AndreaBozzo/ceres-open-data-index huggingface dataset:
ROSETTA-ORBITER CHECK MIDAS 3 EAR1 PC0 V1.0

The Micro-Imaging Dust Analysis System (MIDAS) is an instrument on the ROSETTA Orbiter that will provide 3D images and statistical parameters of pristine cometary particles hitting the detector. This data set includes all data from the EARTH SWING-BY 1 mission phase.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3299 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2010-01-01 to 2012-12-31. It is a Global Gravity measurement and covers the time 2012-05-15T12:00:00.500 to 2012-05-27T08:17:11.500.

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Organization: National Aeronautics and Space Administration
Spitzer Wide-area InfraRed Extragalactic Survey XMM-LSS Optical-IRAC-MIPS24 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
ROSETTA-ORBITER CHECKOUT OSINAC 4 CR2 RDR V1.0

This CODMAC level 4 data set contains radiometric calibrated and geometric distortion corrected (resampled) image data in W/m^2/sr/nm,  acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft  during the CRUISE 2 mission phase, covering the period  from 2005-04-05T00:00:00.000 to 2006-07-28T23:59:59.000. The prime objective was commissioning / calibration. Several targets of opportunity were observed, but none of them is identifiable as prime target. This version V1.0 is the first version of this dataset.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER SW RPCMAG 2 RVM1 RAW V9.0

This dataset contains EDITED RAW DATA (CODMAC LEVEL 2) of theRENDEZVOUS MANOEUVRE 1 (RVM1) from November 22, 2010 until December 06, 2010of the ROSETTA orbiter magnetometer RPCMAG.The current version of the dataset is V9.0.The difference to the datasets of earlier versions is mainly a significantlyimproved sensor temperature model, more detailed documentation about magneticdisturbance sources, more data handling information for the user andalso an improved quality flagging system.This applies mainly to CALIBRATED and RESAMPLED datasets. The RAW dataset,however, has been updated as well in order provide all datasets at thesame stage, although RAW data proper did not change.

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Organization: National Aeronautics and Space Administration
Spitzer Extragalactic First Look Survey MIPS 24 micron Calibration Star Catalog

The Extragalactic First Look Survey is composed of 4 square degrees of imaging with MIPS and IRAC centered at J1718+5930, with extensive ancillary data from ground-based optical and radio telescopes. As one of the first observations made with Spitzer after the completion of Science Verification at the end of 2003 November, the aim of this 67 hr survey was to characterize the extragalactic source populations observed with Spitzer down to sub-millijansky levels in the mid-infrared.

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Organization: National Aeronautics and Space Administration
Planck Catalog of Compact Sources 217GHz Catalog

The Planck Catalogue of Compact Sources (PCCS) is a sample of reliable sources, both Galactic and extragalactic, extracted directly from the Planck nominal maps. The first public version of the PCCS, a component of Planck Data Release 1, is derived from the data acquired by Planck between August 13 2009 and November 26 2010. The PCCS consists of nine lists of sources, extracted independently from each of Planck's nine frequency channels. The source lists contain 24 columns per source at the LFI and HFI bands. The 857 GHz source list has six additional columns which give the flux densities and flux density uncertainties at the three adjacent lower frequencies: 217, 353, and 545 GHz.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 ROSETTA EXTENSION 1 1399 V1.0

This is a Rosetta Radio Science data set, collected during the ROSETTA EXTENSION 1 phase 2016-01-01 to 2016-04-05. It is a Global Gravity measurement at the comet 67P and covers the time 2016-02-04T23:33:05.000 to 2016-02-05T08:44:20.000.

