Zobrazeno 1 - 10
of 230
pro vyhledávání: '"N. Förster"'
Publikováno v:
Journal of Applied Botany and Food Quality, Vol 82, Iss 1 (2012)
Due to the benefits of herbal medicine and their wide range of application for human health, the usage of natural drug products, such as willow bark extract, has increased in the last few years. The principle active compounds of the drugs comprised p
Externí odkaz:
https://doaj.org/article/beeb67c0dd254bb3a303460960e750a3
Autor:
Henríquez-Brocal, K., Herrera-Camus, R., Tacconi, L., Genzel, R., Bolatto, A., Bovino, S., Demarco, R., Schreiber, N. Förster, Lee, M., Lutz, D., Rubio, M.
We use a combination of new NOrthern Extended Millimeter Array (NOEMA) observations of the pair of [CI] transitions, the CO(7-6) line, and the dust continuum, in addition to ancillary CO(1-0) and CO(3-2) data, to study the molecular gas properties of
Externí odkaz:
http://arxiv.org/abs/2109.01684
Autor:
Herrera-Camus, R., Schreiber, N. Förster, Genzel, R., Tacconi, L., Bolatto, A., Davies, R. L., Fisher, D., Lutz, D., Naab, T., Shimizu, T., Tadaki, K., Übler, H.
Publikováno v:
A&A 649, A31 (2021)
We present new Atacama Large Millimeter/Submillimeter Array (ALMA) observations of the [CII] 158 $\mu$m transition and the dust continuum in HZ4, a typical star-forming galaxy when the Universe was only $\sim1$ Gyr old ($z\approx5.5$). Our high $\app
Externí odkaz:
http://arxiv.org/abs/2101.05279
Autor:
Wilman, D. J., Fossati, M., Mendel, J. T., Saglia, R., Wisnioski, E., Wuyts, S., Schreiber, N. Förster, Beifiori, A., Bender, R., Belli, S., Übler, H., Lang, P., Chan, J. C. C., Davies, R. L., Nelson, E. J., Genzel, R., Tacconi, L. J., Galametz, A., Davies, R. I., Lutz, D., Price, S., Burkert, A., Tadaki, K., Herrera-Camus, R., Brammer, G., Momcheva, I., van Dokkum, P.
We present half-light sizes measured from H${\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:
Davies, R., Schubert, J., Hartl, M., Alves, J., Clénet, Y., Lang-Bardl, F., Nicklas, H., Pott, J. -U., Ragazzoni, R., Tolstoy, E., Agocs, T., Anwand-Heerwart, H., Barboza, S., Baudoz, P., Bender, R., Bizenberger, P., Boccaletti, A., Boland, W., Bonifacio, P., Briegel, F., Buey, T., Chapron, F., Cohen, M., Czoske, O., Dreizler, S., Falomo, R., Feautrier, P., Schreiber, N. Förster, Gendron, E., Genzel, R., Glück, M., Gratadour, D., Greimel, R., Grupp, F., Häuser, M., Haug, M., Hennawi, J., Hess, H. -J., Hörmann, V., Hofferbert, R., Hopp, U., Hubert, Z., Ives, D., Kausch, W., Kerber, F., Kravcar, H., Kuijken, K., Leitzinger, M., Leschinski, K., Massari, D., Mei, S., Merlin, F., Mohr, L., Monna, A., Müller, F., Navarro, R., Plattner, M., Przybilla, N., Ramlau, R., Ramsay, S., Ratzka, T., Rhode, P., Richter, J., Rix, H. -W., Rodeghiero, G., Rohloff, R. -R., Rousset, G., Ruddenklau, R., Schaffenroth, V., Schlichter, J., Sevin, A., Stuik, R., Sturm, E., Thomas, J., Tromp, N., Turatto, M., Verdoes-Kleijn, G., Vidal, F., Wagner, R., Wegner, M., Zeilinger, W., Ziegler, B., Zins, G.
MICADO will equip the E-ELT with a first light capability for diffraction limited imaging at near-infrared wavelengths. The instrument's observing modes focus on various flavours of imaging, including astrometric, high contrast, and time resolved. Th
Externí odkaz:
http://arxiv.org/abs/1607.01954
Autor:
Oteo, I., Magdis, G., Bongiovanni, Á., Pérez-García, A. M., Cepa, J., Cedrés, B., Ederoclite, A., Sánchez-Portal, M., Aguerri, J. A. L., Alfaro, E. J., Altieri, B., Andreani, P., Aparicio-Villegas, T., Aussel, H., Benítez, N., Berta, S., Broadhurst, T., Cabrera-Caño, J., Castander, F. J., Cerviño, M., Cimatti, A., Cristobal-Hornillos, D., Daddi, E., Elbaz, D., Fernandez-Soto, A., Schreiber, N. Förster, Genzel, R., Gonzalez-Delgado, R. M., Husillos, C., Infante, L., Floc'h, E. Le, Lutz, D., Magnelli, B., Maiolino, R., Márquez, I., Martínez, V. J., Masegosa, J., Matute, I., Moles, M., Molino, A., del Olmo, A., Perea, J., Pérez-Martínez, R., Pintos-Castro, I., Poglitsch, A., Polednikova, J., Popesso, P., Pović, M., Pozzi, F., Prada, F., Quintana, J. M., Riguccini, L., Sturm, E., Tacconi, L., Valtchanov, I., Viironen, K.
