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83 results for “HERMES”
Figure 61 from: Grishin N, Cong Q (2014) A new Hermeuptychia (Lepidoptera, Nymphalidae, Satyrinae) is sympatric and synchronic with H. sosybius in southeast US coastal plains, while another new Hermeuptychia species – not hermes – inhabits south Texas and northeast Mexico. ZooKeys 379: 43-91. https://doi.org/10.3897/zookeys.379.6394
Figure 61 - Dorsoposterior view of male abdomens of Hermeuptychia from USA: Texas. a Hermeuptychia intricata, DNA voucher NVG-1548 (mirror image, i.e. left-right inverted) b Hermeuptychia hermybius, DNA voucher NVG-1635 (also shown in Fig. 62j, specimen Fig. 52) c Hermeuptychia sosybius, DNA voucher NVG-1553. Data in Table 1. Scales are brushed off the abdomen tip to expose distal parts of genitalia. The easiest to observe character (the shape of the distal end of uncus) is indicated.
Figures 1-9 from: Grishin N, Cong Q (2014) A new Hermeuptychia (Lepidoptera, Nymphalidae, Satyrinae) is sympatric and synchronic with H. sosybius in southeast US coastal plains, while another new Hermeuptychia species – not hermes – inhabits south Texas and northeast Mexico. ZooKeys 379: 43-91. https://doi.org/10.3897/zookeys.379.6394
Figures 1-9 - Historical illustrations and specimens of Hermeuptychia sosybius, its original description, and neotype. 1–3 Illustration of Hermeuptychia sosybius syntype(s) by William Jones [1745–1818] from an unpublished book called the "Icones" (Vane-Wright 2010), currently in Oxford University Museum of Natural History, UK (Smith 1986). 1 shows the upper right quadrant of the plate LII from Volume 5 2, 3 are magnified cropped images off this plate showing dorsal and ventral aspects, respectively; ventral image (3) is rotated clockwise for the ease of comparison with specimens. The specimen with ventral side illustrated (3 and on the right in 1) is designated as the lectotype herein and is apparently lost 4–7 Two possible syntypes of Hermeuptychia sosybius from the Macleay collection (Macleay Museum, The University of Sydney, Australia). Neither specimen bears any labels 4, 6 show dorsal aspect and 5, 7 show ventral aspect 8 Original description of Hermeuptychia sosybius and its translations. Note that the Jones illustrations of Hermeuptychia sosybius are currently bound within Volume 5, and not 6 as per description 9 Neotype of Hermeuptychia sosybius (designated herein, also see Figs 10–11, genitalia Fig. 62p, DNA barcode tree Fig. 66b), in USNM collection, from USA: Georgia: Chatham Co., Savannah, 28-Jul-1958, leg. G. B. Small, genitalia NVG131102-61, DNA voucher 13386A07, GenBank accession for mitochondrial DNA COI barcode KJ025561. Scale bar refers to 9 only, other images are scaled approximately. Images 1–3 are copyright of Oxford University Museum of Natural History, UK (used with permission), and images 4–7 are copyright of Macleay Museum, The University of Sydney, Australia and are photographed by Robert Blackburn (used with permission).
Figure 63 from: Grishin N, Cong Q (2014) A new Hermeuptychia (Lepidoptera, Nymphalidae, Satyrinae) is sympatric and synchronic with H. sosybius in southeast US coastal plains, while another new Hermeuptychia species – not hermes – inhabits south Texas and northeast Mexico. ZooKeys 379: 43-91. https://doi.org/10.3897/zookeys.379.6394
Figure 63 - Morphometric differences between male genitalia of Hermeuptychia sosybius (black) and Hermeuptychia hermybius (blue). Measurements used are marked on dorsal view of uncus (top left) and on lateral view of complete genitalia (bottom left): a width of uncus at the apex b width of uncus at the narrowest point near the base ("neck" at the joint with tegumen) c distance from the uncus apex to the cross-section at the widest point d distance from the uncus apex to the cross-section at the narrowest point near the base l length of valval dorsal "window" h height of valva (in lateral view) at the end of the dorsal "window", direction of height measurement is perpendicular to the direction of length measurement. Measurements of genitalia shown in Fig. 62 are plotted on the right. Horizontal axis combines all uncus measurements into a formula a/b+0.5*c/d and vertical axis shows measurements of valva as h/l. Each point corresponds to a specimen and a letter next to it is the same one that denote its genitalia in Fig. 62.
