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Johana Villamil
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Angela Romero
ECCV 2018 サーベイ cvpaper.challenge はコンピュータビジョン分野の今を映し、創り出す挑戦です。論文読破・まとめ・アイディア考案・議論・実装・論文執筆(・社会実装)に至るまで広く取り組み、あらゆる知識を共有しています。 http://xpaperchallenge.org/cv/
【ECCV 2018】DeepJDOT: Deep Joint Distribution Optimal Transport for Unsupervis...
【ECCV 2018】DeepJDOT: Deep Joint Distribution Optimal Transport for Unsupervis...
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farcrys
Dhggci 2002 V26n6 1209
Dhggci 2002 V26n6 1209
guest7a15
Bjojana Vidhi
Bjojana Vidhi
Mana Manthani
Prelaboratorio PRÁCTICA 8
Prelaboratorio PRÁCTICA 8
Equipo08
Dv VS DV Revised
Dv VS DV Revised
Cherie Anthe Wright
Recommandé
Tasas de interes
Tasas de interes
Johana Villamil
DUOLINGO
DUOLINGO
Angela Romero
ECCV 2018 サーベイ cvpaper.challenge はコンピュータビジョン分野の今を映し、創り出す挑戦です。論文読破・まとめ・アイディア考案・議論・実装・論文執筆(・社会実装)に至るまで広く取り組み、あらゆる知識を共有しています。 http://xpaperchallenge.org/cv/
【ECCV 2018】DeepJDOT: Deep Joint Distribution Optimal Transport for Unsupervis...
【ECCV 2018】DeepJDOT: Deep Joint Distribution Optimal Transport for Unsupervis...
cvpaper. challenge
Plan1
Plan1
farcrys
Dhggci 2002 V26n6 1209
Dhggci 2002 V26n6 1209
guest7a15
Bjojana Vidhi
Bjojana Vidhi
Mana Manthani
Prelaboratorio PRÁCTICA 8
Prelaboratorio PRÁCTICA 8
Equipo08
Dv VS DV Revised
Dv VS DV Revised
Cherie Anthe Wright
kfhg
Proxecto nixeria
Proxecto nixeria
Raulssito
importancia
Importancia de las integrales en el área tecnologica
Importancia de las integrales en el área tecnologica
Maria Navarrete
Tutorialwebquest
Tutorialwebquest
luizmackedanz
Practica 1 y 2 de Fisica 1
Practica uno y dos
Practica uno y dos
Jose Garcia
Cocinas Regionales de Perú
Cocinas regionales tesen asanza (1)
Cocinas regionales tesen asanza (1)
Wendy Fiorella Tesen Asanza
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13530912_2.PPT
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Il Notiziario Mamò con le principali novità in materia di Lavoro & Sicurezza sul Lavoro.
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News SSL 12 2016
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MASENO: O EQUADOR CRISS CROSS CENTRO URBANO
MASENO: O EQUADOR CRISS CROSS CENTRO URBANO
weblogbasquetenba65
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Abhishek
prashantsharma000
Learn more: https://www.brainlab.com/traumacad VoyantMark is a single marker X-ray calibration and marking device. Designed specifically to work with TraumaCad® surgical planning software, VoyantMark aids in accurately measuring patient anatomy— hip, knee, shoulder, ankle and foot.
VoyantMark Accurate Calibration Flyer
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Brainlab
Algoparanuncaesquecer
Algoparanuncaesquecer
Gabriele de Almeida Silva
Logan was funded by the Rockefeller Center for a Summer 2014 internship, with generous support from the Mr. E. John Rosenwald Jr. ’52 Public Affairs Internship Fund.
Named Internship Profile Summary - Logan Brog (Rosenwald)
Named Internship Profile Summary - Logan Brog (Rosenwald)
Rockefeller Center for Public Policy at Dartmouth College
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mavi9522
Microbiology
Conjugation, transduction and transformation
Conjugation, transduction and transformation
Areesha Ahmad
M.pharm Pharmaceutics 2nd sem. introduction to Pulmonary drug delivery system, mechanism, Aersools, and aerosol parts barriers, physiological properties, preparation methods, evaluation parameters, advantages and diadvantages.
