![Graphene Plasmonic Metasurfaces to Steer Infrared Light www.nature.com/scientificreports Zubin Li](http://s1.studyres.com/store/data/008938531_1-02a0af961f329b1f981ea012f6cbe575-300x300.png)
Graphene Plasmonic Metasurfaces to Steer Infrared Light www.nature.com/scientificreports Zubin Li
... of the dielectric spacing layer, while the amplitude of reflectivity remains high and only shows moderate variations. These two properties allow us to design a variety of planar graphene photonic devices in the reflective configuration that are easy to fabricate and integrate. It should be emphasize ...
... of the dielectric spacing layer, while the amplitude of reflectivity remains high and only shows moderate variations. These two properties allow us to design a variety of planar graphene photonic devices in the reflective configuration that are easy to fabricate and integrate. It should be emphasize ...
Simulating the outer layers of Procyon A: a comparison with the Sun
... of up to about half a local pressure scaleheight (about 500 km). By computing the FWHM of the vertical velocity, we obtain a mean granule diameter of about 10 000 km (details of how we estimate the granule diameter are given in Robinson et al. 2004), while the run of rms vertical velocity (Fig. 4) p ...
... of up to about half a local pressure scaleheight (about 500 km). By computing the FWHM of the vertical velocity, we obtain a mean granule diameter of about 10 000 km (details of how we estimate the granule diameter are given in Robinson et al. 2004), while the run of rms vertical velocity (Fig. 4) p ...
Techreportjul09 - University of Reading
... note that the value in the OPAC (Hess et al, 2008) data base of 1.74, -0.44i at 550nm, which is widely used by climate modellers) is drawn from incompletely graphitised carbon and has a lower absorption refractive index than most atmospheric soot. That study provides a range of refractive indices f ...
... note that the value in the OPAC (Hess et al, 2008) data base of 1.74, -0.44i at 550nm, which is widely used by climate modellers) is drawn from incompletely graphitised carbon and has a lower absorption refractive index than most atmospheric soot. That study provides a range of refractive indices f ...
The Herschel Orion Protostar Survey: Luminosity and Envelope
... The discovery of Class 0 objects (André et al. 1993), which were difficult to detect in the mid-IR until the launch of Spitzer, motivated additional criteria not based on the slope of the SED. The bolometric temperature Tbol , the effective temperature of a blackbody with the same mean frequency as ...
... The discovery of Class 0 objects (André et al. 1993), which were difficult to detect in the mid-IR until the launch of Spitzer, motivated additional criteria not based on the slope of the SED. The bolometric temperature Tbol , the effective temperature of a blackbody with the same mean frequency as ...
Radiation-driven wind models of massive stars
... dynamical role, as they are responsible for a large amount of momentum and energy input into the ISM due to stellar winds and supernova explosions. See Abbott (1982b) and Leitherer et al. (1992) for an overview. Moreover, as massive stars are hot, with effective temperatures in the range of about 10 ...
... dynamical role, as they are responsible for a large amount of momentum and energy input into the ISM due to stellar winds and supernova explosions. See Abbott (1982b) and Leitherer et al. (1992) for an overview. Moreover, as massive stars are hot, with effective temperatures in the range of about 10 ...
Lichtenknecker- Database of the BAV
... series of photographic pictures or visual observations. In addition reports about weak images on photographic plates are included, although these are no minimum in the proper meaning. The criteria for an inclusion of eclipsing binaries into the database are a magnitude not fainter than 13mag during ...
... series of photographic pictures or visual observations. In addition reports about weak images on photographic plates are included, although these are no minimum in the proper meaning. The criteria for an inclusion of eclipsing binaries into the database are a magnitude not fainter than 13mag during ...
The Spatial Distribution of Satellite Galaxies Ing´olfur ´ Ag´ ustsson
... ∼ 30% of the MRS host galaxies are classified as ellipticals, while the rest are classified as disk galaxies (either spiral or lenticular). See AB10 and De Lucia et al. (2006) for details of the classification scheme. In addition, we divide our sample of theoretical host galaxies according to their ...
... ∼ 30% of the MRS host galaxies are classified as ellipticals, while the rest are classified as disk galaxies (either spiral or lenticular). See AB10 and De Lucia et al. (2006) for details of the classification scheme. In addition, we divide our sample of theoretical host galaxies according to their ...
a new vla–hipparcos distance to betelgeuse and its implications
... VLBA Pie Town antenna to obtain maximum spatial resolution. As part of this radio study we have also obtained new multiepoch radio positions. In this paper we combine radio positions from our observing programs and archival data, published VLA positions, and the Hipparcos Intermediate Astrometric Da ...
... VLBA Pie Town antenna to obtain maximum spatial resolution. As part of this radio study we have also obtained new multiepoch radio positions. In this paper we combine radio positions from our observing programs and archival data, published VLA positions, and the Hipparcos Intermediate Astrometric Da ...
Testing the Initial-Final Mass Relationship of White Dwarfs Silvia Catal´ an Ruiz
... The initial-final mass relationship can be determined using two different approaches. The first approach involves an indirect measurement. This is done by studying the influence of the initial-final mass relationship in the two fundamental tools typically used to statistically analyze the properties ...
