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

Total number of projects 69
Total number of users 342

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 75 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 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 11 6
45 VOICE 2 OMEGACAM False 21 4
46 FOCUS 2 OMEGACAM False 39 7
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
AWACHOIAWCHEYMANSAWCSIFON
AWDAPPLEGATEAWDBOXHOORNAWEHELMICH
AWFGETMANAWGCOVONEAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWJDEJONGAWJMCFARLANDAWKKUIJKEN
AWMRADOVICHAWMVACCARIAWMVIOLA
AWNNAPOLITANOAWRVANDERBURGAWTERBEN
AWADVORNIKAWARAJAWDBOXHOORN
AWEHELMICHAWEVALENTYNAWFGETMAN
AWGSIKKEMAAWGVERDOESAWJBOUT
AWJDEJONGAWJMCFARLANDAWMBILICKI

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

AWAVENHOLAAWDBOXHOORNAWEHELMICH
AWGSIKKEMAAWGVERDOESAWJMCFARLAND
AWRPELETIER

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

All users

VST GTO Hercules supercluster

AWEHELMICHAWGVERDOES

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

All public data for WFI

AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWJBOUT
AWJMCFARLANDAWKBEGEMANAWLKELVIN
AWRBUTAAWWVRIEND
AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGVERDOESAWJDEJONGAWJMCFARLAND
AWKBEGEMANAWMTEMPELAARAWRVERMEIJ
AWWVRIEND

None

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.

OmegaCAM lab tests

All users

AWEHELMICHAWGCOVONEAWGVERDOES
AWMVACCARI
AWDBOXHOORNAWEIODICEAWMSPAVONE

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.

Sandbox for Astro-WISE tutorial users.

AWDBOXHOORNAWJDEJONGAWJMCFARLAND
AWNNAPOLITANO

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.

AWEHELMICHAWGVERDOESAWJMCFARLAND
AWEHELMICHAWGVERDOESAWMVANDENBERG
AWSVATS
AWWVRIEND
AWAVENHOLAAWDBOXHOORNAWEHELMICH
AWGSIKKEMAAWJDEJONGAWJMCFARLAND
AWNCHOQUEAWPMANCERAPINA
AWABELIKOVAWEHELMICHAWGVERDOES
AWJBOUTAWJMCFARLANDAWJPIZAGNO
AWRWILLIAMS

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.

Probing the accretion of matter around massive galaxy clusters with splashback

OmegaCAM/VST Guaranteed Time

AWARAJAWFGETMAN
AWBBURGGRAFAWCTRACHTERNACHAWDBOMANS
AWDROSENBAUMAWFBRIMIOULLEAWHHILDEBRANDT
AWHISRAELAWJDIETRICHAWKWEIS
AWMLERCHSTERAWOCORDESAWOSCHMITHUESEN
AWTERBENAWTSCHRABBACKKRAHE

All users

AWABELIKOV

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 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.

AWDBOXHOORNAWEHELMICHAWGVERDOES
AWKBEGEMANAWPGROOTAWSMACFARLANE

All users

AWGSIKKEMAAWGVERDOESAWJBOUT

The Westerbork Northern Sky Survey

AWEHELMICHAWGVERDOESAWJHOLT
AWJMCFARLANDAWMFRANXAWRWILLIAMS
AWABELIKOVAWDBOXHOORNAWEDEUL
AWEHELMICHAWEVALENTYNAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJBOUT
AWJDEJONGAWJMCFARLANDAWJPIZAGNO
AWKBEGEMANAWKKUIJKENAWRHOOK
AWWVRIEND
AWEHELMICH

For testing purposes only.

All users

AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGVERDOESAWJDEJONGAWJMCFARLAND
AWKBEGEMANAWMTEMPELAARAWRVERMEIJ
AWWVRIEND

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

AWDBOXHOORNAWEIODICEAWMSPAVONE
AWARAMESHAWAVENHOLAAWBLAP
AWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWJDEJONGAWJMCFARLAND
AWJVANDENBORNAWNCHOQUEAWPMANCERAPINA
AWRPELETIERAWTVOS

KiDS ATLAS Bridging Survey

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.

AWEHELMICHAWGVERDOESAWJMCFARLAND

All public data for OCAM

None

AWATUDORICAAWEHELMICHAWGVERDOES
AWHHILDEBRANDTAWJMCFARLAND

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.

AWEHELMICHAWGVERDOESAWJDEJONG
AWJMCFARLAND
AWEHELMICHAWJDEJONG
AWABELIKOVAWDBOXHOORNAWEHELMICH
AWGVERDOESAWJMCFARLANDAWJMWEBAZE
AWKBEGEMANAWWVRIEND
AWOCONTIGIANI

Search for comets

MYDB for JMCFARLAND

Groningen tutorial, July 10 and 11.

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.

AWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJMCFARLANDAWKBEGEMANAWWVRIEND

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

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

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

AWABOSELLIAWAGRADOAWAHELMI
AWARAJAWAVENHOLAAWDBOXHOORN
AWEGREBELAWEHELMICHAWEIODICE
AWELAURIKAINENAWETOLOBAAWEVALENTYN
AWFGETMANAWFLABARBERAAWGHENSLER
AWGSIKKEMAAWGVANDEVENAWGVERDOES
AWHBUDDELMEIJERAWHSALOAWJDEJONG
AWJFALCONBARROSOAWJJANZAWJMCFARLAND
AWKKUIJKENAWMCAPACCIOLIAWMHILKER
AWMPAOLLILOAWMSPAVONEAWNNAPOLITANO
AWRMUNOZAWRPELETIERAWSMIESKE
AWSPAUDELAWSTRAGERAWTLISKER
AWTPUZIAAWTSAIFOLLAHIAWVSPRINGEL

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

AWDBOXHOORNAWJDEJONGAWJMCFARLAND
AWNNAPOLITANO

All users

AWJMCFARLAND
AWJMCFARLAND
AWJMCFARLAND
AWAVENHOLAAWDBOXHOORNAWEHELMICH
AWGVERDOESAWJMCFARLANDAWPRAMIREZMORETA
AWRPELETIER
AWEHELMICHAWETOLSTOYAWGSIKKEMA
AWGVERDOESAWJDEJONGAWTDEBOER

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 users

Data for the VISTA Kilo-degree Infrared Galaxy survey.

All users

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

AWABELIKOVAWGSIKKEMAAWGVERDOES

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.

Ultra deep near-infrared survey for the early Universe.

AWATUDORICAAWGVERDOESAWJMCFARLAND
AWGVERDOESAWJBOUT
AWGVERDOESAWJMCFARLANDAWWVRIEND
AWDBOXHOORNAWEHELMICHAWGVERDOES
AWHHILDEBRANDTAWJDEJONGAWKKUIJKEN

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

AWADVORNIKAWCSPINIELLOAWEHELMICH
AWEIODICEAWGDAGOAWGVERDOES
AWJDEJONGAWJMCFARLANDAWLKELVIN
AWMBILICKIAWMSPAVONEAWRPELETIER
AWTSAIFOLLAHI

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

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

LOw Frequency ARray - The largest radio telescope in the world

AWABELIKOVAWACHOIAWADVORNIK
AWAEDGEAWAGRADOAWARAJ
AWARIFATTOAWATUDORICAAWAWRIGHT
AWBALTIERIAWBJOACHIMIAWBVENEMANS
AWCHEYMANSAWCMORRISONAWCSIFON
AWCSPINIELLOAWCTORTORAAWDBOXHOORN
AWDKLAESAWDWILLIAMSAWEDEUL
AWEHELMICHAWEIODICEAWEPETRILLO
AWEPUDDUAWEVALENTYNAWEVANUITERT
AWFGETMANAWFKOEHLINGERAWFLABARBERA
AWGCOVONEAWGDAGOAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWHHILDEBRANDT
AWHHOEKSTRAAWJDEJONGAWJMCFARLAND
AWJPEACOCKAWKBEGEMANAWKFRANTSEVA
AWKKUIJKENAWLKELVINAWLMILLER
AWMBILICKIAWMCAPACCIOLIAWMCOSTADUARTE
AWMDALLORAAWMIRWINAWMMAHLKE
AWMPAOLILLOAWMRADOVICHAWMSPAVONE
AWMVIOLAAWNNAPOLITANOAWOCORDES
AWPHUDELOTAWPNOORISHADAWPSCHNEIDER
AWPSIMONAWRHERBONNETAWRNAKAJIMA
AWRPELETIERAWRVANDERBURGAWSDRIVER
AWTERBENAWTKITCHINGAWTLISKER
AWTSCHRABBACKKRAHEAWTSHANKSAWWSUTHERLAND
AWWVRIENDAWYDEVRIESAWZHUANG
AWEVALENTYNAWGVERDOESAWJMCFARLAND

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

All users

AWDBOXHOORNAWEHELMICHAWETOLSTOY
AWEVALENTYNAWGSIKKEMAAWGVERDOES
AWHBUDDELMEIJERAWJDEJONGAWJMCFARLAND
AWKKUIJKENAWTDEBOER

All users

AWEDEMOOIJAWEDEULAWEHELMICH
AWEVANUITERTAWGVERDOESAWHHILDEBRANDT
AWISNELLENAWJHOLTAWJMCFARLAND
AWKKUIJKENAWKVERBEEKAWMFRANX
AWMSMITAWMVELANDERAWOSPOOREN
AWRWILLIAMSAWTSCHRABBACKKRAHE

All users

AWJMCFARLAND

All public data for WFC

AWEHELMICHAWGVERDOESAWJHOLT
AWJMCFARLANDAWMFRANX

Sandbox for Astro-WISE tutorial users.

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.

