LAKE COUNTY, Calif. — Lake County Animal Care and Control has five cats waiting to meet new families this week.
Call Lake County Animal Care and Control at 707-263-0278 or visit the shelter online at http://www.co.lake.ca.us/Government/Directory/Animal_Care_And_Control.htm for information on visiting or adopting.
The following cats at the shelter have been cleared for adoption.
Female domestic shorthair
This female domestic shorthair kitten has a calico coat.
She is in cat room kennel No. 78, ID No. LCAC-A-3461.
‘Dave’
“Dave” is a young male brown tabby with a short coat.
He is in cat room kennel No. 96, ID No. LCAC-A-3299.
Female domestic shorthair
This young female domestic shorthair cat has a gray tabby coat.
She is in cat room kennel No. 120a, ID No. LCAC-A-3575.
Male domestic shorthair
This young male domestic shorthair cat has a black coat.
He is in cat room kennel No. 120b, ID No. LCAC-A-3576.
Male domestic longhair cat
This 2-year-old male domestic longhair cat has a white coat with gray markings.
He is in cat room kennel No. 129, ID No. LCAC-A-3529.
Email Elizabeth Larson at This email address is being protected from spambots. You need JavaScript enabled to view it.. Follow her on Twitter, @ERLarson, or Lake County News, @LakeCoNews.
LAKE COUNTY, Calif. — Lake County Animal Care and Control has new dogs of various breeds ready to be adopted this week.
Dogs available for adoption this week include mixes of Australian shepherd, Chihuahua, chow chow, dachshund, German shepherd, husky, Labrador retriever, pit bull, shepherd and terrier.
Dogs that are adopted from Lake County Animal Care and Control are either neutered or spayed, microchipped and, if old enough, given a rabies shot and county license before being released to their new owner. License fees do not apply to residents of the cities of Lakeport or Clearlake.
The following dogs at the Lake County Animal Care and Control shelter have been cleared for adoption.
Call Lake County Animal Care and Control at 707-263-0278 or visit the shelter online for information on visiting or adopting.
Female pit bull terrier
This 3-year-old female pit bull terrier has a short gray coat.
She is in kennel No. 12, ID No. LCAC-A-3524.
Male shepherd-chow chow
This 2-year-old male shepherd-chow chow mix has a gold coat.
He is in kennel No. 13, ID No. LCAC-A-3573.
‘Heidi’
“Heidi” is a 5-year-old female Australian shepherd with a long tricolor coat.
She is in kennel No. 14, ID No. LCAC-A-3567.
‘Lucky’
“Lucky” is a 3-year-old male Labrador retriever with a short yellow coat.
He is in kennel No. 15, ID No. LCAC-A-3520.
‘Casandra’
“Casandra” is a 3-year-old female pit bull terrier with a short tan coat.
She is in kennel No. 16, ID No. LCAC-A-3479.
Dachshund-Chihuahua mix
This young male dachshund-Chihuahua mix has a short gray and tan coat.
He is in kennel No. 17, ID No. LCAC-A-3508.
‘Rocky’
“Rocky” is a 6-year-old male Chihuahua with a short tan and white coat.
He is in kennel No. 18, ID No. LCAC-A-3478.
Female shepherd mix
This 1-year-old female shepherd mix has a short gray brindle coat.
She is in kennel No. 19, LCAC-A-3342.
Female Labrador retriever mix
This 3-year-old female Labrador retriever mix has a short yellow coat.
She is in kennel No. 20, ID No. LCAC-A-3438.
Male shepherd
This 2-year-old male shepherd mix has a short black and white coat.
He is in kennel No. 22, ID No. LCAC-A-3466.
Female shepherd mix
This young female shepherd mix has a white coat.
She is in kennel No. 23, ID No. LCAC-A-3472.
Female German shepherd mix
This 2-year-old female German shepherd mix has a short tan coat.
She is in kennel No. 32, ID No. LCAC-A-3491.
Male husky
This 2-year-old male husky has a gray and white coat.
He is in kennel No. 33, ID No. LCAC-A-3484.
Pit bull terrier
This young female pit bull terrier has a short black and white coat.
She is in kennel No. 34, ID No. LCAC-A-3353.
Email Elizabeth Larson at This email address is being protected from spambots. You need JavaScript enabled to view it.. Follow her on Twitter, @ERLarson, or Lake County News, @LakeCoNews.
The California Highway Patrol’s 128 newest officers graduated from the CHP Academy in West Sacramento on Friday after completing 27 weeks of training.
Cadets crossed the stage to receive their badge and assignment at one of the CHP’s 103 area offices throughout the state, as family and friends packed the gymnasium in support of the new officers.
“Completing Academy training is a tremendous achievement,” said CHP Commissioner Amanda Ray. “These women and men are not just starting a new job, they are embarking on a lifelong career that requires extreme dedication and a passion for service.”
At the CHP Academy, cadet training starts with nobility in policing, leadership, professionalism and ethics, and cultural diversity.
Cadets receive instruction on mental illness response and crisis intervention techniques. The training covers vehicle patrol, crash investigation, first aid, and the apprehension of suspected violators, including drivers under the influence of alcohol or drugs.
The cadets receive training in traffic control, report writing, recovery of stolen vehicles, assisting the motoring public, issuing citations, emergency scene management, and knowledge of the California vehicle code, penal code, and health and safety code.
The CHP’s newest officers join the ranks of the more than 6,700 uniformed personnel serving in communities throughout the state.
