AO-1 Programmes

The 1st Announcement of Opportunity (AO-1) for the PLATO Guest Observers (GO) Programme opened on 7 April 2026 and closed on 21 May 2026, covering observing windows during the first two years of the mission. A total of 117 proposals were received, comprising approximately 76,000 observing requests. All eligible proposals underwent technical review by mission experts in June and were then scientifically evaluated by the PLATO Time Allocation Committee (TAC) during its meetings in July 2026.

Based on the TAC's recommendation, ESA's Director of Science has approved the awards and waitlist listed below. In total, 23 proposals were awarded observing time and a further 28 placed on the waitlist, spanning a broad range of scientific investigations complementary to PLATO's core science objectives. The demand for the AO-1 Call corresponds to an estimated oversubscription of 2.3 to 5.1 in number of proposals, depending on the inclusion of waitlisted proposals in the final observing schedule. Final values will depend on in-orbit performance and scheduling optimisation.

All Principal Investigators (PIs) are informed of the outcome by email and receive the TAC feedback for their proposals. As with any space mission, an award or waitlist status cannot guarantee execution, as technical and operational constraints may affect the final observing programme. All teams of awarded and waitlisted proposals are therefore requested to carefully review the information regarding “Scheduling, Constraints, and Required Actions” provided below.

The PLATO team congratulates the successful proposers and thanks all applicants for their interest in the mission and in this inaugural opportunity. 

A short article highlighting the breadth and diversity of the new science programmes enabled through the AO-1 Call can be found here.

 

Awards

ID PI (Country) Title
5 Plachy (HU) Probing Low-Amplitude and Long-Term Variability in Cepheid Pulsators
21 Van Daele (UK) Constraining interior rotation and mixing from stochastic low-frequency variability in massive stars
34 Uzundag (BE) Asteroseismology of white dwarfs in the era of PLATO
39 Henneco (UK) Identifying binary interaction products using asteroseismology
64 Williams (UK) Planetary debris transiting white dwarfs
67 Thomson-Paressant (UK) The relationship between magnetism and pulsations in classical pulsators
72 Bryant (UK) Confirming Long-Period Transiting Giants
78 Veresvarska (ES) Shadows in the cave: Synoptic Survey of Cataclysmic Variables in PLATO
81 Coti Zelati (ES) Testing X-ray reprocessing and scattering geometry in the eclipsing and dipping LMXB 2S 0921-63 with PLATO
82 Veresvarska (ES) Tracing Accretion Disc Structure Through Simultaneous Blue–Red Variability with PLATO FASTCAM
91 Handler (PL) Asteroseismology of a Golden Sample of massive pulsators
117 Ashraf (IN) The First 100 Million Years: A PLATO Multi-Science Survey of Young Stellar and Planetary Systems
120 Li (AU) PLATO-TIDES: Tidal Interactions and Dynamics in pulsating Eclipsing Systems
121 Neiner (FR) What is the internal magnetic field of pulsating hot (β Cep, SPB, δ Scu) stars?
128 Van Grootel (BE) Hot subdwarf stars in the PLATO era: a key window for intermediate stages of stellar evolution
131 Southworth (UK) A Complete Census of Semi-Detached Eclipsing Binaries in the PLATO Field
133 Sana (BE) Intermediate-mass stripped stars with main-sequence companions
135 Gillen (UK) Extending PLATO's reach to study young stars and planetary systems
142 Miglio (IT) From detection to inference: a PLATO testbed for globular-cluster seismology
153 Mas Sanz (DK) Do A/F stars exhibit magnetic cycles? A PLATO study of rotational modulation and surface variability
162 Leitinger (IT) Mapping the accretion history of the Galactic halo with precision stellar ages
164 Osborn (CH) PLATO Exoplanet Community K-dwarf Survey (PECKS)
178 Pittman (DE) Following Dusty Signposts of Short-Period Planet Formation

 

Abstracts for all awarded proposals can be found here.

 

