Zobrazeno 1 - 10
of 3 361
pro vyhledávání: '"A García Marin"'
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:
Gómez, A. Crespo, Colina, L., Álvarez-Márquez, J., Bik, A., Boogaard, L., Östlin, G., Peißker, F., Walter, F., Labiano, A., Pérez-González, P. G., Greve, T. R., Wright, G., Alonso-Herrero, A., Caputi, K. I., Costantin, L., Eckart, A., García-Marín, M., Gillman, S., Hjorth, J., Iani, E., Langeroodi, D., Pye, J. P., Rinaldi, P., Tikkanen, T., van der Werf, P., Lagage, P. O., van Dishoeck, E. F.
Despite the importance of the dusty star-forming galaxies (DSFGs) at $z$>2 for understanding the galaxy evolution in the early Universe, their stellar distributions traced by the near-IR emission were spatially unresolved until the arrival of the JWS
Externí odkaz:
http://arxiv.org/abs/2402.18672
A NIRCam-dark galaxy detected with the MIRI/F1000W filter in the MIDIS/JADES Hubble Ultra Deep Field
Autor:
Pérez-González, Pablo G., Rinaldi, Pierluigi, Caputi, Karina I., Álvarez-Márquez, Javier, Annunziatella, Marianna, Langeroodi, Danial, Moutard, Thibaud, Boogaard, Leindert, Iani, Edoardo, Melinder, Jens, Costantin, Luca, Östlin, Goran, Colina, Luis, Greve, Thomas R., Wright, Gillian, Alonso-Herrero, Almudena, Bik, Arjan, Bosman, Sarah E. I., Gómez, Alejandro Crespo, Dicken, Daniel, Eckart, Andreas, García-Marín, Macarena, Gillman, Steven, Güdel, Manuel, Henning, Thomas, Hjorth, Jens, Jermann, Iris, Labiano, Álvaro, Meyer, Romain A., Peisker, Florian, Pye, John P., Ray, Thomas P., Tikkanen, Tuomo, Walter, Fabian, van der Werf, Paul P.
We report the discovery of Cerberus, an extremely red object detected with the MIRI Deep Imaging Survey (MIDIS) observations in the F1000W filter of the Hubble Ultra Deep Field. The object is detected at $S/N\sim6$, with $\mathrm{F1000W}\sim27$ mag,
Externí odkaz:
http://arxiv.org/abs/2402.16942
Autor:
Rinaldi, P., Caputi, K. I., Iani, E., Costantin, L., Gillman, S., Perez-Gonzalez, P. G., Ostlin, G., Colina, L., Greve, T. R., Noorgard-Nielsen, H. U., Wright, G. S., Alvarez-Marquez, J., Eckart, A., Garcia-Marin, M., Hjorth, J., Ilbert, O., Kendrew, S., Labiano, A., Fevre, O. Le, Pye, J., Tikkanen, T., Walter, F., van der Werf, P., Ward, M., Annunziatella, M., Azzollini, R., Bik, A., Boogaard, L., Bosman, S. E. I., Gomez, A. Crespo, Jermann, I., Langeroodi, D., Melinder, J., Meyer, R. A., Moutard, T., Peissker, F., Gudel, M., Henning, Th., Lagage, P. -O., Ray, T., Vandenbussche, B., Waelkens, C., Dayal, P.
By using the ultra-deep \textit{JWST}/MIRI image at 5.6 $\mu m$ in the Hubble eXtreme Deep Field, we constrain the role of strong H$\alpha$-emitters (HAEs) during Cosmic Reionization at $z\simeq7-8$. Our sample of HAEs is comprised of young ($<35\;\r
Externí odkaz:
http://arxiv.org/abs/2309.15671
Autor:
Álvarez-Márquez, J., Colina, L., Gómez, A. Crespo, Rinaldi, P., Melinder, J., Östlin, G., Annunziatella, M., Labiano, A., Bik, A., Bosman, S., Greve, T. R., Wright, G., Alonso-Herrero, A., Boogaard, L., Azollini, R., Caputi, K. I., Costantin, L., Eckart, A., GarcÍa-MarÍn, M., Gillman, S., Hjorth, J., Iani, E., Ilbert, O., Jermann, I., Langeroodi, D., Meyer, R., Peissker, F., Pérez-González, P., Pye, J. P., Tikkanen, T., Topinka, M., van der Werf, P., Walter, F., Henning, Th., Ray, T.