A new cadet class is scheduled to begin training at the CHP Academy on June 20. Another class of more than 100 cadets is expected to complete training and graduate in early August.
On Thursday, the CHP launched a multiyear recruiting campaign to fill 1,000 vacant officer positions by hiring qualified individuals from diverse communities.
For more information about the “Join the CHP 1,000” campaign, or to apply, visit https://recruitment.chp.ca.gov/ or call the statewide Recruitment Unit at 916-843-4300.
“Joining the CHP family is an opportunity to be the change and make a difference in the community and the lives of those we serve,” added Commissioner Ray.
The mission of the CHP is to provide the highest level of safety, service and security.
MIDDLETOWN, Calif. — Anyone who has been to the top of Rabbit Hill in Middletown knows that the small peak, almost in the middle of town, offers views of surrounding mountains that are breathtaking.
It has long been a dream of the Lake County Land Trust, or LCLT, and local citizens to place directional signs at the summit of Rabbit Hill to point out each significant peak in the panoramic 360 degree view of the surrounding mountains, including St. Helena, Cobb and Harbin.
On a recent Saturday morning the signage project was started with the help of Hidden Valley Lake resident Jean Goulart, who has become a volunteer for the LCLT and will be over-seeing the Rabbit Hill Park.
Goulart is a University of California Naturalist and Climate Steward and a new member of the LCLT Stewardship Committee.
She gathered students from Middletown High School to work on the sign project as part of their community service. Meeting Jean were Cade Dubose, Jose Montanez and Evan Johnson.
Lake County Land Trust volunteers, including Middletown’s Gail Wright, Stewardship Committee member Bob Schoenherr and LCLT board member Val Nixon joined in the effort.
Many thanks to Hardester’s Market in Middletown for donating the use of an auger to dig the hole for the post where the directional signs will be mounted. Hardester’s also donated spray paint to paint the concrete picnic table at the top of the hill.
After the pole was placed in cement, the Middletown High students pruned over growth along the path and near the cement picnic table. They removed steel post fencing and did general cleanup of the area. Painting the concrete table was postponed because of wind.
The small nine-acre park was originally donated to the Madrone Audubon Society in Sonoma County by the late Skee and Huck Hamann. The beloved couple lived atop the little hill and hosted many education programs for local school children.
Over 20 years ago Madrone Audubon transferred ownership to the Lake County Land Trust. Since that time the Land Trust has worked with the local Middletown Art Center and Middletown residents to improve and care for the park.
There are now comfortable benches, a picnic table, and art installations. Soon the public will be able to enjoy informative signs.
The park is open to the public and is used by many local residents for exercising and dog walking. Besides its stunning views it features native serpentine vegetation that includes wildflowers, forbes and native grasses.
The Lake County Land Trust, founded in 1994, is a charitable non-profit dedicated to protecting natural habitats, wetlands, and valuable open space in Lake County go to www.lakecountylandtrust.org.
Astronomers may have discovered the first free-floating black hole in the Milky Way galaxy, thanks to a technique called gravitational microlensing. With new observations, they hope to find many more 'ghost' stars. (Video by Roxanne Makasdjian and Alan Toth, with microlensing animations from Casey Lam and Sean Terry, UC Berkeley’s Moving Universe Lab, and image data courtesy of the OGLE collaboration)
BERKELEY — If, as astronomers believe, the death of large stars leave behind black holes, there should be hundreds of millions of them scattered throughout the Milky Way galaxy. The problem is, isolated black holes are invisible.
Now, a team led by University of California, Berkeley, astronomers has for the first time discovered what may be a free-floating black hole by observing the brightening of a more distant star as its light was distorted by the object's strong gravitational field — so-called gravitational microlensing.
The team, led by graduate student Casey Lam and Jessica Lu, a UC Berkeley associate professor of astronomy, estimates that the mass of the invisible compact object is between 1.6 and 4.4 times that of the sun.
Because astronomers think that the leftover remnant of a dead star must be heavier than 2.2 solar masses in order to collapse to a black hole, the UC Berkeley researchers caution that the object could be a neutron star instead of a black hole.
Neutron stars are also dense, highly compact objects, but their gravity is balanced by internal neutron pressure, which prevents further collapse to a black hole.
Whether a black hole or a neutron star, the object is the first dark stellar remnant — a stellar “ghost” — discovered wandering through the galaxy unpaired with another star.
"This is the first free-floating black hole or neutron star discovered with gravitational microlensing," Lu said. "With microlensing, we're able to probe these lonely, compact objects and weigh them. I think we have opened a new window onto these dark objects, which can’t be seen any other way."
Determining how many of these compact objects populate the Milky Way galaxy will help astronomers understand the evolution of stars — in particular, how they die — and of our galaxy, and perhaps reveal whether any of the unseen black holes are primordial black holes, which some cosmologists think were produced in large quantities during the Big Bang.
The analysis by Lam, Lu and their international team has been accepted for publication in The Astrophysical Journal Letters.
The analysis includes four other microlensing events that the team concluded were not caused by a black hole, though two were likely caused by a white dwarf or a neutron star. The team also concluded that the likely population of black holes in the galaxy is 200 million — about what most theorists predicted.
Same data, different conclusions
Notably, a competing team from the Space Telescope Science Institute (STScI) in Baltimore analyzed the same microlensing event and claims that the mass of the compact object is closer to 7.1 solar masses and indisputably a black hole. A paper describing the analysis by the STScI team, led by Kailash Sahu, has been accepted for publication in The Astrophysical Journal.
