中文
相关论文

相关论文: The miniJPAS survey: clusters and galaxy groups de…

200 篇论文

Galaxy clusters are an essential tool to understand and constrain the cosmological parameters of our Universe. Thanks to its multi-band design, J-PAS offers a unique group and cluster detection window using precise photometric redshifts and…

The impending Javalambre Physics of the accelerating universe Astrophysical Survey (J-PAS) will be the first wide-field survey of $\gtrsim$ 8500 deg$^2$ to reach the `stage IV' category. Because of the redshift resolution afforded by 54…

We present AMICO (Adaptive Matched Identifier of Clustered Objects), a new algorithm for the detection of galaxy clusters in photometric surveys. AMICO is based on the Optimal Filtering technique, which allows to maximise the…

宇宙学与河外天体物理 · 物理学 2017-12-13 Fabio Bellagamba , Mauro Roncarelli , Matteo Maturi , Lauro Moscardini

We present a new galaxy cluster search in the COSMOS field through the use of the Adaptive Matched Identifier of Clustered Objects (AMICO). We produced a new cluster and group catalogue up to $z=2$, by performing an innovative application…

宇宙学与河外天体物理 · 物理学 2024-06-26 Greta Toni , Matteo Maturi , Alexis Finoguenov , Lauro Moscardini , Gianluca Castignani

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) is an ongoing survey mapping thousands of square degrees in the Northern Hemisphere using 56 narrow-band filters, delivering IFU-like photometric data well…

The Javalambre-Physics of the Accelerated Universe Astrophysical Survey (J-PAS) is a narrow band, very wide field Cosmological Survey to be carried out from the Javalambre Observatory in Spain with a purpose-built, dedicated 2.5m telescope…

宇宙学与河外天体物理 · 物理学 2014-03-21 N. Benitez , R. Dupke , M. Moles , L. Sodre , J. Cenarro , A. Marin-Franch , K. Taylor , D. Cristobal , A. Fernandez-Soto , C. Mendes de Oliveira , J. Cepa-Nogue , L. R. Abramo , J. S. Alcaniz , R. Overzier , C. Hernandez-Monteagudo , E. J. Alfaro , A. Kanaan , J. M. Carvano , R. R. R. Reis , E. Martinez Gonzalez , B. Ascaso , F. Ballesteros , H. S. Xavier , J. Varela , A. Ederoclite , H. Vazquez Ramio , T. Broadhurst , E. Cypriano , R. Angulo , J. M. Diego , A. Zandivarez , E. Diaz , P. Melchior , K. Umetsu , P. F. Spinelli , A. Zitrin , D. Coe , G. Yepes , P. Vielva , V. Sahni , A. Marcos-Caballero , F. Shu Kitaura , A. L. Maroto , M. Masip , S. Tsujikawa , S. Carneiro , J. Gonzalez Nuevo , G. C. Carvalho , M. J. Reboucas , J. C. Carvalho , E. Abdalla , A. Bernui , C. Pigozzo , E. G. M. Ferreira , N. Chandrachani Devi , C. A. P. Bengaly , M. Campista , A. Amorim , N. V. Asari , A. Bongiovanni , S. Bonoli , G. Bruzual , N. Cardiel , A. Cava , R. Cid Fernandes , P. Coelho , A. Cortesi , R. G. Delgado , L. Diaz Garcia , J. M. R. Espinosa , E. Galliano , J. I. Gonzalez-Serrano , J. Falcon-Barroso , J. Fritz , C. Fernandes , J. Gorgas , C. Hoyos , Y. Jimenez-Teja , J. A. Lopez-Aguerri , C. Lopez-San Juan , A. Mateus , A. Molino , P. Novais , A. OMill , I. Oteo , P. G. Perez-Gonzalez , B. Poggianti , R. Proctor , E. Ricciardelli , P. Sanchez-Blazquez , T. Storchi-Bergmann , E. Telles , W. Schoennell , N. Trujillo , A. Vazdekis , K. Viironen , S. Daflon , T. Aparicio-Villegas , D. Rocha , T. Ribeiro , M. Borges , S. L. Martins , W. Marcolino , D. Martinez-Delgado , M. A. Perez-Torres , B. B. Siffert , M. O. Calvao , M. Sako , R. Kessler , A. Alvarez-Candal , M. De Pra , F. Roig , D. Lazzaro , J. Gorosabel , R. Lopes de Oliveira , G. B. Lima-Neto , J. Irwin , J. F. Liu , E. Alvarez , I. Balmes , S. Chueca , M. V. Costa-Duarte , A. A. da Costa , M. L. L. Dantas , A. Y. Diaz , J. Fabregat , F. Ferrari , B. Gavela , S. G. Gracia , N. Gruel , J. L. L. Gutierrez , R. Guzman , J. D. Hernandez-Fernandez , D. Herranz , L. Hurtado-Gil , F. Jablonsky , R. Laporte , L. L. Le Tiran , J Licandro , M. Lima , E. Martin , V. Martinez , J. J. C. Montero , P. Penteado , C. B. Pereira , V. Peris , V. Quilis , M. Sanchez-Portal , A. C. Soja , E. Solano , J. Torra , L. Valdivielso

