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

Total number of projects 66
Total number of users 319

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 True 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
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 95 30
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 10
37 EUCLID 2 None False 49 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 10 6
45 VOICE 2 OMEGACAM False 21 4
46 FOCUS 2 OMEGACAM False 36 6
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 11 3
54 KABS 2 OMEGACAM False 13 1
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

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.

MYDB for AWDEMO

None

Sandbox for Astro-WISE tutorial users.

All public data for WFI

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

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.

AWGVERDOESAWJBOUT
AWDBOXHOORNAWEHELMICHAWGRAMSAY
AWGVERDOESAWKBEGEMANAWPGROOT
AWRTOMAAWSMACFARLANE

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

AWEHELMICHAWGVERDOESAWJMCFARLAND

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.

All public data for MDM8K

AWAGRADOAWANONYMOUSAWAROJBI
AWCHAINESAWDBOXHOORNAWDWILMAN
AWEBERTINAWEDEULAWEHELMICH
AWEVALENTYNAWFGETMANAWGFEULNER
AWGSIKKEMAAWGVERDOESAWHHILDEBRANDT
AWJDIETRICHAWJKOPPENHOEFERAWJMCFARLAND
AWJSNIGULAAWKBEGEMANAWKKOVAC
AWKKUIJKENAWLHABERZETTLAWLMORALESRUEDA
AWMNEESERAWMPAVLOVAWMPOHLEN
AWMSMITAWMTEMPELAARAWNRAMANUJAM
AWOCORDESAWOSCHMITHUESENAWPGROOT
AWPHERAUDEAUAWRRENGELINKAWRSILVOTTI
AWRVERMEIJAWSLECCIAAWTERBEN
AWTSCHNEIDERAWWVRIENDAWYMELLIER
AWAVENHOLAAWGSIKKEMAAWJMCFARLAND

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 users

AWEHELMICHAWGVERDOESAWJHOLT
AWJMCFARLANDAWMFRANX

All users

Groningen tutorial, July 10 and 11.

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.

INT data for Virtual Observations lecture series

AWAKARICKAWCOMALSAWDBOXHOORN
AWEHELMICHAWEVALENTYNAWGVERDOES
AWJMCFARLANDAWLDOMINGUEZAWMDENBROK
AWMTEMPELAAR

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

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

All public data for ACS

AWJMCFARLAND

All users

AWADVORNIKAWAGRADOAWARAJ
AWARIFATTOAWCTORTORAAWDBOXHOORN
AWDKLAESAWEDEULAWEHELMICH
AWEPUDDUAWEVALENTYNAWFGETMAN
AWGCOVONEAWGSIKKEMAAWGVERDOES
AWHBUDDELMEIJERAWJBOUTAWJDEJONG
AWJMCFARLANDAWKKUIJKENAWMBILICKI
AWMDALLORAAWMIRWINAWMPAOLILLO
AWMRADOVICHAWNNAPOLITANOAWOCORDES
AWPHUDELOTAWRSAGLIAAWTERBEN

All users

AWDBOXHOORNAWEHELMICHAWGVERDOES
AWKBEGEMANAWPGROOTAWSMACFARLANE
AWDBOXHOORNAWDSOBRALAWGVERDOES
AWJMATTHEEAWJMCFARLAND

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.

Search for faint features in the outskirts of isolated galaxies

AWEDEMOOIJAWEDEULAWEHELMICH
AWEVANUITERTAWGVERDOESAWHHILDEBRANDT
AWISNELLENAWJHOLTAWJMCFARLAND
AWKKUIJKENAWKVERBEEKAWMFRANX
AWMSMITAWMVELANDERAWOSPOOREN
AWRWILLIAMSAWTSCHRABBACKKRAHE

All users

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.

