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Observing Unique sTars and gaLactic chemIcal Evidence of the fiRst relicS

Project description

Understanding the formation of the first stars

The study of star formation is essential for understanding our universe and the solar system. While we have identified more low-metallicity stars, Population III (Pop III) stars, which lack metals altogether, remain undiscovered. Recent simulations suggest the existence of low-mass counterparts. Additionally, Population II (Pop II) stars, formed after the first supernova, show chemical traits that could deepen our understanding of Pop III stars. The ERC-funded OUTLIERS project aims to combine observational effort, the latest spectroscopic survey, Gaia BP/RP data, and state-of-the-art models and analysis tools to search for Pop III and identify key Pop II stars to deduce key insights for astrophysics and expand our understanding of the formation of the first stars.

Objective

The number of identified primitive low-metallicity stars has steadily grown. Today, we know of stars with less than one ten-millionth of the solar iron content, but no stars completely devoid of metals —known as Population III (Pop III)— have been identified so far. It was commonly accepted that only massive, short-lived Pop III stars formed from metal-free clouds, but recent simulations suggest that their low-mass counterparts (<1M☉) could also form and may still survive today. However, the mass distribution of these first stars remains unknown, though most are expected to be massive, reaching up to 1000M☉.

The first supernova (SN) enriched the medium with heavy elements, enabling the formation of long-lived Population II (Pop II) stars from this processed material. These stars exhibit distinct chemical peculiarities that are key to understanding their Pop III progenitors, including mass and SN explosion energy. However, identifying and characterising these exceedingly rare chemically peculiar stars poses significant challenges. Finding long-lived Pop III stars or second-generation stars polluted by very massive Pop III SNe will revolutionise modern astronomy.

With OUTLIERS I propose a novel approach that combines an unprecedented observational effort, encompassing my large program with the 10.4m GTC, privileged access to the latest spectroscopic surveys (DESI, 4MOST, WEAVE), and Gaia BP/RP data. Together with state-of-the-art models and my advanced analysis tools (FESWI, PISN-explorer), this approach will increase the number of chemically peculiar stars by over an order of magnitude, allowing us, for the first time, to:

-Search for Pop III stars within the largest spectroscopic dataset ever compiled
-Identify and characterise second-generation stars to reconstruct the mass and energy of their progenitors

Achieving these objectives will shed light on a critical issue in astrophysics: the formation of the first stars as evidenced by their Pop II descendants.

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(opens in new window) ERC-2025-STG

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Host institution

INSTITUTO DE ASTROFISICA DE CANARIAS
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 1 500 000,00
Address
CALLE VIA LACTEA
38205 SAN CRISTOBAL DE LA LAGUNA
Spain

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Region
Canarias Canarias Tenerife
Activity type
Research Organisations
Links
Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 1 500 000,00

Beneficiaries (1)

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