AndreaBozzo/ceres-open-data-index huggingface dataset:
CGRO/COMPTEL Low-Level Data and Maps

COMPTEL is both the name of the Imaging Compton Telescope on the Compton Gamma Ray Observatory (CGRO) and the name of this HEASARC database table which allows the user to select low-level data and maps produced by this instrument. Much more information on the COMPTEL instrument, data products, and data analysis techniques can be obtained from the Compton Observatory Science Support Center (COSSC) web site at &lt;pre&gt; &lt;a href="https://heasarc.gsfc.nasa.gov/docs/cgro/"&gt;https://heasarc.gsfc.nasa.gov/docs/cgro/&lt;/a&gt; &lt;/pre&gt; and from the article in Legacy No. 7 on the HEASARC CGRO Data Archive &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; Interactions in COMPTEL occur in a two stage process: First, a Compton collision occurs in one of seven (low-Z) liquid scintillators and is usually then completely absorbed in one of fourteen (high-Z) NaI(Tl) scintillators. The unusual aspect of this detector is that the location of the gamma-ray on the sky is given by an annulus and not a point. The correlation of many events enables the localization of point sources or the creation of sky maps. Time-of-flight measurements, pulse shape discrimination and anti-coincidence shields are used to reject background events. COMPTEL has a wide field of view (about 1 steradian, equivalent to a FWHM of about 40 degrees), an angular resolution under optimal conditions of about 1 degree, and an energy resolution that ranges from 5-10% at 1 MeV. During Phase 1 of the CGRO mission, COMPTEL completed the first all-sky survey in the energy range of 0.75-30 MeV (in four energy bands). In addition, COMPTEL can measure energy spectra of solar flares or bright cosmic gamma-ray bursts between 0.1-10 MeV, and neutrons from solar flares. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
2MASS Calibration Point Source Working Database

Photometric calibration for 2MASS was performed using observations of calibration fields made at regular intervals during each night of survey operations. Measurements of standard stars in the fields were used to derive the photometric zero point offsets as a function of time during each night. Atmospheric extinction coefficients were derived from 2MASS observations made over long periods.\n\n2MASS calibration fields, or tiles, are 1° long in declination and approximately 8.5' wide in right ascension. There are 35 regular survey calibration fields distributed at approximately two hour intervals in right ascension near declinations of approximately -30°, 0° and +30°. An additional five calibration fields were defined in and around the Large and Small Magellanic Clouds to support the deep observation (6x) campaign towards the end of survey operations.\n\nOver the course of the survey, the regular calibration fields were scanned between 562 and 3692 times in nominally photometric conditions. Equatorial fields were observed from both observatories, so were observed more frequently than those near ±30° which were observed with only one telescope. The special Magellanic Cloud calibration fields were observed 108 to 468 times between November 2000 and February 2001.\n\nCalibration scan Atlas Images, and Point and Extended Source Working Databases (Cal-PSWDB and Cal-XSWDB), analogous to those from the main survey, were produced from the calibration scan pipeline data reduction. The calibration Image Atlas and WDBs are the fundamental processing archives of the data from 73,230 calibration scans taken in photometric conditions during 2MASS survey operations. The Cal-WDBs contain positions, magnitudes and characteristics of 191,464,020 and 403,811 point and extended "source" extractions, respectively. The calibration Image Atlas contains 878,769 FITS images in the three survey bandpasses redundantly covering ~5 deg2 of sky. Unlike the main survey and 6x observations, "Catalogs" have not been derived from the Calibration WDBs.

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Organization: National Aeronautics and Space Administration
Single cell transcriptional profiling of femur bone marrow from mice flown on Rodent Research Reference Mission-2 (RRRM-2)

In the Rodent Research Reference Mission (RRRM-2), forty female C57BL/6NTac mice were flown on the International Space Station. To assess differences in outcomes due to age, twenty 12 week-old and twenty 29 week-old mice were flown, respectively. To directly assess spaceflight effects, half of the young and old mice (10 old, 10 young) were sacrificed on-orbit after 55-58 days (ISS Terminal, ISS-T), while the other half (10 old, 10 young) were returned live to Earth after 32 days and allowed to recover for 24 days (Live Animal Return, LAR) before sacrifice. ISS-T and LAR mice were the same age at sacrifice. Both the ISS-T and LAR animals had independent ground controls (10 mice per group housed in flight hardware in matched environmental conditions), basal controls (10 mice per group sacrificed 2 days before launch), and vivarium controls (10 mice per group housed within standard vivarium habitats). Thus RRRM-2 included a total of 160 mice. This study includes single cell transcriptional profiling data from femur bone marrow from 4 young LAR flight animals, 4 old LAR flight animals, 4 young LAR ground control animals, and 4 old LAR ground control animals.

