Iras-allsky

NASA Exoplanet Archive Digital Object Identifiers

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.

43 DOIs
10.26133/NEA1 Confirmed Planets Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Confirmed Planets Table

Description

The Confirmed Planets table contains physical and orbital parameters for the planet and the host star, as available from the default literature reference for each planet. This table has been retired as of 2021 and it has been replaced by the Planetary Systems table (10.26133/NEA12).

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA2 Composite Planet Data Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Composite Planet Data Table

Description

The Composite Planet Data table provides a collection of stellar and planetary parameters for confirmed exoplanets, one row per planet. The table automatically selects the data from other available literature references for the same planet to fill in gaps from the default literature reference. This table has been retired as of 2021 and it has been replaced by the Planetary Systems Composite Parameters table (10.26133/NEA13).

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA3 K2 Candidates Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

K2 Candidates Table

Description

The K2 candidates table lists objects from the published literature identified as candidates or false positives. If objects are confirmed as planets, their status in this table is updated but the objects remain. This table has been retired as of 2021 and it has been replaced by the K2 Planets and Candidates table (10.26133/NEA19).

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA4 Kepler Objects of Interest Cumulative Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Kepler Objects of Interest Cumulative Table

Description

The Kepler Objects of Interest (KOI) cumulative table gathers information from the individual KOI activity tables that describe the current results of different searches of the Kepler light curves. The intent of the cumulative table is to provide the most accurate dispositions and stellar and planetary information for all KOIs in one place. All the information in this table has provenance in other KOI activity tables.

Please note that the Kepler Objects of Interest table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA4, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA4 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{cumulative,

doi = {10.26133/NEA4},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA4},

author = {{NASA Exoplanet Archive}},

title = {Kepler Objects of Interest Cumulative Table},

publisher = {NExScI-Caltech/IPAC},

version = {Version: 20YY-MM-DD HH:MM},

year = {yyyy}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(yyyy)}]{k2pandc}

{NASA Exoplanet Archive}. yyyy, Kepler Objects of Interest Cumulative Table,

Version: YYYY-MM-DD HH:MM, NExScI-Caltech/IPAC, \href{https://doi.org/10.26133/NEA4}{doi:10.26133/NEA4}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{cumulative}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA5 Kepler Objects of Interest DR 25 Table

Publisher

IPAC

Author(s)

Kepler Mission

Title

Kepler Objects of Interest DR 25 Table

Description

The Q1–Q17 Data Release 25 (DR25) Supplemental Kepler Objects-of-Interest (KOI) activity table reports dispositions based on the final processing (DR25) of the Kepler data and a combination of automated and human-based vetting to produce a "best-knowledge" catalog of planetary CANDIDATEs and FALSE POSITIVEs for use by the Astronomical community in selecting KOIs for follow-up observations and further study.

Please note that the Kepler Objects of Interest DR 25 Table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA5, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA5 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{koidr25,

doi = {10.26133/NEA5},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA19},

author = {{NASA Exoplanet Archive}},

title = {Kepler Objects of Interest DR25},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{k2pandc}

{NASA Exoplanet Archive}. YYYY, Kepler Objects of Interest DR25,

Version: YYYY-MM-DD HH:MM, NExScI-Caltech/IPAC, \href{https://doi.org/10.26133/NEA5}{doi:10.26133/NEA5}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{k2pandc}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA6 Kepler Stellar Properties Table

Publisher

IPAC

Author(s)

Kepler Mission

Title

Kepler Stellar Properties Table

Description

The Kepler Stellar interactive table contains parameters for all targets observed by Kepler for the purpose of finding transiting planets. Individual tables include the values used for that specific processing, including the Q1-12, Q1-16, Q1-17 DR 24, and Q1-17 DR 25 pipeline runs. One additional table, the Q1-17 DR 25 Supplemental Stellar, includes values provided by the Kepler Stellar Properties Working Group (SPWG) independent of any pipeline processing in order to report their most current stellar values.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA7 UKIRT Microlensing Survey

Publisher

IPAC

Author(s)

