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 <<O>>  Difference Topic ChamaeleonWorkflow (r1.15 - 30 Jan 2004 - MarcoLeoni)

META TOPICPARENT GalacticScenario
Deleted:
<
<

Chamaeleon SFR

Line: 20 to 19

Changed:
<
<
  • Load > Surveys in Vizier Vizier
>
>
  • Load > Surveys in Vizier

    • Load 2MASS
  • Make sure contours and catalogue are higher in stack, use zoom window to shift 2MASS field of view to select region with ISO contours (2/3 magnification).
    • Note about a dozen ISO sources (YSO, HH objects etc.)

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.14 - 26 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario
Added:
>
>

Chamaeleon SFR

Chamaeleon SFR near PMS star HD97048

Changed:
<
<
links are to Aladin screenshots
>
>
Links in normal type are to Aladin screenshots on wiki page http://www.euro-vo.org/twiki/bin/view/Avo/ChamaeleonWorkflow

  • Target HD97048
Changed:
<
<
    • Radius 10 arcmin at all times
  • VOdemo tab
  • Vizier surveys
    • 2MASS, load,
  • Make sure contours and catalogue are higher in stack, view 2MASS and zoom in on good ISO region
>
>
  • Default search radius unless specified
  • Load > VOdemo tab
  • Load > Aladin tab, tree view
  • Main window
  • Load > Surveys in Vizier Vizier
    • Load 2MASS
  • Make sure contours and catalogue are higher in stack, use zoom window to shift 2MASS field of view to select region with ISO contours (2/3 magnification).

    • Note about a dozen ISO sources (YSO, HH objects etc.)
Changed:
<
<
  • Plugins - VOPlot (developed by VO India)
>
>

    • Functions menu in VOPlot
      • VOPlot Create Filters (to exclude points if Kmag error > 0.2)
Changed:
<
<
>
>

  • In main Aladin window,
Changed:
<
<
>
>

      • HD97048 probably Class II, other objects II and I or II
Changed:
<
<
    • VOPlot Mode Select
>
>
    • VOPlot Mode
      • Clear all Selections
      • Select

      • Use cursor (drag from top left) to select various regions in VOPlot colour-colour plot, e.g. Class III have [J-H]<1.6 and [H-K]<0.4
Changed:
<
<
>
>

  • Central 3 objects
    • All bright at K-band and ISO 7 um
    • HD97048 maybe more evolved, later class?
    • Or evolving faster - higher mass?
Changed:
<
<
>
>

    • HD97048 faint very soft
      • suggests high-mass evolved YSO
    • Two objects above have bluer=harder X-ray colours
Line: 53 to 59

    • Other objects with redder=softer X-ray colours
      • suggests low-mass T Tauri stars
Changed:
<
<
Suggested classification of ISO-bright objects around HD97048 (5 in image):

Aladin image No. JHK Colour age-class X-ray mass for age
1 I/II non-det. - v. embedded?
2 II soft - low-mass
3 I/II hard - young low-mass
4 II medium-hard - youngish low-mass
5 II v.faint soft - older/high mass
6 II soft? (chip edge) - older/low mass
7 II soft - low-mass/late
8 II/III non-det. - high-mass?

Also see

J/AJ/121/974 JHK photometry in Cha I (Gomez+, 2001)
J/A+A/357/219 ISOCAM observations in Cha I. (Persi+, 2000)
>
>
-- AnitaRichards - 26 Jan 2004

<!--

Line: 78 to 67

META FILEATTACHMENT CHAMAELEON.png attr="" comment="Workflow for AVO investigation of Chamaeleon" date="1075108229" path="CHAMAELEON.png" size="11044" user="AnitaRichards" version="1.2"
Added:
>
>
META FILEATTACHMENT cham10_xmmsel.png attr="h" comment="" date="1075114023" path="cham10_xmmsel.png" size="327190" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham11_xmmrgb.png attr="h" comment="" date="1075114043" path="cham11_xmmrgb.png" size="430367" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham12_xmmzoom.png attr="h" comment="" date="1075114059" path="cham12_xmmzoom.png" size="439563" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham1_loadiso.png attr="h" comment="" date="1075114076" path="cham1_loadiso.png" size="233366" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham2_load2mass.png attr="h" comment="" date="1075114106" path="cham2_load2mass.png" size="360125" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham3_isocontours.png attr="h" comment="" date="1075114132" path="cham3_isocontours.png" size="343652" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham4_2masscat.png attr="h" comment="" date="1075114155" path="cham4_2masscat.png" size="318530" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham5_vofilt.png attr="h" comment="" date="1075114180" path="cham5_vofilt.png" size="181174" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham6_vocol.png attr="h" comment="" date="1075114202" path="cham6_vocol.png" size="188520" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham7_voplot.png attr="h" comment="" date="1075114223" path="cham7_voplot.png" size="170437" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham8_vohd.png attr="h" comment="" date="1075114244" path="cham8_vohd.png" size="306723" user="AnitaRichards" version="1.1"
META FILEATTACHMENT cham9_voiii.png attr="h" comment="" date="1075114264" path="cham9_voiii.png" size="309573" user="AnitaRichards" version="1.1"

