Differences between revisions 1 and 7 (spanning 6 versions)
⇤ ← Revision 1 as of 2013-11-24 14:58:28 →
Size: 449
Editor: NikolaiPiskunov
Comment:
← Revision 7 as of 2013-12-02 12:45:57 → ⇥
Size: 1440
Editor: ThomasMarquart
Comment: remove comflict
Deletions are marked like this. Additions are marked like this.
Line 1: Line 1:
= The VALD3/SHoP/SME workshop = = Uppsala-Moscow VALD3/SHoP/SME workshop =
Line 4: Line 4:
Participants: === Participants: ===
Line 6: Line 6:
 * S. Alexeeva (INASAN)
 * U. Heiter (UU)
 * L.I. Mashonkina (INASAN)
 * B. Nizamov (INASAN)
 * T. Nordlander (UU)
 * Yu. Pakhomov (INASAN)
 * N. Piskunov (UU)
 * T.A. Ryabchikova (INASAN)
 * T. Sitnova (INASAN)
 * E. Stempels (UU)
 * A. Titarenko (INASAN)
 * ...
Line 7: Line 19:
=== Presentations on SHoP/SME: ===
Line 8: Line 21:
1) Selection of target stars
2) Data reduction and rectification of the continuum
3) Selection of line data and spectral segments
4) Testing line data
5) Global stellar parameters with SME
6) Uncertainties
7) LTE abundance analysis
8) NLTE abundance analysis
9) Paper		  1. Introduction (N. Piskunov)
 1. Selection of target stars (A. Titarenko)
 1. Data reduction and rectification of the continuum (N. Piskunov, Yu. Pakhomov, B. Nizamov)
 1. Selection of line data and spectral segments (T. Ryabchikova)
 1. Testing line data (A. Titarenko, T. Ryabchikova)
 1. Global stellar parameters with SME (T. Ryabchikova, A. Titarenko)
 1. Uncertainties (T. Ryabchikova, L. Mashonkina, Yu. Pakhomov, A. Titarenko)
 1. LTE abundance analysis (T. Ryabchikova, A. Titarenko, T. Sitnova, S. Alexeeva, B. Nizamov)
 1. NLTE abundance analysis
        8.#1 "Stellar chemical abundances based on NLTE" L. Mashonkina
        8. "NLTE analysis of O and Ca" T. Sitnova
        8. "NLTE analysis of C and Na" S. Alexeeva
Line 18: Line 34:
VALD 3
1) Current status
2) Outstanding problems
3) Announcement
4) Paper		 === Presentations on VALD3: ===

 1. Current status of software (N. Piskunov)
 1. Current status of data (T. Ryabchikova)
 1. Outstanding problems - general discussion
 
=== Other agenda items ===
 
 1. Writing the VALD3 paper
 1. Writing the SHoP paper

Uppsala-Moscow VALD3/SHoP/SME workshop

Uppsala 25-29 November 2013

Participants:

  • S. Alexeeva (INASAN)
  • U. Heiter (UU)
  • L.I. Mashonkina (INASAN)
  • B. Nizamov (INASAN)
  • T. Nordlander (UU)
  • Yu. Pakhomov (INASAN)
  • N. Piskunov (UU)
  • T.A. Ryabchikova (INASAN)
  • T. Sitnova (INASAN)
  • E. Stempels (UU)
  • A. Titarenko (INASAN)
  • ...

Presentations on SHoP/SME:

  1. Introduction (N. Piskunov)
  2. Selection of target stars (A. Titarenko)
  3. Data reduction and rectification of the continuum (N. Piskunov, Yu. Pakhomov, B. Nizamov)
  4. Selection of line data and spectral segments (T. Ryabchikova)
  5. Testing line data (A. Titarenko, T. Ryabchikova)
  6. Global stellar parameters with SME (T. Ryabchikova, A. Titarenko)
  7. Uncertainties (T. Ryabchikova, L. Mashonkina, Yu. Pakhomov, A. Titarenko)
  8. LTE abundance analysis (T. Ryabchikova, A. Titarenko, T. Sitnova, S. Alexeeva, B. Nizamov)
  9. NLTE abundance analysis
    1. "Stellar chemical abundances based on NLTE" L. Mashonkina
    2. "NLTE analysis of O and Ca" T. Sitnova
    3. "NLTE analysis of C and Na" S. Alexeeva

Presentations on VALD3:

  1. Current status of software (N. Piskunov)
  2. Current status of data (T. Ryabchikova)
  3. Outstanding problems - general discussion

Other agenda items

  1. Writing the VALD3 paper
  2. Writing the SHoP paper

ValdWiki: VALD3 final testing and paper writing. Uppsala, November 2013 (last edited 2013-12-02 12:45:57 by ThomasMarquart)