THE OLD HOST-GALAXY ENVIRONMENT OF SSS17A, THE FIRST ELECTROMAGNETIC COUNTERPART TO A GRAVITATIONAL WAVE SOURCE* ABSTRACT We pre
![A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations [GA] | arXiver A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations [GA] | arXiver](https://i0.wp.com/arxiver.moonhats.com/wp-content/uploads/2018/01/CantielloEtAl-1801.06080_f2.jpg)
A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations [GA] | arXiver
![Upper left: false-color (RGB channels corresponding to PS1 irg filters)... | Download Scientific Diagram Upper left: false-color (RGB channels corresponding to PS1 irg filters)... | Download Scientific Diagram](https://www.researchgate.net/publication/320435983/figure/fig2/AS:667626963496991@1536186080890/Upper-left-false-color-RGB-channels-corresponding-to-PS1-irg-filters-image-of-the.png)
Upper left: false-color (RGB channels corresponding to PS1 irg filters)... | Download Scientific Diagram
![Pseudo-color images of SSS17a in the galaxy NGC 4993. Images are 1 × 1... | Download Scientific Diagram Pseudo-color images of SSS17a in the galaxy NGC 4993. Images are 1 × 1... | Download Scientific Diagram](https://www.researchgate.net/profile/Eduardo_Banados/publication/320436900/figure/fig1/AS:550640138100736@1508294247137/Pseudo-color-images-of-SSS17a-in-the-galaxy-NGC-4993-Images-are-1-1-and-centered-on.png)
Pseudo-color images of SSS17a in the galaxy NGC 4993. Images are 1 × 1... | Download Scientific Diagram
![Main panel shows the first-epoch F110W HST/WFC3-IR image of the field... | Download Scientific Diagram Main panel shows the first-epoch F110W HST/WFC3-IR image of the field... | Download Scientific Diagram](https://www.researchgate.net/publication/320436295/figure/fig3/AS:667648434118656@1536191199003/Main-panel-shows-the-first-epoch-F110W-HST-WFC3-IR-image-of-the-field-of-AT2017gfo.png)