Mission Overview
The All-Sky PLATO Input Catalog (asPIC)
Primary Investigator: Giampaolo Piotto
HLSP Authors: Marco Montalto
Released: 2021-09-01
Updated: 2021-09-01
Primary Reference(s): Montalto et al. 2021
Citations: See ADS Statistics
Overview
The ESA PLAnetary Transits and Oscillations of stars (PLATO) mission will search for terrestrial planets in the habitable zone of solar-type stars. Because of telemetry limitations, PLATO targets need to be pre-selected. We present an all sky catalog that will be fundamental to select the best PLATO fields and the most promising target stars, derive their fundamental parameters, analyze the instrumental performances, and then plan and optimize follow-up observations. This catalog also represents a valuable resource for the general definition of stellar samples optimized for the search of transiting planets. The first public release of the all sky PLATO Input catalogue (asPIC version 1.1) contains a total of 2,675 ,539 stars, among which are 2,378,177 FGK dwarfs and subgiants and 297,362 M dwarfs. It was produced using Gaia Data Release 2 (DR2) astrometry and photometry and 3D maps of the local interstellar medium.
Data Products
The catalog is available as a FITS file with the following naming convention:
hlsp_aspic_gaia_astrometric-photometric_all-sky_multi_v1.1_cat.fits
Data file types:
_cat.fits | The PLATO input catalog. |
Catalog Column Definitions
Click to expand below and see the catalog columns, data types, and descriptions.
Column Name | Data Type | Description |
---|---|---|
PICidDR1 | bigint[8] | PLATO identifier for asPIC1.1 |
PICnameDR1 | varchar[32] | PLATO identifier for asPIC1.1 with version number |
sourceId | bigint[8] | Gaia DR2 sourceId |
RAdeg | float[8] | Barycentric right ascension of the source in ICRS at the reference epoch |
eRAdeg | real[4] | Standard error e_RA*=e_RA x cosDE of the right ascension in ICRS at the reference epoch |
DEdeg | float[8] | Barycentric declination of the source in ICRS at the reference epoch |
eDEdeg | real[4] | Standard error of the declination in ICRS at the reference epoch |
Plx | float[8] | Parallax |
ePlx | real[4] | Standard error on parallax |
pmRA | float[8] | Proper motion in right ascension direction pmRA* = pmRA x cosDE in ICRS at the reference epoch |
epmRA | real[4] | Standard error on proper motion in right ascension direction |
pmDE | float[8] | Proper motion in declination direction in ICRS at the reference epoch |
epmDE | real[4] | Standard error on proper motion in declination direction |
PM | float[8] | The total proper motion calculated as PM = sqrt(pmRA^2 + pmDE^2) |
ePM | real[4] | Error on the total proper motion |
Epoch | float[8] | Reference epoch to which the astrometric source parameters are referred |
Gflux | float[8] | Mean flux in the G band |
eGflux | float[8] | Error on G band mean flux |
Gmag | float[8] | Mean magnitude in the G band |
eGmag | float[8] | Error on mean magnitude in the G band |
BPflux | float[8] | Mean flux in the integrated BP band |
eBPflux | float[8] | Error on mean flux in the integrated BP band |
BPmag | float[8] | Mean magnitude in the integrated BP band |
eBPmag | float[8] | Error in the mean magnitude in the integrated BP band |
RPflux | float[8] | Mean flux in the integrated RP band |
eRPflux | float[8] | Error on mean flux in the integrated RP band |
RPmag | float[8] | Mean magnitude in the integrated RP band |
eRPmag | float[8] | Error in the mean magnitude in the integrated RP band |
BPRPexcess | real[4] | BP/RP excess factor |
BPRP | float[8] | GBP - GRP color |
