activity
20162026
most citedDiscovery of a red supergiant donor star in SN2010da/NGC 300 ULX-1

58 citations · 227 across the 28 of their papers we have counts for

collaborators
Showing 2024Show all

11 papers · 1 filter

astro-ph.HE2024

JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip

Melissa Shahbandeh, Ori D. Fox, Tea Temim +42

Dust from core-collapse supernovae (CCSNe), specifically Type IIP SNe, has been suggested to be a significant source of the dust observed in high-redshift galaxies. CCSNe eject lar…

astro-ph.HE2024★ 5 cited

Disappearance of a massive star in the Andromeda Galaxy due to formation of a black hole

Kishalay De, Morgan MacLeod, Jacob E. Jencson +11

When a massive star reaches the end of its lifetime, its core collapses and releases neutrinos that drive a shock into the outer layers (stellar envelope). A sufficiently strong sh…

astro-ph.SR2024

Possible anti-correlations between pulsation amplitudes and the disk growth of Be stars in giant-outbursting Be X-ray binaries

Masafumi Niwano, Michael M. Fausnaugh, Ryan M. Lau +15

The mechanism of X-ray outbursts in Be X-ray binaries remains a mystery, and understanding their circumstellar disks is crucial for a solution of the mass-transfer problem. In part…

astro-ph.GA2024★ 2 cited

Revealing Potential Initial Mass Function variations with metallicity: JWST observations of young open clusters in a low-metallicity environment

Chikako Yasui, Natsuko Izumi, Masao Saito +3

We present the substellar mass function of star-forming clusters (0.1 Myr old) in a low-metallicity environment (0.7 dex). We performed deep JWST/NIRCam and MIRI…

astro-ph.SR2024

Investigating the Electron Capture Supernova Candidate AT 2019abn with JWST Spectroscopy

Sam Rose, Ryan M. Lau, Jacob E. Jencson +5

The James Webb Space Telescope (JWST) has opened up a new window to study highly reddened explosive transients. We present results from late-time (1421 days post-explosion) JWST fo…

astro-ph.SR2024

An infrared census of R Coronae Borealis Stars II -- Spectroscopic classifications and implications for the rate of low-mass white dwarf mergers

Viraj R. Karambelkar, Mansi M. Kasliwal, Patrick Tisserand +18

We present results from a systematic infrared (IR) census of R Coronae Borealis (RCB) stars in the Milky Way, using data from the Palomar Gattini IR (PGIR) survey. R Coronae Boreal…

astro-ph.GA2024★ 8 cited

Overview Results of JWST Observations of Star-Forming Clusters in the Extreme Outer Galaxy

Natsuko Izumi, Michael E. Ressler, Ryan M. Lau +4

The extreme outer Galaxy (EOG), which we define as the region of the Milky Way with a galactocentric radius of more than 18 kpc, provides an excellent opportunity to study star for…

astro-ph.IM2024★ 5 cited

The first Palomar Gattini-IR catalog of J-band light curves: construction and public data release

Shion Murakawa, Kishalay De, Michael C. B. Ashley +7

Palomar Gattini-IR (PGIR) is a wide-field, synoptic infrared time domain survey covering \,sq.\,deg. of the \textbf{accessible} sky at \,night cadence t…

astro-ph.HE2024

WTP19aalnxx: Discovery of a bright mid-infrared transient in the emerging class of low luminosity supernovae revealed by delayed circumstellar interaction

Charlotte Myers, Kishalay De, Lin Yan +11

While core-collapse supernovae (SNe) often show early and consistent signs of circumstellar (CSM) interaction, some exhibit delayed signatures due to interaction with distant mater…

astro-ph.HE2024★ 47 cited

Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A

C. Fransson, M. J. Barlow, P. J. Kavanagh +31

The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which indicates that a compact object (a neutron star or black hole) was formed in the explosion. There…

astro-ph.SR2024

JWST MIRI Imager Observations of Supernova SN 1987A

P. Bouchet, R. Gastaud, A. Coulais +31

There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 years, gives us the opportunity to explore th…