Both teams used the same data: photometric measurements of the distant star's brightening as its light was distorted or "lensed" by the super-compact object, and astrometric measurements of the shifting of the distant star's location in the sky as a result of the gravitational distortion by the lensing object.
The photometric data came from two microlensing surveys: the Optical Gravitational Lensing Experiment, or OGLE, which employs a 1.3-meter telescope in Chile operated by Warsaw University, and the Microlensing Observations in Astrophysics, or MOA, experiment, which is mounted on a 1.8-meter telescope in New Zealand operated by Osaka University. The astrometric data came from NASA’s Hubble Space Telescope. STScI manages the science program for the telescope and conducts its science operations.
Because both microlensing surveys caught the same object, it has two names: MOA-2011-BLG-191 and OGLE-2011-BLG-0462, or OB110462, for short.
While surveys like these discover about 2,000 stars brightened by microlensing each year in the Milky Way galaxy, the addition of astrometric data is what allowed the two teams to determine the mass of the compact object and its distance from Earth. The UC Berkeley-led team estimated that it lies between 2,280 and 6,260 light years (700-1920 parsecs) away, in the direction of the center of the Milky Way Galaxy and near the large bulge that surrounds the galaxy's central massive black hole.
The STScI group estimated that it lies about 5,153 light years (1,580 parsecs) away.
Looking for a needle in a haystack
Lu and Lam first became interested in the object in 2020 after the STScI team tentatively concluded that five microlensing events observed by Hubble — all of which lasted for more than 100 days, and thus could have been black holes — might not be caused by compact objects after all.
Lu, who has been looking for free-floating black holes since 2008, thought the data would help her better estimate their abundance in the galaxy, which has been roughly estimated at between 10 million and 1 billion.
To date, star-sized black holes have been found only as part of binary star systems. Black holes in binaries are seen either in X-rays, produced when material from the star falls onto the black hole, or by recent gravitational wave detectors, which are sensitive to mergers of two or more black holes. But these events are rare.
"Casey and I saw the data and we got really interested. We said, 'Wow, no black holes. That's amazing,' even though there should have been," Lu said. "And so, we started looking at the data. If there were really no black holes in the data, then this wouldn’t match our model for how many black holes there should be in the Milky Way. Something would have to change in our understanding of black holes — either their number or how fast they move or their masses.”
When Lam analyzed the photometry and astrometry for the five microlensing events, she was surprised that one, OB110462, had the characteristics of a compact object: The lensing object seemed dark, and thus not a star; the stellar brightening lasted a long time, nearly 300 days; and the distortion of the background star's position also was long-lasting.
The length of the lensing event was the main tipoff, Lam said. In 2020, she showed that the best way to search for black hole microlenses was to look for very long events. Only 1% of detectable microlensing events are likely to be from black holes, she said, so looking at all events would be like searching for a needle in a haystack. But, Lam calculated, about 40% of microlensing events that last more than 120 days are likely to be black holes.
"How long the brightening event lasts is a hint of how massive the foreground lens bending the light of the background star is," Lam said. "Long events are more likely due to black holes. It's not a guarantee, though, because the duration of the brightening episode not only depends on how massive the foreground lens is, but also on how fast the foreground lens and background star are moving relative to each other. However, by also getting measurements of the apparent position of the background star, we can confirm whether the foreground lens really is a black hole."
According to Lu, the gravitational influence of OB110462 on the light of the background star was amazingly long. It took about one year for the star to brighten to its peak in 2011, then about a year to dim back to normal.
More data will distinguish black hole from neutron star
To confirm that OB110462 was caused by a super-compact object, Lu and Lam asked for more astrometric data from Hubble, some of which arrived last October. That new data showed that the change in position of the star as a result of the gravitational field of the lens is still observable 10 years after the event. Further Hubble observations of the microlens are tentatively scheduled for fall 2022.
Analysis of the new data confirmed that OB110462 was likely a black hole or neutron star.
Lu and Lam suspect that the differing conclusions of the two teams are due to the fact that the astrometric and photometric data give different measures of the relative motions of the foreground and background objects. The astrometric analysis also differs between the two teams. The UC Berkeley-led team argues that it is not yet possible to distinguish whether the object is a black hole or a neutron star, but they hope to resolve the discrepancy with more Hubble data and improved analysis in the future.
"As much as we would like to say it is definitively a black hole, we must report all allowed solutions. This includes both lower mass black holes and possibly even a neutron star," Lu said.
"If you can't believe the light curve, the brightness, then that says something important. If you don't believe the position versus time, that tells you something important," Lam said. "So, if one of them is wrong, we have to understand why. Or the other possibility is that what we measure in both data sets is correct, but our model is incorrect. The photometry and astrometry data arise from the same physical process, which means the brightness and position must be consistent with each other. So, there's something missing there. "
Both teams also estimated the velocity of the super-compact lensing object. The Lu/Lam team found a relatively sedate speed, less than 30 kilometers per second. The STScI team found an unusually large velocity, 45 km/s, which it interpreted as the result of an extra kick that the purported black hole got from the supernova that generated it.
Lu interprets her team's low velocity estimate as potentially supporting a new theory that black holes are not the result of supernovas — the reigning assumption today — but instead come from failed supernovas that don't make a bright splash in the universe or give the resulting black hole a kick.
