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18 KiB
18 KiB
1 | ABBR | TERM |
---|---|---|
2 | 21CSLC | 21st Century Space Launch Complex |
3 | 4LGSF | Four-Laser Guide Star Facility |
4 | 4MOST | 4-metre Multi-Object Spectroscopic Telescope (Proposed new spectroscopic instrument for VISTA) |
5 | 4T | Four Telescope (VLTI mode) |
6 | A&A | Journal, Astronomy & Astrophysics |
7 | A&ARv | Journal, Annual Review of Astronomy and Astrophysics |
8 | ACD | Amplitude Calibration Device (ALMA) |
9 | ACe | Astaldi Cimolai EIE (Consortium) |
10 | ADA | ALMA Department of Administration |
11 | ADO | ALMA Director’s Office |
12 | ADS | International Italian optics company working on the DSM for the VLT |
13 | AEM | ALMA construction consortium |
14 | AFNOR | Association Française de Normalisation |
15 | AFTA | Astrophysics Focused Telescope Assets |
16 | AGN | Active Galactic Nucleus |
17 | AIDA | Astronomical Infrastructure for Data Access |
18 | AIP | Leibniz Institute for Astrophysics Potsdam |
19 | AIT | Assembly, Integration and Test |
20 | AIV | Assembly, Integration and Verification |
21 | AJ | The Astronomical Journal |
22 | ALMA | Atacama Large Millimeter/submillimeter Array |
23 | AMBER | Astronomical Multi-BEam combineR (VLTI Instrument) |
24 | AN | Journal, Astronomische Nachrichten |
25 | Antu | VLT Unit Telescope 1 |
26 | AO | Adaptive Optics |
27 | AOF | Adaptive Optics Facility |
28 | AOS | Array Operations Site (ALMA) |
29 | APE | Active Phasing Experiment |
30 | APEX | Atacama Pathfinder Experiment |
31 | ApJ | Astrophysical Journal |
32 | ApJS | Journal, Astrophysical Journal Supplement Series |
33 | AQUARIUS | Mid-infrared detector array (VISIR) |
34 | ARAL | Alignment facility for the VLTI |
35 | ARC | ALMA Regional Centre |
36 | ArTeMiS | Bolometric camera for APEX |
37 | ASAC | ALMA Science Advisory Committee |
38 | ASIAA | East Asia FEIC (ALMA) |
39 | ASIC | Application Specific Integrated Circuit |
40 | ASSIST | Adaptive Secondary Setup and Instrument Simulator (AOF test bench) |
41 | AstraLux | Lucky Imaging camera for the Calar Alto 2.2-metre telescope |
42 | AT | Auxiliary Telescope for the VLTI |
43 | ATC | Astronomy Technology Centre (United Kingdom) |
44 | ATILO | Administrative Tribunal of the International Labour Organisation |
45 | AU | Astronomical Unit |
46 | AUI | Associated Universities Inc. |
47 | AVM | Astronomical Visualisation Metadata |
48 | BAM | Construction company for the Headquarters extension |
49 | BE | Back-End (ALMA) |
50 | BELLA | Building Europe Link to Latin America |
51 | BFL | Budget and Forward Look |
52 | BlackGEM | (La Silla) Telescope array searching for optical counterparts of gravitational wave sources |
53 | BLIP | Background photon noise limited |
54 | C2PAP | Computational Center for Particle and Astrophysics, Universe Cluster, Garching |
55 | CAD | Computer Aided Design |
56 | CADC | Canadian Astronomy Data Centre |
57 | CAPj | Communicating Astronomy with the Public Journal |
58 | CARLA | Clusters Around Radio-Loud AGN (Spitzer) |
59 | CASA | Common Astronomy Software Applications (ALMA) |
60 | CCD | Charge Coupled Device |
61 | CCTV | Closed Circuit TeleVision |
62 | CDR | Critical Design Review |
63 | CDS | Centre de Données astronomiques de Strasbourg (Strasbourg astronomical Data Center) |
64 | CEA | Commissariat à L’Energie Atomique, France |
65 | CELAC_EU | Summit of the Community of Latin American and Caribbean States–European Union |
66 | CES | Coude Echelle Spectrometer |
67 | CfP | Call for Proposal |
68 | CfT | Call for tender |
69 | CHAMP+ | Dual channel heterodyne receiver array (APEX) |
70 | CLIF | Convolution with Linearized Inverse Filter algorithm for wavefront sensing |