VST/OmegaCAM Exploration of SUperclusters Voids and Intermediate Objects

FOrnax Cluster Ultradeep Survey

AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGSIKKEMAAWGVERDOESAWJBOUT
AWJDEJONGAWJMCFARLAND
AWATUDORICAAWEHELMICHAWGVERDOES
AWHHILDEBRANDTAWJMCFARLAND
AWADVORNIKAWAGRADOAWARAJ
AWARIFATTOAWAWRIGHTAWCTORTORA
AWDBOXHOORNAWDKLAESAWEDEUL
AWEHELMICHAWEPUDDUAWEVALENTYN
AWFGETMANAWGCOVONEAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJMCFARLANDAWKKUIJKENAWMBILICKI
AWMDALLORAAWMIRWINAWMPAOLILLO
AWMRADOVICHAWNNAPOLITANOAWOCORDES
AWPHUDELOTAWTERBEN

All users

AWJMCFARLAND

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

AWABELIKOVAWACHAMBALLUAWAJAFFE
AWAPIEMONTEAWATSYGANOVAWBDROEGE
AWBNICHOLAWCBACCIGALUPIAWCROUSSEL
AWCTAOAWDBOXHOORNAWEAUBOURG
AWEHELMICHAWEVALENTYNAWFABDALLA
AWFRAISONAWGBLANCAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJKOPPENHOEFERAWJMCFARLANDAWJMOHR
AWJPIZAGNOAWJSNIGULAAWKBEGEMAN
AWKGANGAAWKKUIJKENAWMJARVIS
AWMKUEMMELAWMSAUVAGEAWMVACCARI
AWMWETZSTEINAWNBUSCAAWOLAHAV
AWOMARGGRAFAWPHUDELOTAWRCABANAC
AWRHENDERSONAWRSAGLIAAWRWILLIAMS
AWSDESAIAWSSERJEANTAWTERBEN
AWTGIANNANTONIOAWVBECKMANNAWWVRIEND
AWYMELLIER
AWEHELMICHAWGVERDOESAWJDEJONG
AWJMCFARLAND

MYDB for AWDEMO

AWAUSOVAWDBOXHOORNAWEVALENTYN
AWWVRIEND

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.

AWABELIKOVAWEHELMICHAWGVERDOES
AWHBUDDELMEIJERAWJMCFARLANDAWKBEGEMAN

All public data for all instruments

AWDBOXHOORNAWEHELMICHAWEVALENTYN
AWGVERDOESAWJDEJONGAWJMCFARLAND
AWKBEGEMANAWMTEMPELAARAWRVERMEIJ
AWWVRIEND
AWDBOXHOORNAWEVALENTYNAWGVERDOES
AWJBOUTAWJMCFARLANDAWKBEGEMAN

All users

AWDBOXHOORNAWEHELMICHAWGSIKKEMA
AWGVERDOESAWHBUDDELMEIJERAWJDEJONG
AWJMCFARLANDAWKBEGEMANAWWVRIEND
AWASAVINOAWDBOXHOORNAWDDING
AWEHELMICHAWJDEJONGAWKFRANTSEVA
AWMMAHLKEAWNCHOQUEAWOCONTIGIANI
AWPMANCERAPINAAWTNUTMAAWYDEVRIES

The HST-ACS Coma Legacy Survey

AWDBOXHOORNAWGVERDOESAWJMCFARLAND

All public data for ACS

All public data for PDS

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.

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.

All public data for MDM8K

AWJMCFARLAND
AWDBOXHOORNAWDSOBRALAWGVERDOES
AWJMATTHEEAWJMCFARLAND

Search for faint features in the outskirts of isolated galaxies

AWDBOXHOORNAWEHELMICHAWGVERDOES
AWMHEEMSKERKAWMVANDENBERGAWSVATS

All public data for VIRCAM

All users

AWGVERDOES

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.

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

Test project for AIUB

All users

AWAKARICKAWCOMALSAWDBOXHOORN
AWEHELMICHAWEVALENTYNAWGVERDOES
AWJMCFARLANDAWLDOMINGUEZAWMDENBROK
AWMTEMPELAAR
AWATUDORICAAWAVENHOLAAWEHELMICH
AWEPETRILLOAWGVERDOESAWMVANDENBERG
AWSVATS

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

AWEHELMICHAWGVERDOES

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

AWJMCFARLAND

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/

All users

AWOCONTIGIANI

INT data for Virtual Observations lecture series

All users

AWEHELMICHAWGVERDOESAWJDEJONG
AWKKUIJKEN

All users

AWDBOXHOORNAWEHELMICHAWGRAMSAY
AWGVERDOESAWKBEGEMANAWPGROOT
AWRTOMAAWSMACFARLANE

None

Leiden Tutorial. August 18-20.

All users

All users

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

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

All users

AWARAJAWARIFATTOAWDBOXHOORN
AWEPUDDUAWEVALENTYNAWFGETMAN
AWFLABARBERAAWGVERDOESAWJDEJONG
AWKKUIJKENAWMDALLORAAWMPAOLILLO
AWMRADOVICHAWNNAPOLITANO

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