All users

AWGSIKKEMAAWGVERDOESAWJBOUT

The HST-ACS Coma Legacy Survey

All public data for VIRCAM

AWABELIKOVAWABUDDENDIEKAWACHOI
AWADVORNIKAWAEDGEAWAGRADO
AWAJAKOBSAWARAJAWARIFATTO
AWATUDORICAAWBALTIERIAWBJOACHIMI
AWBLAUAWBPILADIEZAWBVENEMANS
AWCBLOKZIJLAWCHEYMANSAWCMORRISON
AWCSIFONAWCSPINIELLOAWCTORTORA
AWDAPPLEGATEAWDBOXHOORNAWDKLAES
AWDWILLIAMSAWEDEULAWEHELMICH
AWEIODICEAWEPETRILLOAWEPUDDU
AWESEMBOLONIAWEVALENTYNAWEVANUITERT
AWFGETMANAWFKOEHLINGERAWFLABARBERA
AWGCOVONEAWGDAGOAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWHHOEKSTRAAWJBOUTAWJDEJONG
AWJMCFARLANDAWJMWEBAZEAWJPEACOCK
AWJSNIGULAAWKBEGEMANAWKKUIJKEN
AWLKELVINAWLMILLERAWMBILICKI
AWMCACCIATOAWMCAPACCIOLIAWMCOSTADUARTE
AWMDALLORAAWMIRWINAWMMAHLKE
AWMPAOLILLOAWMRADOVICHAWMSEGERS
AWMSMITAWMSPAVONEAWMVELANDER
AWMVELLISCIGAWMVIOLAAWNIRISARRI
AWNNAPOLITANOAWOCORDESAWPHUDELOT
AWPNOORISHADAWPSCHNEIDERAWPSIMON
AWRBENDERAWRHERBONNETAWRNAKAJIMA
AWRPELETIERAWRSAGLIAAWRVANDERBURG
AWSDRIVERAWSGIODINIAWSSEITZ
AWSVLAARAWSWARRENAWTERBEN
AWTKITCHINGAWTLISKERAWTSCHRABBACKKRAHE
AWTSHANKSAWWSUTHERLANDAWWVRIEND
AWYMELLIERAWZHUANG

All public data for WFC

AWDBOXHOORNAWEHELMICHAWETOLSTOY
AWEVALENTYNAWGSIKKEMAAWGVERDOES
AWHBUDDELMEIJERAWJDEJONGAWJMCFARLAND
AWKKUIJKENAWTDEBOER
AWABELIKOV
AWATUDORICAAWEHELMICHAWGVERDOES
AWHHILDEBRANDTAWJMCFARLAND

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.

None

AWJMCFARLAND

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).

AWAUSOVAWDBOXHOORNAWEVALENTYN
AWWVRIEND
AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWJBOUT
AWJDEJONGAWJMCFARLAND

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.

AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGVERDOESAWJDEJONGAWJMCFARLAND
AWKBEGEMANAWMTEMPELAARAWRVERMEIJ
AWWVRIEND

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

AWAVENHOLAAWDBOXHOORNAWEHELMICH
AWGVERDOESAWJMCFARLANDAWPRAMIREZMORETA
AWRPELETIER

Test project for AIUB

MYDB for JMCFARLAND

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

AWEHELMICHAWETOLSTOYAWGSIKKEMA
AWGVERDOESAWJDEJONGAWTDEBOER

FOrnax Cluster Ultradeep Survey

AWABELIKOVAWEHELMICHAWGVERDOES
AWHBUDDELMEIJERAWJMCFARLANDAWKBEGEMAN
AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGVERDOESAWJDEJONGAWJMCFARLAND
AWKBEGEMANAWMTEMPELAARAWRVERMEIJ
AWWVRIEND

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.

AWJMCFARLAND
AWABELIKOVAWBPILADIEZAWBVENEMANS
AWCBLOKZIJLAWCSIFONAWDBOXHOORN
AWEHELMICHAWEVALENTYNAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWJBOUTAWJDEJONGAWJMCFARLAND
AWJMWEBAZEAWJPIZAGNOAWKBEGEMAN
AWKKUIJKENAWMCACCIATOAWMCAPACCIOLI
AWMNEESERAWMRADOVICHAWNIRISARRI
AWNWISSEAWPHERAUDEAUAWRBENDER
AWRSAGLIAAWRSILVOTTIAWRVANDERBURG
AWRWILLIAMSAWSCASEWELLAWSVLAAR
AWTERBENAWWVRIENDAWYMELLIER

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.