BPG | float[8] | GBP - G color |
GRP | float[8] | G - GRP color |
GLON | float[8] | Galactic longitude of the object at the reference epoch |
GLAT | float[8] | Galactic latitude of the object at the reference epoch |
ELON | float[8] | Ecliptic longitude of the object at the reference epoch |
ELAT | float[8] | Ecliptic latitude of the object at the reference epoch |
rest | float[8] | The estimated distance from Bailer-Jones et al. 2018, AJ, 156, 58 |
rlo | float[8] | The lower bound of the confidence interval of the estimated distance from Bailer-Jones et al. 2018, AJ, 156, 58 |
rhi | float[8] | The higher bound of the confidence interval of the estimated distance from Bailer-Jones et al. 2018, AJ, 156, 58 |
erest | float[8] | The error in the estimated distance calculated as e_rest= 0.5(rhi - rlo) |
AG | float[8] | Estimate of the extinction AG in the G band |
eAG | float[8] | Uncertainty on AG estimate |
EBPRP | float[8] | Estimate of reddening E(GBP-GRP) |
eEBPRP | float[8] | Uncertainty on reddening E(GBP-GRP) |
EBV | float[8] | Estimate of reddening E(B-V) |
eEBV | float[8] | Uncertainty on E(B-V) reddening |
extStatus | int[4] | extStatus value. If extStatus=1 the star is outside the limits of the reddening map |
BPRP0 | float[8] | Dereddened (GBP - GRP) color |
eBPRP0 | float[8] | Error on dereddened (GBP - GRP) color (BP-RP)0 |
gaiaV0 | float[8] | Dereddened apparent visual magnitude V in the Johnson-Cousin system |
egaiaV0 | float[8] | Error on intrinsic visual magnitude (gaiaV0) |
BJgaiaMV0 | float[8] | Absolute intrinsic visual magnitude obtained as: BJgaiaMV0 = gaiaV0 - 5*log10(rest) + 5 |
eBJgaiaMV0 | float[8] | Error on absolute intrinsic visual magnitude (BJgaiaMV0) |
gaiaV | float[8] | Visual apparent magnitude in the Johnson-Cousin system obtained as: gaiaV = gaiaV0 + 3.1*E(B-V) |
egaiaV | float[8] | Error on apparent visual magnitude V (gaiaV) |
BJgaiaMG0 | float[8] | Absolute intrinsic G magnitude obtained as: BJgaiaMG0 = Gmag - 5*log10(rest) + 5 - AG |
eBJgaiaMG0 | float[8] | Error on intrinsic absolute G magnitude (BJgaiaMG0) |
Teff | real[4] | Estimate of stellar effective temperature (Teff) |
eTeff | real[4] | Uncertainty on Teff estimate |
Radius | real[4] | Estimate of stellar radius |
eRadius | real[4] | Uncertainty on stellar radius estimate |
Mass | real[4] | Estimate of stellar mass |
eMass | real[4] | Uncertainty on mass estimate |
sourceFlag | int[4] | Bitmask indicating if the source is a FGK or M star and if the star hosts known planet(s) [0=reset all bits, 1=FGK star, 2= M star, 4=Host Planet(s)] |
contGaiaMag60 | float[8] | Total G magnitude of the Gaia contaminants within 60 arcsec |
contNumber60 | int[4] | Total number of Gaia contaminants within 60 arcsec |
contGaiaMag45 | float[8] | Total G magnitude of the Gaia contaminants within 45 arcsec |
contNumber45 | int[4] | Total number of Gaia contaminants within 45 arcsec |
contGaiaMag30 | float[8] | Total G magnitude of the Gaia contaminants within 30 arcsec |
contNumber30 | int[4] | Total number of Gaia contaminants within 30 arcsec |
Data Access
Direct Download
The catalog can be downloaded as a FITS file (size ~1.4 GB): hlsp_aspic_gaia_astrometric-photometric_all-sky_multi_v1.1_cat.fits
CasJobs
The catalog is also available as a table in the MAST CasJobs SQL interface. The catalog is stored in a table called "CatalogRecord" in the "HLSP_ASPIC" Context.
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A web-based SQL interface to query and cross-match between catalogs. Export tables, saved queries, long query submissions.