_version_ 1866916410535444480
author Brooks, Hunter
Caselden, Dan
Kirkpatrick, J. Davy
Raghu, Yadukrishna
Elachi, Charles
Grigorian, Jake
Trek, Asa
Washburn, Andrew
Higashimura, Hiro
Meisner, Aaron
Schneider, Adam
Faherty, Jacqueline
Marocco, Federico
Gelino, Christopher
Gagné, Jonathan
Bickle, Thomas
Tang, Shih-yun
Rothermich, Austin
Burgasser, Adam
Kuchner, Marc J.
Beaulieu, Paul
Bell, John
Colin, Guillaume
Colombo, Giovanni
Dereveanco, Alexandru
Flores, Deiby
Glebov, Konstantin
Gramaize, Leopold
Hamlet, Les
Hinckley, Ken
Kabatnik, Martin
Kiwy, Frank
Martin, David
Palma, Raul
Pendrill, William
Ruiz, Lizzeth
Sanchez, John
Sainio, Arttu
SchÜmann, JÖrg
Schonau, Manfred
Tanner, Christopher
Andersen, Nikolaj Stevnbak
Stenner, Andrés
Thévenot, Melina
Thakur, Vinod
Voloshin, Nikita
Wedracki, Zbigniew
author_facet Brooks, Hunter
Caselden, Dan
Kirkpatrick, J. Davy
Raghu, Yadukrishna
Elachi, Charles
Grigorian, Jake
Trek, Asa
Washburn, Andrew
Higashimura, Hiro
Meisner, Aaron
Schneider, Adam
Faherty, Jacqueline
Marocco, Federico
Gelino, Christopher
Gagné, Jonathan
Bickle, Thomas
Tang, Shih-yun
Rothermich, Austin
Burgasser, Adam
Kuchner, Marc J.
Beaulieu, Paul
Bell, John
Colin, Guillaume
Colombo, Giovanni
Dereveanco, Alexandru
Flores, Deiby
Glebov, Konstantin
Gramaize, Leopold
Hamlet, Les
Hinckley, Ken
Kabatnik, Martin
Kiwy, Frank
Martin, David
Palma, Raul
Pendrill, William
Ruiz, Lizzeth
Sanchez, John
Sainio, Arttu
SchÜmann, JÖrg
Schonau, Manfred
Tanner, Christopher
Andersen, Nikolaj Stevnbak
Stenner, Andrés
Thévenot, Melina
Thakur, Vinod
Voloshin, Nikita
Wedracki, Zbigniew
contents We present the discovery of 118 new ultracool dwarf candidates, discovered using a new machine learning tool, named \texttt{SMDET}, applied to time series images from the Wide-field Infrared Survey Explorer. We gathered photometric and astrometric data to estimate each candidate's spectral type, distance, and tangential velocity. This sample has a photometrically estimated spectral class distribution of 28 M dwarfs, 64 L dwarfs, and 18 T dwarfs. We also identify a T subdwarf candidate, two extreme T subdwarf candidates, and two candidate young ultracool dwarfs. Five objects did not have enough photometric data for any estimations to be made. To validate our estimated spectral types, spectra were collected for 2 objects, yielding confirmed spectral types of T5 (estimated T5) and T3 (estimated T4). Demonstrating the effectiveness of machine learning tools as a new large-scale discovery technique.
format Preprint
id arxiv_https___arxiv_org_abs_2408_14447
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Discovery of 118 New Ultracool Dwarf Candidates Using Machine Learning Techniques
Brooks, Hunter
Caselden, Dan
Kirkpatrick, J. Davy
Raghu, Yadukrishna
Elachi, Charles
Grigorian, Jake
Trek, Asa
Washburn, Andrew
Higashimura, Hiro
Meisner, Aaron
Schneider, Adam
Faherty, Jacqueline
Marocco, Federico
Gelino, Christopher
Gagné, Jonathan
Bickle, Thomas
Tang, Shih-yun
Rothermich, Austin
Burgasser, Adam
Kuchner, Marc J.
Beaulieu, Paul
Bell, John
Colin, Guillaume
Colombo, Giovanni
Dereveanco, Alexandru
Flores, Deiby
Glebov, Konstantin
Gramaize, Leopold
Hamlet, Les
Hinckley, Ken
Kabatnik, Martin
Kiwy, Frank
Martin, David
Palma, Raul
Pendrill, William
Ruiz, Lizzeth
Sanchez, John
Sainio, Arttu
SchÜmann, JÖrg
Schonau, Manfred
Tanner, Christopher
Andersen, Nikolaj Stevnbak
Stenner, Andrés
Thévenot, Melina
Thakur, Vinod
Voloshin, Nikita
Wedracki, Zbigniew
Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
We present the discovery of 118 new ultracool dwarf candidates, discovered using a new machine learning tool, named \texttt{SMDET}, applied to time series images from the Wide-field Infrared Survey Explorer. We gathered photometric and astrometric data to estimate each candidate's spectral type, distance, and tangential velocity. This sample has a photometrically estimated spectral class distribution of 28 M dwarfs, 64 L dwarfs, and 18 T dwarfs. We also identify a T subdwarf candidate, two extreme T subdwarf candidates, and two candidate young ultracool dwarfs. Five objects did not have enough photometric data for any estimations to be made. To validate our estimated spectral types, spectra were collected for 2 objects, yielding confirmed spectral types of T5 (estimated T5) and T3 (estimated T4). Demonstrating the effectiveness of machine learning tools as a new large-scale discovery technique.
title Discovery of 118 New Ultracool Dwarf Candidates Using Machine Learning Techniques
topic Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2408.14447