Figures 32-47 from: Grishin N, Cong Q (2014) A new Hermeuptychia (Lepidoptera, Nymphalidae, Satyrinae) is sympatric and synchronic with H. sosybius in southeast US coastal plains, while another new Hermeuptychia species – not hermes – inhabits south Texas and northeast Mexico. ZooKeys 379: 43-91. https://doi.org/10.3897/zookeys.379.6394
Figures 32-47 - Hermeuptychia intricata paratypes and Hermeuptychia sosybius specimens. 32–35, 40–43 Hermeuptychia intricata 36–39, 44–47 Hermeuptychia sosybius; data in text and Table 1. Sexes and DNA voucher codes are: 32 ♂ 13385G11 33 ♀ 13385G08 34 ♂ 13385G07 35 ♂ 13386A02 36 ♂ 13385G10 37 ♀ 13385G12 38 ♀ 13386A04 39 ♀ 13386A06 40 ♂ 13385H02 41 ♂ 13385H01 42 ♂ 13386A05 43 ♂ 13386A03 44 ♂ 15609E04 45 ♀ 13385H07 46 ♂ 13385H08 47 ♂ 13386A01. All specimens are in USNM collection. Ventral wing surfaces are shown. "F" specifies mirror image (left-right inverted).
Figures 22-31 from: Grishin N, Cong Q (2014) A new Hermeuptychia (Lepidoptera, Nymphalidae, Satyrinae) is sympatric and synchronic with H. sosybius in southeast US coastal plains, while another new Hermeuptychia species – not hermes – inhabits south Texas and northeast Mexico. ZooKeys 379: 43-91. https://doi.org/10.3897/zookeys.379.6394
Figures 22-31 - Hermeuptychia intricata. 22–23 holotype, others are paratypes, data in text and Table 1. Sexes and DNA voucher codes are: 24 ♀ NVG-1554 25 ♀ NVG-1565 26–27 ♀ 13385G09 28–29 ♂ NVG-1631 30–31 ♀ NVG-1629. Dorsal/ventral surfaces are in even/odd-numbered figures, except 24, which is ventral. Labels are shown for the holotype and are reduced 2.5-fold compared to specimens as indicated by a smaller scale bar. "F" specifies mirror image (left-right inverted).
Figure 69 from: Grishin N, Cong Q (2014) A new Hermeuptychia (Lepidoptera, Nymphalidae, Satyrinae) is sympatric and synchronic with H. sosybius in southeast US coastal plains, while another new Hermeuptychia species – not hermes – inhabits south Texas and northeast Mexico. ZooKeys 379: 43-91. https://doi.org/10.3897/zookeys.379.6394
Figure 69 - Life history of Hermeuptychia sosybius. USA: TX: Brazoria County, Bar-X Ranch, Rd. 971N, 29.13252, -95.58340, ex ovum ex ♀ collected on 4-Mar-2000, except o, which is TX: Wise Co., LBJ National Grassland. a ovum, 6-Mar-2000 b–d 1st instars, photographed on 14- 14- & 16-Mar-2000, respectively e–g 2nd instars photographed on 21- 19- & 21-Mar-2000 e, f are just after molt, shed larval skins are behind and 1st instar head capsule (black) is on the left in e, f is in a curled position adopted when disturbed h pre-molt quiescent 2nd instar larvae in a typical "head-to-head" resting position, 24-Mar-2000 i–j 3rd instars, 24- & 27-Mar-2000 k–l 4th (ultimate) instars, ♂♂, 3- & 6-Apr-2000 l close to pupation, note the color and shape change m prepupa, 6-Apr-2000 n–p pupae, 9-Apr-2000, 8-Aug-1998, & 17-Apr-2000 o is from Wise Co., wing color is starting to develop p near eclosion, dark adult is seen through semi-transparent pupal cuticle. Most images show different individuals. Images a–g are enlarged 2 times (scale on f) compared to the rest (scale on l).
