Huei Sears, PhD 🌟
@starlights.bsky.social
✨ she/her ✨ astrophysicist studying supernovae + GRBs ✨ reputation is my favorite album ✨
i love Italian juices
November 8, 2025 at 4:46 PM
i love Italian juices
: ) 365 giorni of italiana 🇮🇹
November 6, 2025 at 7:22 PM
: ) 365 giorni of italiana 🇮🇹
i think it's really beautiful that through the most powerful telescope in space, stars look like snowflakes
October 31, 2025 at 7:24 PM
i think it's really beautiful that through the most powerful telescope in space, stars look like snowflakes
indeed, i do practice what i preach
October 21, 2025 at 3:41 AM
indeed, i do practice what i preach
yeah… i’m a paid influencer (◡ ‿ ◡ ✿)
October 21, 2025 at 1:50 AM
yeah… i’m a paid influencer (◡ ‿ ◡ ✿)
why…. is it phrased this way
October 20, 2025 at 4:56 PM
why…. is it phrased this way
Rubin Observatory tiramisu for a trip to UDelaware today to see @fedhere.bsky.social + Somayeh Khakpash (+ luckily @yymao.bsky.social !)
October 3, 2025 at 3:09 AM
Rubin Observatory tiramisu for a trip to UDelaware today to see @fedhere.bsky.social + Somayeh Khakpash (+ luckily @yymao.bsky.social !)
i was v honored to give a seminar at the @amnh.org yesterday on my GRB + SN Ia research. They let me tour the museum after too and ah ah ah !!!!!! what a fantastic place !!!!!!!!!!!!
September 19, 2025 at 5:28 PM
i was v honored to give a seminar at the @amnh.org yesterday on my GRB + SN Ia research. They let me tour the museum after too and ah ah ah !!!!!! what a fantastic place !!!!!!!!!!!!
was v excited to see work by @danmil.bsky.social (+ many others!) featured at the @amnh.org today !!
September 18, 2025 at 9:38 PM
was v excited to see work by @danmil.bsky.social (+ many others!) featured at the @amnh.org today !!
very very excited to see this work from Berkeley postdoc, Nayana AJ, on the X-ray and radio properties of the most luminous fast, blue optical transient (L/FBOT), AT 2024wpp! Their analysis suggests that 2024wpp is likely caused by super-Eddington accretion onto a neutron star or black hole!
🧪🔭☄️🦖👩🔬
🧪🔭☄️🦖👩🔬
September 3, 2025 at 1:31 PM
very very excited to see this work from Berkeley postdoc, Nayana AJ, on the X-ray and radio properties of the most luminous fast, blue optical transient (L/FBOT), AT 2024wpp! Their analysis suggests that 2024wpp is likely caused by super-Eddington accretion onto a neutron star or black hole!
🧪🔭☄️🦖👩🔬
🧪🔭☄️🦖👩🔬
very very excited to see this new work from Berkeley graduate student, Natalie LeBaron, on the UV/O/IR properties of the most luminous fast, blue optical transient (L/FBOT), AT 2024wpp (see figure below)! These transients are luminous, fast, and blue, and their origins remain uncertain!
🧪🔭☄️🦖👩🔬
🧪🔭☄️🦖👩🔬
September 3, 2025 at 1:19 PM
very very excited to see this new work from Berkeley graduate student, Natalie LeBaron, on the UV/O/IR properties of the most luminous fast, blue optical transient (L/FBOT), AT 2024wpp (see figure below)! These transients are luminous, fast, and blue, and their origins remain uncertain!
🧪🔭☄️🦖👩🔬
🧪🔭☄️🦖👩🔬
saw these identical gnome twins at the thrift store and Their name (for they have only one) is “Columbine”
August 30, 2025 at 8:57 PM
saw these identical gnome twins at the thrift store and Their name (for they have only one) is “Columbine”
new work led by Daniel Brethauer, a graduate student at UC Berkeley, shows that at very early times, (quasi)non-local thermodynamic effects (Q/NLTE) can be important! Fig. 11 (below) shows some of their modeling compared to observations of AT2017gfo—our best observed kilonova!
🧪🔭☄️🦖
🧪🔭☄️🦖
August 29, 2025 at 12:50 PM
new work led by Daniel Brethauer, a graduate student at UC Berkeley, shows that at very early times, (quasi)non-local thermodynamic effects (Q/NLTE) can be important! Fig. 11 (below) shows some of their modeling compared to observations of AT2017gfo—our best observed kilonova!
🧪🔭☄️🦖
🧪🔭☄️🦖
!!! i know her !! yay Vic !!!!
August 27, 2025 at 1:23 AM
!!! i know her !! yay Vic !!!!
New from Peter Blanchard! A possible NIR-counterpart (observed with JWST, “NIR-1”) to an extremely close and bright fast radio burst (FRB). The origins of FRBs are uncertain, and until now*, haven’t been observed in any non-radio wavelength! very very cool !! 🧪🔭☄️
www.cfa.harvard.edu/news/origin-...
www.cfa.harvard.edu/news/origin-...
August 22, 2025 at 5:00 AM
New from Peter Blanchard! A possible NIR-counterpart (observed with JWST, “NIR-1”) to an extremely close and bright fast radio burst (FRB). The origins of FRBs are uncertain, and until now*, haven’t been observed in any non-radio wavelength! very very cool !! 🧪🔭☄️
www.cfa.harvard.edu/news/origin-...
www.cfa.harvard.edu/news/origin-...
