Distribuição de Tempo 2026V - STELES Science Verification
Verificação de Ciência do STELES - Resultados da Seleção de Propostas e Alocação de Tempo
STELES Science Verification - Proposal Selection Results and Time Allocation
STELES Science Verification Program
The SOAR Telescope Echelle Spectrograph (STELES) will conduct its first Science Verification observations during the second half of 2026. The program is intended to demonstrate the instrument's scientific capabilities under real observing conditions and to provide the astronomical community with an initial assessment of its performance.
The Science Verification campaign comprises 11 nights of observing time, distributed across three observing runs in September, October, and December 2026 (more information is provided in the SV Call webpage). Observations will be conducted in queue mode by the STELES and SOAR teams, allowing targets to be selected according to their visibility and the prevailing observing conditions.
The program will focus on demonstrating the capabilities of STELES across its broad wavelength range, with particular emphasis on its high spectral resolution and near-UV sensitivity. The selected programs cover a broad range of scientific topics, providing an opportunity to assess the instrument's performance for different types of astronomical sources and observing strategies.
STELES SV Outcome
71 proposals received / 538.6 hours of telescope time requested
23 proposals selected / 100 hours of telescope time allocated
Oversubscription factor: 5.4
11 nights available (100 hours)
18 Institutions represented
Call for Proposals and TAC Evaluation
The Call for Proposals for the STELES Science Verification program was opened in July 2026 and was open to the astronomical community (link). Proposals were encouraged to make use of the distinctive capabilities of STELES, particularly its high spectral resolution, broad wavelength coverage, and near-UV sensitivity.
A total of 71 proposals were received, requesting a total of 538.6 hours of observing time. Following the evaluation, 23 programs were selected for execution, corresponding to approximately 32% of the submitted proposals. The total amount of time requested resulted in an oversubscription of 5.4 relative to the available Science Verification time (approximately 100 hours).
The proposals were evaluated by the STELES Science Verification Time Allocation Committee (TAC), which considered the scientific merit of each program, its suitability for the capabilities of STELES, the feasibility of the proposed observations, its potential contribution to the scientific verification of the instrument and the pressure factor of each observing run to accommodate all approved projects.
The selected programs represent a broad range of scientific topics and observing strategies, providing a representative test of STELES across different types of astronomical targets and scientific applications.
Scientific Scope of the Submitted Proposals
The proposals received for the STELES Science Verification program covered a broad range of scientific topics, reflecting the versatility of the instrument and the diverse interests of the astronomical community. The submitted programs included studies of stellar abundances and stellar astrophysics, star formation and young stellar objects, Solar System objects, exoplanets, emission-line and nebular sources, and time-domain phenomena, among other topics.
The distribution of proposals and requested observing time across the main scientific areas is summarized below. Both the number of proposals and the amount of requested time are shown, as these provide complementary measures of the scientific demand for STELES.
|
Scientific Area |
Submitted proposals |
Requested time (hours) |
|
Stellar abundances, stellar astrophysics |
27 |
184.3 |
|
Exoplanets |
10 |
74.3 |
|
Stellar populations, clusters, chemical evolution |
7 |
81.3 |
|
Binary/multiple stellar systems |
7 |
44.2 |
|
SNe, stellar remnants, compact objects, stellar mergers, GW counterparts |
7 |
73.2 |
|
ISM, HII, PNe, YSOs |
5 |
36.3 |
|
Solar System astrophysics |
3 |
22.4 |
|
Novae, cataclysmic variables |
2 |
9.0 |
|
AGNs |
1 |
13.7 |
|
Total |
71 |
538.6 |
Selected Programs and Time Allocation
Following the TAC evaluation, 23 programs were selected for the STELES Science Verification campaign. The approved times ranged between 0.64 to 9.60 hours per project. The selected projects span a broad range of scientific topics and collectively make use of the main capabilities of STELES, including high spectral resolution, broad wavelength coverage, and near-UV spectroscopy.
The table below lists the approved programs.
