Record holder animals Jeev jantuon ke karname chapter 13 rejuvenation -Hydra ; Seasquirt B.leachii

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HYDRA IS A CHAMPION LIKE AXOLOTL AND PLANARIA BUT B.leachii SEA SQUIRT IS CHAMPION OF CHAMPIONS IN THE SCIENCE AND ART OF REJUVENATION WITH AN UNPARALALLED LIFE CYCLE -A MOST AMAZING ONE INDEED

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Record holder animals Jeev jantuon ke karname chapter 13 rejuvenation -Hydra ; Seasquirt B.leachii

EXO ELECTROGENIC SPECIES ARE FOUND IN MANY GENERA OF EUKARYOTIC AS WELL AS PROKARYOTIC ORGANISMS ;BUT BACTERIA ,PARTICULARLY CYANOBACTERIA AND PHOTOSYNTHETIC EUKAROTES LIKE ALGAE AREIN THE FOREFRONT - BOTH MICRO AMD MACRO ALGAE ARE BEING UTILISED WITH OR WITHOUT BACTERIA IN MFCs FOR TREARING POLLUTED WATER AND SIMULTANEOUS PRODUCTION OF ELECTRICITY -THE ADVANTAGE WITH ALGAE IS THEY SUCK IN CO2 AND GIVE OUT O2 AND ARE THUS BETTER FOR ENVIRONMENT NITZCHIA IS A LARGE GENUS OF DIATOMS WHICH INCLUDES BOTH FRESH WATER AND MARINE SPECIES -MANY TOXIC ALSO;BUT THEY ALSO SERVES AS GOOD BIOSENSORS MAINLY DUE TO THEIR BIOLUMINESCENT POROUS SILICON FRISTULE DIATOMS LIKE NITZSCIA ARE ALSO PREFERRED DUE TO THEIR OIL PRODUCTION AND OTHER USES OF THEIR FRISTULE

Exoelectrogens - Micro Algae - Chlorella - SNIPED.docx

SantoshBhatnagar1

EXOELECTROGENS ARE ORGANISMS WHICH CAN RECEIVE ELECTRONS FROM DONARS AND CAN EXPORT ELECTRONS OUTSIDE THE CELL OR CELLS THE ELECTRONS PRODUCED DURING PHOTOSYNTHESIS OR RESPIRATION AVAILABLE TO THEM CAN BE PASSED ON TO ELCTRON ACCEPTORS VIA ELECTRODES AND DURING THE PROCESS ELECTRICITY GETS GENERATED IN THE CIRCUIT . THE CHALLENGE IS TO EXTRACT ELECTRONS AND USE THEM FOR POWER GENERATION AS WELL AS SIMULTANEOUSLY CLEAN POLLUTED WATER AND PRODUCE HYDROGEN ETC AND OTHER BY PRODUCTS .

SHEWANELLA - VERSATILE EXOELECTROGENIC FACULTATIVE ANAEROBE CAPABLE OF GENERATING ELECTRICITY BY REDUCING MANY METALS WHILE RESPIRING AND TRANSFERING ELECTRONS EXTRACELLULARLY HENCE THEIR BIOFILMS AREUSED IN MFCs,MECs. ;KNOWN FOR THRIVING ON A VARIETY OF SUBSTRATES AND REDUCING MANY NOBLE METALS LIKE GOLD SILVER PLATINUM ETC ; ALSO CAPABLE OF PRODUCING HYDROGEN AND H2S; ALSO FAMOUS FOR BIOSYNTHESIS OF NANOPARICLES ;PRAISED FOR EFFICIENCY OF ITS NANOWIRES AND BIOFILMS ; CAN GENERATE ELECTRICITY FROM WASTE ALSO;HENCE SELECTED FOR DEEPSPACE RESEARCH -COULD SOLVE ASTRAUNOTS URINE DISPOSAL PROBLEM AS IT CAN MAKE IT REUSABLE WHILE PROVIDING POWER TO SATELLITE;IT IS ALSO INFAMOUS FOR SPOILING FOOD-FISH MEAT ETC AND CAUSING DISEASES IN HUMANS .

