Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT (AB)

Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one (AB)

In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable) (AB)

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them (AB)

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known (AB)

-- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
  • Comparison of an observed SED with a theoretical model (Use Case 2)

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
  • topcat_aladin.jpg
  • case1_hist_plx_Pleiades.jpg
  • case1_Xray_source.jpg

  • Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image.

IPHAS and 2MASS color-color diagrams for matched point sources (case 4) selected in a box 1 degree wide and centred at ra=38.78 and deg=61.43

    • Use case 5: The field of streams
Topic attachments
I Attachment Action Size Date Who Comment
jpgjpg Aladin.jpg manage 49.4 K 01 Apr 2009 - 15:47 AidaSchool usercase1_a
jpgjpg Aladin_after.jpg manage 67.0 K 01 Apr 2009 - 15:48 AidaSchool usercase1_d
jpgjpg IMF_case.jpg manage 116.6 K 01 Apr 2009 - 15:39 AidaSchool Comparison of an observed SED with a theoretical model (Use Case 2)
pngpng Picture_5.png manage 255.5 K 02 Apr 2009 - 07:46 AidaSchool Halpha emitters in the IPHAS and 2MASS diagrams
pngpng VO_galaxy.png manage 667.0 K 01 Apr 2009 - 15:50 AidaSchool Galaxy and some foreground point sources.
pngpng Virgo2808.png manage 896.3 K 01 Apr 2009 - 16:10 AngelaBragaglia Virgo : NGC2808 & search for dataset of high-res VLT spectra
jpgjpg ana.jpg manage 199.2 K 01 Apr 2009 - 15:44 AidaSchool Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image.
jpgjpg case1_Xray_source.jpg manage 25.6 K 01 Apr 2009 - 16:07 AidaSchool The Xray sources in the field correspond to rhe bright stars.
jpgjpg case1_hist_plx_Pleiades.jpg manage 22.5 K 01 Apr 2009 - 16:14 AidaSchool Histogram of the paralax. Blue are the bright stars.
jpgjpg color_color2.jpg manage 48.8 K 01 Apr 2009 - 15:48 AidaSchool usercase1_c
jpgjpg histogram.jpg manage 23.2 K 01 Apr 2009 - 15:47 AidaSchool usercase1_b
jpgjpg im_all.jpg manage 18.8 K 01 Apr 2009 - 15:51 AidaSchool An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.
jpgjpg topcat_aladin.jpg manage 386.5 K 01 Apr 2009 - 15:59 AidaSchool Collaboration between TOPCAT and Aladin
pngpng tuvikene_streams.png manage 127.2 K 01 Apr 2009 - 15:37 AidaSchool Use Case 5: The Field of Streams
jpgjpg vospec.jpg manage 35.0 K 01 Apr 2009 - 15:16 AngelaBragaglia Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec
Topic revision: r12 - 02 Apr 2009 - 09:36:38 - AngelaBragaglia
 
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