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641. Oxford 1 AC Zone Data Reduced to ACRS
ID:
ivo://CDS.VizieR/I/224
Title:
Oxford 1 AC Zone Data Reduced to ACRS
Short Name:
I/224
Date:
21 Oct 2021
Publisher:
CDS
Description:
The U.S. Naval Observatory is in the process of making new reductions of the Astrographic Catalogue (AC) using a modern reference system, the ACRS, which represents the system of the FK5. The data from the Oxford 1 Zone, whose plates are centered between declinations +25 and +31 degrees (eq. 1900), have been analyzed for scale, rotation, tilt, coma, magnitude equation, radial distortion and distortions introduced by the use of reseaux in the Carte du Ciel program. The result is a positional catalog of over 277,000 stars on eq. J2000.0, epoch of observation. Additionally, all stars have been matched with the Tycho Input Catalog (revised); those numbers have been added for additional identification purposes.
642. Oxygen abundance in disk galaxies
ID:
ivo://CDS.VizieR/J/A+A/623/A7
Title:
Oxygen abundance in disk galaxies
Short Name:
J/A+A/623/A7
Date:
21 Oct 2021
Publisher:
CDS
Description:
We examine the possible dependence of the radial oxygen abundance distribution on non-axisymmetrical structures (bar/spirals) and other macroscopic parameters such as the mass, the optical radius R25, the color g-r, and the surface brightness of the galaxy. A sample of disk galaxies from the third data release of the Calar Alto Legacy Integral Field Area Survey (CALIFA DR3) is considered. We adopted the Fourier amplitude A2 of the surface brightness as a quantitative characteristic of the strength of nonaxisymmetric structures in a galactic disk, in addition to the commonly used morphologic division for A, AB, and B types based on the Hubble classification. To distinguish changes in local oxygen abundance caused by the non-axisymmetrical structures, the multiparametric mass-metallicity relation was constructed as a function of parameters such as the bar/spiral pattern strength, the disk size, color index g-r in the Sloan Digital Sky Survey (SDSS) bands, and central surface brightness of the disk. The gas-phase oxygen abundance gradient is determined by using the R calibration We find that there is no significant impact of the non-axisymmetric structures such as a bar and/or spiral patterns on the local oxygen abundance and radial oxygen abundance gradient of disk galaxies. Galaxies with higher mass, however, exhibit flatter oxygen abundance gradients in units of dex/kpc, but this effect is significantly less prominent for the oxygen abundance gradients in units of dex/R25 and almost disappears when the inner parts are avoided (R>0.25R25). We show that the oxygen abundance in the central part of the galaxy depends neither on the optical radius R25 nor on the color g-r or the surface brightness of the galaxy. Instead, outside the central part of the galaxy, the oxygen abundance increases with g-r value and central surface brightness of the disk.
643. Oxygen abundance maps of CALIFA galaxies
ID:
ivo://CDS.VizieR/J/MNRAS/462/2715
Title:
Oxygen abundance maps of CALIFA galaxies
Short Name:
J/MNRAS/462/2715
Date:
21 Oct 2021
Publisher:
CDS
Description:
We construct maps of the oxygen abundance distribution across the discs of 88 galaxies using Calar Alto Legacy Integral Field Area survey (CALIFA) Data Release 2 (DR2) spectra. The position of the centre of a galaxy (coordinates on the plate) was also taken from the CALIFA DR2. The galaxy inclination, the position angle of the major axis, and the optical radius were determined from the analysis of the surface brightnesses in the Sloan Digital Sky Survey (SDSS) g and r bands of the photometric maps of SDSS Data Release 9. We explore the global azimuthal abundance asymmetry in the discs of the CALIFA galaxies and the presence of a break in the radial oxygen abundance distribution. We found that there is no significant global azimuthal asymmetry for our sample of galaxies, i.e. the asymmetry is small, usually lower than 0.05dex. The scatter in oxygen abundances around the abundance gradient has a comparable value, <~0.05dex. A significant (possibly dominant) fraction of the asymmetry can be attributed to the uncertainties in the geometrical parameters of these galaxies. There is evidence for a flattening of the radial abundance gradient in the central part of 18 galaxies. We also estimated the geometric parameters (coordinates of the centre, the galaxy inclination and the position angle of the major axis) of our galaxies from the analysis of the abundance map. The photometry-map-based and the abundance-map-based geometrical parameters are relatively close to each other for the majority of the galaxies but the discrepancy is large for a few galaxies with a flat radial abundance gradient.
644. OzDES DR1
ID:
ivo://CDS.VizieR/J/MNRAS/472/273
Title:
OzDES DR1
Short Name:
J/MNRAS/472/273
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present results for the first three years of OzDES, a six-year program to obtain redshifts for objects in the Dark Energy Survey (DES) supernova fields using the 2dF fibre positioner and AAOmega spectrograph on the Anglo-Australian Telescope. OzDES is a multi-object spectroscopic survey targeting multiple types of targets at multiple epochs over a multi-year baseline, and is one of the first multi-object spectroscopic surveys to dynamically include transients into the target list soon after their discovery. At the end of three years, OzDES has spectroscopically confirmed almost 100 supernovae, and has measured redshifts for 17,000 objects, including the redshifts of 2,566 supernova hosts. We examine how our ability to measure redshifts for targets of various types depends on signal-to-noise, magnitude, and exposure time, finding that our redshift success rate increases significantly at a signal-to-noise of 2 to 3 per 1-Angstrom bin. We also find that the change in signal-to-noise with exposure time closely matches the Poisson limit for stacked exposures as long as 10 hours. We use these results to predict the redshift yield of the full OzDES survey, as well as the potential yields of future surveys on other facilities such as 4MOST, PFS, and MSE. This work marks the first OzDES data release, comprising 14,693 redshifts. OzDES is on target to obtain over 30,000 redshifts over the six-year duration of the survey, including a yield of approximately 5,700 supernova host-galaxy redshifts.
