J/AJ/165/193     ∼30000 Gaia EDR3 nearby accelerating stars     (Whiting+, 2023)

A Catalog of Nearby Accelerating Star Candidates in Gaia DR3. Whiting M.L., Hill J.B., Bromley B.C., Kenyon S.J. <Astron. J., 165, 193 (2023)> =2023AJ....165..193W 2023AJ....165..193W
ADC_Keywords: Stars, double and multiple; Optical; Proper motions; Parallaxes, trigonometric Keywords: Binary stars ; Substellar companion stars ; Multiple stars Abstract: We describe a new catalog of accelerating star candidates with Gaia G≤17.5mag and distances d≤100pc. Designated as the Gaia Nearby Accelerating Star Catalog (GNASC), it contains 29684 members identified using a supervised machine-learning algorithm trained on the Hipparcos-Gaia Catalog of Accelerations (HGCA), Gaia Data Release 2, and Gaia Early Data Release 3. We take advantage of the difference in observation timelines between the two Gaia catalogs and information about the quality of the astrometric modeling based on the premise that acceleration will correlate with astrometric uncertainties. Catalog membership is based on whether constant proper motion over three decades can be ruled out at high confidence (greater than 99.9%). Test data suggest that catalog members each have a 68% likelihood of true astrometric acceleration; subsets of the catalog perform even better, with the likelihood exceeding 85%. We compare the GNASC with Gaia Data Release 3 and its table of stars for which acceleration is detected at high confidence based on precise astrometric fits. Our catalog, derived without this information, captures over 96% of the sources in the table that meet our selection criteria. In addition, the GNASC contains bright, nearby candidates that were not in the original Hipparcos survey, including members of known binary systems as well as stars with companions yet to be identified. It thus extends the HGCA and demonstrates the potential of the machine-learning approach for discovering hidden partners of nearby stars in future astrometric surveys. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 234 29684 *Gaia nearby accelerating star catalog -------------------------------------------------------------------------------- Note on table2.dat: All columns up to and including the column MPeak are from the Gaia EDR3 catalog. -------------------------------------------------------------------------------- See also: I/337 : Gaia DR1 (Gaia Collaboration, 2016) I/345 : Gaia DR2 (Gaia Collaboration, 2018) I/350 : Gaia EDR3 (Gaia Collaboration, 2020) J/A+A/525/A66 : 4 close binaries BVR light curves (Djurasevic+, 2011) J/AJ/143/134 : Candidate members of βPic/ABDor groups (McCarthy+, 2012) J/AJ/147/85 : Solar neighborhood. XXXIII. 45 M dwarfs (Riedel+, 2014) J/A+A/578/A136 : Period changes in SuperWASP eclipsing binaries (Lohr+, 2015) J/ApJ/844/103 : Orbit alignment in triple stars (Tokovinin, 2017) J/other/Nat/563.365 : Barnard's star radial velocity curve (Ribas+, 2018) J/AJ/160/215 : Solar neighborhood.XLVI. New Mdwarf binaries (Vrijmoet+, 2020) J/AJ/161/179 : Predicted positions of βPictoris b and c (Brandt+, 2021) J/ApJS/254/42 : Hipparcos-Gaia (EDR3) Catalog of Accelerations (Brandt, 2021) J/ApJS/254/10 : Compilation of W UMa stars (Latkovic+, 2021) J/AJ/162/61 : RVel follow up of Barnard's star with HPF (Lubin+, 2021) J/MNRAS/517/2925 : ORB6 binaries in Gaia EDR3 (Chulkov+, 2022) J/A+A/657/A7 : Stellar & substellar companions Gaia EDR3 (Kervella+, 2022) J/AJ/163/178 : Solar Neighborhood. XLIV. M dwarfs with SOAR (Vrijmoet+, 2022) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- EDR3 Gaia EDR3 source identifier 21- 33 F13.9 deg RAdeg [0/360] Right Ascension (ICRS) at Ep=2016.0 35- 47 F13.9 deg DEdeg [-90/90] Declination (ICRS) at Ep=2016.0 49- 61 F13.9 deg GLON [0/360] Galactic longitude 63- 75 F13.9 deg GLAT [-89/90] Galactic latitude 77- 85 F9.3 mas/yr pmRA [-2248/3430] Proper motion along Right Ascension 87- 95 F9.3 mas/yr pmDE [-5095/1712] Proper motion along Declination 97-101 F5.3 mas/yr e_pmRA [0.007/2] Uncertainty in pmRA 103-107 F5.3 mas/yr e_pmDE [0.009/1] Uncertainty in pmDE 109-115 F7.3 mas plx [10/375] Parallax 117-125 F9.3 mas e_plx [10/10083] Uncertainty in plx 127-132 F6.3 mag gmag [2.87/17.5] The G-band apparent magnitude 134-139 F6.3 mag BP-RP [-0.48/5.31] The (BP-RP) color 141-147 F7.4 --- RUWE [0.69/89.2] Renormalized unit-weighted error 149-159 F11.4 --- Excess [0.4/117646] Excess noise, astrometry; s.d 161-168 F8.4 --- GoF [-6.95/914] Goodness of fit, astrometry 170-174 A5 --- Dup Duplicated source flag; True or False 176-178 I3 % MPeak [0/100] Fields w/multiple peaks 180-198 I19 --- DR2 Gaia DR2 source identifier 200-208 F9.3 mas/yr pmRA2 [-2251/3430] Gaia DR2 proper motion along RA 210-218 F9.3 mas/yr pmDE2 [-5097/1714] Gaia DR2 proper motion along DE 220 I1 --- NSSFlag [0/3] NSS table flag (1) 222 I1 --- NKnown [0/2] Number of neighbors, known parallax (2) 224-225 I2 --- NUnKnown [0/53] Number of neighbors, unknown parallax (2) 227-234 F8.3 --- chi2 [28.7/5994] Predicted linear drift chi2 (3) -------------------------------------------------------------------------------- Note (1): Flags as follows: 0 = not a Gaia DR3 nss source 1 = nss_acceleration source 2 = nss_twobody source Note (2): The number of Gaia EDR3 neighbors within 200AU of each source. Note (3): This χ2 value is the machine Learning estimate from the hypothesis that a source has no acceleration. The minimum value for sources reported here is 28.75, corresponding to a 5-sigma outlier from the expected distribution of non-accelerating sources. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 19-Sep-2023
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