71 | CLP | Chilean Peso |
72 | CMB | Cosmic Microwave Background |
73 | CMBR | Cosmic Microwave Background Radiation |
74 | CME | Coronal Mass Ejection (usually Sun) |
75 | CNAM | Conservatoire National des Arts et Métiers |
76 | CNRS | Centre national de la recherche scientifique |
77 | CO | Carbon monoxide |
78 | CO | Carried Over budget |
79 | COFUND | EU fellowship funding programme |
80 | CONDOR | 1.5 THz heterodyne receiver (APEX) |
81 | CONICA | COudé Near-Infrared CAmera (VLT) |
82 | CORALIE | Echelle Spectrograph on the 1.2-metre Leonard Euler Swiss telescope |
83 | CoRoT | COnvection ROtation and planetary Transits (French Satellite) |
84 | COSMOS | HST survey programme |
85 | Cou- | Council Document |
86 | CP | Calibration Programme |
87 | CPI | Consumer Price Index |
88 | CRIRES+ | Planned upgrade to CRIRES |
89 | CRIRES | Cryogenic InfraRed Echelle Spectrometer (VLT) |
90 | CSV | Commissioning and Science Verification |
91 | CTA | Cherenkov Telescope Array |
92 | CTA-S | Cherenkov Telescope Array South |
93 | CTAO | Cherenkov Telescope Array Observatory |
94 | CUBES | Cassegrain U-band Brazilian ESO Spectrograph |
95 | CuRe | Fast wavefront reconstruction algorithms for XAO with pyramid WFS |
96 | CuReD | Fast wavefront reconstruction algorithms for XAO with pyramid WFS with pre-processing |
97 | DC | Direct Current |
98 | DDS | Data DistributIOn middleware for SPARTA |
99 | DDT | Director’s Discretionary Time |
100 | DFG | Deutsche Forschungsgemeinschaft |
101 | DFS | (VLT) Data Flow System |
102 | DG | Director General |
103 | DIG | Deep Imaging Group (Vitacura) |
104 | DL | Delay Line (VLTI) |
105 | DMO | Data Management and Operations Division |
106 | DMS | Dome and Main Structure |
107 | DRS | DRS, formerly Boeing, detector manufacturer |
108 | DSC | Directorate for Science |
109 | DSM | Deformable Secondary Mirror |
110 | DSO | Department of Science Operations (ALMA) |
111 | eAPD | electron Avalanche Photodiode Detector |
112 | EASC | European ALMA Support Centre |
113 | EC | European Commission |
114 | ECRI | European Conference on Research Infrastructures |
115 | EFOSC2 | ESO Faint Object Spectrograph and Camera (v.2) |
116 | EIB | European Investment Bank |
117 | EIROforum | Organisation consisting of the seven largest scientific European international organisations devoted to fostering mutual activities |
118 | ELT | Extremely Large Telescope |
119 | EM&P | Journal, Earth, Moon, and Planets |
120 | EMAC | ELT Management Advisory Committee |
121 | EMBL | European Molecular Biology Laboratory (Germany) |
122 | EMMI | ESO Multi-Mode Instrument (NTT) |
123 | ePOD | education and Public Outreach Department |
124 | ERC | European Research Council |
125 | ERIS | Enhanced Resolution Imager and Spectrograph |
126 | ERP | Enterprise Resource Planning (Administration software) |
127 | ESAC | European Science Advisory Committee (for ALMA) |
128 | ESAC | European Space Astronomy Centre (ESA, Spain) |
129 | ESC | ELT Subcommittee |
130 | ESE | ELT Science and Engineering |
131 | ESM | European School Munich |
132 | ESO | European Organisation for Astronomical Research in the Southern Hemisphere |
133 | ESOF | Euroscience Open Forum |
134 | ESON | ESO Science Outreach Network |
135 | ESPRESSO | Echelle SPectrograph for Rocky Exoplanet- and Stable Spectroscopic Observations |
136 | ESRC | ELT Standing Review Committee |
137 | ETF | ELT Technical Facility |
138 | EVALSO | Enabling Virtual Access to Latin-american Southern Observatories |
139 | EWASS | European Week of Astronomy and Space Science |
140 | ExA | Journal, Experimental Astronomy |
141 | ExTrA | (La Silla) Exoplanets in Transit and their Atmospheres |
