A Digital Object Identifier (DOI) is a permanent and unique string used to identify a digital resource and link to it on the web. IPAC has created DOIs for many astronomical data sets and for its data or collection services, e.g., NED. If you are writing a manuscript that uses one of these data sets or services, we recommend that you reference the corresponding DOI in your manuscript’s bibliography, in addition to the appropriate refereed journal article. If you are submitting to an AAS Journal, instructions for referencing IPAC DOIs in your manuscript are provided here: https://journals.aas.org/aastexguide/#softwareandthirdparty. Tools such as doi2bib.org are useful for quickly generating BibTeX markup for these DOIs.
• 10.26135/KOA1 • 3 • 05 Nov 2020 • Dataset
J. O'Meara
This dataset or service is made available by the Keck Observatory Archive (KOA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.
• 10.26135/KOA2 • 1.0 • 16 Sep 2020 • Dataset
Bruce Berriman
This dataset or service is made available by the Keck Observatory Archive (KOA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration. KOA is a collaboration between the NASA Exoplanet Science Institute (NExScI) and the W. M. Keck Observatory (WMKO).
• 10.26135/KOA3 • 1.0 • Dataset
Bruce Berriman
This dataset is made available by the Keck Observatory Archive (KOA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.
• 10.26135/KOA4 • 1.0 • Dataset
Bruce Berriman
This dataset or service is made available by the Keck Observatory Archive (KOA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.
• 10.26135/KOA5 • v1 • 18 Jun 2024 • Dataset
Andrew Howard
A table of 2332 radial velocity and stellar activity measurements obtained from HIRES spectra for 84 stars. The data were acquired for the 'Exploring the Compositional Diversity of Small Exoplanets from K2' project.
This dataset is made available by the Keck Observatory Archive (KOA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.
• 10.26135/KOA6 • v1 • 18 Jun 2024 • Dataset
Andrew Howard
The table of empirical and synthetic derivations of several stellar properties for 440 stars observed by the 'Exploring the Compositional Diversity of Small Exoplanets from K2' project
This dataset is made available by the Keck Observatory Archive (KOA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.