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# Program information file
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PROGRAM_ID 2024A987
PROGRAM_TITLE SpeX Spectroscopy of Extragalactic Transients
PROGRAM_INV1 Willem Hoogendam
PROGRAM_INV2
PROGRAM_INV3
PROGRAM_INV4
PROGRAM_INV5
PROGRAM_SCICAT extra-galactic
PROGRAM_ABSTRACT_BEG
We seek NIR follow-up of the following particularly interesting transients. 3C-273 is the first identified quasar, and it is undergoing an incredible dimming event where it is no longer the brightest QSO in the sky. We want to monitor 3C-273 in the NIR using SXD to see if NIR features change during this dimming. This could be part of the 'changing-look' AGN phenomenon.
Previous IRTF NIR spectra show slight variations compared to archival, but nothing major. Having more IRTF observations will help us compare to a good
baseline from the start of the dimming. SN 2023wrk is a nearby 2003fg-like SN Ia, which is posited to collide and interact with C-rich CSM. Previous IRTF time has detected a narrow C I feature post-peak, and we wish to study the evolution of this narrow C I from colliding ejecta with the C-rich CSM. SN 2023ixf is the nearest type II SN in a decade, and we would like to get
a NIR time series to synergize with an upcoming JWST observation in May. Likewise, SN 2024ahv is a nearby stripped-envelope SN with an upcoming JWST observation in March. We plan to use the SpeX/SXD mode.
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