Science Release: 4 June 2020 — noirlab2012es
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Science Release: 7 May 2020 — noirlab2011
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Mollit qui qui laborum nulla quis nisi esse reprehenderit eiusmod nostrud nisi quis ea cupidatat. Mollit tempor ea nostrud ad quis. Lorem nostrud laborum nostrud adipisicing incididunt excepteur irure pariatur. Reprehenderit nisi velit laborum quis sint laboris. Proident Lorem cillum Lorem Lorem duis mollit ex duis fugiat amet duis quis quis. Dolore aliquip fugiat Lorem nulla culpa consectetur in proident anim tempor deserunt veniam dolore. Veniam voluptate et sint cillum minim. Elit culpa culpa laborum aliquip officia dolor exercitation nulla veniam irure labore voluptate enim. Occaecat proident proident exercitation irure elit nulla nulla. Non sit adipisicing aliquip aute aliqua. Magna reprehenderit occaecat laboris aliquip fugiat cupidatat reprehenderit et ea. Aliqua ea commodo aliqua duis laborum officia fugiat culpa ea est esse sit adipisicing. Aute sit nulla dolor voluptate officia voluptate veniam adipisicing dolor sunt nostrud amet do. Esse est elit commodo aliqua minim qui non ullamco id amet deserunt ullamco enim magna. Et irure dolor labore laboris occaecat do duis. Officia dolor tempor incididunt ad aliqua adipisicing cupidatat eu officia ad. Reprehenderit qui cupidatat nisi incididunt ea do et proident enim dolor. Duis aliquip ipsum eiusmod dolore dolore id adipisicing ex cillum magna.
Photo Release: 16 April 2020 — noirlab2010
Small but Mighty
Barnard’s Galaxy, a dwarf galaxy neighboring the Milky Way, is revealed in this stunning image from the Victor. M. Blanco 4-m telescope at the Cerro Tololo Inter-American Observatory, a program of NSF’s NOIRLab. The image reveals regions of intense star formation and a scattering of immense cosmic bubbles.
Science Release: 14 April 2020 — noirlab2009
Researchers using the Gemini North telescope on Hawaiʻi’s Maunakea have detected the most energetic wind from any quasar ever measured. This outflow, which is travelling at nearly 13% of the speed of light, carries enough energy to dramatically impact star formation across an entire galaxy. The extragalactic tempest lay hidden in plain sight for 15 years before being unveiled by innovative computer modeling and new data from the international Gemini Observatory.
Organization Release: 3 April 2020 — noirlab2008
Nighttime U.S. / International Astronomy Gets New Identity
NSF’s National Optical-Infrared Astronomy Research Laboratory, which in 2019 brought together NSF’s optical and infrared nighttime astronomy under one entity, will now go by the shortened name of NSF’s NOIRLab (no-wah-lab), abbreviated from its longer formal name. NOIRLab is headquartered in Tucson, Arizona and operates Kitt Peak National Observatory, the international Gemini Observatory, the Community Science and Data Center, Cerro Tololo Inter-American Observatory, and the operations of the Vera C. Rubin Observatory.
Coronavirus COVID-19 Measures at NOIRLab
After an internal Operations Restart Readiness Review, Gemini-North in Hawai‘i has been given the green light to restart night-time observations on the night of 19 May.
NOIRLab response to #ShutDownSTEM
#ShutDownSTEM, Wednesday 10 June 2020, is a day of international protest of systemic racism in research and academia. STEM and research professionals are asked to stop their normal activities of research, teaching and meetings for one day, in the wake ...
Joan Najita from NOIRLab Awarded John Simon Guggenheim Fellowship
Joan Najita from NSF’s NOIRLab, headquartered in Tucson, has been awarded a John Simon Guggenheim Fellowship in astronomy & astrophysics for 2020. Guggenheim Fellows are appointed on the basis of past achievement and exceptional promise for future ...
North American Regional Office of Astronomy for Development Launched
The North American Regional Office of Astronomy for Development (NA ROAD) became a reality today at a signing ceremony in Cape Town, South Africa. This milestone brings the vision of the global Office of Astronomy for Development (OAD) to North America...
2020 Breakthrough Prize Awarded to Event Horizon Telescope Team
The 347-person team that made the first image of a supermassive black hole has been awarded the Breakthrough Prize in Fundamental Physics, one of the “Oscars of Science.” By synchronizing 8 radio telescopes, the team created a virtual telescope the siz...
Revealing the Intimate Lives of MASSIVE Galaxies
Every galaxy has a story, and every galaxy has been many others in the past (unlike for humans, this is not purely metaphorical, as galaxies grow via hierarchical assembly). Generally speaking, the most massive galaxies have led the most interesting li...