Publikováno v:
A&A 686, A85 (2024)
We present MIRI/JWST medium-resolution spectroscopy (MRS) and imaging (MIRIM) of the lensed galaxy MACS1149-JD1 at a redshift of $z$=9.1092$\pm$0.0002 (Universe age about 530 Myr). We detect, for the first time, spatially resolved H$\alpha$ emission
Externí odkaz:
http://arxiv.org/abs/2309.06319
ONLINE APPENDIX -Alfalla-Luque, Luján-García, Marin-Garcia(2023)“Supply chain agility and performance: Evidence from a Meta-Analysis" . International Journal of Operations & Production Management. DOI: https://doi.org/10.1108/IJOPM-05-2022-0316
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f0d20f5a038c4c6968e3a706e8b3c53
Autor:
Bosman, Sarah E. I., Álvarez-Márquez, Javier, Colina, Luis, Walter, Fabian, Alonso-Herrero, Almudena, Ward, Martin J., Östlin, Göran, Greve, Thomas R., Wright, Gillian, Bik, Arjan, Boogaard, Leindert, Caputi, Karina I., Costantin, Luca, Eckart, Andreas, García-Marín, Macarena, Gillman, Steven, Güdel, Manuel, Henning, Thomas, Hjorth, Jens, Iani, Edoardo, Ilbert, Olivier, Jermann, Iris, Labiano, Alvaro, Lagage, Pierre-Olivier, Langeroodi, Danial, Peißker, Florian, Ray, Tom P., Rinaldi, Pierluigi, Topinka, Martin, van Dishoeck, Ewine F., van der Werf, Paul, Vandenbussche, Bart
We present a JWST/MRS spectrum of the quasar J1120+0641 at z=7.0848, the first spectroscopic observation of a reionisation-era quasar in the rest-frame infrared ($0.6<\lambda<3.4\mu$m). In the context of the mysterious fast assembly of the first supe
Externí odkaz:
http://arxiv.org/abs/2307.14414
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:
Pérez-González, Pablo G., Costantin, Luca, Langeroodi, Danial, Rinaldi, Pierluigi, Annunziatella, Marianna, Ilbert, Olivier, Colina, Luis, Noorgaard-Nielsen, Hans Ulrik, Greve, Thomas, Ostlin, Göran, Wright, Gillian, Alonso-Herrero, Almudena, Álvarez-Márquez, Javier, Caputi, Karina I., Eckart, Andreas, Fèvre, Olivier Le, Labiano, Álvaro, García-Marín, Macarena, Hjorth, Jens, Kendrew, Sarah, Pye, John P., Tikkanen, Tuomo, van der Werf, Paul, Walter, Fabian, Ward, Martin, Bik, Arjan, Boogaard, Leindert, Bosman, Sarah E. I., Gómez, Alejandro Crespo, Gillman, Steven, Iani, Edoardo, Jermann, Iris, Melinder, Jens, Meyer, Romain A., Moutard, Thibaud, van Dishoek, Ewine, Henning, Thomas, Lagage, Pierre-Olivier, Guedel, Manuel, Peissker, Florian, Ray, Tom, Vandenbussche, Bart, García-Argumánez, Ángela, Mérida, Rosa María
We present the ultraviolet luminosity function and an estimate of the cosmic star formation rate density at $8
Externí odkaz:
http://arxiv.org/abs/2302.02429
Autor:
Rinaldi, P., Caputi, K. I., Costantin, L., Gillman, S., Iani, E., Gonzalez, P. G. Perez, Oestlin, G., Colina, L., Greve, T., Noorgard-Nielsen, H. U., Wright, G. S., Alonso-Herrero, A., Alvarez-Marquez, J., Eckart, A., Garcia-Marin, M., Hjorth, J., Ilbert, O., Kendrew, S., Labiano, A., Fevre, O. Le, Pye, J., Tikkanen, T., Walter, F., van der Werf, P., Ward, M., Annunziatella, M., Azzollini, R., Bik, A., Boogard, L., Bosman, S., Crespo, A., Jermann, I., Langeroodi, D., Melinder, J., Meyer, R., Moutard, T., Peissker, F., Topinka, M., van Dishoeck, E., Guedel, M., Henning, Th., Lagage, P. -O., Ray, T., Vandenbussche, B., Waelkens, C., Navarro-Carrera, R., Kokorev, V.
We make use of \textit{JWST} medium and broad-band NIRCam imaging, along with ultra-deep MIRI $5.6 \rm \mu m$ imaging, in the Hubble eXtreme Deep Field (XDF) to identify prominent line emitters at $z\simeq 7-8$. Out of a total of 58 galaxies at $z\si
Externí odkaz:
http://arxiv.org/abs/2301.10717