- 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
Hz 43
alpha(2000) = 13h 16m 21.99s , delta(2000) = +29d 05' 57.0''
V = 12.91, B-V = -0.30, Spectral type: DA1
Field is 10.0 x 10.0 arcmin
Bohlin et al. (1995) FOS data + WD model atmosphere
ftp access to UV+visible wavelength data files for this standard