1. BlackGEM (Blagorodnova).
   Wide field and shallow optical synoptic surveyor.
2. Dark Energy Camera surveys (Dawson).
   A 5-sq degree imager on a 4-m telescope. Available now for all sorts of astrophysical projects.
3. DESI (Nugent).
   Massively multiplexed (5000 channels) optical spectrograph with 8 sq degrees.
4. Gattini IR (De).
   Wide field and shallow NIR synoptic surveyer.
5. KMT Network (Sang-Chul KIM)
   A trio of 1.6-m telescopes (Chile, Australia, South Africa) equipped with moderate field (2 sq degree) fine optical imagers and optimized for 24-hour coverage of the Southern Sky (particularly the Bulge).
6. KPED (Kitt Peak Electron Multiplying CCD Demonstrator) (Coughlin & Kulkarni)).
   A dedicated optical imager suitable for fast framing (electron multiplying CCD) on the robotic Kitt Peak 84-inch telescope.
7. The Kyoto 3.8-m Telescope (Maeda).
   A spanking new, moderate size (3.8-m) fast slewing large telescope right here in Japan.
8. LAMOST (Mao).
   Large field of view (5 sq deg), massively multipliexed (4000 channels) optical spectropgrah behind 4-m Schimidt type telescope.
9. MAXI (Kawai).
   Wide field and shallow X-ray synoptic surveyor.
10. MOA (Sumi).
    A 1.8-m telescope equipped 2.2 sq degree fine optical imager, located in New Zealand, and dedicated for micro-lensing studies.
11. PFS (Yasuda).
    Moderate field (1.3 sq deg), massively multiplexed (2394) and high sensitivity 0.38-1.26 micron spectrograph on 8-m telescope.
12. PRIME (Sumi).
    A 1.8-m telescope equipped with the widest field NIR imager (1.5 sq deg) and also a spectrograph, located in South Africa.
13. SDSS Phase V (Konidaris & Kollmeier).
    The next phase of SDSS aimed at "dynamic highly multiplexed stellar and interstellar" spectroscopy.
14. SEDM (Spectral Energy Distribution Machine) (Konidaris).
    An IFU spectrograph optimised for transient classification and high operational efficiency. Presentation by the PI of SEDM.
15. SEDM: Performance & DRP (Neill).
    The current performance and data reduction pipeline (DRP) of the SEDM (after upgrade and fixes). Presentation by the Project Scientist.
16. Supernova Surveys from China (Wang).
    A variety of SN searches from China.
17. Subaru Transient Surveys (Tominaga).
    Deep (25 mag or better) nightly (including intra-night) surveys for shock breakout and super-luminous supernovae.
18. Spektr Roengten Gamma (Rau).
    Synoptic X-ray survey of the sky. Rosat on steroids. Imminent launch.
19. TESS (provided by Blagorodnova).
    Wide field and high precision survey of the bright (I<14 mag) sky. Aimed at extra-solar planes. Unique. Already working.
20. Tomo-e Gozen (provided by Tanaka).
    Wide field but second timescale survey of the optical sky. Unique. Working already.
21. Zwicky Transient Facility: Coaddition Facility (Goldstein).
    Coadding allows a good match between ZTF & DESI and perhaps even ZTF & PFS.
22. Zwicky Transient Facility: Science (Yan).
    Science from ZTF.

# For Unix aficionados: 
# Problem: how to automatically "build a book" from a website?
# (you can have any ordering by using sort but here it is by alpha)

# change directory to Files4Facilities/

$ wkhtmltopdf ../IndexedFacilities.html AAATable.pdf
$ pdfunite $(ls -1 *.pdf | xargs) ../AllFacilities.pdf