- Science Users Information
-
- Observing Facilities
- Future Facilities and Development
- Observing with ESO Telescopes
- Policies and Procedures
- Telescope Time Allocation
- Phase 1 Proposals
- Phase 2 Preparation
- Observing conditions
- Service Mode Philosophy
- Service Mode Policies
- Phase 2 Instrument Table
- Service Mode Guidelines
- Special Procedures
- Visitor Mode Guidelines
- The p2 Tool
- Other Tools and Services
- Run Progress Report
- Post-observation Support
- Using ESO Mac & Linux software repositories
- Using conda with esoreflex
- The User Support Department
- User Workshops
- Phase 3
- Public Surveys
- Observing Tools and Services
- Visiting Astronomers
- Phase 2 Preparation
- Observing conditions
- Service Mode Philosophy
- Service Mode Policies
- Phase 2 Instrument Table
- Service Mode Guidelines
- Special Procedures
- Visitor Mode Guidelines
- The p2 Tool
- Other Tools and Services
- Run Progress Report
- Post-observation Support
- Using ESO Mac & Linux software repositories
- Using conda with esoreflex
- The User Support Department
- User Workshops
- APEX Science Verification
- Science in Garching and Santiago
- Science in Garching
- Science in Santiago
- Special Visitor Programme for Scientists working in Ukraine
- Fellowships and Studentships
- PhD Thesis Topics offered by ESO Faculty Members
- Instrument Commissioning
- VLT/VLTI Science Verification
- VISTA Science Verification
GD 108
alpha(2000) = 10h 00m 47.33s , delta(2000) = -07d 33' 31.2''
V = 13.56, B-V = -0.22, Spectral type: sdB
Field is 14.0 x 14.0 arcmin
Oke (1990) data (1A steps 3200-4700A; 2A steps 4702-9200A) + IUE (1.2A steps 2000A; 1.8A steps 2000-3200A). Note the limitations of these Oke data; see Cautionary Note.
ftp access to visible wavelength data files for this standard
ftp access to UV+visible wavelength data files for this standard