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Projects of db.astro.rug.astro-wise.org

Total number of projects 69
Total number of users 343

Click on a project name to set the project.Only projects you are a member of are selectable.

ID Project Privileges Instrument Member of Member count Manager(s)
1 ALL 4 None True public 0
10 ACS@HST 4 ACS True public 0
101 WORKSHOP2005 2 WFI False 42 0
102 BONN2005 2 None False 14 0
103 LEIDENTUTORIAL2008 2 None False 17 1
104 TUTORIAL2014 2 None False 7 2
105 TUTORIAL2015 2 None False 13 4
106 TUTORIAL 2 None False 12 2
11 LBCBLUE@LBT 4 LBCBLUE True public 0
115 TESTCOMALS 2 ACS False 10 0
119 TESTATLAS3D 2 None False 0 0
12 VESUVIO 4 OMEGACAM True public 0
13 OCAM ILT 2 OCAM False 10 0
14 KIDS 2 OMEGACAM False 76 29
15 COMALS 5 ACS True public 1
16 COMETS 2 None False 2 0
17 OCAMVSTGT 2 OMEGACAM False 3 0
18 STUDENTWISE 4 None True public 1
19 ATLAS3D 2 None False 0 0
2 MDM8K 4 MDM8K True public 0
20 MONICA@WENDELSTEIN 4 MONICA True public 0
201 TESTALL 2 None False 9 9
202 COMM2011 2 OMEGACAM False 16 8
21 ULTRAVISTA 2 None False 5 0
22 ISAAC@VLT 2 ISAAC False 6 0
23 LBCRED@LBT 4 LBCRED True public 0
24 WFCAM@UKIRT 4 WFCAM True public 0
25 UKIDSS 2 WFCAM False 6 1
26 MEGACAM@CFHT 4 MEGACAM True public 3
27 OCAM 2008 2 OCAM False 10 0
28 GRATAMA@BLAAUW 4 GRATAMA True public 1
29 ANDICAM@CTIO1.3m 4 ANDICAM True public 1
3 OCAM@VST 4 OCAM True public 0
30 WISER 2 MEGACAM False 8 1
31 OMA 2 WFI False 3 0
32 OCAM2009 2 OCAM False 10 0
33 VIRCAM@VISTA 4 VIRCAM True public 1
34 VIKING 2 None False 36 7
35 ESOSCHMIDT@ESO1m 5 ESOSCHMIDT True public 2
36 OMEGACAM@VST 4 OMEGACAM True public 12
37 EUCLID 2 None False 50 1
38 OMEGAWHITE 2 OMEGACAM False 8 6
39 ACAM@WHT 4 ACAM True public 3
4 PDS 4 PDS True public 0
40 OMEGADWARFS 2 OMEGACAM False 11 6
41 ATLAS 4 OMEGACAM True public 4
42 VPHASPLUS 4 OMEGACAM True public 0
43 DECAM@BLANCO 4 DECAM True public 3
44 HERCULES 2 OMEGACAM False 11 6
45 VOICE 2 OMEGACAM False 21 4
46 FOCUS 2 OMEGACAM False 41 8
47 MICADO@E-ELT 4 MICADO True public 3
48 KIDS-PHOTZTEST 2 OMEGACAM False 6 4
49 SPARCS 2 DECAM False 5 5
5 WFC@INT 4 WFC True public 0
50 OMEGACLUSTER 2 OMEGACAM False 6 4
5030 DDT295A5030 2 OMEGACAM False 4 4
51 AMIGADEEP 2 OMEGACAM False 7 3
52 OMEGALAE 2 OMEGACAM False 5 3
53 DEEPCLUSTERS 2 WFC False 14 8
54 KABS 2 OMEGACAM False 14 2
55 PAMC 2 OMEGACAM False 1 1
56 VEGAS 2 OMEGACAM False 3 3
6 WFI@2.2m 4 WFI True public 0
7 WENSS 4 WSRT True public 1
8 LOFAR 2 LOFAR False 4 0
9 SUP@SUBARU 4 SUP True public 1
9225 AWJMCFARLAND 0 None False 0 0
9233 AWDEMO 1 None False 0 0
AWGSIKKEMAAWGVERDOESAWJBOUT