645. PADC TAP Server on voparis-rr.obspm.fr TAP service
ID:
ivo://purx/tap
Title:
PADC TAP Server on voparis-rr.obspm.fr TAP service
Short Name:
PADC TAP
Date:
30 Dec 2024 11:06:13
Publisher:
Paris Astronomical Data Centre
Description:
The PADC TAP Server on voparis-rr.obspm.fr'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: columns, services, tables from the glots schema, obscore from the ivoa schema, alt_identifier, authorities, capability, g_num_stat, interface, intf_param, registries, relationship, res_date, res_detail, resource, res_role, res_schema, res_subject, res_table, 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.
646. PADC TAP Server on voparis-tap-astro.obspm.fr TAP service
ID:
ivo://padc.obspm.astro/tap
Title:
PADC TAP Server on voparis-tap-astro.obspm.fr TAP service
Short Name:
PADC TAP
Date:
16 Jul 2024 14:01:13
Publisher:
Paris Astronomical Data Centre
Description:
The PADC TAP Server on voparis-tap-astro.obspm.fr'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: main from the esor schema, galaxies from the hyperleda schema, obscore from the ivoa schema, main from the posse schema, galaxyzoo, rcsed, rcsed_fibermags, rcsed_gasmet, rcsed_lines_gauss, rcsed_lines_nonpar, rcsed_lines_nonpar_reg, simard_table2, simard_table3 from the specphot schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
647. PADC TAP Server on voparis-tap-helio.obspm.fr TAP service
ID:
ivo://padc.obspm.helio/tap
Title:
PADC TAP Server on voparis-tap-helio.obspm.fr TAP service
Short Name:
PADC TAP
Date:
16 Jul 2024 00:11:28
Publisher:
Paris Astronomical Data Centre
Description:
The PADC TAP Server on voparis-tap-helio.obspm.fr'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 bass2000 schema, epn_core from the hfc1ar schema, epn_core from the hfc1t3 schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
648. PADC TAP Server on voparis-tap-he.obspm.fr TAP service
ID:
ivo://padc.obspm.he/tap
Title:
PADC TAP Server on voparis-tap-he.obspm.fr TAP service
Short Name:
PADC TAP
Date:
16 Jul 2024 13:57:56
Publisher:
Paris Astronomical Data Centre
Description:
The PADC TAP Server on voparis-tap-he.obspm.fr'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: obscore, obscore_test from the hess_dr schema, obscore from the ivoa schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
649. PADC TAP Server on voparis-tap-maser.obspm.fr TAP service
ID:
ivo://padc.obspm.maser/tap
Title:
PADC TAP Server on voparis-tap-maser.obspm.fr TAP service
Short Name:
PADC TAP
Date:
16 Jul 2024 14:07:24
Publisher:
Paris Astronomical Data Centre
Description:
The PADC TAP Server on voparis-tap-maser.obspm.fr'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 cassini_jupiter schema, epn_core from the cassini_rpws schema, epn_core from the expres schema, epn_core from the juno_waves schema, epn_core from the lofar4sw_proto schema, epn_core from the maser_services schema, epn_core from the spase_vespa schema, epn_core from the stereo_waves schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core, fogg_akr_wind, leblanc_nda_jupiter_emi, leblanc_nda_jupiter_obs, louis_juno_waves, marques_nda_jupiter, taubenschuss_frp_saturn, wu_anomalous_nsmr, wu_nkom_saturn, wu_skr_harmonic from the tfcat schema, epn_core from the voyager_pra schema, epn_core from the wind_waves schema.
650. PADC TAP Server on voparis-tap-planeto.obspm.fr TAP service
ID:
ivo://padc.obspm.planeto/tap
Title:
PADC TAP Server on voparis-tap-planeto.obspm.fr TAP service
Short Name:
PADC TAP
Date:
18 Oct 2024 18:07:32
Publisher:
Paris Astronomical Data Centre
Description:
The PADC TAP Server on voparis-tap-planeto.obspm.fr'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 apis schema, epn_core from the basecom schema, epn_core, observatories from the bdip schema, epn_core from the crism_speclib schema, epn_core from the dynastvo schema, epn_core from the exoplanet schema, epn_core from the gmap schema, epn_core from the hst_planeto schema, epn_core from the iks schema, epn_core from the lunar_craters schema, epn_core from the m4ast schema, epn_core from the mars_craters schema, epn_core from the mars_craters_lagain schema, epn_core from the mercury_craters schema, epn_core from the meteor_showers schema, epn_core from the moonsprop schema, epn_core from the planets schema, epn_core from the spectro_asteroids schema, epn_core from the spectro_m_ast schema, epn_core from the spectro_planets schema, epn_core from the spectro_stars schema, epn_core from the spectro_trojans schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the titan_profiles schema, epn_core from the tnosarecool schema, epn_core from the usgs_wms schema, epn_core from the venus_craters schema, epn_core from the vims_satellites schema, epn_core from the voccdb schema, epn_core from the vvex schema.

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