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US National Gemini Office

@usngo.bsky.social
1.2K followers 417 following 1.2K posts

The US NGO at NSF NOIRLab supports Gemini Observatory users in the stages of the astronomical observing cycle, from proposal to data reduction. Visit our website at noirlab.edu/science/programs/csdc/u….

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US National Gemini Office @usngo.bsky.social · 16h
Queue programs observed at Gemini Observatory N/S on 10/08/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 16h
Credit: International Gemini Observatory/NOIRLab/NSF/AURA/T. A. Rector (University of Alaska Anchorage)
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US National Gemini Office @usngo.bsky.social · 16h
The Long-period Spectroscopic Orbit and Dust Creation in the Wolf─Rayet Binary System WR 125, by Noel D. Richardson et al. 2024 ui.adsabs.harvard.edu/abs/2024ApJ....
A scatter plot showing radial velocity versus orbital phase. The vertical y-axis is labeled "RADIAL VELOCITY (km s^-1)" and ranges from 0 to over 80. The horizontal x-axis is labeled "ORBITAL PHASE" with tick marks at 0.0, 0.5, and 1.0. A continuous, wave-like solid black curve is fitted to the data, peaking around phase 0.3 (roughly 85 km/s) and reaching a minimum near phase 0.9 (roughly 18 km/s). The plot includes data points with vertical error bars from three sources, identified in a text legend: GMOS as blue open diamonds, LRIS as red crosses, and ESI as solid black circles. GMOS data is clustered near phases 0.0 and 1.0, LRIS data is clustered near phase 0.5, and ESI data points are scattered across the entire plotted phase range.
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US National Gemini Office @usngo.bsky.social · 16h
This week’s image is of NGC 7232/3! Captured by Gemini South, this cosmic dance between three interacting galaxies reveals dark lanes of dust, brilliant foreground stars, and the raw ingredients for future stars. Check out the 🧵 for another paper. #Astronomy 📸 in thread
An image of an interacting trio of galaxies known as the Lyon Group of Galaxies #455 against a dark background scattered with distant stars. The galaxy NGC 7232 is in the upper right, NGC 7233 is in the lower right, and NGC 7232B is on the left. Two extremely bright Milky Way foreground stars with distinct diffraction spikes dominate the center of the frame. Dark lanes of cosmic dust are visible within NGC 7232 and NGC 7233, while NGC 7232B displays bright, glowing clusters of young blue stars along its faint, diffuse spiral arms.
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US National Gemini Office @usngo.bsky.social · 16h
This is Pa 30, an explosive cloud of gas and dust bursting from a central hot blue star. Astronomers say it’s likely the remnant of a supernova that people on Earth saw in 1181. #astronomy
Gemini image of Pa 30 (IRAS 00500+6713), the remnant of the 1181 supernova in Cassiopeia. Hundreds of thin orange filaments radiate outward from a bright blue-white central star, the hot white dwarf WD J005311, forming a round, dandelion-like nebula roughly 8,000 light-years away. Blue and white foreground stars are scattered across the black sky.
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 07/10/2026
Watch a year of astronomy unfold! This awesome animation maps out every single science observation made by the Gemini North and South telescopes in 2025. Watch the universe come alive as 12 months of stellar targets are mapped before your eyes. #Astronomy Link: www.youtube.com/watch?v=z6DQ...
youtube.com
Gemini Observatory 2025 - Science Observations
YouTube video by NOIRLabAstro
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 07/10/2026
One Gemini South wasn’t quite enough for this sunset. Thanks to a perfectly still patch of water on Cerro Pachón in Chile, the telescope looks like it has a twin reflected beneath it. #astronomy Credit: NOIRLab/NSF/AURA/C. Corco
Gemini South's silver dome stands silhouetted against a vivid red-and-orange sunset on Cerro Pachón, mirrored in a still puddle in the foreground, with patches of snow along the roadside.
