Zobrazeno 1 - 10
of 61
pro vyhledávání: '"Mendel, J. T."'
Autor:
Koller, M., Ziegler, B., Ciocan, B. I., Thater, S., Mendel, J. T., Wisnioski, E., Battisti, A. J., Harborne, K. E., Foster, C., Lagos, C., Croom, S. M., Grasha, K., Papaderos, P., Remus, R. S., Sharma, G., Sweet, S. M., Valenzuela, L. M., van de Ven, G., Zafar, T.
Star formation rates (SFRs), gas-phase metallicities, and stellar masses are crucial for studying galaxy evolution. The different relations resulting from these properties give insights into the complex interplay of gas inside galaxies and their evol
Externí odkaz:
http://arxiv.org/abs/2406.20017
Autor:
Davies, Rebecca L., Schreiber, N. M. Förster, Genzel, R., Shimizu, T. T., Davies, R. I., Schruba, A., Tacconi, L. J., Übler, H., Wisnioski, E., Wuyts, S., Fossati, M., Herrera-Camus, R., Lutz, D., Mendel, J. T., Naab, T., Price, S. H., Renzini, A., Wilman, D., Beifiori, A., Belli, S., Burkert, A., Chan, J., Contursi, A., Fabricius, M., Lee, M. M., Saglia, R. P., Sternberg, A.
We investigate what drives the redshift evolution of the typical electron density ($n_e$) in star-forming galaxies, using a sample of 140 galaxies drawn primarily from KMOS$^{\rm 3D}$ ($0.6\lesssim{z}\lesssim{2.6}$) and 471 galaxies from SAMI ($z<0.1
Externí odkaz:
http://arxiv.org/abs/2012.10445
Autor:
Foster, C., Mendel, J. T., Lagos, C. D. P., Wisnioski, E., Yuan, T., D'Eugenio, F., Barone, T. M., Harborne, K. E., Vaughan, S. P., Schulze, F., Remus, R. -S., Gupta, A., Collacchioni, F., Khim, D. J., Taylor, P., Bassett, R., Croom, S. M., McDermid, R. M., Poci, A., Battisti, A. J., Bland-Hawthorn, J., Bellstedt, S., Colless, M., Davies, L. J. M., Derkenne, C., Driver, S., Ferré-Mateu, A., Fisher, D. B., Gjergo, E., Johnston, E. J., Khalid, A., Kobayashi, C., Oh, S., Peng, Y., Robotham, A. S. G., Sharda, P., Sweet, S. M., Taylor, E. N., Tran, K. -V. H., Trayford, J. W., van de Sande, J., Yi, S. K., Zanisi, L.
We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during wh
Externí odkaz:
http://arxiv.org/abs/2011.13567
Autor:
Wilman, D. J., Fossati, M., Mendel, J. T., Saglia, R., Wisnioski, E., Wuyts, S., Schreiber, N. Förster, Beifiori, A., Bender, R., Belli, S., Übler, H., Lang, P., Chan, J. C. C., Davies, R. L., Nelson, E. J., Genzel, R., Tacconi, L. J., Galametz, A., Davies, R. I., Lutz, D., Price, S., Burkert, A., Tadaki, K., Herrera-Camus, R., Brammer, G., Momcheva, I., van Dokkum, P.
We present half-light sizes measured from H${\alpha}$ emission tracing star-formation in 281 star-forming galaxies from the KMOS3D survey at 0.7 < z < 2.7. Sizes are derived by fitting 2D exponential disk models, with bootstrap errors averaging 20%.
Externí odkaz:
http://arxiv.org/abs/2002.09499
Autor:
Wisnioski, E., Schreiber, N. M. Förster, Fossati, M., Mendel, J. T., Wilman, D., Genzel, R., Bender, R., Wuyts, S., Davies, R. L., Übler, H., Bandara, K., Beifiori, A., Belli, S., Brammer, G., Chan, J., Davies, R. I., Fabricius, M., Galametz, A., Lang, P., Lutz, D., Nelson, E. J., Momcheva, I., Price, S., Rosario, D., Saglia, R., Seitz, S., Shimizu, T., Tacconi, L. J., Tadaki, K., van Dokkum, P. G., Wuyts, E.
