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1. AKARI Far-infrared All-Sky Survey Maps
ID:
ivo://jvo/isas/akari/fis_v1
Title:
AKARI Far-infrared All-Sky Survey Maps
Short Name:
AKARI_FIS_V1
Date:
18 Dec 2022 01:11:53
Publisher:
JVO
Description:
The AKARI Far-infrared All-Sky Survey Maps is produced with the participation of people from the following institutes: University of Tokyo, ISAS/JAXA, Tohoku University, and University of Tsukuba. The image data in this release are produced based on the AKARI All-Sky Survey with 4 far-infrared bands at N60 (65 um), WIDE-S (90 um), WIDE-L (140 um), and N160 (160 um).
2. AKARI N60
ID:
ivo://nasa.heasarc/skyview/akari
Title:
AKARI N60
Short Name:
AKARI
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The AKARI (formerly Astro-F) mission is a Japanese second generation all-sky infrared survey mission. SkyView currently includes surveys from the four bands of the FIS instrument: N60, WIDE-S, WIDE-L and N160. <p> These surveys cover 99% of the sky in four photometric bands centred at 65μm, 90μm, 140μm, and 160μm, with spatial resolutions ranging from 1-1.5'. <p> These data provide crucial information on the investigation and characterisation of the proper- ties of dusty material in the interstellar medium (ISM), since a significant portion of its energy is emitted between ∼50 and 200 μm. The large-scale distribution of interstellar clouds, their thermal dust temperatures, and their column densities can be investigated with the improved spatial resolution compared to earlier all-sky survey observations. In addition to the point source distribution, the large-scale distribution of ISM cirrus emis- sion, and its filamentary structure, are well traced. <p> Data are obtained using using the <a href="https://jvo.nao.ac.jp/index-e.html">JVO</a> AKARI Simple Image Access Service. Provenance: AKARI FIS map making team [Univ of Tokyo, ISAS/JAXA, Tohoku Univ, Tsukuba Univ, The Rutherford Appleton Laboratory, The Open Univ]. This is a service of NASA HEASARC.
3. Bonn 1420 MHz Survey
ID:
ivo://nasa.heasarc/skyview/1420mhz
Title:
Bonn 1420 MHz Survey
Short Name:
1420MHz
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
This survey was taken with the Bonn Stockert 25m telescope. It was distributed on the NRAO <i>Images from the Radio Sky</i> CD-ROM. This image was delivered as a four map mosaic but was combined into a single map before being included in <i>SkyView</i>. Provenance: Max Planck Institute for Radio Astronomy, generated by P. Reich and W. Reich. This is a service of NASA HEASARC.
4. CGRO Compton Telescope: 3 channel data
ID:
ivo://nasa.heasarc/skyview/comptel
Title:
CGRO Compton Telescope: 3 channel data
Short Name:
Comptel
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
This survey is a maximum entropy solution to the data taken by the CompTel instrument on the <i> Compton </i> Gamma Ray Observatory. The data in this survey are intended only to give the general appearance of the MeV gamma-ray sky. Fluxes, flux limits and spectra should be derived using the Compass system for the analysis of CompTel data. Compass is available at the <a href="https://web.archive.org/web/20100622161007/http://wwwgro.unh.edu/comptel/compass/compass_users.html"> Compton Observatory Science Support Center </a>. <P> The maps were originally generated by the CompTel Instrument Team as three separate maps in the bands: <UL> <LI>1-3 MeV <LI>3-10 MeV <LI>10-30 MeV </ul> <P> All CompTel observations from phases 1, 2 and 3 were included in the maps (May 1991 through October 1994). These maps were combined into a single 3-D map at <i> SkyView </i> <P> Provenance: CompTel Instrument Team. Maps generated by Andrew Strong, Max-Planck Institute for Extraterrestrial Physics (Garching).. This is a service of NASA HEASARC.
5. CO Galactic Plane Survey
ID:
ivo://nasa.heasarc/skyview/co
Title:
CO Galactic Plane Survey
Short Name:
CO
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
New large-scale CO surveys of the first and second Galactic quadrants and the nearby molecular cloud complexes in Orion and Taurus, obtained with the Harvard-Smithsonian Center for Astrophysics 1.2 m telescope, have been combined with 31 other surveys obtained over the past two decades with that instrument and a similar telescope on Cerro Tololo in Chile, to produce a new composite CO survey of the entire Milky Way. The survey consists of 488,000 spectra that Nyquist or beamwidth (1/8 deg) sample the entire Galactic plane over a strip 4 deg-10 deg wide in latitude, and beamwidth or 1/4 deg sample nearly all large local clouds at higher latitudes. Compared with the previous composite CO survey of Dame et al. (1987), the new survey has 16 times more spectra, up to 3.4 times higher angular resolution, and up to 10 times higher sensitivity per unit solid angle. <P> Users should be aware that both the angular resolution and the sensitivity varies from region to region in the velocity-integrated map. The component surveys were integrated individually using clipping or moment masking in order to display nearly all statistically significant emission but little noise above a level of ~1.5 K km/s. See the reference below and the <a href="https://lweb.cfa.harvard.edu/mmw/"> Millimeter-Wave Group site</a> for more details Provenance: Data taken by two nearly-identical 1.2 m telescopes in Cambridge, MA and on Cerro Tololo, Chile combined into a complete survey of the Milky Way with CO integrated over all velocities.. This is a service of NASA HEASARC.
