Zobrazeno 1 - 10
of 387
pro vyhledávání: '"Mizusawa, T."'
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:
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:
Meidt, Sharon E., Schinnerer, Eva, van de Ven, Glenn, Zaritsky, Dennis, Peletier, Reynier, Knapen, Johan, Sheth, Kartik, Regan, Michael, Querejeta, Miguel, Munoz-Mateos, Juan-Carlos, Kim, Taehyun, Hinz, Joannah L., de Paz, Armando Gil, Athanassoula, E., Bosma, Albert, Buta, Ronald J., Cisternas, Mauricio, Ho, Luis C., Holwerda, Benne, Skibba, Ramin, Laurikainen, E., Salo, H., Gadotti, D. A., Laine, Jarkko, Erroz-Ferrer, S., Comeron, Sebastien, Menendez-Delmestre, K., Seibert, M., Mizusawa, T.
We present a new approach for estimating the 3.6 micron stellar mass-to-light ratio in terms of the [3.6]-[4.5] colors of old stellar populations. Our approach avoids several of the largest sources of uncertainty in existing techniques. By focusing o
Externí odkaz:
http://arxiv.org/abs/1402.5210
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:
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:
Bosh, A.S., Person, M.J., Levine, S.E., Zuluaga, C.A., Zangari, A.M., Gulbis, A.A.S., Schaefer, G.H., Dunham, E.W., Babcock, B.A., Davis, A.B., Pasachoff, J.M., Rojo, P., Servajean, E., Förster, F., Oswalt, T., Batcheldor, D., Bell, D., Bird, P., Fey, D., Fulwider, T., Geisert, E., Hastings, D., Keuhler, C., Mizusawa, T., Solenski, P., Watson, B.
Publikováno v:
In Icarus 15 January 2015 246:237-246
Publikováno v:
In Journal of Sound and Vibration 2008 317(1):329-353