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361. GAMA. Stellar mass budget
ID:
ivo://CDS.VizieR/J/MNRAS/462/4336
Title:
GAMA. Stellar mass budget
Short Name:
J/MNRAS/462/4336
Date:
21 Oct 2021
Publisher:
CDS
Description:
We build on a recent photometric decomposition analysis of 7506 Galaxy and Mass Assembly (GAMA) survey galaxies to derive stellar mass function fits to individual spheroid and disc component populations down to a lower mass limit of log(M_*_/M_{sun}_)=8. We find that the spheroid/disc mass distributions for individual galaxy morphological types are well described by single Schechter function forms. We derive estimates of the total stellar mass densities in spheroids ({rho}_spheroid_=1.24+/-0.49x10^8^M_{sun}_Mpc^-3^h_0.7_) and discs ({rho}_disc_=1.20+/-0.45x10^8^M_{sun}_Mpc^-3^h_0.7_), which translates to approximately 50 per cent of the local stellar mass density in spheroids and 48 per cent in discs. The remaining stellar mass is found in the dwarf 'little blue spheroid' class, which is not obviously similar in structure to either classical spheroid or disc populations. We also examine the variation of component mass ratios across galaxy mass and group halo mass regimes, finding the transition from spheroid to disc mass dominance occurs near galaxy stellar mass ~10^11^M_{sun}_ and group halo mass ~10^12.5^M_{sun}_/h. We further quantify the variation in spheroid-to-total mass ratio with group halo mass for central and satellite populations as well as the radial variation of this ratio within groups.
362. Gas content in 1038 interacting galaxies
ID:
ivo://CDS.VizieR/J/A+A/422/941
Title:
Gas content in 1038 interacting galaxies
Short Name:
J/A+A/422/941
Date:
21 Oct 2021
Publisher:
CDS
Description:
A study of the gas content in 1038 interacting galaxies, essentially selected from Arp (<VII/74>), Arp and Madore (<VII/170>), Vorontsov-Velyaminov (<VII/236>) catalogues and some of the published literature, is presented here. The data on the interstellar medium have been extracted from a number of sources in the literature and compared with a sample of 1916 normal galaxies. The mean values for each of the different ISM tracers (FIR, 21cm, CO lines, X-ray) have been estimated by means of survival analysis techniques, in order to take into account the presence of upper limits.
363. Gas exchanges between galaxies and IGM
ID:
ivo://CDS.VizieR/J/MNRAS/421/2888
Title:
Gas exchanges between galaxies and IGM
Short Name:
J/MNRAS/421/2888
Date:
21 Oct 2021
Publisher:
CDS
Description:
Using a representative sample of 65 intermediate-mass galaxies at z~0.6, we have investigated the interplay between the main ingredients of chemical evolution: metal abundance, gas mass, stellar mass and star formation rate (SFR). All quantities have been estimated using deep spectroscopy and photometry from ultraviolet to infrared and assuming an inversion of the Kennicutt-Schmitt law for the gas fraction. Six billion years ago, galaxies had a mean gas fraction of 32+/-3 per cent, i.e. twice that of their local counterparts. Using higher redshift samples from the literature, we explore the gas phases and estimate the evolution of the mean gas fraction of distant galaxies over the last 11Gyr.
364. Gas kinematics in CALIFA survey
ID:
ivo://CDS.VizieR/J/A+A/573/A59
Title:
Gas kinematics in CALIFA survey
Short Name:
J/A+A/573/A59
Date:
21 Oct 2021
Publisher:
CDS
Description:
Ionized gas kinematics provide important clues to the dynamical structure of galaxies and hold constraints to the processes driving their evolution. The motivation of this work is to provide an overall characterization of the kinematic behavior of the ionized gas of the galaxies included in the Calar Alto Legacy Integral field Area (CALIFA), offering kinematic clues to potential users of the CALIFA survey for including kinematical criteria in their selection of targets for specific studies. From the first 200 galaxies observed by CALIFA survey in its two configurations, we present the two-dimensional kinematic view of the 177 galaxies satisfaying a gas content/detection threshold. After removing the stellar contribution, we used the cross-correlation technique to obtain the radial velocity of the dominant gaseous component for each spectrum in the CALIFA data cubes for different emission lines (namely, [OII] {lambda}{lambda}3726,3729, [OIII] {lambda}{lambda}4959,5007, H{alpha}+[NII] {lambda}{lambda}6548,6584, and [SII]{lambda}{lambda}6716,6730). The main kinematic parameters measured on the plane of the sky were directly derived from the radial velocities with no assumptions on the internal prevailing motions. Evidence of the presence of several gaseous components with different kinematics were detected by using [OIII] {lambda}{lambda}4959,5007 emission line profiles.