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Organization: National Aeronautics and Space Administration
SpaceX Inspiration4 Stool Metagenome Profiling

The SpaceX Inspiration4 mission was a 3-day mission with four private astronauts to low Earth orbit that occurred in September 2021. The crew collected biospecimen samples before, during, and after flight. One of these biospecimen collections included stool collected in OMNIgene•GUT tubes (DNA Genotek, OMR-200). Samples were collected pre-flight (L-92, L-44) and post-flight (R+45, R+82). This study hosts stool data. Additional skin, oral and nasal metagenome data is deposited in OSD-572. Dragon capsule data metagenome is deposited in OSD-573. Skin biopsy-site metagenome data is deposited in OSD-574.

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Organization: National Aeronautics and Space Administration
LMC X-Ray Discrete Sources

This database table contains 105 &quot;discrete&quot; (i.e., more compact than 1.25 arcminutes) and 9 &quot;large-diameter&quot; (detected using a detection circle radius of 2 arcminutes) Einstein IPC X-ray sources in the direction of the Large Magellanic Cloud (LMC) that are tabulated in Tables 2 and 4, respectively, of Wang et al. (1991, ApJ, 374, 475). For full details of the data processing and selection used to create this source catalog, the above reference should be consulted. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
NEW HORIZONS  MVIC PLUTO ENCOUNTER  CALIBRATED V3.0

This data set contains Calibrated data taken by the New Horizons  Multispectral Visible Imaging Camera  instrument during the  Pluto encounter  mission phase. This is VERSION 3.0 of this data set.   This data set contains MVIC observations taken during the  the Approach (Jan-Jul, 2015), Encounter, Departure, and  Transition mission sub-phases, including flyby observations  taken on 14 July, 2015, and departure and calibration data  through late October, 2016. This data set completes the  Pluto mission phase deliveries for MVIC.   This is version 3.0 of this dataset. Changes since version 2.0 include  the addition of data downlinked between the end of January, 2016 and the end of October, 2016, completing the delivery of all data covering the  Pluto Encounter and subsequent Calibration Campaign. It includes multi-  map observations from the Approach phase, observations of the moons, hi- res, full-frame observations from Pluto Encounter and Departure, and  ring search observations. There may be some overlap between prior  datasets and this dataset, due to only partial, windowed, or lossy data  in prior datasets. This dataset also includes functional tests from the Calibration Campaign, including calibration observations of the M6 and  M7 clusters, and HD205905.   Also, updates were made to the calibration files, documentation, and  catalog files.   For any data previously delivered as sub-frame windows, this delivery  will fill in the image data outside those windows.   Changes to the calibration involved only changes to the  spectrum-specific calibration constants provided in FITS headers and  in PDS labels; the calibrated Data Number values in the calibrated  data set, excluding image data outside the sub-frame windows  mentioned above, will not be substantively changed.

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Organization: National Aeronautics and Space Administration
Transcriptional profiling of roots and shoots from Brachypodium distachyon seedlings flown on the ISS

Most major cereal grain crops are monocots. Yet, most investigations of plant adaptation to the spaceflight environment have been carried out on the dicotyledonous model plant, Arabidopsis thaliana. It remains unknown whether the conclusions from such studies can be extrapolated to monocotyledonous plants. To fill this knowledge gap, seedlings of three different accessions of Brachypodium distachyon (Bd21, Bd21-3, and Gaz8), a model for temperate grasses including cereal crops, were grown on the International Space Station in the Veggie hardware and on the ground in matched conditions. To synchronize germination, seedlings were grown for 24 hours in red light. Then, seedlings were grown with green/blue/red light using a 24 hour photo period for 4 additional days. At this point, seedlings were harvested and placed in room temperature RNAlater for 24 hours before being moved to -80 C for storage and later dissection into roots and shoots. This dataset features ribodepleted RNA-seq data from the Bd21, Bd21-3 and Gaz8 accessions.

