Zobrazeno 1 - 10
of 14 079
pro vyhledávání: '"McIntosh, D"'
Autor:
Mcintosh, D
Isotope analysis was present at the birth of mass spectrometry and has since found application in a diverse array of fields including biology, medicine, archaeology, geology, chronology, forensics and environmental science. Quadrupole mass spectromet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e63ca277b8c02b1b35ffd4e2b0f3e49
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:
Sánchez-Menguiano, L., Sánchez, S. F., Pérez, I., Debattista, V. P., Ruiz-Lara, T., Florido, E., Cavichia, O., Galbany, L., Marino, R. A., Mast, D., Sánchez-Blázquez, P., Méndez-Abreu, J., de Lorenzo-Cáceres, A., Catalán-Torrecilla, C., Cano-Díaz, M., Márquez, I., McIntosh, D. H., Ascasibar, Y., García-Benito, R., Delgado, R. M. Gónzalez, Kehrig, C., López-Sánchez, Á. R., Mollá, M., Bland-Hawthorn, J., Walcher, C. J., Costantin, L.
Publikováno v:
A&A 603, A113 (2017)
Spiral arms are the most singular features in disc galaxies. These structures can exhibit different patterns, namely grand design and flocculent arms, with easily distinguishable characteristics. However, their origin and the mechanisms shaping them
Externí odkaz:
http://arxiv.org/abs/1705.05733
Autor:
Vieta E; Hospital Clinic, Institute of Neuroscience, University of Barcelona, IDIBAPS, CIBERSAM, Barcelona, Spain., Tohen M; Department of Psychiatry and Behavioral Sciences, University of New Mexico Health Science Center, Albuquerque, New Mexico, USA., McIntosh D; Department of Psychiatry, University of British Columbia, Vancouver, British Columbia, Canada., Kessing LV; Copenhagen Affective Disorder Research Center (CADIC), Psychiatric Center Copenhagen, Frederiksberg, Copenhagen, Denmark.; Department of Clinical Medicine, Faculty of Health and Medical Sciences, University of Copenhagen, Copenhagen, Denmark., Sajatovic M; Department of Psychiatry, University Hospitals Cleveland Medical Center, Cleveland, Ohio, USA.; Department of Neurology, University Hospitals Cleveland Medical Center, Cleveland, Ohio, USA.; Neurological and Behavioral Outcomes Center, University Hospitals Cleveland Medical Center, Cleveland, Ohio, USA.; Case Western Reserve University School of Medicine, Cleveland, Ohio, USA., McIntyre RS; University of Toronto, Toronto, Ontario, Canada.; Brain and Cognition Discovery Foundation, Toronto, Ontario, Canada.
Publikováno v:
Bipolar disorders [Bipolar Disord] 2024 Oct 22. Date of Electronic Publication: 2024 Oct 22.
Autor:
Huertas-Company, M., Gravet, R., Cabrera-Vives, G., Pérez-González, P. G., Kartaltepe, J. S., Barro, G., Bernardi, M., Mei, S., Shankar, F., Dimauro, P., Bell, E. F., Kocevski, D., Koo, D. C., Faber, S. M., Mcintosh, D. H.
