Aidan McBride
5 Papers
20 Citations
Aidan McBride is an academic researcher. The author has contributed to research in topics: Stars & Orion Nebula. The author has an hindex of 2, co-authored 3 publications.
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Papers
Peer Review
The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V
Andres Almeida,Scott F. Anderson,M. Argudo-Fern'andez,Carles Badenes,Kathleen A. Barger,Jorge K. Barrera-Ballesteros,Chad F. Bender,Erika Benítez,Felipe E. Besser,Dmitry Bizyaev,Michael R. Blanton,John J. Bochanski,Jo Bovy,W. N. Brandt,Joel R. Brownstein,Johannes Buchner,Esra Bulbul,Joseph N. Burchett,Mariana Cano D'iaz,Joleen K. Carlberg,Andrew R. Casey,Vedant Chandra,Brian Cherinka,Cristina Chiappini,Abigail Coker,Johan Comparat,Charlie Conroy,Gabriella Contardo,Arlin Cortes,Kevin R. Covey,Jeffrey D. Crane,Katia Cunha,C. Dabbieri,James W. Davidson,M. Davis,Nathan De Lee,J. A. Delgado,Sebastian Demasi,F. Di Mille,John Donor,Peter Dow,Tom Dwelly,Michael Eracleous,Jamey E. Eriksen,Xiaohui Fan,Emily Farr,Sara Frederick,Logan B. Fries,Peter M. Frinchaboy,B. Gaensicke,Junqiang Ge,C. Ávila,Kathleen Grabowski,Catherine J. Grier,Guillaume Guiglion,Pramod Gupta,Patrick B. Hall,Keith Hawkins,Christian R. Hayes,J. J. Hermes,Lorena Hern'andez-Garc'ia,David W. Hogg,Jon A. Holtzman,Hector Ibarra-Medel,Alexander P. Ji,Paula Jofre,Jennifer A. Johnson,Amy Jones,Karen Kinemuchi,M. Kluge,Anton M. Koekemoer,Juna A. Kollmeier,Marina Kounkel,Dhanesh Krishnarao,Mirko Krumpe,Ivan Lacerna,Paulo J. A. Lago,Chervin F. P. Laporte,A. P. Liu,Chao Chao Liu,Xin Liu,A. Roman Lopes,Matin Macktoobian,Viktor Malanushenko,Dan Maoz,Thomas Masseron,Karen L. Masters,G. Matijevič,Aidan McBride,Ilija Medan,Andrea Merloni,Sean M. Morrison,Natalie K. Myers,Szabolcs M'esz'aros,Alenka Negrete,David L. Nidever,Christian Nitschelm,Audrey Oravetz,Daniel Oravetz,Kaike Pan,Yingjie Peng,Marc H. Pinsonneault,Richard W. Pogge,Dan Qiu,Anna B. A. Queiroz,Solange V. Ramirez,Hans-Walter Rix,Daniela Rosso,Jessie C. Runnoe,Mara Salvato,Sebastián F. Sánchez,Felipe A. Santana,Andrew K. Saydjari,Conor Sayres,Kevin C. Schlaufman,Donald P. Schneider,Axel Schwope,J. Serna,Yue-Yun Shen,Jennifer Sobeck,Yingyi Song,Diogo Souto,Taylor Spoo,Keivan G. Stassun,Matthias Steinmetz,Ilya Straumit,B. Stringfellow,Jos'e S'anchez-Gallego,Manuchehr Taghizadeh-Popp,Jamie Tayar,Aniruddha R. Thakar,Patricia B. Tissera,Andrew Tkachenko,Hector Hernandez Toledo,Benny Trakhtenbrot,Jose Gregorio Fernandez Trincado,Nicholas W. Troup,Jonathan R. Trump,Sarah Tuttle,N. Ulloa,J. A. Vázquez-Mata,Pablo Vera Alfaro,Sandro Villanova,Stefanie Wachter,Anne-Marie Weijmans,Adam Wheeler,John C. Wilson,Leigh Wojno,J. Wolf,Xiang-Xiang Xue,Jason E. Ybarra,E. Zari,Gail Zasowski +152 more
- 18 Jan 2023
TL;DR: SDSS-V as mentioned in this paper is the first one for the fifth generation of the survey and contains extensive targeting information for the two multi-object spectroscopy programs (MWM and BHM), including input catalogs and selection functions for their numerous scientific objectives.
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Runaway Young Stars in the Orion Nebula
Aidan McBride,Marina Kounkel +1 more
TL;DR: In this paper, the authors search for the pre-main sequence stars with unusually high proper motions that may be representative of a dynamical ejection from unstable young triple systems or other close three-body encounters.
20
Runaway Young Stars near the Orion Nebula
Aidan McBride,Marina Kounkel +1 more
TL;DR: In this article, the authors search for the pre-main sequence stars with unusually high proper motions that may be representative of a dynamical ejection from unstable young triple systems or other close three-body encounters.
•Posted Content
Untangling the Galaxy III: Photometric Search for Pre-main Sequence Stars with Deep Learning
TL;DR: In this article, a trained neural network model, Sagitta, was proposed to identify pre-main sequence stars and to derive their age estimates using Gaia DR2 and 2MASS photometry.
Searching for young runaways across the sky
TL;DR: In this paper , a catalog of 3354 candidate young stars within 500 kilometres of their parent associations with relative speeds of > 5 km s−1 is presented, which are homogeneously selected through performing a 2D spherical traceback of previously identified pre-main sequence candidates to various star forming regions, ensuring that the traceback age as well as the estimated age of a star is consistent with the age of the population.