A recent history of science cases for optical interferometry

Optical long-baseline interferometry is a unique and powerful technique for astronomical research. Since the 1980’s (with I2T, GI2T, Mark I to III, SUSI, ...), optical interferometers have produced an increasing number of scientific papers covering various fields of astrophysics. As current interferometric facilities are reaching their maturity, we take the opportunity in this paper to summarize the conclusions of a few key meetings, workshops, and conferences dedicated to interferometry. We present the most persistent recommendations related to science cases and discuss some key technological developments required to address them. In the era of extremely large telescopes, optical long-baseline interferometers will remain crucial to probe the smallest spatial scales and make breakthrough discoveries.

[1]  C. Aerts,et al.  Echography of young stars reveals their evolution , 2014, Science.

[2]  William J. Chaplin,et al.  Asteroseismology of Solar-Type and Red-Giant Stars , 2013, 1303.1957.

[3]  Howard Isaacson,et al.  FUNDAMENTAL PROPERTIES OF KEPLER PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY , 2013, 1302.2624.

[4]  Andrea Richichi,et al.  The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation , 2008 .

[5]  Andrea M. Ghez,et al.  LUMINOSITY-VARIATION INDEPENDENT LOCATION OF THE CIRCUM-NUCLEAR, HOT DUST IN NGC 4151 , 2010, 1003.4757.

[6]  D. Dravins,et al.  Long-baseline optical intensity interferometry: Laboratory demonstration of diffraction-limited imaging , 2015, 1506.05804.

[7]  N. Scott,et al.  First fringes on the sky with an upconversion interferometer tested on a telescope Array , 2016 .

[8]  J. Sturmann,et al.  No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry , 2016, Nature.

[9]  Oliver P. Lay,et al.  Status of the Terrestrial Planet Finder Interferometer (TPF-I) , 2006, SPIE Astronomical Telescopes + Instrumentation.

[10]  O. Absil,et al.  SOUTHERN MASSIVE STARS AT HIGH ANGULAR RESOLUTION: OBSERVATIONAL CAMPAIGN AND COMPANION DETECTION , 2014, 1409.6304.

[11]  Heidelberg,et al.  The dusty torus in the Circinus galaxy: a dense disk and the torus funnel , 2013, 1312.4534.

[12]  P. Giommi,et al.  The PLATO 2.0 mission , 2013, 1310.0696.

[13]  A. Michelson,et al.  Measurement of the Diameter of Alpha-Orionis by the Interferometer. , 1921, Proceedings of the National Academy of Sciences of the United States of America.

[14]  Mark Clampin,et al.  Transiting Exoplanet Survey Satellite , 2014, 1406.0151.

[15]  J. Surdej,et al.  Colloquium recommendations: next steps into the future , 2014, IPCO 2014.

[16]  Walter Jaffe,et al.  DUST EMISSION FROM A PARSEC-SCALE STRUCTURE IN THE SEYFERT 1 NUCLEUS OF NGC 4151 , 2009, 0909.5191.

[17]  P. Véron,et al.  A catalogue of quasars and active nuclei: 13th edition , 2010 .

[18]  Walter Jaffe,et al.  Resolving the obscuring torus in NGC 1068 with the power of infrared interferometry: revealing the inner funnel of dust , 2009, 0901.1306.

[19]  L. Woltjer,et al.  Optical Telescopes of the Future , 1984 .

[20]  Antoine Labeyrie,et al.  Resolved imaging of extra-solar planets with future 10 100 km optical interferometric arrays , 1996, astro-ph/9602093.

[21]  Takayuki Kotani,et al.  Exploring the inner region of type 1 AGNs with the Keck interferometer , 2009, 0911.0666.

[22]  MPE,et al.  DUST IN THE POLAR REGION AS A MAJOR CONTRIBUTOR TO THE INFRARED EMISSION OF ACTIVE GALACTIC NUCLEI , 2013, 1306.4312.

[23]  C. Aerts The age and interior rotation of stars from asteroseismology , 2015, 1503.06690.

[24]  G. Meynet,et al.  Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass , 2016, Astronomy & Astrophysics.

[25]  Albert A. Michelson,et al.  Measurement of Jupiter's Satellites by Interference , 1891, Nature.

[26]  Observatoire de la Cote d'Azur,et al.  Resolving the complex structure of the dust torus in the active nucleus of the Circinus galaxy , 2007, 0709.0209.