We present a catalog of visual like H-band morphologies of $\sim50.000$ galaxies ($H_{f160w}<24.5$) in the 5 CANDELS fields (GOODS-N, GOODS-S, UDS, EGS and COSMOS). Morphologies are estimated with Convolutional Neural Networks (ConvNets). The median
Externí odkaz:
http://arxiv.org/abs/1509.05429
Autor:
Barrera-Ballesteros, J. K., García-Lorenzo, B., Falcón-Barroso, J., van de Ven, G., Lyubenova, M., Wild, V., Méndez-Abreu, J., Sánchez, S. F., Marquez, I., Masegosa, J., Monreal-Ibero, A., Ziegler, B., del Olmo, A., Verdes-Montenegro, L., García-Benito, R., Husemann, B., Mast, D., Kehrig, C., Iglesias-Paramo, J., Marino, R. A., Aguerri, J. A. L., Walcher, C. J., Vílchez, J. M., Bomans, D. J., Cortijo-Ferrero, C., Delgado, R. M. González, Bland-Hawthorn, J., McIntosh, D. H., Bekeraite, Simona, Collaboration, the CALIFA
We present spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close companions, pairs with morphological signatures of interaction, and coalesced merger remnants. We
Externí odkaz:
http://arxiv.org/abs/1506.03819
The modern merger hypothesis offers a method of forming a new elliptical galaxy through merging two equal-mass, gas-rich disk galaxies fuelling a nuclear starburst followed by efficient quenching and dynamical stabilization. A key prediction of this
Externí odkaz:
http://arxiv.org/abs/1505.01493
Autor:
Del Moro, A., Alexander, D. M., Bauer, F. E., Daddi, E., Kocevski, D. D., McIntosh, D. H., Stanley, F., Brandt, W. N., Elbaz, D., Harrison, C. M., Luo, B., Mullaney, J. R., Xue, Y. Q.
We present the infrared (IR) and X-ray properties of a sample of 33 mid-IR luminous quasars ($\nu$L(6 micron)>6x10$^{44}$ erg/s) at redshift z~1-3, identified through detailed spectral energy distribution analyses of distant star-forming galaxies, us
Externí odkaz:
http://arxiv.org/abs/1504.03329
Autor:
Papovich, Casey, Labbé, I., Quadri, R., Tilvi, V., Behroozi, P., Bell, E. F., Glazebrook, K., Spitler, L., Straatman, C. M. S., Tran, K. -V., Cowley, M., Davé, R., Dekel, A., Dickinson, M., Ferguson, H., Finkelstein, S. L., Gawiser, E., Inami, H., Faber, S. M., Kacprzak, G. G., Kawinwanchakij, L., Kocevski, D., Koekemoer, A., Koo, D. C., Kurczynski, P., Lotz, J. M., Lu, Y., Lucas, R. A., McIntosh, D., Mehrtens, N., Mobasher, B., Monson, A., Morrison, G., Nanayakkara, T., Perrson, S. E., Salmon, B., Simons, R., Tomczak, A., van Dokkum, P., Weiner, B., Willner, S. P.
Galaxies with stellar masses near M* contain the majority of stellar mass in the universe, and are therefore of special interest in the study of galaxy evolution. The Milky Way (MW) and Andromeda (M31) have present day stellar masses near M*, at 5x10
Externí odkaz:
http://arxiv.org/abs/1412.3806
Autor:
Rosario, D. J., McIntosh, D. H., van der Wel, A., Kartaltepe, J., Lang, P., Santini, P., Wuyts, S., Lutz, D., Rafelski, M., Villforth, C., Alexander, D. M., Bauer, F. E., Bell, E. F., Berta, S., Brandt, W. N., Conselice, C. J., Dekel, A., Faber, S. M., Ferguson, H. C., Genzel, R., Grogin, N. A., Kocevski, D. D., Koekemoer, A. M., Koo, D. C., Lotz, J. M., Magnelli, B., Maiolino, R., Mozena, M., Mullaney, J. R., Papovich, C. J., Popesso, P., Tacconi, L. J., Trump, J. R., Avadhuta, S., Bassett, R., Bell, A., Bernyk, M., Bournaud, F., Cassata, P., Cheung, E., Croton, D., Donley, J., DeGroot, L., Guedes, J., Hathi, N., Herrington, J., Hilton, M., Lai, K., Lani, C., Martig, M., McGrath, E., Mutch, S., Mortlock, A., McPartland, C., O'Leary, E., Peth, M., Pillepich, A., Poole, G., Snyder, D., Straughn, A., Telford, O., Tonini, C., Wandro, P.
Publikováno v:
A&A 573, A85 (2015)
We study the relationship between the structure and star-formation rate (SFR) of X-ray selected low and moderate luminosity active galactic nuclei (AGNs) in the two Chandra Deep Fields, using Hubble Space Telescope imaging from the Cosmic Assembly Ne
Externí odkaz:
http://arxiv.org/abs/1409.5122