Zobrazeno 1 - 10
of 168
pro vyhledávání: '"Momcheva, I."'
Autor:
Chary, R., Helou, G., Brammer, G., Capak, P., Faisst, A., Flynn, D., Groom, S., Ferguson, H. C., Grillmair, C., Hemmati, S., Koekemoer, A., Lee, B., Malhotra, S., Miyatake, H., Melchior, P., Momcheva, I., Newman, J., Masiero, J., Paladini, R., Prakash, A., Rusholme, B., Stickley, N. R., Smith, A., Wood-Vasey, W. M., Teplitz, H. I.
The Euclid, Rubin/LSST and Roman (WFIRST) projects will undertake flagship optical/near-infrared surveys in the next decade. By mapping thousands of square degrees of sky and covering the electromagnetic spectrum between 0.3 and 2 microns with sub-ar
Externí odkaz:
http://arxiv.org/abs/2008.10663
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:
Chary, R., Brammer, G., Capak, P., Dawson, W., Faisst, A., Fajardo-Acosta, S., Ferguson, H. C., Grillmair, C. J., Hemmati, S., Koekemoer, A., Lee, B., Lupton, R., Malhotra, S., Melchior, P., Momcheva, I., Newman, J., Masiero, J., Paladini, R., Prakash, A., Rhodes, J., Rusholme, B., Schneider, M., Stickley, N., Smith, A., Wood-Vasey, W. M., Berriman, G. B.
Joint survey processing (JSP) is the pixel level combination of LSST, Euclid, and WFIRST datasets. By combining the high spatial resolution of the space-based datasets with deep, seeing-limited, ground-based images in the optical bands, systematics l
Externí odkaz:
http://arxiv.org/abs/1910.01259
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:
Hviding, R. E., Brammer, G. B., Momcheva, I. G., Lundgren, B. F., Marchesini, D., Pirzkal, N., Ryan, R. E., Vang, A., Wake, D. A., Bourque, M., Martlin, C., Nedkova, K. V.
We present spatially resolved emission diagnostics for eight $z\sim0.9$ galaxies that demonstrate extended low ionization emission-line regions (LIERs) over kpc scales. Eight candidates are selected based on their spatial extent and emission line flu
Externí odkaz:
http://arxiv.org/abs/1810.02819
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:
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
Autor:
Übler, H., Schreiber, N. M. Förster, Genzel, R., Wisnioski, E., Wuyts, S., Lang, P., Naab, T., Burkert, A., Tacconi, L. J., Wilman, D. J., Fossati, M., Mendel, J. T., Beifiori, A., Belli, S., Bender, R., Brammer, G., Chan, J., Davies, R., Fabricius, M., Galametz, A., Lutz, D., Momcheva, I., Nelson, E. J., Saglia, R. P., Seitz, S., Tadaki, K., van Dokkum, P. G.
We investigate the stellar mass and baryonic mass Tully-Fisher relations (TFRs) of massive star-forming disk galaxies at redshift z~2.3 and z~0.9 as part of the KMOS^3D integral field spectroscopy survey. Our spatially resolved data allow reliable mo
Externí odkaz:
http://arxiv.org/abs/1703.04321