UKIRT Microlensing Team

Title

UKIRT Microlensing Survey

Description

Light curves from the ongoing UKIRT microlensing survey made available with help from the UKIRT Microlensing Team.The Wide Field Camera (WFCAM) on the United Kingdom Infrared Telescope (UKIRT), located at Mauna Kea Observatory, has been used to conduct microlensing surveys with a variety of science goals.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA8 KELT Survey Light Curves

Publisher

IPAC

Author(s)

KELT Team

Title

KELT Survey Light Curves

Description

The Kilodegree Extremely Little Telescope (KELT) survey consists of two robotic telescopes that are conducting a survey for transiting exoplanets around bright stars. The NASA Exoplanet Archive currently contains about 1.1 million light curves in selected Northern fields.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA9 SuperWASP Survey Light Curves

Publisher

IPAC

Author(s)

SuperWASP Consortium

Title

SuperWASP Survey Light Curves

Description

SuperWASP consists of two robotic observatories that operate continuously throughout the year, allowing coverage of both hemispheres of the sky. The first, SuperWASP-North, is located on the island of La Palma among the Isaac Newton Group (ING) of telescopes. The second, SuperWASP-South, is located at the site of the South African Astronomical Observatory (SAAO), just outside Sutherland, South Africa. The NASA Exoplanet Archive hosts over 18 million light curves collected between 2004 and 2008.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA10 Transmission Spectroscopy Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Transmission Spectroscopy Table

Description

The transmission spectroscopy table contains wavelength-dependent transit measurements from the published literature. The transit measurements are published as either transit depths, planet-to-star radius ratios, or planet radii, and span wavelengths across the electromagnetic spectrum.

Please note that the Transit Spectroscopy table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA10, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA10 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{transitspec,

doi = {10.26133/NEA10},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA10},

author = {{NASA Exoplanet Archive}},

title = {Transmission Spectroscopy Table},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{transitspec}

{NASA Exoplanet Archive}. YYYY, Transmission Spectroscopy Table,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA10}{doi:10.26133/NEA10}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{transitspec}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA11 Emission Spectroscopy Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Emission Spectroscopy Table

Description

The emission spectroscopy table contains wavelength-dependent eclipse measurements from the published literature. The eclipse measurements are published as either eclipse depths or brightness temperature, and span wavelengths across the electromagnetic spectrum.

Please note that the Emission Spectroscopy table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA11, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA11 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{emissionspec,

doi = {10.26133/NEA11},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA11},

author = {{NASA Exoplanet Archive}},

title = {Emission Spectroscopy Table},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{emissionspec}

{NASA Exoplanet Archive}. YYYY, Emission Spectroscopy Table,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA11}{doi:10.26133/NEA11}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{emissionspec}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA12 Planetary Systems Table

Publisher

IPAC

Author(s)

NASA Exoplanet Science Institute

Title

Planetary Systems Table

Description

The Planetary Systems Table contains, for all published confirmed exoplanets, the physical and orbital parameters for the exoplanets and the host stars. This table replaced the now-retired Confirmed Planets table (10.26133/NEA1).

Please note that the Planetary Systems table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA12, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA12 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{ps,

doi = {10.26133/NEA12},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA12},

author = {{NASA Exoplanet Archive}},

title = {Planetary Systems},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{ps}

{NASA Exoplanet Archive}. YYYY, Planetary Systems,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA12}{doi:10.26133/NEA12}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{ps}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Collection

Version

Table is updated wee

Date of data collection

Year of publication

10.26133/NEA13 Planetary Systems Composite Table

Publisher

IPAC

Author(s)

NASA Exoplanet Science Institute

Title

Planetary Systems Composite Table

Description

The Planetary Systems Composite Table provides, for all confirmed exoplanetary systems, a compilation of planetary and stellar parameters. The table pulls data from the Planetary Systems Table (10.26133/NEA12) and uses multiple references to fill in gaps to produce as "full" of a table as possible. This table is updated in parallel with Planetary Systems Table updates. This table replaced the now-retired Composite Parameters table (10.26133/NEA2).

