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

Total number of projects 88
Total number of users 394

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ID Project Privileges Instrument Member of Member count Manager(s)
1 ALL 4 None True public 1
2 MDM8K 4 MDM8K True public 1
3 OCAM@VST 4 OCAM True public 1
4 PDS 4 PDS True public 1
5 WFC@INT 4 WFC True public 1
6 WFI@2.2m 4 WFI True public 1
7 WENSS 4 WSRT True public 1
8 LOFAR 2 LOFAR False 4 1
9 SUP@SUBARU 4 SUP True public 2
10 ACS@HST 4 ACS True public 1
11 LBCBLUE@LBT 4 LBCBLUE True public 1
12 VESUVIO 4 OMEGACAM True public 1
13 OCAM ILT 2 OCAM False 10 1
14 KIDS 2 OMEGACAM False 82 32
15 COMALS 5 ACS True public 2
16 COMETS 2 None False 3 1
17 OCAMVSTGT 2 OMEGACAM False 4 1
18 STUDENTWISE 4 None True public 2
19 ATLAS3D 2 None False 1 1
20 MONICA@WENDELSTEIN 4 MONICA True public 1
21 ULTRAVISTA 2 None False 6 1
22 ISAAC@VLT 2 ISAAC False 7 1
23 LBCRED@LBT 4 LBCRED True public 1
24 WFCAM@UKIRT 4 WFCAM True public 1
25 UKIDSS 2 WFCAM False 7 2
26 MEGACAM@CFHT 4 MEGACAM True public 4
27 OCAM 2008 2 OCAM False 10 1
28 GRATAMA@BLAAUW 4 GRATAMA True public 2
29 ANDICAM@CTIO1.3m 4 ANDICAM True public 2
30 WISER 2 MEGACAM False 8 2
31 OMA 2 WFI False 4 1
32 OCAM2009 2 OCAM False 10 1
33 VIRCAM@VISTA 4 VIRCAM True public 2
34 VIKING 2 None False 37 8
35 ESOSCHMIDT@ESO1m 5 ESOSCHMIDT True public 3
36 OMEGACAM@VST 4 OMEGACAM True public 14
37 EUCLID 2 None False 50 2
38 OMEGAWHITE 2 OMEGACAM False 9 7
39 ACAM@WHT 4 ACAM True public 4
40 OMEGADWARFS 2 OMEGACAM False 12 7
41 ATLAS 4 OMEGACAM True public 5
42 VPHASPLUS 4 OMEGACAM True public 1
43 DECAM@BLANCO 4 DECAM True public 4
44 HERCULES 2 OMEGACAM False 11 7
45 VOICE 2 OMEGACAM False 22 5
46 FOCUS 2 OMEGACAM False 45 8
47 MICADO@E-ELT 4 MICADO True public 3
48 KIDS-PHOTZTEST 2 OMEGACAM False 7 5
49 SPARCS 2 DECAM False 6 6
50 OMEGACLUSTER 2 OMEGACAM False 8 5
51 AMIGADEEP 2 OMEGACAM False 8 4
52 OMEGALAE 2 OMEGACAM False 6 4
53 DEEPCLUSTERS 2 WFC False 16 9
54 KABS 2 OMEGACAM False 16 3
55 PAMC 2 OMEGACAM False 3 2
56 VEGAS 2 OMEGACAM False 8 7
57 ALICE 2 OMEGACAM False 4 3
58 YMCA 2 OMEGACAM False 6 5
101 WORKSHOP2005 2 WFI False 42 1
102 BONN2005 2 None False 15 1
103 LEIDENTUTORIAL2008 2 None False 18 2
104 TUTORIAL2014 2 None False 8 3
105 TUTORIAL2015 2 None False 15 5
106 TUTORIAL 2 None False 13 3
115 TESTCOMALS 2 ACS False 11 1
119 TESTATLAS3D 2 None False 1 1
120 A2626HA 2 INT False 2 2
201 TESTALL 2 None False 9 9
202 COMM2011 2 OMEGACAM False 16 9
301 SMASH 2 OMEGACAM False 4 4
302 TIMEDOMES 2 OMEGACAM False 6 6
303 HYPER-MAX 2 OMEGACAM False 4 4
304 GALRSG 2 OMEGACAM False 3 3
305 MHONGOOSE 2 OMEGACAM False 5 5
306 SEEING 2 OMEGACAM False 3 3
307 CRAM 2 OMEGACAM False 3 3
308 MAGNHIFFIC 2 OMEGACAM False 4 4
309 NEOVST 2 OMEGACAM False 4 4
310 SCULPTOR 2 OMEGACAM False 3 3
311 BDROT 2 OMEGACAM False 5 5
312 SEFIS 2 OMEGACAM False 3 3
313 INTERBARS 2 OMEGACAM False 3 3
314 ARP@VST 2 OMEGACAM False 5 5
315 HAGRPS 2 OMEGACAM False 4 4
316 SUITS 2 OMEGACAM False 3 3
5030 DDT295A5030 2 OMEGACAM False 5 5
9225 AWJMCFARLAND 0 None False 1 1
9233 AWDEMO 1 None False 2 2

