Zobrazeno 1 - 10
of 651
pro vyhledávání: '"Teague, R"'
Autor:
Rampinelli, L., Facchini, S., Leemker, M., Bae, J., Benisty, M., Teague, R., Law, C. J., Öberg, K. I., Portilla-Revelo, B., Cridland, A. J.
Publikováno v:
A&A 689, A65 (2024)
With two directly detected protoplanets, the PDS 70 system is a unique source in which to study the complex interplay between forming planets and their natal environment. The large dust cavity carved by the two giant planets can affect the disk chemi
Externí odkaz:
http://arxiv.org/abs/2407.06272
This paper introduced a clustered estimator of the Network Information Criterion (NICc) to approximate leave-one-cluster-out cross-validated deviance, which can be used as an alternative to cluster-based cross-validation when modeling clustered data.
Externí odkaz:
http://arxiv.org/abs/2405.20400
Autor:
Paneque-Carreño, T., Izquierdo, A. F., Teague, R., Miotello, A., Bergin, E. A., Loomis, R., van Dishoeck, E. F.
Constraining turbulence in disks is key towards understanding their evolution through the transport of angular momentum. Until now measurements of high turbulence have remained elusive and methods for estimating turbulence relay mostly on complex rad
Externí odkaz:
http://arxiv.org/abs/2312.04618
Autor:
Portilla-Revelo, B., Kamp, I., Facchini, S., van Dishoeck, E. F., Law, C., Rab, Ch., Bae, J., Benisty, M., Öberg, K., Teague, R.
Publikováno v:
A&A 677, A76 (2023)
Embedded planets are potentially the cause of substructures like gaps and cavities observed in several protoplanetary disks. Thus, the substructures observed in the continuum and in line emission encode information about the presence of planets in th
Externí odkaz:
http://arxiv.org/abs/2306.16850
Intensive longitudinal (IL) data are increasingly prevalent in psychological science, coinciding with technological advancements that make it simple to deploy study designs such as daily diary and ecological momentary assessments. IL data are charact
Externí odkaz:
http://arxiv.org/abs/2305.13444
Autor:
Slipetz, Lindley R., Eberle, Jeremy W., Levinson, Cheri A., Falk, Ami, Cusack, Claire E., Henry, Teague R.
Ecological momentary assessment (EMA) data have a broad base of application in the study of time trends and relations. In EMA studies, there are a number of design considerations which influence the analysis of the data. One general modeling framewor
Externí odkaz:
http://arxiv.org/abs/2305.03214
When using ecological momentary assessment data (EMA), missing data is pervasive as participant attrition is a common issue. Thus, any EMA study must have a missing data plan. In this paper, we discuss missingness in time series analysis and the appr
Externí odkaz:
http://arxiv.org/abs/2301.13144
Autor:
Bohn, A. J., Benisty, M., Perraut, K., van der Marel, N., Wölfer, L., van Dishoeck, E. F., Facchini, S., Manara, C. F., Teague, R., Francis, L., Berger, J-P., Garcia-Lopez, R., Ginski, C., Henning, T., Kenworthy, M., Kraus, S., Ménard, F., Mérand, A., Pérez, L. M.
Publikováno v:
A&A 658, A183 (2022)
For several transition disks (TDs), dark regions interpreted as shadows have been observed in scattered light imaging and are hypothesized to originate from misalignments between distinct disk regions. We aim to investigate the presence of misalignme
Externí odkaz:
http://arxiv.org/abs/2112.00123
Autor:
Boehler, Y., Ménard, F., Robert, C. M. T., Isella, A., Pinte, C., Gonzalez, J. -F., van der Plas, G., Weaver, E., Teague, R., Garg, H., Méheut, H.
Publikováno v:
A&A 650, A59 (2021)
Vortices are one of the most promising mechanisms to locally concentrate millimeter dust grains and allow the formation of planetesimals through gravitational collapse. The outer disk around the binary system HD 142527 is known for its large horsesho
Externí odkaz:
http://arxiv.org/abs/2103.13474
Autor:
Podio, L., Garufi, A., Codella, C., Fedele, D., Rygl, K., Favre, C., Bacciotti, F., Bianchi, E., Ceccarelli, C., Mercimek, S., Teague, R., Testi, L.
Publikováno v:
A&A 644, A119 (2020)
Planets form in protoplanetary disks and inherit their chemical composition. It is therefore crucial to understand the disks molecular content. We aim to characterize the distribution and abundance of molecules in the disk of DG Tau. In the context o
Externí odkaz:
http://arxiv.org/abs/2011.01081