For testing purposes only.

AWJMCFARLAND

All users

Data for the VISTA Kilo-degree Infrared Galaxy survey.

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

AWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJMCFARLANDAWKBEGEMANAWWVRIEND

All users

AWDBOXHOORNAWJDEJONGAWJMCFARLAND
AWNNAPOLITANO
AWABELIKOVAWGSIKKEMAAWGVERDOES
AWABOSELLIAWAGRADOAWAHELMI
AWAVENHOLAAWDBOXHOORNAWEGREBEL
AWEHELMICHAWEIODICEAWELAURIKAINEN
AWETOLOBAAWEVALENTYNAWFLABARBERA
AWGHENSLERAWGSIKKEMAAWGVANDEVEN
AWGVERDOESAWHBUDDELMEIJERAWHSALO
AWJDEJONGAWJFALCONBARROSOAWJJANZ
AWJMCFARLANDAWKKUIJKENAWMCAPACCIOLI
AWMHILKERAWMPAOLLILOAWNNAPOLITANO
AWRMUNOZAWRPELETIERAWSMIESKE
AWSPAUDELAWSTRAGERAWTLISKER
AWTPUZIAAWTSAIFOLLAHIAWVSPRINGEL

All users

AWDBOXHOORNAWJDEJONGAWJMCFARLAND
AWNNAPOLITANO

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

LOw Frequency ARray - The largest radio telescope in the world

AWABELIKOVAWDBOXHOORNAWEDEUL
AWEHELMICHAWEVALENTYNAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJBOUT
AWJDEJONGAWJMCFARLANDAWJPIZAGNO
AWKBEGEMANAWKKUIJKENAWRHOOK
AWWVRIEND
AWAVENHOLAAWEHELMICHAWGSIKKEMA
AWGVERDOESAWJMCFARLANDAWRPELETIER

All public data for PDS

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

AWEHELMICHAWGVERDOESAWJDEJONG
AWKKUIJKEN

All public data for all instruments

AWADVORNIKAWDBOXHOORNAWEHELMICH
AWEVALENTYNAWGSIKKEMAAWGVERDOES
AWJBOUTAWJDEJONGAWJMCFARLAND
AWMBILICKI
AWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJMCFARLANDAWKBEGEMANAWWVRIEND
AWGVERDOES
AWABELIKOVAWDBOXHOORNAWEHELMICH
AWGVERDOESAWJMCFARLANDAWJMWEBAZE
AWKBEGEMANAWWVRIEND
AWEHELMICHAWGVERDOESAWJDEJONG
AWJMCFARLAND

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

All public data for OCAM

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/

AWBBURGGRAFAWCTRACHTERNACHAWDBOMANS
AWDROSENBAUMAWFBRIMIOULLEAWHHILDEBRANDT
AWHISRAELAWJDIETRICHAWKWEIS
AWMLERCHSTERAWOCORDESAWOSCHMITHUESEN
AWTERBENAWTSCHRABBACKKRAHE
AWEHELMICHAWGVERDOESAWMVANDENBERG
AWSVATS
AWARAJAWARIFATTOAWEPUDDU
AWEVALENTYNAWFGETMANAWFLABARBERA
AWGVERDOESAWJDEJONGAWKKUIJKEN
AWMDALLORAAWMPAOLILLOAWMRADOVICH
AWNNAPOLITANO
AWJMCFARLAND
AWGVERDOESAWJMCFARLANDAWWVRIEND

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.