All users

AWGVERDOESAWJBOUT

Search for faint features in the outskirts of isolated galaxies

AWDBOXHOORNAWDSOBRALAWGVERDOESAWJMATTHEE
AWJMCFARLAND

The Altas3D Survey is a proposed project to observe a complete sample of all early-type galaxies within the local (40Mpc) volume, using the SAURON integral-field spectrograph on the William Herschel Telescope.

The HST-ACS Coma Legacy Survey uses new data from the Hubble Space Telescope's Advanced Camera for Surveys and legacy data sources such as Subaru, Isaac Newton Telescope, etc. to study the nature of objects in and around the Coma Cluster.

All users

All users

AWABELIKOV

Search for comets

AWABELIKOVAWEHELMICHAWGVERDOESAWHBUDDELMEIJER
AWJMCFARLANDAWKBEGEMAN
AWDBOXHOORNAWGVERDOESAWJMCFARLAND

None

All users

All public data for ACS

All users

All users

Project for the public data from the ANDICAM (A Novel Dual Imaging CAMera) mounted on the former 1.3m 2MASS telescope at Cerro Tololo observatory, Chile. The ANDICAM has two detectors that can operate simultaneously, observing the same pointing in both the optical and near-infrared.

All public data for WFC

AWATUDORICAAWEHELMICHAWGVERDOESAWHHILDEBRANDT
AWJMCFARLAND

VOICE aims at covering 4 square degrees around the CDFS in deep ugri imaging.

AWEHELMICHAWGVERDOESAWJDEJONGAWJMCFARLAND

All public data for PDS

All users

Test project for AIUB

The Large Binocular Camera (red arm) at the Large Binocular Telescope at Mount Graham

AWATUDORICAAWAVENHOLAAWEHELMICHAWEPETRILLO
AWGVERDOESAWMVANDENBERGAWSVATS

A census of the close-binary population in old open clusters.

Einstein cross around a massive super-compact galaxy in the KiDS survey: a VST follow-up

AWEHELMICHAWGVERDOESAWJMCFARLAND
AWDBOXHOORNAWEHELMICHAWGVERDOESAWKBEGEMAN
AWPGROOTAWSMACFARLANE
AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGVERDOES
AWJDEJONGAWJMCFARLANDAWKBEGEMANAWMTEMPELAAR
AWRVERMEIJAWWVRIEND
AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGVERDOES
AWJDEJONGAWJMCFARLANDAWKBEGEMANAWMTEMPELAAR
AWRVERMEIJAWWVRIEND
AWDBOXHOORNAWEHELMICHAWGSIKKEMAAWGVERDOES
AWHBUDDELMEIJERAWJDEJONGAWJMCFARLANDAWKBEGEMAN
AWWVRIEND

All users

All users

AWEHELMICHAWGVERDOES

LOw Frequency ARray - The largest radio telescope in the world

AWAUSOVAWDBOXHOORNAWEVALENTYNAWWVRIEND

ACAM is mounted permanently at a folded-Cassegrain focus of the 4.2-m William Herschel Telescope. It can be used for high-throughput broad-band imaging, narrow-band imaging and low-resolution spectroscopy.

All users

AWADVORNIKAWAGRADOAWARAJAWARIFATTO
AWAWRIGHTAWCTORTORAAWDBOXHOORNAWDKLAES
AWEDEULAWEHELMICHAWEPUDDUAWEVALENTYN
AWFGETMANAWGCOVONEAWGSIKKEMAAWGVERDOES
AWHBUDDELMEIJERAWJDEJONGAWJMCFARLANDAWKKUIJKEN
AWMBILICKIAWMDALLORAAWMIRWINAWMPAOLILLO
AWMRADOVICHAWNNAPOLITANOAWOCORDESAWPHUDELOT
AWTERBEN

