- 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)
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- 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)
- 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)
- 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.
- 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)
- 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)
- 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)
- ID:
- ivo://ia2.inaf.it/hosted/wings/cone/locdens
- Title:
- WINGS local densities (Mv<-19.5)
- Short Name:
- WINGSLocDens19.5
- Date:
- 13 Mar 2019 11:59:19
- Publisher:
- IA2
- Description:
- For each WINGS galaxy with V absolute magnitude brighter than -16, the local density calculated as the Log (decimal) of the number of galaxies with M_V <= -19.5 per Mpc**2 is given. It is computed from the circular area enclosing the first 10 closest galaxies, plus the background counts expected from Berta et al. (2006). The Local Densities are also corrected for border effects. The Coverage field fraction are also given, both at CCDX, i.e. the fraction of the circular area of radius CCDX and centered in the X-ray center, which is included in the field of the CCD mosaics, and at CCDB (centered in the BCG). For clusters without velocity dispersion the distances are given in pixels and NOT in R200. These clusters are A311, A2665, A3164, and Z1261.
19. WINGS morphology
- ID:
- ivo://ia2.inaf.it/hosted/wings/cone/morphot
- Title:
- WINGS morphology
- Short Name:
- WINGSMorphot
- Date:
- 13 Mar 2019 11:59:29
- Publisher:
- IA2
- Description:
- The catalogue contains a total number of ~39 900 galaxies, for which we provide the automated estimates of the morphological type, applying the purposely devised tool MORPHOT to the V-band WINGS imaging. The used tool is non-parametric and fully empirical. In particular, MORPHOT exploits 21 morphological diagnostics, directly and easily computable from the galaxy image, to provide two independent classifications: one based on a maximum likelihood (ML), semi- analytical technique and the other one on a neural network (NN) machine. A suitably selected sample of ∼1000 visually classified WINGS galaxies is used to calibrate the diagnostics for theML estimator and as a training set in the NN machine. The final morphological estimator combines the two techniques. (http://adsabs.harvard.edu/abs/2012MNRAS.420..926F)
- ID:
- ivo://ia2.inaf.it/hosted/wings/cone/opt
- Title:
- WINGS Optical photometry
- Short Name:
- WINGSOpt
- Date:
- 13 Mar 2019 00:00:05
- Publisher:
- IA2
- Description:
- Optical (V, B) photometric catalog of WINGS detections (galaxies, stars, unclassified objects) in the 76 wide--fields of the WINGS survey of local clusters of galaxies. (http://adsabs.harvard.edu/abs/2009A%26A...497..667V)
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