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
sakshisoni2385
Clean In Place
Clean In Place(CIP).pptx .
Clean In Place(CIP).pptx .
Poonam Aher Patil
Cotton crops are vulnerable to a variety of sucking pests, which can severely impact plant health, yield, and fiber quality. These pests primarily feed on plant sap, extracting nutrients directly from the plant's vascular system. Here's a breakdown of some of the most significant sucking pests in cotton cultivation: Aphids: Cotton aphids or melon aphids can cause direct damage by sucking sap and indirect damage by secreting honeydew, which encourages sooty mold growth. This can interfere with photosynthesis and weaken the plant. Aphids can also transmit viral diseases. Whiteflies: Two species, the silverleaf whitefly and the bandedwinged whitefly, are particularly troublesome. They not only suck sap from the underside of leaves, causing yellowing and leaf drop, but their honeydew excretion promotes sooty mold and they can transmit several plant viruses. Thrips: While thrips can chew on plants, their primary damage to cotton is through sucking. They attack the cotton plant during its seedling stage, which can stunt growth and reduce vigor. Thrips are also capable of transmitting the Cotton Bud disease. Spider Mites: These are not insects but arachnids. Spider mites, such as the two-spotted spider mite, suck cell contents from the leaves, leading to speckled discoloration and potentially significant leaf loss if infestations are severe. Leafhoppers: Including various species, leafhoppers can cause direct damage through feeding, which results in leaf curling and stunted growth. They can also be vectors for plant diseases. Mealybugs: These pests are less common but can be problematic, especially in clustered planting conditions. They suck sap and secrete honeydew, which leads to sooty mold. Mealybugs can also spread viruses. Stink Bugs: Although primarily known for their chewing mouthparts, certain stink bugs can cause damage similar to sucking pests by injecting saliva into the plant and sucking out nutrients, leading to boll damage and stained lint. Management Strategies: Cultural Controls: This includes practices such as crop rotation, using resistant varieties, and managing planting and harvesting times to avoid peak pest populations. Biological Controls: Beneficial insects like lady beetles, lacewings, and predatory mites can naturally control sucking pest populations. Parasitic wasps also play a role in controlling aphid and whitefly populations. Chemical Controls: Insecticides may be used but should be chosen carefully to minimize resistance development and preserve beneficial insects. Systemic insecticides can be particularly effective against sucking pests. Integrated Pest Management (IPM): Combining multiple control strategies based on monitoring and thresholds to apply the most effective and environmentally sensitive approach. Effective management of sucking pests in cotton requires a thorough understanding of the pest species present, their life cycles, and the ecological balance of the field environment.
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
PirithiRaju
Botany is the branch of biology that deals with the scientific study of plants, including their structure, growth, reproduction, metabolism, development, and classification. It encompasses a wide range of topics, from the molecular biology of plant cells to the ecological relationships between plants and their environments. Botany is essential for understanding plant diversity, ecology, evolution, and the roles plants play in ecosystems and human societies.
Botany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdf
Sumit Kumar yadav
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kfhg
Proxecto nixeria
Proxecto nixeria
Raulssito
importancia
Importancia de las integrales en el área tecnologica
Importancia de las integrales en el área tecnologica
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Tutorialwebquest
luizmackedanz
Practica 1 y 2 de Fisica 1
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Practica uno y dos
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Cocinas regionales tesen asanza (1)
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13530912_2.PPT
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Il Notiziario Mamò con le principali novità in materia di Lavoro & Sicurezza sul Lavoro.
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Financiera
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Don Logie CV (1)
Donald Logie
7mobasico saez tecnología_recursos naturales
7mobasico saez tecnología_recursos naturales
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A alemanha pode ser pensado desde a terra de salsicha, cerveja, Beethoven e BMW, porem, na realidade...
