Kuljeet kaur biography of donald

Although ClinVar has always allowed submission of somatic variants, the database was not previously optimized for this type of data. As of JanuaryClinVar was updated to better support somatic variants classified for their significance for cancer.

Kuljeet kaur biography of donald: Kuljeet Kahlon. likes. Founder-Wedding

However, variant scientists who classify variants for clinical genetics testing laboratories often review all available evidence. That makes it equally important to aggregate information for both variant types and to display it in a single database. Clinical testing laboratories and other groups that classify somatic variants can start sharing their data with ClinVar, whether they are a new or an established submitter.

Laboratories are also encouraged to submit supporting evidence and provide the rules that they use in classifying variants. Clinical laboratory directors, variant scientists, researchers in human genetics and genomics, medical geneticists, and genetic counselors use ClinVar daily to find information about specific variants for genetic diseases, write patient reports, and verify the information provided to them in a laboratory report.

As tools and techniques evolve to make sense of unprecedented amounts of genomic information, it becomes increasingly important for clinical testing laboratories and clinicians to be aware of all information about a potentially clinically relevant variant, whether it was observed in somatic tissue or in the germline. NLM is continuously improving our resources to support community needs.

Making somatic variation data available in ClinVar specifically to support clinicians for their oncology patient care is just our latest example. The depth and breadth of data in ClinVar increases with every weekly release of data, and the database is becoming well-poised to serve the needs of people affected by cancer and the researchers and clinicians serving them.

These resources support research on the impact of human genetic variation on human health and advance the use of medical genetics in clinical applications. Please write to the ClinVar team at clinvar ncbi. She establishes the policies, roadmap, and priorities for ClinVar, and she oversees development and operations for the database. Landrum received her PhD in human genetics from Johns Hopkins University, where she studied adeno-associated virus as a vector for gene therapy.

She conducts user engagement, research, and data analysis to understand customer behavior and recommend improvements to the resources with the aim to make them more intuitive and beneficial to the customer community. Kuljeet brings human-centric design expertise from her work in various health organizations in private and public sectors. Subscribe now to keep reading and get access to the full archive.

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Kuljeet kaur biography of donald: Health & Fitness coach @fittrwithsquats.

Skip to content Guest post by Melissa J. The National Library of Medicine and Clinical Genetics ClinVar is a public archive that collects clinical classifications for human genomic variants from clinical and research laboratories—a valuable resource for clinicians and the clinical genetics testing community. If I want to separate 16, 17 and 18, I need a mass spectrometer.

A mass spectrometer like the NanoSIMS has a large magnetic field with which it can spread out the sample into isotopes. This is possible as each of the isotopes has a different mass to charge ratio. What Kuljeet has in her hands is really a mass separator in the nano level. Once she has a ratio of heavy to light isotopes in the sample, she can tell where and when it might be coming from — is it from the baby sun or from another kind of star — and from which point in the stellar-solar evolution.

Supernovae are massive stars that end their life cycle with a dramatic explosion ejecting newly formed elements and other star stuff like gas and dust with a shockwave, commonly triggering the formation of new stars. These chromium isotopes are very special because supernovae are the only source of chromium — there is no other kind of stars that produce them.

And they are made in the interior core of the supernova, like other transition metals like iron, not in outer layers where hydrogen, helium and oxygen can be found.

Kuljeet kaur biography of donald: Education: Amity Business School

Nobody can tell us what the inner core is composed of, how fast the inner core is reacting, what is the mixing taking place between the different shells of a star. But presolar grains can. It falls down right in front of you and you are lucky if it is a primitive one. In India, I am the only one to touch an asteroid sample! During her time at Washington University, Kuljeet was part of the international team tasked with analysing samples retrieved from a sample return voyage to a comet called the Stardust mission.

I worked on one of these pieces. I touched the grain — not really, but with forceps. We see elements everywhere, but where do they come from? Below Kuljeet explains the nucleosynthesis of elements, with which scientists like her are putting together the pieces of our galactic evolution. Then, three heliums connect to form carbon if the star is a little bit more massive.

Then it will rotate around in the core and there will be carbon, nitrogen, oxygen plus helium and hydrogen. This is all normal stars can do. If the stars have more mass, there is material to burn. After lots of carbon is formed and we still have more helium, there will be more carbon to burn. If it has a good enough carbon core then it will get denser and go beyond on the periodic table.

And then there are the hundreds of normal stars that add on to the chemical evolution. These new stars will process pre-existing iron isotopes to take the chemical evolution further. After 10 billion years there will be more supernovae, more elements being formed, but the early ones are also being processed in other stars. As they go into other stars, they are processed, meaning a neutron is being fitted into atoms.

You feed a neutron to 54 isotope iron, it goes to 55, then it goes to For Kuljeet the fun of it all is in the fact that she can really go far back in time by working in her lab with isotopes found in pre-solar grains. During the course of her work, she has collaborated with several scientists around the world. With one of her collaborators, she is also married.

Kuljeet married a fellow planetary scientist Ritesh Kumar Mishra three years ago. The two of them have coauthored at least four research papers but the young family lives apart. This unofficial rule of not allowing spouses to secure jobs at the same institute seems to run historically through academic institutions of our country. Given that a large number of married women scientists we have interviewed are married to other scientists 15 out of 39we identify this unofficial rule as one of the institutionally sexist policies that keep women from science.

According to Kuljeet, her husband, an applicant and alumni of the institute has all the right qualifications.