From the 1 of 77 papers with an AI index.
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- Osservatorio Astronomico di PadovaIT57 papers
- National Institute for AstrophysicsIT52 papers
- Brera Astronomical ObservatoryIT50 papers
- Institut d'Estudis Espacials de CatalunyaES49 papers
- Institute of Space SciencesES49 papers
- University of FerraraIT46 papers
- Arcetri Astrophysical ObservatoryIT45 papers
- DAWN Center for Independent LivingUS45 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di FerraraIT45 papers
- Max Planck Institute for Extraterrestrial PhysicsDE45 papers
- Osservatorio di Astrofisica e Scienza dello Spazio45 papers
- University of PaduaIT45 papers
19 papers · 1 filter
The Next Generation Virgo Cluster Survey (NGVS). II. A Catalog of Galaxies in the Virgo Cluster
Laura Ferrarese, Patrick Cote, Lauren A. MacArthur +51
The Next Generation Virgo Cluster Survey (NGVS) is a deep, high resolution imaging campaign that used the 1 deg MegaCam instrument on the Canada-France-Hawaii Telescope to carr…
Euclid: Calibrating distances from surface brightness fluctuations with Early Release Observations of the Fornax cluster
R. Habas, M. Cantiello, G. Riccio +169
Surface brightness fluctuations (SBF), the pixel-to-pixel variations in flux that arise from the statistical distribution of stars in galaxy images, provide a powerful tool to meas…
Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies
Euclid Collaboration, R. Hill, A. Abghari +302
The first Euclid Quick Data Release contains millions of galaxies with excellent optical and near-infrared (IR) coverage. To complement this dataset, we investigate the average far…
Euclid Quick Data Release (Q1). Searching for radio-selected \Euclid-dark galaxies in the EDF-N
Euclid Collaboration, M. Giulietti, I. Prandoni +308
We present and investigate the properties of a sample of radio-selected, Euclid-dark galaxies, identified from LOFAR HBA observations at 144 MHz within the Euclid Deep Field-North…
Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP
E. Bortolas, E. Portaluri, E. Dalla Bonta' +3
Massive black hole (MBH) binaries form as a result of galaxy mergers and can coalesce into a single MBH by emitting gravitational waves detectable by LISA and pulsar timing array c…
Euclid Quick Data Release (Q1): The geometry of dark matter halos from extragalactic streams
Euclid Collaboration, N. Starkman, J. Nibauer +295
Wide-field surveys like Euclid mark a new era of extragalactic stellar stream studies. With a large number of streams, it is now possible to constrain the dark matter halos of gala…