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.13 - 26 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 76 to 76

-->

Changed:
<
<
META FILEATTACHMENT CHAMAELEON.png attr="" comment="Workflow for AVO investigation of Chamaeleon" date="1075050167" path="CHAMAELEON.png" size="119596" user="AnitaRichards" version="1.1"
>
>

META FILEATTACHMENT CHAMAELEON.png attr="" comment="Workflow for AVO investigation of Chamaeleon" date="1075108229" path="CHAMAELEON.png" size="11044" user="AnitaRichards" version="1.2"

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.12 - 25 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 75 to 75

<!-- -->
Added:
>
>

META FILEATTACHMENT CHAMAELEON.png attr="" comment="Workflow for AVO investigation of Chamaeleon" date="1075050167" path="CHAMAELEON.png" size="119596" user="AnitaRichards" version="1.1"

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.11 - 22 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 33 to 33

    • Hover over HD97048 and other 2 central ISO/2MASS objects
    • In VOPlot window note positions in VOPlot
    • Also select objects
Changed:
<
<
    • Compare with JHK colour-colour regions Haisch et al. 2000 AJ 120 1396 fig. 8
>
>

      • HD97048 probably Class II, other objects II and I or II
    • VOPlot Mode Select
      • Use cursor (drag from top left) to select various regions in VOPlot colour-colour plot, e.g. Class III have [J-H]<1.6 and [H-K]<0.4

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.10 - 22 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 10 to 10

  • Target HD97048
    • Radius 10 arcmin at all times
Changed:
<
<
  • VOdemo
    • ISO Images
      • Load ISO CAM01 SE,
>
>
  • VOdemo tab
    • ISO Images (discovered directly from the ISO Archive)
      • Load ISO CAM01 SE
        • Make ISO contours

Added:
>
>
    • Aladin tab
      • 2MASS K

  • Vizier surveys
Changed:
<
<
    • 2MASS, load, zoom in on good ISO region
>
>
    • 2MASS, load,
  • Make sure contours and catalogue are higher in stack, view 2MASS and zoom in on good ISO region

    • Note about a dozen ISO sources (YSO, HH objects etc.)
Changed:
<
<
  • Plugins - VOPlot
>
>
  • Plugins - VOPlot (developed by VO India)

Line: 25 to 29

        • name J-H, expression $3-$4
        • name H-K, expression $4-$5
    • Select Y-axis J-H, X-axis H-K, Filter Kaccurate and Plot
Deleted:
<
<
      • Compare with No. of outliers if Filter All is selected

  • In main Aladin window,
Changed:
<
<
    • Click on central object HD97048
    • Select all 3 central ISO/2MASS objects
  • In VOPlot window, note
    • HD97048 red
    • all 3 objects in green boxes
>
>
    • Hover over HD97048 and other 2 central ISO/2MASS objects
    • In VOPlot window note positions in VOPlot
    • Also select objects

    • Compare with JHK colour-colour regions Haisch et al. 2000 AJ 120 1396 fig. 8
      • HD97048 probably Class II, other objects II and I or II
    • VOPlot Mode Select
Line: 42 to 43

    • HD97048 maybe more evolved, later class?
    • Or evolving faster - higher mass?
  • Aladin Load VOdemo
Changed:
<
<
>
>


 <<O>>  Difference Topic ChamaeleonWorkflow (r1.9 - 22 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 15 to 15

Changed:
<
<
    • 2MASS, load
  • Select 2MASS K image as view, overlaid with sources and ISO contours
    • Zoom in to x2
>
>
    • 2MASS, load, zoom in on good ISO region

    • Note about a dozen ISO sources (YSO, HH objects etc.)
  • Plugins - VOPlot
    • Functions menu in VOPlot
Line: 36 to 34

    • all 3 objects in green boxes
    • Compare with JHK colour-colour regions Haisch et al. 2000 AJ 120 1396 fig. 8
      • HD97048 probably Class II, other objects II and I or II
Changed:
<
<
    • Mode Select
>
>
    • VOPlot Mode Select

  • Central 3 objects
    • All bright at K-band and ISO 7 um
    • HD97048 maybe more evolved, later class?
    • Or evolving faster - higher mass?
Changed:
<
<
  • VOdemo
>
>
  • Aladin Load VOdemo

