Approved
SST2020-519 |
Setting the stage for ground-based parallax of the nearest and brightest T subdwarf |
Approved
SST2020-518 |
Polarimetry of the super luminous supernova SN2020qlb |
Approved
SST2020-517 |
The hunt for the most massive neutron stars: PSR J1908+2105 |
Approved
SST2020-516 |
Determining the spectral type of a young SB2 and its wide companions |
SST2020-513 |
Metallicity determination of members of the young moving group 29 in Taurus |
Approved
SST2020-512 |
Spectroscopic characterisation of wide substellar companions to young nearby stars. |
Approved
SST2020-511 |
OCCASO survey: Calibration between used telescopes/instruments |
Approved
SST2020-510 |
Polarimetric follow-up of the gamma-ray binary PSR J2032+4127 |
Approved
SST2020-509 |
UCAC2 46706450 - a rapidly rotating K-type subgiant with an extremely hot white dwarf companion |
Approved
SST2020-508 |
Identification of strongly-lensed QSO systems |
Approved
SST2020-506 |
Spectroscopic confirmation of wide companions to M and L subdwarfs with Gaia and the Virtual Observatory |
Approved
SST2020-505 |
Measuring the SED of an enigmatic radio weak BL Lac object - the near-IR range |
Approved
SST2020-500 |
UV-VIS spectroscopic characterization of primitive asteroids |
Approved
SST2020-498 |
An insight to the low mass stars sequence in two open clusters |
Approved
SST2020-497 |
Blue-VIS spectroscopic characterization of primitive asteroids |
Approved
SST2020-496 |
Reconnaissance spectroscopy of 4 new M-type pre-main sequence stars |
SST2020-495 |
Fluorine in phosphorus -rich stars |
SST2020-492 |
Mapping basaltic material in the asteroid belt |
SST2020-490 |
Homogenous photometry of globular clusters |
Approved
SST2019-487 |
Study of the stellar parameters, individual atomic lines and Balmer-line profiles of LB1, the companion of the massive black hole |
Approved
SST2019-483 |
A "missing star" in the Milky Way |