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Metalearning and AI for Time-Domain Astrophysics of AGNs in the Era of Large Scale Surveys

Published online by Cambridge University Press:  05 October 2026

Andjelka B. Kovačević*
Affiliation:
University of Belgrade, Faculty of Mathematics, Department of Astronomy, Studentski trg 16, 11000 Belgrade, Serbia
Dragana Ilić
Affiliation:
University of Belgrade, Faculty of Mathematics, Department of Astronomy, Studentski trg 16, 11000 Belgrade, Serbia
Aman Raju
Affiliation:
DARK, Niels Bohr Institute, University of Copenhagen, Jagtvej155, Copenhagen N, 2200, Denmark
Luka C. Popović
Affiliation:
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia
Marina S. Pavlović
Affiliation:
Vera C. Rubin Observatory, Av. Juan Cisternas 1500, La Serena, 1700000, Chile
Iva Čvorović Hajdinjak
Affiliation:
University of Belgrade, Faculty of Mathematics, Department of Astronomy, Studentski trg 16, 11000 Belgrade, Serbia
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Abstract

Active galactic nuclei (AGNs), powered by accretion onto supermassive black holes (SMBHs), display variability that encodes information on SMBH mass and emission processes. Upcoming time-domain surveys will deliver data for $\mathcal{O}(10^7)$ AGN including light curves with irregular cadences, noise, and sparsity. We report tests on a probabilistic meta-learning framework based on Attentive Latent Neural Processes (ALNPs) on simulated AGN light curves for reconstructing variability, transfer functions, and SMBH-related parameters. We also present a prototype of ALNP quantum-hybrid extension applied to observed AGN.

Information

Type
Contributed Paper
Copyright
© The Author(s), 2026. Published by Cambridge University Press on behalf of The International Astronomical Union
Figure 0

Figure 1. Architecture of the ALNP (left) and prototype of quantum hybrid variant (right). Left: Context data (xc,yc)$(x_c, y_c)$ are encoded into representations Rc$R_c$ via encoder h. Rc$R_c$ are aggregated via two paths: attention and averaging to produce a local representation R(xt)$R(x_t)$ and a global latent variable z. These are passed to a decoder (multi layer perceptron, MLP) to predict target outputs. Right: The PQC consists of 6 input qubits and 4 layers. A small MLP compresses context points mean and standard deviation into per-qubit angles that seed a data-driven RX,RY,RZ layer that is followed by nearest-neighbor CNOT entanglers. After the final block we measure on each qubit and take the first 6 components as the latent vector r for the classical neural decoder.

Figure 1

Figure 2. Testing ALNP on a simulated light curve for a validation AGN. Left Light-curve and transfer function inference for a single simulated AGN. Left: Predicted light curve (blue line) with ±1σ$\pm 1\sigma$ posterior uncertainty (shaded band), compared to the ground-truth fluxes (yellow points). Right: Predicted mean transfer function (blue), compared to the true transfer function (yellow). Lag is given in days. The model is evaluated on jittered realizations of the input light curve, emulating observational noise.

Figure 2

Figure 3. Posterior distributions of SMBH and variability parameters for the same AGN as in Figure 2. Corner plots inference for six parameters: black hole mass log10⁡MBH$\log_{10} M_{\mathrm{BH}}$, Eddington ratio log10⁡λEdd$\log_{10}\lambda_{\mathrm{Edd}}$, long-term variability amplitude SF∞$SF_\infty$, damping timescale log10⁡τDRW$\log_{10}\tau_{\mathrm{DRW}}$, redshift z, and inclination i (here stored as sin⁡i$\sin i$). Blue contours denote 1-3 σ$\sigma$ confidence levels. Vertical and horizontal yellow lines mark the ground-truth values from the simulated dataset.

Figure 3

Figure 4. ALNP predicted vs true values for SMBH parameters: log⁡MBH[M⊙]$\log M_\mathrm{BH}[M_{\odot}]$ (a), log⁡λEdd$\log \lambda_{\mathrm{Edd}}$ (b), SF∞$SF_\infty$ (c), log⁡τDRW$\log \tau_{\mathrm{DRW}}$ (d), z (e), and sin⁡i$\sin i$ (f) obtained from a validation set of 50 synthetic light curves. Dashed line is perfect correlartion, with the mean absolute error (MAE).

Figure 4

Figure 5. Testing PCQ on representative AGN. Quantum Neural Process reconstruction (green) of the observed AGN light curve (blue), with context points (black) and 95% predictive band (gray).