The work of Lu and Lam is supported by the National Science Foundation (1909641) and the National Aeronautics and Space Administration (NNG16PJ26C, NASA FINESST 80NSSC21K2043).
Robert Sanders writes for the UC Berkeley News Center.
Administration of a decedent’s probate or trust estate may include sizable financial investment assets (e.g., brokerage accounts) and/or cash assets (e.g., bank accounts).
Brokerage account values change constantly and may include assets too risky and inappropriate given the administration.
The administration will need to determine how much cash is needed to pay debts of decedent, expenses of administration, and make gifts (typically at the end of administration).
On the other hand, too much uninvested cash (e.g., bank deposits) means unproductive assets that do not earn sufficient income and gradually lose value to inflation. This is increasingly problematic as months pass before distribution is made to beneficiaries.
A personal representative or trustee, as relevant, may want to invest cash assets, reinvest already invested assets, and/or to sell investments to create cash needed to pay debts, expenses, and make gifts to beneficiaries.
What investment powers does a personal representative in a probate or a trustee in a trust administration have to manage the decedent’s assets?
First let us consider the question in a probate. A personal representative is not required or expected to invest in the stock market.
The duties of a personal representative are that he or she must manage the estate assets with the care of a prudent person dealing with someone else's property. He or she must be cautious and may not make any speculative investments. Except for checking accounts intended for ordinary administration expenses, estate accounts must earn interest.
First, if the personal representative has full authority under the Independent Administration of Estates Act (“IAEA”), then he or she may invest in certain very low risk debt assets.
Next, with permission of the beneficiaries (and sometimes other persons too), the personal representative may also invest in certain additional low-risk debt instruments (e.g., bonds and obligations).
Second, if the probate involves a decedent’s will, the will may include investment powers. If so, the personal representative may invest using such powers, but only if certain important conditions safeguarding payment of the decedent’s debts and expenses of administration are first satisfied. This cannot occur earlier than four months from commencing probate. Sometimes it is necessary or advisable to obtain a court order for certain investments.
Next, in a trust administration, a trustee has a fiduciary (legal) duty to invest and manage trust assets impartially for the benefit of all beneficiaries.
Generally, the trustee must make all assets economically productive, unless the trust provides otherwise. The duty to make assets income producing becomes increasingly important the longer the trust administration takes and the larger the value of the trust estate.
In all events, however, the trustee must evaluate the suitability of the risks and returns associated with the existing investments in the contest of the trust administration.
The trustee’s investment powers are found, first, in the trust itself and, secondarily, in the Probate Code. A trust may expand or restrict the trustee’s standard duties and limitations in the Probate Code. Generally speaking, a trustee may invest in assets that are often off limits in a probate administration.
California’s prudent investor rule requires a trustee to consider the trust’s purposes, terms, distribution requirement and other relevant circumstances when establishing an overall investment strategy.
Investment decisions — including the balancing of investment risk with investment return goals — must be made in the context of an overall investment strategy. No one asset is considered in isolation and investment diversity is the general rule.
Under the prudent investor rule, a trustee can delegate investment decisions to a professional investment advisor. If the trustee follows the following three rules the trustee will not be liable to beneficiaries for following the investment advice: (1) The trustee must select the advisor prudently; (2) trustee must establish the scope and terms of the delegation consistent with the purposes and terms of the trust; and (3) the trustee must periodically monitor the advisor’s performance and compliance with the delegation.
Selecting an advisor prudently means interviewing several different advisors and considering each advisor’s credentials, experience investing trust assets in similar situations, and any possible conflicts of interest. This process should be documented.
The foregoing is not legal or investment advice. Anyone confronting these issues in the administration of a decedent’s estate should seek appropriate legal and investment counsel before proceeding.
Dennis A. Fordham, attorney, is a State Bar-Certified Specialist in estate planning, probate and trust law. His office is at 870 S. Main St., Lakeport, Calif. He can be reached at This email address is being protected from spambots. You need JavaScript enabled to view it. and 707-263-3235.
Emily Brant, University of Pittsburgh Health Sciences and Kristina E. Rudd, University of Pittsburgh Health Sciences
Can an otherwise healthy young woman die from what starts out as something akin to a common cold? The answer is, shockingly, yes, when certain telltale signs of a more serious problem go undetected.
Though many people haven’t even heard of it, sepsis – the body’s extreme response to infection – is the leading killer of hospitalized patients in the United States. Worldwide, sepsis is responsible for 1 in 5 deaths every year. Even among those who survive, many will never be able to return to work, and some won’t be able to return home from the hospital, requiring life support or ongoing critical care.
We are two researchers and critical care doctors at the University of Pittsburgh School of Medicine who are working to change the way scientists and doctors think about sepsis. We are interested in understanding and spreading awareness about how sepsis starts and how it can elude even the most astute physicians.
We are also learning more about how community factors are at play and how a better understanding of the communities we all live in could help everyday people and health care workers alike recognize and stop this deadly disease.
What is sepsis?
Sepsis is a medical emergency that begins with an infection – perhaps even a mild infection. Upon detecting bacteria or a virus, your body releases a choreographed cascade of chemicals into the bloodstream. This chemical alert beckons an artillery of immune cells that work in concert to fight the bug.
When this system works well, your body clears the infection and you get better. But when the system doesn’t work well, sepsis can ensue.
