Zobrazeno 1 - 10
of 260
pro vyhledávání: '"Muñoz-Mateos, J. C."'
Autor:
Querejeta, M., Schinnerer, E., Meidt, S., Sun, J., Leroy, A. K., Emsellem, E., Klessen, R. S., Munoz-Mateos, J. C., Salo, H., Laurikainen, E., Beslic, I., Blanc, G. A., Chevance, M., Dale, D. A., Eibensteiner, C., Faesi, C., Garcia-Rodriguez, A., Glover, S. C. O., Grasha, K., Henshaw, J., Herrera, C., Hughes, A., Kreckel, K., Kruijssen, J. M. D., Liu, D., Murphy, E. J., Pan, H. -A., Pety, J., Razza, A., Rosolowsky, E., Saito, T., Schruba, A., Usero, A., Watkins, E. J., Williams, T. G.
Publikováno v:
A&A 656, A133 (2021)
We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct morphological masks of sub-galactic environments based on Spitzer 3.6 micron images. At the simplest level, we distinguish centres, bars, spiral arms, interarm an
Externí odkaz:
http://arxiv.org/abs/2109.04491
Autor:
Ramirez-Moreta, P., Verdes-Montenegro, L., Blasco-Herrera, J., Leon, S., Venhola, A., Yun, M., Peris, V., Peletier, R., Kleijn, G. Verdoes, Unda-Sanzana, E., Espada, D., Bosma, A., Athanassoula, E., Argudo-Fernandez, M., Sabater, J., Munoz-Mateos, J. C., Jones, M. G., Huchtmeier, W., Ruiz, J. E., Iglesias-Paramo, J., Fernandez-Lorenzo, M., Beckman, J., Sanchez-Exposito, S., Garrido, J.
Publikováno v:
A&A 619, A163 (2018)
Asymmetries in HI in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project has demonstrated that isolated galaxies show the lowest level of asymme
Externí odkaz:
http://arxiv.org/abs/1809.09949
Autor:
Holoien, T. W. -S., Brown, J. S., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Prieto, J. L., Dong, Subo, Brimacombe, J., Bishop, D. W., Basu, U., Beacom, J. F., Bersier, D., Chen, Ping, Danilet, A. B., Falco, E., Godoy-Rivera, D., Goss, N., Pojmanski, G., Simonian, G. V., Skowron, D. M., Thompson, Todd A., Woźniak, P. R., Avíla, C. G., Bock, G., Carballo, J. -L. G., Conseil, E., Contreras, C., Cruz, I., andújar, J. M. F., Guo, Zhen, Hsiao, E. Y., Kiyota, S., Koff, R. A., Krannich, G., Madore, B. F., Marples, P., Masi, G., Morrell, N., Monard, L. A. G., Munoz-Mateos, J. C., Nicholls, B., Nicolas, J., Wagner, R. M., Wiethoff, W. S.
This manuscript presents information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during 2015, its second full year of operations. The same information is presented for bright ($m_V\leq17$), spectroscopically
Externí odkaz:
http://arxiv.org/abs/1610.03061
Autor:
Barro, G., Kriek, M., Pérez-González, P. G., Trump, J. R., Koo, D. C., Faber, S. M., Dekel, A., Primack, J. R., Guo, Y., Kocevski, D. D., Muñoz-Mateos, J. C., Rujoparkarn, W., Sheth, K.
We present spatially-resolved Atacama Large Millimeter/sub-millimeter Array (ALMA) 870 $\mu$m dust continuum maps of six massive, compact, dusty star-forming galaxies (SFGs) at $z\sim2.5$. These galaxies are selected for their small rest-frame optica
Externí odkaz:
http://arxiv.org/abs/1607.01011
Autor:
van der Wel, A., Noeske, K., Bezanson, R., Pacifici, C., Gallazzi, A., Franx, M., Munoz-Mateos, J. C., Bell, E. F., Brammer, G., Charlot, S., Chauke, P., Labbe, I., Maseda, M. V., Muzzin, A., Rix, H. -W., Sobral, D., van de Sande, J., van Dokkum, P. G., Wild, V., Wolf, C.
