AndreaBozzo/ceres-open-data-index huggingface dataset:
ROSETTA-ORBITER 9P MIRO 3 CR2 9P-TEMPEL1 V1.1

This data set contains Spectroscopic and Continuum data taken by the Microwave Instrument for the Rosetta Orbiter (MIRO) during the second cruise phase of the mission. The data consist entirely of observations of comet 9P/Tempel 1 before, during and after the planned collision of the Deep Impact mission impactor spacecraft with that comet in July 2005. These data have been calibrated to antenna temperatures and are presented as a series of binary table files. Version 1.1 added UTC to the data files, added a GEOMETRY directory and incorporated a number of minor documentation additions and corrections.

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Organization: National Aeronautics and Space Administration
HERITAGE SMC Band-Matched Catalog

Observations from the HERschel Inventory of the Agents of Galaxy Evolution (HERITAGE) have been used to identify dusty populations of sources in the Large and Small Magellanic Clouds (LMC and SMC).\nThe study used the HERITAGE catalogs of point sources from both the Photodetector Array Camera and Spectrometer (PACS; 100 and 160 microns) and Spectral and Photometric Imaging Receiver (SPIRE; 250, 350, and 500 microns) cameras. These catalogs are matched to each other to create a Herschel band-merged catalog and then further matched to archival Spitzer IRAC and MIPS catalogs from the Spitzer Surveying the Agents of Galaxy Evolution (SAGE) and SAGE-SMC surveys to create single mid- to far-infrared (far-IR) point source catalogs that span the wavelength range from 3.6 to 500 microns. There are 35,322 unique sources in the LMC and 7503 in the SMC.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0293 V1.0

This is a Rosetta Radio Science data set, collected during the PRELANDING phase 2014-01-21 to 2014-11-18. It is a Global Gravity measurement at the comet 67P and covers the time 2014-09-14T06:17:02.000 to 2014-09-14T15:12:09.000.

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Organization: National Aeronautics and Space Administration
XMM-Newton CFHTLS W1 Field Galaxy Groups Catalog

This table contains a catalog of 128 X-ray galaxy groups, covering a redshift (z) range 0.04 &lt; z &lt;1.23, selected in the ~ 3 deg&lt;sup&gt;2&lt;/sup&gt; part of the CFHTLS W1 field overlapping XMM-Newton observations performed under the XMM-LSS project. The authors carry out a statistical study of the redshift evolution out to redshift 1 of the magnitude gap between the first and the second brightest cluster galaxies of a well defined mass-selected group sample. They find that the slope of the relation between the fraction of groups and the magnitude gap steepens with redshift, indicating a larger fraction of fossil groups at lower redshifts. They also find that 22.2% +/- 6% of their groups at z &lt;= 0.6 are fossil groups. The authors compare their results with the predictions of three semi-analytic models based on the Millennium simulation. The intercept of the relation between the magnitude of the brightest galaxy and the value of magnitude gap becomes brighter with increasing redshift. This trend is steeper than the model predictions which the authors attribute to the younger stellar age of the observed brightest cluster galaxies. This trend argues in favor of stronger evolution of the feedback from active galactic nuclei at z &lt; 1 compared to the models. The slope of the relation between the magnitude of the brightest cluster galaxy and the value of the gap does not evolve with redshift and is well reproduced by the models, indicating that the tidal galaxy stripping, put forward as an explanation of the occurrence of the magnitude gap, is both a dominant mechanism and sufficiently well modeled. In this study, the authors analyzed the XMM-Newton observations of the CFHTLS wide (W1) field as a part of the XMM-LSS survey (Pierre et al., 2007, MNRAS, 382, 279). The details of the observations and the data reduction are presented in Bielby et al. (2010, A&amp;A, 523, A66). The authors concentrate on the low-z counterparts of the X-ray sources and use all XMM-Newton observations performed until 2009, covering an area of 2.276 x 2.276 square degrees. The CFHTLS wide observations were carried out in the period between 2003 and 2008, covering an effective survey area of ~ 154 square degrees. The optical images and data of the CFHTLS were obtained with the MegaPrime instrument mounted on the CFHT in the five filters u*, g&#39;, r&#39;, i&#39; and z&#39;. This table was created by the HEASARC in December 2014 based on &lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/566/A140"&gt;CDS catalog J/A+A/566/A140&lt;/a&gt; file table1.dat. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
Planck 2nd Sunyaev-Zeldovich Source Catalog