EXOELECTROGENS - GEOBACTER - P D SNIPED.docx

SantoshBhatnagar1

GEOBACTER IS ONE OF THE MOST FAMOUS EXOELECTROGENIC BACTERIA WHICH WAS THE FIRST BACTERIUM DISCOVERED WITH CAPABLITY OF OXIDISING ORGANIC COMPONDS AND METALS( INCLUDING RADIOACTIVE METALS AND PETROLEUM COMPOUNDS )INTO CO2 USING IRONOXIDE ETC AS ELECTRON ACCEPTOR AND PRODUCING ELECTRIC CURRENT. ITHAS BEEN USED IN VARY MANY EXPERIMENTS TO TEST THE WONDERFUL QUALITIES, ABILITIES AND CAPABILITIES OF VERSATILE EXOELECTROGENS AND THEIR USE FOR BIOREMEDIATION AND BIOFUEL PRODUCTION., THEY ARE ALSO CAPABLE OF RESPIRING ON GRAPHITE ELECTRODES

EXOELECTROGENS -INTRODUCTION II SNIPE.docx

SantoshBhatnagar1

EXOELECTROGENS ARE VERSATILE HEROES CAPABLE OF SIMULTANEOUSLY DELIVERING MULTIPLE BENEFITS TO US INVARIOUS FIELDS RANGING FROM BIOREMEDIATION TO ENERGY,ENVIRONMENT, SENSORS, CLEAN BIO FUELS DESALINATION,Etc AND ARE POISED TO SOLVE OUR WASTE DISPOSAL PROBLEM EVEN IN SPACE. ONE FEALS LIKE SALUTING THEM FOR THEIR MULTIPLE TALENTS. THEY INCLUDE MAINLY BACTERIA BUT ALSO MICRO ALGAE, FUNGI,AND EVEN SOME ANGIOSPERMS .

Exoelectrogens -cover-Introduction - SNIPED.docx

SantoshBhatnagar1

CHAMPIONS OF THE PLANT KINGDOM - CONTENTS SNIP.docx

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CHAMPION FUNGI -PHELLINUS ELLIPSOIDEUS - LARGEST FRUITING BODY - SNIP PD.docx

SantoshBhatnagar1

Champion Viruses -Largest - Pithovirus- S.docx

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VIRUSES ARE NOT CONSIDERED LIVING BEINGS BUT EVEN IF THEY WERE THEY WOULD NOT FIT IN ANY KINGDOM ;THEY ARE ACTUALLY ENEMIES OF ALL KINGDOMS OF LIVING BEINGS; HENCE I WAS INITIALLY RELUCTENT TO INCLUDE THEM IN ABOOK ABOUT LIVING BEINGS BUT THEN I THOUGHT WITHOUT THEM THE STORY OF LIVING BEINGS IS NOT COMPLETE ;FURTHER THEY ARE NOT TREATED AS LIVING BY OUR DEFINITION OF LIFE AND LIVING BEINGS OTHERWISE THEY HAVE MANY CHARCTERISTICS OF BEINGS AND ARE WORTHY OF DUE CONSIDERATION AND FIT INTO OUR DEFINITION OF CHAMPIONS AMONGST VIRUSES PITHO VIRUSESARE LARGEST AND MOST ANCIENT AND WITH MANY INTERESTING FEATURES .

Champion of champions -Prayer to vishvkarma.docx

SantoshBhatnagar1

CHAMPION LILLIPUTS -SMALLEST VIRUS - CIRCO ; RSV SNIP PD.docx

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CHAMPION LILLIPUTS- SMALLEST BACTERIA - PELAGIBACTER SNIP PD.docx

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CHAMPION LILLIPUTS - BACTERIA -MYCOPLASMA -SMALLEST SNIP PD.docx

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CHAMPION LILLIPUTS - SMALLEST FUNGI 2 -CHYTRIDS SNIP PD.docx

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CHAMPION LILLIPUTS - YEAST -SMALLEST FUNGI SNIP.docx

SantoshBhatnagar1

YEAST IS ONE OF THE SMALLEST FUNGI KNOWN ;BUT IT IS UNLIKE TYPICAL FUNGI .ITS MAIN FEATURE IS ITS UNICELLULAR CHARACTER AND ITS ABILITY TO CAUSE FERMENTATION BY ANAEROBIC RESPIRATION ;AND THEREFORE ITS USE IN BEER &BREAD MAKING ; ITS USE FOR GENERATING ELECTRICITY IS ALSO EMERGING AS ANOTHER USEFUL FEATURE .FOR SCIENTISTS IT IS A MODEL ORGANISM FOR SCIENTIFIC RESEARCH TO LEARN ABOUT INTRA CCELLULAR PROCESSES OF EUKARYOTES AND GENETICS

