Zobrazeno 1 - 10 of 204 pro vyhledávání: '"luminosity function [galaxies]"'
1
The role of mass and environment in the build up of the quenched galaxy population since cosmic noon
Autor: Elizabeth Taylor, Omar Almaini, Michael Merrifield, David Maltby, Vivienne Wild, William G Hartley, Kate Rowlands
We conduct the first study of how the relative quenching probability of galaxies depends on environment over the redshift range $0.5 < z < 3$, using data from the UKIDSS Ultra-Deep Survey. By constructing the stellar mass functions for quiescent and
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::802e363ee0e02776c7a613383e583b4b
http://arxiv.org/abs/2304.09169
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2
The H I mass function of group galaxies in the ALFALFA survey
Autor: Lourdes Verdes-Montenegro, Elizabeth A. K. Adams, Michael G. Jones, Kelley M. Hess
Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab975066609c29aea1e97e4f29c82a77
https://doi.org/10.1093/mnras/staa810
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3
Galaxy And Mass Assembly (GAMA)
Autor: Simon P Driver, Sabine Bellstedt, Aaron S G Robotham, Ivan K Baldry, Luke J Davies, Jochen Liske, Danail Obreschkow, Edward N Taylor, Angus H Wright, Mehmet Alpaslan, Steven P Bamford, Amanda E Bauer, Joss Bland-Hawthorn, Maciej Bilicki, Matías Bravo, Sarah Brough, Sarah Casura, Michelle E Cluver, Matthew Colless, Christopher J Conselice, Scott M Croom, Jelte de Jong, Franceso D’Eugenio, Roberto De Propris, Burak Dogruel, Michael J Drinkwater, Andrej Dvornik, Daniel J Farrow, Carlos S Frenk, Benjamin Giblin, Alister W Graham, Meiert W Grootes, Madusha L P Gunawardhana, Abdolhosein Hashemizadeh, Boris Häußler, Catherine Heymans, Hendrik Hildebrandt, Benne W Holwerda, Andrew M Hopkins, Tom H Jarrett, D Heath Jones, Lee S Kelvin, Soheil Koushan, Konrad Kuijken, Maritza A Lara-López, Rebecca Lange, Ángel R López-Sánchez, Jon Loveday, Smriti Mahajan, Martin Meyer, Amanda J Moffett, Nicola R Napolitano, Peder Norberg, Matt S Owers, Mario Radovich, Mojtaba Raouf, John A Peacock, Steven Phillipps, Kevin A Pimbblet, Cristina Popescu, Khaled Said, Anne E Sansom, Mark Seibert, Will J Sutherland, Jessica E Thorne, Richard J Tuffs, Ryan Turner, Arjen van der Wel, Eelco van Kampen, Steve M Wilkins
Publikováno v: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 513(1), 439-467. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, Vol.513(1), pp.439-467 [Peer Reviewed Journal]
2022, ' Galaxy And Mass Assembly (GAMA) Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions ', Monthly Notices of the Royal Astronomical Society, vol. 513, no. 1, pp. 439-467 . https://doi.org/10.1093/mnras/stac472
Monthly Notices of the Royal Astronomical Society, 513(1), 439-467
In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earlier surveys, results in 330542 redshifts across five sky regions coveri
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04c745d723e0af45b8c35921975bc75f
https://doi.org/10.1093/mnras/stac472
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4
A super-linear 'radio-AGN main sequence' links mean radio-AGN power and galaxy stellar mass since z$\sim$3
Autor: I. Delvecchio, E. Daddi, M. T. Sargent, J. Aird, J. R. Mullaney, B. Magnelli, D. Elbaz, L. Bisigello, L. Ceraj, S. Jin, B. S. Kalita, D. Liu, M. Novak, I. Prandoni, J. F. Radcliffe, C. Spingola, G. Zamorani, V. Allevato, G. Rodighiero, V. Smolčić
Publikováno v: Delvecchio, I, Daddi, E, Sargent, M T, Aird, J, Mullaney, J R, Magnelli, B, Elbaz, D, Bisigello, L, Ceraj, L, Jin, S, Kalita, B S, Liu, D, Novak, M, Prandoni, I, Radcliffe, J F, Spingola, C, Zamorani, G, Allevato, V, Rodighiero, G & Smolčić, V 2022, ' A super-linear 'radio-AGN main sequence' links mean radio-AGN power and galaxy stellar mass since z ~ 3 ', Astronomy and Astrophysics, vol. 668, A81 . https://doi.org/10.1051/0004-6361/202244639