All public data for all instruments

All users

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All public data for MDM8K

All users

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All public data for OCAM

All users

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All public data for PDS

All users

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All public data for WFC

All users

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All public data for WFI

All users

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The Westerbork Northern Sky Survey

All users

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LOw Frequency ARray - The largest radio telescope in the world

AWAUSOVAWDBOXHOORNAWEVALENTYNAWWVRIEND
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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.

All users

AWJMCFARLANDAWWVRIEND

All public data for ACS

All users

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

All users

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VST/OmegaCAM Exploration of SUperclusters Voids and Intermediate Objects

All users

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OmegaCAM lab tests

AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGVERDOES
AWJDEJONGAWJMCFARLANDAWKBEGEMANAWMTEMPELAAR
AWRVERMEIJAWWVRIEND
AWWVRIEND

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

AWABELIKOVAWACHOIAWADVORNIKAWAEDGE
AWAGRADOAWARAJAWARIFATTOAWATUDORICA
AWAWRIGHTAWBALTIERIAWBJOACHIMIAWBNAGAM
AWBSCHEERSAWBVENEMANSAWCHEYMANSAWCMORRISON
AWCSIFONAWCSPINIELLOAWCTORTORAAWDBOXHOORN
AWDKLAESAWDWILLIAMSAWEBALBINOTAWEDEUL
AWEHELMICHAWEIODICEAWEPETRILLOAWEPUDDU
AWEVALENTYNAWEVANUITERTAWFGETMANAWFKOEHLINGER
AWFLABARBERAAWGCOVONEAWGDAGOAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDTAWHHOEKSTRA
AWJDEJONGAWJMCFARLANDAWJPEACOCKAWKBEGEMAN
AWKFRANTSEVAAWKKUIJKENAWLKELVINAWLMILLER
AWMBILICKIAWMCAPACCIOLIAWMCOSTADUARTEAWMDALLORA
AWMIRWINAWMMAHLKEAWMPAOLILLOAWMRADOVICH
AWMSPAVONEAWMVIOLAAWNNAPOLITANOAWOCORDES
AWPCORCHOCABALLEROAWPHUDELOTAWPNOORISHADAWPSCHNEIDER
AWPSIMONAWRHERBONNETAWRNAKAJIMAAWRPELETIER
AWRVANDERBURGAWSDRIVERAWSLAHADAWTERBEN
AWTKITCHINGAWTLISKERAWTSAIFOLLAHIAWTSCHRABBACKKRAHE
AWTSHANKSAWWMULDERAWWSUTHERLANDAWWVRIEND
AWYDEVRIESAWZHUANG
AWADVORNIKAWAGRADOAWARAJAWARIFATTO
AWAWRIGHTAWCTORTORAAWDBOXHOORNAWDKLAES
AWEBALBINOTAWEDEULAWEHELMICHAWEPUDDU
AWEVALENTYNAWFGETMANAWGCOVONEAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONGAWJMCFARLAND
AWKKUIJKENAWMBILICKIAWMDALLORAAWMIRWIN
AWMPAOLILLOAWMRADOVICHAWNNAPOLITANOAWOCORDES
AWPCORCHOCABALLEROAWPHUDELOTAWTERBENAWWVRIEND

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

AWGVERDOESAWWVRIEND

Search for comets

AWGVERDOESAWJBOUTAWWVRIEND
AWWVRIEND

OmegaCAM/VST Guaranteed Time

AWEVALENTYNAWGVERDOESAWJMCFARLANDAWWVRIEND
AWWVRIEND

INT data for Virtual Observations lecture series

All users

AWABELIKOVAWWVRIEND

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.