The nature, clustering and evolution of Lyman-¿ emitters with the largest Lyman-¿ survey at z ¿ 2.4

AWAVENHOLAAWDBOXHOORNAWEHELMICHAWGVERDOES
AWJMCFARLANDAWPRAMIREZMORETAAWRPELETIER

All users

AWDBOXHOORNAWEHELMICHAWGSIKKEMAAWGVERDOES
AWHBUDDELMEIJERAWJDEJONGAWJMCFARLANDAWKBEGEMAN
AWWVRIEND
AWDBOXHOORNAWJDEJONGAWJMCFARLANDAWNNAPOLITANO

All users

Project for the public data from the 0.4m Gratama telescope at the Blaauw Observatory atop the Bernoulliborg in Groningen, The Netherlands, run by the Kapteyn Institute.

AWEHELMICHAWGVERDOESAWJDEJONGAWJMCFARLAND
AWEHELMICHAWGVERDOESAWJHOLTAWJMCFARLAND
AWMFRANXAWRWILLIAMS
AWJMCFARLAND

All public data for OCAM

AWATUDORICAAWEHELMICHAWGVERDOESAWHHILDEBRANDT
AWJMCFARLAND

This project contains all public data from the MONICA CCD camera on the 0.8m telescope at Wendelstein Observatory, operated by the Institute for Astronomy and Astrophysics of the University of Munich.

AWABELIKOVAWDBOXHOORNAWEHELMICHAWGVERDOES
AWJMCFARLANDAWJMWEBAZEAWKBEGEMANAWWVRIEND
AWJMCFARLAND
AWDBOXHOORNAWEVALENTYNAWGVERDOESAWJBOUT
AWJMCFARLANDAWKBEGEMAN
AWABOSELLIAWAGRADOAWAHELMIAWARAJ
AWAVENHOLAAWDBOXHOORNAWEGREBELAWEHELMICH
AWEIODICEAWELAURIKAINENAWETOLOBAAWEVALENTYN
AWFGETMANAWFLABARBERAAWGHENSLERAWGSIKKEMA
AWGVANDEVENAWGVERDOESAWHBUDDELMEIJERAWHSALO
AWJDEJONGAWJFALCONBARROSOAWJJANZAWJMCFARLAND
AWKKUIJKENAWMCAPACCIOLIAWMHILKERAWMPAOLLILO
AWMSPAVONEAWNNAPOLITANOAWNZABELAWRMUNOZ
AWRPELETIERAWSMIESKEAWSPAUDELAWSTRAGER
AWTLISKERAWTPUZIAAWTSAIFOLLAHIAWVSPRINGEL
AWWVRIEND

Data for the VISTA Kilo-degree Infrared Galaxy survey.

AWABELIKOVAWBPILADIEZAWBVENEMANSAWCBLOKZIJL
AWCSIFONAWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWJBOUTAWJDEJONGAWJMCFARLANDAWJMWEBAZE
AWJPIZAGNOAWKBEGEMANAWKKUIJKENAWMCACCIATO
AWMCAPACCIOLIAWMNEESERAWMRADOVICHAWNIRISARRI
AWNWISSEAWPHERAUDEAUAWRBENDERAWRSAGLIA
AWRSILVOTTIAWRVANDERBURGAWRWILLIAMSAWSCASEWELL
AWSVLAARAWTERBENAWWVRIENDAWYMELLIER

All public data for VIRCAM

AWEHELMICHAWGVERDOESAWJDEJONGAWKKUIJKEN
AWDBOXHOORNAWEIODICEAWMSPAVONE

The Altas3D Survey is a proposed project to observe a complete sample of all early-type galaxies within the local (40Mpc) volume, using the SAURON integral-field spectrograph on the William Herschel Telescope.

