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11. 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)
12. 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)
13. 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)
14. The VIMOS Public Extragalactic Redshift Survey (VIPERS) Spectra
ID:
ivo://ia2.inaf.it/hosted/vipers/ssap
Title:
The VIMOS Public Extragalactic Redshift Survey (VIPERS) Spectra
Short Name:
VIPERS Spectra
Date:
02 Mar 2015 19:00:00
Publisher:
IA2
Description:
VIMOS Public Extragalactic Redshift Survey" (VIPERS) is an ongoing ESO Large Program to map in detail the spatial distribution of normal galaxies over an unprecedented volume of the z~1 Universe. VIPERS is using VIMOS at the VLT to measure 100,000 redshifts for galaxies with red magnitude I(AB) brighter than 22.5 over an area of 24 square degrees. At this redshift, VIPERS fills a unique niche in galaxy surveys, optimizing the combination of 5-band accurate photometry from the CFHTLS with the multiplexing capability of VIMOS. A robust color-color pre-selection allows the survey to focus its measurements on the 0.5 <= z <= 1.2 redshift range, yielding an optimal combination of large volume (5 x 107 h-3 Mpc3) and high effective spectroscopic sampling (> 40%). With these figures, the VIPERS data set represents the z~1 equivalent of state-of-the-art "local" (z<=0.2) surveys. VIPERS scientific investigations focus on measurements of large-scale structure and cosmological parameters at an epoch when the Universe was about half its current age. At the same time, the survey can explore the ensemble properties of luminous galaxies, groups and clusters with unprecedented statistical accuracy at these redshifts.
15. Tirgo IR Archive
ID:
ivo://ia2.inaf.it/hosted/tirgo/arnica
Title:
Tirgo IR Archive
Date:
13 Mar 2019 11:37:19
Publisher:
IA2
Description:
The Archive is formed with all files measured with ARcetri Near Infrared CAmera ( ARNICA). Each files contains (in FITS format) or a single exposure or the mean of single exposures taken at the same telescope position. The filer used can be either a Johnson broad band infrared filter (J, H, K), or a narrow band filter (see ARNICA) page for details). Most measures was acquired at the TIRGO telescope, while a smaller sample cames from the few telescopes Arnica was ported to (WHT, NOT, VATT and TNG). All frame are in FITS format and are 256x256 pixels in size. The archive contains more than 250.000 frames. Most files belongs to a compound measure (we call them "a mosaic").
16. TNG - LRS @ IA2 image archive
ID:
ivo://ia2.inaf.it/tng/lrs/siap
Title:
TNG - LRS @ IA2 image archive
Date:
13 Mar 2019 11:38:26
Publisher:
IA2
Description:
DOLORES (Device Optimized for the LOw RESolution) is a focal reducer instrument installed at the Nasmyth B focus of the TNG. The detector is a 2048 x 2048 E2V 4240 Thinned back-illuminated, deep-depleted, Astro-BB coated CCD with a pixel size of 13.5 µ. The scale is 0.252 arcsec/px which yields a field of view of about 8.6 x 8.6 arcmin. The instrument allows imaging through broad and narrow band filters as well as spectroscopic observations with resolving powers between RS=~500 and RS=~6000. A multi-slit mode, based on custom masks manufactured by a dedicate cutting machine, is also available. Please note that MOS programs are bound to strict constraints on the number of masks and on the time necessary to design and manufacture them. In particular, each program can request up to a maximum of 5 masks per night and 10 masks per observing run.
17. TNG - NICS @ IA2 image archive
ID:
ivo://ia2.inaf.it/tng/nics/siap
Title:
TNG - NICS @ IA2 image archive
Date:
13 Mar 2019 11:38:50
Publisher:
IA2
Description:
NICS (Near Infrared Camera Spectrometer) is the TNG infrared (0.9-2.5 µm) multimode instrument which is based on a HgCdTe Hawaii 1024x1024 array. Its observing capabilities include imaging (4.2' x 4.2' f.o.v.), high-throughput low resolution spectroscopy (RS=50-500), medium resolution spectoscopy (max-R=2500), imaging polarimetry, spectropolarimetry and, when coupled to the adaptive optics module, nearly diffraction limited imaging.
18. TNG - OIG @ IA2
ID:
ivo://ia2.inaf.it/tng/oig/siap
Title:
TNG - OIG @ IA2
Date:
13 Mar 2019 11:39:14
Publisher:
IA2
Description:
OIG is a CCD camera for direct imaging at optical wavelengths (between 0.32 nd 1.1 microns) for the TNG. It is mounted on the Nasmyth A Adapter interface. OIG is designed to host a variety of CCD chips or mosaics for a field of view up to 10 arcmin. At the moment it is equipped with a mosaic of two thinned and back-illuminated EEV 42-80 CCDs with 2048 x 4096 pixels each (pixel size of 13.5 microns). The resulting pixel scale is 0.072 arcsec/pix for a total field of view of about 4.9 x 4.9 arcmin.
19. 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)
20. 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 &#8764; 3590 to &#8764; 6800 AA for the WHT observations, while spectra taken at the AAT cover the &#8764; 3600 to &#8764; 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.