The Large Early Galaxy Census (LEGA-C) is a Public Spectroscopic Survey of $\sim3200$ $K$-band selected galaxies at redshifts $z=0.6-1.0$ with stellar masses M_star > 1e10M_sun, conducted with VIMOS on ESO's Very Large Telescope. The survey is embedd
Externí odkaz:
http://arxiv.org/abs/1603.05479
Autor:
Catalán-Torrecilla, C., de Paz, A. Gil, Castillo-Morales, A., Iglesias-Páramo, J., Sánchez, S. F., Kennicutt, R. C., Pérez-González, P. G., Marino, R. A., Walcher, C. J., Husemann, B., García-Benito, R., Mast, D., Delgado, R. M. González, Muñoz-Mateos, J. C., Bland-Hawthorn, J., Bomans, D. J., del Olmo, A., Galbany, L., Gomes, J. M., Kehrig, C., López-Sánchez, Á. R., Mendoza, M. A., Monreal-Ibero, A., Pérez-Torres, M., Sánchez-Blázquez, P., Vilchez, J. M., collaboration, the CALIFA
Publikováno v:
A&A 584, A87 (2015)
The Star Formation Rate (SFR) is one of the main parameters used to analyze the evolution of galaxies through time. The need for recovering the light reprocessed by dust commonly requires the use of low spatial resolution far-infrared data. Recombina
Externí odkaz:
http://arxiv.org/abs/1507.03801
Autor:
Buta, R., Sheth, K., Athanassoula, E., Bosma, A., Knapen, J., Laurikainen, E., Salo, H., Elmegreen, D., Ho, L., Zaritsky, D., Courtois, H., Hinz, J., Muñoz-Mateos, J-C., Kim, T., Regan, M., Gadotti, D., de Paz, A. Gil, Laine, J., Menendez-Delmestre, K., Comeron, Sebastien, Ferrer, S. Erroz, Seibert, M., Mizusawa, T., Holwerda, B., Madore, B.
The Spitzer Survey of Stellar Structure in Galaxies (S4G) is the largest available database of deep, homogeneous middle-infrared (mid-IR) images of galaxies of all types. The survey, which includes 2352 nearby galaxies, reveals galaxy morphology only
Externí odkaz:
http://arxiv.org/abs/1501.00454
Autor:
Querejeta, M., Meidt, S. E., Schinnerer, E., Cisternas, M., Muñoz-Mateos, J. C., Sheth, K., Knapen, J., van de Ven, G., Norris, M. A., Peletier, R., Laurikainen, E., Salo, H., Holwerda, B. W., Athanassoula, E., Bosma, A., Groves, B., Ho, L. C., Gadotti, D. A., Zaritsky, D., Regan, M., Hinz, J., de Paz, A. Gil, Menendez-Delmestre, K., Seibert, M., Mizusawa, T., Kim, T., Erroz-Ferrer, S., Laine, J., Comerón, S.
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6$\mu m$ IRAC band has been exploited to this effect, but such mass estimates can be biased by dust emission. We present our pipeline to reveal the old stellar f
Externí odkaz:
http://arxiv.org/abs/1410.0009
Autor:
Hunt, L. K., Draine, B. T., Bianchi, S., Gordon, K. D., Aniano, G., Calzetti, D., Dale, D. A., Helou, G., Hinz, J. L., Kennicutt, R. C., Roussel, H., Wilson, C. D., Bolatto, A., Boquien, M., Croxall, K. V., Galametz, M., de Paz, A. Gil, Koda, J., Munoz-Mateos, J. C., Sandstrom, K. M., Sauvage, M., Vigroux, L., Zibetti, S.
Publikováno v:
A&A 576, A33 (2015)
Physical conditions of the interstellar medium in galaxies are closely linked to the ambient radiation field and the heating of dust grains. In order to characterize dust properties in galaxies over a wide range of physical conditions, we present her
Externí odkaz:
http://arxiv.org/abs/1409.5916
Autor:
Laine, J., Laurikainen, E., Salo, H., Comerón, S., Buta, R. J., Zaritsky, D., Athanassoula, E., Bosma, A., Muñoz-Mateos, J. C., Gadotti, D. A., Hinz, J. L., Erroz-Ferrer, S., de Paz, A. Gil, Kim, T., Menéndez-Delmestre, K., Mizusawa, T., Regan, M. W., Seibert, M., Sheth, K.
Publikováno v:
MNRAS 441, 3 (2015)
We study the surface brightness profiles of disc galaxies in the 3.6 micron images from the Spitzer Survey of Stellar Structure in Galaxies (S4G) and K_s-band images from the Near Infrared S0-Sa galaxy Survey (NIRS0S). We particularly connect propert
Externí odkaz:
http://arxiv.org/abs/1404.0559