6. Cosmic Background Explorer DIRBE Annual\ Average\ Map
ID:
ivo://nasa.heasarc/skyview/cobe
Title:
Cosmic Background Explorer DIRBE Annual\ Average\ Map
Short Name:
COBE
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The DIRBE Project Data Sets cover the whole sky and provide photometric data in 10 bands ranging in wavelength from 1.25 to 240 microns. SkyView has supported three maps: an early averaged map including including zodiacal and Galactic components (COBE DIRBE (OLD)), a more recent cleaner version of that data (COBE DIRBE/AAM) and a map with the zodaical light subtracted out (COBE DIRBE/ZSMA). The early data is no longer supported. Please contact us if you want access to these data. <P> Detailed descriptions of the DIRBE, the data processing, and the data products are given in an Explanatory Supplement. A Small Source Spectral Energy Distribution Browser can be used to assess the visibility of an unresolved or small extended source in the DIRBE data and see its spectral energy distribution. As noted in section 5.6.6 of the Explanatory Supplement, the DIRBE Time-ordered Data are required to derive definitive point source fluxes. <p> These maps provide an estimate of the infrared intensity at each pixel and wavelength band based on an interpolation of the observations made at various times at solar elongations close to 90&amp;#176;;. <P> These COBE DIRBE maps are a combination original ten band passes with the following wavelengths: <UL> <LI>Band 1 - 1.25 &amp;#181;;m <LI>Band 2 - 2.2 &amp;#181;;m <LI>Band 3 - 3.5 &amp;#181;;m <LI>Band 4 - 4.9 &amp;#181;;m <LI>Band 5 - 12 &amp;#181;;m <LI>Band 6 - 25 &amp;#181;;m <li>Band 7 - 60 &amp;#181;;m <li>Band 8 - 100 &amp;#181;;m <li>Band 9 - 140 &amp;#181;;m <li>Band 10 - 240 &amp;#181;;m </ul> <p> The default two dimensional array uses Band 8 (100 &amp;#181;;m). <P> The COBE DIRBE/Annual Average Maps (AAM) is the cumulative weighted average of the photometry. This average is calculated using the weighted number of observations from each Weekly Averaged Map ( WtNumObs from the Weekly Averaged Map) as the weight, such that annual_average =sum( weekly_average * weekly_weight )/ sum( weekly_weight ) <p> COBE DIRBE/Zodi-Subtracted Mission Average (ZSMA) Skymap represents the extra-Solar system sky brightness. It is the average residual map that results after the modelled interplanetary dust (IPD) signal is subtracted from each of the DIRBE Weekly Skymaps from the cryogenic mission. Individual weekly residual maps can be reconstructed from the data supplied in the DIRBE Sky and Zodi Atlas (DSZA). Provenance: COBE Team. This is a service of NASA HEASARC.
7. Dickey and Lockman HI map
ID:
ivo://nasa.heasarc/skyview/nh
Title:
Dickey and Lockman HI map
Short Name:
nH
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
This survey is derived from the 21cm maps presented by Dickey and Lockman in the <i>ARAA</i> 28, p215. The nH is derived assuming optically thin emission. The nH given should be considered a lower limit when the nH is greater than several times 10<sup>20</sup>. Provenance: provided by S. Snowden from data by Dickey and Lockman. This is a service of NASA HEASARC.
8. Digitized First Byurakan Survey (DFBS) Extracted Spectra
ID:
ivo://org.gavo.dc/dfbsspec/q/spectra
Title:
Digitized First Byurakan Survey (DFBS) Extracted Spectra
Short Name:
dfbsspec.spectra
Date:
06 Feb 2024 09:11:09
Publisher:
The GAVO DC team
Description:
This table contains basic metadata as well as the spectra from the Digital First Byurakan Survey (DFBS).
9. Digitized First Byurakan Survey (DFBS) Plate Scans
ID:
ivo://org.gavo.dc/dfbs/q/i
Title:
Digitized First Byurakan Survey (DFBS) Plate Scans
Short Name:
DFBS plates
Date:
05 Jan 2023 13:10:51
Publisher:
The GAVO DC team
Description:
First Byurakan survey plate scan service
10. Digitized First Byurakan Survey (DFBS) Plate Scans
ID:
ivo://padc.obspm.astro/dfbs/q/i
Title:
Digitized First Byurakan Survey (DFBS) Plate Scans
Short Name:
DFBS plates
Date:
26 Feb 2021 10:16:00
Publisher:
Paris Astronomical Data Centre
Description:
First Byurakan survey plate scan service