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Organization: National Aeronautics and Space Administration
Herschel GOODS-N Catalog

GOODS-Herschel (Elbaz et al, 2011) is in ESA open time key project consisting of the deepest Herschel observations of the two Great Observatories Origins Deep Survey (GOODS) fields in the Northern and Southern hemispheres.\n\nThe GOODS catalogs include photometry from Spitzer IRAC & MIPS and Herschel PACS & SPIRE observations.

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Organization: National Aeronautics and Space Administration
9C 15-GHz Ryle Telescope Survey of VSA Fields Source Catalog

The fields chosen for the first observations of the cosmic microwave background (CMB) with the Very Small Array (VSA) have been surveyed with the Ryle Telescope at 15 GHz. The authors have covered three regions around RA = 00&lt;sup&gt;h&lt;/sup&gt;20&lt;sup&gt;m&lt;/sup&gt; and Dec = +30&lt;sup&gt;o&lt;/sup&gt;, RA = 09&lt;sup&gt;h&lt;/sup&gt;40m and Dec = +32&lt;sup&gt;o&lt;/sup&gt; and RA = 15&lt;sup&gt;h&lt;/sup&gt;40&lt;sup&gt;m&lt;/sup&gt; and Dec = +43&lt;sup&gt;o&lt;/sup&gt; (J2000.0), comprising an area of 520 deg&lt;sup&gt;2&lt;/sup&gt;. There are 465 sources in this entire area which are above the estimated completeness limit of ~ 25 mJy, although a total of ~ 760 sources were detected, some as faint as 10 mJy. The prime motivation of this study was to define a catalog of the foreground sources that must be monitored by the VSA during its observations at 34 GHz. In particular, it provides a means of identifying GigaHertz peaked spectrum (GPS) sources, which are important for the study of radio source evolution, as well as being a significant foreground for CMB observations over a range of wavelengths. Since this will be a new and quite extensive survey, it was desgignated as &#39;9C&#39; or the Ninth Cambridge survey. For the purpose of this particular component of the 9C survey, the authors designated as a subset, 3 circular areas, VSA1, VSA2 and VSA3, defined by the properties listed in Table 2 of the reference paper and reproduced below: &lt;pre&gt; Field Centre J2000.0 Center B1950.0 Radius Area RA Dec RA Dec (degrees) (sq. degrees) VSA1 00 17 36.5 +30 16 39 00 15 00.0 +30 00 00 5.5 95.0 VSA2 09 40 57.7 +31 46 21 09 38 00.0 +32 00 00 6.0 113.0 VSA3 15 36 42.7 +43 20 11 15 35 00.0 +43 30 00 5.0 78.5 &lt;/pre&gt; There are 242 sources which were both above the 25 mJy completeness limit and were in the 286.5 deg&lt;sup&gt;2&lt;/sup&gt; contained within these 3 circular fields. These source were listed in 3 tables in the reference paper, Table 4 (VSA1), Table 5 (VSA2) and Table 6 (VSA3). These have been combined into this one HEASARC table, in which the HEASARC added a new parameter vsa_field, which is set to 1 for the VSA1 sources, 2 for the VSA2 sources, and 3 for the VSA3 sources. This table was created in November 2010 based on &lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/MNRAS/342/915"&gt;CDS catalog J/MNRAS/342/915&lt;/a&gt; files table4.dat, table5.dat and table6.dat. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
NEW HORIZONS  LORRI JUPITER ENCOUNTER  RAW V3.0

This data set contains Raw data taken by the New Horizons  Long Range Reconnaissance Imager  instrument during the  Jupiter encounter  mission phase. This is VERSION 3.0 of this data set.   LORRI science observations for the Jupiter Phase include  observations of the Jovian system: the Jovian atmosphere and  clouds including full disk rotation movie and resolved images of  selected features like the Great Red Spot and the Little Red Spot;  Jovian ring system and associated small satellites; the Galilean  satellites with particular attention to Io under both sunlit and  eclipse conditions, and eclipse observations of both Europa and  Ganymede; the small irregular satellites Elara, Himalia,  Callirrhoe. Additional observations were taken to test and/or  characterize and/or calibrate the modes and performance of the  LORRI.   LORRI V3.0 provides a few updates from LORRI V2.0. The lossy images  were recalibrated, including expanding the 'bad' pixel designation  of 8x8 boxes affected by the first 34 pixels of header information  in the calibrated quality map. Also, updates were made to the  documentation and catalog files, primarily to resolve liens from the  V2.0 peer review. No new observations were added with Version 3.0

