The Delta Scuti Network (DSN)
The Delta Scuti Network (DSN) is a collaboration of astronomers from all around
the globe who observe and study short period variable stars. It was founded by Michel
Breger at the University of Texas (McDonald Observatory) and at the University of Vienna
(Institute of Astronomy) in 1983 with the goal to improve the frequency solutions of
multiperiodic Delta Scuti stars.
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DSN observation sites
What is the advantage of multisite campaigns?
Further information:
What are the Delta Scuti Stars? Why do we observe Delta Scuti Stars? General properties of Delta Scuti Stars The history of Delta Scuti Stars What is Asteroseismology? Nonradial PulsationCampaigns of the DSN
| DSN 1 | Theta 2 Tauri | 1983 | |
| DSN 2 | 4 CVn | 1984 | |
| DSN 3 | Theta 2 Tauri | 1986 | |
| DSN 4 | HR729 | 1988 | |
| DSN 5 | BU Cnc & EP Cnc |
1989 | |
| DSN 6 | 63 Her | 1990 | |
| DSN 7 | HN CMa | 1990 | |
| DSN 8 | CD -24 7599 | 1992 | |
| DSN 9 | FG Vir | 1993 | |
| DSN 10 | IC 418 | 1993 | |
| DSN 11 | CD -24 7599 | 1994 | |
| DSN 12 | Theta 2 Tauri | 1994 | |
| DSN 13 | IC 418 | 1994 | |
| DSN 14 | FG Vir | 1995 | |
| DSN 15 | 4 CVn | 1996 | |
| DSN 16 | 4 CVn | 1997 | |
| DSN 17 | CD -24 7599 | 1998 | |
| DSN 18 | BI CMi | 1998/1999 | |
| DSN 19 | BI CMi | 1999/2000 | |
| DSN 20 | 44 Tau | 2000 | |
| DSN 21 | 44 Tau | 2001 | |
| DSN 22 | FG Vir | 2002 | |
| DSN 23 | FG Vir | 2003 | |
| DSN 24 | 44 Tau | 2003 | |
| DSN 25 | FG Vir | 2004 | |
| DSN 26 | 44 Tau | 2004 | |
| DSN 27 | HD210111 & AS Eri |
2005 | |
| DSN 28 | UV Oct & SS For | 2005 | |
| DSN 29 | 44 Tau | 2005 | |
| DSN 30 | 4 CVn | 2005 | |
| DSN 31 | 44 Tau | 2006 | |
| DSN 32 | 4 CVn | 2006 | |
| DSN 33 | EE Cam | 2006 | |
| DSN 34 | 4 CVn | 2007 | |
| DSN 35 | EE Cam | 2007 | |
| DSN 36 | 4 CVn | 2008 | |
| DSN 37 | EE Cam | 2008 |
Observing techniques |
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Photometry
The Three-Star Technique
Spectroscopy |