Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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693.932 PEOPLE
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Naji, M.
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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (4/4 displayed)

  • 2022Scaling K2. V. Statistical Validation of 60 New Exoplanets From K2 Campaigns 2-1822citations
  • 2022Scaling K2. V. Statistical Validation of 60 New Exoplanets From K2 Campaigns 2-18citations
  • 2022A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor member HIP 9423523citations
  • 2017Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS Parallaxes226citations

Places of action

Chart of shared publication
Bojsen-Hansen, Mathias
1 / 1 shared
Zinn, Joel
1 / 1 shared
Sahlholdt, Christian
1 / 1 shared
Bedding, Timothy R.
1 / 1 shared
Pinsonneault, Marc
1 / 1 shared
Bastien, Fabienne
1 / 1 shared
Chaplin, William J.
1 / 1 shared
Buchhave, Lars A.
1 / 1 shared
García, Rafael A.
1 / 1 shared
Davies, Guy R.
1 / 1 shared
Mathur, Savita
1 / 1 shared
Sharma, Sanjib
1 / 1 shared
Mosser, Benoit
1 / 1 shared
Huber, Daniel
1 / 8 shared
Tayar, Jamie
1 / 1 shared
Serenelli, Aldo
1 / 2 shared
Silva Aguirre, Victor
1 / 1 shared
Stassun, Keivan
1 / 2 shared
Stello, Dennis
1 / 1 shared
Chart of publication period
2022
2017

Co-Authors (by relevance)

  • Bojsen-Hansen, Mathias
  • Zinn, Joel
  • Sahlholdt, Christian
  • Bedding, Timothy R.
  • Pinsonneault, Marc
  • Bastien, Fabienne
  • Chaplin, William J.
  • Buchhave, Lars A.
  • García, Rafael A.
  • Davies, Guy R.
  • Mathur, Savita
  • Sharma, Sanjib
  • Mosser, Benoit
  • Huber, Daniel
  • Tayar, Jamie
  • Serenelli, Aldo
  • Silva Aguirre, Victor
  • Stassun, Keivan
  • Stello, Dennis
OrganizationsLocationPeople

article

Scaling K2. V. Statistical Validation of 60 New Exoplanets From K2 Campaigns 2-18

  • Berberyann, Arthur
  • Barclay, Thomas
  • Ziegler, Carl
  • Dunlavy, Ava
  • Calkins, Michael L.
  • Gilbert, Emily A.
  • Giacalone, Steven
  • Latham, David W.
  • Macqueen, Phillip J.
  • Dai, Fei
  • Ciardi, David R.
  • Hirsch, Lea A.
  • Dressing, Courtney D.
  • Tamura, Motohide
  • Weiss, Lauren M.
  • Gonzales, Erica J.
  • Isaacson, Howard
  • Adkins, Britt Duffy
  • Berlind, Perry
  • Morton, Timothy D.
  • Christiansen, Jessie L.
  • Zink, Jon K.
  • Crossfield, Ian J. M.
  • Allen, Bridgette E.
  • Matthews, Elisabeth C.
  • Esquerdo, Gilbert A.
  • Ciardi, Krys N.
  • Endl, Michael
  • Glassford, Sofia H.
  • Hirano, Teruyuki
  • Petigura, Erik A.
  • Beichman, Charles
  • Everett, Mark E.
  • Fulton, Benjamin J.
  • Bieryla, Allyson
  • Schlieder, Joshua E.
  • Livingston, John H.
  • Cochran, William D.
  • Howard, Andrew W.
  • Hardegree-Ullman, Kevin K.
  • Hedges, Christina
  • Bhure, Sakhee
Abstract

The NASA K2 mission, salvaged from the hardware failures of the Kepler telescope, has continued Kepler's planet-hunting success. It has revealed nearly 500 transiting planets around the ecliptic plane, many of which are the subject of further study, and over 1000 additional candidates. Here we present the results of an ongoing project to follow-up and statistically validate new K2 planets, in particular to identify promising new targets for further characterization. By analyzing the reconnaissance spectra, high-resolution imaging, centroid variations, and statistical likelihood of the signals of 91 candidates, we validate 60 new planets in 46 systems. These include a number of planets amenable to transmission spectroscopy (K2-384 f, K2-387 b, K2-390 b, K2-403 b, and K2-398 c), emission spectroscopy (K2-371 b, K2-370 b, and K2-399 b), and both (K2-405 b and K2-406 b); several systems with planets in or close to mean motion resonances (K2-381 and K2-398) including a compact, TRAPPIST-1-like system of five small planets orbiting a mid-M dwarf (K2-384); an ultra-short-period sub-Saturn in the hot Saturn desert (K2-399 b); and a super-Earth orbiting a moderately bright (V = 11.93), metal-poor ([Fe/H] = -0.579 ± 0.080) host star (K2-408 b). In total we validate planets around four F stars, 26 G stars, 13 K stars, and three M dwarfs. In addition, we provide a list of 37 vetted planet candidates that should be prioritized for future follow-up observation in order to be confirmed or validated....

Topics
  • spectroscopy