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pro vyhledávání: '"Lutz, K A"'
Modelling epidemics via classical population-based models suffers from shortcomings that so-called individual-based models are able to overcome, as they are able to take heterogeneity features into account, such as super-spreaders, and describe the d
Externí odkaz:
http://arxiv.org/abs/2205.06539
Autor:
Pothuri, B., Sawaged, Z., Karpel, H.C., Li, X., Lee, J., Musa, F., Lutz, K., Reese, E., Blank, S.V., Boyd, L.R., Curtin, J.P., Goldberg, J.D., Muggia, F.M.
Publikováno v:
In Gynecologic Oncology November 2024 190:209-214
Autor:
Lutz, K. A., Saintonge, A., Catinella, B., Cortese, L., Eisenhauer, F., Kramer, C., Moran, S. M., Tacconi, L. J., Vollmer, B., Wang, J.
Publikováno v:
A&A 649, A39 (2021)
Context. The xGASS and xCOLD GASS surveys have measured the atomic (HI) and molecular gas (H2) content of a large and representative sample of nearby galaxies (redshift range of 0.01 $\lt$ z $\lt$ 0.05). Aims. We present optical longslit spectra for
Externí odkaz:
http://arxiv.org/abs/2102.09909
With SKA precursor and pathfinder operations in full swing, radio and (sub-)mm astronomy is entering the era of super big data. The big questions is how to make (sub-)mm and radio data available to the astronomical community, preferably using FAIR (f
Externí odkaz:
http://arxiv.org/abs/2012.11907
Publikováno v:
A&A 635, A69 (2020)
This paper presents the analysis of optical integral field spectra for the HI eXtreme (HIX) galaxy sample. HIX galaxies host at least 2.5 times more atomic gas (HI) than expected from their optical R-band luminosity. Previous examination of their sta
Externí odkaz:
http://arxiv.org/abs/2001.07516
Autor:
Lutz, K. A., Kilborn, V. A., Koribalski, B. S., Catinella, B., Józsa, G. I. G., Wong, O. I., Stevens, A. R. H., Obreschkow, D., Dénes, H.
Publikováno v:
MNRAS 476 (2018) 3744
By analysing a sample of galaxies selected from the HI Parkes All Sky Survey (HIPASS) to contain more than 2.5 times their expected HI content based on their optical properties, we investigate what drives these HI eXtreme (HIX) galaxies to be so HI-r
Externí odkaz:
http://arxiv.org/abs/1802.04043
Autor:
Accurso, G., Saintonge, A., Catinella, B., Cortese, L., Dave, R., Dunsheath, S. H., Genzel, R., Gracia-Carpio, J., Heckman, T. M., Jimmy, Kramer, C., Li, Cheng, Lutz, K., Schiminovich, D., Schuster, K., Sternberg, A., Sturm, E., Tacconi, L. J., Tran, K. V., Wang, J.
We present Herschel PACS observations of the [CII] 158 micron emission line in a sample of 24 intermediate mass (9
Externí odkaz:
http://arxiv.org/abs/1702.03888
Autor:
Lutz, K. A., Kilborn, V. A., Catinella, B., Koribalski, B. S., Brown, T. H., Cortese, L., Dénes, H., Józsa, G. I. G., Wong, O. I.
We present the HI eXtreme (HIX) galaxy survey targeting some of the most HI rich galaxies in the southern hemisphere. The 13 HIX galaxies have been selected to host the most massive HI discs at a given stellar luminosity. We compare these galaxies to
Externí odkaz:
http://arxiv.org/abs/1701.02447
Autor:
Saintonge, A., Catinella, B., Cortese, L., Genzel, R., Giovanelli, R., Haynes, M. P., Janowiecki, S., Kramer, C., Lutz, K. A., Schiminovich, D., Tacconi, L. J., Wuyts, S., Accurso, G.
We use spectra from the ALFALFA, GASS and COLD GASS surveys to quantify variations in the mean atomic and molecular gas mass fractions throughout the SFR-M* plane and along the main sequence (MS) of star-forming galaxies. Although galaxies well below
Externí odkaz:
http://arxiv.org/abs/1607.05289
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