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www.bing.com Bing
bing.com › ck › a?!&am...ZHktdGV4dA&ntb=1
Facebook share link - can you customize the message body text?
Feb 17, 2011 · Facebook will not allow developers pre-fill messages. Developers may customize the story by providing OG meta tags, but it's up to the user to fill the message. This is only possible ...
arxiv.org arXiv
arxiv.org › abs › 2104.06448v2
Highly structured inner planetary system debris around the intermediate age Sun-like star TYC 8830 410 1
We present detailed characterization of the extremely dusty main sequence star TYC 8830 410 1. This system hosts inner planetary system dust (Tdust~300 K) with a fractional infrared luminosity of ~1%....
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Facebook share link without JavaScript - Stack Overflow
Learn how to create a Facebook share link without using JavaScript, including tips and solutions for effective sharing.
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0310637v1
Photometric Mapping with ISOPHOT using the "P32" Astronomical Observation Template
The ``P32'' Astronomical Observation Template (AOT) provided a means to map large areas of sky (up to 45 x 45 arcmin) in the far-infrared (FIR) at high redundancy and with sampling close to the Nyquis...
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How to resolve Facebook Login is currently unavailable for this app ...
Jul 28, 2021 · In the facebook developers console for your app, go to App Review-> Permissions and Features. Set the public_profile and email to have advanced access. This will allow all facebook â...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0007001v1
Hubble Space Telescope Photometry of the Dwarf Spheroidal Galaxy ESO 410-G005
We present HST WFPC2 imaging of the nearby low-surface-brightness dwarf spheroidal galaxy ESO 410-G005, which has been resolved into stars for the first time. The resulting color-magnitude diagram for...
arxiv.org arXiv
arxiv.org › abs › 2110.10935v1
Spectral Analysis of Solar Radio Type III Bursts from 20 kHz to 410 MHz
We present the statistical analysis of the spectral response of solar radio type III bursts over the wide frequency range between 20 kHz and 410 MHz. For this purpose, we have used observations that w...
arxiv.org arXiv
arxiv.org › abs › 1302.0821v1
Measurement of the scalar polarizability within the 5P1/2-6S1/2, 410 nm transition in atomic indium
We have completed a new measurement of the Stark shift in 115In within the 410 nm 5P1/2- 6S1/2 transition. We measure the Stark shift constant to be kS= - 122.92(33)kHz/(kV/cm)^2, corresponding to a d...
arxiv.org arXiv
arxiv.org › abs › 0704.0966v1
Cluster properties from two-particle angular correlations in p+p collisions at $\sqrt{s}$ = 200 and 410 GeV
We present results on two-particle angular correlations in proton-proton collisions at center of mass energies of 200 and 410 GeV. The PHOBOS experiment at the Relativistic Heavy Ion Collider has a un...
arxiv.org arXiv
arxiv.org › abs › 1205.4257v1
Thermoelastic Properties of Olivine and Wadsleyite [Fe_x,Mg_(1-x)]_2SiO_4: Their Relationship to the 410 km Seismic Discontinuity
We combine density functional theory (DFT) within the local density approximation (LDA), the quasiharmonic approximation (QHA), and a model of vibrational density of states (VDoS) to calculate elastic...
arxiv.org arXiv
arxiv.org › abs › 1901.08485v2
Transit timing variations, radial velocities and long-term dynamical stability of the system Kepler-410
Transit timing variations of Kepler-410Ab were already reported in a few papers. Their semi-amplitude is about 14.5 minutes. In our previous paper, we found that the transit timing variations could be...
arxiv.org arXiv
arxiv.org › abs › cond-mat › 0311093v1
On-surface and Subsurface Adsorption of Oxygen on Stepped Ag(210) and Ag(410) Surfaces
The adsorption of atomic oxygen and its inclusion into subsurface sites on Ag(210) and Ag(410) surfaces have been investigated using density functional theory. We find that--in the absence of adatoms ...
arxiv.org arXiv
arxiv.org › abs › 0911.0700v1
A Multi-Wavelength Investigation of the Unidentified Gamma-Ray Source HESS J1708-410
We report on recent XMM-Newton observations, archival radio continuum and CO data, and SED modeling of the unidentified Galactic plane source HESS J1708-410. No significant extended X-ray emission is ...