SwgGal (r1.1 vs. r1.8)

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<<O>> Difference Topic SwgGal (r1.8 - 07 May 2004 - MarcoLeoni)

  META TOPICPARENT  ScienceWorkingGroup
-<
<
+  Galaxy Structure and Formation Working Group
->
>
+  Galaxy Structure and Formation Working Group
-<
<
+  Co-Chairs: Pepi Fabbiano (pepi@head.cfa.harvard.edu) and Richard de Grijs (R.deGrijs@sheffield.ac.uk)
->
>
+  Co-Chairs: Pepi Fabbiano (pepi@head.cfa.harvard.edu) and Richard de Grijs (R.deGrijs@sheffield.ac.uk)
-<
<
+  Meeting Overviews
->
>
+  Meeting Overviews
-<
<
+  Jan 21 2003
->
>
+  Jan 21 2003
 Notes from this meeting are avalable here
-<
<
+  Jan 28 2004
->
>
+  Jan 28 2004
 The group assessed options for scientific drivers.
-<
<
+  Telecons
->
>
+  Telecons
-<
<
+  Science Cases
->
>
+  Science Cases
-<
<
+. Stellar population parameters (age, metallicity, extinction, mass)

 2. Stellar population parameters plus internal kinematics from high-resolution spectra

 3. Spectral time variability of AGN

 4. Cross-ID cases: proper motion, weird populations, identifications of X-ray sources, morphology of galaxies at different redshifts
->
>
+ Stellar population parameters (age, metallicity, extinction, mass)

 Stellar population parameters plus internal kinematics from high-resolution spectra

 Spectral time variability of AGN

 Cross-ID cases: proper motion, weird populations, identifications of X-ray sources, morphology of galaxies at different redshifts
-<
<
+  Background Materials
->
>
+  Background Materials
  META FILEATTACHMENT  table_Jan28.ppt  attr="h" comment="" date="1075297105" path="C:\Documents and Settings\Administrator\My Documents\AVO_ADEC\table_Jan28.ppt" size="30208" user="NicholasWalton" version="1.1" 
 META FILEATTACHMENT  table_Jan28.pdf  attr="h" comment="slides written up during splinter session" date="1076436542" path="table_Jan28.pdf" size="14025" user="MarkusDolensky" version="1.1"
- META FILEATTACHMENT
+ attr="h" comment="" date="1075297105" path="C:\Documents and Settings\Administrator\My Documents\AVO_ADEC\table_Jan28.ppt" size="30208" user="NicholasWalton" version="1.1"
- META FILEATTACHMENT
+ attr="h" comment="slides written up during splinter session" date="1076436542" path="table_Jan28.pdf" size="14025" user="MarkusDolensky" version="1.1"

<<O>> Difference Topic SwgGal (r1.7 - 05 May 2004 - PaoloPadovani)

META TOPICPARENT	ScienceWorkingGroup

Galaxy Structure and Formation Working Group

Line: 29 to 29

Science Cases

Added:

>
>

1. Stellar population parameters (age, metallicity, extinction, mass)
2. Stellar population parameters plus internal kinematics from high-resolution spectra
3. Spectral time variability of AGN
4. Cross-ID cases: proper motion, weird populations, identifications of X-ray sources, morphology of galaxies at different redshifts

Background Materials

<<O>> Difference Topic SwgGal (r1.6 - 31 Mar 2004 - MarcoLeoni)

META TOPICPARENT	ScienceWorkingGroup

Galaxy Structure and Formation Working Group

Changed:

<
<

Co-Chairs: Pepi Fabbiano (pepi@head.cfa.harvard.edu) and Richard de Grijs (R.deGrijs@sheffield.ac.uk)

>
>

Co-Chairs: Pepi Fabbiano (pepi@head.cfa.harvard.edu) and Richard de Grijs (R.deGrijs@sheffield.ac.uk)

Added:

>
>

Added:

>
>

TOC: No TOC in "Avo.SwgGal"

Meeting Overviews

<<O>> Difference Topic SwgGal (r1.5 - 10 Feb 2004 - MarkusDolensky)

META TOPICPARENT	ScienceWorkingGroup

Galaxy Structure and Formation Working Group

Line: 16 to 16

The group assessed options for scientific drivers.

Changed:

<
<

The slides are available in ppt format

>
>

Here is the report (.pdf, .ppt).

Line: 29 to 29

Background Materials

META FILEATTACHMENT	table_Jan28.ppt	attr="h" comment="" date="1075297105" path="C:\Documents and Settings\Administrator\My Documents\AVO_ADEC\table_Jan28.ppt" size="30208" user="NicholasWalton" version="1.1"

Added:

>
>

META FILEATTACHMENT	table_Jan28.pdf	attr="h" comment="slides written up during splinter session" date="1076436542" path="table_Jan28.pdf" size="14025" user="MarkusDolensky" version="1.1"

<<O>> Difference Topic SwgGal (r1.4 - 05 Feb 2004 - RdeGrijs)

META TOPICPARENT	ScienceWorkingGroup

Galaxy Structure and Formation Working Group

Changed:

<
<

Co-Chairs: Pepi Fabbiano (pepi@head.cfa.harvard.edu) and Richard de Grijs (R.DeGrijs@sheffield.ac.uk)

>
>

Co-Chairs: Pepi Fabbiano (pepi@head.cfa.harvard.edu) and Richard de Grijs (R.deGrijs@sheffield.ac.uk)

<<O>> Difference Topic SwgGal (r1.3 - 04 Feb 2004 - PaoloPadovani)

META TOPICPARENT	ScienceWorkingGroup

Galaxy Structure and Formation Working Group

Deleted:

<
<

Added:

>
>

Co-Chairs: Pepi Fabbiano (pepi@head.cfa.harvard.edu) and Richard de Grijs (R.DeGrijs@sheffield.ac.uk)

Meeting Overviews

Changed:

<
<

Jan 2003

>
>

Jan 21 2003

Changed:

<
<

Notes from this meeting are avalable at ...

>
>

Notes from this meeting are avalable here

Jan 28 2004

<<O>> Difference Topic SwgGal (r1.2 - 28 Jan 2004 - NicholasWalton)

META TOPICPARENT	ScienceWorkingGroup

Changed:

<
<

?Title?

>
>

Galaxy Structure and Formation Working Group

Added:

>
>

Meeting Overviews

Changed:

<
<

<!--

- Set ALLOWTOPICRENAME = TWikiAdminGroup

-->

>
>

Jan 2003

Notes from this meeting are avalable at ...

Jan 28 2004

The group assessed options for scientific drivers.

The slides are available in ppt format

Telecons

Science Cases

Background Materials

META FILEATTACHMENT	table_Jan28.ppt	attr="h" comment="" date="1075297105" path="C:\Documents and Settings\Administrator\My Documents\AVO_ADEC\table_Jan28.ppt" size="30208" user="NicholasWalton" version="1.1"

<<O>> Difference Topic SwgGal (r1.1 - 28 Jan 2004 - NicholasWalton)

Line: 1 to 1

Added:

>
>

META TOPICPARENT	ScienceWorkingGroup

?Title?

<!--

- Set ALLOWTOPICRENAME = TWikiAdminGroup

-->

Revision r1.1 - 28 Jan 2004 - 13:04 - NicholasWalton
Revision r1.8 - 07 May 2004 - 13:21 - MarcoLeoni