The Spitzer Adaptation of the Red-sequence Cluster Survey is a z'-passband imaging survey of the SWIRE Legacy Survey Fields. Observations of the six fields have been made at all seven Spitzer (3.6, 4.5, 5.8, 8.0, 24, 70, 160 micron) passbands. SpARCS consists of deep (z'= 24 AB) observations made from both hemispheres using MegaCam at CFHT (Northern Fields) and MOSAICII at CTIO (Southern Fields). The cluster detection (z'-imaging) phase is now complete and has yielded hundreds of z > 1 cluster candidates detected based upon z'-[3.6] color. With a total effective area of 41.9 square degrees, SpARCS is currently the largest completed z > 1 cluster survey. This project is for the processing of new (DECAM) and legacy SpARCS data.

AWJMCFARLAND

Sandbox for Astro-WISE tutorial users.

AWAVENHOLAAWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWJMCFARLANDAWRPELETIERAWWVRIEND

Sandbox for Astro-WISE tutorial users.

All users

Probing the accretion of matter around massive galaxy clusters with splashback

AWABELIKOVAWEHELMICHAWGVERDOESAWJBOUT
AWJMCFARLANDAWJPIZAGNOAWRWILLIAMS

All public data for OmegaCAM. OmegaCAM is a 1 square degree wide field, optical, 16k X 16k pixel camera for the VLT Survey Telescope (VST) on Paranal Observatory.

AWDBOXHOORNAWEIODICEAWMSPAVONE

All users

AWARAMESHAWAVENHOLAAWBLAPAWDBOXHOORN
AWEHELMICHAWGSIKKEMAAWGVERDOESAWJDEJONG
AWJMCFARLANDAWJVANDENBORNAWNCHOQUEAWPMANCERAPINA
AWRPELETIERAWTVOS
AWABELIKOVAWACHOIAWADVORNIKAWAEDGE
AWAGRADOAWARAJAWARIFATTOAWATUDORICA
AWAWRIGHTAWBALTIERIAWBJOACHIMIAWBVENEMANS
AWCHEYMANSAWCMORRISONAWCSIFONAWCSPINIELLO
AWCTORTORAAWDBOXHOORNAWDKLAESAWDWILLIAMS
AWEDEULAWEHELMICHAWEIODICEAWEPETRILLO
AWEPUDDUAWEVALENTYNAWEVANUITERTAWFGETMAN
AWFKOEHLINGERAWFLABARBERAAWGCOVONEAWGDAGO
AWGSIKKEMAAWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWHHOEKSTRAAWJDEJONGAWJMCFARLANDAWJPEACOCK
AWKBEGEMANAWKFRANTSEVAAWKKUIJKENAWLKELVIN
AWLMILLERAWMBILICKIAWMCAPACCIOLIAWMCOSTADUARTE
AWMDALLORAAWMIRWINAWMMAHLKEAWMPAOLILLO
AWMRADOVICHAWMSPAVONEAWMVIOLAAWNNAPOLITANO
AWOCORDESAWPHUDELOTAWPNOORISHADAWPSCHNEIDER
AWPSIMONAWRHERBONNETAWRNAKAJIMAAWRPELETIER
AWRVANDERBURGAWSDRIVERAWTERBENAWTKITCHING
AWTLISKERAWTSCHRABBACKKRAHEAWTSHANKSAWWMULDER
AWWSUTHERLANDAWWVRIENDAWYDEVRIESAWZHUANG

OmegaCAM lab tests

Subaru is an 8.2 meter optical-infrared telescope at the summit of Mauna Kea, Hawaii, operated by the National Astronomical Observatory of Japan (NAOJ), National Institutes of Natural Science. SuprimeCam is the 10k x 8k mosaic camera at the prime focus.

