- Nov 2022
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www.cs.ucr.edu www.cs.ucr.edu
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Dr. Miho Ohsaki re-examined workshe and her group had previously published and confirmed that the results are indeed meaningless in the sensedescribed in this work (Ohsaki et al., 2002). She has subsequently been able to redefine the clustering subroutine inher work to allow more meaningful pattern discovery (Ohsaki et al., 2003)
Look into what Dr. Miho Ohsaki changed about the clustering subroutine in her work and how it allowed for "more meaningful pattern discovery"
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- Nov 2021
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link.springer.com link.springer.com
- Oct 2021
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twitter.com twitter.com
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Pablo Tsukayama on Twitter. (n.d.). Twitter. Retrieved 4 October 2021, from https://twitter.com/pablotsukayama/status/1435725621599027202
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- Oct 2020
- Jun 2020
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twitter.com twitter.com
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van Smeden, M. (2020, May 26). "RT @MaartenvSmeden: Often more than 300 COVID-19 related scientific articles published per day Data from @evidencelive." Twitter. https://twitter.com/SciBeh/status/1265657595307667457
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OSF Coronavirus Outbreak Research Collection
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www.cos.io www.cos.io
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Science, C. for O. (2020 May 5). TOP Factor to appear in Master Journal List. https://www.cos.io/about/news/cos-and-the-web-of-science-collaborate-to-bring-top-factor-to-master-journal-list
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- Jun 2018
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iopscience.iop.org iopscience.iop.org
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Figure 9. Constraint plots
This is another example of a form of online data we support for our authors. In this case the 83 objects analyzed in this paper each had graphical representations of the model fits. All 83 elements can be viewed in the online journal via a filmstrip UI element. Readers can read individual captions for each element, download individual plots, or the entire set.
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Only a portion of this table is shown here to demonstrate its form and content. A machine-readable version of the full table is available.
This is an example of one of the Journal's machine readable tables. The reader clicks from the a shortened "example" version of the table inline to the main article to an ASCII text file that they can download and reuse. One of the Journal's data editors built this full ASCII text file from data provided by the author. This process includes standardizing formats, units and column explanations, which are all proofed by the author after the paper has been accepted.
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Our posterior samples are available online (10.5281/zenodo.162965).
This is an example of our current data linking markup. Data links are inline to the text through a parenthetical anchored link to the DOI resource.
There is a bug in the current version of the article. Our formal practice is to include this in the "Article Data" tab, which didn't happen this time. We will have to do some more work standardizing our production practices. We are also still thinking about how best to markup the anchored text.
We have not yet adopted a formal XML schema for including data links. We are working on this, which may be made easier when we adopt the most recent JATS schema.
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datacentral.aao.gov.au datacentral.aao.gov.auADC | S71
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S7 Data Release 2.0
The paper associated with this data release is now published: "Probing the Physics of Narrow-line Regions in Active Galaxies. IV. Full Data Release of the Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)", Thomas et al. (2017), ApJS, https://doi.org/10.3847/1538-4365/aa855a
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iopscience.iop.org iopscience.iop.org
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1- 13 A13 --- Planet Planet 15- 15 I1 --- robust Robust flag (1) 17- 23 F7.3 d Per Orbital period 25- 28 F4.1 Rgeo Rad Planet radius 30- 33 F4.2 Rgeo E_Rad 1{sigma} upper error bound on Rad 35- 38 F4.2 Rgeo e_Rad 1{sigma} lower error bound on Rad 40- 40 A1 --- r_Rad Source of planet-star radius ratio (2) 42- 44 F3.1 solMass Mstar Mass of host star 46- 49 F4.2 solMass E_Mstar 1{sigma} upper error bound on Mstar 51- 54 F4.2 solMass e_Mstar 1{sigma} lower error bound on Mstar 56- 56 I1 --- l_Md Md upper limit flag (3) 58- 63 F6.2 Mgeo Md Planet mass from default prior 65- 69 F5.2 Mgeo E_Md ?="" 1{sigma} upper error bound on Md 71- 74 F4.2 Mgeo e_Md ?="" 1{sigma} lower error bound on Md 76- 81 F6.2 g/cm3 rhod Planet density from default prior 83- 87 F5.2 g/cm3 E_rhod ?="" 1{sigma} upper error bound on rhod 89- 92 F4.2 g/cm3 e_rhod ?="" 1{sigma} lower error bound on rhod 94- 94 I1 --- l_Mh Mh upper limit flag (3) 96-100 F5.1 Mgeo Mh Planet mass from high mass prior 102-107 F6.2 Mgeo E_Mh ?="" 1{sigma} upper error bound on Md 109-112 F4.2 Mgeo e_Mh ?="" 1{sigma} lower error bound on Md 114-119 F6.2 g/cm3 rhoh Planet density from high mass prior 121-126 F6.2 g/cm3 E_rhoh ?="" 1{sigma} upper error bound on rhod 128-131 F4.2 g/cm3 e_rhoh ?="" 1{sigma} lower error bound on rhod 133-155 A23 --- Ref References (4)
This is the main header block of the AAS Journal's "Machine Readable Format" for structured tables. It is based on the CDS table format, and follows their structuring rules. There are columns for the numerical format, units, labels, and explanations for each column.
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- Aug 2017
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iopscience.iop.org iopscience.iop.org
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Figure 1. K2 light curve of HD 3167 from Vanderburg et al. (2016).
The data used in this figure came from a "Data behind the Figure" provided by Vanderburg et al. (2016), Figure 1.
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- Jun 2017
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iopscience.iop.org iopscience.iop.org
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#2016.1.01293.S
The data for this ALMA observation can be obtained at this dataset link: http://almascience.nrao.edu/aq/?project_code=2016.1.01293.S
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ADS/JAO.ALMA#2015.1.00504.S
The data for this ALMA observation can be obtained at this dataset link: http://almascience.nrao.edu/aq/?project_code=2015.1.00504.S
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