142 | FC | Finance Committee |
143 | FDR | Final Design Review |
144 | FE IPT | Front-End Integrated Project Team (ALMA) |
145 | FE | Front End |
146 | FEA | Finite Element Analysis |
147 | FEED | Front-End Engineering Design (ELT) |
148 | FEIC | Front End Integration Centre (ALMA) |
149 | FEROS | Fibre-fed, Extended Range, Échelle Spectrograph (MPG/ESO 2.2-metre) |
150 | FIAT | Facility (for) Infrared Arrays Testing |
151 | FITS | Flexible Image Transport System |
152 | FLAMES | Fibre Large Array Multi Element Spectrograph (VLT) |
153 | FORS1 | FOcal Reducer/low dispersion Spectrograph (VLT)-1 |
154 | FORS2 | FOcal Reducer/low dispersion Spectrograph (VLT)-2 |
155 | FOS | Faint Object Spectrograph (HST) |
156 | FP | Fabry-Perot |
157 | FP6 | Sixth EC Framework Programme |
158 | FP7 | Seventh EC Framework Programme |
159 | FWHM | Full Width at Half Maximum |
160 | GALACSI | Ground Atmospheric Layer Adaptive Optics for Spectroscopic Imaging (AOF) |
161 | GIRAFFE | Fibre-fed multi-object spectrograph and part of the VLT FLAMES facility |
162 | GLAO | Ground Layer Adaptive Optics |
163 | gNLT | Garching Night Log Tool |
164 | GRAAL | GRound-layer Adaptive optics Assisted by Lasers (AOF) |
165 | GROND | Gamma-Ray Burst Optical/Near-Infrared Detector (MPG/ESO 2.2-metre) |
166 | GTC | Gran Telescopio Canarias |
167 | GTO | Guaranteed Time for Observation |
168 | GWh | Gigawatt hours |
169 | GÉANT | European multi-gigabit computer network for research and education purposes |
170 | H-LTAO | HARMONI Laser Tomography Adaptive Optics |
171 | H2020 | (EU) Horizon 2020 Programme |
172 | HARMONI | Proposed first light integral field spectrograph for the ELT |
173 | HARPS | High Accuracy Radial Velocity Planetary Searcher (3.6-metre) |
174 | HAWK-I | High Acuity Wide field K-band Imager |
175 | HCI | Human Computer Interface |
176 | HIA | Herzberg Institute of Astrophysics (Canada) |
177 | HIRES | (ELT) HIgh REsolution Spectrograph |
178 | HODM | High Order Deformable Mirror |
179 | HST | Hubble Space Telescope |
180 | IAS | International Accounting Standards |
181 | IAU | International Astronomical Union |
182 | Icar | Icarus, Planetary science journal, Planetary science journal |
183 | IFU | Integral Field Unit |
184 | INAF | Italian National Institute for Astrophysics |
185 | INRIA | Institut National de Recherche en Informatique et en Automatique |
186 | IPAG | Institut de Planetologie et d’Astrophysique de Grenoble |
187 | IPC | (Chilean) Índice de Precios al Consumidor |
188 | IPP | Max-Planck Institute for Plasma Physics (Germany) |
189 | IPSAS | International Public Sector Accounting Standards |
190 | IPT | Integrated Product Team (ALMA) |
191 | IR | Infrared |
192 | IRAM | Institut de Radioastronomie Millimétrique |
193 | IRDIS | InfraRed Dual-beam Imager and Spectrograph (SPHERE, ELT) |
194 | IRIS | VLTI Infrared Image Sensor |
195 | IRLOS | InfraRed Low Order Sensor |
196 | IRO | International Relations Office |
197 | ISAAC | Infrared Spectrometer And Array Camera (VLT) |
198 | ISERD | Israeli inter-ministerial agency for R&D cooperation with Europe |
199 | ISM | International Staff Member |
200 | ISS | International Space Station |
201 | IT | Information Technology |
202 | ITAR | International Traffic in Arms Regulations |
203 | ITER | International Thermonuclear Experimental Reactor |
204 | IVOA | International Virtual Observatory Alliance |
205 | IVSLA | Istituto Veneto di Scienze ed Arti |
206 | IYA2009 | International Year of Astronomy 2009 |
207 | JAO | Joint ALMA Observatory |
208 | JENAM | Joint European and National Astronomy Meeting |
209 | JPL | Jet Propulsion Laboratory |