MASENO: O EQUADOR CRISS CROSS CENTRO URBANO
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weblogbasquetenba65
Abhishek
Abhishek
prashantsharma000
Learn more: https://www.brainlab.com/traumacad VoyantMark is a single marker X-ray calibration and marking device. Designed specifically to work with TraumaCad® surgical planning software, VoyantMark aids in accurately measuring patient anatomy— hip, knee, shoulder, ankle and foot.
VoyantMark Accurate Calibration Flyer
VoyantMark Accurate Calibration Flyer
Brainlab
Algoparanuncaesquecer
Algoparanuncaesquecer
Gabriele de Almeida Silva
Logan was funded by the Rockefeller Center for a Summer 2014 internship, with generous support from the Mr. E. John Rosenwald Jr. ’52 Public Affairs Internship Fund.
Named Internship Profile Summary - Logan Brog (Rosenwald)
Named Internship Profile Summary - Logan Brog (Rosenwald)
Rockefeller Center for Public Policy at Dartmouth College
Nutre todo
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mavi9522
En vedette
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Proxecto nixeria
Proxecto nixeria
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Importancia de las integrales en el área tecnologica
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Cocinas regionales tesen asanza (1)
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13530912_2.PPT
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News SSL 12 2016
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Don Logie CV (1)
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MASENO: O EQUADOR CRISS CROSS CENTRO URBANO
Abhishek
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Named Internship Profile Summary - Logan Brog (Rosenwald)
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Dernier
Microbiology
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Conjugation, transduction and transformation
Areesha Ahmad
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Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
sakshisoni2385
Clean In Place
Clean In Place(CIP).pptx .
Clean In Place(CIP).pptx .
Poonam Aher Patil
Cotton crops are vulnerable to a variety of sucking pests, which can severely impact plant health, yield, and fiber quality. These pests primarily feed on plant sap, extracting nutrients directly from the plant's vascular system. Here's a breakdown of some of the most significant sucking pests in cotton cultivation: Aphids: Cotton aphids or melon aphids can cause direct damage by sucking sap and indirect damage by secreting honeydew, which encourages sooty mold growth. This can interfere with photosynthesis and weaken the plant. Aphids can also transmit viral diseases. Whiteflies: Two species, the silverleaf whitefly and the bandedwinged whitefly, are particularly troublesome. They not only suck sap from the underside of leaves, causing yellowing and leaf drop, but their honeydew excretion promotes sooty mold and they can transmit several plant viruses. Thrips: While thrips can chew on plants, their primary damage to cotton is through sucking. They attack the cotton plant during its seedling stage, which can stunt growth and reduce vigor. Thrips are also capable of transmitting the Cotton Bud disease. Spider Mites: These are not insects but arachnids. Spider mites, such as the two-spotted spider mite, suck cell contents from the leaves, leading to speckled discoloration and potentially significant leaf loss if infestations are severe. Leafhoppers: Including various species, leafhoppers can cause direct damage through feeding, which results in leaf curling and stunted growth. They can also be vectors for plant diseases. Mealybugs: These pests are less common but can be problematic, especially in clustered planting conditions. They suck sap and secrete honeydew, which leads to sooty mold. Mealybugs can also spread viruses. Stink Bugs: Although primarily known for their chewing mouthparts, certain stink bugs can cause damage similar to sucking pests by injecting saliva into the plant and sucking out nutrients, leading to boll damage and stained lint. Management Strategies: Cultural Controls: This includes practices such as crop rotation, using resistant varieties, and managing planting and harvesting times to avoid peak pest populations. Biological Controls: Beneficial insects like lady beetles, lacewings, and predatory mites can naturally control sucking pest populations. Parasitic wasps also play a role in controlling aphid and whitefly populations. Chemical Controls: Insecticides may be used but should be chosen carefully to minimize resistance development and preserve beneficial insects. Systemic insecticides can be particularly effective against sucking pests. Integrated Pest Management (IPM): Combining multiple control strategies based on monitoring and thresholds to apply the most effective and environmentally sensitive approach. Effective management of sucking pests in cotton requires a thorough understanding of the pest species present, their life cycles, and the ecological balance of the field environment.