VST/OmegaCAM Exploration of SUperclusters Voids and Intermediate Objects

The Large Binocular Camera (blue arm) at the Large Binocular Telescope at Mount Graham

OmegaCAM/VST Guaranteed Time

AWARAJAWFGETMAN

INT data for Virtual Observations lecture series

AWJMCFARLAND
AWADVORNIKAWCSPINIELLOAWEHELMICHAWEIODICE
AWGDAGOAWGVERDOESAWJDEJONGAWJMCFARLAND
AWLKELVINAWMBILICKIAWMSPAVONEAWRPELETIER
AWTSAIFOLLAHI

All users

AWASAVINOAWDBOXHOORNAWDDINGAWEHELMICH
AWJDEJONGAWKFRANTSEVAAWMMAHLKEAWNCHOQUE
AWOCONTIGIANIAWPMANCERAPINAAWTNUTMAAWYDEVRIES
AWAGRADOAWANONYMOUSAWAROJBIAWCHAINES
AWDBOXHOORNAWDWILMANAWEBERTINAWEDEUL
AWEHELMICHAWEVALENTYNAWFGETMANAWGFEULNER
AWGSIKKEMAAWGVERDOESAWHHILDEBRANDTAWJDIETRICH
AWJKOPPENHOEFERAWJMCFARLANDAWJSNIGULAAWKBEGEMAN
AWKKOVACAWKKUIJKENAWLHABERZETTLAWLMORALESRUEDA
AWMNEESERAWMPAVLOVAWMPOHLENAWMSMIT
AWMTEMPELAARAWNRAMANUJAMAWOCORDESAWOSCHMITHUESEN
AWPGROOTAWPHERAUDEAUAWRRENGELINKAWRSILVOTTI
AWRVERMEIJAWSLECCIAAWTERBENAWTSCHNEIDER
AWWVRIENDAWYMELLIER

All public data for MDM8K

Groningen tutorial, July 10 and 11.

The VST/OmegaCam Photometric H¿ Survey of the Southern Galactic Plane.

AWARAJAWARIFATTOAWDBOXHOORNAWEPUDDU
AWEVALENTYNAWFGETMANAWFLABARBERAAWGVERDOES
AWJDEJONGAWKKUIJKENAWMDALLORAAWMPAOLILLO
AWMRADOVICHAWNNAPOLITANO
AWEHELMICHAWJDEJONG
AWDBOXHOORNAWEHELMICHAWETOLSTOYAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJMCFARLANDAWKKUIJKENAWTDEBOER

All users

This project contains data taken during the OmegaCAM integration test of October 2008. Instrument and detector were reassembled on Paranal, but not joined together. The shutter and filter mechanics were operated but not present in front of the detector.

KiDS ATLAS Bridging Survey

AWEHELMICHAWGVERDOESAWMVANDENBERGAWSVATS
AWACHOIAWCHEYMANSAWCSIFONAWDAPPLEGATE
AWDBOXHOORNAWEHELMICHAWFGETMANAWGCOVONE
AWGSIKKEMAAWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWJDEJONGAWJMCFARLANDAWKKUIJKENAWMRADOVICH
AWMVACCARIAWMVIOLAAWNNAPOLITANOAWRVANDERBURG
AWTERBEN

Astro-Wise Workshop - 14-18 November 2005, Lorentz Center, Leiden.

AWJMCFARLAND

All users

UKIDSS (UKIRT Infrared Deep Sky Survey) is the next generation near-infrared sky survey, the successor to 2MASS using the infrared WFCAM survey instrument attached to the UK InfraRed Telescope (UKIRT) on Mauna Kea, Hawaii. UKIDSS began in May 2005 and will survey 7500 square degrees of the Northern sky, extending over both high and low Galactic latitudes, in JHK to K=18.3. This depth is three magnitudes deeper than 2MASS. UKIDSS will be the true near-infrared counterpart to the Sloan survey, and will produce as well a panoramic clear atlas of the Galactic plane.

AWABELIKOVAWDBOXHOORNAWEDEULAWEHELMICH
AWEVALENTYNAWGSIKKEMAAWGVERDOESAWHBUDDELMEIJER
AWJBOUTAWJDEJONGAWJMCFARLANDAWJPIZAGNO
AWKBEGEMANAWKKUIJKENAWRHOOKAWWVRIEND
AWOCONTIGIANI
AWDBOXHOORNAWEHELMICHAWGVERDOESAWHHILDEBRANDT
AWJDEJONGAWKKUIJKEN
AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGSIKKEMA
AWGVERDOESAWJBOUTAWJDEJONGAWJMCFARLAND

OMA (ontological machine for Astro-Wise) is a prototype of the system for incorporation of external data sources in Astro-Wise. It will be used to test scientific use cases for OMA as well.

