showed the Catalina Real Time Survey-- nice variability survey

Werner Becker, Tom - SNe Remnants

Mara - AGN

  • could we test for variability on PS1 and DES?
  • can we work together to combine data from different bands? (i, UKIDS/WISE/DES?)

Discussion items:

  • specific questions:
    • We need some kind of footprint service-- using Mangle???
    • Start with crude coverage maps... ultimately will likely need detailed coverage maps.
    • Healpix has been thought of, but it's not very efficient...
    • Polygons seem to be better for this- well accepted.
    • Database server- bringing the Johns Hopkins here to start with quickly. It would be at the Rechenzentrum.
    • New person would be hired at MPE to handle this work.
  • A shared region of the sky.... Stripe82 is an option. 2 deg^2 would be a good start. PS1+DES+SDSS....
  • Discussion of links to the images from particular surveys for...
    • need to store the coadds and offer cutouts....
    • need an interactive tool to create cutouts... this serves most people.
  • Discussion of X-ray image cutouts... should it be in image space or
    • should it be the photon lists.
      • Tom doing this for spectra and light curves...
      • Would work for lists of sources... is good for stacking...
      • X-ray contour line overlays for survey cutouts
  • Further discussion of database issues....
    • looking for an additional person supported by MPE...
    • will try to get Marion Cadolle Bel involved in this, starting this fall
    • RZG is sharing DBA half and half with MPA...
  • To do list: by October...
    • Joe: will track down PS1 and DES photometry over stripe 82... get back to Mara about this.
    • Hermann, Gerard, Jaiwon... - will look into database issues
      • will interact wit RZG re. hosting JHU SkyQuery catalog DB (cortesy Alex Szalay, see GL's/HB's presentations)

      • will look into attaching Millenium/TAP services to SkyQuery DB

      • longterm (given availability of suitable developer/maintainer): port functionality of Frank's SMC DB system to SkyQuery/Millenium/TAP, tailor for eROSITA...
  • Will post talks on the wiki... (for now)
    • will try to circulate notes, too...
  • Discussion of October meeting --
    • Schedule for the next consortium meeting....
      • + 2.5 days of meeting...

EROSITAwiki: DiscussionNotes (last edited 2013-07-30 10:01:19 by HermannBrunner)