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
PirithiRaju
Botany is the branch of biology that deals with the scientific study of plants, including their structure, growth, reproduction, metabolism, development, and classification. It encompasses a wide range of topics, from the molecular biology of plant cells to the ecological relationships between plants and their environments. Botany is essential for understanding plant diversity, ecology, evolution, and the roles plants play in ecosystems and human societies.
Botany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdf
Sumit Kumar yadav
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Seismic Method
Seismic Method Estimate velocity from seismic data.pptx
Seismic Method Estimate velocity from seismic data.pptx
AlMamun560346
Site Acceptance test
Site Acceptance Test .
Site Acceptance Test .
Poonam Aher Patil
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Basic concept of chemistry
GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)
Areesha Ahmad
Introduction to Microbiology
GBSN - Microbiology (Unit 1)
GBSN - Microbiology (Unit 1)
Areesha Ahmad
Understanding circumstellar disks is of prime importance in astrophysics, however, their birth process remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, often wrapped into a sub-grid model, play a crucial role in disk formation and evolution. This calls for a combined approach in which both the protostar and circumstellar disk are studied in concert. Aims. We aim to elucidate the small scale physics and constrain sub-grid parameters commonly chosen in the literature by resolving the star-disk interaction. Methods. We carry out a set of very high resolution 3D radiative-hydrodynamics simulations that self-consistently describe the collapse of a turbulent dense molecular cloud core to stellar densities. We study the birth of the protostar, the circumstellar disk, and its early evolution (< 6 yr after protostellar formation). Results. Following the second gravitational collapse, the nascent protostar quickly reaches breakup velocity and sheds its surface material, thus forming a hot (∼ 103 K), dense, and highly flared circumstellar disk. The protostar is embedded within the disk, such that material can flow without crossing any shock fronts. The circumstellar disk mass quickly exceeds that of the protostar, and its kinematics are dominated by self-gravity. Accretion onto the disk is highly anisotropic, and accretion onto the protostar mainly occurs through material that slides on the disk surface. The polar mass flux is negligible in comparison. The radiative behavior also displays a strong anisotropy, as the polar accretion shock is shown to be supercritical whereas its equatorial counterpart is subcritical. We also f ind a remarkable convergence of our results with respect to initial conditions. Conclusions. These results reveal the structure and kinematics in the smallest spatial scales relevant to protostellar and circumstellar disk evolution. They can be used to describe accretion onto regions commonly described by sub-grid models in simulations studying larger scale physics.