This table contains the all-sky Planck catalog of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full Planck mission data. The catalog (PSZ2) is the largest SZ-selected sample of galaxy clusters yet produced and the deepest systematic all-sky survey of galaxy clusters. It contains 1,653 detections, of which 1,203 are confirmed clusters with identified counterparts in external data sets, and is the first SZ-selected cluster survey containing more than 10&lt;sup&gt;3&lt;/sup&gt; confirmed clusters. In the reference paper, the authors present a detailed analysis of the survey selection function in terms of its completeness and statistical reliability, placing a lower limit of 83% on the purity. Using simulations, they find that the estimates of the SZ strength parameter Y&lt;sub&gt;5R500&lt;/sub&gt; are robust to pressure-profile variation and beam systematics, but accurate conversion to Y&lt;sub&gt;500&lt;/sub&gt; requires the use of prior information on the cluster extent. The authors also describe the multi-wavelength search for counterparts in ancillary data, which makes use of radio, microwave, infrared, optical, and X-ray data sets, and which places emphasis on the robustness of the counterpart match. They discuss the physical properties of the new sample and identify a population of low-redshift X-ray under-luminous clusters revealed by SZ selection. These objects appear in optical and SZ surveys with consistent properties for their mass, but they are almost absent from ROSAT X-ray selected samples. Three pipelines were used to detect SZ clusters: two independent implementations of the Matched Multi-Filter (MMF1 and MMF3) and PowellSnakes (PwS). The main catalog contained in this HEASARC table is constructed as the union of the catalogs from the three detection methods. The completeness and reliability of the catalogs have been assessed through internal and external validation as described in section 4 of the reference paper. The HEASARC has changed the names of many of the parameters from those given in the original table. In such cases we have listed the original names in parentheses at the end of the parameter descriptions given below. This table was created by the HEASARC in May 2017 based upon the &lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/594/A27"&gt;CDS Catalog J/A+A/594/A27&lt;/a&gt; file psz2.dat, the main (union of 3 pipelines) SZ source catalog. The source catalogs from the 3 individual pipelines are available at &lt;a href="http://cdsarc.u-strasbg.fr/ftp/cats/J/A+A/594/A27/"&gt;http://cdsarc.u-strasbg.fr/ftp/cats/J/A+A/594/A27/&lt;/a&gt; as the files pszmmf1.dat, pszmmf3.dat and pszpws.dat. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
37-Month MAXI/GSC High Galactic-Latitude Source Catalog

This table contains the catalog of high Galactic-latitude (|b| &gt; 10&lt;sup&gt;o&lt;/sup&gt;) X-ray sources detected in the first 37 months of data accumulation of the Monitor of All-sky X-ray Image/Gas Slit Camera (MAXI/GSC). To achieve the best sensitivity, the authors developed a background model of the GSC that well reproduced the data based on the detailed on-board calibration. Source detection was performed through image fits with a Poisson likelihood algorithm. The catalog contains 500 objects detected with significances &gt;= 7 in the 4-10 keV band. The limiting sensitivity is ~7.5 x 10&lt;sup&gt;-12&lt;/sup&gt; erg cm&lt;sup&gt;-2&lt;/sup&gt; s&lt;sup&gt;-1&lt;/sup&gt; ( ~0.6 mCrab) in the 4-10 KeV band for 50% of the survey area, which is the highest ever achieved in an all-sky survey mission covering this energy band. In their paper, the authors summarize the statistical properties of the catalog and results from cross-matching with the Swift/BAT 70-month catalog (BAT70), the meta-catalog of X-ray detected clusters of galaxies (MCXC), and the MAXI/GSC 7-month catalog (GSC7). This catalog lists the source name (2MAXI), the position and its error, the detection significances and fluxes in the 4-10 keV and 3-4 keV bands, the hardness ratio, and the basic information on the likely counterpart (the latter available for 296 of the sources). This table was created by the HEASARC in September 2013 based on the electronic version of Table 1 from the reference paper which was obtained from The ApJS web site. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
z0MGS_Dust Catalog

The z0MGS_Dust project consists of Herschel images from PACS and SPIRE available for 1578 galaxies, dust emission parameters for 819 galaxies, and integrated photometry and dust parameters for 877 galaxies. The final catalog used in this study uses WISE and Herschel data to derive interstellar dust parameters and scaling relations with other galactic information such as stellar mass, star formation rate, and related values.