We present the mass calibration for galaxy clusters detected with the AMICO code in KiDS DR3 data. The cluster sample comprises $\sim$ 7000 objects and covers the redshift range 0.1 < $z$ < 0.6. We perform a weak lensing stacked analysis by…

Future astrophysical surveys such as J-PAS will produce very large datasets, which will require the deployment of accurate and efficient Machine Learning (ML) methods. In this work, we analyze the miniJPAS survey, which observed about 1…

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will soon start to scan thousands of square degrees of the northern extragalactic sky with a unique set of $56$ optical filters from a dedicated $2.55$m…

宇宙学与河外天体物理 · 物理学 2021-09-08 S. Bonoli , A. Marín-Franch , J. Varela , H. Vázquez Ramió , L. R. Abramo , A. J. Cenarro , R. A. Dupke , J. M. Vílchez , D. Cristóbal-Hornillos , R. M. González Delgado , C. Hernández-Monteagudo , C. López-Sanjuan , D. J. Muniesa , T. Civera , A. Ederoclite , A. Hernán-Caballero , V. Marra , P. O. Baqui , A. Cortesi , E. S. Cypriano , S. Daflon , A. L. de Amorim , L. A. Díaz-García , J. M. Diego , G. Martínez-Solaeche , E. Pérez , V. M. Placco , F. Prada , C. Queiroz , J. Alcaniz , A. Alvarez-Candal , J. Cepa , A. L. Maroto , F. Roig , B. B. Siffert , K. Taylor , N. Benitez , M. Moles , L. Sodré , S. Carneiro , C. Mendes de Oliveira , E. Abdalla , R. E. Angulo , M. Aparicio Resco , A. Balaguera-Antolínez , F. J. Ballesteros , D. Brito-Silva , T. Broadhurst , E. R. Carrasco , T. Castro , R. Cid Fernandes , P. Coelho , R. B. de Melo , L. Doubrawa , A. Fernandez-Soto , F. Ferrari , A. Finoguenov , R. García-Benito , J. Iglesias-Páramo , Y. Jiménez-Teja , F. S. Kitaura , J. Laur , P. A. A. Lopes , G. Lucatelli , V. J. Martínez , M. Maturi , M. Quartin , C. Pigozzo , J. E. Rodrìguez-Martìn , V. Salzano , A. Tamm , E. Tempel , K. Umetsu , L. Valdivielso , R. von Marttens , A. Zitrin , M. C. Díaz-Martín , G. López-Alegre , A. López-Sainz , A. Yanes-Díaz , F. Rueda-Teruel , S. Rueda-Teruel , J. Abril Ibañez , J. L Antón Bravo , R. Bello Ferrer , S. Bielsa , J. M. Casino , J. Castillo , S. Chueca , L. Cuesta , J. Garzarán Calderaro , R. Iglesias-Marzoa , C. Íniguez , J. L. Lamadrid Gutierrez , F. Lopez-Martinez , D. Lozano-Pérez , N. Maícas Sacristán , E. L. Molina-Ibáñez , A. Moreno-Signes , S. Rodríguez Llano , M. Royo Navarro , V. Tilve Rua , U. Andrade , E. J. Alfaro , S. Akras , P. Arnalte-Mur , B. Ascaso , C. E. Barbosa , J. Beltrán Jiménez , M. Benetti , C. A. P. Bengaly , A. Bernui , J. J. Blanco-Pillado , M. Borges Fernandes , J. N. Bregman , G. Bruzual , G. Calderone , J. M. Carvano , L. Casarini , A. L Chies-Santos , G. Coutinho de Carvalho , P. Dimauro , S. Duarte Puertas , D. Figueruelo , J. I. González-Serrano , M. A. Guerrero , S. Gurung-López , D. Herranz , M. Huertas-Company , J. A. Irwin , D. Izquierdo-Villalba , A. Kanaan , C. Kehrig , C. C. Kirkpatrick , J. Lim , A. R. Lopes , R. Lopes de Oliveira , A. Marcos-Caballero , D. Martínez-Delgado , E. Martínez-González , G. Martínez-Somonte , N. Oliveira , A. A. Orsi , R. A. Overzier , M. Penna-Lima , R. R. R. Reis , D. Spinoso , S. Tsujikawa , P. Vielva , A. Z. Vitorelli , J. Q. Xia , H. B. Yuan , A. Arroyo-Polonio , M. L. L. Dantas , C. A. Galarza , D. R. Gonçalves , R. S. Gonçalves , J. E. Gonzalez , A. H. Gonzalez , N. Greisel , R. G. Landim , D. Lazzaro , G. Magris , R. Monteiro-Oliveira , C. B. Pereira , M. J. Rebouças , J. M. Rodriguez-Espinosa , S. Santos da Costa , E. Telles

With a unique set of 54 overlapping narrow-band and two broader filters covering the entire optical range, the incoming Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will provide a great opportunity for…

Context. Galaxy clusters provide key insights into cosmic structure formation, galaxy formation and are essential for cosmological studies. Aims. We present a catalog of galaxy clusters detected in the Kilo-Degree Survey (KiDS-DR4)…

The detection of galaxy clusters, the most massive bounded structures in the universe, is crucial for cosmological analysis. Weak lensing signals allow us to track the distribution of all (dark and baryonic) matter regardless of its…

宇宙学与河外天体物理 · 物理学 2025-07-16 Leonardo Trobbiani , Matteo Maturi , Carlo Giocoli , Lauro Moscardini , Gabriele Panebianco

A catalogue of galaxy clusters was obtained in an area of 414 sq deg up to a redshift $z\sim0.8$ from the Data Release 3 of the Kilo-Degree Survey (KiDS-DR3), using the Adaptive Matched Identifier of Clustered Objects (AMICO) algorithm. The…

MiniJPAS is a ~1 deg^2 imaging survey of the AEGIS field in 60 bands, performed to demonstrate the scientific potential of the upcoming JPAS survey. Full coverage of the 3800-9100 \AA range with 54 narrow and 6 broad optical filters allow…

This thesis aims at discerning the effect of environment on galaxy evolution and on the properties of galaxies, using the data from the miniJPAS survey, a 1~deg$^2$ survey that uses the same photometric filter system as the incoming J-PAS…

星系天体物理 · 物理学 2024-10-24 Julio E. Rodríguez-Martín
‹ 上一页 1 2 3 10 下一页 ›