A Whirlpool Warhol
It all depends on how you look at it—galaxies appear different in visible light (i.e., wavelengths that our eyes are sensitive to) than at longer wavelengths, in the infrared. In visible light (panel a), the Whirlpool galaxy M51 and its companion show ...
Discovering Patterns in Io's Volcanoes
Jupiter’s volcanic moon Io brought astronomers and geologists together to reveal that this moon’s hot spots fluctuate on unexpected timescales.
The team utilized the Gemini North telescope and the W.M. Keck Observatory, both located on Maunakea, Hawai...
What’s Your Moonshot?
To celebrate the 50th anniversary of the moon landing, Newsweek is highlighting pioneers in science and technology, their moonshots, and how they hope to change the world. This week’s issue features NOAO Astronomer Aaron Meisner, who describes the insp...
Einstein's General Relativity Illustrated by a Single Star
By observing a single star orbiting around the supermassive black hole at the center of our Milky Way Galaxy, a team of astronomers have tested Einstein’s one hundred-year-old theory of General Relativity in an unprecedented new regime. Unlike Sir Isaa...
New Sky Surveys Set the Stage for Dark Energy Experiment
Three new imaging surveys pave the way for an upcoming spectroscopic experiment, the Dark Energy Spectroscopic Instrument (DESI), which will explore the role of dark energy in the expansion history of the Universe. Images from the surveys, which were c...
Is the Mystery of the Dark Matter Deficient Galaxy Resolved?
To have, or not to have dark matter? That is the question.
In early 2018, a team of researchers led by Pieter van Dokkum of Yale University shook up the astrophysics world when they announced that the dwarf, “ultra-diffuse galaxy,” which was referred ...
LSST Mirror Arrives at Cerro Pachón
The 8.4m-diameter primary mirror of the Large Synoptic Survey Telescope (LSST) has reached its home at Cerro Pachón in Chile. Earlier this month, the mirror reached the port at Coquimbo, where it was loaded onto a 72-wheeled transport vehicle for the t...
Mystery of the Universe’s Expansion
New results from the Hubble Space Telescope confirm that the Universe today is expanding faster than expected, based on how the Universe appeared 13 billion years ago. Possible explanations for the discrepancy include a surprise appearance of dark ener...
Two New Planets Discovered Using Artificial Intelligence
Using an artificial intelligence algorithm to sift through massive amounts of data from NASA’s Kepler Space Telescope, a team of astronomers, led by an undergraduate at UT Austin, has discovered two new exoplanets. The planets are “super-Earths” — plan...
Making Good Use of Bad Weather: Finding Metal-poor Stars Through the Clouds
The Gemini telescopes helped identify low-metallicity stars by gathering medium-resolution spectroscopic GMOS data for 666 bright stars under poor weather conditions. These data provide a unique opportunity to explore the chemical evolution of the Mil...
Seeing the ‘Unseeable’
Observations made with the Event Horizon Telescope, a planet-scale array of eight ground-based radio telescopes, have captured the first picture of a supermassive black hole. The black hole appears as a bright ring as it gravitationally bends the light...
Dark Energy Spectroscopic Instrument’s Lenses See First Light
On April 1, the Mayall telescope at Kitt Peak emerged from hibernation—its dome reopened to the night sky, and starlight poured through the six large lenses of its powerful new research tool: the Dark Energy Spectroscopic Instrument (DESI). Early next ...
11 June 2020 — iotw2024
3 June 2020 — iotw2023
Silver Galactic Sliver
27 May 2020 — iotw2022
Larger than Life
20 May 2020 — iotw2021
Dazzling in the dark
6 May 2020 — iotw2019
A (Galactic) Arm’s Length Away
29 April 2020 — iotw2018
An Insider’s View
22 April 2020 — iotw2017
15 April 2020 — iotw2016
WIYN Enveloped by Celestial Aura
8 April 2020 — iotw2015
Sunlight Paints a Crimson Sky Over Gemini South
1 April 2020 — iotw2014
A Backdrop of Blue and Red
From the first observations in 1965, Cerro Tololo, located in Chile, has served as the principal platform for U.S. astronomical investigation of the southern skies.
Programs within the Community Science and Data Center support and enable a broad range of astronomical community science activities across the US ground-based optical and infrared system.
Founded in 1958, Kitt Peak National Observatory is home to one of the largest arrays of optical and radio telescopes in the world.
The Gemini Observatory consists of twin 8.1-meter diameter optical/infrared telescopes located on two of the best observing sites on the planet.
Vera C. Rubin Observatory, currently under construction on Cerro Pachón in Chile, is an 8-meter-class telescope coupled to a 3.2-gigapixel camera – the world’s largest digital camera ever fabricated for optical astronomy.