- ID:
- ivo://asu.cas.cz/tap
- Title:
- AIASCR VO Services TAP service
- Short Name:
- AIASCR TAP
- Date:
- 19 Apr 2017 08:23:36
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- The AIASCR VO Services's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: objcat, objects_observed, objobs_complete, objobs_lightcurves, observation_info from the bextract schema, dim_exposure, dim_observation_objcat, exposure, objcat, objobs_complete, objobs_lightcurves, observation, observation_objcat from the bextract_jan16 schema, reduced_images from the dk154_reduced schema, exposure, objcat, objobs_complete, objobs_lightcurves, observation from the bextract_jan15 schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, dim_exposure, dim_observation_objcat, exposure, objcat, objobs_complete, objobs_lightcurves, objobs_lightcurves_ssap, observation, observation_objcat from the bextract_apr18 schema, data from the ccd700 schema, dim_exposure, dim_observation_objcat, exposure, objcat, objobs_complete, objobs_lightcurves, observation, observation_objcat from the bextract_jan15_v2 schema, emptyobscore, obscore from the ivoa schema, data from the heros schema, reduced_images from the dk154_reduced_jan18 schema, dim_exposure, dim_observation_objcat, exposure, objcat, objobs_complete, objobs_lightcurves, observation, observation_objcat from the bextract_jul15 schema, dim_exposure, dim_observation_objcat, exposure, objcat, objobs_complete, objobs_lightcurves, objobs_lightcurves_ssap, observation, observation_objcat from the bextract_jul16 schema, data from the lamost_dr2 schema, data from the lamost_dr3 schema, data from the lamost schema, data from the lamost_dr1 schema, dim_exposure, dim_observation_objcat, exposure, objcat, objobs_complete, objobs_lightcurves, objobs_lightcurves_ssap, observation, observation_objcat from the bextract_jan18 schema, dim_exposure, dim_observation_objcat, exposure, objcat, objobs_complete, objobs_lightcurves, objobs_lightcurves_ssap, observation, observation_objcat from the bextract_dec17 schema, raw_images from the dk154_rawdata schema.
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- ID:
- ivo://aip.gavo.org/tap
- Title:
- AIP DaCHS TAP service
- Short Name:
- AIP GAVO TAP
- Date:
- 17 Jul 2024 11:34:42
- Publisher:
- GAVO at Leibniz-Institute for Astrophysics Potsdam
- Description:
- The AIP DaCHS's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: dens256, fof, redshifts from the bolshoi schema, columns, services, tables from the glots schema, fof, fofmtree, fofparticles, particles85, redshifts, treesnapnums from the mdr1 schema, rave_dr4 from the ravedr4 schema, alt_identifier, authorities, capability, g_num_stat, interface, intf_param, registries, relationship, res_date, res_detail, res_role, res_schema, res_subject, res_table, resource, stc_spatial, stc_spectral, stc_temporal, subject_uat, table_column, tap_table, validation from the rr schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Catalogue_AllSky_ASTFLUX_1.0
- Title:
- AKARI Asteroid Flux Catalogue Version 1
- Short Name:
- AKARI_ASTEROID_V1
- Date:
- 27 Mar 2025 01:36:54
- Publisher:
- JVO
- Description:
- The AKARI Asteroid Flux Catalog contains photometric data of 5201 asteroids observed with the Infrared Camera (IRC) on board the Japanese infrared astronomical satellite AKARI. The catalog objects comprise the near-Earth asteroids, the main belt asteroids, the Cybeles, the Hildas, and the Jovian Trojan asteroids. The observations were performed by the all-sky survey in 9 or 18 micron bands as well as the slow-scan observations in 9 or 18 micron bands, and the pointed observations in 4, 7, 11, 15, and/or 24 micron bands.
- ID:
- ivo://CDS.VizieR/II/327
- Title:
- AKARI Far-Infrared Surveyor YSO catalog
- Short Name:
- II/327
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- We demonstrate the use of the AKARI all-sky survey photometric data in the study of galactic star formation. Our aim was to select young stellar objects (YSOs) in the AKARI Far-Infrared Surveyor (FIS) Bright Source Catalogue. We used AKARI/FIS and Wide-field Infrared Survey Explorer (WISE) data to derive mid- and far-infrared colors of YSOs. Classification schemes based on quadratic discriminant analysis (QDA) have been given for YSOs and the training catalog for QDA was the whole-sky selection of previously known YSOs (i.e., listed in the SIMBAD database). A new catalog of AKARI FIS YSO candidates including 44001 sources has been prepared; the reliability of the classification is over 90%, as tested in comparison to known YSOs. As much as 76% of our YSO candidates are from previously uncatalogued types. The vast majority of these sources are Class I and II types according to the Lada classification. The distribution of AKARI FIS YSOs is well correlated with that of the galactic ISM; local over-densities were found on infrared loops and towards the cold clumps detected by Planck.
- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Spectrum_Pointed_SlitlessMIR_spectrum_1.0
- Title:
- AKARI/IRC MIR-S slit-less spectroscopic catalogue
- Short Name:
- AKARI_IRC_SPEC_V1
- Date:
- 27 Mar 2025 01:25:07
- Publisher:
- JVO
- Description:
- A catalogue of mid-infrared slit-less spectra (5.5-12.5 ?m) extracted from the AKARI/IRC MIR-S spectroscopic observation data. All 886 MIR-S spectroscopic data obtained in Phases 1&2 are analyzed, and 862 spectra of 604 individual sources that are little contaminated by nearby sources are catalogued. We also present a 9 ?m point source catalogue generated as a by-product. The point source catalogue contains 42,387 sources brighter than 0.3 mJy.
- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Spectrum_Pointed_SlitlessMIR_psc_1.0
- Title:
- AKARI/IRC MIR-S slit-less 9um point source catalogue
- Short Name:
- AKARI_IRC_SPEC_PSC_V1
- Date:
- 27 Mar 2025 01:22:25
- Publisher:
- JVO
- Description:
- This is a 9 um point source catalogue generated as a by-product of the "AKARI/IRC MIR-S slit-less spectroscopic catalogue". The point source catalogue contains 42,387 sources brighter than 0.3 mJy.
- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Spectrum_Pointed_DiffuseSkyPatch_1.0
- Title:
- AKARI/IRC NIR Low-resolution Spectral Catalogue of Diffuse Sky Patches
- Short Name:
- AKARI_IRC_SPEC_DSP
- Date:
- 27 Mar 2025 01:20:46
- Publisher:
- JVO
- Description:
- This catalog contains the 278 low-resolution (R~20) near-infrared (1.8-5.3 micron) spectra of diffuse sky covering a wide range of galactic and ecliptic latitudes with the Infrared Camera (IRC) onboard AKARI before the exhaustion of liquid-helium (from September 2006 to May 2007). Advanced reduction methods specialized for the slit spectroscopy of diffuse sky spectra are developed for constructing this spectral catalog.
- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Spectrum_Pointed_GALPN_1.0
- Title:
- AKARI/IRC NIR Spectral Atlas of Galactic Planetary Nebulae
- Short Name:
- AKARI_IRC_SPEC_GALPN
- Date:
- 27 Mar 2025 01:19:46
- Publisher:
- JVO
- Description:
- This catalog contains near-infrared (2.5--5.0 micron) low-resolution (R ~ 100) spectra of 72 Galactic Planetary Nebulae (PNe), obtained with the InfraRed Camera (IRC) onboard the AKARI satellite in the post-helium phase. The objects were treated as almost point sources for the IRC. Grism spectroscopy was carried out in the 1-arcmin window. The near-infrared spectra were obtained in a slit-less mode without any flux loss due to a slit. The spectra show emission features including hydrogen recombination lines, helium recombination lines, the 3.3--3.5 micron hydrocarbon features, [MgIV] at 4.49 micron, and [ArVI] at 4.53 micron. This catalog also contains the intensity and equivalent width of these emission features measured by spectral fitting. The source list (source.dat) summarizes observations. As ancillary data, the magnitudes in the V- and Ks-band, the extinction at V-band toward the objects, and the effective temperature collected from literature are listed in another table (misc.dat). The intensities and the equivalent widths of the emission features are tabulated in different tables (intens.dat and equivw.dat). Each object is identified by the PNG ID (PNG) or an observation ID (Obs-ID). One-dimensional near-infrared spectra are stored in a directory (spc/). Each spectrum is identified by the observation ID.
- ID:
- ivo://CDS.VizieR/J/MNRAS/444/846
- Title:
- AKARI NEP Survey sources at 18um
- Short Name:
- J/MNRAS/444/846
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- We present the first galaxy counts at 18{mu}m using the Japanese AKARI satellite's survey at the North Ecliptic Pole (NEP), produced from the images from the NEP-Deep and NEP-Wide surveys covering 0.6 and 5.8deg^2^, respectively. We describe a procedure using a point source filtering algorithm to remove background structure and a minimum variance method for our source extraction and photometry that delivers the optimum signal to noise for our extracted sources, confirming this by comparison with standard photometry methods. The final source counts are complete and reliable over three orders of magnitude in flux density, resulting in sensitivities (80 per cent completeness) of 0.15 and 0.3mJy for the NEP-Deep and NEP-Wide surveys, respectively, a factor of 1.3 deeper than previous catalogues constructed from this field. The differential source counts exhibit a characteristic upturn from Euclidean expectations at around a milliJansky and a corresponding evolutionary bump between 0.2-0.4mJy consistent with previous mid-infrared surveys with ISO and Spitzer at 15 and 24{mu}m. We compare our results with galaxy evolution models confirming the striking divergence from the non-evolving scenario. The models and observations are in broad agreement implying that the source counts are consistent with a strongly evolving population of luminous infrared galaxies at redshifts higher than unity. Integrating our source counts down to the limit of the NEP survey at the 150{mu}Jy level we calculate that AKARI has resolved approximately 55 per cent of the 18{mu}m cosmic infrared background relative to the predictions of contemporary source count models.
- ID:
- ivo://jvo/isas/darts/akari/ObsTAP
- Title:
- AKARI ObsTAP service
- Short Name:
- AKARI_OBSTAP
- Date:
- 29 May 2024 05:06:13
- Publisher:
- JVO
- Description:
- This is an ObsTAP service for AKARI data.