It covers a 37" x 37" solid angle with 2,400 optical fibers efficiently coupled by a double-sided microlens-array, producing R = 2, 000 spectra with 0.7511 spatial resolution. The Large Lenslet Array Magellan Spectrograph (LLAMAS) is an NSF-funded facility-class Integral Field Unit (IFU) spectrograph under construction for the 6.5-meter Magellan Telescopes. This paper describes the development status of the project. The project has passed the Final Design Review and is currently in manufacturing and integration phase. Besides of the consortium programs on guaranteed time, the instrument is offered to the ESO community for any kind of astrophysical target. It will also have the scope to observe active galactic nuclei and blazars, tidal disruption events, fast radio bursts, and more. SOXS will study a mixture of transients encompassing all distance scales and branches of astronomy, including fast alerts (such as gamma-ray bursts and gravitational waves), mid-term alerts (such as supernovae and X-ray transients), and fixed-time events (such as the close-by passage of a minor planet or exoplanets). ![]() It will provide a key spectroscopic partner to any kind of imaging survey, becoming one of the premier transient follow-up instruments in the Southern hemisphere. ![]() The consortium is focussed on a clear scientific goal: the spectrograph will observe all kind of transient and variable sources discovered by different surveys with a highly flexible schedule, updated daily, based on the Target of Opportunity concept. SOXS (Son Of X-Shooter) is a single object spectrograph, characterized by offering a wide simultaneous spectral coverage from U- to H-band, built by an international consortium for the 3.6-m ESO New Technology Telescope at the La Silla Observatory, in the Southern part of the Chilean Atacama Desert. We also review recent changes in nighttime operations at the observatory in response to the COVID-19 pandemic and plans for the implementation of the Health and Instrument Performance plan for the Observatory (HIPO), a program to proactively monitor the health and stability of the facility instruments. We discuss the ”binocular lifestyle” including the unique challenges of using LBT in three ways: Duplex mode, with identical configurations on both sides (effectively an 11.8 meter mirror) Fraternal Twin (same instruments with different configurations) or Mixed mode, (different instruments on each side) which gives observers two 8.4 meter telescopes to use or 22.65 meters in interferometry (LBTI) mode. Recently, the Potsdam Echelle Polarietric and Spectroscopic Instrument (PEPSI), a fiber-fed high resollution optical echelle spectrograph with polarimetry capabilities, has transitioned from a Principal Investigator (PI) instrument to a facility instrument. These include: the prime-focus optical Large Binocular Cameras (LBCs) optical Multi-Object Double Spectrograph (MODS) for imaging and spectroscopy and the two LBT Utility Camera in the Infrared (LUCIs) for imaging and spectroscopy, which include the commissioning of the Single conjugated adaptive Optics Upgrade for LBT (SOUL). Inquiries may be sent to M.Presented here is a review of the status of facility instruments at the Large Binocular Telescope Observatory (LBTO). ![]() ![]() If you find your name, you may file a claim on the Department's web site at From this site, you may download a claim form with instructions to file your claim or track progress of your claim online. The following list of Unclaimed Property Owners was reported and delivered to the Department. Common types of unclaimed property are savings or checking accounts, stocks, dividends, checks that have not been cashed such as payroll, certificates of deposit, unclaimed insurance benefits, insurance premium refunds, and the like. 20-1603 NOTICES DEPARTMENT OF TREASURY Unclaimed Property OwnersĮach year, the Treasury Department (Department) receives millions of dollars in unclaimed property.
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