CHAMPION LILLIPUTS - ALGAE SMALLEST - B BIGELOII SNIP PD.docx

SantoshBhatnagar1

CHAMPION LILLIPUTS - AZOLLA ANABAENA SYMBIOSIS - SNIP.docx

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Champion lilliputs - Azolla Anabaena symbiosis - Agriculturistmusa.com.docx

SantoshBhatnagar1

CHAMPION LILLIPUTS - SMALLEST : ANGIOSPERMS ; GYMNOSPERMS ;PTERIDPHYTES ;BR...

SantoshBhatnagar1

CHAMPIONS ARE THOSE WHICH EXCEL IN SOME FIELD AND OUTBIDDING NEAREST RIVALS SHOWING THEY ARE THE BEST AND REACH THE TOP ;EXCELLENCE IS NOT THE PRESERVE OF THE TALLEST BIGGEST LARGESTOR HIGHEST -IT CAN BE EXHIBITED EVEN THE SMALLEST SHORTEST OR LIGHTEST;HERE INTERESTING EXAMPLES HAVE BEEN GIVEN FROM ALL TYPES DESCRIBING THEIR SPECIAL FEATURES AND CONSIDERING THEM CHAMPIONS ON THE BASIS OF SCIENTIFICALLY ESTABLISHED FACTS

CHAMPION UNICELLULAR ALGA -ACETABULARIA SNIP PD.docx

SantoshBhatnagar1

CHAMPION LIVING FOSSILS -META SEQOIA WOLLEMI PINE CYCAD SNIP PD.docx

SantoshBhatnagar1

一比一原版美国佩斯大学毕业证如何办理

gyhwyo

原版一模一样【微信：741003700 】【美国佩斯大学毕业证成绩单】【微信：741003700 】学位证，留信认证（真实可查，永久存档）原件一模一样纸张工艺/offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。本公司拥有海外各大学样板无数，能完美还原。 1:1完美还原海外各大学毕业材料上的工艺：水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠。文字图案浮雕、激光镭射、紫外荧光、温感、复印防伪等防伪工艺。材料咨询办理、认证咨询办理请加学历顾问Q/微741003700 【主营项目】一.毕业证【q微741003700】成绩单、使馆认证、教育部认证、雅思托福成绩单、学生卡等！二.真实使馆公证(即留学回国人员证明,不成功不收费) 三.真实教育部学历学位认证（教育部存档！教育部留服网站永久可查）四.办理各国各大学文凭(一对一专业服务,可全程监控跟踪进度) 如果您处于以下几种情况： ◇在校期间，因各种原因未能顺利毕业……拿不到官方毕业证【q/微741003700】 ◇面对父母的压力，希望尽快拿到； ◇不清楚认证流程以及材料该如何准备； ◇回国时间很长，忘记办理； ◇回国马上就要找工作，办给用人单位看； ◇企事业单位必须要求办理的 ◇需要报考公务员、购买免税车、落转户口 ◇申请留学生创业基金留信网认证的作用: 1:该专业认证可证明留学生真实身份 2:同时对留学生所学专业登记给予评定 3:国家专业人才认证中心颁发入库证书 4:这个认证书并且可以归档倒地方 5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息 6:个人职称评审加20分 7:个人信誉贷款加10分 8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才办理美国佩斯大学毕业证【微信：741003700 】外观非常简单，由纸质材料制成，上面印有校徽、校名、毕业生姓名、专业等信息。办理美国佩斯大学毕业证【微信：741003700 】格式相对统一，各专业都有相应的模板。通常包括以下部分：校徽：象征着学校的荣誉和传承。校名:学校英文全称授予学位：本部分将注明获得的具体学位名称。毕业生姓名：这是最重要的信息之一，标志着该证书是由特定人员获得的。颁发日期：这是毕业正式生效的时间，也代表着毕业生学业的结束。其他信息：根据不同的专业和学位，可能会有一些特定的信息或章节。办理美国佩斯大学毕业证【微信：741003700 】价值很高，需要妥善保管。一般来说，应放置在安全、干燥、防潮的地方，避免长时间暴露在阳光下。如需使用，最好使用复印件而不是原件，以免丢失。综上所述，办理美国佩斯大学毕业证【微信：741003700 】是证明身份和学历的高价值文件。外观简单庄重，格式统一，包括重要的个人信息和发布日期。对持有人来说，妥善保管是非常重要的。

MICROBIAL INTERACTION PPT/ MICROBIAL INTERACTION AND THEIR TYPES // PLANT MIC...