210 | JUICE | JUpiter ICy moons Explorer |
211 | JWST | James Webb Space Telescope |
212 | k | kilo/1,000 |
213 | KIDS | (VST) Kilo-Degree Survey |
214 | KMOS | K-band Multi-Object Spectrograph (VLT) |
215 | KTS | Klaus Tschira Stiftung |
216 | Kueyan | VLT Unit Telescope 2 |
217 | LABOCA | Large APEX Bolometer CAmera |
218 | LAOG | Laboratoire d'Astrophysique de l'Observatoire de Grenoble |
219 | LCS | Local Control System |
220 | LEO | Low Earth Orbit |
221 | LFC | Laser Frequency Comb |
222 | LGS | Laser Guide Star |
223 | LGSF | Laser Guide Star Facility |
224 | LMC | Large Magellanic Cloud |
225 | LMU | Ludwig-Maximilians-Universität München |
226 | LN2 | Liquid nitrogen |
227 | LOFAR | Low Frequency Array |
228 | LOPS | Local Optical Phasing Sensor |
229 | LP | Large Programme |
230 | LPG | Liquefied Petroleum Gas |
231 | LPO | La Silla Paranal Observatory |
232 | LSM | Local Staff Members |
233 | LSP | La Silla Paranal Subcommittee |
234 | LTAO | Laser Tomography Adaptive Optics |
235 | LVSM | Large Visible Sensor Module |
236 | M# | Mirror # |
237 | M | million/1,000,000 |
238 | MACAO | Multiple Application Curvature Adaptive Optic |
239 | MACCON | Motion controller manufacturer |
240 | MAD | Multi-conjugate Adaptive optics Demonstrator |
241 | MAORY | (ELT) Multi-conjugate Adaptive Optics RelaY |
242 | mas | milliarcseconds |
243 | MASCOT | Mini All-Sky Cloud Observation Tool (Paranal) |
244 | MATISSE | Multi AperTure mid-Infrared SpectroScopic Experiment (VLTI) |
245 | MCAO | Multi-Conjugate Adaptive Optics |
246 | Melipal | VLT Unit Telescope 3 |
247 | MELT | Minuscule ELT |
248 | MENLO systems | Optical equipment manufacturer |
249 | MERAC | Mobilising European Research in Astrophysics and Cosmology |
250 | MERIL | Mapping the European Research Infrastructure Landscape |
251 | METIS | Mid-infrared ELT Imager and Spectrograph |
252 | MICADO | Adaptive optics imaging camera (ELT) |
253 | MIDI | Mid-infrared Interferometric Instrument (VLTI) |
254 | MIT | Massachusetts Institute of Technology |
255 | mmVLBI | Millimeter Very Long Baseline Interferometry |
256 | Mn | Mirror #n |
257 | MOAO | Multiple-Object Adaptive Optics |
258 | MOONS | Multi Object Optical and Near-infrared Spectrograph (VLT third generation) |
259 | MOS | (ELT) Multi-Object Spectroscopy |
260 | MOSAIC | (ELT) Multi-Object Spectrograph (Multi-Object Spectrograph for Astrophysics, Intergalactic medium studies and Cosmology) |
261 | MOSFIRE | Near-infrared multi-object spectrograph (Keck) |
262 | MPA | Max Planck Institute for Astrophysics |
263 | MPE | Max Planck Institute for Extraterrestrial Physics |
264 | MPG | Max-Planck-Gesellschaft |
265 | MPIA | Max Planck Institute for Astronomy |
266 | MPIfR | Max-Planck Institute for Radioastronomy (Germany) |
267 | MS | Member State(s) |
268 | MUSE | Multi Unit Spectroscopic Explorer (VLT) |
269 | NACO | NAOS-CONICA (VLT) |
270 | NAOJ | National Astronomical Observatory of Japan |
271 | NAOMI | Adaptive optics system for the ATs (VLTI) |
272 | NAOS | Nasmyth Adaptive Optics System (VLT) |
273 | NASA | National Aeronautics and Space Administration |
274 | NAV | Navision |
275 | NDF | Non-Deliverable Forward Agreement |
276 | NEAR | New Earths in the Alpha Cen Region experiment |
277 | NEO | Near-Earth Object |
278 | NFM | Narrow Field Mode |
279 | NGC | New General Catalogue |
280 | NGC | New General detector Controller |
281 | NGSD | Proposed large natural/laser guide star WFS detector (ELT) |
282 | NGTS | Next Generation Transit Survey |
283 | NINS | National Institutes of Natural Sciences |
284 | NIRPS | (NNT) Near Infra Red Planet Searcher |
285 | NOVA | The Netherlands Research School for Astronomy (Nederlandse Onderzoekschool voor Astronomie) |
