J/A+A/695/A195      New ultracool dwarf candidates from unTimely (Karpov+, 2025)

New ultracool dwarf candidates from multi-epoch WISE data. Karpov S., Malkov O., Avdeeva A. <Astron. Astrophys. 695, A195 (2025)> =2025A&A...695A.195K 2025A&A...695A.195K (SIMBAD/NED BibCode)
ADC_Keywords: Stars, brown dwarf ; Spectral types ; Proper motions; Stars, distances Keywords: surveys - proper motions - brown dwarfs Abstract: Thirty years after the discovery of brown dwarfs, the search for these objects continues, particularly in the vicinity of the Sun. Objects near the Sun are characterized by large proper motions, making them seen as fast-moving objects. While the Gaia DR3 catalogue is a comprehensive source of proper motions, it lacks the depth needed for discovering fainter objects. Modern multi-epoch surveys, with their greater depth, offer a new opportunity for systematic search for ultracool dwarfs. The study aims to systematically search for high proper motion objects using the newly released catalogue of epochal WISE data in order to identify new brown dwarf candidates in the solar neighborhood, estimate their spectral types, distances and spatial velocities. We used recently released unTimely catalogue of epochal detections in unWISE coadds to search for objects with high proper motions using simple motion detection algorithm, combined with machine learning based artefact rejection routine. This method was used to identify objects with proper motions exceeding approximately 0.3 arcseconds per year. The identified objects were then cross-referenced with data from other large-scale sky surveys to further analyze their characteristics. The search yielded 21885 moving objects with significant proper motions, 258 of which had not been previously published. All except 6 of them are compatible with being ultracool dwarfs. Among these, at least 33 were identified as most promising new T dwarf candidates, with estimated distances closer than about 40 parsecs, and effective temperatures less than 1300K. Description: The catalogue contains high proper motion objects detected in unTimely catalogue of WISE epochal photometry that lack Simbad or Gaia DR3 counterparts and have not been published previously. Their multi-wavelength photometry is recovered from positional cross-match with other large-scale optical and infrared catalogues, and used to estimate their effective temperatures via SED fitting with BT-Settl atmosphere model grid. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 1854 258 New high-proper-motion objects detected in this work -------------------------------------------------------------------------------- See also: I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) II/365 : The CatWISE2020 catalog (updated version 28-Jan-2021) (Marocco+, 2021) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 22 A22 --- Candid Candidate ID from unTimely 24- 42 A19 --- CWISE Candidate ID from CatWISE2020, JHHMMSS.ss+DDMMSS.s 44- 63 F20.16 deg RAdeg Right ascension (ICRS) at Ep=J2016.0 65- 85 F21.17 deg DEdeg Declination (ICRS) at Ep=J2016.0 87- 109 F23.20 arcsec/yr pmRA Proper motion in Right ascension 111- 131 F21.19 arcsec/yr e_pmRA Error of pmRA 133- 153 F21.18 arcsec/yr pmDE Proper motion in Declination 155- 175 F21.19 arcsec/yr e_pmDE Error of pmDE 177- 195 F19.17 arcsec/yr PM Proper motion 197- 217 F21.19 arcsec/yr e_PM Error of PM 219- 236 F18.15 mag W1 WISE W1 band magnitude 238- 257 F20.18 mag e_W1 Error of W1 259- 276 F18.15 mag W2 WISE W2 band magnitude 278- 297 F20.18 mag e_W2 Error of W2 299- 317 F19.15 mag uSMSS ? SkyMapper DR4 u band magnitude 319- 339 F21.18 mag e_uSMSS ? Error of uSMSS 341- 359 F19.15 mag gDELVE ? DELVE DR2 g band magnitude 361- 381 F21.18 mag e_gDELVE ? Error of gDELVE 383- 401 F19.15 mag gNSC ? NSC DR2 g band magnitude 403- 423 F21.18 mag e_gNSC ? Error of gNSC 425- 443 F19.15 mag gPS1 ? PanSTARRS DR2 g band magnitude 445- 464 F20.17 mag