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Organization: National Aeronautics and Space Administration
COSMOSFieldX-Ray&FIRDetectedAGNMultiwavelengthPropertiesCatalog

The coeval AGN and galaxy evolution and the observed local relations between super-massive black holes (SMBHs) and galaxy properties suggest some connection or feedback between SMBH growth and galaxy build-up. The authors looked for correlations between properties of X-ray detected AGN and their far-infrared (FIR) detected host galaxies, to find quantitative evidences for this connection, highly debated in recent years. They exploit the rich multi-wavelength data set (from X-ray to FIR) that is available in the COSMOS field for a large sample (692 sources) of AGN and their hosts, in the redshift range 0.1 &lt; z &lt; 4, and use X-ray data to select AGN and determine their properties (intrinsic luminosity and nuclear obscuration), and broad-band (from UV to FIR) spectral energy distribution (SED) fitting to derive host galaxy properties, viz., the stellar mass (M&lt;sub&gt;*&lt;/sub&gt;) and the star formation rate (SFR). The authors find that the AGN 2-10 keV luminosity (L&lt;sub&gt;X&lt;/sub&gt;) and the host galaxy 8-1000 um star formation luminosity (L&lt;sup&gt;SF&lt;/sup&gt;&lt;sub&gt;IR&lt;/sub&gt;) are significantly correlated. However, the average host L&lt;sup&gt;SF&lt;/sup&gt;&lt;sub&gt;IR&lt;/sub&gt; has a flat distribution in bins of AGN L&lt;sub&gt;X&lt;/sub&gt;, while the average AGN L&lt;sub&gt;X&lt;/sub&gt; increases in bins of host L&lt;sup&gt;SF&lt;/sup&gt;&lt;sub&gt;IR&lt;/sub&gt;, with a logarithmic slope of ~ 0.7, in the redshifts range 0.4 &lt; z &lt; 1.2. In the reference paper, the authors also discuss the comparison between the distribution of these two quantities and the predictions from hydrodynamical simulations. Finally, they find that the average column density (N&lt;sub&gt;H&lt;/sub&gt;) shows a positive correlation with the host M&lt;sub&gt;*&lt;/sub&gt;, at all redshifts, but not with the SFR (or L&lt;sup&gt;SF&lt;/sup&gt;&lt;sub&gt;IR&lt;/sub&gt;). This translates into a negative correlation with specific SFR. These results are in agreement with the idea that BH accretion and SFRs are correlated, but occur with different variability time scales. The presence of a positive correlation between N&lt;sub&gt;H&lt;/sub&gt; and host M&lt;sub&gt;*&lt;/sub&gt; suggests that the X-ray N&lt;sub&gt;H&lt;/sub&gt; is not entirely due to the circumnuclear obscuring torus, but may also include a contribution from the host galaxy. This table summarizes the multiwavelength properties of the 692 AGN-host systems detected in the COSMOS field both in the X-ray and in the FIR (the X-FIR sample). This table was created by the HEASARC in July 2017, based on &lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/602/A123"&gt;CDS Catalog J/A+A/602/A123&lt;/a&gt; file table1.dat, which contains the multiwavelength properties of the 692 sources in the X-FIR sample. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
Fermi LAT Bright Source List

The Fermi LAT table of bright sources is a list of bright LAT sources that have statistical significances of 10 sigma or higher, based on the first three months of survey data. The primary purpose of this list is to assist proposers for Guest Investigator Cycle 2 (due date 6 March). This list will eventually be superseded by the LAT Source Catalog, to be released about one year after launch. This database table was created by the HEASARC in February 2009 based on the electronic data obtained from the Fermi Science Support Center (FSSC) available at &lt;a href="http://fermi.gsfc.nasa.gov/ssc/data/access/lat/bright_src_list/"&gt;http://fermi.gsfc.nasa.gov/ssc/data/access/lat/bright_src_list/&lt;/a&gt;. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
Updated Planck Catalog of Sunyaev-Zeldovich Sources Release 1

