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opencc-by-4.0Feb 2023View details →

Microseism-catalog-2009-2019

Microseism-catalog-2009-2019

opennotspecifiedSep 2023View details →

FIGURES 79–90. 79 in Catalog of the Chrysomelinae (Coleoptera: Chrysomelidae) deposited in the entomological collections of the Instituto Nacional de Pesquisas da Amazônia (INPA) and the Universidade Federal do Amazonas (UFAM), Manaus, Brazil, with an illustrated key for the genera occurring in Brazil (except Aeneolucentia,

FIGURES 79–90. 79, holotype of Platyphora imperialis, labels; 80–83, holotype of Platyphora excellens, 80, dorsal view, 81, ventral view, 82, lateral view, 83, labels; 84, Platyphora olivenca, dorsal view; 85–88, syntype of Platyphora olivenca, 85, dorsal view, 86, ventral view, 87, abdominal sternites, 88, labels; 89, Platyphora olivenca, dorsal view; 90, Platyphora olivenca ab. evittata, dorsal view. Scale bar: 1 mm. Figs. 79–83 (Scale bar: 5 mm) photographed by Anna Jerve (© 2023 Naturhistoriska Riksmuseet). Original photos cropped and background removed. Made available by the Swedish Museum of Natural History under Creative Commons Attribution 4.0 International Public License, CC-BY 4.0, https://creativecommons.org/licenses/by/4.0/ legalcode. Figs. 85–88, 90 photographed by Christoph Germann (© 2023 Naturhistorisches Museum Basel). Original photos cropped and background removed.

opennotspecifiedSep 2023View details →

FIGURES 67–78. 67 in Catalog of the Chrysomelinae (Coleoptera: Chrysomelidae) deposited in the entomological collections of the Instituto Nacional de Pesquisas da Amazônia (INPA) and the Universidade Federal do Amazonas (UFAM), Manaus, Brazil, with an illustrated key for the genera occurring in Brazil (except Aeneolucentia,

FIGURES 67–78. 67, Platyphora alvarengai, dorsal view; 68, Platyphora angulata, dorsal view; 69, Platyphora arcuata, dorsal view; 70, Platyphora batesei, dorsal view; 71, Platyphora cinctella, dorsal view; 72, Platyphora concentrica, dorsal view; 73, Platyphora dejeanii, dorsal view; 74, Platyphora gratiosa, dorsal view; 75, Platyphora imperialis, dorsal view; 76–78, holotype of Platyphora imperialis, 76, dorsal view, 77, ventral view, 78, lateral view. Scale bar: 1 mm. Figs. 76–78 (Scale bar: 3 mm) photographed by Anna Jerve (© 2023 Naturhistoriska Riksmuseet). Original photos cropped and background removed. Made available by the Swedish Museum of Natural History under Creative Commons Attribution 4.0 International Public License, CCBY 4.0, https://creativecommons.org/licenses/by/4.0/legalcode.

FIGURE 1 in An annotated catalog of the type material of Mecoptera deposited in the Florida State Collection of Arthropods in Gainesville, Florida, USA

FIGURE 1. Dorsal habitus and labels of holotype of Panorpa appalachia Byers, 2002. Scale bar = 5 mm.

FIGURES 161b–164a in An annotated and illustrated catalog of the primary type material of Hemiptera deposited in the Florida State Collection of Arthropods

FIGURES 161b–164a. Front and back of syntype slides of 161b). Lindingaspis floridana Ferris, 1942; Ventral view of 162a). Lindingaspis floridana Ferris, 1942; Front and back of syntype slides of 162b). Lindingaspis floridana Ferris, 1942; Ventral view of 163a). Lindingaspis floridana Ferris, 1942; Front and back of syntype slides of 163b). Lindingaspis floridana Ferris, 1942; Ventral view of 164a). Lindingaspis floridana Ferris, 1942. Scale bars 162a, 163a & 164a = 0.5 mm, scale bars 161b, 162b & 163b = 1 cm.

FIGURES 16–18 in An annotated and illustrated catalog of the primary type material of Hemiptera deposited in the Florida State Collection of Arthropods

FIGURES 16–18. Dorsal habitus and labels of holotypes of 16). Carineta seriemaculata Sanborn, 2020; 17). Carineta trinidadensis Sanborn, 2020; 18). Cicadetta ramosi Sanborn, 2009. Scale bars = 5 mm.