AWWVRIEND
AWWVRIEND

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

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Ultra deep near-infrared survey for the early Universe.

AWEHELMICHAWGVERDOESAWJHOLTAWJMCFARLAND
AWMFRANXAWWVRIEND
AWWVRIEND

None

AWEHELMICHAWGVERDOESAWJHOLTAWJMCFARLAND
AWMFRANXAWRWILLIAMSAWWVRIEND
AWWVRIEND

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

All users

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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).

All users

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.

AWABELIKOVAWEHELMICHAWGVERDOESAWHBUDDELMEIJER
AWJMCFARLANDAWKBEGEMANAWWVRIEND
AWJMCFARLANDAWWVRIEND

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.

All users

AWGSIKKEMAAWGVERDOESAWJBOUTAWWVRIEND

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.

AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGVERDOES
AWJDEJONGAWJMCFARLANDAWKBEGEMANAWMTEMPELAAR
AWRVERMEIJAWWVRIEND
AWWVRIEND

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

AWJMCFARLANDAWWVRIEND

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

AWJMCFARLANDAWWVRIEND

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.

AWABELIKOVAWDBOXHOORNAWEHELMICHAWGVERDOES
AWJMCFARLANDAWJMWEBAZEAWKBEGEMANAWWVRIEND
AWJMCFARLANDAWWVRIEND

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.

AWABELIKOVAWGSIKKEMAAWGVERDOESAWWVRIEND
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.

AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGVERDOES
AWJDEJONGAWJMCFARLANDAWKBEGEMANAWMTEMPELAAR
AWRVERMEIJAWWVRIEND
AWWVRIEND

All public data for VIRCAM

All users

AWJMCFARLANDAWWVRIEND

Data for the VISTA Kilo-degree Infrared Galaxy survey.

AWABELIKOVAWBPILADIEZAWBVENEMANSAWCBLOKZIJL
AWCSIFONAWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWJBOUTAWJDEJONGAWJMCFARLANDAWJMWEBAZE
AWJPIZAGNOAWKBEGEMANAWKKUIJKENAWMCACCIATO
AWMCAPACCIOLIAWMNEESERAWMRADOVICHAWNIRISARRI
AWNWISSEAWPHERAUDEAUAWRBENDERAWRSAGLIA
AWRSILVOTTIAWRVANDERBURGAWRWILLIAMSAWSCASEWELL
AWSVLAARAWTERBENAWTSAIFOLLAHIAWWVRIEND
AWYMELLIER
AWABELIKOVAWEHELMICHAWGVERDOESAWJBOUT
AWJMCFARLANDAWJPIZAGNOAWRWILLIAMSAWWVRIEND

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

All users

AWEHELMICHAWGVERDOESAWWVRIEND

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.

All users

AWADVORNIKAWARAJAWDBOXHOORNAWEHELMICH
AWEVALENTYNAWFGETMANAWGSIKKEMAAWGVERDOES
AWJBOUTAWJDEJONGAWJMCFARLANDAWKKUIJKEN
AWMBILICKIAWWVRIEND