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Organization: National Aeronautics and Space Administration
EUVE Bright Sources

This database table contains a detailed list of verified bright EUVE sources detected during the survey phase of the EUVE mission (calibration targets are also included). Two distinct surveys, the all-sky and deep surveys, were conducted by the four EUVE telescopes during the first six months of the mission. Further documentation is available through the HEASARC. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 8 4270 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2021-01-01 to 2022-12-31. It is a Occultation measurement and covers the time 2022-05-27T03:23:00.200 to 2022-05-27T03:45:08.549.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT OSINAC 2 EDR MTP 015 V1.0

This data set contains raw EDR images acquired by the OSIRIS Narrow AngleCamera during the escort phase of the Rosetta mission at the comet 67P,covering the period from 2015-04-08 to 2015-05-05.

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Organization: National Aeronautics and Space Administration
First Byurakan Survey (Markarian) Catalog of UV-Excess Galaxies

A catalog of galaxies with UV-continuum (Markarian galaxies) detected during the First Byurakan Survey (FBS) is presented. The purpose of the FBS was to search for peculiar faint extragalactic objects with UV-excess radiation and to study them. The procedure of observations and processing, the FBS areas, the object selection and classification criteria and also several selection effects are described in the reference. The catalog contains the following initial data on all the objects: the precise coordinates, visual magnitudes, angular sizes, redshifts and classification types. The observational results of slit spectra, UBV-photometry, IR-photometry (IRAS data), morphology and some other data are also included in the catalog. While compiling the catalog, the authors introduced some necessary corrections in the data of the earlier published lists on galaxies with UV-continuum excesses. In addition, the authors included the objects with numbers 1501-1515. In most cases, they are well-known Seyfert galaxies omitted by the authors in the lists, but detected on the plates. 48 objects from their lists are not included in the catalog, since they are either stars of our Galaxy or star projections on the galaxies. This catalog presents the largest homogeneous sample of AGN of different types on the northern sky for bright objects (apparent magnitude &lt; 16.0). Up to the middle of 1987 redshifts were measured for 1459 out of 1469 objects in the catalog. This table was created by the HEASARC in November 2009 based on the electronic version of the First Byurakan Survey (Markarian galaxies catalog) which was obtained from the CDS (their catalog VII/172 file table7.dat). It replaced an earlier version of the &#39;Markarian Catalog&#39; which was based on the original galaxy lists of Markarian et al. (&lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/VII/61A"&gt;CDS catalog VII/61A&lt;/a&gt;). This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
The VIIth Catalog of Galactic Wolf-Rayet Stars

The VIIth Catalogue of Galactic Population I Wolf-Rayet (WR) Stars provides improved coordinates, spectral types, and bv photometry of known WR stars and adds 71 new stars compared to the VIth Catalog. This census of galactic WR stars has reached 227 stars (226 entries in this catalog), comprising 127 WN stars, 87 WC stars, 10 WN/WC stars, and 3 WO stars. This includes 15 WNL and 11 WCL stars within 30 pc of the Galactic Center. The catalog includes information on periodicity, binarity, terminal wind velocities, correlations with open clusters, OB associations, H I bubbles, H II regions, and ring nebulae, observed and dereddened narrow-band bv photometry, and distances, both heliocentric and galactocentric, and lists the references from which this information was obtained. This catalog was created by the HEASARC in April 2001, based on electronic versions of Tables 13, 14, 15, and 28 from the published paper containing the catalog which were directly supplied to the HEASARC by the author. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 CAL RDR ELECTRON SPECTROMTR EXT4 V1.0

This data set contains calibrated Mars Express ASPERA-3         Electron Spectrometer (ELS) data for the fourth mission         extension (January 1, 2013 - Dec. 31, 2014).  These data         are provided in units of Differential Number Flux (DNF):         cnts/(cm**2-sr-sec-eV)

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Organization: National Aeronautics and Space Administration
Spitzer Wide-area InfraRed Extragalactic Survey XMM-LSS MIPS24 Single-Band Catalog

