Asteroid phase curves from ATLAS dual-band photometry

[1]  J. Masiero,et al.  NEOSM Survey Cadence and Simulation , 2020 .

[2]  A. Rivkin,et al.  Twenty Years of SpeX: Accuracy Limits of Spectral Slope Measurements in Asteroid Spectroscopy , 2020, The Astrophysical Journal Supplement Series.

[3]  H. Flewelling,et al.  Investigating Taxonomic Diversity within Asteroid Families through ATLAS Dual-band Photometry , 2020, The Astrophysical Journal Supplement Series.

[4]  Michael Mommert,et al.  sbpy: A Python module for small-body planetary astronomy , 2019, J. Open Source Softw..

[5]  M. Birlan,et al.  Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS) , 2019, Icarus.

[6]  J. Licandro,et al.  Taxonomic classification of asteroids based on MOVIS near-infrared colors , 2018, Astronomy & Astrophysics.

[7]  E. Wright,et al.  A Family-based Method of Quantifying NEOWISE Diameter Errors , 2018, The Astronomical Journal.

[8]  B. Stalder,et al.  ATLAS: A High-cadence All-sky Survey System , 2018, 1802.00879.

[9]  Benoit Carry,et al.  Solar System Science with ESA Euclid , 2017, 1711.01342.

[10]  M. Kaasalainen,et al.  Adaptive optics and lightcurve data of asteroids: twenty shape models and information content analysis , 2017, 1708.05191.

[11]  R. C. Domingos,et al.  The asteroid population in g-type non-linear secular resonances , 2017 .

[12]  J. Licandro,et al.  Near-infrared colors of minor planets recovered from VISTA - VHS survey (MOVIS) , 2016, 1605.05594.

[13]  John Salvatier,et al.  Probabilistic programming in Python using PyMC3 , 2016, PeerJ Comput. Sci..

[14]  K. Muinonen,et al.  H, G1, G2 photometric phase function extended to low-accuracy data , 2016 .

[15]  K. Muinonen,et al.  Asteroid observations at low phase angles. IV: Average parameters for the new H, G1, G2 magnitude system , 2016 .

[16]  H. Campins,et al.  Spectral variability on primitive asteroids of the Themis and Beagle families: Space weathering effects or parent body heterogeneity? , 2016, 1601.05277.

[17]  S. Urakawa,et al.  Against the biases in spins and shapes of asteroids , 2015, 1711.02429.

[18]  T. Grav,et al.  NEOWISE REACTIVATION MISSION YEAR ONE: PRELIMINARY ASTEROID DIAMETERS AND ALBEDOS , 2015, 1509.02522.

[19]  W. Burgett,et al.  Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 – Preliminary results , 2015, 1506.00762.

[20]  Andrea Milani,et al.  Asteroid family ages , 2015, 1504.05461.

[21]  B. Buratti,et al.  Asteroid Photometry , 2015, 1502.06302.

[22]  Richard Greenberg,et al.  Collisional family structure within the Nysa–Polana complex , 2015, 1501.04649.

[23]  J. Carvano,et al.  Shape and solar phase angle effects on the taxonomic classification of asteroids , 2014 .

[24]  J. Masiero,et al.  MAIN-BELT ASTEROIDS WITH WISE/NEOWISE: NEAR-INFRARED ALBEDOS , 2014, 1406.6645.

[25]  M. Barucci,et al.  Aqueous alteration on main belt primitive asteroids: Results from visible spectroscopy☆ , 2014, 1402.0175.

[26]  Alberto Cellino,et al.  Asteroid families classification: Exploiting very large datasets , 2013, 1312.7702.

[27]  Francesca DeMeo,et al.  The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys , 2013, 1307.2424.

[28]  J. Masiero,et al.  ASTEROID FAMILY IDENTIFICATION USING THE HIERARCHICAL CLUSTERING METHOD AND WISE/NEOWISE PHYSICAL PROPERTIES , 2013, 1305.1607.

[29]  V. Carruba An analysis of the Hygiea asteroid family orbital region , 2013 .

[30]  Paolo Tanga,et al.  Asteroid spectroscopy with Gaia , 2012 .

[31]  A. Rivkin The fraction of hydrated C-complex asteroids in the asteroid belt from SDSS data , 2012 .

[32]  E. Solano,et al.  SVO Filter Profile Service Version 1.0 , 2012 .

[33]  Paul Mann,et al.  Phase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classification , 2012, 1205.0248.

[34]  D. A. Oszkiewicz,et al.  Asteroid taxonomic signatures from photometric phase curves , 2012, 1202.2270.

