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11. Planck Early Release Compact Source Catalog (70GHz) @ IA2
ID:
ivo://ia2.inaf.it/planck/ercsc/f070
Title:
Planck Early Release Compact Source Catalog (70GHz) @ IA2
Short Name:
PlanckERCSCf070
Date:
13 Mar 2019 00:01:55
Publisher:
IA2
Description:
The Planck Early Release Compact Source Catalogue (ERCSC) is a list of all high reliability sources, both Galactic and extragalactic, derived from the first sky coverage. The data that went into this early release comprise all observations undertaken between 13 August 2009 and 6 June 2010, corresponding to Planck operational days 91-389. Since the Planck scan strategy results in the entire sky being observed every 6 months, the data considered in this release correspond to more than the first sky coverage. The source lists have reliability goals of 90% across the entire sky and > 95% at high Galactic latitude. The goals on photometric accuracy are 30% while the positional accuracy goal translates to a positional root mean square (RMS) uncertainty that is less than 1/5 of the beam full width at half maximum (FWHM). ref.: "Planck Early Results: The Early Release Compact Source Catalog" (ADS BibCode: 2011arXiv1101.2041P)
12. Planck Early Release Compact Source Catalog (44GHz) @ IA2
ID:
ivo://ia2.inaf.it/planck/ercsc/f044
Title:
Planck Early Release Compact Source Catalog (44GHz) @ IA2
Short Name:
PlanckERCSCf044
Date:
13 Mar 2019 00:01:46
Publisher:
IA2
Description:
The Planck Early Release Compact Source Catalogue (ERCSC) is a list of all high reliability sources, both Galactic and extragalactic, derived from the first sky coverage. The data that went into this early release comprise all observations undertaken between 13 August 2009 and 6 June 2010, corresponding to Planck operational days 91-389. Since the Planck scan strategy results in the entire sky being observed every 6 months, the data considered in this release correspond to more than the first sky coverage. The source lists have reliability goals of 90% across the entire sky and > 95% at high Galactic latitude. The goals on photometric accuracy are 30% while the positional accuracy goal translates to a positional root mean square (RMS) uncertainty that is less than 1/5 of the beam full width at half maximum (FWHM). ref.: "Planck Early Results: The Early Release Compact Source Catalog" (ADS BibCode: 2011arXiv1101.2041P)
13. Planck Early Release Compact Source Catalog (30GHz) @ IA2
ID:
ivo://ia2.inaf.it/planck/ercsc/f030
Title:
Planck Early Release Compact Source Catalog (30GHz) @ IA2
Short Name:
PlanckERCSCf030
Date:
13 Mar 2019 00:01:37
Publisher:
IA2
Description:
The Planck Early Release Compact Source Catalogue (ERCSC) is a list of all high reliability sources, both Galactic and extragalactic, derived from the first sky coverage. The data that went into this early release comprise all observations undertaken between 13 August 2009 and 6 June 2010, corresponding to Planck operational days 91-389. Since the Planck scan strategy results in the entire sky being observed every 6 months, the data considered in this release correspond to more than the first sky coverage. The source lists have reliability goals of 90% across the entire sky and > 95% at high Galactic latitude. The goals on photometric accuracy are 30% while the positional accuracy goal translates to a positional root mean square (RMS) uncertainty that is less than 1/5 of the beam full width at half maximum (FWHM). ref.: "Planck Early Results: The Early Release Compact Source Catalog" (ADS BibCode: 2011arXiv1101.2041P)
14. Planck Early Release Sunyaev Zel'dovich detected cluster candidates @ IA2
ID:
ivo://ia2.inaf.it/planck/ercsc/esz
Title:
Planck Early Release Sunyaev Zel'dovich detected cluster candidates @ IA2
Short Name:
PlanckERCSCesz
Date:
13 Mar 2019 00:01:26
Publisher:
IA2
Description:
The Planck Early Release Compact Source Catalogue (ERCSC) is a list of all high reliability sources, both Galactic and extragalactic, derived from the first sky coverage. The data that went into this early release comprise all observations undertaken between 13 August 2009 and 6 June 2010, corresponding to Planck operational days 91-389. Since the Planck scan strategy results in the entire sky being observed every 6 months, the data considered in this release correspond to more than the first sky coverage. The source lists have reliability goals of 90% across the entire sky and > 95% at high Galactic latitude. The goals on photometric accuracy are 30% while the positional accuracy goal translates to a positional root mean square (RMS) uncertainty that is less than 1/5 of the beam full width at half maximum (FWHM). ref.: "Planck Early Results: The Early Release Compact Source Catalog" (ADS BibCode: 2011arXiv1101.2041P)
15. [TEST] DAbrusco et al 2009 Catalogue of SDSS Quasar candidates
ID:
ivo://ia2.inaf.it/hosted/dabrusco2009/cqso
Title:
[TEST] DAbrusco et al 2009 Catalogue of SDSS Quasar candidates
Date:
13 Mar 2019 11:56:22
Publisher:
IA2
Description:
[TEST] We present a method for the photometric selection of candidate quasars in multiband surveys. The method makes use of a priori knowledge derived from a subsample of spectroscopic confirmed quasi-stellar objects (QSOs) to map the parameter space. The disentanglement of QSOs candidates and stars is performed in the colour space through the combined use of two algorithms, the probabilistic principal surfaces and the negative entropy clustering, which are for the first time used in an astronomical context. Both methods have been implemented in the VONEURAL package on the Astrogrid Virtual Observatory platform. Even though they belong to the class of the unsupervised clustering tools, the performances of the method are optimized by using the available sample of confirmed quasars and it is therefore possible to learn from any improvement in the available `base of knowledge'. The method has been applied and tested on both optical and optical plus near-infrared data extracted from the visible Sloan Digital Sky Survey (SDSS) and infrared United Kingdom Infrared Deep Sky Survey-Large Area Survey public data bases. In all cases, the experiments lead to high values of both efficiency and completeness, comparable if not better than the methods already known in the literature. A catalogue of optical candidate QSOs extracted from the SDSS Data Release 7 Legacy photometric data set has been produced and is publicly available at the URL http://voneural.na.infn.it/qso.html.
