Zobrazeno 1 - 10
of 117
pro vyhledávání: '"Hinz, J. L."'
Autor:
Dale, D. A., Cook, D. O., Roussel, H., Turner, J. A., Armus, L., Bolatto, A. D., Boquien, M., Brown, M. J. I., Calzetti, D., Looze, I. De, Galametz, M., Gordon, K. D., Groves, B. A., Jarrett, T. H., Helou, G., Herrera-Camus, R., Hinz, J. L., Hunt, L. K., Kennicutt, R. C., Murphy, E. J., Rest, A., Sandstrom, K. M., Smith, J.-D. T., Tabatabaei, F. S., Wilson, C. D.
We present an update to the ultraviolet-to-radio database of global broadband photometry for the 79 nearby galaxies that comprise the union of the KINGFISH (Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel) and SINGS (Spitzer Infr
Externí odkaz:
http://hdl.handle.net/10150/624375
http://arizona.openrepository.com/arizona/handle/10150/624375
http://arizona.openrepository.com/arizona/handle/10150/624375
Autor:
Hunt, L. K., De Looze, I., Boquien, M., Nikutta, R., Rossi, A., Bianchi, S., Dale, D. A., Granato, G. L., Kennicutt, R. C., Silva, L., Ciesla, L., Relano, M., Viaene, S., Brandl, B., Calzetti, D., Croxall, K. V., Draine, B. T., Galametz, M., Gordon, K. D., Groves, B. A., Helou, G., Herrera-Camus, R., Hinz, J. L., Koda, J., Salim, S., Sandstrom, K. M., Smith, J. D., Wilson, C. D., Zibetti, S.
Publikováno v:
A&A 621, A51 (2019)
We have fit the far-ultraviolet (FUV) to sub-millimeter (850 micron) spectral energy distributions (SEDs) of the 61 galaxies from the "Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel" (KINGFISH). The fitting has been performed us
Externí odkaz:
http://arxiv.org/abs/1809.04088
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
Autor:
Zaritsky, Dennis, Courtois, Helene, Muñoz-Mateos, Juan-Carlos, Sorce, Jenny, Erroz-Ferrer, S., Comerón, S., Gadotti, D. A., de Paz, A. Gil, Hinz, J. L., Laurikainen, E., Kim, T., Laine, J., Menéndez-Delmestre, K., Mizusawa, T., Regan, M. W., Salo, H., Seibert, M., Sheth, K., Athanassoula, E., Bosma, A., Cisternas, M., Ho, Luis C., Holwerda, B.
We combine data from the Spitzer Survey for Stellar Structure in Galaxies (S$^4$G), a recently calibrated empirical stellar mass estimator from Eskew et al., and an extensive database of HI spectral line profiles to examine the baryonic Tully-Fisher
Externí odkaz:
http://arxiv.org/abs/1402.6315
Autor:
Comerón, S., Salo, H., Laurikainen, E., Knapen, J. H., Buta, R. J., Herrera-Endoqui, M., Laine, J., Holwerda, B. W., Sheth, K., Regan, M. W., Hinz, J. L., Muñoz-Mateoz, J. C., de Paz, A. Gil, Menéndez-Delmestre, K., Seibert, M., Mizusawa, T., Kim, T., Erroz-Ferrer, S., Gadotti, D. A., Athanassoula, E., Bosma, A., Ho, L. C.
Resonance rings are the consequence of secular evolution processes that redistribute material and angular momentum in discs. We produced a Catalogue and an Atlas of the rings detected in the Spitzer Survey of Stellar Structure in Galaxies (S4G) and t
Externí odkaz:
http://arxiv.org/abs/1312.0866
Autor:
Holwerda, B. W., Munoz-Mateos, J-C., Comeron, S., Meidt, S., Sheth, K., Laine, S., Hinz, J. L., Regan, M. W., Gil-de-Paz, A., Menendez-Delmestre, K., Seibert, M., Kim, T., Mizusawa, T., Laurikainen, E., Salo, H., Laine, J., Gadotti, D. A., Zaritsky, D., Erroz-Ferrer, S., Ho, L. C., Knapen, J. H., Athanassoula, E., Bosma, A., Pirzkal, N.
The morphology of galaxies can be quantified to some degree using a set of scale-invariant parameters. Concentration (C), Asymmetry (A), Smoothness (S), the Gini index (G), relative contribution of the brightest pixels to the second order moment of t
Externí odkaz:
http://arxiv.org/abs/1309.1444
Autor:
Croxall, Kevin V., Smith, J. D., Brandl, B. R., Groves, B. A., Kennicutt, R. C., Kreckel, K., Johnson, B. D., Pellegrini, E., Sandstrom, K. M., Walter, F., Armus, L., Beirao, P., Calzetti, D., Dale, D. A., Galametz, M., Hinz, J. L., Hunt, L. K., Koda, J., Schinnerer, E.
Publikováno v:
2013 ApJ 777 96
The metal content of a galaxy is a key property for distinguishing between viable galaxy evolutionary scenarios, and it strongly influences many of the physical processes in the interstellar medium. An absolute and robust determination of extragalact
Externí odkaz:
http://arxiv.org/abs/1309.0817
Autor:
Muñoz-Mateos, J. C., Sheth, K., de Paz, A. Gil, Meidt, S. E., Athanassoula, E., Bosma, A., Comerón, S., Elmegreen, D. M., Elmegreen, B. G., Erroz-Ferrer, S., Gadotti, D. A., Hinz, J. L., Ho, L. C., Holwerda, B., Jarrett, T. H., Kim, T., Knapen, J. H., Laine, J., Laurikainen, E., Madore, B. F., Menendez-Delmestre, K., Mizusawa, T., Regan, M., Salo, H., Schinnerer, E., Seibert, M., Skibba, R., Zaritsky, D.
We have analyzed the radial distribution of old stars in a sample of 218 nearby face-on disks, using deep 3.6um images from the Spitzer Survey of Stellar Structure in Galaxies (S4G). In particular, we have studied the structural properties of those d
Externí odkaz:
http://arxiv.org/abs/1304.6083
Autor:
Galametz, M., Kennicutt, R. C., Calzetti, D., Aniano, G., Draine, B. T., Boquien, M., Brandl, B., Croxall, K. V., Dale, D. A., Engelbracht, C. W., Gordon, K. D., Groves, B., Hao, C. -N., Helou, G., Hinz, J. L., Hunt, L. K., Johnson, B. D., Li, Y., Murphy, E., Roussel, H., Sandstrom, K., Skibba, R. A., Tabatabaei, F. S.
We present new empirical calibrations to estimate resolved and integrated total infrared luminosities from Spitzer and Herschel bands used as monochromatic or combined tracers. We base our calibrations on resolved elements of nearby galaxies (3 to 30
Externí odkaz:
http://arxiv.org/abs/1302.4363