Please note that the Planetary Systems table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA12, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA13 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{PSCompPars,

doi = {10.26133/NEA13},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA13},

author = {{NASA Exoplanet Archive}},

title = {Planetary Systems Composite Parameters},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{PSCompPars}

{NASA Exoplanet Archive}. YYYY, Planetary Systems,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA13}{doi:10.26133/NEA13}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{PSCompPars}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Collection

Version

Table updated weekly

Date of data collection

Year of publication

10.26133/NEA14 Kepler Mission Completeness and Reliability Products

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Mission Completeness and Reliability Products

Description

This dataset contains data products produced by the Kepler Project related to completeness and reliability of the Kepler pipeline.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

DR24 and DR25 (Final

Date of data collection

Year of publication

10.26133/NEA15 Kepler Threshold Crossing Events DR25

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Threshold Crossing Events DR25

Description

This is a table of the Threshold Crossing Events (TCEs) which are a sequence of transit-like features in the Kepler flux time series of a given target that resembles the signature of a transiting planet to a sufficient degree that the target is passed on for further analysis. There are four versions of this product [Q1-Q12], [Q1-Q16], [Q1-Q17, DR24] and [Q1-Q17, DR25]. The DR25 version is the final version

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Multiple Versions

Date of data collection

Year of publication

10.26133/NEA16 Kepler KOI Positional Probabilities

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler KOI Positional Probabilities

Description

Kepler Mission product that contains information on the possibility of the transit signal arising from an astrophysical source other than the target star.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA17 Kepler Misson False Positive Probabilities

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Misson False Positive Probabilities

Description

The Kepler Project False Positive Probabilities table contains the results of running an automated transit false-positive-probability (FPP) calculating procedure on all KOIs.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

DR25

Date of data collection

Year of publication

10.26133/NEA18 Kepler Certified False Positives

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Certified False Positives

Description

This Kepler Mission product contains information about the False Positive nature of Kepler Objects of Interest as determined by the Kepler False Positive Working Group.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

10.26133/NEA19 K2 Planets and Candidates Table

Publisher

IPAC

Author(s)

David Ciardi

Title

K2 Planets and Candidates Table

Description

The K2 Planets and Candidates table lists objects from the published literature identified as confirmed planets, candidates or false positives discovered by the K2 Mission. If objects are confirmed as planets, their status in this table is updated but the objects remain.

Please note that the K2 Planets and Candidates table is continuously updated. When referring to it, please cite the DOI: 10.26133/NEA19, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA19 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{k2pandc,

doi = {10.26133/NEA19},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA19},

author = {{NASA Exoplanet Archive}},

title = {K2 Planets and Candidates},

publisher = {IPAC},

version = {Version: 20YY-MM-DD HH:MM},

year = {2021}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(2021)}]{k2pandc}

{NASA Exoplanet Archive}. 2021, K2 Planets and Candidates Table,

Version: 20YY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA19}{doi:10.26133/NEA19}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{k2pandc}\footnote{Accessed on 20YY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Collection

Version

Date of data collection

Year of publication

10.26133/NEA20 Kepler Project Document: Uniform Modeling of KOIs - MCMC Data Release Notes

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: Uniform Modeling of KOIs - MCMC Data Release Notes

Description

This document describes data products related to the reported planetary parameters and uncertainties for the Kepler Objects of Interest (KOIs) based on a Markov-Chain-Monte- Carlo (MCMC) analysis. Reported parameters, uncertainties and data products can be found at the NASA Exoplanet Archive. The relevant paper for details of the calculations is Rowe et al. 2015.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

1

Date of data collection

02 Mar 2015

Year of publication

10.26133/NEA21 Kepler Project Document: Planet Detection Metrics: Automatic Detection of Background Objects Using the Centroid Robovetter

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: Planet Detection Metrics: Automatic Detection of Background Objects Using the Centroid Robovetter

Description

An overview of the automated method of identifying background eclipsing binaries masquerading as planet candidates in the Kepler planet candidate catalogs is described. The manual vetting process for Kepler Objects of Interest (KOIs) described in Bryson et al. (2013) with a series of measurements and tests that can be performed algorithmically is codified. The automated results are compared with a sample of manually vetted KOIs from the catalog of Burke et al. (2014).