All users

AWEHELMICH

The initial aim of ATLAS is to survey 4500 deg2 of the Southern Sky at high galactic latitudes to comparable depths to the SDSS in the North. The VST ATLAS will be the first step towards a panoramic digital survey of the Southern Sky in the optical bands.

VST GTO Hercules supercluster

All users

All public data for WFI

All users

AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGSIKKEMA
AWGVERDOESAWJBOUTAWJMCFARLANDAWKBEGEMAN
AWLKELVINAWRBUTAAWWVRIEND
AWAKARICKAWCOMALSAWDBOXHOORNAWEHELMICH
AWEVALENTYNAWGVERDOESAWJMCFARLANDAWLDOMINGUEZ
AWMDENBROKAWMTEMPELAAR

Ultra deep near-infrared survey for the early Universe.

AWDBOXHOORNAWJDEJONGAWJMCFARLANDAWNNAPOLITANO

All users

AWOCONTIGIANI
AWBBURGGRAFAWCTRACHTERNACHAWDBOMANSAWDROSENBAUM
AWFBRIMIOULLEAWHHILDEBRANDTAWHISRAELAWJDIETRICH
AWKWEISAWMLERCHSTERAWOCORDESAWOSCHMITHUESEN
AWTERBENAWTSCHRABBACKKRAHE
AWABELIKOVAWGSIKKEMAAWGVERDOES

None

All users

All users

AWJMCFARLAND

Euclid is an ESA medium class mission selected for launch in 2019 in the Cosmic Vision 2015-2025 programme

All users

MICADO will be a near-infrared wide-field camera at the European Extremely Large Telescope.

DECam is the 3 square-degree (2.2 degree wide) Dark Energy Camera mounted on the 4.0m Blanco telescope at Cerro Tololo Inter-American Observatory (CTIO) in central Chile for the purpose of collecting data for DES, the Dark Energy Survey.

All users

FOrnax Cluster Ultradeep Survey

Testing the photometric redshift and shear measurements of the Kilo Degree Survey

MYDB for AWDEMO

MYDB for JMCFARLAND

All public data for all instruments

AWWVRIEND

In december 2009 the CCD 'Sculptor' of the OmegaCAM detector was replaced. The data in this project were taken to confirm the success of this procedure. RawFitsData were created artificially; the order of extensions is not constant or the same as in the other OCAM datasets.

MegaPrime is the wide-field optical imaging facility at CFHT (Canada-France-Hawaii telescope) atop Mauna Kea, Hawaii. At the heart of MegaPrime is the wide-field imager, MegaCam, consisting of 36 2048 x 4612 pixel CCDs (a total of 340 megapixels), covering a full 1 degree x 1 degree field-of-view with a resolution of 0.187 arcsecond per pixel to properly sample the 0.7 arcsecond median seeing offered by the CFHT at Mauna Kea.

AWDBOXHOORNAWEHELMICHAWGVERDOESAWMHEEMSKERK
AWMVANDENBERGAWSVATS
AWEVALENTYNAWGVERDOESAWJMCFARLAND
AWAVENHOLAAWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWJDEJONGAWJMCFARLANDAWNCHOQUEAWPMANCERAPINA
AWEHELMICHAWGVERDOES
AWEHELMICHAWETOLSTOYAWGSIKKEMAAWGVERDOES
AWJDEJONGAWTDEBOER

1700 Square degree 5 band survey of the equatorial strip and 2dF South region

The HST-ACS Coma Legacy Survey

The Wide-field Imaging Survey Evaluation of Readiness (WISER) project seeks to evaluate the readiness of our system to deal with large-scale survey data from wide-field imagers.

Leiden Tutorial. August 18-20.

