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- ID:
- ivo://CDS.VizieR/J/PASP/122/347
- Title:
- Chinese Small Telescope ARray (CSTAR)
- Short Name:
- J/PASP/122/347
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- In 2008 January the twenty-fourth Chinese expedition team successfully deployed the Chinese Small Telescope ARray (CSTAR) to Dome A, the highest point on the Antarctic plateau. CSTAR consists of four 14.5cm optical telescopes, each with a different filter (g,r,i, and open) and has a 4.5{deg}x4.5{deg} field of view (FOV). It operates robotically as part of the Plateau Observatory, PLATO, with each telescope taking an image every ~30s throughout the year whenever it is dark. During 2008, CSTAR 1 performed almost flawlessly, acquiring more than 0.3 million -band images for a total integration time of 1728hr during 158 days of observations. For each image taken under good sky conditions, more than 10,000 sources down to magnitude could be detected. We performed aperture photometry on all the sources in the field to create the catalog described herein. Since CSTAR has a fixed pointing centered on the south celestial pole (Dec=-90{deg}), all the sources within the FOV of CSTAR were monitored continuously for several months. The photometric catalog can be used for studying any variability in these sources, and for the discovery of transient sources such as supernovae, gamma-ray bursts, and minor planets.
- ID:
- ivo://CDS.VizieR/III/74
- Title:
- Faint Blue Stars near the South Galactic Pole
- Short Name:
- III/74
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- A search for faint blue stars conducted at the Observatories of Tonantzintla and Minnesota has yielded 8746 objects which are somewhat blue. The data file is organized into three sections with the same column format. The first 1569 records are for stars with U-V of -0.4 or bluer, which are very definitely blue (Table II of the paper). The next 2929 stars are somewhat blue, with U-V values of -0.3 or -0.2 (Table III of the paper). The final 4248 records give data for stars with U-V of -0.1 or 0.0 (Table IV of the paper). Photometric, spectroscopic, and proper-motion data have later been acquired for these objects, which revealed the great variety of the objects in this catalogue: white dwarfs, subdwarfs, QSOs (quasars), compact and active galaxies. Finding charts and details about the nature of these blue objects can be found in the following papers: Haro G., and Chavira E.: 1987RMxAA..15..107H ; Chavira E.: 1988RMxAA..16..123C, Chavira E., 1990RMxAA..20...47C, and 1992RMxAA..24..139C
- ID:
- ivo://CDS.VizieR/J/A+AS/104/1
- Title:
- Faint ring-shaped galaxies near South Pole
- Short Name:
- J/A+AS/104/1
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- A list of probable ring galaxies with a limiting magnitude of 17.5 has been prepared based on visual inspection of the film copies of the J SRC/ESO survey. About 88% of the sample of 125 selected objects seem to be new, hitherto unrecognized as ring galaxies. The candidate objects have been classified following the ring structure and the nucleus appearance.
- ID:
- ivo://CDS.VizieR/VIII/109
- Title:
- GLEAM III. South Galactic Pole
- Short Name:
- VIII/109
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- We present the South Galactic Pole (SGP) data release from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey. These data combine both years of GLEAM observations at 72-231MHz conducted with the Murchison Widefield Array (MWA) and cover an area of 5,113 deg^2^ centred on the SGP at 20h40m<RA<05h04m and -48{deg}<Dec<-2{deg}. At 216MHz, the typical rms noise is ~5mJy/beam and the angular resolution ~2 arcmin. The source catalogue contains a total of 108851 components above 5{sigma}, of which 77 per cent have measured spectral indices between 72 and 231MHz. Improvements to the data reduction in this release include the use of the GLEAM Extragalactic catalogue as a sky model to calibrate the data, a more efficient and automated algorithm to deconvolve the snapshot images, and a more accurate primary beam model to correct the flux scale. This data release enables more sensitive large-scale studies of extragalactic source populations as well as spectral variability studies on a one-year timescale.
- ID:
- ivo://CDS.VizieR/J/AJ/103/514
- Title:
- High-velocity stars toward South Galactic Cap
- Short Name:
- J/AJ/103/514
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- We present spectroscopic observations of stars identified in Murray's (1986) astrometric survey of the South Galactic Cap
- ID:
- ivo://CDS.VizieR/J/A+AS/97/835
- Title:
- K giants at the South Galactic Pole
- Short Name:
- J/A+AS/97/835
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- (no description available)
- ID:
- ivo://CDS.VizieR/J/AJ/83/1090
- Title:
- Late-type M dwarfs towards the SGP
- Short Name:
- J/AJ/83/1090
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- A catalog, including finding charts, is presented which contains 282 faint stars of spectral type M3 and later, located in an area of 173 square degrees near the South Galactic Pole. The catalog is based on a spectroscopic survey undertaken with the Curtis Schmidt at CTIO and provides a finding list of M stars free of any possible kinematic bias. The majority of these stars are expected to be dwarfs. To the same limiting magnitude, the observed surface density is comparable to that of the faint M stars in the direction of the North Galactic Pole, named 273 over 190 square degrees.
- ID:
- ivo://CDS.VizieR/VII/169
- Title:
- Optical Identifications of IRAS Point Sources
- Short Name:
- VII/169
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- Optical identifications are given of IRAS point sources: 312 sources in a 304 square deg area centred on the South Galactic Pole, of which 148 are identified with stars, 154 with galaxies and 10 are unidentified down to 21st magnitude; 206 point sources in a 113 square deg area centred on the Virgo cluster, of which 54 are identified with stars, 113 with optically bright (B_J<16) galaxies, 32 with faint galaxies, and 7 are apparently empty fields; (66, 114, 61) sources in the regions of (Fornax, Hydra I, Coma) cluster of galaxies, of which (35, 48, 18) are identified with stars, (43, 58, 41) with galaxies.
- ID:
- ivo://CDS.VizieR/I/129
- Title:
- Parallaxes and Proper Motions near SGP
- Short Name:
- I/129
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- The catalog contains 6125 stars brighter than B=17.5, V=17.0 in the south galactic cap. The data have been obtained using the UK Schmidt telescope between 1975 and 1981. The plates were measured on the GALAXY machine at RGO. External errors of the parallaxes range between -/+0.012 and -/+0.017 arcsec according to magnitude. Internal proper motion errors range from -/+0.006 and -/+0.008 arcsec. In addition to the positions, proper motions, and parallaxes, the photometric data include B and V.
