The faculty of language: what is it, who has it, and how did it evolve?
We argue that an understanding of the faculty of language requires substantial interdisciplinary
cooperation. We suggest how current developments in linguistics can be profitably …
cooperation. We suggest how current developments in linguistics can be profitably …
The cosmic infrared background: measurements and implications
MG Hauser, E Dwek - Annual Review of Astronomy and …, 2001 - annualreviews.org
… The stray light was demonstrated to be less than 1 nW m −2 … , with uncertainties less than a
few nW m −2 sr −1 in all bands… was ∼2 nW m −2 sr −1 at 1.25 and 2.2 μm, 0.5–1 nW m −2 sr …
few nW m −2 sr −1 in all bands… was ∼2 nW m −2 sr −1 at 1.25 and 2.2 μm, 0.5–1 nW m −2 sr …
[HTML][HTML] The mystery of language evolution
MD Hauser, C Yang, RC Berwick, I Tattersall… - Frontiers in …, 2014 - frontiersin.org
Understanding the evolution of language requires evidence regarding origins and processes
that led to change. In the last 40 years, there has been an explosion of research on this …
that led to change. In the last 40 years, there has been an explosion of research on this …
[BOOK][B] The evolution of communication
MD Hauser - 1996 - books.google.com
Bound to become a classic and to stimulate debate and research, The Evolution of Communication
looks at species in their natural environments as a way to begin to understand what …
looks at species in their natural environments as a way to begin to understand what …
Energy spectrum of cosmic-ray electrons at TeV energies
…, P Goret, C Hadjichristidis, D Hauser, M Hauser… - Physical Review Letters, 2008 - APS
The very large collection area of ground-based γ-ray telescopes gives them a substantial
advantage over balloon or satellite based instruments in the detection of very-high-energy (> …
advantage over balloon or satellite based instruments in the detection of very-high-energy (> …
The COBE diffuse infrared background experiment search for the cosmic infrared background. I. Limits and detections
MG Hauser, RG Arendt, T Kelsall, E Dwek… - The Astrophysical …, 1998 - iopscience.iop.org
… in 10 photometric bands from 1.25 to 240 μ m. The results of that search are presented here.
… at 3.5 μ m (ν I ν< 64 nW m-2 sr-1, 95% confidence level) and at 240 μ m (ν I ν< 28 nW m-2 sr-…
… at 3.5 μ m (ν I ν< 64 nW m-2 sr-1, 95% confidence level) and at 240 μ m (ν I ν< 28 nW m-2 sr-…
Complement factor H variant increases the risk of age-related macular degeneration
… We thank all of the study participants and their relatives; M. de la Paz, … Bunch for valuable
technical assistance; JM Vance and M. Summar for critical reading of the manuscript; and DJM …
technical assistance; JM Vance and M. Summar for critical reading of the manuscript; and DJM …
[HTML][HTML] The gaia mission
…, NC Hambly, DL Harrison, M Hauser… - Astronomy & …, 2016 - aanda.org
Gaia is a cornerstone mission in the science programme of the EuropeanSpace Agency (ESA).
The spacecraft construction was approved in 2006, following a study in which the original …
The spacecraft construction was approved in 2006, following a study in which the original …
Spontaneous number representation in semi–free–ranging rhesus monkeys
MD Hauser, S Carey… - Proceedings of the …, 2000 - royalsocietypublishing.org
… three apple slices plus a rock condition M), and ¢ve apple … in experiment 1 conditions K^M,
plus condition O, corresponding … each box was the same conditions K^M), the total time spent …
plus condition O, corresponding … each box was the same conditions K^M), the total time spent …
[HTML][HTML] Gaia data release 1-summary of the astrometric, photometric, and survey properties
…, NC Hambly, DL Harrison, M Hauser… - Astronomy & …, 2016 - aanda.org
Context. At about 1000 days after the launch of Gaia we present the first Gaia data release,
Gaia DR1, consisting of astrometry and photometry for over 1 billion sources brighter than …
Gaia DR1, consisting of astrometry and photometry for over 1 billion sources brighter than …