286 | NRAO | National Radio Astronomy Observatory |
287 | NSF | National Science Foundation |
288 | NTT | New Technology Telescope |
289 | NUVA | Network for UltraViolet Astrophysics |
290 | OAA | Arcetri Astrophysical Observatory |
291 | OBAMA | Optical Bidule for Aberration Measurement on the ATs |
292 | OCA-NICE | Cote d’Azur Observatory (Observatoire de la Cote d’Azur) |
293 | ODG | Office of the Director General |
294 | OECD | Organisation for Economic Co-operation and Development |
295 | OmegaCAM | Optical Camera for the VST |
296 | OPC | Observing Programmes Committee |
297 | OPO | Observing Programmes Office |
298 | OPTICON | Optical Infrared Coordination Network for Astronomy |
299 | OSF | ALMA Operations Support Facilities |
300 | OSO | Onsala Space Observatory |
301 | OT | Observing Tool |
302 | OTS | Operations Technical Support |
303 | P2PP | Peer to Peer Protocol |
304 | P86 | Observing Period 86 |
305 | P87 | Observing Period 87 |
306 | PA | Product Assurance |
307 | PAC | Provisional Acceptance Chile |
308 | PACMAN | Fringe tracker for PRIMA (VLTI) |
309 | PAE | Provisional Acceptance Europe |
310 | PARSEC | Sodium line laser for VLT AO |
311 | PDR | Preliminary Design Review |
312 | PESSTO | Public ESO Spectroscopic Survey of Transient Objects |
313 | PFS | (ELT) Pre-Focal Station |
314 | PFS-A | (ELT) Pre-Focal Station for Nasmyth A |
315 | PhD | Doctor of Philosophy |
316 | PI | Principal Investigator |
317 | PIO | Public Information Officer |
318 | PIONIER | VLTI visitor instrument |
319 | PIP | Paranal Instrumentation Programme |
320 | PLC | Programmable Logic Controllers (ELT) |
321 | PMD | Project Management Department |
322 | PMPD | Performance Management and Professional Development |
323 | PRIMA | Phase-Referenced Imaging and Micro-arcsecond Astrometry facility (VLTI) |
324 | PSF | Point Spread Function |
325 | PTP | Precision Time Protocol |
326 | Q | Quarter |
327 | QUEST | QUasar Equatorial Survey Team |
328 | R&D | Research and Development |
329 | RAB | Reflector Assembly Building |
330 | RCL | Radioastronomy Chajnantor Limitada |
331 | RedCLARA | Latin American Advanced Networks Cooperation (Academic data network in Latin America) |
332 | REM | Rapid Eye Mount Telescope (La Silla) |
333 | REUNA | Red Universitaria Nacional (Academic data network in Chile) |
334 | RM | Rossiter-McClaughlin (effect) |
335 | RMN | Reflective Memory Network (VLTI) |
336 | rms | Root Mean Square |
337 | SABOCA | Shortwave Apex BOlometer Camera |
338 | SAC | EURO-VO Science Advisory Committee |
339 | SAF | Science Archive Facility |
340 | SAFRAN-REOSC | High performance optics company |
341 | SAPHIRA | Detector for the GRAVITY wavefront sensor |
342 | SAXO | SPHERE’S AO system (VLT) |
343 | SCAO | Single-conjugate adaptive optics |
344 | SCO | Santiago Central Office (ALMA/ESO Vitacura) |
345 | SDD | Software Development Division |
346 | SDSS | Sloan Digital Sky Survey |
347 | SEPIA | Swedish ESO PI receiver for APEX |
348 | SHFI | Swedish Heterodyne Facility Instrument |
349 | SiC | (ELT) SiliconCarbide-mirrorsubstrate |
350 | SINFONI | Spectrograph for INtegral Field Observations in the Near Infrared (VLT) |
351 | SKA | Square Kilometer Array |
352 | SM | Service Mode (observing) |
353 | SM4 | Servicing Mission 4 (HST) |
354 | SOFI | SOn oF Isaac (NTT) |
355 | SOPHIE | Spectrographe pour l’Observation des Phénomènes des Intérieurs stellaires et des Exoplanètes |
356 | SOXS | (NTT) Son Of X-Shooter |
357 | SPARTA | Real-time computer for the AOF |
358 | SPC | Scientific Personnel Committee |
359 | SPECULOOS | (Paranal) Search for habitable Planets EClipsing ULtra-cOOl Stars |
