Approved
SST2023-638 |
Inter-outburst evolution of the Halpha line Trough in HT Cas |
Approved
SST2023-637 |
Exploring the Spectral Characteristics of a Potential Hot White Dwarf hosting a Planet candidate |
Approved
SST2023-636 |
Atmospheric study of the sub-Neptune HR 858b |
Approved
SST2023-635 |
Characterizing nuclear outflows in Flat Spectrum Radio Quasars (II) |
Approved
SST2023-634 |
Characterizing nuclear outflows in Flat Spectrum Radio Quasars |
Approved
SST2023-632 |
INT follow-up of very metal-poor stars identified from Gaia XP spectra |
Approved
SST2023-631 |
Spectra (one slit) for an object near M104. |
SST2023-625 |
Estimating stellar rotation periods to unveil planetary signals in the KOBE experiment |
SST2023-623 |
Planet formation around massive stars: the key of the metals |
Approved
SST2023-622 |
Polarimetry of the gravitational lens system of the faded strongly lensed supernova 2022qmx (aka SN Zwicky) |
Approved
SST2023-621 |
Investigating Rapid Changes in the Dynamics of the emerging ionized wind at the core of M2-9 |
SST2023-620 |
Confirmation of the pre-main sequence (PMS) nature of selected candidates in the Taurus-Auriga field |
Approved
SST2023-617 |
Tracing the optical spectroscopic variability of the ULXP Swift J0243.6+6124 during its current giant outburst |
Approved
SST2023-616 |
Unravelling the origin of Anomalous Cepheids |
Approved
SST2023-615 |
Globular Clusters in the Gaia era |
SST2023-613 |
The KOBE experiment. Unveiling activity-induced radial velocities through the activity-rotation relation |
SST2023-612 |
Characterization of low-mass eclipsing binaries with IDS |
SST2023-607 |
The great dimming of RW Cep |
Approved
SST2023-606 |
A pending task to get to know Q0957+561 better |
SST2023-602 |
Understanding the nature of small planets across stellar types |
SST2023-601 |
A very-high-resolution spectroscopic legacy survey of the ISM in absorption |
Approved
SST2023-599 |
Characterizing the rotation effect on the lithium depletion pattern in coeval open clusters |
SST2023-598 |
Optical Spectroscopy of T Tauri Stars to Understand Planetary Formation |