The Spitzer Wide-area InfraRed Extragalactic survey (SWIRE), the largest Spitzer Legacy program, is a wide-area, imaging survey to trace the evolution of dusty, star-forming galaxies, evolved stellar populations, and AGN as a function of environment, from redshifts z~3 to the current epoch. SWIRE surveys 6 high-latitude fields, totaling ~50 sq. deg. in all 7 Spitzer bands: 3.6, 4.5, 5.8, and 8 microns with IRAC and 24, 70, and 160 microns with MIPS (Lonsdale et al. 2003). The SWIRE Legacy Extragalactic Source Catalogs will eventually contain in excess of 2 million IR-selected galaxies, from those dominated by the light of stellar populations detected primarily by IRAC, to starbursts, ultra-luminous infrared galaxies and AGN detected also by MIPS.\n\nThe main SWIRE catalogs for 24 micron data are the Optical-IRAC-MIPS24 bandmerged catalogs. The bandmerged catalogs require a detection in the shortest IRAC band (3.6 microns). The SWIRE project has produced single-band 24 micron catalogs to cover regions that lie outside the IRAC images, and to include sources that for some reason were not associated with a 3.6 micron detection.

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Organization: National Aeronautics and Space Administration
Spitzer Survey of Stellar Structure in Galaxies Catalog

The Spitzer Survey of Stellar Structure in Galaxies (S4G) is a volume-, magnitude-, and size-limited survey of over 2300 nearby galaxies at 3.6 and 4.5 microns. This is an extremely deep survey reaching an unprecedented 1 sigma surface brightness limit of μ3.6(AB) = 27 mag arcsec-2. This translates to a stellar surface density of << 1 Msun pc-2.\n\nThe S4G Catalog provides photometry and model parameters derived from the IRAC images, as well as a link to the summary and data access page for each galaxy and a variety of quantities taken from previously published work.

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Organization: National Aeronautics and Space Administration
ROSAT All-Sky Survey: Soft High Galactic-Latitude X-Ray Sources 2

This table contains a summary of spectroscopic identifications of bright soft high-galactic-latitude X-ray sources from the ROSAT All-Sky Survey (RASS) with total PSPC count rates 0.11 &lt; CR &lt; 0.5 cts/s and hardness ratios HR1 &lt; 0. This study supplements the identification program of a complete sample of sources with CR &gt;= 0.5 cts/s presented previously (Thomas et al. 1998, A&amp;A, 335, 467; available at the HEASARC as the RASSHGSOFT table). Spectroscopic identifications are presented for 70 of 77 sources, 5 sources are identified by other means, and subsidiary information is given for 2 as yet unidentified sources. In practically all cases, a unique optical counterpart exists. As for the brighter fraction of the sample, the largest source classes are Seyfert 1 galaxies, magnetic cataclysmic variables, and hot white dwarfs. In the Galactic Pole caps at |b| &gt; 40 degrees, Seyfert galaxies dominate, whereas at intermediate latitudes galactic objects as magnetic cataclysmic variables and white dwarfs become relatively more frequent. This table was created by the HEASARC in May 2012 based on &lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/347/47"&gt;CDS Catalog J/A+A/347/47&lt;/a&gt; file table3,dat. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
VG2 JUP PLS PLASMA DERIVED ION MOMENTS    96.0 SEC V1.0

This data set contains the best    estimates of the total ion density from Voyager 2 at Jupiter in the PLS    voltage range (10-5950 eV/Q). It is calculated using the method of    which to first order consists of taking the total measured current and    dividing by the collector area and plasma bulk velocity. This method is    only accurate for high mach number flows directly into the detector, and    may result in underestimates of the total density of a factor of 2 in the    outer magnetosphere. Thus absolute densities should be treated with    caution, but density variations in the data set can be trusted. The low    resolution mode density is used at all times except day 190 2100-2200 when    the larger of the high and low resolution mode densities in a 96 sec    period is used. Corotation is assumed inside L=17.5, and a constant    velocity component of 200 km/s into the D cup is used outside of this.    Data format: column 1 is time (yyyy-mm-ddThh:mm:ss.sssZ), column 2 is    the moment density in cm^-3. Each row has format (a24, 1x, 1pe9.2). Values    of -9.99e+10 indicate that the parameter could not be obtained from the    data using the standard analysis technique. Additional information about    this data set and the instrument which produced it can be found elsewhere    in this catalog.

