Zobrazeno 1 - 10
of 294
pro vyhledávání: '"Dicken, D."'
Autor:
Tadhunter, C., Oosterloo, T., Morganti, R., Almeida, C. Ramos, Martín, M. Villar, Emonts, B., Dicken, D.
The jets of radio AGN provide one of the most important forms of AGN feedback, yet considerable uncertainties remain about how they are triggered. Since the molecular gas reservoirs of the host galaxies can supply key information about the dominant t
Externí odkaz:
http://arxiv.org/abs/2407.10970
Autor:
Alonso-Herrero, A., Muñoz, L. Hermosa, Labiano, A., Guillard, P., Buiten, V. A., Dicken, D., van der Werf, P., Álvarez-Márquez, J., Böker, T., Colina, L., Eckart, A., García-Marín, M., Jones, O. C., Pantoni, L., Pérez-González, P. G., Rouan, D., Ward, M. J., Baes, M., Östlin, G., Royer, P., Wright, G. S., Güdel, M., Henning, Th., Lagage, P. -O., van Dishoeck, E. F.
We present JWST/MIRI MRS spatially resolved $\sim 5-28\,\mu$m observations of the central ~4-8kpc of the ultraluminous infrared galaxy and broad absorption line quasar Mrk231. These are part of the Mid-Infrared Characterization of Nearby Iconic galax
Externí odkaz:
http://arxiv.org/abs/2407.02180
Autor:
Costantin, L., Gillman, S., Boogaard, L. A., Pérez-González, P. G., Iani, E., Rinaldi, P., Melinder, J., Gómez, A. Crespo, Colina, L., Greve, T. R., Östlin, G., Wright, G., Alonso-Herrero, A., Álvarez-Márquez, J., Annunziatella, M., Bik., A., Caputi, K. I., Dicken, D., Eckart, A., Hjorth, J., Ilbert, O., Jermann, I., Labiano, A., Langeroodi, D., Peißker, F., Pye, J. P., Tikkanen, T. V., van der Werf, P. P., Walter, F., Ward, M., Güdel, M., Henning, T. K.
Thanks to decades of observations using HST, the structure of galaxies at redshift $z>2$ has been widely studied in the rest-frame ultraviolet regime, which traces recent star formation from young stellar populations. But, we still have little inform
Externí odkaz:
http://arxiv.org/abs/2407.00153
Autor:
Libralato, M., Argyriou, I., Dicken, D., Marín, M. García, Guillard, P., Hines, D. C., Kavanagh, P. J., Kendrew, S., Law, D. R., Noriega-Crespo, A., Álvarez-Márquez, J.
Astrometry is one of the main pillars of astronomy, and one of its oldest branches. Over the years, an increasing number of astrometric works by means of Hubble Space Telescope (HST) data have revolutionized our understanding of various phenomena. Wi
Externí odkaz:
http://arxiv.org/abs/2311.12145
Autor:
Colina, L., Gómez, A. Crespo, Álvarez-Márquez, J., Bik, A., Walter, F., Boogaard, L., Labiano, A., Peissker, F., Pérez-González, P., Östlin, G., Greve, T. R., Nørgaard-Nielsen, H. U., Wright, G., Alonso-Herrero, A., Azollini, R., Caputi, K. I., Dicken, D., García-Marín, M., Hjorth, J., Ilbert, O., Kendrew, S., Pye, J. P., Tikkanen, T., van der Werf, P., Costantin, L., Iani, E., Gillman, S., Jermann, I., Langeroodi, D., Moutard, T., Rinaldi, P., Topinka, M., van Dishoeck, E. F., Güdel, M., Henning, Th., Lagage, P. O., Ray, T., Vandenbussche, B.
Publikováno v:
A&A 673, L6 (2023)
Luminous infrared galaxies at high redshifts ($z$>4) include extreme starbursts that build their stellar mass over short periods of time (>100 Myr). These galaxies are considered to be the progenitors of massive quiescent galaxies at intermediate red
Externí odkaz:
http://arxiv.org/abs/2304.13529
Autor:
Dicken, D., Tadhunter, C. N., Nesvadba, N. P. H., Bernhard, E., Könyves, V., Morganti, R., Almeida, C. Ramos, Oosterloo, T.
The far-IR/sub-mm wavelength range contains a wealth of diagnostic information that is important for understanding the role of radio AGN in galaxy evolution. Here we present the results of Herschel PACS and SPIRE observations of a complete sample of
Externí odkaz:
http://arxiv.org/abs/2211.13031
Autor:
Álvarez-Márquez, J., Labiano, A., Guillard, P., Dicken, D., Argyriou, I., Patapis, P., Law, D. R., Kavanagh, P. J., Larson, K. L., Gasman, D., Mueller, M., Alberts, A., Brandl, B. R., Colina, L., García-Marín, M., Jones, O. C., Noriega-Crespo, A., Shivaei, I., Temim, T., Wright, G. S.
Publikováno v:
A&A 672, A108 (2023)
During the commissioning of the James Webb Space Telescope (JWST), the mid-infrared instrument (MIRI) observed NGC6552 with the MIRI Imager and the medium-resolution spectrograph (MRS). NGC6552 is an active galactic nucleus (AGN) at redshift 0.0266 c
Externí odkaz:
http://arxiv.org/abs/2209.01695
Autor:
Boccaletti, A., Cossou, C., Baudoz, P., Lagage, P. O., Dicken, D., Glasse, A., Hines, D. C., Aguilar, J., Detre, O., Nickson, B., Noriega-Crespo, A., Gáspár, A., Labiano, A., Stark, C., Rouan, D., Reess, J. M., Wright, G. S., Rieke, G., Marin, M. Garcia
Publikováno v:
A&A 667, A165 (2022)
Characterization of directly imaged exoplanets is one of the most eagerly anticipated science functions of the James Webb Space Telescope. MIRI, the mid-IR instrument has the capability to provide unique spatially resolved photometric data points in
Externí odkaz:
http://arxiv.org/abs/2207.11080
Autor:
Bernhard, E., Tadhunter, C. N., Pierce, J. C. S., Dicken, D., Morganti, R., Almeida, C. Ramos, Daddi, E.
We use deep Herschel observations of the complete 2Jy sample of powerful radio AGNs in the local universe (0.05 < z < 0.7) to probe their cool interstellar medium (ISM) contents and star-forming properties, comparing them against other samples of nea
Externí odkaz:
http://arxiv.org/abs/2202.08276
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