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US National Gemini Office @usngo.bsky.social · 07/10/2026
Queue programs observed at Gemini Observatory N/S on 10/06/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 07/10/2026
Science observations @GeminiObs from 2026-10-01 to 2026-10-07: #astronomy
Gemini weekly footprint
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US National Gemini Office @usngo.bsky.social · 07/10/2026
Watch a year of astronomy unfold! This awesome animation maps out every single science observation made by the Gemini North and South telescopes in 2025. Watch the universe come alive as 12 months of stellar targets are mapped before your eyes. #Astronomy Link: www.youtube.com/watch?v=z6DQ...
youtube.com
Gemini Observatory 2025 - Science Observations
YouTube video by NOIRLabAstro
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US National Gemini Office @usngo.bsky.social · 07/10/2026
One Gemini South wasn’t quite enough for this sunset. Thanks to a perfectly still patch of water on Cerro Pachón in Chile, the telescope looks like it has a twin reflected beneath it. #astronomy Credit: NOIRLab/NSF/AURA/C. Corco
Gemini South's silver dome stands silhouetted against a vivid red-and-orange sunset on Cerro Pachón, mirrored in a still puddle in the foreground, with patches of snow along the roadside.
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 05/10/2026
A week in the life of Gemini North! 🔭 Check out some of the gorgeous targets we pointed at between 09-27-2026 and 10-04-2026. #Astronomy
A 3x3 grid of nine images captured by the Gemini North telescope between September 27 and October 4, 2026. A legend at the top indicates the only instrument used is ALOPEKE. The grid showcases various deep-space targets against black, star-filled backgrounds. Most of the panels feature a brilliantly bright, central star or object with a dark, saturated artifact at its core, surrounded by glowing, colorful halos in shades of blue, white, green, and orange. Each of the nine panels is labeled "ALOPEKE" in yellow text in the bottom-left corner.
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 05/10/2026
From @noirlabastro.bsky.social : Gemini Observatory FT review process has new guidelines on AI use to ensure each proposal's confidentiality. Please review them here: gemini.edu/observing/ph...
Infrared image of Jupiter from Gemini North, shown in glowing orange and yellow against black. Bright, turbulent bands of escaping heat alternate with dark cloud zones, and the Great Red Spot appears as a dark oval near the center.
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US National Gemini Office @usngo.bsky.social · 06/10/2026
Queue programs observed at Gemini Observatory N/S on 10/05/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 05/10/2026
Queue programs observed at Gemini Observatory N/S on 10/04/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 05/10/2026
A week in the life of Gemini North! 🔭 Check out some of the gorgeous targets we pointed at between 09-27-2026 and 10-04-2026. #Astronomy
A 3x3 grid of nine images captured by the Gemini North telescope between September 27 and October 4, 2026. A legend at the top indicates the only instrument used is ALOPEKE. The grid showcases various deep-space targets against black, star-filled backgrounds. Most of the panels feature a brilliantly bright, central star or object with a dark, saturated artifact at its core, surrounded by glowing, colorful halos in shades of blue, white, green, and orange. Each of the nine panels is labeled "ALOPEKE" in yellow text in the bottom-left corner.
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US National Gemini Office @usngo.bsky.social · 05/10/2026
From @noirlabastro.bsky.social : Gemini Observatory FT review process has new guidelines on AI use to ensure each proposal's confidentiality. Please review them here: gemini.edu/observing/ph...
Infrared image of Jupiter from Gemini North, shown in glowing orange and yellow against black. Bright, turbulent bands of escaping heat alternate with dark cloud zones, and the Great Red Spot appears as a dark oval near the center.
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 02/10/2026
This week’s image is of NGC 6164-5! Captured by Gemini South, this dramatic inverted S-shaped cloud is a nebula sculpted by gases ejected from the rapidly aging, massive star at its core. Check out the 🧵 for another paper. #Astronomy 📸 in thread
An image of the emission nebula NGC 6164-5 set against a black, star-filled background. At the very center shines the exceptionally bright star HD 148937, radiating intense white and purple light. Surrounding the star is a thick, glowing bipolar cloud of gas and dust that forms an inverted S-shape with somewhat rectangular, rounded corners. The outer edges of these nebula lobes glow brightly in striking orange and reddish hues, especially along the top-right and bottom-left curves. The interior of the nebula, closer to the central star, features darker, heavily textured clouds in shades of deep red, brown, and purple. Several prominent stars with diffraction spikes and countless smaller, fainter stars are scattered throughout the surrounding space.