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Organization: National Aeronautics and Space Administration
Subaru Prime Focus Camera (Suprime-Cam) Exposures Log

This table contains the Subaru Prime Focus Camera (Suprime-Cam) log of exposures having observation type = &#39;OBJECT&#39; (those with &#39;BIAS&#39;, &#39;FLAT&#39; and other types are not included) which have been made since April 2001. Note that from the version of Nov. 2005 on, the number of rows has significantly increased because those data with worse position determination (up to 30 arcsec error) are now included. The data currently extend to November 2005 and it is anticipated that they will be regularly updated Suprime-Cam is an 80-mega pixels (10240 x 8192) mosaic CCD camera, for the wide-field prime focus of the 8.2m Subaru telescope. Suprime-Cam covers a field of view 34&#39; x 27&#39;, a unique facility among the 8-10m class telescopes, with a resolution of 0.202 arcseconds per pixel. The focal plane consists of ten high-resistivity 2kx2k CCDs developed by MIT Lincoln Laboratory, which are cooled by a large Stirling-cycle cooler. The CCD readout electronics was designed to be scalable, which allows the multiple read-out of tens of CCDs. It takes 50 seconds to readout entire arrays. A filter-exchange mechanism of the jukebox type is designed that can hold up to ten large filters (205 x 170 x 15 mm&lt;sup&gt;3&lt;/sup&gt;). The wide-field corrector is basically a three-lens Wynne-type, but has a new type of atmospheric dispersion corrector. The corrector provides a flat focal plane and an un-vignetted field of view of 30&#39; in diameter. The achieved co-planarity of the focal array mosaic is smaller than 30 um peak-to-peak, which realizes mostly the seeing limited image over the entire field. The median seeing in the I_c-band, measured over one year and a half, is 0.61 arcseconds. The PSF anisotropy in Suprime-Cam images, estimated by stellar ellipticities, is about 2% under this median seeing condition. At the time of its commissioning, Suprime-Cam had the largest survey speed, which is defined as the field of view multiplied by the primary mirror area of the telescope, among those cameras built for sub-arcsecond imaging. For more details, see: Miyazaki et al., Publ. Astron. Soc. Japan 54, 833-853, 2002 (2002PASJ...54..833M). This table was created by the HEASARC in September 2007 based on CDS table B/subaru/suprimc.dat (the ReadMe file for the latter was tagged with a date of August 25th, 2007). This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
Ginga LAC Mode Catalog

The GINGAMODE database table contains selected information from the Large Area Counter (LAC) aboard the third Japanese X-ray astronomy satellite Ginga. The Ginga experiment began on day 36, 5 February 1987 and ended in November 1991. Ginga consisted of the LAC, the all-sky monitor (ASM) and the gamma-ray burst detector (GBD). The satellite was in a circular orbit at 31 degree inclination with apogee 670 km and perigee 510 km, and with a period of 96 minutes. A Ginga observation consisted of varying numbers of major frames which had lengths of 4, 32, or 128 seconds, depending on the setting of the bitrate. Each GINGAMODE database entry consists of data from the first record of a series of observations having the same values of the following: &quot;BITRATE&quot;, &quot;LACMODE&quot;, &quot;DISCRIMINATOR&quot;, or &quot;ACS MONITOR&quot;. When any of these changed, a new entry was written into GINGAMODE. The other Ginga catalog database, GINGALOG is also a subset of the same LAC dump file used to create GINGAMODE. GINGALOG contains a listing only whenever the &quot;ACS monitor&quot; (Attitude Control System) changes. Thus, GINGAMODE monitors changes in four parameters and GINGALOG is a basic log database mapping the individual FITS files. Ginga FITS files may have more than one entries in the GINGAMODE database. Both databases point to the same archived Flexible Image Transport System (FITS) files created from the LAC dump files. The user is invited to browse though the observations available from Ginga using GINGALOG or GINGAMODE, then extract the FITS files for more detailed analysis. The Ginga LAC Mode Catalog was prepared from data sent to NASA/GSFC from the Institute of Space and Astronautical Science (ISAS) in Japan. &lt;p&gt; Duplicate entries were removed from the HEASARC implementation of this catalog in June 2019. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration