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461. Isolated Triplets of galaxies
ID:
ivo://CDS.VizieR/VII/83
Title:
Isolated Triplets of galaxies
Short Name:
VII/83
Date:
21 Oct 2021
Publisher:
CDS
Description:
The complete data for radial velocities of components of triple galaxies are presented. The main part of observations was accomplished with the 6-meter telescope.
462. Isophotal shapes of early-type galaxies
ID:
ivo://CDS.VizieR/J/ApJ/787/102
Title:
Isophotal shapes of early-type galaxies
Short Name:
J/ApJ/787/102
Date:
21 Oct 2021
Publisher:
CDS
Description:
We report on a study of the isophotal shapes of early-type galaxies to very faint levels, reaching ~0.1% of the sky brightness. The galaxies are from the Large Format Camera (LFC) fields obtained using the Palomar 5 m Hale Telescope, with integrated exposures ranging from 1 to 4 hr in the Sloan Digital Sky Survey r, i, and z bands. The shapes of isophotes of early-type galaxies are important, as they are correlated with the physical properties of the galaxies and are influenced by galaxy formation processes. In this paper, we report on a sample of 132 E and SO galaxies in one LFC field. We have redshifts for 53 of these, obtained using AAOmega on the Anglo-Australian Telescope. The shapes of early-type galaxies often vary with radius. We derive average values of isophotal shape parameters in four different radial bins along the semi-major axis in each galaxy. We obtain empirical fitting formulae for the probability distribution of the isophotal parameters in each bin and investigate for possible correlations with other global properties of the galaxies. Our main finding is that the isophotal shapes of the inner regions are statistically different from those in the outer regions. This suggests that the outer and inner parts of early-type galaxies have evolved somewhat independently.
463. JacobsUni EPN TAP service
ID:
ivo://jacobsuni/tap
Title:
JacobsUni EPN TAP service
Short Name:
JacobsUni EPN node TAP
Date:
27 Apr 2022 10:04:00
Publisher:
JacobsUni EPN node
Description:
The JacobsUni EPN'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: epn_core from the mars_craters schema, epn_core from the mars_craters_lagain schema, epn_core from the planetserver_crism schema, epn_core from the planmap schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the usgs_wms schema.
464. JCMT/SCUBA2 objects in COSMOS and UDS fields
ID:
ivo://CDS.VizieR/J/MNRAS/469/492
Title:
JCMT/SCUBA2 objects in COSMOS and UDS fields
Short Name:
J/MNRAS/469/492
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present physical properties [redshifts (z), star-formation rates (SFRs) and stellar masses (M*)] of bright (S_850_>=4mJy) submm galaxies in the ~=2deg^2^ COSMOS and UDS fields selected with SCUBA-2/JCMT. We complete the galaxy identification process for all (~=2000) S/N>=3.5 850-{mu}m sources, but focus our scientific analysis on a high-quality subsample of 651 S/N>=4 sources with complete multiwavelength coverage including 1.1-mm imaging. We check the reliability of our identifications, and the robustness of the SCUBA-2 fluxes by revisiting the recent ALMA follow-up of 29 sources in our sample. Considering >4mJy ALMA sources, our identification method has a completeness of ~=86 per cent with a reliability of ~=92 per cent, and only ~=15-20 per cent of sources are significantly affected by multiplicity (when a secondary component contributes >1/3 of the primary source flux). The impact of source blending on the 850-{mu}m source counts as determined with SCUBA-2 is modest; scaling the single-dish fluxes by ~=0.9 reproduces the ALMA source counts. For our final SCUBA-2 sample, we find median z=2.40^+0.10^_-0.04_, SFR=287+/-6M_{sun}_/yr and log(M*/M_{sun)_=11.12+/-0.02 (the latter for 349/651 sources with optical identifications). These properties clearly locate bright submm galaxies on the high-mass end of the 'main sequence' of star-forming galaxies out to z~= 6, suggesting that major mergers are not a dominant driver of the high-redshift submm-selected population. Their number densities are also consistent with the evolving galaxy stellar mass function. Hence, the submm galaxy population is as expected, albeit reproducing the evolution of the main sequence of star-forming galaxies remains a challenge for theoretical models/simulations.
465. JMMC Stellar Diameters Catalogue - JSDC
ID:
ivo://CDS.VizieR/II/300
Title:
JMMC Stellar Diameters Catalogue - JSDC
Short Name:
II/300
Date:
21 Oct 2021
Publisher:
CDS
Description:
This catalogue contains stellar angular diameter estimate for bright stars, complete for all stars with Hipparcos parallaxes. The JMMC Calibrator Workgroup has long developed methods to estimate the angular diameter of stars, and provides this expertise in the SearchCal software (http://www.jmmc.fr/searchcal). "SearchCal" creates a dynamical catalogue of stars suitable to calibrate Optical Long-Baseline Interferometry (OLBI) observations from on-line queries of CDS catalogues, according to observational parameters. In essence, SearchCal is limited only by the completeness of the stellar catalogues it uses, and in particular is not limited in magnitude. SearchCal being an application centered on OLBI peculiar purposes, it appeared useful to publish the estimated angular diameters of all stars with known parallaxes in a static catalogue. The present catalogue of stellar angular diameters has been obtained from an automated SearchCal results aggregation on the whole celestial sphere. For each star, the value of the limb-darkened angular diameters are computed using a surface brightness method and calibrations for (B-V), (V-R) and (V-K) color indexes. Stars whose angular diameters estimated from the various color indexes are not comparable, are rejected, and a reliable error on the estimated diameter is computed (1). For details of the method see Bonneau et al. (2006A&A...456..789B). To avoid specific confusion problems, spectroscopic binaries in the 9th Catalogue of Spectroscopic Binary Orbits (Pourbaix et al., 2009, Cat. B/sb9) or close visual binaries with a separation of less than 2 arc seconds in the Washington Visual Double Star Catalog (Mason et al., 2001, Cat. B/wds) have been filtered out.