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

AWABELIKOVAWACHAMBALLUAWAJAFFEAWAPIEMONTE
AWATSYGANOVAWBDROEGEAWBNICHOLAWCBACCIGALUPI
AWCROUSSELAWCTAOAWDBOXHOORNAWEAUBOURG
AWEHELMICHAWEVALENTYNAWFABDALLAAWFRAISON
AWGBLANCAWGSIKKEMAAWGVERDOESAWHBUDDELMEIJER
AWJDEJONGAWJKOPPENHOEFERAWJMCFARLANDAWJMOHR
AWJPIZAGNOAWJSNIGULAAWKBEGEMANAWKGANGA
AWKKUIJKENAWMJARVISAWMKUEMMELAWMSAUVAGE
AWMVACCARIAWMWETZSTEINAWNBUSCAAWOLAHAV
AWOMARGGRAFAWPHUDELOTAWRCABANACAWRHENDERSON
AWRSAGLIAAWRWILLIAMSAWSDESAIAWSSERJEANT
AWTERBENAWTGIANNANTONIOAWVBECKMANNAWWMULDER
AWWVRIENDAWYMELLIER
AWEHELMICHAWWVRIEND

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/

AWDBOXHOORNAWEHELMICHAWGRAMSAYAWGVERDOES
AWKBEGEMANAWPGROOTAWRTOMAAWSMACFARLANE
AWWVRIEND
AWDBOXHOORNAWEHELMICHAWGVERDOESAWKBEGEMAN
AWPGROOTAWSMACFARLANEAWWVRIEND

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

AWEHELMICHAWGVERDOESAWJMCFARLANDAWWVRIEND

None

AWDBOXHOORNAWEHELMICHAWETOLSTOYAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJMCFARLANDAWKKUIJKENAWTDEBOERAWWVRIEND
AWEHELMICHAWETOLSTOYAWGSIKKEMAAWGVERDOES
AWJDEJONGAWTDEBOERAWWVRIEND

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.

All users

AWEHELMICHAWGVERDOESAWJDEJONGAWJMCFARLAND
AWWVRIEND

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

All users

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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

AWATUDORICAAWGVERDOESAWJMCFARLANDAWWVRIEND

VST GTO Hercules supercluster

AWDBOXHOORNAWEHELMICHAWEVALENTYNAWGSIKKEMA
AWGVERDOESAWJBOUTAWJMCFARLANDAWKBEGEMAN
AWLKELVINAWRBUTAAWWVRIEND
AWDBOXHOORNAWEVALENTYNAWGVERDOESAWJBOUT
AWJMCFARLANDAWKBEGEMANAWWVRIEND

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

AWACHOIAWCHEYMANSAWCSIFONAWDAPPLEGATE
AWDBOXHOORNAWEHELMICHAWFGETMANAWGCOVONE
AWGSIKKEMAAWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWJDEJONGAWJMCFARLANDAWKKUIJKENAWMRADOVICH
AWMVACCARIAWMVIOLAAWNNAPOLITANOAWRVANDERBURG
AWTERBENAWWVRIEND
AWEHELMICHAWGCOVONEAWGVERDOESAWMVACCARI
AWWVRIEND

FOrnax Cluster Ultradeep Survey

AWABOSELLIAWAGRADOAWAHELMIAWALONI
AWARAJAWASUAWAVENHOLAAWDBOXHOORN
AWEGREBELAWEHELMICHAWEIODICEAWELAURIKAINEN
AWETOLOBAAWEVALENTYNAWFGETMANAWFLABARBERA
AWFMACCAGNIAWGHENSLERAWGSIKKEMAAWGVANDEVEN
AWGVERDOESAWHBUDDELMEIJERAWHSALOAWJDEJONG
AWJFALCONBARROSOAWJJANZAWJMCFARLANDAWKKUIJKEN
AWMCAPACCIOLIAWMHILKERAWMPAOLLILOAWMSPAVONE
AWNNAPOLITANOAWNZABELAWRMUNOZAWRPELETIER
AWSMIESKEAWSPAUDELAWSSENAWSTRAGER
AWTLISKERAWTPUZIAAWTSAIFOLLAHIAWVSPRINGEL
AWWVRIEND
AWAVENHOLAAWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWJMCFARLANDAWRPELETIERAWWVRIEND

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

All users

AWGVERDOESAWJMCFARLANDAWWVRIEND

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

AWDBOXHOORNAWEHELMICHAWGVERDOESAWHHILDEBRANDT
AWJDEJONGAWKKUIJKENAWWVRIEND
AWEHELMICHAWGVERDOESAWJDEJONGAWKKUIJKEN
AWWVRIEND

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.

