Zobrazeno 1 - 10
of 17
pro vyhledávání: '"observational galaxies"'
Autor:
Yu Rong
Publikováno v:
Universe, Vol 10, Iss 7, p 286 (2024)
We present an analysis of the ellipticities of galaxy groups, derived from the spatial distribution of member galaxies, revealing a notable incongruity between the observed local galaxy groups and their counterparts in the Lambda cold dark matter cos
Externí odkaz:
https://doaj.org/article/5a4450f0eaa949b2b4c3d96dd9cc963c
Akademický článek
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Autor:
Hanae Inami, Hiddo S B Algera, Sander Schouws, Laura Sommovigo, Rychard Bouwens, Renske Smit, Mauro Stefanon, Rebecca A A Bowler, Ryan Endsley, Andrea Ferrara, Pascal Oesch, Daniel Stark, Manuel Aravena, Laia Barrufet, Elisabete da Cunha, Pratika Dayal, Ilse De Looze, Yoshinobu Fudamoto, Valentino Gonzalez, Luca Graziani, Jacqueline A Hodge, Alexander P S Hygate, Themiya Nanayakkara, Andrea Pallottini, Dominik A Riechers, Raffaella Schneider, Michael Topping, Paul van der Werf
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Inami, H, Algera, H S B, Schouws, S, Sommovigo, L, Bouwens, R, Smit, R, Stefanon, M, Bowler, R A A, Endsley, R, Ferrara, A, Oesch, P, Stark, D, Aravena, M, Barrufet, L, da Cunha, E, Dayal, P, De Looze, I, Fudamoto, Y, Gonzalez, V, Graziani, L, Hodge, J A, Hygate, A P S, Nanayakkara, T, Pallottini, A, Riechers, D A, Schneider, R, Topping, M & van der Werf, P 2022, ' The ALMA REBELS Survey : dust continuum detections at z > 6.5 ', Monthly Notices of the Royal Astronomical Society, vol. 515, no. 3, pp. 3126-3143 . https://doi.org/10.1093/mnras/stac1779
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 515(3), 3126-3143
Monthly Notices of the Royal Astronomical Society, 515, 3126-3143. Oxford University Press
Inami, H, Algera, H S B, Schouws, S, Sommovigo, L, Bouwens, R, Smit, R, Stefanon, M, Bowler, R A A, Endsley, R, Ferrara, A, Oesch, P, Stark, D, Aravena, M, Barrufet, L, da Cunha, E, Dayal, P, De Looze, I, Fudamoto, Y, Gonzalez, V, Graziani, L, Hodge, J A, Hygate, A P S, Nanayakkara, T, Pallottini, A, Riechers, D A, Schneider, R, Topping, M & van der Werf, P 2022, ' The ALMA REBELS Survey : dust continuum detections at z > 6.5 ', Monthly Notices of the Royal Astronomical Society, vol. 515, no. 3, pp. 3126-3143 . https://doi.org/10.1093/mnras/stac1779
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 515(3), 3126-3143
Monthly Notices of the Royal Astronomical Society, 515, 3126-3143. Oxford University Press
We report 18 dust continuum detections ($\geq 3.3\sigma$) at $\sim88{\rm \mu m}$ and $158{\rm \mu m}$ out of 49 ultraviolet(UV)-bright galaxies ($M_{\rm UV} < -21.3$ mag) at $z>6.5$, observed by the Cycle-7 ALMA Large Program, REBELS and its pilot pr
Autor:
A. Ignesti, G. Brunetti, T. Shimwell, M. Gitti, L. Birzan, A. Botteon, M. Brüggen, F. de Gasperin, G. Di Gennaro, A. C. Edge, C. J. Riseley, H. J. A. Röttgering, R. J. van Weeren
Publikováno v:
Astronomy & Astrophysics, 659:A20
Astronomy & astrophysics, 2022, Vol.659, pp.A20 [Peer Reviewed Journal]
Astronomy & astrophysics, 2022, Vol.659, pp.A20 [Peer Reviewed Journal]
Radio observations represent a powerful probe of the physics occurring in the intracluster medium (ICM) because they trace the relativistic cosmic rays in the cluster magnetic fields, or within galaxies themselves. By probing the low-energy cosmic ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::806a08623f9fe472b2d0cd2dfe91808e
http://arxiv.org/abs/2111.15517
http://arxiv.org/abs/2111.15517
Autor:
Damien Gratadour, Yves Magnard, C. Petit, Frédéric Marin, Eric Lagadec, M. Montargès, Johannes Pragt, S. Hunziker, Lucas Grosset, M. Carle, Daniel Rouan
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 648, pp.A42. ⟨10.1051/0004-6361/202038260⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 648, pp.A42. ⟨10.1051/0004-6361/202038260⟩
Astronomy & Astrophysics, 648
Astronomy and Astrophysics-A&A, 2021, 648, pp.A42. ⟨10.1051/0004-6361/202038260⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 648, pp.A42. ⟨10.1051/0004-6361/202038260⟩
Astronomy & Astrophysics, 648
Context Polarisation is a decisive method to study the inner region of active galactic nuclei (AGNs) since, unlike classical imaging, it is not affected by contrast issues. When coupled with high angular resolution (HAR), polarisation can help to dis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f06b6c4999f63847ce6882c6b17c5fef
https://hal.science/hal-03194929
https://hal.science/hal-03194929
Autor:
Makariev, Martin, Maneva, Galina, Minev, Milen, Temnikov, Petar, Verguilov, Vassil, Acciari, V.A. ... et al
We report a characterization of the multiband flux variability and correlations of the nearby (z = 0.031) blazar Markarian 421 (Mrk 421) using data from Metsähovi, Swift, Fermi-LAT, MAGIC, FACT, and other collaborations and instruments from 2014 Nov
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______9626::3e772b1144e8373b1d5725d75d056db2
Autor:
Franz E. Bauer, Chiara Mazzucchelli, Roberto Decarli, Bin Luo, Gianni Zamorani, Ohad Shemmer, Enrico Congiu, Nico Cappelluti, Thomas Connor, Eduardo Bañados, Riccardo Nanni, Andrea Comastri, M. Mignoli, Simona Gallerani, Federica Ricci, Francesco Calura, Marcella Brusa, Francesca Civano, Fabio Vito, Roberto Gilli, W. N. Brandt, Cristian Vignali
The discovery of hundreds of QSOs in the first Gyr of the Universe powered by already grown SMBHs challenges our knowledge of SMBH formation. In particular, investigations of $z>6$ QSOs presenting notable properties can provide unique information on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16523afa9dadc887d817fbd9f4d70da7
https://hdl.handle.net/11590/420020
https://hdl.handle.net/11590/420020
Akademický článek
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Autor:
W. N. Brandt, Franz E. Bauer, Ohad Shemmer, Fabio Vito, Riccardo Nanni, Francesca Civano, Francesco Calura, Chiara Mazzucchelli, Gianni Zamorani, M. Mignoli, Marta Volonteri, Cristian Vignali, Marcella Brusa, Andrea Comastri, Nico Cappelluti, Roberto Gilli, Bin Luo
While theoretical arguments predict that most of the early growth of supermassive black holes (SMBHs) happened during heavily obscured phases of accretion, current methods used for selecting $z>6$ quasars (QSOs) are strongly biased against obscured Q
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92f8bbfdfcaad1d6c722d4461e3b2a17
http://hdl.handle.net/11585/734857
http://hdl.handle.net/11585/734857