Zobrazeno 1 - 10
of 344
pro vyhledávání: '"Cisternas, M."'
Autor:
Bhuyan, H., Escalona, M., Villegas, R., Mal, E., Cisternas, M., Saikia, P., Bora, B., Kausik, S.S., Wyndham, E., Favre, M.
Publikováno v:
In Optics and Laser Technology February 2025 181 Part B
Autor:
Donley, J. L., Kartaltepe, J., Kocevski, D., Salvato, M., Santini, P., Suh, H., Civano, F., Koekemoer, A. M., Trump, J., Brusa, M., Cardamone, C., Castro, A., Cisternas, M., Conselice, C., Croton, D., Hathi, N., Liu, C., Lucas, R. A., Nair, P., Rosario, D., Sanders, D., Simmons, B., Villforth, C., Alexander, D. M., Bell, E. F., Faber, S. M., Grogin, N. A., Lotz, J., McIntosh, D. H., Nagao, T.
While major mergers have long been proposed as a driver of both AGN activity and the M-sigma relation, studies of moderate to high redshift Seyfert-luminosity AGN hosts have found little evidence for enhanced rates of interactions. However, both theo
Externí odkaz:
http://arxiv.org/abs/1712.02424
Autor:
Peters, S. P. C., van der Kruit, P. C., Knapen, J. H., Trujillo, I., Fliri, J., Cisternas, M., Kelvin, L. S.
We use data from the IAC Stripe82 Legacy Project to study the surface photometry of 22 nearby, face-on to moderately inclined spiral galaxies. The reprocessed and combined Stripe 82 $g'$, $r'$ and $i'$ images allow us to probe the galaxy down to 29-3
Externí odkaz:
http://arxiv.org/abs/1705.03555
Autor:
Mechtley, M., Jahnke, K., Windhorst, R. A., Andrae, R., Cisternas, M., Cohen, S. H., Hewlett, T., Koekemoer, A. M., Schramm, M., Schulze, A., Silverman, J. D., Villforth, C., van der Wel, A., Wisotzki, L.
Publikováno v:
ApJ (2016) 820, 2, 156
The most frequently proposed model for the origin of quasars holds that the high accretion rates seen in luminous active galactic nuclei are primarily triggered during major mergers between gas-rich galaxies. While plausible for decades, this model h
Externí odkaz:
http://arxiv.org/abs/1510.08461
Autor:
Tomás Icaran P., María Luz Rubio V., Dagoberto Ojeda D., Isabel Carranza L., Álvaro Jorquera S., Mariela Agurto V., Patricia Cisternas M.
Publikováno v:
Revista Chilena de Anestesia, Vol 49, Iss 6, Pp 874-881 (2020)
Externí odkaz:
https://doaj.org/article/247b75f1930d4d07b6f0eb6325863585
Autor:
Cisternas, M., Bhuyan, H., Retamal, M.J., Casanova-Morales, N., Favre, M., Volkmann, U.G., Saikia, P., Diaz-Droguett, D.E., Mändl, S., Manova, D., Moraga, N., Chandía-Cristi, A., Alvarez, A., Guzman, F.
Publikováno v:
In Materials Science & Engineering C August 2020 113
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:
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:
Elvis, M., Hao, H., Civano, F., Brusa, M., Salvato, M., Bongiorno, A., Capak, P., Zamorani, G., Comastri, A., Jahnke, K., Lusso, E., Mainieri, V., Trump, J. R., Ho, L. C., Aussel, H., Cappelluti, N., Cisternas, M., Frayer, D., Gilli, R., Hasinger, G., Huchra, J. P., Impey, C. D., Koekemoer, A. M., Lanzuisi, G., Floc'h, E. Le, Lilly, S. J., Liu, Y., McCarthy, P., McCracken, H. J., Merloni, A., Roeser, H. J., Sanders, D. B., Sargent, M., Scoville, N., Schinnerer, E., Schiminovich, D., Silverman, J., Taniguchi, Y., Vignali, C., Urry, C. M., Zamojski, M. A., Zatloukal, M.
The "Cosmic Evolution Survey" (COSMOS) enables the study of the Spectral Energy Distributions (SEDs) of Active Galactic Nuclei (AGN) because of the deep coverage and rich sampling of frequencies from X-ray to radio. Here we present a SED catalog of 4
Externí odkaz:
http://arxiv.org/abs/1209.1478
Autor:
Civano, F., Elvis, M., Brusa, M., Comastri, A., Salvato, M., Zamorani, G., Aldcroft, T., Bongiorno, A., Capak, P., Cappelluti, N., Cisternas, M., Fiore, F., Fruscione, A., Hao, H., Kartaltepe, J., Koekemoer, A., Gilli, R., Impey, C. D., Lanzuisi, G., Lusso, E., Mainieri, V., Miyaji, T., Lilly, S., Masters, D., Puccetti, S., Schawinski, K., Scoville, N. Z., Silverman, J., Trump, J., Urry, M., Vignali, C., Wright, N. J.
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central 0.9 deg^2 of the COSMOS field down to limiting depths of 1.9 10^-16 erg cm^-2 s-1 in the 0.5-2 keV band, 7.3 10^-16 erg cm^-2 s^-1 in the 2-10 keV ba
Externí odkaz:
http://arxiv.org/abs/1205.5030