The onset of sepsis occurs when your immune cells pivot from fighting the infection to fighting your own tissues and organs. This reaction can be similar to an autoimmune response, a condition in which the body’s immune system turns on itself. Many people are familiar with chronic autoimmune diseases such as rheumatoid arthritis or Crohn’s disease, but sometimes this type of autoimmune response can occur even in healthy people.
When sepsis occurs, the immune system can commonly injure the heart, lungs, kidneys or blood cells, among other important body systems. Inflammation in the blood vessels can make them leaky, causing blood flow to the brain and other organs to become severely diminished. When this occurs, a person’s blood pressure may become dangerously low, which is a severe form of sepsis known as septic shock.
Without prompt and proper treatment – and sometimes even despite treatment – sepsis can cause organ damage and even death. Once shock develops, mortality from sepsis is estimated to jump from 10% to as high as 40%.
Sepsis can result from nearly any infection. Most commonly it develops from pneumonia or a urinary tract infection. Severe COVID-19 can also cause sepsis. Often, sepsis patients are seen by a medical professional for infection symptoms in the week preceding sepsis hospitalization. However, predicting which infected patients will go on to develop sepsis is very difficult.
Treatment options
The cornerstones of sepsis treatment are prompt recognition of sepsis symptoms, followed by antibiotics and fluids. But even the most careful and attentive physicians can miss the early signs of sepsis.
This is largely because there is no single test to positively diagnose sepsis. Sepsis symptoms may mimic other life-threatening conditions such as heart attacks, blood clots, bleeding or even an allergic reaction. Patients often display vague and variable symptoms such as weakness, lightheadedness and rapid breathing, making the diagnosis even more challenging.
For example, a young, otherwise healthy person with sepsis due to pneumonia may look much different from an older diabetic who develops sepsis from a smoldering skin infection.
Sepsis patients nearly always require admission to the hospital or even the ICU, and those with severe forms of sepsis often require life support. This may include dialysis or mechanical ventilation to support failing organs. The source of infection needs to be identified and, in some cases, surgically removed. Delaying sepsis treatment by even a few hours can have deadly consequences.
Recognizing sepsis before it’s too late
Differences in sepsis go beyond symptoms. COVID-19 has laid bare that severe illness isn’t a game of chance. Like COVID-19 infection, sepsis susceptibility – and who is most likely to get sick and die – is part of a complex interplay of social influences that include racism, poverty, geography and community dynamics.
Research strongly suggests that certain people are at far higher risk of developing sepsis than others. Much like COVID-19, older people with underlying chronic diseases like obesity and diabetes face a heightened risk for sepsis. Such factors as race, poverty and even driving distance to the hospital may have a significant impact on who survives sepsis.
Most of the work done to improve sepsis detection and treatment has focused on the hospital setting. Doctors, researchers and even government agencies have concentrated their efforts on improving sepsis recognition and treatment once a patient reaches the hospital. Research aimed at understanding an individual’s sepsis risk has focused on personal health history and social and economic factors such as income and race, or community features such as primary care access.
While these approaches have advanced the field’s understanding of sepsis, they have led to little progress in reducing the incidence of sepsis in the U.S.
New approaches to catching a killer
Given what is known about the importance of early sepsis treatment, researchers like us are taking a closer look at the role of communities in improving sepsis detection and understanding sepsis risk.
The early stages of sepsis can evolve rapidly when a patient is at home. Scientists estimate that 87% of sepsis cases start outside the hospital. When a patient does present for care, it’s often in a clinic or emergency medical services setting in the days and even hours preceding sepsis hospitalization. These critical treatment windows may mean the difference between life and death for a sepsis patient.
Alongside researchers based at Kaiser Permanente Northern California, we are now working to advance sepsis care by studying sepsis patient symptoms, community factors, diagnosis and treatment patterns outside the hospital. We are also expanding work to improve sepsis diagnosis among hospitalized patients. This coast-to-coast collaboration will study patients cared for at over 40 hospitals, 30 EMS agencies and a critical mass of ambulatory clinics. We hope that our work will shed light on the early stages of sepsis, including signs that may signal that an infected patient is progressing to sepsis, and explore diagnostic and treatment approaches that could help stop sepsis before it advances too far.
We are also learning a great deal more about the complicated role of community factors like poverty on health outcomes, including sepsis. Using “syndemic theory” – a framework to describe synergistic epidemics that arise from harmful social conditions – we are studying how two co-occurring epidemics, like poverty and asthma, can work together to increase negative health outcomes. Though this framework is only beginning to be used to study acute illness, it has the potential to transform the way we think about sepsis.
LAKE COUNTY, Calif. — The Lake County Registrar of Voters Office reported Friday on the work taking place to finalize the official canvass for Tuesday’s primary election, including counting thousands of unprocessed ballots.
Registrar Maria Valadez’s office said the results from the June 7 Statewide Direct Primary Election results are not yet final.
As is normal after an election, Valadez’s office still has thousands of ballots to process, with more expected to arrive in the mail by Tuesday.
As of June 8 report, Valadez’s office has the following ballots yet to count within the 30-day official canvass period:
• Vote-by-mail ballots: 7,523. • Provisional ballots: 830. • Conditional voter registration provisional ballots: 39. • Vote-by-mail ballots that require further review for various reasons: 149. • Grand total: 8,541.
A newly enacted law changed the deadline for elections officials to receive vote-by-mail ballots returned by mail for the June 7 primary, the elections office reported.