AWATUDORICAAWEHELMICHAWGVERDOESAWHHILDEBRANDT
AWJMCFARLANDAWWVRIEND
AWATUDORICAAWEHELMICHAWGVERDOESAWHHILDEBRANDT
AWJMCFARLANDAWWVRIEND

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

AWDBOXHOORNAWEHELMICHAWGVERDOESAWMHEEMSKERK
AWMVANDENBERGAWSVATSAWTSAIFOLLAHIAWWVRIEND
AWEHELMICHAWGVERDOESAWMVANDENBERGAWSVATS
AWWVRIEND

Search for faint features in the outskirts of isolated galaxies

AWAVENHOLAAWDBOXHOORNAWEHELMICHAWGVERDOES
AWJMCFARLANDAWPRAMIREZMORETAAWRPELETIERAWWVRIEND
AWEHELMICHAWGVERDOESAWJMCFARLANDAWWVRIEND

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

AWDBOXHOORNAWDSOBRALAWGVERDOESAWJMATTHEE
AWJMCFARLANDAWWVRIEND
AWDBOXHOORNAWGVERDOESAWJMCFARLANDAWWVRIEND

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.

AWARAMESHAWAVENHOLAAWBLAPAWDBOXHOORN
AWEHELMICHAWGSIKKEMAAWGVERDOESAWJDEJONG
AWJMCFARLANDAWJVANDENBORNAWNCHOQUEAWPMANCERAPINA
AWRPELETIERAWSSENAWTVOSAWWVRIEND
AWAVENHOLAAWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWJDEJONGAWJMCFARLANDAWNCHOQUEAWPMANCERAPINA
AWWVRIEND

KiDS ATLAS Bridging Survey

AWARAJAWARIFATTOAWDBOXHOORNAWEPUDDU
AWEVALENTYNAWFGETMANAWFLABARBERAAWGVERDOES
AWJDEJONGAWKKUIJKENAWMDALLORAAWMPAOLILLO
AWMRADOVICHAWNNAPOLITANOAWTSAIFOLLAHIAWWVRIEND
AWARAJAWFGETMANAWWVRIEND

Probing the accretion of matter around massive galaxy clusters with splashback

AWDBOXHOORNAWOCONTIGIANIAWWVRIEND
AWOCONTIGIANIAWWVRIEND

None

AWALONIAWDBOXHOORNAWEIODICEAWMPAOLILLO
AWMRADOVICHAWMSPAVONEAWRCALVIAWWVRIEND
AWALONIAWDBOXHOORNAWEIODICEAWMPAOLILLO
AWMSPAVONEAWRCALVIAWWVRIEND

In this project we observed with VST-OmegaCam in the ugri bands a sample of galaxy clusters selected from the Planck-SZ catalog at different redshifts. The data will be used to calibrate the mass estimate of the clusters by weak-lensing and the cluster mass/richness relation, that will be applied to larger samples available from other surveys such as KiDS

AWDBOXHOORNAWFGETMANAWMRADOVICHAWWVRIEND
AWFGETMANAWMRADOVICHAWWVRIEND

A survey to study the star formation history and the extended structure of the outskirts of the Magellanic Clouds

AWDBOXHOORNAWFCIBARDOAWMGATTOAWMSPAVONE
AWVRIPEPIAWWVRIEND
AWDBOXHOORNAWMGATTOAWMSPAVONEAWVRIPEPI
AWWVRIEND

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

AWAGRADOAWANONYMOUSAWAROJBIAWCHAINES
AWDBOXHOORNAWDWILMANAWEBERTINAWEDEUL
AWEHELMICHAWEVALENTYNAWFGETMANAWGFEULNER
AWGSIKKEMAAWGVERDOESAWHHILDEBRANDTAWJDIETRICH
AWJKOPPENHOEFERAWJMCFARLANDAWJSNIGULAAWKBEGEMAN
AWKKOVACAWKKUIJKENAWLHABERZETTLAWLMORALESRUEDA
AWMNEESERAWMPAVLOVAWMPOHLENAWMSMIT
AWMTEMPELAARAWNRAMANUJAMAWOCORDESAWOSCHMITHUESEN
AWPGROOTAWPHERAUDEAUAWRRENGELINKAWRSILVOTTI
AWRVERMEIJAWSLECCIAAWTERBENAWTSCHNEIDER
AWWVRIENDAWYMELLIER
AWWVRIEND

