Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Spavone, M."'
Autor:
Napolitano, N. R., Gatto, M., Spiniello, C., Cantiello, M., Hilker, M., Arnaboldi, M., Tortora, C., Chaturvedi, A., D'Abrusco, R., Li, R., Paolillo, M., Peletier, R., Saifollahi, T., Spavone, M., Venhola, A., Pota, V., Capaccioli, M., Longo, G.
Publikováno v:
Astronomy and astrophysics, 657:A94. EDP Sciences
The COld STream finder Algorithm (COSTA) is a novel algorithm to find streams in the phase space of planetary nebulae (PNe) and globular cluster (GCs) populations. COSTA isolates groups of particles with small velocity dispersion, using an iterative
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d00d15319a161f64607373bd4a30a904
http://urn.fi/urn:nbn:fi-fe2023030830678
http://urn.fi/urn:nbn:fi-fe2023030830678
Autor:
Martin, G., Bazkiaei, A. E., Spavone, M., Iodice, E., Mihos, J. C., Montes, M., Benavides, J. A., Brough, S., Carlin, J. L., Collins, C. A., Duc, P. A., Gómez, F. A., Galaz, G., Hernández-Toledo, H. M., Jackson, R. A., Kaviraj, S., Knapen, J. H., Martínez-Lombilla, C., McGee, S., O'Ryan, D., Prole, D. J., Rich, R. M., Román, J., Shah, E. A., Starkenburg, T. K., Watkins, A. E., Zaritsky, D., Laigle, C., Pichon, C., Armus, L., Bianconi, M., Buitrago, F., Busá, I., Davis, F., Demarco, R., Desmons, A., García, P., Graham, A. W., Holwerda, B., Hon, D. S. -H., Khalid, A., Klehammer, J., Klutse, D. Y., Lazar, I., Nair, P., Noakes-Kettel, E. A., Rutkowski, M., Saha, K., Sahu, N., Sola, E., Vázquez-Mata, J. A., Vera-Casanova, A., Yoon, I.
Tidal features in the outskirts of galaxies yield unique information about their past interactions and are a key prediction of the hierarchical structure formation paradigm. The Vera C. Rubin Observatory is poised to deliver deep observations for pot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0da1ea1cd081845e09f4d44466ac1e7
http://arxiv.org/abs/2203.07675
http://arxiv.org/abs/2203.07675
Autor:
Cantiello, Michele, Venhola, A., Paolillo, M., D'Abrusco, R., Grado, A., Iodice, E., Peletier, R., Capaccioli, M., Hilker, M., Mieske, S., Napolitano, N., Riccio, G., Spavone, M., Quintini, M., Bragaglia, A., Davies, M., Sills, A., Vesperini, E.
Publikováno v:
Star Clusters: From the Milky Way to the Early Universe, 14, 68-71
The Fornax Deep Survey (FDS) is a multi-band imaging survey of the Fornax cluster of galaxies, executed with the ESO VLT Survey Telescope (VST). The survey is designed to reach unprecedented surface brightness and point-source magnitude depth over on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3b9c473c11ba27f0b484a0fc627fc169
http://hdl.handle.net/20.500.12386/31140
http://hdl.handle.net/20.500.12386/31140
We present the first data release (DR1) of the VST Early-type GAlaxy Survey (VEGAS). This is a deep multi-band (u'g'r'i') imaging survey, carried out with the ESO VLT Survey Telescope (VST). To date, using about 90% of the total observing time, VEGAS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d549cc6197630c47231470c33bf7b15b
Autor:
Su, A. H. (A. H.), Salo, H. (H.), Janz, J. (J.), Laurikainen, E. (E.), Venhola, A. (A.), Peletier, R. F. (R. F.), Iodice, E. (E.), Hilker, M. (M.), Cantiello, M. (M.), Napolitano, N. (N.), Spavone, M. (M.), Raj, M. A. (M. A.), van de Ven, G. (G.), Mieske, S. (S.), Paolillo, M. (M.), Capaccioli, M. (M.), Valentijn, E. A. (E. A.), Watkins, A. E. (A. E.)
Context: Galaxies either live in a cluster, a group, or in a field environment. In the hierarchical framework, the group environment bridges the field to the cluster environment, as field galaxies form groups before aggregating into clusters. In prin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::7a79479285093dd523084dcd95730d0f
http://urn.fi/urn:nbn:fi-fe2021090245005
http://urn.fi/urn:nbn:fi-fe2021090245005
Autor:
Raj, M. A. (M. A.), Iodice, E. (E.), Napolitano, N. R. (N. R.), Spavone, M. (M.), Su, H.-S. (H-S.), Peletier, R. F. (R. F.), Davis, T. A. (T. A.), Zabel, N. (N.), Hilker, M. (M.), Mieske, S. (S.), Barroso, J. F. (J. Falcon), Cantiello, M. (M.), van de Ven, G. (G.), Watkins, A. E. (A. E.), Salo, H. (H.), Schipani, P. (P.), Capaccioli, M. (M.), Venhola, A. (A.)