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

1

Date of data collection

22 May 2017

Year of publication

10.26133/NEA22 Kepler Project Document: KSCI-19085 Planet Detection Metrics: Window and 1sigma Depth Functions for DR24

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19085 Planet Detection Metrics: Window and 1sigma Depth Functions for DR24

Description

This document describes the window and one-sigma depth functions produced by the Transiting Planet Search (TPS) algorithm in the Kepler pipeline (Jenkins 2002). The window function specifies the fraction of phase space over which three transits are observable as a function of orbital period. The one-sigma depth function specifies the depth of a signal (in ppm) for a given light curve that results in a one-sigma detection of a transit signature as a function of orbital period when averaged over phase.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

15 Dec 2016

Year of publication

10.26133/NEA23 Kepler Project Document: KSCI-19091 Autovetter Planet Candidate Catalog for Q1-Q17 DR24

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19091 Autovetter Planet Candidate Catalog for Q1-Q17 DR24

Description

This document describes the Kepler autovetter, and how it is used to produce a catalog of Planet Candidates from the Q1-Q17 DR24 TCEs (Threshold Crossing Events) that are identified in the Kepler SOC (Science Operations Center) pipeline [Jenkins 2010ab] version 9.2 [Seader et al. 2015].

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

1

Date of data collection

20 Jul 2015

Year of publication

10.26133/NEA24 Kepler Project Document: KSCI-19092: Planet Reliability Metrics: Astrophysical Positional Probabilities

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19092: Planet Reliability Metrics: Astrophysical Positional Probabilities

Description

This document describes the Kepler astrophysical positional probabilities (APP) table hosted at the Exoplanet Archive1. This table lists the stars with the highest probability of being co-located with the source of an observed transit, as well as the probability of the transit being on an unknown background source. The position of the transit signal source relative to the target star is found in the KOI tables at the Exoplanet Archive. These probabilities measure how well a star’s location matches the location of the transit signal – they do not measure the probability that the transit signal is consistent with a planet orbiting that star.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

13 Nov 2015

Year of publication

10.26133/NEA25 Kepler Project Document: KSCI-19093 Kepler Certified False Positive Table

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19093 Kepler Certified False Positive Table

Description

This document describes the Kepler Certified False Positive table hosted at the Exoplanet Archive1, herein referred to as the “CFP table”. This table is the result of detailed examina- tion by the Kepler False Positive Working Group (FPWG) of declared false positives in the Kepler Object of Interest (KOI) tables at the Exoplanet Archive. A KOI is considered a false positive in the CFP table if it is not due to a planet orbiting the KOI’s target star. The CFP table contains all KOIs in the Exoplanet Archive cumulative KOI table.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

4

Date of data collection

04 Oct 2019

Year of publication

10.26133/NEA26 Kepler Project Document: KSCI-19094 Planet Detection Metrics: Pipeline Detection Efficiency

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19094 Planet Detection Metrics: Pipeline Detection Efficiency

Description

This document describes the results of the third pixel-level transit injection experiment designed to measure the detection efficiency of the Kepler pipeline.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

22 Oct 2015

Year of publication

10.26133/NEA27 Kepler Project Document: KSCI-19096 Planet Detection Metrics: Vetting Detection Efficiency

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19096 Planet Detection Metrics: Vetting Detection Efficiency

Description

This document describes the results of running the Kepler robovetter on the recovered injected TCEs to determine the TCERT detection efficiency. The results of both exercises are available at the NASA Exoplanet Archive.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

19 Nov 2015

Year of publication

10.26133/NEA28 Kepler Project Document: KSCI-19101 Planet Detection Metrics: Window and 1sigma Depth Functions for DR25

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19101 Planet Detection Metrics: Window and 1sigma Depth Functions for DR25

Description

This document describes the window and one-sigma depth functions relevant to the Transiting Planet Search (TPS) algorithm in the Kepler pipeline. The window function specifies the fraction of unique orbital ephemeris epochs over which three transits are observable as a function of orbital period. In this context, the epoch and orbital period, together, comprise the ephemeris of an orbiting companion, and ephemerides with the same period are considered equivalent if their epochs differ by an integer multiple of the period. The one-sigma depth function specifies the depth of a signal (in ppm) for a given light curve that results in a one-sigma detection of a transit signature as a function of orbital period when averaged over all unique orbital ephemerides.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

