Fig. 3 Near-infrared spectrum of EM at 4.5 days after merger.

Slides:

Advertisements

Similar presentations

Cold Spots on Saturn P.A. Yanamandra-Fisher (JPL), G.S. Orton, B.M. Fisher, A. Sanchez- Lavega P.A. Yanamandra-Fisher et al. 2001, Icarus, 150, 189.

Advertisements

Hydrogen Peroxide on Mars Th. Encrenaz 1, B. Bezard, T. Greathouse, M. Richter, J. Lacy, S. Atreya, A. Wong, S. Lebonnois, F. Lefevre, F. Forget 1 Observatoire.

Metr Lab #9 Satellite Imagery. The visible spectrum covers less than half an octave.

Electromagnetic Radiation. Is light a wave or a particle? Yes It’s both, and neither At atomic scales, we have no exact analogs for phenomena For some.

Atmosphere ASTR 3010 Lecture 5 not from the Textbook.

Subaru HDS Transmission Spectroscopy of the Transiting Extrasolar Planet HD b The University of Tokyo Norio Narita collaborators Yasushi Suto, Joshua.

The Interstellar Medium. Red, White, and Blue : Nebulae.

The Electromagnetic Spectrum Scripps Classroom Connection

Figure 1. Left – a small region of a typical polarized spectrum acquired with the ESPaDOnS instrument during the MiMeS project. This figure illustrates.

From: Discovery of carbon-rich Miras in the Galactic bulge

الإشعاع الكهرومغناطيسي ووسائل الاستشعار عن بعد

Regional climate and development.

Radiation in the Atmosphere

Modulation of Neuronal Interactions Through Neuronal Synchronization

CH 3: The Electromagnetic Spectrum

The circadian clock modulates the size control in 12:12 LD cycles.

Andrea Benucci, Robert A. Frazor, Matteo Carandini Neuron

Quantum squeezing of motion in a mechanical resonator

Volume 98, Issue 8, Pages (April 2010)

Direct imaging discovery of a Jovian exoplanet within a triple-star system by Kevin Wagner, Dániel Apai, Markus Kasper, Kaitlin Kratter, Melissa McClure,

Orbital Identification of Carbonate-Bearing Rocks on Mars

The University of Tokyo Norio Narita

Quasar quartet embedded in giant nebula reveals rare massive structure in distant universe by Joseph F. Hennawi, J. Xavier Prochaska, Sebastiano Cantalupo,

Trichromatic theory can explain foveal measurements.

Fig. 2 Rydberg-EIT spectra without control pulse.

by Naoki Uchida, Takeshi Iinuma, Robert M

Fig. 3 Comparison between predicted change in DT since the LIG and observed sea-level highstands. Comparison between predicted change in DT since the LIG.

Fig. 1 Pump-probe signatures of vermilion (red HgS), black HgS, and metallic Hg. Pump-probe signatures of vermilion (red HgS), black HgS, and metallic.

Fig. 3 Critical pressure analysis for reentrant and doubly reentrant geometries. Critical pressure analysis for reentrant and doubly reentrant geometries.

Fig. 3 Near-field maps of a multiply cracked α-(BEDT-TTF)2I3 crystal.

Fig. 3 Electron PSD in various regions.

Fig. 4 Twist grain boundary free energies as a function of misalignment angle for the (110)-(100) crystal planes of a nanocrystal with 1135 atoms. Twist.

Fig. 1 Mean swarm response to an oscillating swarm marker.

Fig. 1 CFHT photometry converted into spectral reflectivity obtained on UT (Universal Time) 22 and 25 October 2014, is shown in comparison to the VLT reflectivity.

Fig. 1 Study area and field site setting.

Fig. 2 Full-frame images recording the violation of a Bell inequality in four images. Full-frame images recording the violation of a Bell inequality in.

Destabilization of the WAIS in the unperturbed reference simulation

Fig. 2 Time series of ice loss from the Amundsen Sea sector for the cases of unperturbed destabilization (black) and mass deposition (colored). Time series.

Drug response profiles and experimental validation.

Fig. 4 The results of HRTEM and high-angle annular dark-field scanning TEM investigations. The results of HRTEM and high-angle annular dark-field scanning.