All users

All users

AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGVERDOESAWJDEJONGAWJMCFARLAND
AWKBEGEMANAWMTEMPELAARAWRVERMEIJ
AWWVRIEND
AWARAMESHAWAVENHOLAAWBLAP
AWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWJMCFARLANDAWJVANDENBORN
AWRPELETIERAWTVOS

All users

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

KiDS ATLAS Bridging Survey

AWACHOIAWCHEYMANSAWCSIFON
AWDAPPLEGATEAWDBOXHOORNAWEHELMICH
AWFGETMANAWGCOVONEAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWJDEJONGAWJMCFARLANDAWKKUIJKEN
AWMRADOVICHAWMVACCARIAWMVIOLA
AWNNAPOLITANOAWRVANDERBURGAWTERBEN

OmegaCAM lab tests

AWWVRIEND
AWATUDORICAAWEHELMICHAWGVERDOES
AWHHILDEBRANDTAWJMCFARLAND

All users

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.

AWEHELMICHAWGCOVONEAWGVERDOES
AWMVACCARI

All users

AWDBOXHOORNAWEHELMICHAWGVERDOES
AWHHILDEBRANDTAWJDEJONGAWKKUIJKEN
AWEHELMICHAWGVERDOES

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.

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.

VST/OmegaCAM Exploration of SUperclusters Voids and Intermediate Objects

AWEHELMICHAWGVERDOESAWJHOLT
AWJMCFARLANDAWMFRANXAWRWILLIAMS
AWDBOXHOORNAWEVALENTYNAWGVERDOES
AWJBOUTAWJMCFARLANDAWKBEGEMAN

Leiden Tutorial. August 18-20.

AWJMCFARLAND

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

AWABELIKOVAWACHAMBALLUAWAJAFFE
AWAPIEMONTEAWATSYGANOVAWBDROEGE
AWBNICHOLAWCBACCIGALUPIAWCROUSSEL
AWCTAOAWDBOXHOORNAWEAUBOURG
AWEHELMICHAWEVALENTYNAWFABDALLA
AWFRAISONAWGBLANCAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJKOPPENHOEFERAWJMCFARLANDAWJMOHR
AWJPIZAGNOAWJSNIGULAAWKBEGEMAN
AWKGANGAAWKKUIJKENAWMJARVIS
AWMKUEMMELAWMSAUVAGEAWMVACCARI
AWMWETZSTEINAWNBUSCAAWOLAHAV
AWOMARGGRAFAWPHUDELOTAWRCABANAC
AWRHENDERSONAWRSAGLIAAWRWILLIAMS
AWSDESAIAWSSERJEANTAWTERBEN
AWTGIANNANTONIOAWVBECKMANNAWWVRIEND
AWYMELLIER
AWADVORNIKAWCSPINIELLOAWEHELMICH
AWEIODICEAWGDAGOAWGVERDOES
AWJDEJONGAWJMCFARLANDAWLKELVIN
AWMBILICKIAWMSPAVONEAWRPELETIER
AWTSAIFOLLAHI
AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWJBOUT
AWJMCFARLANDAWKBEGEMANAWLKELVIN
AWWVRIEND
AWATUDORICAAWAVENHOLAAWEHELMICH
AWEPETRILLOAWGVERDOESAWMVANDENBERG
AWSVATS
AWDBOXHOORNAWGVERDOESAWJMCFARLAND
AWDBOXHOORNAWEHELMICHAWGVERDOES
AWMHEEMSKERKAWMVANDENBERGAWSVATS
AWATUDORICAAWGVERDOESAWJMCFARLAND
AWABELIKOVAWEHELMICHAWGVERDOES
AWJBOUTAWJMCFARLANDAWJPIZAGNO
AWRWILLIAMS

All users

All users

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.

All users

AWEHELMICHAWGVERDOES
AWEHELMICHAWGVERDOESAWJMCFARLAND

All users

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

AWEHELMICH
AWFGETMAN
AWEVALENTYNAWGVERDOESAWJMCFARLAND

Search for comets

All users

AWEHELMICHAWGVERDOESAWJDEJONG
AWJMCFARLAND

All users

OmegaCAM/VST Guaranteed Time

All users

AWJMCFARLAND

All users

The Westerbork Northern Sky Survey

VST GTO Hercules supercluster

Ultra deep near-infrared survey for the early Universe.

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

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.

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

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

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