UniDAM: TESS-HERMES
<p>UniDAM results for TESS-HERMES data with Gaia DR2 parallaxes</p>
Male head of a herm
Male head of a herm from the window reveals of the Berlin Bauakademie. The object is made of terracotta and was made in the 1830s. From 1831 to 1836, the Bauakademie building designed by Karl Friedrich Schinkel was built in place of the Altes Packhof at the Schleusenbrücke. Based on drawings by Schinkel and subsequent models by various artists, part of the terracotta decoration of the building was produced in the pottery factory of August Cornelius Gormann. See the object in our database: https://sammlung-online.stadtmuseum.de/Details/Index/348360 **CC-BY-Attribution: Stadtmuseum Berlin | Oliver Ziebe** Source: Objaverse 1.0 / Sketchfab
Female head of a herm
Female head of a herm from the window reveals of the Berlin Bauakademie. The object is made of terracotta and was made in the 1830s. From 1831 to 1836, the Bauakademie building designed by Karl Friedrich Schinkel was built in place of the Altes Packhof at the Schleusenbrücke. Based on drawings by Schinkel and subsequent models by various artists, part of the terracotta decoration of the building was produced in the pottery factory of August Cornelius Gormann. See the object in our database: https://sammlung-online.stadtmuseum.de/Details/Index/348351 **CC-BY-Attribution: Stadtmuseum Berlin | Oliver Ziebe** Source: Objaverse 1.0 / Sketchfab
Head of Hermes
A pentelic marble Early Roman head of Hermes, from a herm. Height, 0.326, m Given to the museum in 1850 by Dr John Disney. Documentation: Michaelis, Adolf. 1882. Ancient marbles in Great Britain. no. 53 Budde, Ludwig. Nicholls, Richard V.. 1967. Catalogue of the Greek and Roman sculpture in the Fitzwilliam Museum, Cambridge. no. 48, pl. 14 Disney, J.. 1846. Museum Disneianum : being a description of a collection of ancient marbles, in the possession of John Disney. pl. xvi Object Number: GR.22.1850 (Antiquities) http://data.fitzmuseum.cam.ac.uk/id/object/65491 Source: Objaverse 1.0 / Sketchfab
Improving Information to Caregivers Via Adaptation and Implementation of the HERMES Intervention
ClinicalTrials.gov study NCT04437563. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Human Insulin Analogs: Evaluation of Inflammatory mRNA Expression of Macrophages and Endothelial Function of Short-acting Insulin - HERMES Pilot Study
ClinicalTrials.gov study NCT01417897. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Hermes
Figure relief depicting the messenger of the gods Hermes on the former post office building in Purkersdorf. The building in early classicist style from the year 1797 is decorated with a total of 6 reliefs around the activities of the post office. The building was built by hereditary postmaster Joseph Edler von Fürnberg, imperial knight and k.u.k. Colonel. Source: Objaverse 1.0 / Sketchfab
Statuette of Hermes - Pompeian wreck
Statuette of Hermes - Pompeian wreck. The god has youthful features, with a beardless face, a head covered by a winged and plumed brimmed petasus. The figure is supported on the right leg, while the left is relaxed forward. Camarina, Ragusa, Sicily, Italy. Roman Age. 1st century AD. Museo Archeologico Ibleo di Ragusa. 439 images. GDH ID and Catalog No. RG9150 Citation: Di Stefano, G., Sammito, A. & Scerra, S. (2008): ""Tesori camarinesi" … in fondo al mare della storia", in Thesaurus Hyblaeus: 14-27. We acknowledge the collaboration of the "Soprintendenza per i Beni Culturali ed Ambientali di Ragusa" and the "Parco Archeologico di Kamarina e Cava d'Ispica". Our most sincere thanks to General CC, retired, Renato Scuzzarello, the archaeologist Dr. Saverio Scerra, the architect Giorgio Battaglia, the restorer Stefania Patti Occhipinti and the archaeologists Veronica Falcone and Alessandra D'Izzia, the custodians of Parco Archeologico Marco Giardina, Giovanna Brugaletta e Rosario Licitra Source: Objaverse 1.0 / Sketchfab
MODEL-010 Hermitage Museum - Hermes
another model i did for a measium project Source: Objaverse 1.0 / Sketchfab
HerMES 250 micron SUSSEXtractor 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.
HerMES 500 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.
HerMES 250 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.
HerMES 500 micron SUSSEXtractor 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.
HerMES Band-merged Catalog (24 micron positions)
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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