03 May 2017

Year of publication

10.26133/NEA29 Kepler Project Document: KSCI-19108 Planet Detection Metrics: Astrophysical Positional Probabilties for DR25

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19108 Planet Detection Metrics: Astrophysical Positional Probabilties for DR25

Description

This document describes the Kepler astrophysical positional probabilities (APP) table hosted at the Exoplanet Archive updated for DR25. This table lists the stars with the highest probability of being co-located with the source of an observed transit, as well as the probability of the transit being on an unknown background source. The position of the transit signal source relative to the target star is found in the KOI tables at the Exoplanet Archive. These probabilities measure how well a star’s location matches the location of the transit signal – they do not measure the probability that the transit signal is consistent with a planet orbiting that star.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

1

Date of data collection

28 Feb 2017

Year of publication

10.26133/NEA30 Kepler Project Document: KSCI-19111 Planet Detection Metrics: Per Target Detection Contours for DR25

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19111 Planet Detection Metrics: Per Target Detection Contours for DR25

Description

This document describes the use of the Kepler planet occurrence rate products in order to calculate a per-target detection contour for the measured Data Re- lease 25 (DR25) pipeline performance. A per-target detection contour measures for a given combination of orbital period, Porb, and planet radius, Rp, what fraction of transit signals are recoverable by the Kepler pipeline.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

13 Jun 2017

Year of publication

10.26133/NEA31 Kepler Project Document: KSCI-19104: Description of the TCERT Vetting Products for Q1-Q17 DR24 Catalog

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19104: Description of the TCERT Vetting Products for Q1-Q17 DR24 Catalog

Description

This document describes the Q1-Q17 DR24 TCERT Vetting products - a collection of plots and diagnostics used by the Threshold Crossing Event Review Team (TCERT) to evaluate threshold crossing events (TCEs). While designation of Kepler Objects of Interest (KOIs) and classification of them as Planet Candidates (PCs) or False Positives (FPs) is completely automated via a robotic vetting procedure for the Q1-Q17 DR24 planet catalog described in Coughlin et al. (2015), these products help to evaluate those robotic decisions for individual objects. For each TCE identified in the Q1-Q17 DR24 transit search, these products collect in one readily accessible place: (a) the DV one-page summary, (b) selected pertinent diagnostics and plots from the full DV report, and (c) supplemental plots and diagnostics not included in the full DV report, including an alternate means of data detrending. This document describes each plot in detail, and how it can be used to evaluate the various data sources to determine if a TCE is a PC or FP.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

1

Date of data collection

22 Jun 2015

Year of publication

10.26133/NEA32 Kepler Project Document: KSCI-19105: Description of the TCERT Vetting Products for Q1-Q17 DR25 Catalog

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19105: Description of the TCERT Vetting Products for Q1-Q17 DR25 Catalog

Description

This document describes the Q1–Q17 DR25 TCERT Vetting Reports: a collection of plots and diagnostics used by the Threshold Crossing Event Review Team (TCERT) to evaluate threshold crossing events (TCEs). While designation of Kepler Objects of Interest (KOIs) and classification of them as Planet Candidates (PCs) or False Positives (FPs) is completely automated via a robotic vetting procedure (the Robovetter) for the Q1–Q17 DR25 planet catalog, as described in Thompson et al. (2017), these reports help to visualize the metrics used by the Robovetter and evaluate those robotic decisions for individual objects. For each Q1–Q17 DR25 TCE, these reports include the following products: (a) the DV one-page summary, (b) selected pertinent diagnostics and plots from the full DV report, and (c) additional plots and diagnostics not included in the full DV report, including an alternate means of data detrending.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

21 Sep 2017

Year of publication

10.26133/NEA33 Kepler Project Document: KSCI-19109 Planet Detection Metrics: Per-Target Flux-Level Transit Injection Tests of TPS for DR25

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19109 Planet Detection Metrics: Per-Target Flux-Level Transit Injection Tests of TPS for DR25