ABHISHEK SONI NIMT INSTITUTE OF MEDICAL AND PARAMEDCIAL SCIENCES , GOVT PG COLLEGE NOIDA

Microbial interaction Microorganisms interacts with each other and can be physically associated with another organisms in a variety of ways. One organism can be located on the surface of another organism as an ectobiont or located within another organism as endobiont. Microbial interaction may be positive such as mutualism, proto-cooperation, commensalism or may be negative such as parasitism, predation or competition Types of microbial interaction Positive interaction: mutualism, proto-cooperation, commensalism Negative interaction: Ammensalism (antagonism), parasitism, predation, competition I. Mutualism: It is defined as the relationship in which each organism in interaction gets benefits from association. It is an obligatory relationship in which mutualist and host are metabolically dependent on each other. Mutualistic relationship is very specific where one member of association cannot be replaced by another species. Mutualism require close physical contact between interacting organisms. Relationship of mutualism allows organisms to exist in habitat that could not occupied by either species alone. Mutualistic relationship between organisms allows them to act as a single organism. Examples of mutualism: i. Lichens: Lichens are excellent example of mutualism. They are the association of specific fungi and certain genus of algae. In lichen, fungal partner is called mycobiont and algal partner is called II. Syntrophism: It is an association in which the growth of one organism either depends on or improved by the substrate provided by another organism. In syntrophism both organism in association gets benefits. Compound A Utilized by population 1 Compound B Utilized by population 2 Compound C utilized by both Population 1+2 Products In this theoretical example of syntrophism, population 1 is able to utilize and metabolize compound A, forming compound B but cannot metabolize beyond compound B without co-operation of population 2. Population 2is unable to utilize compound A but it can metabolize compound B forming compound C. Then both population 1 and 2 are able to carry out metabolic reaction which leads to formation of end product that neither population could produce alone. Examples of syntrophism: i. Methanogenic ecosystem in sludge digester Methane produced by methanogenic bacteria depends upon interspecies hydrogen transfer by other fermentative bacteria. Anaerobic fermentative bacteria generate CO2 and H2 utilizing carbohydrates which is then utilized by methanogenic bacteria (Methanobacter) to produce methane. ii. Lactobacillus arobinosus and Enterococcus faecalis: In the minimal media, Lactobacillus arobinosus and Enterococcus faecalis are able to grow together but not alone. The synergistic relationship between E. faecalis and L. arobinosus occurs in which E. faecalis require folic acid

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一比一原版美国佩斯大学毕业证如何办理

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Sérgio Sacani

Context. The early-type galaxy SDSS J133519.91+072807.4 (hereafter SDSS1335+0728), which had exhibited no prior optical variations during the preceding two decades, began showing significant nuclear variability in the Zwicky Transient Facility (ZTF) alert stream from December 2019 (as ZTF19acnskyy). This variability behaviour, coupled with the host-galaxy properties, suggests that SDSS1335+0728 hosts a ∼ 106M⊙ black hole (BH) that is currently in the process of ‘turning on’. Aims. We present a multi-wavelength photometric analysis and spectroscopic follow-up performed with the aim of better understanding the origin of the nuclear variations detected in SDSS1335+0728. Methods. We used archival photometry (from WISE, 2MASS, SDSS, GALEX, eROSITA) and spectroscopic data (from SDSS and LAMOST) to study the state of SDSS1335+0728 prior to December 2019, and new observations from Swift, SOAR/Goodman, VLT/X-shooter, and Keck/LRIS taken after its turn-on to characterise its current state. We analysed the variability of SDSS1335+0728 in the X-ray/UV/optical/mid-infrared range, modelled its spectral energy distribution prior to and after December 2019, and studied the evolution of its UV/optical spectra. Results. From our multi-wavelength photometric analysis, we find that: (a) since 2021, the UV flux (from Swift/UVOT observations) is four times brighter than the flux reported by GALEX in 2004; (b) since June 2022, the mid-infrared flux has risen more than two times, and the W1−W2 WISE colour has become redder; and (c) since February 2024, the source has begun showing X-ray emission. From our spectroscopic follow-up, we see that (i) the narrow emission line ratios are now consistent with a more energetic ionising continuum; (ii) broad emission lines are not detected; and (iii) the [OIII] line increased its flux ∼ 3.6 years after the first ZTF alert, which implies a relatively compact narrow-line-emitting region. Conclusions. We conclude that the variations observed in SDSS1335+0728 could be either explained by a ∼ 106M⊙ AGN that is just turning on or by an exotic tidal disruption event (TDE). If the former is true, SDSS1335+0728 is one of the strongest cases of an AGNobserved in the process of activating. If the latter were found to be the case, it would correspond to the longest and faintest TDE ever observed (or another class of still unknown nuclear transient). Future observations of SDSS1335+0728 are crucial to further understand its behaviour. Key words. galaxies: active– accretion, accretion discs– galaxies: individual: SDSS J133519.91+072807.4

Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...

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Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation

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We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS + 53.13485 − 27.82088 with a host spectroscopic redshift of 2.903 ± 0.007 . The transient was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Photometric and spectroscopic followup with NIRCam and NIRSpec, respectively, confirm the redshift and yield UV-NIR light-curve, NIR color, and spectroscopic information all consistent with a Type Ia classification. Despite its classification as a likely SN Ia, SN 2023adsy is both fairly red ( � ⁢ ( � − � ) ∼ 0.9 ) despite a host galaxy with low-extinction and has a high Ca II velocity ( 19 , 000 ± 2 , 000 km/s) compared to the general population of SNe Ia. While these characteristics are consistent with some Ca-rich SNe Ia, particularly SN 2016hnk, SN 2023adsy is intrinsically brighter than the low- � Ca-rich population. Although such an object is too red for any low- � cosmological sample, we apply a fiducial standardization approach to SN 2023adsy and find that the SN 2023adsy luminosity distance measurement is in excellent agreement ( ≲ 1 ⁢ � ) with Λ CDM. Therefore unlike low- � Ca-rich SNe Ia, SN 2023adsy is standardizable and gives no indication that SN Ia standardized luminosities change significantly with redshift. A larger sample of distant SNe Ia is required to determine if SN Ia population characteristics at high- � truly diverge from their low- � counterparts, and to confirm that standardized luminosities nevertheless remain constant with redshift.

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JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDS

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The pathway(s) to seeding the massive black holes (MBHs) that exist at the heart of galaxies in the present and distant Universe remains an unsolved problem. Here we categorise, describe and quantitatively discuss the formation pathways of both light and heavy seeds. We emphasise that the most recent computational models suggest that rather than a bimodal-like mass spectrum between light and heavy seeds with light at one end and heavy at the other that instead a continuum exists. Light seeds being more ubiquitous and the heavier seeds becoming less and less abundant due the rarer environmental conditions required for their formation. We therefore examine the different mechanisms that give rise to different seed mass spectrums. We show how and why the mechanisms that produce the heaviest seeds are also among the rarest events in the Universe and are hence extremely unlikely to be the seeds for the vast majority of the MBH population. We quantify, within the limits of the current large uncertainties in the seeding processes, the expected number densities of the seed mass spectrum. We argue that light seeds must be at least 103 to 105 times more numerous than heavy seeds to explain the MBH population as a whole. Based on our current understanding of the seed population this makes heavy seeds (Mseed > 103 M⊙) a significantly more likely pathway given that heavy seeds have an abundance pattern than is close to and likely in excess of 10−4 compared to light seeds. Finally, we examine the current state-of-the-art in numerical calculations and recent observations and plot a path forward for near-future advances in both domains.

快速办理(UAM毕业证书)马德里自治大学毕业证学位证一模一样

hozt8xgk

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The cost of acquiring information by natural selection

Carl Bergstrom

This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome. It's based on the first part of this research paper: The cost of information acquisition by natural selection Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577

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快速办理(UAM毕业证书)马德里自治大学毕业证学位证一模一样

The cost of acquiring information by natural selection

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