Delvecchio, I, Daddi, E, Sargent, M T, Aird, J, Mullaney, J R, Magnelli, B, Elbaz, D, Bisigello, L, Ceraj, L, Jin, S, Kalita, B S, Liu, D, Novak, M, Prandoni, I, Radcliffe, J F, Spingola, C, Zamorani, G, Allevato, V, Rodighiero, G & Smolcic, V 2022, ' A super-linear ‘radio-AGN main sequence’ links mean radio-AGN power and galaxy stellar mass since z ∼ 3 ', Astronomy and Astrophysics, vol. 668, A81, pp. 1-27 . https://doi.org/10.1051/0004-6361/202244639
Mapping the average AGN luminosity across galaxy populations and over time encapsulates important clues on the interplay between supermassive black hole (SMBH) and galaxy growth. This paper presents the demography, mean power and cosmic evolution of
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c5742a11d77b97a3f70c85e72ab91c11
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5
J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
Autor: Mariano Moles, A. Lumbreras-Calle, Lluís Galbany, Jailson Alcaniz, David Cristóbal-Hornillos, Kerttu Viironen, José M. Vílchez, C. López-Sanjuan, R. M. González Delgado, Laerte Sodré, Antonio Marín-Franch, R. A. Dupke, C. Hernández-Monteagudo, Patricia Sanchez-Blazquez, Raul E. Angulo, Jesús A. Varela, David Sobral, R. Logroño-García, G. Vilella-Rojo, Alessandro Ederoclite, Antonio Hernán-Caballero, H. Vázquez Ramió, A. J. Cenarro
Publikováno v: Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 650
Aims. Our goal is to estimate the star formation main sequence (SFMS) and the star formation rate density (SFRD) at z = 0.017 (d . 75 Mpc) using the Javalambre Photometric Local Universe Survey (J-PLUS) first data release, that probes 897.4 deg2 with
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a264c6b34b813acae27c15f5da17fa3c
http://hdl.handle.net/10261/247359
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6
The OTELO survey: Faint end of the luminosity function of [O II]3727 emitters at ⟨z⟩ = 1.43
Autor: Miguel Sánchez-Portal, José A. de Diego, B. Cedrés, J. Ignacio González-Serrano, Maritza A. Lara-López, Carmen P. Padilla Torres, Ana María Pérez García, Héctor O. Castañeda, Mauro González, J. Jesús González, Ángel Bongiovanni, Jesús Gallego, Ricardo Pérez Martínez, Jordi Cepa, Miguel Cerviño, Rocío Navarro Martínez, Emilio J. Alfaro, Jakub Nadolny
Publikováno v: Astronomy & Astrophysics, 2021, 649, A73
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
Digital.CSIC. Repositorio Institucional del CSIC
E-Prints Complutense. Archivo Institucional de la UCM
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Cedres, B, Bongiovanni, A, Cervino, M, Nadolny, J, Cepa, J, de Diego, J A, Perez Garcia, A M, Gallego, J, Lara-Lopez, M A, Sanchez-Portal, M, Gonzalez-Serrano, J, Alfaro, E J, Navarro Martinez, R, Perez Martinez, R, Gonzalez, J J, Padilla Torres, C P, Castaneda, H O & Gonzalez, M 2021, ' The OTELO survey : Faint end of the luminosity function of [OII]3727 emitters at z=1.43 ', Astronomy & Astrophysics, vol. 649, A73 . https://doi.org/10.1051/0004-6361/202039880
[Aims]: In this paper, we aim to study the main properties and luminosity function (LF) of the [O II]3727 emitters detected in the OTELO survey in order to characterise the star formation processes in low-mass galaxies at z ∼ 1.43 and to constrain
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9daa53f0b3a8c920078c2b15ff2fec9
http://hdl.handle.net/10261/246942
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7