FIGURES 167b–169a in An annotated and illustrated catalog of the primary type material of Hemiptera deposited in the Florida State Collection of Arthropods

FIGURES 167b–169a. Ventral view of 167b). Palinaspis quohogiformis (Merrill, 1923); Front and back of syntype slides of 167c). Palinaspis quohogiformis (Merrill, 1923); Ventral view of 168a). Palinaspis quohogiformis (Merrill, 1923); Ventral view of 168b). Palinaspis quohogiformis (Merrill, 1923); Front and back of syntype slides of 168c). Palinaspis quohogiformis (Merrill, 1923); Ventral view of 169a). Praecocaspis diversa Ferris, 1942. Scale bars 167b, 168a, 168b & 169a = 0.1 mm, Scale bars 167c & 168c = 1 cm.

publicSep 2016View details →

dryad20/100

Supplemental BOSS Emission Line Catalog

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Einstein Catalog IPC EMSS Survey

This database table contains information from the Einstein Extended Medium Sensitivity Survey (EMSS) which consists of 835 serendipitous X-ray sources detected at or above 4 times the rms level in 1435 IPC fields with their centers located away from the galactic plane. Their limiting sensitivities range from ~5*10E-14 to ~3*10-12 ergs cm-3 s-1 in the 0.3-3.5keV band. A total area of 778 square degrees of the high galactic latitude sky (|b|>20) has been covered. The analysis has been performed using data from the Rev 1 processing system at the CfA. The resulting EMSS catalog is a flux-limited and homogeneous sample of astronomical objects that can be used for statistical studies. Additional information is available from the HEASARC. This is a service provided by NASA HEASARC .

Herschel SPIRE Point Source Catalog: 250 microns

The Herschel-SPIRE instrument mapped about 9% of the sky in Submillimeter broad-band filters centered at 250, 350, and 500 microns (1199, 857, 600 GHz) with spatial resolutions of 17.9", 24.2", 35.4" respectively. In total, we used the 6878 standard configuration scan maps that are available, including calibration observations. The SPIRE Point Source Catalog contains the result of a systematic and homogeneous source extraction on those maps using 4 different photometry extraction methods. Only regions affected by strong Galactic emission, mostly in the Galactic Plane, were excluded, as they tested the limits of the available source extraction methods. Aimed primarily at point sources, that allow for the best photometric accuracy, the catalog contains also significant fractions of slightly extended sources up to a limit. With most SPIRE maps being confusion limited, uncertainties in flux densities were established as a function of structure noise and flux density, based on the results of artificial source insertion experiments into real data along a range of celestial backgrounds. Many sources have been rejected that do not pass the imposed SNR threshold, especially at flux densities approaching the extragalactic confusion limit. A range of additional flags provide information on the reliability of the flux information, as well as the spatial extent and orientation of a source. Users are encouraged to check the flux density estimates of all 4 methods and follow the guidelines given in the Explanatory Supplement regarding their interpretation for point- and extended sources. For tracing back catalog objects to the originally contributing detections in SPIRE observations, a cross identification table is available that provides the relevant observation identifiers used by the Herschel Science Archive. For further details on catalog construction, detailed content, and validation, please see the Explanatory Supplement.

GOODS-S MIPS 24 micron Photometry Catalog

The Great Observatories Origins Deep Survey (GOODS) aims to unite extremely deep observations from NASA's Great Observatories (Spitzer, Hubble and Chandra), ESA's Herschel and XMM-Newton, and the most powerful ground-based facilities. The aim is to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. This catalog provides a list of sources for the MIPS 24 micron imaging of the GOODS-S field. It is limited to flux densities greater than 80 microJy, where the source extraction is highly complete and reliable.

LAT 2-year Point Source Catalog

The Fermi Gamma-ray Space Telescope (Fermi) Large Area Telescope (LAT) is a successor to EGRET, with greatly improved sensitivity, resolution, and energy range. This web page presents the second full catalog of LAT sources, based on the first 24 months of survey data. For a full explanation about the catalog and its construction see the LAT 2-year Catalog Paper (also available on arxiv).

Revised Luyten Half-Second (LHS) Catalog

The Revised Luyten Half-Second (LHS) Catalog contains refined coordinates and proper motion data for the high proper motion (HPM) stars listed in the Original Luyten Half-Second (LHS) catalog. The positional uncertainty in the Original LHS catalog is typically >10" and is often >30". The authors of the Revised LHS Catalog used the digital scans of the Palomar Observatory Sky Survey (POSS) I and POSS II plates to derive more accurate positions and proper motions for these objects. Out of the 4470 candidates in the LHS catalog, 4323 objects were manually re-identified in the POSS I and POSS II scans. A small fraction of the stars were not found due to the lack of finder charts and digitized POSS II scans. The uncertainties in the revised positions are typically ~2", but can be as high as ~8" in a few cases, which is a large improvement over the original data. Cross-correlation with the Tycho-2 and Hipparcos catalogs yielded 819 candidates (with red magnitude m_R <~12. For these brighter sources, the position and proper motion data were replaced with the more accurate Tycho/Hipparcos data. In total, there are revised proper motion measurements and coordinates for 4040 stars and revised coordinates for 4330 stars. This table was created by the HEASARC in October 2002 based on <a href="https://cdsarc.cds.unistra.fr/ftp/cats/I/279">CDS Catalog I/279</a> (the 24-May-2002 version of the file catalog.dat). This is a service provided by NASA HEASARC .