... The initial-final mass relationship can be determined using two different approaches. The first approach involves an indirect measurement. This is done by studying the influence of the initial-final mass relationship in the two fundamental tools typically used to statistically analyze the properties ...
Accretion Power in Astrophysics, Third Editiion
... The subject of this book is astrophysical accretion, especially in those circumstances where accretion is believed to make an important contribution to the total light of an astrophysical system. Our discussion therefore centres mainly on close binary systems containing compact objects and on active ...
... The subject of this book is astrophysical accretion, especially in those circumstances where accretion is believed to make an important contribution to the total light of an astrophysical system. Our discussion therefore centres mainly on close binary systems containing compact objects and on active ...
OPTICAL ELEMENTS, SYSTEMS, OR APPARATUS (G02F takes
... array, e.g. frequency selective surfaces (for use with wavelengths longer than the infra-red light H01Q 15/0006)} Definition statement This place covers: Filters in which the spectral filtering is performed by a conductive grid or mesh. The background is that for microwave optics, there has long exi ...
... array, e.g. frequency selective surfaces (for use with wavelengths longer than the infra-red light H01Q 15/0006)} Definition statement This place covers: Filters in which the spectral filtering is performed by a conductive grid or mesh. The background is that for microwave optics, there has long exi ...
Coherent Control of Atoms and Molecules
... the one I experienced. For that, my advisors Margaret Murnane and Henry Kapteyn must take a large share of the credit. They have been friends and mentors to me, allowing me to explore just about anything that interested me. In fact, we even did a few of Henry's famous "one-day" experiments in more-o ...
... the one I experienced. For that, my advisors Margaret Murnane and Henry Kapteyn must take a large share of the credit. They have been friends and mentors to me, allowing me to explore just about anything that interested me. In fact, we even did a few of Henry's famous "one-day" experiments in more-o ...
3011800000630
... Figure 1 shows the best model fit to all data. Table 1 details the features of this fit. For each band of radiation, the effective blackbody temperature representing that band and the radius R in the disk corresponding to that effective temperature were listed. The last column gives the ratio of dis ...
... Figure 1 shows the best model fit to all data. Table 1 details the features of this fit. For each band of radiation, the effective blackbody temperature representing that band and the radius R in the disk corresponding to that effective temperature were listed. The last column gives the ratio of dis ...
first results of the qa_2plates procedure
... The fist result obtained by this software has put in evidence that not all the plate pairs have given reliable results both in pipeline and in the objects matching, for which in some cases the parameters extracted from the Database are resulted completely wrong (null values or inconsistent values). ...
... The fist result obtained by this software has put in evidence that not all the plate pairs have given reliable results both in pipeline and in the objects matching, for which in some cases the parameters extracted from the Database are resulted completely wrong (null values or inconsistent values). ...
Synthetic Light Curves of Shocked Dense Circumstellar Shells
... R-band LC without the bolometric correction. We need to compare LCs in the R band (Figure 1b). We find that the numerical R-band LCs do not match the observed R-band LC even in the models which give a good fit in Figure 1a. This is simply because of high temperatures in the shell and most of the emi ...
... R-band LC without the bolometric correction. We need to compare LCs in the R band (Figure 1b). We find that the numerical R-band LCs do not match the observed R-band LC even in the models which give a good fit in Figure 1a. This is simply because of high temperatures in the shell and most of the emi ...
Femtosecond spectroscopy of solid hydrogen - diss.fu
... focused on vibrational and rotational decay times in pure solid hydrogen [29, 30], and to our knowledge, there was only one experiment with femtoseconds time resolution. The latter studied the lattice response onto an impulsive electronic excitation of an NO impurity and revealed an over damped, rat ...
... focused on vibrational and rotational decay times in pure solid hydrogen [29, 30], and to our knowledge, there was only one experiment with femtoseconds time resolution. The latter studied the lattice response onto an impulsive electronic excitation of an NO impurity and revealed an over damped, rat ...
2004 “The Physics of attosecond light pulses”
... laser media (Shank and Ippen 1974) further reduced the duration to less than 1 ps, another four orders of narrowing. The next three-order reduction took another 10–15 years to achieve. The main development was the ring cavity with intra-cavity prism compensation of the group velocity dispersion with ...
... laser media (Shank and Ippen 1974) further reduced the duration to less than 1 ps, another four orders of narrowing. The next three-order reduction took another 10–15 years to achieve. The main development was the ring cavity with intra-cavity prism compensation of the group velocity dispersion with ...
Tidal Effects on the Oort Cloud Comets and Dynamics of the Sun in
... The Solar System presents a complex dynamical structure and is not isolated from the Galaxy. In particular the comet reservoir of our planetary system, the Oort cloud, is extremely sensitive to the the galactic environment due to its peripheral collocation inside the Solar System. In this framework, ...
... The Solar System presents a complex dynamical structure and is not isolated from the Galaxy. In particular the comet reservoir of our planetary system, the Oort cloud, is extremely sensitive to the the galactic environment due to its peripheral collocation inside the Solar System. In this framework, ...
Astronomical spectroscopy
![](https://commons.wikimedia.org/wiki/Special:FilePath/Star-Spectroscope.jpg?width=300)
Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.