Zobrazeno 1 - 10
of 490
pro vyhledávání: '"Smolcic, V."'
Autor:
Rujopakarn, W., Nyland, K., Rieke, G. H., Barro, G., Elbaz, D., Ivison, R. J., Jagannathan, P., Silverman, J. D., Smolčić, V., Wang, T.
We present a sub-kiloparsec localization of the sites of supermassive black hole (SMBH) growth in three active galactic nuclei (AGNs) at z similar to 3 in relation to the regions of intense star formation in their hosts. These AGNs are selected from
Externí odkaz:
http://hdl.handle.net/10150/627111
http://arizona.openrepository.com/arizona/handle/10150/627111
http://arizona.openrepository.com/arizona/handle/10150/627111
Autor:
Šlaus, B., Smolcic, V., Ivezic, Ž., Fotopoulou, S., Willott, C. J., Pendo, P., Vignali, C., Chiappetti, L., Pierre, M.
We model the evolution of active galactic nuclei by constructing their radio luminosity functions. We use a set of surveys of varying area and depth, namely the deep COSMOS survey of $1,916$ AGN sources, the wide shallow 3CRR, 7C and 6CE surveys, con
Externí odkaz:
http://arxiv.org/abs/2312.14683
Autor:
Jiménez-Andrade, E. F., Cantalupo, S., Magnelli, B., Romano-Díaz, E., Gómez-Guijarro, C., Mackenzie, R., Smolčić, V., Murphy, E., Matthee, J., Toft, S.
Ly$\alpha$ $\lambda$1216 (Ly$\alpha$) emission extending over $\gtrsim\,\rm 10\,kiloparsec\,(kpc)$ around dusty, massive starbursts at $z\gtrsim3$ might represent a short-lived phase in the evolution of present-day, massive quiescent galaxies. To obt
Externí odkaz:
http://arxiv.org/abs/2210.07982
Autor:
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.
Publikováno v:
A&A 668, A81 (2022)
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:
http://arxiv.org/abs/2209.12585
Autor:
Weaver, J. R., Kauffmann, O. B., Ilbert, O., McCracken, H. J., Moneti, A., Toft, S., Brammer, G., Shuntov, M., Davidzon, I., Hsieh, B. C., Laigle, C., Anastasiou, A., Jespersen, C. K., Vinther, J., Capak, P., Casey, C. M., McPartland, C. J. R., Milvang-Jensen, B., Mobasher, B., Sanders, D. B., Zalesky, L., Arnouts, S., Aussel, H., Dunlop, J. S., Faisst, A., Franx, M., Furtak, L. J., Fynbo, J. P. U., Gould, K. M. L., Greve, T. R., Gwyn, S., Kartaltepe, J. S., Kashino, D., Koekemoer, A. M., Kokorev, V., Fevre, O. Le, Lilly, S., Masters, D., Magdis, G., Mehta, V., Peng, Y., Riechers, D. A., Salvato, M., Sawicki, M., Scarlata, C., Scoville, N., Shirley, R., Sneppen, A., Smolcic, V., Steinhardt, C., Stern, D., Tanaka, M., Taniguchi, Y., Teplitz, H. I., Vaccari, M., Wang, W. -H., Zamorani, G.
The Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a wealth of new imaging and spectroscopic data has been collected in the COSMOS field. This paper describes the collectio
Externí odkaz:
http://arxiv.org/abs/2110.13923
Publikováno v:
A&A 646, A174 (2021)
Submillimetre galaxies (SMGs) are bright sources at submillimetre wavelengths. Made up of mostly of high-z galaxies, SMGs are amongst the most luminous dusty galaxies in the Universe. Studying their environments and clustering strength is thus import
Externí odkaz:
http://arxiv.org/abs/2101.02977
Autor:
Delvecchio, I., Daddi, E., Sargent, M. T., Jarvis, M. J., Elbaz, D., Jin, S., Liu, D., Whittam, I. H., Algera, H., Carraro, R., D'Eugenio, C., Delhaize, J., Kalita, B. S., Leslie, S., Molnar, D. Cs., Novak, M., Prandoni, I., Smolcic, V., Ao, Y., Aravena, M., Bournaud, F., Collier, J. D., Randriamampandry, S. M., Randriamanakoto, Z., Rodighiero, G., Schober, J., White, S. V., Zamorani, G.
Publikováno v:
A&A 647, A123 (2021)
Several works in the past decade have used the ratio between total (rest 8-1000$\mu$m) infrared and radio (rest 1.4~GHz) luminosity in star-forming galaxies (q$_{IR}$), often referred to as the "infrared-radio correlation" (IRRC), to calibrate radio
Externí odkaz:
http://arxiv.org/abs/2010.05510
Autor:
Van der Vlugt, D., Algera, H. S. B., Hodge, J. A., Novak, M., Radcliffe, J. F., Riechers, D. A., Röttgering, H., Smolčić, V., Walter, F.
We present ultra-deep, matched-resolution Karl G. Jansky Very Large Array (VLA) observations at 10 and $3$ GHz in the COSMOS field: the COSMOS-XS survey. The final 10 and $3$ GHz images cover $\sim16\rm{arcmin}^{2}$ and $\sim180\rm{arcmin}^{2}$ and r
Externí odkaz:
http://arxiv.org/abs/2009.13528
Autor:
Algera, H. S. B., Van der Vlugt, D., Hodge, J. A., Smail, I., Novak, M., Radcliffe, J. F., Riechers, D. A., Röttgering, H., Smolčić, V., Walter, F.
Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clear understanding of the relative contribution from radio AGN to be used to their fullest potential. We study the composition of the $\mu$Jy radio popul
Externí odkaz:
http://arxiv.org/abs/2009.13531
Autor:
Vardoulaki, E., Andrade, E. F. Jiménez, Delvecchio, I., Smolčić, V., Schinnerer, E., Sargent, M. T., Gozaliasl, G., Finoguenov, A., Bondi, M., Zamorani, G., Badescu, T., Leslie, S. K., Ceraj, L., Tisanić, K., Karim, A., Magnelli, B., Bertoldi, F., Romano-Diaz, E., Harrington, K.
Publikováno v:
A&A 648, A102 (2021)
($ABRIDGED$) We probe the physical properties and large-scale environment of radio AGN in the faintest FR population to-date, and link them to their radio structure. We use the VLA-COSMOS Large Project at 3 GHz, with resolution and sensitivity of 0".
Externí odkaz:
http://arxiv.org/abs/2009.10721