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Organization: National Aeronautics and Space Administration
EPOXI EARTH OBS - HRII CALIBRATED SPECTRA V2.0

This dataset contains calibrated, 1.05- to 4.8-micron spectra of Earth acquired by the High Resolution Infrared Spectrometer (HRII) during the EPOCh and Cruise 2 phases of the EPOXI mission. Five sets of observations were acquired on 18-19 March, 28-29 May and 04-05 June 2008 and on 27-28 March and 04-05 October 2009 to characterize Earth as an analog for extrasolar planets. Each observing period lasted approximately 24 hours, and spectra were acquired twice every 2 hours. During the observing period in May 2008, the Moon transited across Earth as seen from the spacecraft. HRII spectra were not acquired during the first attempt of an Earth south polar observation on 27-28 September 2009 because fault protection turned that instrument off; the full sequence was successfully rerun on 04-05 October 2009. Version 2 corrects an error in the IR absolute calibration that previously inflated all spectra by a factor of 2.

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Organization: National Aeronautics and Space Administration
ABI/GOES-17 Dark Target Aerosol 10-Min L2 Full Disk 10 km

The ABI/GOES-17 Dark Target Aerosol 10-Min L2 Full Disk 10 km product, short-name XAERDT_L2_ABI_G17 is provided at 10-km spatial resolution (at-nadir) and a 10-minute full-disk cadence that typically yields about 144 granules over the daylit hours of a 24-hour period. The Geostationary Operational Environmental Satellite – GOES-17 served in the operational GOES-West position (near -137°W), from February 12, 2019, through January 4, 2023. The GOES-16/ABI collection record spans from January 2019 through December 2022. The XAERDT_L2_ABI_G17 product is a part of the Geostationary Earth Orbit (GEO)–Low-Earth Orbit (LEO) Dark Target Aerosol project under NASA’s Making Earth System Data Records for Use in Research Environments (MEaSUREs) program, led by Robert Levy, uses a special version of the MODIS Dark Target (DT) aerosol retrieval algorithm to produce Aerosol Optical Depth (AOD) and other aerosol parameters derived independently from seven sensor/platform combinations, where 3 are in GEO and 4 are in LEO. The 3 GEO sensors include Advanced Baseline Imagers (ABI) on both GOES-16 (GOES-East) and GOES-17 (GOES-West), and Advanced Himawari Imager (AHI) on Himawari-8. The 4 LEO sensors include MODIS on both Terra and Aqua, and VIIRS on both Suomi-NPP and NOAA-20. Adding the LEO sensors reinforces a major goal of this project, which is to render a consistent science maturity level across DT aerosol products derived from both types and sources of orbital satellites. The XAERDT_L2_ABI_G17 product, in netCDF4 format, contains 45 Science Data Set (SDS) layers that include 8 geolocation and 37 geophysical SDSs. For more information consult LAADS product description page at: https://ladsweb.modaps.eosdis.nasa.gov/missions-and-measurements/products/XAERDT_L2_ABI_G17 Or, Dark Target aerosol team Page at: https://darktarget.gsfc.nasa.gov/

Tags: earth-science-aerosols-atmosphere, earth-science-aerosols-atmosphere-aerosol-optical-depth-thickness, earth-science-aerosols-atmosphere-aerosol-optical-depth-thickness-angstrom-exponent, earth-science-aerosols-atmosphere-aerosol-particle-properties
Organization: National Aeronautics and Space Administration
Transcriptional profiling of livers from mice flown on Rodent Research Reference Mission-1 (RRRM-1)

In the Rodent Research Reference Mission (RRRM-1), forty female BALB/cAnNTac mice were flown on the International Space Station. To assess differences in outcomes due to age, twenty 10-12 week-old and twenty 32 week-old mice were flown, respectively. To directly assess spaceflight effects, half of the young and old mice (10 old, 10 young) were sacrificed on-orbit after 22-23 days (ISS Terminal, ISS-T), while the other half (10 old, 10 young) were returned live to Earth after 40 days and allowed to recover for 2 days (Live Animal Return, LAR) before sacrifice. Both the ISS-T and LAR animals had independent ground controls (10 mice housed in flight hardware in matched environmental conditions), basal controls (10 mice sacrificed 1 day after launch), and vivarium controls (10 mice housed within standard vivarium habitats). Thus RRRM-1 included a total of 160 mice. This datasets features ribodepleted total RNA-seq data from livers dissected from all groups in RRRM-1. Data from 7-10 livers per group are included. All samples include either Mix 1 or Mix 2 of the ERCC spike-in control.