365. GAVO Data Center ADQL Query
ID:
ivo://org.gavo.dc/__system__/adql/query
Title:
GAVO Data Center ADQL Query
Short Name:
gavoadql
Date:
27 Dec 2024 08:31:06
Publisher:
The GAVO DC team
Description:
An endpoint for submitting ADQL queries to the data center and retrieving the result in various forms.
366. GAVO Data Center TAP service
ID:
ivo://org.gavo.dc/tap
Title:
GAVO Data Center TAP service
Short Name:
GAVO DC TAP
Date:
23 Feb 2022 00:23:41
Publisher:
The GAVO DC team
Description:
The GAVO Data Center'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. In GAVO's data center, we in particular hold several large catalogs like PPMXL, 2MASS PSC, USNO-B2, UCAC4, WISE, SDSS DR7, for you to use in crossmatches, possibly with uploaded tables. Tables exposed through this endpoint include: nucand from the amanda schema, main from the annisred schema, data from the antares schema, data from the antares10 schema, dr10 from the apass schema, frames from the apo schema, main from the applause schema, gfh, id, identified, master, nid, unidentified from the arigfh schema, main from the arihip schema, main from the auger schema, data, phot_all, ssa_time_series from the bgds schema, data from the boydende schema, cat from the browndwarfs schema, cubes, fluxposv1200, fluxposv500, fluxv1200, fluxv500, objects, spectra from the califadr3 schema, images, srccat from the cars schema, meta from the carsarcs schema, main from the cs82morphoz schema, geo from the cstl schema, data from the danish schema, main from the dfbsplates schema, spectra, ssa from the dfbsspec schema, main from the dmubin schema, main from the emi schema, data from the feros schema, fk6join, part1, part3 from the fk6 schema, data from the flare_survey schema, data, ordersmeta from the flashheros schema, data from the fornax schema, dr2_ts_ssa, dr2epochflux, dr2light, edr3lite from the gaia schema, hyacob, maglims5, maglims6, maglims7, main, missing_10mas, rejected, resolvedss from the gcns schema, data from the gcpms schema, main from the gdr2ap schema, main from the gdr2dist schema, main, photometry from the gdr2mock schema, main from the gedr3auto schema, litewithdist, main from the gedr3dist schema, generated_data, maglim_5, maglim_6, maglim_7, main, parsec_props from the gedr3mock schema, main from the gedr3spur schema, columns, services, tables from the glots schema, main from the gps1 schema, main from the hdgaia schema, data from the hiicounter schema, main from the hipparcos schema, main from the hppunion schema, main from the hsoy schema, nucand from the icecube schema, data from the inflight schema, obscore from the ivoa schema, events, photpoints, timeseries from the k2c9vst schema, plates from the kapteyn schema, katkat from the katkat schema, data from the lamost5 schema, ssa_lrs, ssa_mrs from the lamost6 schema, geocounts, measurements, stations from the lightmeter schema, rawframes from the liverpool schema, main from the lspm schema, plates, wolfpalisa from the lsw schema, main from the magic schema, reduced from the maidanak schema, exts from the mcextinct schema, cubes, slitspectra from the mlqso schema, epn_core, mpcorb from the mpc schema, main, stars from the mwsc schema, main, stars from the mwsce14a schema, data from the obscode schema, bibrefs, maps, masers, monitor from the ohmaser schema, measurements, ssa from the onebigb schema, data, shapes from the openngc schema, main from the pcc schema, data from the plc schema, data from the plc2 schema, data from the plc3 schema, data from the plts schema, data from the polcatsmc schema, plates, rawplates from the potsdam schema, cubes, maps from the ppakm31 schema, data from the ppmx schema, main, usnocorr from the ppmxl schema, map10, map6, map7, map8, map9, map_union from the prdust