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The Mexican Asteroid Photometry Campaigns: Aiming for Asteroids' Rotation Periods

  • W. J. Schuster
    ,
  • S. A. Ayala-Gómez
    ,
  • A. Avilés
    ,
  • M. E. Contreras
    ,
  • S. A.R. Haro-Corzo
    ,
  • P. A. Loera-González
  • Universidad Nacional Autónoma de México
    ,
  • Universidad Autonoma de Nuevo Leon
    ,
  • Universidad de Sonora
    ,
  • Universidad Autonoma de Coahuila
    ,
  • Universidad de Monterrey
    ,
  • Instituto Politécnico Nacional
Research Output:
Contribution to journal
Article
Peer-review

Sustainable Development Goals

  • SDG 3 - Good Health and Well-being
    SDG 3 Good Health and Well

Publication metrics

Metrics

SciVal
Author count
17
SciVal
Paper percentile
26

Abstract

Thousands of new asteroids are discovered every year and the rate of discovery is by far larger than the determination rate of their physical properties. In 2015 a group of researchers and students of several Mexican institutions have established an observational program to study asteroids photometrically. The program, named Mexican Asteroid Photometry Campaign, is aiming to derive rotation periods of asteroids based on optical photometric observations. Since then four campaigns have been carried out. The results obtained throughout these campaigns, as well as future work, are presented.

Publication Information

Output type

Research Output:
Contribution to journal
Article
Peer-review

Original language

English

Pages from-to (Number of pages)

Pages 35-38 (4 pages)

Journal (Volume, Issue Number)

Proceedings of the International Astronomical Union (Volume 14, Issue A30)

Publication milestones

  • Published - 01/01/2018

Publication status

Published - 01/01/2018

ISSN

1743-9213

Publication IDs

  • Scopus: 85080960594

Funding Details

WJS gratefully acknowledges financial support from the Universidad Nacional Autónoma de México, grant DGAPA-PAPIIT, project IN100918. M.E.C. acknowledges financial support from CONACyT Fellowship C-841/2018 (México). IRAF is distributed by the National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. Collaborative Asteroids Lightcurve Link (CALL) can be accessed at www.minorplanet.info/ call.html. Asteroid Lightcurve Photometry Database (ALCDEF) can be accessed at alcdef.org.
FundersFunding numbers
DGAPA-PAPIIT
IN100918
NSF
-
CONACYT
C-841/2018
UNAM
-