e_gPS1 ? Error of gPS1 466- 484 F19.15 mag gSDSS ? SDSS DR16 g band magnitude 486- 491 F6.3 mag e_gSDSS ? Error of gSDSS 493- 511 F19.15 mag gSMSS ? SkyMapper DR4 g band magnitude 513- 533 F21.18 mag e_gSMSS ? Error of gSMSS 535- 553 F19.15 mag rDELVE ? DELVE DR2 r band magnitude 555- 574 F20.17 mag e_rDELVE ? Error of rDELVE 576- 594 F19.15 mag rNSC ? NSC DR2 r band magnitude 596- 617 F22.19 mag e_rNSC ? Error of rNSC 619- 637 F19.15 mag rPS1 ? PanSTARRS DR2 r band magnitude 639- 658 F20.17 mag e_rPS1 ? Error of rPS1 660- 678 F19.15 mag rSMSS ? SkyMapper DR4 r band magnitude 680- 700 F21.18 mag e_rSMSS ? Error of rSMSS 702- 720 F19.15 mag iDELVE ? DELVE DR2 i band magnitude 722- 742 F21.18 mag e_iDELVE ? Error of iDELVE 744- 762 F19.15 mag iNSC ? NSC DR2 i band magnitude 764- 785 F22.19 mag e_iNSC ? Error of iNSC 787- 805 F19.15 mag iPS1 ? PanSTARRS DR2 i band magnitude 807- 828 F22.19 mag e_iPS1 ? Error of iPS1 830- 848 F19.15 mag iSDSS ? SDSS DR16 i band magnitude 850- 869 F20.17 mag e_iSDSS ? Error of iSDSS 871- 889 F19.15 mag iSMSS ? SkyMapper DR4 i band magnitude 891- 911 F21.18 mag e_iSMSS ? Error of iSMSS 913- 931 F19.15 mag zDELVE ? DELVE DR2 z band magnitude 933- 954 F22.19 mag e_zDELVE ? Error of zDELVE 956- 974 F19.15 mag zNSC ? NSC DR2 z band magnitude 976- 996 F21.18 mag e_zNSC ? Error of zNSC 998-1016 F19.15 mag zPS1 ? PanSTARRS DR2 z band magnitude 1018-1038 F21.18 mag e_zPS1 ? Error of zPS1 1040-1058 F19.15 mag zSDSS ? SDSS DR16 z band magnitude 1060-1080 F21.18 mag e_zSDSS ? Error of zSDSS 1082-1100 F19.15 mag zSMSS ? SkyMapper DR4 z band magnitude 1102-1122 F21.18 mag e_zSMSS ? Error of zSMSS 1124-1142 F19.15 mag yPS1 ? PanSTARRS DR2 y band magnitude 1144-1164 F21.18 mag e_yPS1 ? Error of yPS1 1166-1184 F19.15 mag YNSC ? NSC DR2 Y band magnitude 1186-1206 F21.18 mag e_YNSC ? Error of YNSC 1208-1226 F19.15 mag YVHS ? VHS DR5 Y band magnitude 1228-1235 F8.5 mag e_YVHS ? Error of YVHS 1237-1255 F19.15 mag IDENIS ? DENIS I band magnitude 1257-1276 F20.17 mag e_IDENIS ? Error of IDENIS 1278-1296 F19.15 mag J2MASS ? 2MASS J band magnitude 1298-1318 F21.18 mag e_J2MASS ? Error of J2MASS 1320-1338 F19.15 mag JDENIS ? DENIS J band magnitude 1340-1359 F20.17 mag e_JDENIS ? Error of JDENIS 1361-1379 F19.15 mag JUHS ? UHS DR2 J band magnitude 1381-1402 F22.19 mag e_JUHS ? Error of JUHS 1404-1422 F19.15 mag JVHS ? VHS DR5 J band magnitude 1424-1444 F21.18 mag e_JVHS ? Error of JVHS 1446-1464 F19.15 mag H2MASS ? 2MASS H band magnitude 1466-1486 F21.18 mag e_H2MASS ? Error of H2MASS 1488-1506 F19.15 mag HVHS ? VHS DR5 H band magnitude 1508-1515 F8.5 mag e_HVHS ? Error of HVHS 1517-1535 F19.15 mag K2MASS ? 2MASS K band magnitude 1537-1556 F20.17 mag e_K2MASS ? Error of K2MASS 1558-1576 F19.15 mag KDENIS ? DENIS K band magnitude 1578-1596 F19.16 mag e_KDENIS ? Error of KDENIS 1598-1616 F19.15 mag KUHS ? UHS DR2 K band magnitude 1618-1639 F22.19 mag e_KUHS ? Error of KUHS 1641-1659 F19.15 mag KsVHS ? VHS DR5 Ks band magnitude 1661-1681 F21.18 mag e_KsVHS ? Error of KsVHS 1683-1693 F11.5 K Teff ? Effective temperature 1695-1705 F11.6 K e_Teff ? Error of Teff 1707-1714 A8 --- SpType Estimated spectral type 1716-1736 F21.17 --- b_SpType Lower bound on spectral type 1738-1758 F21.17 --- B_SpType Upper bound on spectral type 1760 I1 --- SpMet [0/2] Method used to derive spectral type 1762-1771 A10 --- SpMetStr Method used to derive spectral type 1773-1791 F19.15 pc Dist Estimated distance 1793-1812 F20.16 pc e_Dist Error of dist 1814-1833 F20.15 km/s Vtan Estimated tangential velocity 1835-1854 F20.16 km/s e_Vtan Error of vtan -------------------------------------------------------------------------------- Acknowledgements: Sergey Karpov, karpov.sv(at)gmail.com References: Meisner et al., 2023AJ....165...36M 2023AJ....165...36M, The unTimely catalogue
(End) Sergey Karpov [FZU, Czech Republic], Patricia Vannier [CDS] 04-Mar-2025
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