Changed:
<
<
>
>

    • HD97048 faint very soft
      • suggests high-mass evolved YSO
    • Two objects above have bluer=harder X-ray colours

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.8 - 22 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 10 to 10

  • Target HD97048
    • Radius 10 arcmin at all times
Changed:
<
<
  • VOTest
    • SkyView
      • Load 2MASS K
>
>
  • VOdemo

Changed:
<
<
  • Vizier catalogues
    • Catalogue 2MASS, load
>
>
  • Vizier surveys
    • 2MASS, load

  • Select 2MASS K image as view, overlaid with sources and ISO contours
    • Zoom in to x2
    • Note about a dozen ISO sources (YSO, HH objects etc.)
Line: 39 to 37

    • Compare with JHK colour-colour regions Haisch et al. 2000 AJ 120 1396 fig. 8
      • HD97048 probably Class II, other objects II and I or II
    • Mode Select
Changed:
<
<
      • Use cursor to select various regions in VOPlot colour-colour plot, e.g. Class III have [J-H]<1.6 and [H-K]<0.4
>
>
      • Use cursor (drag from top left) to select various regions in VOPlot colour-colour plot, e.g. Class III have [J-H]<1.6 and [H-K]<0.4

Changed:
<
<
  • VOTest
>
>
  • VOdemo


 <<O>>  Difference Topic ChamaeleonWorkflow (r1.7 - 20 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 39 to 39

    • Compare with JHK colour-colour regions Haisch et al. 2000 AJ 120 1396 fig. 8
      • HD97048 probably Class II, other objects II and I or II
    • Mode Select
Changed:
<
<
      • Select various regions in VOPlot
>
>
      • Use cursor to select various regions in VOPlot colour-colour plot, e.g. Class III have [J-H]<1.6 and [H-K]<0.4


 <<O>>  Difference Topic ChamaeleonWorkflow (r1.6 - 20 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 22 to 22

    • Zoom in to x2
    • Note about a dozen ISO sources (YSO, HH objects etc.)
  • Plugins - VOPlot
Changed:
<
<
    • Functions
      • Create Filters (to exclude points if Kmag error > 0.2)
>
>
    • Functions menu in VOPlot
      • VOPlot Create Filters (to exclude points if Kmag error > 0.2)

Line: 37 to 37

    • HD97048 red
    • all 3 objects in green boxes
    • Compare with JHK colour-colour regions Haisch et al. 2000 AJ 120 1396 fig. 8
Deleted:
<
<

      • HD97048 probably Class II, other objects II and I or II
    • Mode Select
      • Select various regions in VOPlot

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.5 - 17 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Line: 36 to 36

Changed:
<
<
    • Compare with JHK colour-colour regions **insert reference
>
>
    • Compare with JHK colour-colour regions Haisch et al. 2000 AJ 120 1396 fig. 8

      • HD97048 probably Class II, other objects II and I or II
    • Mode Select
      • Select various regions in VOPlot

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.4 - 16 Jan 2004 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR

Changed:
<
<

Chamaeleon SFR within 1' of PMS star HD97048

>
>

Chamaeleon SFR near PMS star HD97048


Changed:
<
<
Use HD97048 as object to initiate search in Aladin.
>
>
links are to Aladin screenshots

Deleted:
<
<
Display Skyview 2mass K, J, and HST WFPC images - could make false-colour image.

Changed:
<
<
There is a group of 3 stars, all fairly red:
>
>
  • Target HD97048
    • Radius 10 arcmin at all times
  • VOTest
  • Vizier catalogues
    • Catalogue 2MASS, load
  • Select 2MASS K image as view, overlaid with sources and ISO contours
    • Zoom in to x2
    • Note about a dozen ISO sources (YSO, HH objects etc.)
  • Plugins - VOPlot
  • In main Aladin window,
    • Click on central object HD97048
    • Select all 3 central ISO/2MASS objects
  • In VOPlot window, note
  • Central 3 objects
    • All bright at K-band and ISO 7 um
    • HD97048 maybe more evolved, later class?
    • Or evolving faster - higher mass?
  • VOTest
  • Make X-ray RGB image and note
    • HD97048 faint very soft
      • suggests high-mass evolved YSO
    • Two objects above have bluer=harder X-ray colours
      • suggests early, embedded YSO
    • Other objects with redder=softer X-ray colours
      • suggests low-mass T Tauri stars

Suggested classification of ISO-bright objects around HD97048 (5 in image):

Aladin image No. JHK Colour age-class X-ray mass for age
1 I/II non-det. - v. embedded?
2 II soft - low-mass
3 I/II hard - young low-mass
4 II medium-hard - youngish low-mass
5 II v.faint soft - older/high mass
6 II soft? (chip edge) - older/low mass
7 II soft - low-mass/late
8 II/III non-det. - high-mass?