We present the completed KMOS$^\mathrm{3D}$ survey $-$ an integral field spectroscopic survey of 739, $\log(M_{\star}/M_{\odot})>9$, galaxies at $0.6
Externí odkaz:
http://arxiv.org/abs/1909.11096
Autor:
Schreiber, N. M. Förster, Übler, H., Davies, R. L., Genzel, R., Wisnioski, E., Belli, S., Shimizu, T., Lutz, D., Fossati, M., Herrera-Camus, R., Mendel, J. T., Tacconi, L. J., Wilman, D., Beifiori, A., Brammer, G., Burkert, A., Carollo, C. M., Davies, R. I., Eisenhauer, F., Fabricius, M., Lilly, S. J., Momcheva, I., Naab, T., Nelson, E. J., Price, S., Renzini, A., Saglia, R., Sternberg, A., van Dokkum, P., Wuyts, S.
We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6
Externí odkaz:
http://arxiv.org/abs/1807.04738
Autor:
Fossati, M., Mendel, J. T., Boselli, A., Cuillandre, J. C., Vollmer, B., Boissier, S., Consolandi, G., Ferrarese, L., Gwyn, S., Amram, P., Boquien, M., Buat, V., Burgarella, D., Cortese, L., Cote, P., Cote, S., Durrell, P., Fumagalli, M., Gavazzi, G., Gomez-Lopez, J., Hensler, G., Koribalski, B., Longobardi, A., Peng, E. W., Roediger, J., Sun, M., Toloba, E.
Publikováno v:
A&A 614, A57 (2018)
The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-band H$\alpha$+[NII] imaging survey carried out with MegaCam at the CFHT. During pilot observations we have observed NGC 4330, an intermediate mass, edge-on star
Externí odkaz:
http://arxiv.org/abs/1801.09685
Autor:
Wisnioski, E., Mendel, J. T., Schreiber, N. M. Förster, Genzel, R., Wilman, D., Wuyts, S., Belli, S., Beifiori, A., Bender, R., Brammer, G., Chan, J., Davies, R. I., Davies, R. L., Fabricius, M., Fossati, M., Galametz, A., Lang, P., Lutz, D., Nelson, E. J., Momcheva, I., Rosario, D., Saglia, R., Tacconi, L. J., Tadaki, K., Übler, H., van Dokkum, P. G.
Using integral field spectroscopy we investigate the kinematic properties of 35 massive centrally-dense and compact star-forming galaxies (${\log{\overline{M}_*}}=11.1$, $\log{(\Sigma_\mathrm{1kpc})}>9.5$, $\log{(M_\ast/r_e^{1.5})}>10.3$) at $z\sim0.
Externí odkaz:
http://arxiv.org/abs/1711.02111
Autor:
Lang, P., Schreiber, N. M. Förster, Genzel, R., Wuyts, S., Wisnioski, E., Beifiori, A., Belli, S., Bender, R., Brammer, G., Burkert, A., Chan, J., Davies, R., Fossati, M., Galametz, A., Kulkarni, S. K., Lutz, D., Mendel, J. T., Momcheva, I. G., Naab, T., Nelson, E. J., Saglia, R. P., Seitz, S., Tacchella, S., Tacconi, L. J., Tadaki, K., Übler, H., van Dokkum, P. G., Wilman, D. J.
We exploit the deep resolved Halpha kinematic data from the KMOS^3D and SINS/zC-SINF surveys to examine the largely unexplored outer disk kinematics of star-forming galaxies (SFGs) out to the peak of cosmic star formation. Our sample contains 101 SFG
Externí odkaz:
http://arxiv.org/abs/1703.05491
Autor:
Genzel, R., Schreiber, N. M. Förster, Übler, H., Lang, P., Naab, T., Bender, R., Tacconi, L. J., Wisnioski, E., Wuyts, S., Alexander, T., Beifiori, A., Belli, S., Brammer, G., Burkert, A., Carollo, C. M., Chan, J., Davies, R., Fossati, M., Galametz, A., Genel, S., Gerhard, O., Lutz, D., Mendel, J. T., Momcheva, I., Nelson, E. J., Renzini, A., Saglia, R., Sternberg, A., Tacchella, S., Tadaki, K., Wilman, D.
In cold dark matter cosmology, the baryonic components of galaxies are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter, which dominates the total mass of the galaxy and its dark matter halo. In the local Univers
Externí odkaz:
http://arxiv.org/abs/1703.04310