schema, dr2, dr3, dr4, main from the rave schema, images, photons from the rosat 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_tables, validation from the rr schema, objects, photpar from the sasmirala schema, sources from the sdssdr7 schema, main from the smakced schema, main from the spm4 schema, sources from the supercosmos schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, main from the taptest schema, main from the tenpc schema, main from the tgas schema, data from the theossa schema, epn_core from the titan schema, data, line_tap from the toss schema, data from the twomass schema, icrscorr, main, ppmxlcross from the ucac3 schema, main from the ucac4 schema, main from the ucac5 schema, main from the urat1 schema, data, platecorrs, plates, ppmxcross, spurious, twomasscross from the usnob schema, data from the veronqsos schema, stripe82 from the vlastripe82 schema, main from the wdsdss10 schema, archives, main from the wfpdb schema, main from the wise schema, data from the zcosmos schema.
367. GAVO DC Custom Uploading Crossmatcher
ID:
ivo://org.gavo.dc/cross/q/match
Title:
GAVO DC Custom Uploading Crossmatcher
Short Name:
gavo_crossmatch
Date:
27 Dec 2024 08:31:02
Publisher:
The GAVO DC team
Description:
A plain positional crossmatch service that allows file and URL uploads to be crossmatched to DC-internal tables. In general, you want to use TAP for this kind of thing when it is available, but in a pinch it might come in handy. Larger catalogues that can be matched against include 2MASS, USNO-B, PPMX, CARS, and more.
368. GEMS survey data and catalog
ID:
ivo://CDS.VizieR/J/ApJS/174/136
Title:
GEMS survey data and catalog
Short Name:
J/ApJS/174/136
Date:
21 Oct 2021
Publisher:
CDS
Description:
We describe the data reduction and object cataloging for the GEMS survey, a large-area (800 arcmin^2^) two-band (F606W and F850LP) imaging survey with the Advanced Camera for Surveys on the Hubble Space Telescope, centered on the Chandra Deep Field-South.
369. General Catalogue of Herbig-Haro Objects
ID:
ivo://CDS.VizieR/V/104
Title:
General Catalogue of Herbig-Haro Objects
Short Name:
V/104
Date:
21 Oct 2021
Publisher:
CDS
Description:
Herbig-Haro (HH) objects are small-scale shock regions intimately associated with star forming regions. The present catalogue includes for all known HH objects: the HH number, previous designations if any, a position, the most probable energy source, and the region and distance. Additionally, extensive notes give a brief description of each object with detailed references to the literature. The catalogue will be updated as developments in the field require.
370. General Catalogue of Stars
ID:
ivo://CDS.VizieR/I/180
Title:
General Catalogue of Stars
Short Name:
I/180
Date:
21 Oct 2021
Publisher:
CDS
Description:
The general Catalogue reported here has been Compiled on the basis of the preliminary catalogues consisting of the long series observations of the fundamental programs (mainly of FK4 stars) of the Mark I photoelectric astrolabe of Shaanxi Astronomical Observatory and Mark II photoelectric astrolobes of Beijing, Shanghai and Yunnan Astronomical Observatories, together with a large amount of observations of catalogue stars carried out in Beijing, Shanghai and Shaanxi, as well as 4 preliminary catalogues of Danjon's astrolabes derived from the observations of OPL No.14 of Shanghai, No.30 of Beijing and No.29 of Wuchang. With magnitudes ranging from 0.1 to 7.2, the GCPA consists of 1579 stars. The declinations are from -3.6 degree to 68.8 degree, in which 642 are FK4 stars. The mean precisions of position corrections are 3.3 ms and 0.058" in right ascension and declination, respectively. The mean epoch of GCPA is 1987.8.

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