B/subaruivo://CDS.VizieR/B/subaruCDSADAC NAOJ2007-09-01T17:23:34Z2007-09-01T17:18:30ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frobservational-astronomyThis database contains a log of the Subaru Prime Focus Camera (Suprime-Cam) exposures since April 2001. The data are regularly updated, and the last date of the log is written in "File Summary". Note that from this version of Nov. 2005, the data number is largely increased because those data with worse position determination (up to 30 arcsec error) are included. Suprime-Cam is an 80-mega pixels (10240 x 8192) mosaic CCD camera, for the wide-field prime focus of the 8.2m Subaru telescope. Suprime-Cam covers a field of view 34'x27', a unique facility among the 8-10m class telescopes, with a resolution of 0".202 per pixel. The focal plane consists of ten high- resistivity 2kx2k CCDs developed by MIT Lincoln Laboratory, which are cooled by a large Stirling-cycle cooler. The CCD readout electronics was designed to be scalable, which allows the multiple read-out of tens of CCDs. It takes 50 seconds to readout entire arrays. A filter-exchange mechanism of the jukebox type is designed that can hold up to ten large filters (205x170x15mm^3^). The wide-field corrector is basically a three-lens Wynne- type, but has a new type of atmospheric dispersion corrector. The corrector provides a flat focal plane and an un-vignetted field of view of 30' in diameter. The achieved co-planarity of the focal array mosaic is smaller than 30um peak-to-peak, which realizes mostly the seeing limited image over the entire field. The median seeing in the I_c-band, measured over one year and a half, is 0".61. The PSF anisotropy in Suprime-Cam images, estimated by stellar ellipticities, is about 2% under this median seeing condition. At the time of commissioning, Suprime-Cam had the largest survey speed, which is defined as the field of view multiplied by the primary mirror area of the telescope, among those cameras built for sub-arcsecond imaging. For details, see: Miyazaki et al., Publ. Astron. Soc. Japan 54, 833-853, 2002 (2002PASJ...54..833M)Astronomical Data Analysis Center,https://cdsarc.cds.unistra.fr/viz-bin/cat/B/subaruCatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-tohttp://subarutelescope.org/Observing/Instruments/SCam/ :http://smoka.nao.ac.jp/ :https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=B/subaruhttps://vizier.iucaa.in/viz-bin/VizieR-2?-source=B/subaruhttp://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=B/subaruhttps://vizier.cds.unistra.fr/viz-bin/votable?-source=B/subaruhttps://vizier.iucaa.in/viz-bin/votable?-source=B/subaruhttp://vizieridia.saao.ac.za/viz-bin/votable?-source=B/subaruGETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table B/subaru/suprimc (The Suprime-Cam Observation Log (2005-11-02))https://vizier.cds.unistra.fr/viz-bin/conesearch/B/subaru/suprimc?https://vizier.iucaa.in/viz-bin/conesearch/B/subaru/suprimc?http://vizieridia.saao.ac.za/viz-bin/conesearch/B/subaru/suprimc?GETtext/xml+votable180.050000true172.37447.59620.0055555555555555565/108 257 651 655 658 667 1074 1085 1087 1097 1101 1156 1169 1172 1173 1177 1178 1191 1195 1196 1197 1198 1200 1275 1517 1537 1538 2374 2538 2542 2574 2621 2906 2917 4422 4423 4433 4435 4438 4508 4523 4535 4536 4570 4571 4572 4593 4612 4613 4635 4638 4641 4642 4644 4692 4715 4758 4759 4775 4945 4948 4950 4951 5983 6002 6003 6008 6009 6046 6084 6267 6430 6438 6445 6814 6885 6893 6894 7133 7229 7230 7231 7313 7316 7429 7451 7454 7753 7780 7782 7848 7849 8076 9211 9713 11229 12113 12143 12151 12156 12157 12201 12226 6/0 2 130 230 236 242 248 326 332 358 359 361 364 410 421 429 431 461 462 463 472 474 475 481 483 485 486 496 530 531 534 537 540 541 557 559 568 587 602 608 609 613 615 624 687 698 1025 1027 1036 1040 1042 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48613 48614 48615 48616 48618 48619 48620 48621 48733 48898 48899 48912 48913 48914 48916 48917 48942 48943 48960 48964 48965 48966 49012 49013 49031 49042 49048 49125 49127 49139 49145 49148https://cdsarc.cds.unistra.fr/viz-bin/moc/B/subaru?format=asciiOpticaldefaultB/subaru/suprimcThe Suprime-Cam Observation Log (2005-11-02)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFrameID! Frame ID (1)meta.id;pos.frame;obs.fieldcharRAJ2000Right Ascension (J2000) of the CCD chip centerdegpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) of the CCD chip centerdegpos.eq.dec;meta.mainindexedObsStartObservation start date (year, UT)stime.start;obsExpTimeExposure timestime.duration;obs.exposurefloatObsTypeObservation type (BIAS, FLAT, OBJECT, etc.) * those data other than OBJECT are omitted.meta.notecharObjectObject namemeta.id.assoccharFilterFilter combination (2)meta.id;instr.filtercharAirMassValue of the airmass at the beginning of the exposureobs.airMassfloatNAXIS1Dimension of the image (X-axis)pixphys.angSizeintNAXIS2Dimension of the image (Y-axis)pixphys.angSizeintFF[01] Flat-fielding processing flag (3)meta.notecharSeeingSeeing sizearcsecphys.angSizefloatEllipThe PSF anisotropy estimated by stellar ellipticitiesinstr.det.psffloatSMOKAGet details about the frame in the SMOKA systemmeta.ref.urlchar