The all-sky Planck catalog of 1,227 clusters and cluster candidates (PSZ1) derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations included 683 so-called previously known clusters. PSZ1 was first published in March 2013 (Planck Collaboration 2013 (2013yCat.8091....0P, and 2014A&amp;A...571A..29P). This HEASARC table contains an updated version of the PSZ1 catalog, version 2.1 (10-02-2015) according to the CDS documentation, reporting the further confirmation of 86 Planck-discovered clusters. In total, the PSZ1 now contains 947 confirmed clusters, of which 214 were confirmed as newly discovered clusters through follow-up observations undertaken by the Planck Collaboration. The updated PSZ1 contains redshifts for 913 systems, of which 736 (~80.6%) are spectroscopic, and associated mass estimates derived from the Y&lt;sub&gt;z&lt;/sub&gt; mass proxy. A new SZ quality flag is also provided for the remaining 280 candidates. This flag was derived from a novel artificial neural-network classification of the SZ signal. Based on this assessment, the purity of the updated PSZ1 catalogue is estimated to be 94%. This table was originally ingested by the HEASARC in May 2013. An updated version (2.1) was ingested by the HEASARC in October 2015 based on &lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/581/A14"&gt;CDS Catalog J/A+A/581/A14&lt;/a&gt; files psz1v2_1.dat and notes.dat. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
CGRO/BATSE Trigger Data

The BATSE Trigger data (each trigger is specified by a unique trigger number) are a set of triggered events that are classified as either a (solar) flare, (gamma-ray) burst, soft gamma-ray repeater (sgr), terrestrial gamma flash (tgf), or tagged with the name of a known source. Not all triggers pass the acceptance tests, so not all trigger numbers are present. For each trigger, there is an associated set of FITS data files that represent the raw data sources and some higher level data products. Spectral (SD) data are prefixed with an &#39;s&#39; (e.g. &#39;sher&#39;). Not all data types are available for all triggers due to instrument mode differences. Available data taken prior to the trigger may contain the beginning of the triggering event before it satisfied the triggering criteria. Background-type files can be used to remove background signal levels from the triggered period. The BFITS data files - containing burst and background spectral data as a function of time - and the detector response matrices (DRM) - modeling the instrument response to account for scattering and other effects - are extremely useful for gamma-ray burst analysis. Also, the BFITS and DRM files can be converted to PHA-II and RMF format for analysis with XSPEC using available FTOOLS. Please refer to the Data_Products section for more details on the various file types. A current description of the BATSE data holdings including the TRIGGER files is also available in the 1998 Legacy article, online at: &lt;pre&gt; &lt;a href="https://heasarc.gsfc.nasa.gov/docs/journal/cgro7.html"&gt;https://heasarc.gsfc.nasa.gov/docs/journal/cgro7.html&lt;/a&gt; &lt;/pre&gt; General information about BATSE is available at the Compton Observatory Science Support Center (COSSC) web site at: &lt;pre&gt; &lt;a href="https://heasarc.gsfc.nasa.gov/docs/cgro/batse/"&gt;https://heasarc.gsfc.nasa.gov/docs/cgro/batse/&lt;/a&gt; &lt;/pre&gt; This database table was created through a cooperative effort of the HEASARC and the Compton Observatory Science Support Center (COSSC). The table data were last updated in November, 2003. The HEASARC added Galactic coordinates in August, 2005. The &quot;_trigger&quot; field was renamed to &quot;trigger_id&quot; in September, 2020. 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 4341 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2023-12-31.                                     It is a Occultation                                     measurement and covers the time                                     2023-09-17T01:21:19.000 to                                     2023-09-17T01:43:27.200.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0388 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 2014-10-26T14:54:00.000 to 2014-10-26T21:30:32.000.