360 | SPHERE | Spectro-Polarimetric High-contrast Exoplanet Research instrument (VLT) |
361 | SPIFFI | SPectrometer for Infrared Faint Field Imaging |
362 | SPT | South Pole Telescope |
363 | SSDF | Science Support Discretionary Fund |
364 | SSED | Software System Engineering Department |
365 | SSWG | Science Strategy Working Group |
366 | ST-ECF | Space Telescope European Coordination Facility |
367 | STC | Scientific Technical Committee |
368 | STFC | Science and Technology Facilities Council (UK) |
369 | STRAP | Tip-tilt sensors (VLTI) |
370 | STScI | Space Telescope Science Institute (USA) |
371 | sub-mm | submillimetre |
372 | SUSI2 | Superb Seeing Imager 2 (NTT) |
373 | TAROT | Télescope à Action Rapide pour les Objets Transitoires |
374 | TAROT-S | Télescopes à Action Rapide pour les Objets Transitoires South |
375 | TBT | Test-Bed Telescope |
376 | TEC | Technology Division |
377 | telbib | ESO library telescope bibliography database |
378 | TFB | Tunable Filter Bank (ALMA) |
379 | TIMMI | TIMMI far-infrared camera (ESO 3.6-metre telescope) |
380 | ToO | Target of Opportunity |
381 | TRAPPIST | TRAnsiting Planets and PlanetesImals Small Telescope |
382 | TRR | Test Readiness Review |
383 | TUM | Technische Universität München |
384 | UC | Users Committee |
385 | UK ATC | UK Astronomy Technology Centre |
386 | Ultracam | High-speed camera (VLT) |
387 | UltraVISTA | Ultra-deep near-infrared survey in the COSMOS field |
388 | UNCOPUOS | United Nations Committee for the Peaceful Uses of Outer Space |
389 | USM | University Observatory Munich |
390 | UT | Unit Telescope of the VLT |
391 | UT1–4 | VLT Unit Telescopes 1–4: Antu, Kueyen, Melipal and Yepun |
392 | UV | UltraViolet |
393 | UVES | UV-Visual Echelle Spectrograph (VLT) |
394 | VAT | Value Added Tax |
395 | VHS | VISTA Hemisphere Survey |
396 | VIDEO | VISTA Deep Extragalactic Observations Survey |
397 | VIKING | VISTA Kilo-degree Infrared Galaxy survey |
398 | VIMOS | VIsible MultiObject Spectrograph (VLT) |
399 | VINCI | VLT INterferometer Commissioning Instrument (VLTI) |
400 | VIPERS | VIMOS Public Extragalactic Redshift Survey |
401 | VIRCAM | VISTA Infrared Camera |
402 | VISA | VLTI Sub-Array |
403 | VISIR | VLT Mid-Infrared Imager Spectrometer |
404 | VISTA | Visible and Infrared Survey Telescope for Astronomy |
405 | VLT | Very Large Telescope |
406 | VLT/I | Very Large Telescope and its Interferometer |
407 | VLTI | Very Large Telescope Interferometer |
408 | VLTI-PR# | VLTI projects |
409 | VM | Visitor Mode (observing) |
410 | VMC | VISTA survey of the Magellanic Cloud system |
411 | VO | Virtual Observatory |
412 | VOP | Virtual Observatory Project Office |
413 | VPHAS+ | VST Photometric Hα Survey |
414 | VSS | Variability Sky Survey |
415 | VST | VLT Survey Telescope |
416 | VVDS | VIMOS VLT Deep Survey |
417 | VVV | ESO public survey VISTA Variables in the Vía Láctea |
418 | WASP | Wide Angle Search for Planets survey |
419 | WFCAM | Infrared wide field camera for the UK Infrared Telescope on Mauna Kea |
420 | WFI | Wide Field Imager (MPG/ESO 2.2-metre) |
421 | WiFi | Wireless Fidelity |
422 | WVR | Water Vapour Radiometer (ALMA) |
423 | X-shooter | Wideband ultraviolet-infrared single target spectrograph (VLT) |
424 | XAO | Extreme adaptive optics |
425 | XMM-Newton | X-ray Multi-Mirror satellite (ESA) |
426 | Yepun | VLT Unit Telescope 4 |
427 | Z-Spec | Millimetre-wave spectrograph (APEX visitor instrument) |
428 | zCOSMOS | Large Programme to measure 30 000 galaxies in the HST Cosmic Origins field |
429 | ZIMPOL | Zurich Imaging Polarimeter (SPHERE, ELT) |
430 | ΛCDM | Lambda Cold Dark Matter |
431 | μm | Micrometre |