We report the PACS-100um/160um detections of a sample of 42 GALEX-selected and FIR-detected Lyman break galaxies (LBGs) at z ~ 1 located in the COSMOS field and analyze their ultra-violet (UV) to far-infrared (FIR) properties. The detection of these
Externí odkaz:
http://arxiv.org/abs/1306.1121
Autor:
Oteo, I., Bongiovanni, A., García, A. M. Pérez, Cepa, J., Ederoclite, A., Sánchez-Portal, M., Pintos-Castro, I., Pérez-Martínez, R., Lutz, D., Altieri, B., Andreani, P., Aussel, H., Berta, S., Cimatti, A., Daddi, E., Elbaz, D., Schreiber, N. Förster, Genzel, R., Floc'h, E. Le, Magnelli, B., Maiolino, R., Poglitsch, A., Popesso, P., Pozzi, F., Riguccini, L., Sturm, E., Tacconi, L., Valtchanov, I.
The analysis of the physical properties of low-redshift Ly$\alpha$ emitters (LAEs) can provide clues in the study of their high-redshift analogues. At $z \sim 0.3$, LAEs are bright enough to be detected over almost the entire electromagnetic spectrum
Externí odkaz:
http://arxiv.org/abs/1204.0782
Autor:
Oteo, I., Bongiovanni, A., García, A. M. Pérez, Cepa, J., Ederoclite, A., Sánchez-Portal, M., Pintos-Castro, I., Pérez-Martínez, R., Altieri, B., Andreani, P., Aussel, H., Berta, S., Cimatti, A., Daddi, E., Elbaz, D., Schreiber, N. Förster, Genzel, R., Lutz, D., Magnelli, B., Maiolino, R., Poglitsch, A., Popesso, P., Pozzi, F., Sturm, E., Tacconi, L., Valtchanov, I.
In this work we analyze the physical properties of a sample of 56 spectroscopically selected star-forming (SF) Ly$\alpha$ emitting galaxies at 2.0$\lesssim$z$\lesssim$3.5 using both a spectral energy distribution (SED) fitting procedure from rest-fra
Externí odkaz:
http://arxiv.org/abs/1202.0997
Autor:
Popesso, P., Biviano, A., Rodighiero, G., Baronchelli, I., Salvato, M., Saintonge, A., Finoguenov, A., Magnelli, B., Gruppioni, C., Pozzi, F., Lutz, D., Elbaz, D., Altieri, B., Andreani, P., Aussel, H., Berta, S., Capak, P., Cava, A., Cimatti, A., Coia, D., Daddi, E., Dannerbauer, H., Dickinson, M., Dasyra, K., Fadda, D., Schreiber, N. Förster, Genzel, R., Hwang, H. S., Kartaltepe, J., Ilbert, O., Floch, E. Le, Leiton, R., Magdis, G., Nordon, R., Patel, S., Poglitsch, A., Riguccini, L., Portal, M. Sanchez, Shao, L., Tacconi, L., Tomczak, A., Tran, K., Valtchanov, I.
Star formation in massive galaxies is quenched at some point during hierarchical mass assembly. To understand where and when the quenching processes takes place, we study the evolution of the total star formation rate per unit total halo mass (\Sigma
Externí odkaz:
http://arxiv.org/abs/1110.2946
Autor:
Oteo, I., Bongiovanni, A., García, A. M. Pérez, Cepa, J., Ederoclite, A., Sánchez-Portal, M., Pintos-Castro, I., Lutz, D., Berta, S., Floc'h, E. Le, Magnelli, B., Popesso, P., Pozzi, F., Riguccini, L., Altieri, B., Andreani, P., Aussel, H., Cimatti, A., Daddi, E., Elbaz, D., Schreiber, N. Förster, Genzel, R., Maiolino, R., Poglitsch, A., Sturm, E., Tacconi, L., Valtchanov, I.
One remaining open question regarding the physical properties of Ly$\alpha$ emitters (LAEs) is their dust content and its evolution with redshift. The variety of results is large and with those reported by now is difficult to establish clear relation
Externí odkaz:
http://arxiv.org/abs/1108.3122