such as DOIs, which might be assigned by, for example, “crossref” or “figshare”

statsmodels11packag

Figure 9. Constraint plots

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.

Our posterior samples are available online (10.5281/zenodo.162965).

S7 Data Release 2.0

Acero F., Ackermann M., Ajello M. et al (Fermi-LAT) 2015 arXiv:1501.02003Preprint

The most up-to-date version of the open-source package NPTFit may be found at https://github.com/bsafdi/NPTFit and the latest documentation at http://nptfit.readthedocs.io. In addition, the version used in this paper has been archived at https://zenodo.org/record/380469#.WN_pSFPyvMV.

Foreman-Mackey D., Vousden W., Price-Whelan A. et al 2016 corner.py: corner.py v2.0.0, doi:10.5281/zenodo.53155

Barbary K. 2014 sncosmo Zenodo, 10.5281/zenodo.11938

https://doi.org/10.5281/zenodo.11938

The catalog of fakes used to generate the efficiency grids in Section 3 are available in a persistent directory: doi:10.5258/SOTON/D0030.

Software: hotpants, PostgreSQL, realbogus (Bloom et al. 2012) scamp (Bertin 2006), sextractor (Bertin & Arnouts 1996), sncosmo (Barbary 2014), swarp (Bertin et al. 2002), matplotlib (Hunter 2007), numpy (Van Der Walt et al. 2011).

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)

WISE J085510.83−071442.5

Software: Juypter notebook (http://jupyter.org), Jupyterlab (https://github.com/jupyterlab), VOspace (http://www.canfar.net/en/docs/storage), vos (https://pypi.python.org/pypi/vos), VirtualBox (https://www.virtualbox.org), JupyterHub      (https://jupyterhub.readthedocs.io/en/latest/), ipywidgets (https://ipywidgets.readthedocs.io), NuPyCEE (http://nugrid.github.io/NuPyCEE), NuGridSetExplorer (https://github.com/NuGrid/WENDI), hdf5 (https://www.hdfgroup.org), Cyberlaboratories cyberhubs (https://github.com/cyberlaboratories/cyberhubs), Cyberlaboratories astrohubs        (https://github.com/cyberlaboratories/astrohubs), Cyberhubs Docker repository (https://hub.docker.com/u/cyberhubs), Docker (https://www.docker.com), NOAO data lab (http://datalab.noao.edu), ansible (https://www.ansible.com), puppet (https://puppet.com), mesa_h5 (https://github.com/NuGrid/mesa_h5), Python (https://www.python.org), MESA (http://mesa.sourceforge.net), WENDI (http://wendi.nugridstars.org), OpenMP (http://www.openmp.org), MESA-SDK (http://www.astro.wisc.edu/~townsend/static.php?ref=mesasdk), MPI (https://www.open-mpi.org), gfortran (https://gcc.gnu.org/fortran), SuperLU (http://crd-legacy.lbl.gov/~xiaoye/SuperLU), OpenBLAS (http://www.openblas.net), mencoder (http://www.mplayerhq.hu).

Let’s use some common units as examples: gram (g), erg (erg), and solar mass per cubic megaparsec (Msun / Mpc33^3). g is an atomic, CGS base unit, erg is an atomic unit in CGS, but is not a base unit, and Msun/Mpc33^3 is a combination of atomic units, which are not in CGS, and one of them even has an SI prefix. The dimensions of g are mass and the cgs factor is 1. The dimensions of erg are mass * length$^2$ * time−2−2^{-2} and the cgs factor is 1. The dimensions of Msun/Mpc33^3 are mass / length33^3 and the cgs factor is about 6.8e-41.

Make full-text and cited references available via API. If these products were of equivalent or superior quality to those produced internally by ADS, it would simplify their workflow to rely on these APIs.

Currently, since arXiv lacks an explicit representation of authors and other entities in metadata, ADS must parse author metadata from arXiv heuristically.

ADS shares those matches with us via its API, and we use that information to populate DOI and JREF fields on arXiv papers.

Figure 1. K2 light curve of HD 3167 from Vanderburg et al. (2016).

Common Astronomy Software Application package

AST-1312950

#2016.1.01293.S

ADS/JAO.ALMA#2015.1.00504.S

Geneva group “high” mass-loss evolutionary tracks

Astronomical data take on a multitude of forms

Blender

The word "data" is plural and takes a plural verb.

manuscript

Online-only Figures Online-only figures are intended to provide supplementary information that is not critical to the scientific content of the paper but that provides additional useful information for the reader. They are not allowed when the figures are an integral part of the paper, or simply to limit page charges. Such materials will carry a nominal publication charge depending on the number and size of the figure files, but again this will be a small fraction of the cost of printing the same volume of material. Note that online-only materials are subject to the same peer-review standards as the rest of the manuscript, and their inclusion should be justified on scientific grounds.

In the printed paper, the placement of tables will be determined by their first mention in the text.