Description

This document describes the Flux Level Transit Injection (FLTI) techniques used in the Kepler Pipeline, defines the output file format of the simulated products, and details the various tests run. The document also describes sample python code for calculating pipeline completeness using the FLTI results and provides some worked examples.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

13 Jun 2017

Year of publication

10.26133/NEA34 Kepler Project Document: KSCI-19110 Planet Detection Metrics: Pixel-Level Transit Injection Tests of Pipeline Detection Efficiency for DR25

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19110 Planet Detection Metrics: Pixel-Level Transit Injection Tests of Pipeline Detection Efficiency for DR25

Description

This document describes the results of the fourth pixel-level transit injection experiment, which was designed to measure the detection efficiency of both the Kepler pipeline and the Robovetter.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

1

Date of data collection

01 June 2017

Year of publication

10.26133/NEA35 Kepler Project Document: KSCI-19114: Planet Detection Metrics: Robovetter Completeness and Effectiveness for DR25

Publisher

IPAC

Author(s)

Kepler Project

Title

Kepler Project Document: KSCI-19114: Planet Detection Metrics: Robovetter Completeness and Effectiveness for DR25

Description

This document describes the results of running the Robovetter on the Kepler observed, injected, inverted, and scrambled populations, which are available at the NASA Exoplanet Archive. The document describes the experimental design to calculate the Robovetter completeness and effectiveness, the tables that contain the results of running the Robovetter on the observed, injected, inverted, and scrambled TCEs, and some example results that can be used to compute accurate occurrence rates.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Text

Version

2

Date of data collection

31 Aug 2017

Year of publication

10.26133/NEA36 Atmospheric Spectroscopy Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Atmospheric Spectroscopy Table

Description

The NASA Exoplanet Archive Atmospheric Spectroscopy Table provides a unified interface to browse, visualize, plot, and download exoplanet emission and transmission spectra.

Please note that the Atmospheric Spectroscopy table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA36, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA36 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{spectra,

doi = {10.26133/NEA36},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA36},

author = {{NASA Exoplanet Archive}},

title = {Atmospheric Spectroscopy Table},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{spectra}

{NASA Exoplanet Archive}. YYYY, Atmospheric Spectroscopy Table,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA36}{doi:10.26133/NEA36}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{spectra}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Service

Version

Date of data collection

Year of publication

2023

10.26133/NEA37 Transiting Planets Table

Publisher

IPAC

Author(s)

NASA Exoplanet Science Institute

Title

Transiting Planets Table

Description

The Transiting Planets Table is a simpler interface for accessing all of the transit-specific observables currently in the Exoplanet Archive. These data are a subset of what is available in the Planetary Systems (10.26133/NEA12) and Planetary Systems Composite Data (10.26133/NEA13) tables.

Please note that the Transiting Planets table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA37, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA37 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{td,

doi = {10.26133/NEA37},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA37},

author = {{NASA Exoplanet Archive}},

title = {Transiting Planets Table},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{td}

{NASA Exoplanet Archive}. YYYY, Transit Detection Table,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA37}{doi:10.26133/NEA37}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{td}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Collection

Version

Updated Weekly

Date of data collection

Year of publication

2023

10.26133/NEA38 Microlensing Planets Table

Publisher

IPAC

Author(s)

NASA Exoplanet Science Institute

Title

Microlensing Planets Table

Description

The Microlensing Planets Table is a simpler interface for accessing all of the microlensing-specific observables currently in the Exoplanet Archive. These data are a subset of what is available in the Planetary Systems (10.26133/NEA12) and Planetary Systems Composite Data (10.26133/NEA13) tables.