16. WINGS B surface photometry
ID:
ivo://ia2.inaf.it/hosted/wings/cone/gasphotb
Title:
WINGS B surface photometry
Short Name:
WINGSGasphotb
Date:
13 Mar 2019 11:58:32
Publisher:
IA2
Description:
This catalog contains the surface brightness measurements of ~41500 galaxies detected in the B images of the WINGS cluster survey. For each galaxy B magnitude, mean surface brightness, effective radius, Sersic index and axial ratio are given, together with their errors. These global parameters were obtained by simultaneously fitting the major and minor axis light growth curves of galaxies with a 2D flattened Sersic-law, convolved by the appropriate, space-varying PSF, which was previously evaluated by the tool itself. (http://adsabs.harvard.edu/abs/2006A%26A...446..373P)
17. WINGS equivalent widths
ID:
ivo://ia2.inaf.it/hosted/wings/cone/eqwidth
Title:
WINGS equivalent widths
Short Name:
WINGSEqwidth
Date:
13 Mar 2019 11:58:19
Publisher:
IA2
Description:
The catalog gives the measurements of the optical lines equivalent widths and statistical errors for a sample of ~4400 objects detected in 48 WINGS clusters for which the spectrum is available and reliable. Emission lines have negative EWs, and absorption lines positive EWs, with all the quantities given at rest frame. Spectra were obtained with WYFFOS@WHT and 2dF@AAT and have a resolution of 6 and 9 AA FWHM, respectively. The wavelength coverage ranges from ∼ 3590 to ∼ 6800 AA for the WHT observations, while spectra taken at the AAT cover the ∼ 3600 to ∼ 8000 AA domain. For each object the catalog gives also the magnitude and radial completeness (or weight) that, once combined, describe the global completeness of the sample. Finally a spectral classification is available, made on the basis of the presence/absence and intensity of spectral lines (following Poggianti et al., 1999): 1=e(a); 2=e(b); 3=e(c); 4=k; 5=k+a; 6=a+k.
18. WINGS J photometry
ID:
ivo://ia2.inaf.it/hosted/wings/cone/nirj
Title:
WINGS J photometry
Short Name:
WINGSNirj
Date:
13 Mar 2019 11:59:38
Publisher:
IA2
Description:
Near infrared J photometry for UKIRT detections in 19 belonging to the WINGS survey. (http://adsabs.harvard.edu/abs/2009A%26A...501..851V)
19. WINGS K photometry
ID:
ivo://ia2.inaf.it/hosted/wings/cone/nirk
Title:
WINGS K photometry
Short Name:
WINGSNirk
Date:
13 Mar 2019 11:59:53
Publisher:
IA2
Description:
Near infrared K photometry for UKIRT detections in 26 belonging to the WINGS survey. (http://adsabs.harvard.edu/abs/2009A%26A...501..851V)
20. WINGS K surface photometry
ID:
ivo://ia2.inaf.it/hosted/wings/cone/gasphotk
Title:
WINGS K surface photometry
Short Name:
WINGSGasphotk
Date:
13 Mar 2019 11:58:47
Publisher:
IA2
Description:
This catalog contains the surface brightness measurements of ~71700 galaxies detected in the K images of the WINGS cluster survey for a subsample of 26 clusters observed with the UKIRT WFCAM. For each galaxy K magnitude, mean surface brightness, effective radius, Sersic index and axial ratio are given, together with their erros. These global parameters were obtained by simultaneously fitting the major and minor axis light growth curves of galaxies with a 2D flattened Sersic-law, convolved by the appropriate, space-varying PSF, which was previously evaluated by the tool itself. (http://adsabs.harvard.edu/abs/2006A%26A...446..373P)