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Organization: National Aeronautics and Space Administration
Einstein Catalog IPC Deep Survey

IPCDEEP is created from a table containing basic source parameters for each of the 178 IPC sources detected by the Einstein Deep Survey. The Einstein Deep Survey program (EDS) consists of very deep X-ray exposures in selected regions of the sky at high galactic latitude. The main purposes of the survey are to investigate the nature of the extragalactic X-ray background through direct source counts at very low flux levels and to study the nature of the very faint X-ray sources which comprise a significant fraction, if not all, of the soft X-ray background. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration
Near Infrared Camera and Multi Object Spectrograph

The HST Near Infrared Camera and Multi-Object Spectrometer (NICMOS)         provides imaging capabilities in broad, medium, and narrow band         filters, broad-band imaging polarimetry, coronographic imaging, and         slitless grism spectroscopy, in the wavelength range 0.8-2.5 microns.         NICMOS has three adjacent but not contiguous cameras, designed to         operate independently, each with a dedicated array at a different         magnification scale.

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Organization: National Aeronautics and Space Administration
Comprehensive multi-omics analysis reveals mitochondrial stress as a central biological hub for spaceflight impact

Given the limited knowledge of the biological impact of spaceflight, a multi-omics, systems biology approach was used to investigate NASA’s GeneLab data and astronaut biomedical profiles. These data consist of hundreds of samples flown in space, human metrics from 59 astronauts, and confirmatory data from NASA’s Twin Study, analyzed together for consistent transcriptomic, proteomic, metabolomic, and epigenetic response to spaceflight. Pathway analysis showed significant enrichment of mitochondrial activity and innate immunity. Muscle and liver tissues showed that chronic inflammation, may be a response to mitochondrial dysfunction. Additional pathways altered in spaceflight included cell cycle, circadian rhythm, and olfactory activity pathways, all of which are known to have interactions with mitochondrial activity. Evidence of altered mitochondrial function was also found in the urine and blood metabolic data compiled from the astronaut cohort and NASA Twin Study data, all of which indicate mitochondrial stress as a consistent phenotype of spaceflight.

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Organization: National Aeronautics and Space Administration
HerMES 350 micron StarFinder Catalog

The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme (KPGT_soliver1) designed to map a set of nested fields totalling 380 sq. deg. Fields range in size from 0.01 to 20 sq. deg., using SPIRE at 250, 350 and 500 microns. These bands cover the peak of the redshifted thermal spectral energy distribution from interstellar dust and thus capture the reprocessed optical and ultraviolet radiation from star formation that has been absorbed by dust, and are critical for forming a complete multiwavelength understanding of galaxy formation and evolution.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 4 1183 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 4 phase 2015-10-22 to 2015-12-31. It is a Global Gravity measurement at the comet 67P and covers the time 2015-11-15T10:28:25.000 to 2015-11-15T16:53:20.000.

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Organization: National Aeronautics and Space Administration
Palomar/MSU Nearby Star Survey

The Palomar/Michigan State University Catalogue contains basic data for 1971 stars confirmed by the authors to be late K or M main-sequence stars with absolute visual magnitudes of 8.0 or fainter taken from Tables 1A of papers I and II and Table 1D of paper I. Note that known degenerates have been excluded from this sample. All but 6 of these these star were selected from the Catalogue of Nearby Stars (Gliese &amp; Jahreiss, &quot;Preliminary Version of the Third Catalogue of Nearby Stars&quot;, CNS3), and most (88%) lie within 25 parsecs. This online catalog was created by the HEASARC in July 1999 based on tables obtained from the ADC/CDS data centers. This is a service provided by NASA HEASARC .

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Organization: National Aeronautics and Space Administration