The new law allows county elections officials to count a vote-by-mail ballot if it is postmarked on or before Election Day and delivered to the elections office by the U.S. Postal Service or a private mail delivery company no later than seven days after Election Day, in this case, June 14.
Official canvass and vote-by-mail processing
The registrar’s office reported that there are many checks and balances when certifying the election results.
The process of certifying election results, also known as the official canvass, is mandated by state law to make sure the public can have confidence in the integrity of the final results.
Unofficial results have no bearing on the final outcome of the races and contests. Only final certified results will impact the races and contests.
Valadez reported that her staff members are working very diligently on completing all tasks required to certify the election.
Each voter’s returned vote-by-mail ballot envelope must be examined by staff to see if the signature compares with the voter’s signature on file. After the vote-by-mail voter’s information has been entered and proofed; the vote-by-mail envelopes have to be sorted by voting precinct.
Staff must verify the number of vote-by-mail processed by the voting precinct before the envelopes can be opened. Once staff balances, the envelopes can be opened. Once the ballots are removed, staff must count the number of ballots and the number of envelopes in order to make sure that all of the ballots are removed from the envelopes to be counted.
“Polls provisional ballots” are cast at the polling places on Election Day. Some of the reasons a voter is issued a provisional ballot:
• The voter’s name is listed on the active voter roster list as a vote-by-mail voter and the voter is unable to surrender his/her vote-by-mail ballot in order to be issued a polls ballot. • The voter’s name is not printed in the roster-index, has moved and did not re-register to vote at his/her new residence address. • A voter is voting in the wrong voting precinct and not his/her assigned voting precinct. • A first time voter who is required to provide ID, but is unable to do so. • The voter’s eligibility to vote cannot be determined by the poll worker.
“Conditional voter ballots” issued to a person personally visiting either the Lake County Registrar of Voters or a voting precinct no later than the close of the polls (prior to 8 p.m.) on Election Day. These voters are Lake County residents who missed the regular voter registration deadline of May 23 but they still have the option to vote in an election by conditionally registering to vote and casting a conditional ballot (same day voter registration).
Voters that were able to surrender their vote-by-mail ballot, were allowed to sign the Roster-Index and were issued a ballot at their assigned polling place, and then their voted ballot was deposited into the ballot box.
After the polls closed, the voted precinct ballots were returned to the Registrar of Voters Office and counted on election night.
In addition, all of the roster-indexes must also be examined for errors or omissions. Staff checks the ballot statement including the number of returned voted ballots against the number of voters who signed the roster-index.
Provisional and conditional voter signatures also need to match the number of voter provisional and conditional ballots.
Once this is done, staff must enter voter history from each of the roster-indexes and record it into the voting system as voter history.
For additional information call the Registrar of Voters Office at 707-263-2372 or toll-free at 888-235-6730.
After a decade of observing some of the hottest, densest, and most energetic regions in our universe, this small but powerful space telescope still has more to see.
NASA’s Nuclear Spectroscopic Telescope Array, or NuSTAR, is turning 10. Launched on June 13, 2012, this space telescope detects high-energy X-ray light and studies some of the most energetic objects and processes in the universe, from black holes devouring hot gas to the radioactive remains of exploded stars. Here are some of the ways NuSTAR has opened our eyes to the X-ray universe over the last decade.
Seeing x-rays close to home
Different colors of visible light have different wavelengths and different energies; similarly, there is a range of X-ray light, or light waves with higher energies than those human eyes can detect. NuSTAR detects X-rays at the higher end of the range.
There aren’t many objects in our solar system that emit the X-rays NuSTAR can detect, but the Sun does: Its high-energy X-rays come from microflares, or small bursts of particles and light on its surface. NuSTAR’s observations contribute to insights about the formation of bigger flares, which can cause harm to astronauts and satellites.
These studies could also help scientists explain why the Sun’s outer region, the corona, is many times hotter than its surface. NuSTAR also recently observed high-energy X-rays coming from Jupiter, solving a decades-old mystery about why they’ve gone undetected in the past.
Illuminating black holes
Black holes don’t emit light, but some of the biggest ones we know of are surrounded by disks of hot gas that glow in many different wavelengths of light. NuSTAR can show scientists what’s happening to the material closest to the black hole, revealing how black holes produce bright flares and jets of hot gas that stretch for thousands of light-years into space.
The mission has measured temperature variations in black hole winds that influence star formation in the rest of the galaxy. Recently, the Event Horizon Telescope, or EHT, took the first-ever direct images of the shadows of black holes, and NuSTAR provided support.
Along with other NASA telescopes, NuSTAR monitored the black holes for flares and changes in brightness that would influence EHT’s ability to image the shadow cast by them.
One of NuSTAR’s biggest accomplishments in this arena was making the first unambiguous measurement of a black hole’s spin, which it did in collaboration with the European Space Agency, or ESA, XMM-Newton mission.
Spin is the degree to which a black hole’s intense gravity warps the space around it, and the measurement helped confirm aspects of Albert Einstein’s theory of general relativity.
Finding hidden black holes
NuSTAR has identified dozens of black holes hidden behind thick clouds of gas and dust. Visible light typically can’t penetrate those clouds, but the high-energy X-ray light observed by NuSTAR can. This gives scientists a better estimate of the total number of black holes in the universe.
In recent years scientists have used NuSTAR data to find out how these giants become surrounded by such thick clouds, how that process influences their development, and how obscuration relates to a black hole’s impact on the surrounding galaxy.
