- 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
CD-34 241
alpha(2000) = 00h 41m 46.92s , delta(2000) = -33d 39' 08.5''
V = 11.23, B-V = +0.48, Spectral type: F
Field is 10.0 x 10.0 arcmin
Hamuy et al (1992, 1994) data (50A bins)
Note that this star is mistakenly named LTT 377 in Hamuy et al. (1992, 1994)
ftp access to visible wavelength data files for this standard