Open repository for EU-funded research outputs from Horizon Europe, Euratom, and earlier Framework Programmes.
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February 27, 2026 (v0.5.2)SoftwareOpen
Automatic Plotting of Many Graphs
Uploaded on February 27, 2026
Part of Geneva Graduate Institute - Global Governance Centre
7 more versions exist for this record
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February 27, 2026 (v1)DatasetOpen
This dataset contains the raw data supporting the results reported in the article "3D-printable Nitric Oxide-Releasing PHEMA/Polysilsesquioxane intracoronary stents".
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February 27, 2026 (v1)PosterOpen
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February 27, 2026 (V2.0.0)SoftwareOpen
gdc-samtools-fastq A WDL pipeline to convert GDC BAM files to fastq format utilizing GDC recommended options. For execution on Terra.bio. GDC Samtools FASTQ Workflow This WDL workflow converts aligned BAM files back into paired-end FASTQ format, adhering to GDC Data Harmonization standards. It is designed to run locally using the Dockstore...
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February 27, 2026 (v1)PresentationOpen
Narrow-Line Seyfert 1 galaxies (NLS1s) are among the best local laboratories for studying super-Eddington (S-E) accretion onto supermassive black holes (SMBHs). I present recent results from a systematic broad-band X-ray campaign on eight bona fide S-E AGN from the SEAMBH sample, observed with simultaneous XMM–Newton and NuSTAR (plus Swift for...
Uploaded on February 27, 2026
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February 27, 2026 (v1)PresentationOpen
Are NLS1 intrinsically young AGN, or are their properties shaped by external factors in their host environments? In this talk, I will explore the "nature versus nurture" paradigm as a framework to interpret the multi-faceted characteristics of NLS1s. On the "nature" side, I will discuss intrinsic features such as low black hole masses, high...
Uploaded on February 27, 2026
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February 27, 2026 (v1)PresentationOpen
NLS1 galaxies exhibit narrow permitted Hβ lines (FWHM < 2000 km/s) and strong Fe II multiplets with low BH masses(< 108 M⊙)and high Eddington ratio indicating that they are early-stage AGN. They host the lowest mass SMBHs that can launch relativistic jets and offer insight into the conditions necessary for jet formation. But classifying NLS1s...
Uploaded on February 27, 2026
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February 27, 2026 (v1)PresentationOpen
I use photometric reverberation mapping to measure quasar accretion-disk sizes from interband delays and to test the disk size–luminosity link. For Rubin's Deep Drilling Fields I analyze simulated light curves with realistic cadences, assessing how broadline and diffuse-continuum leakage and survey sampling impact lag recovery and the...
Uploaded on February 27, 2026
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February 27, 2026 (v1)PresentationOpen
To understand how supermassive black holes may have grown through episodes of near/super-Eddington accretion, we need observational constraints on how such episodes affect the physics of AGN central engines. At Eddington ratios above ∼30%, the accretion disk is believed to transition at small radii into a geometrically thick and radiatively...
Uploaded on February 27, 2026
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February 27, 2026 (v1)PresentationOpen
In this talk I give a short overview of radio monitoring of NLS1 galaxies so far, and then focus on the possibilities offered by the new triple-band receiver (3BR) that will be installed at Metsahovi Radio Observatory in late 2025. The receiver is expected to be operational during 2026. The three frequencies 22, 43, and 86 GHz can be used...
Uploaded on February 27, 2026
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