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Organization: National Aeronautics and Space Administration
Hewitt&Burbidge(1991)CatalogofExtragalacticEmission-LineObjects

This is the Hewitt &amp; Burbidge (1991) Optical Catalog of Extragalactic Emission-Line Objects Similar to Quasi-Stellar Objects. It contains a total of 935 galaxies which have optical properties similar to QSOs. Most of the objects appear to be nonstellar. The majority, more than 700, have redshifts z that are &lt;= 0.2, and most have been classified as Seyfert galaxies, N systems, or radio galaxies. The redshift distribution peaks at z ~ 0.025, but there are about 200 powerful radio galaxies in the extended tail of the distribution which have z &gt; 0.2. There is a separate and distinct peak in the redshift distribution at z = 0.06. Notice that this catalog does not include star-like objects with emission-line redshifts &gt;= 0.1 (these can be found in the HEASARC QSO database which contains the Revised and Updated Catalog of Quasi-Stellar Objects&quot; of Hewitt, A. and Burbidge, G. 1993, ApJS, Vol. 87, pp. 451-947). Neither does it contain LINERs (sometimes called Seyfert 3 galaxies) or starburst galaxies. This database was created by the HEASARC in February 2001 based on CDS/ADC Catalog VII/178 (table1.dat). This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P MIRO 4 PRL V2.0

This data set contains Spectroscopic and Continuum level 4 data, in the form of table files, taken during the ROSETTA PRELANDING phase of the Rosetta mission to comet 67P/CHURYUMOV-GERASIMENKO by the MIRO instrument. The major updates with this version (V2.0) are the addition of a Level 4 continuum data product and the elimination of separate geometry files for the spectroscopic data.

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Organization: National Aeronautics and Space Administration
CfA Redshift Survey: South Galactic Cap Data

The Center for Astrophysics (CfA) Redshift Survey South Galactic Cap (CFA2S) Catalog contains redshifts for a sample of about 4300 galaxies with blue (Zwicky B(0) type) magnitude &lt;= 15.5 covering the range from 20 h to 4h in right ascension and from -2.5 deg to 90 deg in declination. This sample is complete for all galaxies in the merge of the Zwicky et al. and Nilson catalogs in the south Galactic cap. Redshifts for 2964 of these were measured as part of the second CfA Redshift Survey. The data reveal large voids in the foreground and background of the Perseus-Pisces Supercluster. The largest of these voids lies at a mean velocity ~ 8000km/s, has diameter of ~ 5000km/s, and is enclosed by a complex of dense structures. The large structure known as the Perseus-Pisces Supercluster forms the near side of this complex. On the far side of this large void, at a mean velocity of ~ 12000km/s, there is another coherent dense wall. The structures in this survey support the view that galaxies generally lie on surfaces surrounding or nearly surrounding low-density regions or voids. This table was created by the HEASARC in March 2005 based on CDS table J/ApJS/121/287/cfa2s.dat.gz This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
NEW HORIZONS REX POST-LAUNCH CHECKOUT RAW V2.0

This data set contains Raw data taken by the New Horizons Radio Science Experiment instrument during the post-launch checkout mission phase. This is VERSION 2.0 of this data set. The REX datasets over the mission include calibrations using known radio sources, Jupiter, and cold sky measurements; operational readiness tests (ORTs); internal test pattern calibration; and prime science radiometry and occultation observations during the Pluto Encounter.

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Organization: National Aeronautics and Space Administration
DEEP2 Galaxy Redshift Survey Fields Chandra Point Source Catalog