Revealing the power of ‘undead’ stars
NuSTAR is a kind of zombie hunter: It’s deft at finding the undead corpses of stars. Known as neutron stars, these are dense nuggets of material left over after a massive star runs out of fuel and collapses.
Though neutron stars are typically only the size of a large city, they are so dense that a teaspoon of one would weigh about a billion tons on Earth. Their density, combined with their powerful magnetic fields, makes these objects extremely energetic: One neutron star located in the galaxy M82 beams with the energy of 10 million Suns.
Without NuSTAR, scientists wouldn’t have discovered just how energetic neutron stars can be. When the object in M82 was discovered, researchers thought that only a black hole could generate so much power from such a small area.
NuSTAR was able to confirm the object’s true identity by detecting pulsations from the star’s rotation – and has since shown that many of these ultraluminous X-ray sources, previously thought to be black holes, are in fact neutron stars. Knowing how much energy these can produce has helped scientists better understand their physical properties, which are unlike anything found in our solar system.
Solving supernova mysteries
During their lives, stars are mostly spherical, but NuSTAR observations have shown that when they explode as supernovae, they become an asymmetrical mess.
The space telescope solved a major mystery in the study of supernovae by mapping the radioactive material left over by two stellar explosions, tracing the shape of the debris and in both cases revealing significant deviations from a spherical shape.
Because of NuSTAR’s X-ray vision, astronomers now have clues about what happens in an environment that would be almost impossible to probe directly. The NuSTAR observations suggest that the inner regions of a star are extremely turbulent at the time of detonation.
More about the mission
NuSTAR launched on June 13, 2012. The mission’s principal investigator is Fiona Harrison, chair of the Division of Physics, Mathematics, and Astronomy at Caltech in Pasadena, California.
A Small Explorer mission managed by the agency’s Jet Propulsion Laboratory in Southern California for NASA’s Science Mission Directorate in Washington, NuSTAR was developed in partnership with the Danish Technical University, or DTU, and the Italian Space Agency, or ASI.
The telescope optics were built by Columbia University, NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and DTU.
The spacecraft was built by Orbital Sciences Corp. in Dulles, Virginia. NuSTAR’s mission operations center is at the University of California, Berkeley, and the official data archive is at NASA’s High Energy Astrophysics Science Archive Research Center. ASI provides the mission’s ground station and a mirror data archive. Caltech manages JPL for NASA.
May was warm and wet across the Lower 48, according to scientists from NOAA’s National Centers for Environmental Information.
The month also wrapped up a warm spring as wildfires continued to burn across the nation.
Below are highlights from NOAA's U.S. monthly climate report for May 2022:
Climate by the numbers
May 2022
The average May temperature across the contiguous U.S. was 61.9 degrees F (1.7 degrees above the 20th-century average), ranking in the warmest third of the 128-year record.
Temperatures across the Northwest and northern Rockies were below average, with much of the Southwest, Deep South and locations east of the Mississippi River above average. Triple-digit heat scorched portions of the South throughout the month, setting a number of temperature records across Texas. Texas had its second-warmest May on record, while Washington state saw its eighth coldest.
The average precipitation for May was 3.17 inches (0.26 of an inch above average), which ranked in the wettest third of the record.
Precipitation was above average across portions of the Northwest, northern and central Plains, Upper Mississippi Valley, Ohio Valley, eastern Gulf of Mexico and the Appalachians. Precipitation was below average from California to Texas and across portions of the Northeast. A dry month across the Southwest resulted in Arizona seeing its fifth-driest May on record, while above-average precipitation gave Washington state its eighth-wettest May.
Meteorological spring (March through May 2022) | Year to date
The average temperature for the contiguous U.S. during meteorological spring was 52.2 degrees F (1.3 degrees F above average), which ranked in the warmest third of the record. Rhode Island ranked fourth warmest while nine additional states — Arizona, Connecticut, Florida, Maine, Massachusetts, New Hampshire, New Jersey, New Mexico and Texas — ranked among their ten-warmest spring seasons on record.
The spring precipitation total of 8.07 inches (0.13 of an inch above average) placed it in the middle third of the record. North Dakota ranked fourth wettest while New Mexico saw its sixth-driest spring.
The average U.S. temperature for the year to date (YTD, January through May) was 44.3 degrees F, 1.0 degree F above average, ranking in the warmest third of the record.
The first five months of 2022 were also quite dry, with a precipitation total of 11.48 inches, 0.91 of an inch below average, and ranking in the driest third of the record. California saw its driest such YTD on record while Arizona, Nevada and Utah ranked third driest for this five-month period. Meanwhile, North Dakota saw its fourth-wettest YTD.
Other notable highlights from the report
Wildfires roared across the landscape: As of May 31, the largest fire in New Mexico history, the Hermits Peak Fire, had consumed more than 315,000 acres and was 50% contained. Across all 50 states, 1.9 million acres have burned from January 1 through June 2 — more than twice the average for this time of year.
Drought improved overall, with exceptions: According to the May 31 U.S. Drought Monitor reportoffsite link, 49.3% of the contiguous U.S. was in drought, down about 4.5% from the beginning of May. Areas of the Pacific Northwest, northern Rocky Mountains and High Plains saw drought conditions improve over the month of May while drought intensified or expanded across the Southwest, West and parts of the Northeast.