Formation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disks
Sérgio Sacani
Theoretical predictions and observational data indicate a class of sub-Neptune exoplanets may have water-rich interiors covered by hydrogen-dominated atmospheres. Provided suitable climate conditions, such planets could host surface liquid oceans. Motivated by recent JWST observations of K2-18 b, we self-consistently model the photochemistry and potential detectability of biogenic sulfur gases in the atmospheres of temperate sub-Neptune waterworlds for the first time. On Earth today, organic sulfur compounds produced by marine biota are rapidly destroyed by photochemical processes before they can accumulate to significant levels. Domagal-Goldman et al. suggest that detectable biogenic sulfur signatures could emerge in Archean-like atmospheres with higher biological production or low UV flux. In this study, we explore biogenic sulfur across a wide range of biological fluxes and stellar UV environments. Critically, the main photochemical sinks are absent on the nightside of tidally locked planets. To address this, we further perform experiments with a 3D general circulation model and a 2D photochemical model (VULCAN 2D) to simulate the global distribution of biogenic gases to investigate their terminator concentrations as seen via transmission spectroscopy. Our models indicate that biogenic sulfur gases can rise to potentially detectable levels on hydrogen-rich water worlds, but only for enhanced global biosulfur flux (20 times modern Earth’s flux). We find that it is challenging to identify DMS at 3.4 μm where it strongly overlaps with CH4, whereas it is more plausible to detect DMS and companion byproducts, ethylene (C2H4) and ethane (C2H6), in the mid-infrared between 9 and 13 μm. Unified Astronomy Thesaurus concepts: Exoplanet atmospheres (487); Exoplanet
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Sérgio Sacani
Research Methodology
COST ESTIMATION FOR A RESEARCH PROJECT.pptx
COST ESTIMATION FOR A RESEARCH PROJECT.pptx
FarihaAbdulRasheed
Wepresent Atacama Large Millimeter/submillimeter Array 12-m, 7-m, and Total Power Array observations of the FUOrionis outbursting system, covering spatial scales ranging from 160 to 25,000 au. The high-resolution interferometric data reveal an elongated 12CO(2–1) feature previously observed at lower resolution in 12CO(3–2). Kinematic modeling indicates that this feature can be interpreted as an accretion streamer feeding the binary system. The mass infall rate provided by the streamer is significantly lower than the typical stellar accretion rates (even in quiescent states), suggesting that this streamer alone is not massive enough to sustain the enhanced accretion rates characteristic of the outbursting class prototype. The observed streamer may not be directly linked to the current outburst, but rather a remnant of a previous, more massive streamer that may have contributed enough to the disk mass to render it unstable and trigger the FU Orionis outburst. The new data detect, for the first time, a vast, slow-moving carbon monoxide molecular outflow emerging from this object. To accurately assess the outflow properties (mass, momentum, and kinetic energy), we employ 13CO(2–1) data to correct for optical depth effects. The analysis indicates that the outflow corresponds to swept-up material not associated with the current outburst, similar to the slow molecular outflows observed around other FUor and Class I protostellar objects.
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Sérgio Sacani
TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C Bushong, Verified Chapters 1 - 40, Complete Newest Version.pdf TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C Bushong, Verified Chapters 1 - 40, Complete Newest Version.pdf
TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...
TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...
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Conjugation, transduction and transformation
Conjugation, transduction and transformation
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
Clean In Place(CIP).pptx .
Clean In Place(CIP).pptx .
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Botany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdf
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service
Seismic Method Estimate velocity from seismic data.pptx
Seismic Method Estimate velocity from seismic data.pptx
Site Acceptance Test .
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Chemical Tests; flame test, positive and negative ions test Edexcel Internati...
Chemical Tests; flame test, positive and negative ions test Edexcel Internati...
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GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)
GBSN - Microbiology (Unit 1)
GBSN - Microbiology (Unit 1)
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hh fit to the GC GeV gamma-ray excess
1.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 130 GeV, hh, χ2 = 35.5, σv = 0.43 × 10−26
2.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 135 GeV, hh, χ2 = 38.6, σv = 0.41 × 10−26
3.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 140 GeV, hh, χ2 = 41.6, σv = 0.39 × 10−26
4.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 145 GeV, hh, χ2 = 44.4, σv = 0.38 × 10−26
5.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 150 GeV, hh, χ2 = 47.0, σv = 0.36 × 10−26
6.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 155 GeV, hh, χ2 = 49.6, σv = 0.35 × 10−26
7.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 160 GeV, hh, χ2 = 52.1, σv = 0.33 × 10−26
8.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 165 GeV, hh, χ2 = 54.4, σv = 0.32 × 10−26
9.
100 101 102 103 Eγ [GeV] 10−7 E2 dN/dE[GeVcm−2 s−1 ] 2 ×
10−8 MDM = 170 GeV, hh, χ2 = 56.6, σv = 0.31 × 10−26
10.
100 101 102 Eγ [GeV] 0 10 20 30 40 50E2 dN/dE[arbitraryunits] χχ →
hh 130 GeV 200 GeV 300 GeV
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