RUNID | PI Name | Prg Type | I-time (h) | Grade | Title |
---|---|---|---|---|---|
19AC13 | Wade | Regular | 2.7 | A | The surprising discovery of a strong magnetic field in the late B-type star HD 221218 |
19AC19 | Shultz | Regular | 7.0 | A | HD 62658: A New Magnetic Eclipsing Hot Binary? |
19AC20 | Shultz | Regular | 2.0 | A | Long- and Short-Term Monitoring of the Ultra-Slowly Rotating Magnetic beta Cep Star xi1 CMa |
19AC22 | Shultz | Regular | 2.0 | A | Magnetic Mapping of the Bp Auroral Magnetosphere Star 3 Sco |
19AC04 | Landstreet | Regular | 12.0 | B | Time series of circular polarisation spectra of magnetic WD1105-340 |
19AC05 | Wade | Regular | 1.0 | B | Measuring the ultra-slow rotation of the magnetic O star HD 54879 |
19AC14 | Wade | Regular | 22.0 | B | Characterisation of the magnetic fields of early-type giants: testing the principle of stellar magnetic flux conservation |
19AC01 | Khalack | Regular | 2.02 | C | Study of the spectral variability of HD85504 |
19AC02 | Perron-Cormier | Regular | 1.42 | C | Revealing the nature of HD176232 |
19AC28 | Farhang | Regular | 5.3 | C | The Northern Complement to the EDIBLES survey (ENCorE) |
19AF11 | Ibata | Regular | 15.0 | A | Exploring the dark sector with Gaias stellar streams |
19AF04 | Bouvier | Regular | 14.2 | B | Deciphering the magnetospheric star-disk interaction process in the young star V2062 Oph |
19AF09 | Carmona | Regular | 20.6 | B | Magnetic field topology in the young eruptive star EX Lup |
19AF20 | Neiner | Regular | 22.0 | C | Characterisation of the magnetic fields of early-type giants: testing the principle of stellar magnetic flux conservation |
19AF21 | Catelan | Snapshot | 26.0 | S | Gaia-based kinematic survey of Blue Horizontal Branch stars in the local Halo |
19AO36 | Helminiak | Regular | 2.25 | B | Radial velocities of the "impossible triple star" - testing multiplicity,deriving masses, and supporting a new hypothesis |
19AT07 | Lee | Regular | 7.4 | A | Follow-up Spectroscopic Observations of Two Be Stars Recently with Eruptive Phase and Quiet Phase |