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Context. The environments where galaxies reside affects their evolutionary histories. Galaxy triplets (systems composed of three physically bound galaxies) are one of simplest groups of galaxies, and are therefore excellent laboratories to study evol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ed66dc3a9712ad0c236448f932359c4
https://hdl.handle.net/10481/81348
https://hdl.handle.net/10481/81348
Autor:
Hyunjin Shim, Hiroyuki Ikeda, Daryl Joe D. Santos, Stephen Serjeant, Artem Poliszczuk, Takamitsu Miyaji, Dongseob Lee, Hideo Matsuhara, Sune Toft, Simon C. C. Ho, Yoshiki Toba, Ho Seong Hwang, Woong-Seob Jeong, Tetsuya Hashimoto, Helen K. Kim, Seong Jin Kim, Ting Chi Huang, Umi Enokidani, Matthew A. Malkan, Tomotsugu Goto, Thomas R. Greve, Nagisa Oi, Agnieszka Pollo, A. Durkalec, W. J. Pearson, Chris Pearson
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Huang, T-C, Matsuhara, H, Goto, T, Santos, D J D, Ho, S C-C, Kim, S J, Hashimoto, T, Ikeda, H, Oi, N, Malkan, M A, Pearson, W J, Pollo, A, Serjeant, S, Shim, H, Miyaji, T, Hwang, H S, Durkalec, A, Poliszczuk, A, Greve, T R, Pearson, C, Toba, Y, Lee, D, Kim, H K, Toft, S, Jeong, W-S & Enokidani, U 2021, ' Optically detected galaxy cluster candidates in the AKARI North Ecliptic Pole field based on photometric redshift from the Subaru Hyper Suprime-Cam ', Monthly Notices of the Royal Astronomical Society, vol. 506, no. 4, pp. 6063-6080 . https://doi.org/10.1093/mnras/stab2128
Huang, T-C, Matsuhara, H, Goto, T, Santos, D J D, Ho, S C-C, Kim, S J, Hashimoto, T, Ikeda, H, Oi, N, Malkan, M A, Pearson, W J, Pollo, A, Serjeant, S, Shim, H, Miyaji, T, Hwang, H S, Durkalec, A, Poliszczuk, A, Greve, T R, Pearson, C, Toba, Y, Lee, D, Kim, H K, Toft, S, Jeong, W-S & Enokidani, U 2021, ' Optically detected galaxy cluster candidates in the AKARI North Ecliptic Pole field based on photometric redshift from the Subaru Hyper Suprime-Cam ', Monthly Notices of the Royal Astronomical Society, vol. 506, no. 4, pp. 6063-6080 . https://doi.org/10.1093/mnras/stab2128
Galaxy clusters provide an excellent probe in various research fields in astrophysics and cosmology. However, the number of galaxy clusters detected so far in the $AKARI$ North Ecliptic Pole (NEP) field is limited. In this work, we provide galaxy clu
Autor:
Leonova, E., Oesch, P. A., Qin, Y., Naidu, R. P., Wyithe, J. S. B., de Barros, S., Bouwens, R. J., Ellis, R. S., Endsley, R. M., Hutter, A., Illingworth, G. D., Kerutt, J., Labbe, Nicole, Laporte, N., Magee, D., Mutch, S. J., Roberts-Borsani, G. W., Smit, R., Stark, D. P., Stefanon, M., Tacchella, S., Zitrin, A.
Publikováno v:
Leonova, E, Oesch, P A, Qin, Y, Naidu, R P, Wyithe, J S B, de Barros, S, Bouwens, R J, Ellis, R S, Endsley, R M, Hutter, A, Illingworth, G D, Kerutt, J, Labbe, N, Laporte, N, Magee, D, Mutch, S J, Roberts-Borsani, G W, Smit, R, Stark, D P, Stefanon, M, Tacchella, S & Zitrin, A 2022, ' The prevalence of galaxy overdensities around UV-luminous Lyman emitters in the Epoch of Reionization ', Monthly Notices of the Royal Astronomical Society, vol. 515, no. 4, pp. 5790-5801 . https://doi.org/10.1093/mnras/stac1908
Before the end of the Epoch of Reionization, the Hydrogen in the Universe was predominantly neutral. This leads to a strong attenuation of Ly alpha lines of z greater than or similar to 6 galaxies in the intergalactic medium. Nevertheless, Ly alpha h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2751::ecfe5d65795aa1fbd0ae6083e6682e42
https://curis.ku.dk/ws/files/318434333/stac1908.pdf
https://curis.ku.dk/ws/files/318434333/stac1908.pdf
Autor:
Noam I. Libeskind, Stefan Gottlöber, Andrés N. Ruiz, C. Yamila Yaryura, Peter Behroozi, Sofía A. Cora, M. G. Abadi, Cristian A. Vega-Martínez, Gustavo Yepes
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Associations of dwarf galaxies are loose systems composed exclusively of dwarf galaxies. These systems were identified in the Local Volume for the first time more than 30 yr ago. We study these systems in the cosmological framework of the λ cold dar
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We study the role of group infall in the assembly and dynamics of galaxy clusters in $\Lambda$CDM. We select $10$ clusters with virial mass $M_{\rm 200} \sim 10^{14} \, M_{\odot}$ from the cosmological hydrodynamical simulation Illustris and follow t
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 494(2), 2090-2108. Oxford University Press
instname
Monthly Notices of the Royal Astronomical Society, 494(2), 2090-2108. Oxford University Press
We estimate the H i mass function (HIMF) of galaxies in groups based on thousands of ALFALFA (Arecibo Legacy Fast ALFA survey) H i detections within the galaxy groups of four widely used SDSS (Sloan Digital Sky Survey) group catalogues. Although diff
Autor:
Simon P Driver, Aaron S G Robotham, Danail Obreschkow, John A Peacock, Ivan K Baldry, Sabine Bellstedt, Joss Bland-Hawthorn, Sarah Brough, Michelle Cluver, Benne W Holwerda, Andrew Hopkins, Claudia Lagos, Jochen Liske, Jon Loveday, Steven Phillipps, Edward N Taylor
Publikováno v:
Driver, S P, Robotham, A S G, Obreschkow, D, Peacock, J A, Baldry, I K, Bellstedt, S, Bland-Hawthorn, J, Brough, S, Cluver, M, Holwerda, B W, Hopkins, A, Lagos, C, Liske, J, Loveday, J, Phillipps, S & Taylor, E N 2022, ' An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data ', Monthly Notices of the Royal Astronomical Society, vol. 515, no. 2, pp. 2138-2163 . https://doi.org/10.1093/mnras/stac581
We construct the halo mass function (HMF) from the GAMA galaxy group catalogue over the mass range 10^12.7M_sol to 10^15.5M_sol, and find good agreement with the expectation from LambdaCDM. In comparison to previous studies, this result extends the m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd0d0c8b2245f408f17177cb20d31181
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 655, pp.A103. ⟨10.1051/0004-6361/202038722⟩
Astronomy and Astrophysics-A&A, 2021, 655, pp.A103. ⟨10.1051/0004-6361/202038722⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 655, pp.A103. ⟨10.1051/0004-6361/202038722⟩
Astronomy and Astrophysics-A&A, 2021, 655, pp.A103. ⟨10.1051/0004-6361/202038722⟩
We aim to study how the orbits of galaxies in clusters depend on the prominence of the corresponding central galaxies. We divided our data set of $\sim$ 100 clusters and groups into four samples based on their magnitude gap between the two brightest
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe04c61aa51a372716363b687409c1f7
https://hal-cea.archives-ouvertes.fr/cea-03461089/document
https://hal-cea.archives-ouvertes.fr/cea-03461089/document
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We analyse the presence of dust around galaxy group members through the reddening of background quasars. By taking into account quasar colour and their dependence on redshift and angular position, we derive mean quasar colours excess in projected reg