[35]  T. B. Spahr,et al.  MAIN BELT ASTEROIDS WITH WISE/NEOWISE. I. PRELIMINARY ALBEDOS AND DIAMETERS , 2011, 1109.4096.

[36]  David E. Trilling,et al.  Online multi-parameter phase-curve fitting and application to a large corpus of asteroid photometric data , 2011 .

[37]  John L. Tonry,et al.  An Early Warning System for Asteroid Impact , 2010, 1011.1028.

[38]  Karri Muinonen,et al.  A three-parameter magnitude phase function for asteroids , 2010 .

[39]  A. Nathues Spectral study of the Eunomia asteroid family Part II: The small bodies , 2010 .

[40]  Mikko Kaasalainen,et al.  DAMIT: a database of asteroid models , 2010 .

[41]  P. H. Hasselmann,et al.  SDSS-based taxonomic classification and orbital distribution of main belt asteroids , 2010 .

[42]  Donald W. Sweeney,et al.  LSST Science Book, Version 2.0 , 2009, 0912.0201.

[43]  Richard P. Binzel,et al.  An extension of the Bus asteroid taxonomy into the near-infrared , 2009 .

[44]  Petr Pravec,et al.  The asteroid lightcurve database , 2009 .

[45]  A. J. Connolly,et al.  Solar System Science with LSST , 2008 .

[46]  F. Velichko,et al.  Asteroid observations at low phase angles: III. Brightness behavior of dark asteroids , 2008 .

[47]  Zeljko Ivezic,et al.  The Size Distributions of Asteroid Families in the SDSS Moving Object Catalog 4 , 2008, 0807.3762.

[48]  Benoit Carry,et al.  A Service of Position and Physical Ephemerides Computation Dedicated to the Small Bodies of the Solar System , 2008 .

[49]  Fernando Roig,et al.  Reanalysis of asteroid families structure through visible spectroscopy , 2005 .

[50]  Walter A. Siegmund,et al.  Design of the Pan‐STARRS telescopes , 2004 .

[51]  R. Lupton,et al.  Color Variability of Asteroids in SDSS Moving Object Catalog , 2003, astro-ph/0309112.

[52]  S. Kaasalainen,et al.  Asteroid photometric and polarimetric phase curves: empirical interpretation , 2003 .

[53]  J. Piironen,et al.  The Opposition Effect and Negative Polarization of Structural Analogs for Planetary Regoliths , 2002 .

[54]  S. Kaasalainen,et al.  Asteroid photometric and polarimetric phase curves: empirical modeling , 2002 .

[55]  J. Brinkmann,et al.  Color Confirmation of Asteroid Families , 2002, astro-ph/0208098.

[56]  Richard P. Binzel,et al.  Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: A Feature-Based Taxonomy , 2002 .

[57]  Y. Krugly,et al.  Asteroid Observations at Low Phase Angles: II. 5 Astraea, 75 Eurydike, 77 Frigga, 105 Artemis, 119 Althaea, 124 Alkeste, and 201 Penelope , 2002 .

[58]  Alan W. Harris,et al.  Asteroids in the Thermal Infrared , 2002 .

[59]  I. Belskaya,et al.  Opposition Effect of Asteroids , 2000 .

[60]  A. Milani,et al.  Synthetic Proper Elements for Outer Main Belt Asteroids , 2000 .

[61]  G. Neukum,et al.  Asteroid observations at low phase angles. I. 50 Virginia, 91 Aegina and 102 Miriam☆ , 1997 .

[62]  Alberto Cellino,et al.  Maria's Family: Physical Structure and Possible Implications for the Origin of Giant NEAs , 1997 .

[63]  Andrea Milani,et al.  Asteroid proper elements and secular resonances , 1992 .

[64]  Alberto Cellino,et al.  Asteroid Families. I. Identification by Hierarchical Clustering and Reliability Assessment , 1990 .

[65]  J. Williams,et al.  A Three-Parameter Asteroid Taxonomy , 1989 .

[66]  Alan W. Harris,et al.  Application of photometric models to asteroids. , 1989 .

[67]  E. Bowell,et al.  Modelling asteroid brightness variations. II - The interpretability of light curves and phase curves , 1989 .

[68]  Robert Connelly,et al.  Convex profiles from asteroid lightcurves , 1983 .

[69]  J. Peacock Two-dimensional goodness-of-fit testing in astronomy , 1983 .

[70]  J. Surdej,et al.  Asteroid lightcurves simulated by the rotation of a three-axes ellipsoid model. , 1978 .

[71]  T. Gehrels Photometric Studies of Asteroids. V. The Light-Curve and Phase Function of 20 Massalia. , 1956 .