Waitlist

ID PI (Country) Title
1 Benko (HU) Multimode pulsations, resonances, and binarity in a homogeneous Galactic RR Lyrae sample
15 Plachy (HU) Tracing the modulation phenomenon in High-Amplitude delta Scuti stars
35 Scott (UK) Constraining interior rotation and mixing of massive pulsating stars: ensemble asteroseismology of β Cephei and SPB stars
36 Deeg (ES) Multiplying the eclipsing binary sample for circumbinary planet detection
37 Neiner (FR) Understanding outbursts and the formation of a decretion disk around Be stars via angular momentum transport
43 Kliapets (BE) High-Precision Asteroseismology of Main-Sequence Hybrid Pulsators with PLATO: Empirical Instability Strips and Differential Rotation
52 Bowman (UK) The impact of metallicity on stochastic low-frequency variability revealed by PLATO light curves of massive stars in the LMC
56 Mahy (BE) A PLATO view of the final evolutionary phases of massive stars
63 Labadie-Bartz (DK) Survey of pulsation in the most rapidly rotating B stars
68 Korth (ES) Eclipse timing variations in short-period binaries: a PLATO search for circumbinary planets and low-mass companions
85 Derekas (HU) Asteroseismology of Mass-Accreting Pulsators: PLATO Survey of Oscillating Eclipsing Algol Systems
88 Helminiak (PL) Long-period eclipsing binaries
101 Emilio (BR) Testing Binary Interaction, Rapid Rotation, and Disk Feeding in Be Stars with PLATO
107 Andrade (BR) Benchmark Be Stars with PLATO and Long-Term Spectroscopic Monitoring
118 Korth (ES) Dead Stars, Living Worlds: Discovering Planets and Debris Around White Dwarfs
124 Nardiello (IT) PLATO observations of open cluster stars
130 Ilin (NL) Stormy Youth: A PLATO survey for planet-induced flaring in young systems
132 Lantzi (ES) M&Ms in PLATO: Benchmarking M-dwarf Eclipsing Binaries to Test Stellar Models
141 Jiang (UK) Tracing Supermassive Black Hole Accretion Disc Variability at the Eddington Limit with PLATO from Kiloseconds to Years
146 Andrych (AU) Tracing second-generation circumbinary disc geometry and disc-binary interaction through optical variability in Galactic post-AGB binaries
149 Swiech (DK) Probing unexplained oscillation spectra in intermediate-mass stars with PLATO
152 Bryant (UK) MainCandsProp
157 Bouchy (CH) Exoplanets around mid-to-late M dwarfs
159 Bergemann (DE) Testing the Spite plateau with PLATO-GO and 4MOST
167 Briganti (IT) Constraining the internal structure of blue straggler stars with asteroseismology
170 Hooton (UK) The SPECULATO survey: searching for planets and characterising the activity of the coolest stars
171 Pedersen (AU) Asteroseismology of early-type stars in OB associations
179 Dimoff (DE) Primordial disc survey with PLATO GO and 4MOST

 

Abstracts for all waitlisted proposals can be found here.

 

Scheduling, Constraints, and Required Actions
 

Publication of Targets and Processing Types: Details of the awarded and waitlisted targets will be published at a later stage, following completion of the GO Programme verification process. This stage will allow PIs to first review and correct implementation-related information provided during proposal submission, if needed. Information on final processing types will likewise be communicated later, as these may evolve during the detailed scheduling optimisation process.

Scheduling: Proposing teams are reminded that a TAC recommendation for award or waitlist status does not guarantee that observations will be scheduled. Scheduling remains contingent on PLATO's in-orbit performance and available resources. Following commissioning, and during each execution of the PLATO Target Planning Tool (currently foreseen prior to each quarterly uplink), available GO resources will first be allocated to awarded proposals and then, where resources remain, to waitlisted proposals.

Technical Constraints: Scheduling is constrained not only by telemetry, but also by other technical limitations, including processing-type budgets and detector-level capacities. The impact of these constraints may also vary between quarters. Consequently, while the TAC ranking of proposals and the PI ranking of targets will be respected wherever possible, the final schedule may not strictly follow these rankings if technical or operational constraints prevent proposals or targets from being accommodated. 

Processing Types (e.g. Centroids): Given the complexity of the technical constraints, the final processing types may need to differ from those requested. The PLATO Science Operations Centre (SOC) may contact affected teams closer to the start of observations to identify the most suitable implementation. In particular, current demand for centroid measurements may exceed available on-board resources. Where necessary, the PLATO SOC will work with PIs to identify alternative solutions that preserve the scientific objectives while remaining within mission constraints. 

Duplicate Targets: To maximise the scientific return of the mission and encourage a collaborative spirit, duplicate targets will be observed only once using the highest requested observing mode, where possible. The resulting data products will be made available simultaneously to all relevant proposing teams, who are encouraged to collaborate or to agree on independent analyses, as appropriate.

Waiving Proprietary Rights: Some proposals may wish to make their data public immediately, which requires the following aspects to be taken into account. Please contact the PLATO Helpdesk closer to the time of your observations to ensure that this preference is implemented when the data are ingested into the PLATO Archive (PAX). In the case of duplicate targets, for example where one team requires proprietary access while another wishes to make the data public immediately, the involved teams are expected to coordinate closely and ensure that the rights and needs of all parties are respected.

Action Required: PIs of awarded and waitlisted proposals are requested to verify that their target lists, including all CfP input and output files, are correct and up to date. Any issues identified should be reported promptly to the PLATO Helpdesk. Where technical reviews have already identified inconsistencies, the PLATO SOC may also contact proposers directly to request updates. Any questions during this process should likewise be directed to the PLATO Helpdesk.

Questions about the PLATO mission or its Guest Observers Programme? Please contact our PLATO Helpdesk. This will connect you with our PLATO Science Operations Centre and technical specialists from our PLATO Mission Consortium, and our team will be happy to assist you. This website was last updated on 14 September 2026.