New from Wynn Jacobson-Galán ! it’s so cool to see such an expansive spectral energy distribution (SED) of such an extraordinary event.
arxiv.org/abs/2508.11747
🧪🔭☄️
arxiv.org/abs/2508.11747
🧪🔭☄️
August 19, 2025 at 7:07 AM
New from Wynn Jacobson-Galán ! it’s so cool to see such an expansive spectral energy distribution (SED) of such an extraordinary event.
arxiv.org/abs/2508.11747
🧪🔭☄️
arxiv.org/abs/2508.11747
🧪🔭☄️
The Whirlpool Galaxy, M51, as seen in the 1800s and today.
Fig. 13 from this "Cornelis Easton:The Milky Way as a spiral galaxy" by Pieter C. van der Kruit on the arXiv at arxiv.org/pdf/2508.03409.
🔭☄️🧪
Fig. 13 from this "Cornelis Easton:The Milky Way as a spiral galaxy" by Pieter C. van der Kruit on the arXiv at arxiv.org/pdf/2508.03409.
🔭☄️🧪
August 8, 2025 at 1:53 AM
The Whirlpool Galaxy, M51, as seen in the 1800s and today.
Fig. 13 from this "Cornelis Easton:The Milky Way as a spiral galaxy" by Pieter C. van der Kruit on the arXiv at arxiv.org/pdf/2508.03409.
🔭☄️🧪
Fig. 13 from this "Cornelis Easton:The Milky Way as a spiral galaxy" by Pieter C. van der Kruit on the arXiv at arxiv.org/pdf/2508.03409.
🔭☄️🧪
the TRex emoji is for this btw
August 7, 2025 at 2:47 AM
the TRex emoji is for this btw
new from Itai ! v exciting new radio results on TDE 2024tvd.
"The off-nuclear TDE 2024tvd exhibits double-peaked radio light curves and the fastest evolving radio emission observed from a TDE to date."
See Figures 1 + 2 below! : )
🦖🔭☄️🧪
"The off-nuclear TDE 2024tvd exhibits double-peaked radio light curves and the fastest evolving radio emission observed from a TDE to date."
See Figures 1 + 2 below! : )
🦖🔭☄️🧪
August 7, 2025 at 2:41 AM
new from Itai ! v exciting new radio results on TDE 2024tvd.
"The off-nuclear TDE 2024tvd exhibits double-peaked radio light curves and the fastest evolving radio emission observed from a TDE to date."
See Figures 1 + 2 below! : )
🦖🔭☄️🧪
"The off-nuclear TDE 2024tvd exhibits double-peaked radio light curves and the fastest evolving radio emission observed from a TDE to date."
See Figures 1 + 2 below! : )
🦖🔭☄️🧪
so excited to be presenting at @astronomyontap.bsky.social - Lansing on 8/13 with Laura Chomiuk !!!! hope to see you there : )
August 4, 2025 at 9:21 PM
so excited to be presenting at @astronomyontap.bsky.social - Lansing on 8/13 with Laura Chomiuk !!!! hope to see you there : )
reason # 1,000,000 why i love @astrobites.bsky.social sm: whenever one of passes our PhD defense we post in #random a congrats and shower them with fun emojis. I think it speaks the strong community and care of each other in the collaboration. ❤️
p.s. congrats to Dr. @suchitra.bsky.social !!! : )
p.s. congrats to Dr. @suchitra.bsky.social !!! : )
July 29, 2025 at 9:17 PM
reason # 1,000,000 why i love @astrobites.bsky.social sm: whenever one of passes our PhD defense we post in #random a congrats and shower them with fun emojis. I think it speaks the strong community and care of each other in the collaboration. ❤️
p.s. congrats to Dr. @suchitra.bsky.social !!! : )
p.s. congrats to Dr. @suchitra.bsky.social !!! : )
@genevieveschroeder.bsky.social (Cornell) et al. present late-time radio imaging of a sample of SNe Ic-BL. In the images here, at the optical location (left) of SN PTF10tqv, they detect very late-time (> 10 years !!!) emission with the VLA (middle) and MeerKAT (right).
🧪🔭☄️👩🔬 #highenergyastro
🧪🔭☄️👩🔬 #highenergyastro
July 23, 2025 at 2:22 AM
@genevieveschroeder.bsky.social (Cornell) et al. present late-time radio imaging of a sample of SNe Ic-BL. In the images here, at the optical location (left) of SN PTF10tqv, they detect very late-time (> 10 years !!!) emission with the VLA (middle) and MeerKAT (right).
🧪🔭☄️👩🔬 #highenergyastro
🧪🔭☄️👩🔬 #highenergyastro
sooo excited to be presenting at @astronomyontap.bsky.social - Trenton next week (July 10) !! gonna be talking about Adele, the big bang theory, and the cosmic microwave background !! hope to see you there !!
🔭🧪👩🔬 #womeninstem
🔭🧪👩🔬 #womeninstem
July 2, 2025 at 8:48 PM
sooo excited to be presenting at @astronomyontap.bsky.social - Trenton next week (July 10) !! gonna be talking about Adele, the big bang theory, and the cosmic microwave background !! hope to see you there !!
🔭🧪👩🔬 #womeninstem
🔭🧪👩🔬 #womeninstem