All users

AWJMCFARLAND

None

For testing purposes only.

All users

AWGVERDOESAWJMCFARLANDAWWVRIEND
AWDBOXHOORNAWEHELMICHAWGRAMSAYAWGVERDOES
AWKBEGEMANAWPGROOTAWRTOMAAWSMACFARLANE

Contains scans of photographic plates taken with the ESO Schmidt 1m telescope on La Silla.

AWABELIKOVAWACHAMBALLUAWAJAFFEAWAPIEMONTE
AWATSYGANOVAWBDROEGEAWBNICHOLAWCBACCIGALUPI
AWCROUSSELAWCTAOAWDBOXHOORNAWEAUBOURG
AWEHELMICHAWEVALENTYNAWFABDALLAAWFRAISON
AWGBLANCAWGSIKKEMAAWGVERDOESAWHBUDDELMEIJER
AWJDEJONGAWJKOPPENHOEFERAWJMCFARLANDAWJMOHR
AWJPIZAGNOAWJSNIGULAAWKBEGEMANAWKGANGA
AWKKUIJKENAWMJARVISAWMKUEMMELAWMSAUVAGE
AWMVACCARIAWMWETZSTEINAWNBUSCAAWOLAHAV
AWOMARGGRAFAWPHUDELOTAWRCABANACAWRHENDERSON
AWRSAGLIAAWRWILLIAMSAWSDESAIAWSSERJEANT
AWTERBENAWTGIANNANTONIOAWVBECKMANNAWWMULDER
AWWVRIENDAWYMELLIER
AWEHELMICHAWGVERDOESAWJMCFARLAND
AWEDEMOOIJAWEDEULAWEHELMICHAWEVANUITERT
AWGVERDOESAWHHILDEBRANDTAWISNELLENAWJHOLT
AWJMCFARLANDAWKKUIJKENAWKVERBEEKAWMFRANX
AWMSMITAWMVELANDERAWOSPOORENAWRWILLIAMS
AWTSCHRABBACKKRAHE
AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGVERDOES
AWJDEJONGAWJMCFARLANDAWKBEGEMANAWMTEMPELAAR
AWRVERMEIJAWWVRIEND
AWATUDORICAAWGVERDOESAWJMCFARLAND
AWEHELMICHAWGVERDOESAWJHOLTAWJMCFARLAND
AWMFRANX
AWADVORNIKAWARAJAWDBOXHOORNAWEHELMICH
AWEVALENTYNAWFGETMANAWGSIKKEMAAWGVERDOES
AWJBOUTAWJDEJONGAWJMCFARLANDAWMBILICKI

One of three large surveys on the William Herschel Telescope (WHT) will be WEAVE-Clusters using the WEAVE Spectrograph. This will study cluster evolution through an analysis of the internal kinematics and stellar populations of dwarf galaxies. In preparation of this survey, deep imaging will be obtained with Wide Field Camera (WFC) on the Isaac Newton Telescope (INT) for some of these clusters. The resulting data set will be analyzed using special photometric techniques developed for the VST-Fornax Survey.

WFCAM is a near-IR wide field camera for the UKIRT telescope on Mauna Kea, Hawaii that has been designed specifically to carry out large-scale survey observations such as the UKIRT Infrared Deep Sky Survey (UKIDSS).

Commissioning data for OmegaCAM, mostly taken from March through June of 2011.

OmegaWhite is a variability survey aimed at periods of less than 2 hours. Using the wide-field camera OmegaCam on the VLT Survey Telescope (VST) 400 square degrees will be monitored for 2 hours in g' and in addition colour information will be obtained by imaging the same area in u', r', i' and narrow band He (5015) and Halpha filters. OmegaWhite is part of the European Galactic Plane Surveys (EGAPS). For additional information on OmegaWhite please have a look at this OmegaWhite survey website - http://www.astro.ru.nl/omegawhite/

AWGVERDOES

The Westerbork Northern Sky Survey

AWEHELMICHAWGCOVONEAWGVERDOESAWMVACCARI

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