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US National Gemini Office @usngo.bsky.social · 04/10/2026
Queue programs observed at Gemini Observatory N/S on 10/03/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 03/10/2026
Queue programs observed at Gemini Observatory N/S on 10/02/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 02/10/2026
Queue programs observed at Gemini Observatory N/S on 10/01/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 02/10/2026
Credit: International Gemini Observatory
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US National Gemini Office @usngo.bsky.social · 02/10/2026
Hydrogen-poor Superluminous Supernovae in the Nebular Phase: Spectral Diversity Due to Ejecta Ionization as a Probe of the Power Source, by Peter K. Blanchard et al. 2026 ui.adsabs.harvard.edu/abs/2026ApJ....
A two-panel line graph displaying Normalized Continuum-Subtracted Flux (0 to 10) versus Rest Wavelength (4000 to 5500 Å). The top panel is labeled t/t_d < 4, and the bottom is t/t_d > 4. Multiple spectra are plotted and color-coded by an L_{7300}/L_{6300} ratio ranging from 0 (dark purple) to 4 (yellow-green). Vertical dashed lines mark specific emission features: H_gamma, [O III], Mg I, H_beta, and a second [O III] region. In the top panel, spectra with higher ratios (yellow/green) exhibit strong, broad emission peaks at the marked hydrogen and oxygen lines. In the bottom panel, spectra are predominantly lower ratio (purple/blue) and exhibit generally weaker, narrower emission features, though sharp [O III] and H_beta peaks are still visible.
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US National Gemini Office @usngo.bsky.social · 02/10/2026
This week’s image is of NGC 6164-5! Captured by Gemini South, this dramatic inverted S-shaped cloud is a nebula sculpted by gases ejected from the rapidly aging, massive star at its core. Check out the 🧵 for another paper. #Astronomy 📸 in thread
An image of the emission nebula NGC 6164-5 set against a black, star-filled background. At the very center shines the exceptionally bright star HD 148937, radiating intense white and purple light. Surrounding the star is a thick, glowing bipolar cloud of gas and dust that forms an inverted S-shape with somewhat rectangular, rounded corners. The outer edges of these nebula lobes glow brightly in striking orange and reddish hues, especially along the top-right and bottom-left curves. The interior of the nebula, closer to the central star, features darker, heavily textured clouds in shades of deep red, brown, and purple. Several prominent stars with diffraction spikes and countless smaller, fainter stars are scattered throughout the surrounding space.
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 01/10/2026
Here is a summary of observations from both Gemini telescopes in September 2026, divided by instrument and color-coded by location. Gemini's ALOPEKE took the most observations last month, totaling over 2,000! #Astronomy
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US National Gemini Office @usngo.bsky.social · 01/10/2026
Queue programs observed at Gemini Observatory N/S on 09/30/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 01/10/2026
Here is a summary of observations from both Gemini telescopes in September 2026, divided by instrument and color-coded by location. Gemini's ALOPEKE took the most observations last month, totaling over 2,000! #Astronomy
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US National Gemini Office @usngo.bsky.social · 30/09/2026
Queue programs observed at Gemini Observatory N/S on 09/29/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 30/09/2026
Science observations @GeminiObs from 2026-09-24 to 2026-09-30: #astronomy
Gemini weekly footprint
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 28/09/2026
A week in the life of Gemini North! 🔭 Check out some of the gorgeous targets we pointed at between 09-20-2026 and 09-27-2026. #Astronomy
A 3x3 grid of nine images captured by the Gemini North telescope between September 20 and 27, 2026. A legend at the top indicates the instruments used: GMOS-N (yellow), GNIRS (blue), and IGRINS-2 (red). The grid showcases various deep-space targets against black backgrounds. The images include dense, glittering star clusters, scattered starfields, bright stars with distinct cross-shaped diffraction spikes, and distant glowing galaxies. Each panel is labeled with the corresponding instrument in the bottom-left corner: four images were taken by GNIRS, three by IGRINS-2, and two by GMOS-N.
