Search

8 Jan 2015: given in Stark et al. (2014). A larger telescope can tol-erate larger zodi levels for the same integration time.Detections of warm dust will also reveal new informa-. ... U. 2000, in Allen’s Astrophysical. Quantities, ed. A. N. Cox (New York: AIP Press)

16 Jun 2015: between the filters’different properties.14, 15 As result of this consulation process two options were offered by Barr, one design basedon standard techniques and a second using an new filter ... 940–944, Sept. 1993. 13. S. D. Lord, “A New Software

14 Sep 2015: In this work we compare new ALMA high-frequency radio continuum observations of HD 142527,obtained at 700 GHz (ALMA band 9; wavelengths of0.43 mm, described in Appendix, Sec. ... Sec. A.1 presentsthe new ALMA observations, Sec. A.2 presents the newATCA

20 Jan 2015: New modeling based on Spitzer/IRS models and KIN observations also suggests a com-.

15 Jan 2015: obtained at two epochs separated by 15 years. The new images and the re-. ... ing Spectrograph, Woodgate et al. 1998) archival dataset and also introduce a new set of.

14 Sep 2015: Goodman2, A. Hoekstra2, K. J.Jek21Department of Astronomy, Yale University, New Haven, CT 06511, USA2Amateur Astronomer3Department of Physics, and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge,

24 Oct 2015: Box 23-141, Taipei, 106,Taiwan12 National Radio Astronomy Observatory, 1003 Lopezville Road, Socorro, New Mexico,87801, USA13 LESIA, Observatoire de Paris, 5 place J. ... The low frequency, high resolution,and excellent sensitivity of the ngVLA will open

10 Mar 2015: 10 March 2015. ABSTRACTWe present new observations of the Kuiper belt analogues around HD 38858 andHD 20794, hosts of super-Earth mass planets within 1 au. ... 2014). 3 DEBRIS DISC OBSERVATIONS. Here we present new observations of HD 38858 with sev-eral

15 Jan 2015: will characterise the exo-zodi luminosity functionwith sufficient detail to provide new information on the dustorigin and evolution.

2 Nov 2015: Road, Cambridge, UK9 Department of Astronomy, Yale University, New Haven, CT10 Visiting Astronomer, NASA Infrared Telescope Facility, op-. ... 2012), these additional pointing variationsrequire new data reduction solutions optimized for K2(e.g.,

16 Jun 2015: 2 European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile3 School of Physics, University of New South Wales, NSW 2052 Sydney, Australia4 Australian Centre for Astrobiology, University of ... New South Wales, NSW