Test project for AIUB

AWBBURGGRAFAWCTRACHTERNACHAWDBOMANSAWDROSENBAUM
AWFBRIMIOULLEAWHHILDEBRANDTAWHISRAELAWJDIETRICH
AWKWEISAWMLERCHSTERAWOCORDESAWOSCHMITHUESEN
AWTERBENAWTSCHRABBACKKRAHEAWWVRIEND
AWWVRIEND

Leiden Tutorial. August 18-20.

AWEDEMOOIJAWEDEULAWEHELMICHAWEVANUITERT
AWGVERDOESAWHHILDEBRANDTAWISNELLENAWJHOLT
AWJMCFARLANDAWKKUIJKENAWKVERBEEKAWMFRANX
AWMSMITAWMVELANDERAWOSPOORENAWRWILLIAMS
AWTSCHRABBACKKRAHEAWWVRIEND
AWJMCFARLANDAWWVRIEND

Groningen tutorial, July 10 and 11.

AWATUDORICAAWAVENHOLAAWEHELMICHAWEPETRILLO
AWGVERDOESAWMVANDENBERGAWSVATSAWWVRIEND
AWEHELMICHAWGVERDOESAWWVRIEND

Sandbox for Astro-WISE tutorial users.

AWADVORNIKAWASUAWCSPINIELLOAWEHELMICH
AWEIODICEAWGDAGOAWGVERDOESAWJDEJONG
AWJMCFARLANDAWLKELVINAWMBILICKIAWMSPAVONE
AWRPELETIERAWTSAIFOLLAHIAWWVRIEND
AWEHELMICHAWGVERDOESAWJDEJONGAWJMCFARLAND
AWWVRIEND

Sandbox for Astro-WISE tutorial users.

AWASAVINOAWDBOXHOORNAWDDINGAWEHELMICH
AWJDEJONGAWKFRANTSEVAAWMMAHLKEAWNCHOQUE
AWOCONTIGIANIAWPMANCERAPINAAWTNUTMAAWWVRIEND
AWYDEVRIES
AWEHELMICHAWJDEJONGAWWVRIEND

The HST-ACS Coma Legacy Survey

AWAKARICKAWCOMALSAWDBOXHOORNAWEHELMICH
AWEVALENTYNAWGVERDOESAWJMCFARLANDAWLDOMINGUEZ
AWMDENBROKAWMTEMPELAARAWWVRIEND
AWWVRIEND

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.

AWWVRIEND
AWWVRIEND

Abell 2626 H-alpha

AWDBOXHOORNAWNCHOQUE
AWDBOXHOORNAWNCHOQUE

For testing purposes only.

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

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AWEVALENTYNAWGSIKKEMAAWGVERDOESAWHBUDDELMEIJER
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AWGVERDOESAWJBOUTAWJDEJONGAWJMCFARLAND
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VST-SMASH (The VST Survey of Mass Assembly and Structural Hierarchy) will perform surface photometry of nearby galaxies in g, r and i, aiming at exploring the galaxy outskirts down to 29 mag arcsec^-2 in g and r and 26 mag arcsec^-2 in i-band

AWAUNNIAWCTORTORAAWDBOXHOORNAWMSPAVONE
AWAUNNIAWCTORTORAAWDBOXHOORNAWMSPAVONE

Project devoted to the temporal monitoring of the LSST Deep Drilling Fields

AWDBOXHOORNAWDDECICCOAWMFATOVICAWMPAOLILLO
AWMSPAVONEAWVPETRECCA
AWDBOXHOORNAWDDECICCOAWMFATOVICAWMPAOLILLO
AWMSPAVONEAWVPETRECCA