restrictednotspecifiedMar 2025View details →

Mercury Map Catalog

The Mercury Map Catalog includes various mappings of the surface of Mercury published by the U.S. Geological Survey from 1976 - 1990.

ChaMPlane Galactic Bulge and Center X-Ray Source Catalog

This table contains the Chandra Multiwavelength Plane (ChaMPlane) Survey catalog of X-ray point sources in the window and four Galactic bulge fields, specifically all source detections with net counts >= 1 in the 0.3-8 keV broad band. In the reference paper, the authors present the log N-log S and spatial distributions of X-ray point sources in seven Galactic bulge (GB) fields within 4 degrees of the Galactic center (GC). They compare the properties of 1159 X-ray point sources discovered in their deep (100 ks) Chandra observations of three low extinction Window fields near the GC with the X-ray sources in the other GB fields centered around Sgr B2, Sgr C, the Arches Cluster, and Sgr A* using Chandra archival data. To reduce the systematic errors induced by the uncertain X-ray spectra of the sources coupled with field-and-distance-dependent extinction, they classify the X-ray sources using quantile analysis and estimate their fluxes accordingly. The result indicates that the GB X-ray population is highly concentrated at the center, more heavily than the stellar distribution models. It extends out to more than 1.4 degrees from the GC, and the projected density follows an empirical radial relation inversely proportional to the offset from the GC. They also compare the total X-ray and infrared surface brightness using the Chandra and Spitzer observations of the regions. The radial distribution of the total infrared surface brightness from the 3.6-micron band images appears to resemble the radial distribution of the X-ray point sources better than that predicted by the stellar distribution models. Assuming a simple power-law model for the X-ray spectra, the closer to the GC, the intrinsically harder the X-ray spectra appear, but adding an iron emission line at 6.7 keV in the model allows the spectra of the GB X-ray sources to be largely consistent across the region. This implies that the majority of these GB X-ray sources can be of the same or similar type. Their X-ray luminosity and spectral properties support the idea that the most likely candidate is magnetic cataclysmic variables (CVs), primarily intermediate polars (IPs). Their observed number density is also consistent with the majority being IPs, provided the relative CV to star density in the GB is not smaller than the value in the local solar neighborhood. This table was created by the HEASARC in January 2010, based on the electronic version of Table 2 from the reference paper, which was obtained from the Astrophysical Journal web site. This is a service provided by NASA HEASARC .

Master X-Ray Catalog

The XRAY database table contains selected parameters from almost all HEASARC X-ray catalogs that have source positions located to better than a few arcminutes. The XRAY database table was created by copying all of the entries and common parameters from the tables listed in the Component Tables section. The XRAY database table has many entries but relatively few parameters; it provides users with general information about X-ray sources, obtained from a variety of catalogs. XRAY is especially suitable for cone searches and cross-correlations with other databases. Each entry in XRAY has a parameter called 'database_table' which indicates from which original database the entry was copied; users can browse that original table should they wish to examine all of the parameter fields for a particular entry. For some entries in XRAY, some of the parameter fields may be blank (or have zero values); this indicates that the original database table did not contain that particular parameter or that it had this same value there. The HEASARC in certain instances has included X-ray sources for which the quoted value for the specified band is an upper limit rather than a detection. The HEASARC recommends that the user should always check the original tables to get the complete information about the properties of the sources listed in the XRAY master source list. This master catalog is updated periodically whenever one of the component database tables is modified or a new component database table is added. This is a service provided by NASA HEASARC .