A stormy May with fewer tornadoes: Several rounds of severe weather hit the U.S. during May, producing 196 preliminary tornado reports. This is 71% of the 1991-2010 average for tornadoes for the month of May (276). On May 4, severe storms formed across the central Plains and produced several tornadoes including an EF3 tornado near Lockett, Texas. A line of severe storms, also known as a derecho, barreled across the central Plains into the Upper Midwest on May 12, causing extensive damage from at least 13 tornadoes and straight-line winds.
LAKE COUNTY, Calif. — Lake County’s Public Health officer said the case rate of COVID-19 in the county is now significant enough to land it within the “high” community level outlined by the U.S. Centers for Disease Control and Prevention.
“Reaching this category, the worst of the agency’s three-tier scale is alarming, as it signifies abundant local transmission which could signal that our community may soon put pressure on our health care resources,” said Dr. Erik McLaughlin, MD, MPH.
“As members of this community, we must take it upon ourselves to change our current trajectory by adhering to safety practices that are known to reduce transmission of COVID-19 such as wearing face coverings indoors when in public, testing when symptomatic or recently exposed, and staying up to date on vaccinations,” McLaughlin said.
McLaughlin said that moving into the CDC’s High Community Level does not trigger any new countywide health measures, however, it signals that reassessing measures may become necessary in order to avoid devastating outcomes if case rates continue to rise.
Although an indoor face covering requirement hasn’t been necessary for months, county health officials have consistently strongly recommended residents wear face coverings indoors while in public as an extra layer of protection against COVID-19 transmission.
McLaughlin said health officials do not want these recommendations and requirements to be seen as a punishment but as a powerful tool in avoidance of more severe outcomes.
He said officials have long noted that the pandemic has plotted a predictable, if painful, path — with increases in new infections triggering corresponding rises in hospitalizations a few weeks later, and in deaths a few weeks after that.
Lake County Health Services data analysis shows the county is now reporting 212 weekly cases for every 100,000 residents, high enough to clear the bar of 200 the CDC has set for the high community level.
Test positivity has been creeping upward over recent weeks to 11% in Lake County, McLaughlin said.
“The task in front of us is similar to work we’ve had to do at other points over the past two and a half years, we must slow transmission,” McLaughlin said. “We know what works — masking, testing and vaccination, along with systems and policies that support the use of these and other effective safety measures.”
He added, “Our hope is that with the encouragement that we’re providing, the easy access to high-quality face coverings, that people will go back to putting those face coverings on while transmission is high.”
LAKE COUNTY, Calif. — The District Attorney’s Office has charged a Cobb man with numerous felony charges for a shooting that occurred after an early Tuesday morning fight at a barbecue.
Hunter Christian Toles, 23, appeared before Judge Andrew Blum in Lake County Superior Court for arraignment on the charges Thursday afternoon.
He was arrested early Tuesday after the shooting, which occurred on Rainbow Road in Cobb, the Lake County Sheriff’s Office reported.
Toles, who has remained in custody since his arrest, appeared via Zoom from the Lake County Jail.
Chief Deputy District Attorney Richard Hinchcliff told the court that Toles has no prior criminal history and that the investigation is ongoing.
Based on the reports so far and speaking to the lead officer in the investigation, Hinchcliff said Toles was at a barbecue where people were drinking and a fight broke out.
Toles is reported to have grabbed a shotgun and fired three shots. One of the shots hit a female victim at close range. Hinchcliff didn’t have a report on her condition. While it wasn’t terminal, “she was shot up pretty good,” he added.
Another shot went through a wall where there was a 3-year-old child sleeping on the other side, Hinchcliff said.
Hinchcliff filed a complaint on Thursday that charged Toles with attempted murder, assault with a firearm and battery causing serious bodily injury for shooting the woman, along with special allegations of personally and intentionally discharging a firearm, personal use of a shotgun and inflicting great bodily injury on the female victim.
Charges also were filed against Toles for another adult victim who was not reported to have been physically injured. For that second victim he’s facing charges of attempted murder and assault with a firearm, and special allegations of personal use of a firearm and personally and intentionally discharging a shotgun.
For the child victim, he was charged with assault with a firearm and felony child endangerment, and special allegations of use of a firearm and that the crime involved great violence and a firearm, and that the victim was particularly vulnerable.
Blum said during the hearing that Toles is facing the potential of three life sentences if convicted of the charges.
Hinchcliff said several of the charges carried $1 million bail requirements, with $25,000 for the child victim. Altogether, the charges called for bail totaling $3,025,000.
Toles said he could not afford an attorney and asked for one to be assigned. Defense attorney Tom Quinn agreed to take the case and asked for it to be set for entry of a plea on Tuesday.
Toles wanted to speak about his case but Quinn told him not to say anything.
“The defendant is claiming self-defense,” Hinchcliff said.
The mother of Toles’ two young children asked Blum to reduce his bail or release him on his own recognizance. Quinn said no one would get such a release on a case like this one.
She told the court the charges filed against him were different from those on his online jail booking sheet.
“The sheriff doesn’t make charges. They arrest people,” said Blum.
Quinn said they might be able to get the bail reduced to $100,000 but couldn’t do that in the Thursday hearing. Toles’ partner said she had money to hire an attorney the same day.
Blum set Toles’ bail at $3,025,000 and ordered him to be present for plea entry in Department 3 at 10 a.m. Tuesday, June 14.
Email Elizabeth Larson at This email address is being protected from spambots. You need JavaScript enabled to view it.. Follow her on Twitter, @ERLarson, or Lake County News, @LakeCoNews.