[27]  S. T. Ridgway,et al.  First Results from the CHARA Array. II. A Description of the Instrument , 2005 .

[28]  K. Menten,et al.  A hot compact dust disk around a massive young stellar object , 2010, Nature.

[29]  F. Millour,et al.  VLTI/AMBER observations of the Seyfert nucleus of NGC 3783 , 2012, 1204.6122.

[30]  Konrad Tristram,et al.  PARSEC-SCALE DUST EMISSION FROM THE POLAR REGION IN THE TYPE 2 NUCLEUS OF NGC 424 , 2012, 1206.4307.

[31]  M.Swain,et al.  Interferometer Observations of Subparsec-Scale Infrared Emission in the Nucleus of NGC 4151 , 2003 .

[32]  R. Antonucci Astrophysics: Quasars still defy explanation , 2013, Nature.

[33]  C. Aerts,et al.  The Interior Angular Momentum of Core Hydrogen Burning Stars from Gravity-mode Oscillations , 2017, 1709.01874.

[34]  M. Schoeller,et al.  The central dusty torus in the active nucleus of NGC 1068 , 2004, Nature.

[35]  Jean Surdej,et al.  Science cases for next generation optical/infrared interferometric facilities (the post VLTI era) : Proceedings of the 37th Liège International Astrophysical Colloquium, 23-25 August 2004 , 2005 .

[36]  James C. Marr,et al.  Space interferometry mission (SIM): overview and current status , 2003, SPIE Astronomical Telescopes + Instrumentation.

[37]  L. Gizon,et al.  Local Helioseismology , 2005 .

[38]  Gerd Weigelt,et al.  The innermost dusty structure in active galactic nuclei as probed by the Keck interferometer , 2010, 1012.5359.

[39]  Gerd Weigelt,et al.  A diversity of dusty AGN tori - Data release for the VLTI/MIDI AGN Large Program and first results for 23 galaxies , 2013, 1307.2068.

[40]  C. Evans,et al.  Binary Interaction Dominates the Evolution of Massive Stars , 2012, Science.

[41]  Max-Planck-Institut fur Radioastronomie,et al.  Revealing the large nuclear dust structures in NGC 1068 with MIDI/VLTI , 2014, 1401.3248.

[42]  Florentin Millour,et al.  Mapping the radial structure of AGN tori , 2011, 1110.4290.

[43]  John D. Monnier,et al.  Contemporaneous Imaging Comparisons of the Spotted Giant σ Geminorum Using Interferometric, Spectroscopic, and Photometric Data , 2017, 1709.10109.

[44]  S. Rabien,et al.  First light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope Interferometer , 2017, 1705.02345.

[45]  Heidelberg,et al.  Resolving the innermost parsec of Centaurus A at mid-infrared wavelengths , 2007, 0707.0177.

[46]  Romain Petrov,et al.  Science cases for a visible interferometer , 2017, 1703.02395.

[47]  G. Weigelt,et al.  VLTI/VINCI observations of the nucleus of NGC 1068 using the adaptive optics system MACAO , 2004 .

[48]  Bruno Lopez,et al.  An Overview of the MATISSE Instrument — Science, Concept and Current Status , 2014 .

[49]  Karine Perraut,et al.  SPICA, Stellar Parameters and Images with a Cophased Array: a 6T visible combiner for the CHARA array. , 2017, Journal of the Optical Society of America. A, Optics, image science, and vision.

[50]  First On-Sky Fringes with an Up-Conversion Interferometer Tested on a Telescope Array. , 2016, Physical review letters.

[51]  A. Labeyrie,et al.  Hypertelescopes: The Challenge of Direct Imaging at High Resolution , 2013, New Concepts in Imaging: Optical and Statistical Models.

[52]  L M Mugnier,et al.  Darwin--a mission to detect and search for life on extrasolar planets. , 2009, Astrobiology.

[53]  Gerd Weigelt,et al.  VLTI/AMBER differential interferometry of the broad-line region of the quasar 3C273 , 2014, Other Conferences.

[54]  Pierre Léena,et al.  The Early Days of the Very Large Telescope Interferometer , 2007 .

[55]  Jean Surdej,et al.  Technology Roadmap for Future Interferometric Facilities Proceedings of the European Interferometry Initiative Workshop organized in the context of the 20005 Joint European and National Astronomy Meeting "Distant Worlds"? , 2005 .