Follow-up program for the photometric coverage of XMM HYPERION QSO fields

AWDBOXHOORNAWDDECICCOAWMPAOLILLOAWMSPAVONE
AWDBOXHOORNAWDDECICCOAWMPAOLILLOAWMSPAVONE

Pre-SN outbursts in Galactic Red Supergiants: predicting the next Galactic SN event

AWDBOXHOORNAWFBOCCHINOAWMSPAVONE
AWDBOXHOORNAWFBOCCHINOAWMSPAVONE

Disentangling gas accretion in nearby deep optical and radio observations

AWDBOXHOORNAWDKLEINERAWFMACCAGNIAWJHEALY
AWMSPAVONE
AWDBOXHOORNAWDKLEINERAWFMACCAGNIAWJHEALY
AWMSPAVONE

Stellar Explosions and their Evolution In Nearby Galaxies - SEEING

AWDBOXHOORNAWLIZZOAWMSPAVONE
AWDBOXHOORNAWLIZZOAWMSPAVONE

Cosmic Rays Accelerators Measurements

AWDBOXHOORNAWIBUSAAWMSPAVONE
AWDBOXHOORNAWIBUSAAWMSPAVONE

MeerKAT AGN HI Feeding and Feedback Investigation Close-by is a survey of 22 nearby Active Galactic Nuclei (AGN) performing sensitive observations of the neutral hydrogen (HI) in nearby Active Galactic Nuclei (AGN), in combination with deep photometrical obserations

AWDBOXHOORNAWDKLEINERAWFMACCAGNIAWJHEALY
AWDBOXHOORNAWDKLEINERAWFMACCAGNIAWJHEALY

None

AWDBOXHOORNAWDPERNAAWMSPAVONEAWPHASSELMANN
AWDBOXHOORNAWDPERNAAWMSPAVONEAWPHASSELMANN

Near-field cosmology with the dwarf galaxy system of the Sculptor group

AWDBOXHOORNAWMSPAVONEAWNHEESTERS
AWDBOXHOORNAWMSPAVONEAWNHEESTERS

We are monitoring 8 young clusters for 5 days in one passband with a 5 minute cadence. The magnitude limit covers the substellar range and we expect to find rotation rates for UCDs

AWDBOXHOORNAWEDISTEFANOAWMSPAVONEAWNLODIEU
AWRSMART
AWDBOXHOORNAWEDISTEFANOAWMSPAVONEAWNLODIEU
AWRSMART

Search for RR Lyrae stars in the ultra-faint dwarf galaxy Sextans II

AWDBOXHOORNAWMGATTOAWMSPAVONE
AWDBOXHOORNAWMGATTOAWMSPAVONE

Stellar bars can form during galaxy-galaxy interactions, which produce an asymmetric distribution of the ionised gas and star formation rate along the bar and in the disc. To con¿¿¿rm whether an interaction is responsible for the bar formation, we obtained deep photometry with the OmegaCAM at VLT Survey telescope using the Halpha ¿¿¿lter for a sample of barred galaxies experiencing di¿¿¿erent galaxy-galaxy interactions and we will derive ionized gas and star formation rate maps.

AWDBOXHOORNAWMSPAVONEAWVCUOMO
AWDBOXHOORNAWMSPAVONEAWVCUOMO

Public survey of the ARP peculiar galaxies with the VST

AWALONIAWDBOXHOORNAWEIODICEAWMSPAVONE
AWRCALVI
AWALONIAWDBOXHOORNAWEIODICEAWMSPAVONE
AWRCALVI

A deep H¿¿ imaging survey of intermediate mass groups (logMhalo = 13-14) in the Local Supercluster

AWDBOXHOORNAWEMANGOLAAWMFOSSATIAWMSPAVONE
AWDBOXHOORNAWEMANGOLAAWMFOSSATIAWMSPAVONE

Searching for UDGs In the Tails of Stripped gas of GASP Jellyfish galaxies

AWDBOXHOORNAWMSPAVONEAWRCALVI
AWDBOXHOORNAWMSPAVONEAWRCALVI

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

AWDBOXHOORNAWJDEJONGAWJMCFARLANDAWNNAPOLITANO
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MYDB for JMCFARLAND

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MYDB for AWDEMO

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AWDEMOAWWVRIEND

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