Deleted:
<
<
ISO-ChaI 126   ISO-ChaI 119
reddest   reddish
x-ray bright   x-ray bright
     
  HD97048 ISO-ChaI 124  
  brightest in optical  
  but still red  

Deleted:
<
<
Make contours e.g. from K-band image to overlay on other images.

Find ISO catalogue and display image (local load if necessary - CAM4 csp7190168801.fits) - all three objects are still bright. ISO astrometry is off but ID is obvious.

Do the same with XMM - in x-ray HD97048 is much less bright suggesting that it is a higher-mass star and the others are T Tauri's

Could also use ACE and SED tool to extract and plot IR to X-ray spectra for each source.

HD97048 has ISO LWS data, can display spectrum (lsan prefix?), measure 60, 100 and 170 micron flux and use colours to estimate age Pezzuto et al. 2002 MNRAS 330 1034, see GalacticRequirements

If we can use the ISO CVF spectra, we can first ascertain the total contributions of each of the 3 stars from the ISO image (dominated at 7 micron by HD97048) and then use the 7 and 15 micron flux and the criteria from Felli et al. 2002 A&A 392 971.


Also see


 <<O>>  Difference Topic ChamaeleonWorkflow (r1.3 - 18 Dec 2003 - MarcoLeoni)

META TOPICPARENT GalacticScenario
Changed:
<
<

Chamaeleon SFR


>
>

Chamaeleon SFR


Deleted:
<
<
Chamaeleon SFR within 1' of PMS star HD97048

Changed:
<
<
Use HD97048 as object to initiate search in Aladin
>
>

Chamaeleon SFR within 1' of PMS star HD97048


Changed:
<
<
Display Skyview 2mass K, J, and HST WFPC images - could make false-colour image
>
>
Use HD97048 as object to initiate search in Aladin.

Display Skyview 2mass K, J, and HST WFPC images - could make false-colour image.


There is a group of 3 stars, all fairly red:

Line: 40 to 39

criteria from Felli et al. 2002 A&A 392 971.
Changed:
<
<
Also see:
>
>

Also see


J/AJ/121/974 JHK photometry in Cha I (Gomez+, 2001)
J/A+A/357/219 ISOCAM observations in Cha I. (Persi+, 2000)

 <<O>>  Difference Topic ChamaeleonWorkflow (r1.2 - 17 Nov 2003 - AnitaRichards)

META TOPICPARENT GalacticScenario

Chamaeleon SFR


Line: 40 to 40

criteria from Felli et al. 2002 A&A 392 971.
Changed:
<
<

>
>
Also see:
J/AJ/121/974 JHK photometry in Cha I (Gomez+, 2001)
J/A+A/357/219 ISOCAM observations in Cha I. (Persi+, 2000)

<!--


 <<O>>  Difference Topic ChamaeleonWorkflow (r1.1 - 27 Oct 2003 - AnitaRichards)
Line: 1 to 1
Added:
>
>
META TOPICPARENT GalacticScenario

Chamaeleon SFR


Chamaeleon SFR within 1' of PMS star HD97048

Use HD97048 as object to initiate search in Aladin

Display Skyview 2mass K, J, and HST WFPC images - could make false-colour image

There is a group of 3 stars, all fairly red:

ISO-ChaI 126   ISO-ChaI 119
reddest   reddish
x-ray bright   x-ray bright
     
  HD97048 ISO-ChaI 124  
  brightest in optical  
  but still red  

Make contours e.g. from K-band image to overlay on other images.

Find ISO catalogue and display image (local load if necessary - CAM4 csp7190168801.fits) - all three objects are still bright. ISO astrometry is off but ID is obvious.

Do the same with XMM - in x-ray HD97048 is much less bright suggesting that it is a higher-mass star and the others are T Tauri's

Could also use ACE and SED tool to extract and plot IR to X-ray spectra for each source.

HD97048 has ISO LWS data, can display spectrum (lsan prefix?), measure 60, 100 and 170 micron flux and use colours to estimate age Pezzuto et al. 2002 MNRAS 330 1034, see GalacticRequirements

If we can use the ISO CVF spectra, we can first ascertain the total contributions of each of the 3 stars from the ISO image (dominated at 7 micron by HD97048) and then use the 7 and 15 micron flux and the criteria from Felli et al. 2002 A&A 392 971.

<!--

-->

Revision r1.1 - 27 Oct 2003 - 17:34 - AnitaRichards
Revision r1.15 - 30 Jan 2004 - 14:46 - MarcoLeoni
Copyright © 2003 by the contributing authors. All material on this collaboration tool is the property of the contributing authors. Ideas, requests, problems regarding AVO TWiki ? Send feedback.