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US National Gemini Office @usngo.bsky.social · 30/09/2026
A few hours to go! #astronomy
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US National Gemini Office @usngo.bsky.social · 29/09/2026
Queue programs observed at Gemini Observatory N/S on 09/28/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 29/09/2026
Have you submitted your proposal for the 2027A semester at Gemini yet? The deadline is September 30, 2026, at 23:59 (Mountain Standard Time). #astronomy
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US National Gemini Office @usngo.bsky.social · 28/09/2026
Queue programs observed at Gemini Observatory N/S on 09/27/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 28/09/2026
A week in the life of Gemini North! 🔭 Check out some of the gorgeous targets we pointed at between 09-20-2026 and 09-27-2026. #Astronomy
A 3x3 grid of nine images captured by the Gemini North telescope between September 20 and 27, 2026. A legend at the top indicates the instruments used: GMOS-N (yellow), GNIRS (blue), and IGRINS-2 (red). The grid showcases various deep-space targets against black backgrounds. The images include dense, glittering star clusters, scattered starfields, bright stars with distinct cross-shaped diffraction spikes, and distant glowing galaxies. Each panel is labeled with the corresponding instrument in the bottom-left corner: four images were taken by GNIRS, three by IGRINS-2, and two by GMOS-N.
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 25/09/2026
This week’s image is of NGC 7253! Captured by Gemini’s GMOS-N, this dramatic scene between the two galaxies is also known as Nā ʻUhane Māhoe Huki Pū i ke Ola (“The twin spirits pulling together creating life”). Check out the 🧵 for another paper. #Astronomy 📸 in thread
An image of NGC 7253, a pair of interacting spiral galaxies set against a dark background scattered with distant stars and galaxies. The galaxy on the left is angled slightly, displaying a bright, glowing core and sprawling spiral arms heavily dotted with bright pink and blue regions of star formation. The galaxy on the right is viewed nearly edge-on, looking like an elongated, warped streak of light stretching toward the first galaxy. A luminous haze of gas, dust, and stars appears to connect the two structures, illustrating the intense gravitational pull between them.
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US National Gemini Office @usngo.bsky.social · 25/09/2026
Credit: International Gemini Observatory/NOIRLab/NSF/AURA Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)
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US National Gemini Office @usngo.bsky.social · 25/09/2026
Final Moments. II. Observational Properties and Physical Modeling of Circumstellar-material-interacting Type II Supernovae, by W. V. Jacobson-Galan et al. 2024 ui.adsabs.harvard.edu/abs/2024ApJ....
A four-panel figure. Top-left: A normalized cumulative distribution function of redshift for Class 1 (blue), Class 2 (yellow), Class 3 (red), and a Comparison group (black dashed line). Top-right: A spectral plot of 2022pgf showing relative flux vs. rest wavelength (5875-5900 Å). It highlights two deep Na absorption features in high and low resolution, with calculated equivalent widths of 1.12 and 0.83 Å. Bottom-left: A cumulative distribution of host extinction, E(B-V), for Gold (blue), Gold+Silver (red), and Comparison samples, alongside reference lines for SN II. Bottom-right: A scatter plot of g-r color (10-20 days) versus Na ID equivalent width (log scale), showing detections (circles) and upper limits (stars) across the color classes with a dashed purple trendline.
