Aren N. Heinze, Ph.D. - Publications

Affiliations: 
2007 Astronomy University of Arizona, Tucson, AZ 
Area:
Astronomy and Astrophysics

15 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2015 Yang H, Apai D, Marley MS, Saumon D, Morley CV, Buenzli E, Artigau É, Radigan J, Metchev S, Burgasser AJ, Mohanty S, Lowrance PJ, Showman AP, Karalidi T, Flateau D, ... Heinze AN, et al. HST rotational spectral mapping of two L-type brown dwarfs: Variability in and out of water bands indicates high-altitude haze layers Astrophysical Journal Letters. 798. DOI: 10.1088/2041-8205/798/1/L13  0.365
2015 Heinze AN, Metchev S, Trollo J. DIGITAL TRACKING OBSERVATIONS CAN DISCOVER ASTEROIDS 10 TIMES FAINTER THAN CONVENTIONAL SEARCHES Astronomical Journal. 150. DOI: 10.1088/0004-6256/150/4/125  0.456
2015 Heinze AN, Metchev S. PRECISE DISTANCES for MAIN-BELT ASTEROIDS in only TWO NIGHTS Astronomical Journal. 150. DOI: 10.1088/0004-6256/150/4/124  0.414
2013 Heinze AN, Metchev S, Apai D, Flateau D, Kurtev R, Marley M, Radigan J, Burgasser AJ, Artigau E, Plavchan P. Weather on other worlds. I. Detection of periodic variability in the L3 dwarf DENIS-P J1058.7-1548 with precise multi-wavelength photometry Astrophysical Journal. 767. DOI: 10.1088/0004-637X/767/2/173  0.374
2010 Hinz PM, Rodigas TJ, Kenworthy MA, Sivanandam S, Heinze AN, Mamajek EE, Meyer MR. Thermal infrared MMTAO observations of the HR8799 planetary system Astrophysical Journal. 716: 417-426. DOI: 10.1088/0004-637X/716/1/417  0.637
2010 Heinze AN, Hinz PM, Kenworthy M, Meyer M, Sivanandam S, Miller D. Constraints on long-period planets from an L′- and M-band survey of nearby sun-like stars: Modeling results Astrophysical Journal. 714: 1570-1581. DOI: 10.1088/0004-637X/714/2/1570  0.696
2010 Heinze AN, Hinz PM, Sivanandam S, Kenworthy M, Meyer M, Miller D. Constraints on long-period planets from an l′- and m-band survey of nearby sun-like stars: Observations Astrophysical Journal. 714: 1551-1569. DOI: 10.1088/0004-637X/714/2/1551  0.733
2009 Kenworthy MA, Mamajek EE, Hinz PM, Meyer MR, Heinze AN, Miller DL, Sivanandam S, Freed M. MMT/AO 5 μm imaging constraints on the existence of giant planets orbiting fomalhaut at 13-40 AU Astrophysical Journal. 697: 1928-1933. DOI: 10.1088/0004-637X/697/2/1928  0.694
2009 Heinze AN, Delahunta D. The rotation period and light-curve amplitude of kuiper belt dwarf planet 136472 Makemake (2005 FY9) Astronomical Journal. 138: 428-438. DOI: 10.1088/0004-6256/138/2/428  0.361
2008 Heinze AN, Hinz PM, Kenworthy M, Miller D, Sivanandam S. Deep L′- and M-band imaging for planets around Vega and ε Eridani Astrophysical Journal. 688: 583-596. DOI: 10.1086/592100  0.713
2006 Kenworthy MA, Hinz PM, Angel JRP, Heinze AN, Sivanandam S. Whack-a-speckle: Focal plane wavefront sensing in theory and practice with a deformable secondary mirror and 5-micron camera Proceedings of Spie - the International Society For Optical Engineering. 6272. DOI: 10.1117/12.672577  0.563
2006 Sivanandam S, Hinz PM, Heinze AN, Freed M, Breuninger AH. Clio: A 3-5 micron AO planet-finding camera Proceedings of Spie - the International Society For Optical Engineering. 6269. DOI: 10.1117/12.672344  0.716
2006 Hinz PM, Heinze AN, Sivanandam S, Miller DL, Kenworthy MA, Brusa G, Freed M, Angel JRP. Thermal infrared constraint to a planetary companion of Vega with the MMT adaptive optics system Astrophysical Journal. 653: 1486-1492. DOI: 10.1086/506581  0.718
2005 Heinze AN, Hinz PM. Spectral types for four OGLE-III transit candidates: Could these be planets? Astronomical Journal. 130: 1929-1938. DOI: 10.1086/432838  0.574
2002 Heinze AN, Hinz PM, McCarthy DW. A 3-5 micron camera for extrasolar planet searches Proceedings of Spie - the International Society For Optical Engineering. 4839: 1154-1164. DOI: 10.1117/12.462962  0.707
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