4–5 Jun 2026
Universidad Complutense de Madrid
Europe/Madrid timezone

Session

Presentations III

4 Jun 2026, 14:35
Facultad de Químicas - Salón de Actos (Universidad Complutense de Madrid)

Facultad de Químicas - Salón de Actos

Universidad Complutense de Madrid

Plaza de Ciencias, 2. Ciudad Universitaria

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  1. Dr Izaskun Jiménez-Serra (Center of Astrobiology (CAB))
    04/06/2026, 14:35
    Invited talk

    In the past decade, Astrochemistry has witnessed an impressive increase in the number of detections of new molecular species in space. The majority of these detections are related to complex organic molecules (or COMs), defined as carbon-based compounds with more than five atoms in their molecular structure. Interestingly, some of these complex organics are of prebiotic interest, and hence,...

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  2. Teresa Huertas Roldán (Instituto de Astrofísica de Canarias)
    04/06/2026, 15:10
    Contributed talk

    This project exploits the sensitivity, angular resolution, and high-frequency coverage of AtLAST to investigate key processes in late stellar evolution. We target compact and extended sources linked to post-AGB stars and planetary nebulae. For compact objects, we focus on pre-planetary nebulae with rotating disks, divided into high- and low-momentum subclasses. Using mm-wavelength radio...

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  3. Dr Víctor M. Rivilla (Centro de Astrobiología (CAB), CSIC-INTA)
    04/06/2026, 15:30
    Contributed talk

    In recent years, two ultra-long (>1000 hr) single-dish spectral surveys toward the cold and quiescent molecular cloud TMC-1 have identified over 20 molecules containing five- and six-membered carbon rings, from benzonitrile (1 ring) to cyanocoronene (7 rings). These species are the simplest representatives of polycyclic aromatic hydrocarbons (PAHs), believed to account for a significant...

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  4. Thomas Morris (Yale University)
    04/06/2026, 15:55
    Contributed talk

    The maria simulator ([https://thomaswmorris.com/maria/][1]) is a python-based, comprehensive tool for simulating mapping observations with direct-detection instruments such as kinetic inductance detectors or bolometers. Ongoing work includes expanding its functionality to include spectroscopy and the use of GPU-accelerated code. I will provide a quick demonstration of its capabilities...

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