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- ID:
- ivo://asu.cas.cz/extract_jan18/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LCs
- Date:
- 08 Jan 2018 15:30:12
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- DK-154 SSAP interpreted lightcurves
- ID:
- ivo://asu.cas.cz/extract_dec17/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LCs
- Date:
- 08 Jan 2018 15:30:12
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- DK-154 SSAP interpreted lightcurves
- ID:
- ivo://asu.cas.cz/extract_jan16/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LC
- Date:
- 30 Nov 2017 09:39:26
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- SSAP interpreted lightcurves
- ID:
- ivo://asu.cas.cz/extract_jul16/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LCs
- Date:
- 19 May 2017 01:42:07
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- DK-154 SSAP interpreted lightcurves
- ID:
- ivo://svo.cab/omc/ssap
- Title:
- OMC: The INTEGRAL Optical Monitoring Camera
- Short Name:
- OMC SSA
- Date:
- 04 Sep 2019 08:32:02
- Publisher:
- SVO
- Description:
- The Optical Monitoring Camera (OMC) observes the optical emission from the prime targets of the gamma-ray instruments on-board the ESA mission INTEGRAL (launched on Oct. 17, 2002). OMC has also the capability to monitor serendipitously a large number of optically variable sources within its field of view.
- ID:
- ivo://anusf.anu.au/macho
- Title:
- The Massive Compact Halo Object (MACHO) Project Data Archive
- Short Name:
- MACHO
- Date:
- 18 Jun 2019 20:15:24
- Publisher:
- ivo://anusf.anu.au
- Description:
- The MACHO Project was a collaboration between scientists at the Mt. Stromlo and Siding Spring Observatories, the Center for Particle Astrophysics at the Santa Barbara, San Diego, and Berkeley campuses of the University of California, and the Lawrence Livermore National Laboratory. Our primary aim was to test the hypothesis that a significant fraction of the dark matter in the halo of the Milky Way is made up of objects like brown dwarfs or planets: these objects have come to be known as MACHOs, for MAssive Compact Halo Objects. The signature of these objects is the occasional amplification of the light from extragalactic stars by the gravitational lens effect. The amplification can be large, but events are extremely rare: it was necessary to monitor photometrically several million stars for a period of 10 years in order to obtain a useful detection rate. For this purpose we built a two channel system that employed eight 2048*2048 CCDs, mounted on the 50 inch telescope at Mt. Stromlo. The MACHO project data archive consists of approximately 127,000 two-colour images of fields collected between 1992 and 2003 covering the large and small Magellanic clouds and the galactic bulge and two-colour light-curves for approximately 18 million stars in the LMC and galactic bulge.
- ID:
- ivo://nci.org.au/macho
- Title:
- The Massive Compact Halo Object (MACHO) Project Data Archive
- Short Name:
- MACHO
- Date:
- 23 Jul 2015 02:55:45
- Publisher:
- ivo://nci.org.au
- Description:
- The MACHO Project was a collaboration between scientists at the Mt. Stromlo and Siding Spring Observatories, the Center for Particle Astrophysics at the Santa Barbara, San Diego, and Berkeley campuses of the University of California, and the Lawrence Livermore National Laboratory. Our primary aim was to test the hypothesis that a significant fraction of the dark matter in the halo of the Milky Way is made up of objects like brown dwarfs or planets: these objects have come to be known as MACHOs, for MAssive Compact Halo Objects. The signature of these objects is the occasional amplification of the light from extragalactic stars by the gravitational lens effect. The amplification can be large, but events are extremely rare: it was necessary to monitor photometrically several million stars for a period of 10 years in order to obtain a useful detection rate. For this purpose we built a two channel system that employed eight 2048*2048 CCDs, mounted on the 50 inch telescope at Mt. Stromlo. The MACHO project data archive consists of approximately 127,000 two-colour images of fields collected between 1992 and 2003 covering the large and small Magellanic clouds and the galactic bulge and two-colour light-curves for approximately 18 million stars in the LMC and galactic bulge.