Context: We present the study of a magnitude limited sample (mB ≤ 16.6 mag) of 13 late type galaxies (LTGs), observed inside the virial radius, Rvir ∼ 0.7 Mpc, of the Fornax cluster within the Fornax Deep Survey (FDS). Aims: The main objective is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::724e3863ba62f88197ef732a92aef395
http://urn.fi/urn:nbn:fi-fe2019081624425
http://urn.fi/urn:nbn:fi-fe2019081624425
Autor:
Venhola, A. (Aku), Peletier, R. (Reynier), Laurikainen, E. (Eija), Salo, H. (Heikki), Iodice, E. (Enrichetta), Mieske, S. (Steffen), Hilker, M. (Michael), Wittmann, C. (Carolin), Paolillo, M. (Maurizio), Cantiello, M. (Michele), Janz, J. (Joachim), Spavone, M. (Marilena), D’Abrusco, R. (Raffaele), van de Ven, G. (Glenn), Napolitano, N. (Nicola), Kleijn, G. V. (Gijs Verdoes), Capaccioli, M. (Massimo), Grado, A. (Aniello), Valentijn, E. (Edwin), Falcón-Barroso, J. (Jesús), Limatola, L. (Luca)
Context: Dwarf galaxies are the most common type of galaxies in galaxy clusters. Due to their low mass, they are more vulnerable to environmental effects than massive galaxies, and are thus optimal for studying the effects of the environment on galax
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::f1b14ad0d3fef2a7a763831e5d06f3d4
http://urn.fi/urn:nbn:fi-fe202003198601
http://urn.fi/urn:nbn:fi-fe202003198601
Autor:
Cantiello, M., D'Abrusco, R., Spavone, M., Paolillo, M., Capaccioli, M., Limatola, L., Grado, A., Iodice, E., Raimondo, G., Napolitano, N., Blakeslee, J. P., Brocato, E., Forbes, D. A., Hilker, M., Mieske, S., Peletier, R., van de Ven, G., Schipani, P.
Publikováno v:
VizieR Online Data Catalog. VizieR
VizieR Online Data Catalog
VizieR Online Data Catalog
Photometric catalogs for globular cluster (GC) candidates over the the 1 sq. degree area around NGC3115 and NGC1399 (ngc3115.dat and ngc1399.dat). The catalogues are based on u-, g- and i- band images from the VST elliptical galaxies survey (VEGAS).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::3606083dcc413fea034504d8af8b3880
https://research.rug.nl/en/publications/09688bb5-934a-441f-9830-f136e08d8867
https://research.rug.nl/en/publications/09688bb5-934a-441f-9830-f136e08d8867
Autor:
Spavone M., Capaccioli M., Cantiello M., Forbes D. A., Grado A., Iodice E., Limatola L., Napolitano N., Paolillo M., Puzia T. H., Raimondo G., Romanowsky A. J., Schipani P.
Publikováno v:
Astrophysics and Space Science Proceedings ISBN: 9783319193298
The VST-VEGAS project is aimed at observing and studying a rich sample of nearby early-type galaxies in order to systematically characterize their properties over a wide baseline of sizes and out to the faint outskirts where data are rather scarce so
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9033a7163ae3d8734d2aedd5e3ceeb5
http://hdl.handle.net/11588/837451
http://hdl.handle.net/11588/837451
Autor:
Iodice, E., Coccato, L., Combes, F., De Zeeuw, T., Arnaboldi, M., Weilbacher, P., Bacon, R., Kuntschner, H., Spavone, M., Gerin, Maryvonne, Falgarone, Edith, Godard, Benjamin, Lis, Darek
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 583, pp.A48. ⟨10.1051/0004-6361/201526446⟩
Astronomy & Astrophysics (0004-6361), 583, A48
Astronomy and Astrophysics-A&A, 2015, 583, pp.A48
Astronomy & Astrophysics (0004-6361)
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 583, pp.A48. ⟨10.1051/0004-6361/201526446⟩
Astronomy & Astrophysics (0004-6361), 583, A48
Astronomy and Astrophysics-A&A, 2015, 583, pp.A48
Astronomy & Astrophysics (0004-6361)
[abridged] The polar disk galaxy NGC4650A was observed during the commissioning of the MUSE at the ESO VLT to obtain the first 2D map of the velocity and velocity dispersion for both stars and gas. The new MUSE data allow the analysis of the structur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38969da2f6a29c8ca662e439147b6482
https://hal.archives-ouvertes.fr/hal-02502266
https://hal.archives-ouvertes.fr/hal-02502266