|
Project ID |
Title |
Principal Investigator |
Institution/TAC |
Approved time (hours) |
SO2026V-002 | Benchmarking Young Exoplanets: Spectroscopic Validation of Candidate Moving Groups with STELES | A. Mann | UNC/UNC | 3.00 |
SO2026V-003 | Unveiling the Star Formation History of the Orion Nebula: From South to North | P. Braz | UFMG/Brazil | 9.50 |
SO2026V-008 | Unveilling the Physical Condition Secrets of RCW120 with STELES | H. Plana | UESC/Brazil | 3.60 |
SO2026V-012 | Spectroscopy of X-ray AGB stars | R. Ortiz | USP/Brazil | 4.00 |
SO2026V-014 | Complete Chemical Inventory of the CEMP Star HE0118-4834 | R. Santucci | UFG/Brazil | 9.60 |
SO2026V-015 | Unlocking Near-UV Heavy Element Signatures in Mildly ?r?-Process Enhanced Stars with SOAR/STELES | H. Reggiani | USP/Brazil | 7.00 |
SO2026V-016 | A Metal-Poor, r-process enhanced, Standard for STELES | H. Reggiani | USP/Brazil | 5.50 |
SO2026V-019 | Distinguishing Between Li-Enrichment Scenarios in a Remarkable (Potential) Triple System with STELES | C. Manea | UU/NOIRLab | 4.74 |
SO2026V-020 | Using Li and Be abundances as a constraint for stellar interior models | A. Rathsam | USP/Brazil | 7.05 |
SO2026V-025 | Atomic Fe and Mg abundances and chromospheric activity in red dwarfs | E. Abreu | OV/UFRJ | 5.00 |
SO2026V-031 | Deriving the full heavy-element pattern of r-process-enhanced stars selected from DESI | A. Burgasser | UCSD/NOIRLab | 4.00 |
SO2026V-033 | A complete STELES view of the chemical clocks across Gaia-Sausage-Enceladus | F. Gran | GeminiObs/NOIRLab | 6.50 |
SO2026V-034 | Chemical-clock ages across the warm-Jupiter eccentricity distribution | J. Vines | UCN/Chile | 7.00 |
SO2026V-044 | Near-UV-to-Red High-Resolution Benchmark of an Extended Cometary Coma with STELES | D. Bodewits | AU/NOIRLab | 2.90 |
SO2026V-047 | Probing Stripped Companions in Be-star Binaries with the He I Continuum Discontinuity | T. Amorim | USP/Brazil | 5.70 |
SO2026V-048 | Unveiling the Primordial Beryllium Baseline in Blanco 1: A Flagship Near-UV Benchmark for STELES | S. Margheim | RubinObs/NOIRLab | 6.00 |
SO2026V-050 | Probing Stellar Diversity: STELES Science Verification within OCEANS | M. Fernandes | ON/Brazil | 3.70 |
SO2026V-051 | Measuring the Volatile Composition of Comet 10P/Tempel 2 with STELES | A. McKay | ASU/NOIRLab | 2.91 |
SO2026V-053 | Homogeneous C/O and Nitrogen Abundances for JWST Exoplanet Hosts with STELES | P. McCreery | JHU/NOIRLab | 3.30 |
SO2026V-057 | Characterizing components of massive binary systems | C. Rodriguez | GeminiObs/NOIRLab | 0.64 |
SO2026V-061 | Tracing Beryllium Enrichment in the Thamnos Accreted Galaxy | L. Monaco | UNAB/NOIRLab | 1.00 |
SO2026V-066 | Planetary Nebula Central Star Winds and Inner-Nebula Kinematics at High Spectral Resolution | H. Monteiro | UNIFEI/Brazil | 2.00 |
SO2026V-069 | The Most Detailed Chemical Template for Neutron-Capture Enrichment in Ultra-Faint Dwarf Galaxies | S. Shah | NCSU/NOIRLab | 4.73 |
Institutional Participation
The STELES Science Verification call attracted proposals from a broad range of institutions, reflecting the interest in the new instrument across the astronomical community. The 23 programs selected for execution involve researchers from 18 institutions, including institutions in South America, North America and Europe.
The distribution of the selected programs by the Principal Investigator's home institution and TAC partner is summarized below, showing both the number of approved programs and the corresponding awarded observing time.
|
Institution/TAC |
Selected programs |
Approved time (hours) |
|
USP/Brazil |
5 |
29.25 |
|
UFG/Brazil |
1 |
9.60 |
|
UFMG/Brazil |
1 |
9.50 |
|
Gemini Obs/NOIRLab |
2 |
7.14 |
|
UCN/Chile |
1 |
7.00 |
|
Rubin Obs/NOIRLab |
1 |
6.00 |
|
OV-UFRJ/Brazil |
1 |
5.00 |
|
UU/NOIRLab |
1 |
4.74 |
|
NCSU/NOIRLab |
1 |
4.73 |
|
UCSD/NOIRLab |
1 |
4.00 |
|
ON/Brazil |
1 |
3.70 |
|
UESC/Brazil |
1 |
3.60 |
|
JHU/NOIRLab |
1 |
3.30 |
|
UNC/UNC |
1 |
3.00 |
|
ASU/NOIRLab |
1 |
2.91 |
|
AU/NOIRLab |
1 |
2.91 |
|
UNIFEI/Brazil |
1 |
2.00 |
|
UNAB/NOIRLab |
1 |
1.00 |
|
TAC |
Selected programs |
Approved time (hours) |
|
NOIRLab |
10 |
36.73 h |
|
Brazil |
11 |
62.65 h |
|
UNC |
1 |
3.00 h |
|
Chile |
1 |
7.00 h |
Next steps
The strong response to the call demonstrates the broad scientific interest in STELES and its capabilities and the selected programs will provide an important first assessment of the instrument's performance for science observations.
The selected programs will be executed during the three STELES Science Verification observing runs scheduled for September 8–11, October 7–10, and December 4–6, 2026. The final scheduling of individual targets will be performed in queue mode, taking into account target visibility, observing conditions, and the operational requirements of the Science Verification campaign.
Data obtained through the Science Verification program will be processed by the STELES/SOAR team and made available to the respective Principal Investigators following the observations. Data products are expected to be delivered within approximately 1-3 weeks after each observing run, with a three-month proprietary period.
For further information or doubts, please contact Felipe Navarete (fnavarete(at)lna.br).
SOAR Brazilian Manager / STELES Instrument Scientist