Optically-Selected QSOS NVSS-Detected Source Catalog

The authors used the 1.4-GHz NRAO VLA Sky Survey (NVSS) to study radio sources in two color-selected QSO samples: a volume-limited sample of 1,313 QSOs defined by Mi < -23 in the redshift range 0.2 < z < 0.45 and a magnitude-limited sample of 2,471 QSOs with mr <= 18.5 and 1.8 < z < 2.5. About 10% were detected above the 2.4-mJy NVSS catalog limit and are powered primarily by active galactic nuclei (AGNs). The space density, rho, of the low-redshift QSOs evolves as rho ~ (1 + z)6. In both redshift ranges, the flux-density distributions and luminosity functions of QSOs stronger than 2.4 mJy are power laws, with no features to suggest more than one kind of radio source. Extrapolating the power laws to lower luminosities predicts the remaining QSOs should be extremely radio quiet, but they are not. Most were detected statistically on the NVSS images with median peak flux densities Sp of ~ 0.3 mJy/beam and ~ 0.05 mJy/beam in the low- and high-redshift samples, corresponding to spectral luminosities log L1.4GHz ~ 22.7 and ~ 24.1 W/Hz, respectively. The authors suggest that the faint radio sources are powered by star formation at rates dM/dt of ~ 20 M_{sun}_/yr in the moderate luminosity (median Mi of ~ -23.4) low-redshift QSOs and dM/dt ~ 500Msun/yr in the very luminous (median Mi ~ -27.5) high-redshift QSOs. Such luminous starbursts (<log(LIR/Lsun)> ~ 11.2 and ~ 12.6, respectively) are consistent with "quasar mode" accretion in which cold gas flows fuel both AGN and starburst. The SDSS DR7 QSO catalog (Schneider et al. 2010, AJ, 139, 2360) is complete to i = 19.1 mag over a solid angle of 2.66 sr around the North Galactic Pole. It contains the small sample of 179 color-selected QSOs defined by Mi < -23 in the narrow redshift range 0.2 < z < 0.3 studied by Kimball et al. (2011, ApJ, 739, L29) and the larger sample of 1,313 QSOs in the wider redshift range 0.2 < z < 0.45 discussed here. Note that these magnitudes were calculated for an H0= 71 km/s/Mpc and OmegaM = 0.27 modern flat LambdaCDM cosmology. The entire SDSS DR7 area is covered by the NVSS, whose source catalog is complete for statistical purposes above a peak flux density Sp ~ 2.4 mJy/beam at 1.4 GHz. In the redshift range 0.2 < z < 0.45 the 45" FWHM (full width between half-maximum points) beam of the NVSS spans 150 - 250 kpc. There are 163 (12%) NVSS detections of the 1,313 QSOs in the redshift range 0.2 < z < 0.45 which are listed in Table 1 of the reference paper. The authors also chose a magnitude-limited sample of all 2,471 color-selected DR7 QSOs brighter than mr = 18.5 in the redshift range 1.8 < z < 2.5. The NVSS detected radio emission stronger than S = 2.4 mJy from only 191 (8%) of them: these are listed in Table 3 of the reference paper. This HEASARC table contains the contents of both samples described above. It thus has 163 + 191 = 354 entries, the sum of Tables 1 and 3 from the reference paper. To select only the entries from Table 1, the user should select entries with redshifts from 0.2 to 0.45. To select only the entries from Table 3, the user should select entries with redshifts > 1.8. This table was created by the HEASARC in January 2015 based on <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/ApJ/768/37">CDS Catalog J/ApJ/768/37</a> files table1.dat and table3.dat. This is a service provided by NASA HEASARC .

SHELA Epoch 3 IRAC Catalog

The Spitzer/HETDEX Exploratory Large-Area (SHELA) survey covers ~24 sq. deg at 3.6 and 4.5 microns. The survey area falls within the footprints of the Sloan Digital Sky Survey "Stripe 82" region, the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), and the Dark Energy Survey. The images and catalogs are 80% (50%) complete to limiting magnitudes of 22.0 (22.6) AB mag in the detection image, which is constructed from the weighted sum of the IRAC 3.6 and 4.5 micron images. The catalogs reach limiting sensitivities of 1.1 microJy at both 3.6 and 4.5 microns (1#, for R = 2" circular apertures).

Spitzer Deep Wide-Field Survey Light Curve Catalog

The Spitzer Deep, Wide-Field Survey (SDWFS) is a four-epoch infrared survey of 10 square degrees in the Boötes field of the NOAO Deep Wide-Field Survey using the IRAC instrument on the Spitzer Space Telescope. SDWFS, a Spitzer Cycle 4 Legacy project, occupies a unique position in the area-depth survey space defined by other Spitzer surveys. The four epochs that make up SDWFS permit - for the first time - the selection of infrared-variable and high proper motion objects over a wide field on timescales of years. Because of its large survey volume, SDWFS is sensitive to galaxies out to z ~ 3 with relatively little impact from cosmic variance for all but the richest systems. The SDWFS data sets will thus be especially useful for characterizing galaxy evolution beyond z ~ 1.5.The SDWFS Light Curve Catalog presents the 3.6 and 4.5 micron magnitudes for each SDWFS source in each of the four epochs. For more details see Kozlowski et al. (2010).

Spitzer Extragalactic First Look Survey MIPS 70 micron 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.