Fig. 2 Four types of MJO propagation patterns along the equator.

Fig. 1 Fluctuation-induced dynamic response patterns.

Fig. 3 1D NMR. 1D NMR. Time-domain (left) and frequency-domain (right) NV NMR signals for (A) water, (B) trimethyl phosphate (TMP), and (C) 1,4-difluorobenzene.

Fig. 1 Localization of GW and associated transient EM

Fig. 4 Model of the average SSE.

Fig. 2 EUV TG signal. EUV TG signal. Black lines in (A), (B), and (C) are the EUV TG signals from Si3N4 membranes at LTG = 110, 85, and 28 nm, respectively,

Fig. 4 EUV TG signal from Si.

Fig. 3 Classification of gene essentiality by transposon mutagenesis.

Fig. 2 Nucleation is maintained but spreading is inhibited by roscovitine treatment. Nucleation is maintained but spreading is inhibited by roscovitine.

Fig. 3 ET dynamics on the control and treatment watersheds during the pretreatment and treatment periods. ET dynamics on the control and treatment watersheds.

ALMA detection and astrobiological potential of vinyl cyanide on Titan

by Toan Trong Tran, Blake Regan, Evgeny A

Fig. 5 Weakened Atlantic Niño–Pacific teleconnection in the CAM3

Fig. 1 HST/STIS spectra showing a distinct 450nm spectral feature, consistent with an NaCl F-center absorption, and a clear lack of a 720nm NaCl M-center.

Relationships between species richness and temperature or latitude

Fig. 2 Comparison of the observed DRs and the estimates by the VR model and FL. Comparison of the observed DRs and the estimates by the VR model and FL.

Fig. 3 Comparisons of NDVI trends over the globally vegetated areas from 1982 to Comparisons of NDVI trends over the globally vegetated areas from.

Fig. 1 ALMA spectra showing three detected transitions of C2H3CN.

Fig. 1 Sketch and schematic diagram of photobleaching reaction in a strongly coupled system. Sketch and schematic diagram of photobleaching reaction in.

Fig. 2 Proton spectrum from 40 GeV to 100 TeV measured with DAMPE (red filled circles). Proton spectrum from 40 GeV to 100 TeV measured with DAMPE (red.

Fig. 2 OH formation and speciation in the PAA – Fe(II) system.

Fig. 3 Interference of quantum clocks.

Fig. 2 Computational modeling indicates that solid particles ricochet off manta ray filter lobes. Computational modeling indicates that solid particles.

Fig. 3 X-ray ptychography and STXM absorption spectromicroscopy.

Fig. 10 Map of light pollution’s visual impact on the night sky.

The combined signal spectra of PSD for protons and helium nuclei

Fig. 1 X-ray structures of the ScoI·Cu2+ and CoxB·CuA holo-proteins, and formation of the ScoI·Cu2+·CoxB complex. X-ray structures of the ScoI·Cu2+ and.

Percentage of papers containing inappropriate image duplications by year of publication. Percentage of papers containing inappropriate image duplications.

Fig. 5 Schematics illustrating enhancement in April tornado activity due to SST. Schematics illustrating enhancement in April tornado activity due to SST.

Fig. 4 Color modulation of fungal bioluminescence.

Presentation transcript:

Fig. 3 Near-infrared spectrum of EM170817 at 4.5 days after merger. Near-infrared spectrum of EM170817 at 4.5 days after merger. For display purposes, the data have been smoothed using a Savitzky-Golay filter (black line), and the unfiltered data are shown in gray. A predicted model macronova spectrum (23) assuming an ejecta mass of Mej = 0.05 M☉ and a velocity of v = 0.1c at a phase of 4.5 days post-merger is shown in red. The spectra have been corrected for Milky Way extinction assuming reddening E(B – V) = 0.1 (10). Regions of low signal-to-noise ratio from strong telluric absorption by Earth’s atmosphere between the near-infrared J, H, and K spectral windows are indicated by the vertical dark gray bars. The light gray shaded band is the blackbody that best fits the photometric measurements at 4.5 days (10). M. M. Kasliwal et al. Science 2017;358:1559-1565 Copyright © 2017, American Association for the Advancement of Science