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US National Gemini Office @usngo.bsky.social · 25/09/2026
This week’s image is of NGC 7253! Captured by Gemini’s GMOS-N, this dramatic scene between the two galaxies is also known as Nā ʻUhane Māhoe Huki Pū i ke Ola (“The twin spirits pulling together creating life”). Check out the 🧵 for another paper. #Astronomy 📸 in thread
An image of NGC 7253, a pair of interacting spiral galaxies set against a dark background scattered with distant stars and galaxies. The galaxy on the left is angled slightly, displaying a bright, glowing core and sprawling spiral arms heavily dotted with bright pink and blue regions of star formation. The galaxy on the right is viewed nearly edge-on, looking like an elongated, warped streak of light stretching toward the first galaxy. A luminous haze of gas, dust, and stars appears to connect the two structures, illustrating the intense gravitational pull between them.
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US National Gemini Office @usngo.bsky.social · 23/09/2026
Queue programs observed at Gemini Observatory N/S on 09/22/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 23/09/2026
Science observations @GeminiObs from 2026-09-17 to 2026-09-23: #astronomy
Gemini weekly footprint
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 21/09/2026
A week in the life of Gemini North! 🔭 Check out some of the gorgeous targets we pointed at between 09-13-2026 and 09-20-2026. #Astronomy
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US National Gemini Office @usngo.bsky.social · 22/09/2026
Queue programs observed at Gemini Observatory N/S on 09/21/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 21/09/2026
Queue programs observed at Gemini Observatory N/S on 09/20/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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US National Gemini Office @usngo.bsky.social · 21/09/2026
A week in the life of Gemini North! 🔭 Check out some of the gorgeous targets we pointed at between 09-13-2026 and 09-20-2026. #Astronomy
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 18/09/2026
This week’s image is of the CK Vulpeculae nebula! This spectacular image was taken with Gemini’s GMOS-N and captures not only the red arcs of outwardly expanding gas but also the blue-white core. Check out the 🧵 for another paper. #Astronomy 📸 in thread
An image of the CK Vulpeculae nebula set against a dense, dark background heavily populated with stars. The nebula features a glowing bluish-white central region, surrounded by hourglass-shaped lobes of reddish-orange gas expanding outward. Further out from the bright center are two faint, small reddish arcs of gas, one located towards the top and the other towards the bottom of the nebula's structure. The surrounding starfield contains stars of varying sizes and brightness, appearing as white, light blue, and orange pinpricks of light.
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US National Gemini Office @usngo.bsky.social · 19/09/2026
Queue programs observed at Gemini Observatory N/S on 09/18/26 (bit.ly/2KhLox3) #astronomy:
Gemini daily update
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Reposted by US National Gemini Office
US National Gemini Office @usngo.bsky.social · 16/09/2026
Throwback post: Our friends at Kitt Peak (home of DESI and NEID) also got a spectacular view of the Lunar eclipse. Note the "tiny" dot in the Southeast starting at 15 seconds! #Astronomy
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US National Gemini Office @usngo.bsky.social · 18/09/2026
Credit: International Gemini Observatory/NOIRLab/NSF/AURA Image processing: Travis Rector (University of Alaska Anchorage), Jen Miller (Gemini Observatory/NSF NOIRLab), Mahdi Zamani & Davide de Martin
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US National Gemini Office @usngo.bsky.social · 18/09/2026
Near-infrared and Optical Nebular-phase Spectra of Type Ia Supernovae SN 2013aa and SN 2017cbv in NGC 5643, by Sahana Kumar et al. 2023 ui.adsabs.harvard.edu/abs/2023ApJ....
A figure with four main quadrants, displaying multiple overlaid line graphs plotting "Normalized Flux" against "Rest Wavelength." The left quadrants show optical spectra between 4400 and 5600 Angstroms, while the right quadrants display near-infrared spectra between 1.5 and 2.4 micrometers.
Colored lines represent different supernovae—including 2011fe, 2013aa, 2014J, and 2017cbv—observed at late epochs, ranging from approximately 300 to 570 days past peak brightness. Vertical tick marks identify specific iron emission lines, categorized into [Fe II] and [Fe III], with specific wavelengths labeled (e.g., 4658 Angstroms and 1.6440 micrometers). The plots compare the emission features of these astronomical objects, showing overall similarities in their broad spectral line profiles.
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