466. JMMC Stellar Diameters Catalogue - JSDC. Version 2
ID:
ivo://CDS.VizieR/II/346
Title:
JMMC Stellar Diameters Catalogue - JSDC. Version 2
Short Name:
II/346
Date:
21 Oct 2021
Publisher:
CDS
Description:
This catalogue contains stellar angular diameter estimates for nearly all the stars of the Hipparcos and Tycho catalogue that have an associated spectral type in Simbad/CDS. The median error on the diameters is around 1.5%, with possible biases of around ~2%. For each object, the limb-darkened diameter retained is the mean value of several estimates performed using different couples of photometries. The chi-square representing the dispersion between these values is also given (it is below 2 for ~400000 stars). An additional flag signals stars that could represent a risk if chosen as calibrators for Optical Long-Baseline Interferometry, independently of the correctness of their apparent diameter estimate. This catalog replaces the catalog II/300/jsdc .
467. J-NEP PDR202107 Catalogue (July, 2024)
ID:
ivo://CEFCA/jnep/J-NEP-PDR202107
Title:
J-NEP PDR202107 Catalogue (July, 2024)
Short Name:
J-NEP-PDR202107
Date:
11 Sep 2024 13:00:00
Publisher:
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Description:
J-NEP PDR202107 Catalogue (July, 2024) is based on scientific images in 60 filters. J-NEP is a 60-band photometric optical survey based on images collected by the JST250 telescope and the Pathfinder instrument at the Observatorio Astrofísico de Javalambre (OAJ, Teruel, Spain) . Please include the following in any published material that makes use of this data: "Based on observations made with the JST250 telescope and PathFinder camera for J-NEP project at the Observatorio Astrofísico de Javalambre, in Teruel, owned, managed and operated by the Centro de Estudios de Física del Cosmos de Aragón."
468. J-PLUS DR3 Catalogue (July, 2022)
ID:
ivo://CEFCA/j-plus/J-PLUS-DR3
Title:
J-PLUS DR3 Catalogue (July, 2022)
Short Name:
J-PLUS-DR3
Date:
20 Sep 2023 06:30:00
Publisher:
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Description:
J-PLUS DR3 Catalogue (July, 2022) is based on scientific images in 12 filters collected from November 2015 to February 2022 covering a total area of ~3000 square degrees. The Javalambre Photometric Local Universe Survey (J-PLUS) is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern Hemisphere from the dedicated JAST80 telescope at the Observatorio Astrofísico de Javalambre (OAJ, Teruel, Spain) . Please include the following in any published material that makes use of this data: "Based on observations made with the JAST80 telescope for the J-PLUS project at the Observatorio Astrofísico de Javalambre, in Teruel, owned, managed and operated by the Centro de Estudios de Física del Cosmos de Aragón."
469. J-PLUS DR2 Catalogue (July, 2020)
ID:
ivo://CEFCA/j-plus/J-PLUS-DR2
Title:
J-PLUS DR2 Catalogue (July, 2020)
Short Name:
J-PLUS-DR2
Date:
20 Sep 2023 06:30:00
Publisher:
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Description:
J-PLUS DR2 Catalogue (July, 2020) is based on scientific images in 12 filters collected from November 2015 to February 2020 covering a total area of ~2000 square degrees. The Javalambre Photometric Local Universe Survey (J-PLUS) is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern Hemisphere from the dedicated JAST80 telescope at the Observatorio Astrofísico de Javalambre (OAJ, Teruel, Spain) . Please include the following in any published material that makes use of this data: "Based on observations made with the JAST80 telescope for the J-PLUS project at the Observatorio Astrofísico de Javalambre, in Teruel, owned, managed and operated by the Centro de Estudios de Física del Cosmos de Aragón."
470. J-PLUS DR1 Catalogue (July, 2018)
ID:
ivo://CEFCA/j-plus/J-PLUS-DR1
Title:
J-PLUS DR1 Catalogue (July, 2018)
Short Name:
J-PLUS-DR1
Date:
20 Sep 2023 06:30:00
Publisher:
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Description:
J-PLUS DR1 Catalogue (July, 2018) is based on scientific images in 12 filters collected from November 2015 to January 2018 covering a total area of ~1020 square degrees. The Javalambre Photometric Local Universe Survey (J-PLUS) is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern Hemisphere from the dedicated JAST80 telescope at the Observatorio Astrofísico de Javalambre (OAJ, Teruel, Spain) . Please include the following in any published material that makes use of this data: "Based on observations made with the JAST80 telescope for the J-PLUS project at the Observatorio Astrofísico de Javalambre, in Teruel, owned, managed and operated by the Centro de Estudios de Física del Cosmos de Aragón."

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