This table contains the X-ray point-source catalog produced from the Chandra Advanced CCD Imaging Spectrometer (ACIS-I) observations of the combined ~3.2 deg&lt;sup&gt;2&lt;/sup&gt; DEEP2 (XDEEP2) survey fields, which consist of four ~ 0.7 - 1.1 deg&lt;sup&gt;2&lt;/sup&gt; fields. The combined total exposures across all four XDEEP2 fields range from ~ 10 ks to 1.1 Ms. The authors detect X-ray point sources in both the individual ACIS-I observations and the overlapping regions in the merged (stacked) images. They find a total of 2976 unique X-ray sources within the survey area with an expected false-source contamination of ~ 30 sources (&lt;~ 1%). In their paper, the authors present the combined log N-log S distribution of sources detected across the XDEEP2 survey fields and find good agreement with the Extended Chandra Deep Field and Chandra-COSMOS fields to f_(X,0.5-2keV)_ ~ 2 x 10&lt;sup&gt;-16&lt;/sup&gt; erg cm&lt;sup&gt;-1&lt;/sup&gt; s&lt;sup&gt;-1&lt;/sup&gt;. Given the large survey area of XDEEP2, they additionally place relatively strong constraints on the log N-log S distribution at high fluxes (f_(X,0.5-2keV) ~ 3 x 10&lt;sup&gt;-14&lt;/sup&gt; erg cm&lt;sup&gt;-1&lt;/sup&gt; s&lt;sup&gt;-1&lt;/sup&gt;), and find a small systematic offset (a factor ~ 1.5) toward lower source numbers in this regime, when compared to smaller area surveys. The number counts observed in XDEEP2 are in close agreement with those predicted by X-ray background synthesis models. Additionally, the authors present a Bayesian-style method for associating the X-ray sources with optical photometric counterparts in the DEEP2 catalog (complete to R&lt;sub&gt;AB&lt;/sub&gt; &lt; 25.2) and find that 2126 (~ 71.4% +/- 2.8%) of the 2976 X-ray sources presented here have a secure optical counterpart with a &lt;~ 6% contamination fraction. The present table provides the DEEP2 optical source properties (e.g., magnitude, redshift) as part of the X-ray-optical counterpart catalog. This table was created by the HEASARC in October 2012 based on electronic versions of Tables 5 and 7 from the reference paper which were obtained from the ApJS web site. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
ICE PLASMA WAVE ELECTRIC FIELD MEASUREMENT DATA

The Plasma Wave Data were submitted to National Space Science Data Center after the Principal Investigator's death (Scarf) by S. Chang of TRW. For the electric field data, the time interval submitted was Sept 9 - 14, 1985 was included. That information, as well as an explanation of the reformatted data is detailed.

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Organization: National Aeronautics and Space Administration
Einstein HRI Photon Event Data

The HRIPHOT database contains information from the High Resolution Imager aboard HEAO-2, the Einstein Observatory, in Event List Format. Einstein incorporated a high-resolution X-ray telescope and a focal plane assembly capable of positioning at its focus one of four instruments: a high- resolution imaging detector (HRI), a broader-field imaging proportional counter (IPC), a solid state spectrometer (SSS), and a Bragg crystal spectrometer (FPCS). Einstein (HEAO-2) was launched on November 13, 1978, and operated successfully until April 1981. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCICA 3 PRL CALIB V1.0

This dataset contains CALIBRATED DATA from the RPCICA instrument onmission ROSETTA during the prelanding phase. Data containsmeasurements of an undisturbed solar wind until Rosetta was closeenough to the comet to obtain measurements of the solar windinteraction with the atmosphere of target comet 67P.

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Organization: National Aeronautics and Space Administration
IRAS Point Source Catalog

This is a catalog of 245,889 well-confirmed point sources, i.e., sources with angular extents less than approximately 0.5', 0.5', 1.0', and 2.0' in the in-scan direction at 12, 25, 60, and 100 µm, respectively. Positions, flux densities, uncertainties, associations with known astronomical objects and various cautionary flags are given for each object. While two other complementary data sets - the Working Survey Database and the Point Source Reject Catalog - give information about point-like sources, the information available in the Point Source Catalog should satisfy almost all users. Away from confused regions of the sky, the survey is complete to about 0.4, 0.5, 0.6, and 1.0 Jy at 12, 25, 60, and 100 µm (cf. Faint Source Catalog). Typical position uncertainties are about 2" to 6" in-scan and about 8" to 16" cross-scan. The processing steps applied to detect and confirm point sources, and the positional and photometric error analyses are described in the Explanatory Supplement. The sources appear in order of increasing (1950.0) right ascension.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 1056 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 3 phase 2015-07-01 to 2015-10-21. It is a Global Gravity measurement at the comet 67P and covers the time 2015-09-25T03:07:15.000 to 2015-09-25T09:27:57.000.

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Organization: National Aeronautics and Space Administration