The ALPINE-ALMA [C II] survey:Luminosity function of serendipitous [C II] line emitters at z similar to 5
Autor: Loiacono, Federica, Decarli, Roberto, Gruppioni, Carlotta, Talia, Margherita, Cimatti, Andrea, Zamorani, Gianni, Pozzi, Francesca, Yan, Lin, Lemaux, Brian C., Riechers, Dominik A., Le Fevre, Olivier, Bethermin, Matthieu, Capak, Peter, Cassata, Paolo, Faisst, Andreas, Schaerer, Daniel, Silverman, John D., Bardelli, Sandro, Boquien, Mederic, Burkutean, Sandra, Dessauges-Zavadsky, Miroslava, Fudamoto, Yoshinobu, Fujimoto, Seiji, Ginolfi, Michele, Hathi, Nimish P., Jones, Gareth C., Khusanova, Yana, Koekemoer, Anton M., Lagache, Guilaine, Lubin, Lori M., Massardi, Marcella, Oesch, Pascal, Romano, Michael, Vallini, Livia, Vergani, Daniela, Zucca, Elena
Publikováno v: Loiacono, F, Decarli, R, Gruppioni, C, Talia, M, Cimatti, A, Zamorani, G, Pozzi, F, Yan, L, Lemaux, B C, Riechers, D A, Le Fevre, O, Bethermin, M, Capak, P, Cassata, P, Faisst, A, Schaerer, D, Silverman, J D, Bardelli, S, Boquien, M, Burkutean, S, Dessauges-Zavadsky, M, Fudamoto, Y, Fujimoto, S, Ginolfi, M, Hathi, N P, Jones, G C, Khusanova, Y, Koekemoer, A M, Lagache, G, Lubin, L M, Massardi, M, Oesch, P, Romano, M, Vallini, L, Vergani, D & Zucca, E 2021, ' The ALPINE-ALMA [C II] survey : Luminosity function of serendipitous [C II] line emitters at z similar to 5 ', Astronomy & Astrophysics, vol. 646, A76 . https://doi.org/10.1051/0004-6361/202038607
We present the first [C II] 158 mu m luminosity function (LF) at z similar to 5 from a sample of serendipitous lines detected in the ALMA Large Program to INvestigate [C II] at Early times (ALPINE). A study of the 118 ALPINE pointings revealed severa
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______2751::6128d90b29791d2ece387826c999d753
https://curis.ku.dk/portal/da/publications/the-alpinealma-c-ii-survey(0f0da2b8-a9d8-4835-9df7-cdb2c7bcc1fa).html
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8
The OTELO survey revealing a population of low-luminosity active star-forming galaxies at z ∼ 0.9
Autor: Laia Barrufet, Mauro González-Otero, Miguel Sánchez-Portal, Ricardo Pérez-Martínez, J. Jesús González, Héctor O. Castañeda, Carmen P. Padilla Torres, B. Cedrés, José A. de Diego, Emilio J. Alfaro, Jakub Nadolny, J. Ignacio González-Serrano, Jesús Gallego, A. M. Pérez-García, Jordi Cepa, Rocío Navarro Martínez, M. A. Lara-Lopez, Miguel Cerviño, Ángel Bongiovanni
Publikováno v: E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
Astronomy & Astrophysics, 2021, 653, A24
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
[Aims]: We study a sample of Hβ emission line sources at z ∼ 0.9 to identify the star-forming galaxies sample and characterise them in terms of line luminosity, stellar mass, star formation rate, and morphology. The final aim is to obtain the Hβ
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec18ab5cef16455d7d8375e6564b4db3
https://eprints.ucm.es/id/eprint/68017/1/jesusgallego149preprint.pdf
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9
Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
Autor: Nicolas Gillet, Andrei Mesinger, Denys Savchenko, Anton Rudakovskyi
Publikováno v: Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 507 (2), pp.3046-3056. ⟨10.1093/mnras/stab2333⟩
The number density of small dark matter (DM) halos hosting faint high-redshift galaxies is sensitive to the DM free-streaming properties. However, constraining these DM properties is complicated by degeneracies with the uncertain baryonic physics gov
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13ec7763d4bb2748993e994e13c0f661
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