Please note that the Microlensing Planets table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA38, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA38 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{ml,

doi = {10.26133/NEA38},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA38},

author = {{NASA Exoplanet Archive}},

title = {Microlensing Planets Table},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{ml}

{NASA Exoplanet Archive}. YYYY, Microlensing Detection Table,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA38}{doi:10.26133/NEA38}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{ml}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Collection

Version

Updated Weekly

Date of data collection

Year of publication

2015

10.26133/NEA39 Habitable Worlds Observatory Preliminary Input Catalog

Publisher

IPAC

Author(s)

Tuchow, Stark, and Mamajek (2024)

Title

Habitable Worlds Observatory Preliminary Input Catalog

Description

This is a list of ∼13,000 bright, nearby objects from TESS and Gaia DR3 that are potential targets for space-based direct imaging with the Habitable Worlds Observatory.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

2024

10.26133/NEA40 Stellar Parameters for Planetary Hosts Table

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Stellar Parameters for Planetary Hosts Table

Description

The Stellar Parameters Table lists all of the stellar parameters for a planetary system currently in the Exoplanet Archive. These data are a superset of what is available in the Planetary Systems (10.26133/NEA12) and Planetary Systems Composite Data (10.26133/NEA13) tables. In addition to listing stellar solutions associated with a given planetary solution (as is the case for the Planetary Systems table), the stellar parameters table also includes stellar parameters that are in the Exoplanet Archive for a planet hosting star but the parameters are not associated with a specific planetary solution and stellar parameters of non-planet hosting stars in a planetary system.

Please note that the Stellar Parameters table is periodically updated. When referring to it, please cite the DOI: 10.26133/NEA40, e.g. in your reference list, and record the date/time of access.

bibtex (built from https://doi2bib.org/bib/10.26133/NEA40 but edited to include a version tag, which works with AASTeX aasjournal.bst style file)

@misc{STELLARHOSTS,

doi = {10.26133/NEA40},

url = {https://catcopy.ipac.caltech.edu/dois/doi.php?id=10.26133/NEA40},

author = {{NASA Exoplanet Archive}},

title = {Stellar Parameters Table},

publisher = {NExScI-Caltech/IPAC},

version = {Version: YYYY-MM-DD HH:MM},

year = {YYYY}

}

AASTeX (no bibtex)

\bibitem[{{NASA Exoplanet Archive}(YYYY)}]{STELLARHOSTS}

{NASA Exoplanet Archive}. YYYY, Stellar Parameters Table,

Version: YYYY-MM-DD HH:MM, IPAC, \href{https://doi.org/10.26133/NEA40}{doi:10.26133/NEA40}

Recommended text snippet:

We obtain the data set from the NASA Exoplanet Archive \citep{STELLARHOSTS}\footnote{Accessed on YYYY-MM-DD at HH:MM, returning NNNN rows.)}

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Service

Version

Date of data collection

Year of publication

2024

10.26133/NEA41 Frontier Data Labs (FDL) PyATMOS Model Atmospheres

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Frontier Data Labs (FDL) PyATMOS Model Atmospheres

Description

The PyATMOS dataset is the result of the work from the FDL 2018 Astrobiology challenge. It comprises a set of model earth-like exoplanet atmospheres, spanning a range of plausible parameter space.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

2022

10.26133/NEA42 Frontier Data Labs (FDL) INARA Data

Publisher

IPAC

Author(s)

NASA Exoplanet Archive

Title

Frontier Data Labs (FDL) INARA Data

Description

The INARA dataset is the result of the work from the FDL 2018 Astrobiology challenge. It comprises a set of 3,112,820 synthetic rocky exoplanetary spectra generated using the NASA Planetary Spectrum Generator (PSG).

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

2023

10.26133/NEA43 Colorado Ultraviolet Transit Experiment (CUTE) Exoplanet Transits

Publisher

IPAC

Author(s)

CUTE Team

Title

Colorado Ultraviolet Transit Experiment (CUTE) Exoplanet Transits

Description

The Colorado Ultraviolet Transit Experiment (CUTE) is a 6U NASA CubeSat launched in 2021 carrying on-board a low-resolution, near-ultraviolet (2479-3306 angstrom) spectrograph. CUTE is designed to monitor transiting extra-solar planets orbiting bright, nearby stars to improve our understanding of planet atmospheric escape and star-planet interaction processes. The CUTE data is processed with the CUTE autONomous daTa ReductiOn pipeLine (CONTROL). The details of the pipeline are described in Sreejith et al., 2022.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Data type

Dataset

Version

Date of data collection

Year of publication

2024