Zobrazeno 1 - 10
of 1 513
pro vyhledávání: '"Marin, M. P."'
Autor:
Nanayakkara, Themiya, Glazebrook, Karl, Schreiber, Corentin, Chittenden, Harry, Brammer, Gabriel, Esdaile, James, Jacobs, Colin, Kacprzak, Glenn G., Kawinwanichakij, Lalitwadee, Kimmig, Lucas C., Labbe, Ivo, Lagos, Claudia, Marchesini, Danilo, Martìnez-Marìn, M., Marsan, Z. Cemile, Oesch, Pascal A., Papovich, Casey, Remus, Rhea-Silvia, Tran, Kim-Vy H.
We present the formation histories of 19 massive ($\gtrsim3\times10^{10}\text{M}_\odot$) quiescent galaxy candidates at $z\sim3.0-4.5$ observed using JWST/NIRSpec. This completes the spectroscopic confirmation of the 24 $K$-selected quiescent galaxy
Externí odkaz:
http://arxiv.org/abs/2410.02076
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:
Velusamy, Thangasamy, Dorcey, Ryan, Kreuser-Jenkins, Nancy, Lamb, Lisa Nichole, Pagano, Erica, Anderson, Marin M., Lazio, Joseph, Levin, Steven
Publikováno v:
2024,RNAAS, 8,163
The Goldstone-Apple Valley Radio Telescope (GAVRT) project conducts a regular monitoring program of the Sun. The GAVRT Solar Patrol project uses a 34 m diameter antenna to produce raster-scan maps of the Sun simultaneously at 4 frequencies ranging fr
Externí odkaz:
http://arxiv.org/abs/2407.00223
Autor:
Martínez-Marín, M., Glazebrook, K., Nanayakkara, T., Jacobs, C., Labbé, I., Kacprzak, G. G., Papovich, C., Schreiber, C.
We present a sample of 22 massive galaxies with stellar masses $>10^{10} M_{\odot}$ at $3
Externí odkaz:
http://arxiv.org/abs/2405.12501
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.
Publikováno v:
A&A 691, A325 (2024)
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
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:
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
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:
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