Director's Discretionary Time Observations
Director’s Discretionary Time (DDT) can be requested for time-critical observations that cannot plausibly be scheduled for the regular proposal cycle. These types of proposals might be appropriate for the follow-up of newly-discovered unexpected transient phenomena or when developments since the last proposal cycle make a time-critical observation necessary. They are also appropriate for timely follow-up of new discoveries that will provide a critical link in the understanding of the phenomena.
To view details about a specific program, click the Program ID.
PID | Title | PI | Instruments | Allocated Hours | Cycle |
---|---|---|---|---|---|
6549 | Lensed Supernova Encore at z=2! The First Galaxy to Host Two Multiply-Imaged Supernovae | Justin Pierel | NIRCam | 7.3 | 2 |
6543 | Stellar Activity Characterization of LHS 1140 - Is LHS 1140 b a Mini-Neptune or a Water World? | Charles Cadieux | NIRISS | 15.8 | 2 |
6541 | JWST NIRSpec/NIRCam Follow-Up of the High-Redshift Transients Discovered in the GOODS-S JADES-Deep Field | Eiichi Egami | NIRCam NIRSpec |
18.3 | 2 |
4621 | Time-sensitive observations of Chiron: a unique active Centaur beyond 15 AU | Ian Wong | NIRSpec | 4.0 | 2 |
4558 | Establishing the Formation of AF Lep b with NIRCam: The Lowest-Mass Imaged Exoplanet with a Dynamical Mass | Kyle Franson | NIRCam | 6.4 | 2 |
4557 | JWST/NIRSpec confirmation of z~3 transients found by JWST/NIRCam | Haojing Yan | NIRSpec | 10.8 | 2 |
4554 | Revealing the progenitor of the dirty fireball gamma-ray burst AT 2023lcr through its supernova component | Antonio Martin-Carrillo | NIRCam NIRSpec |
4.7 | 2 |
4520 | Near- and Mid-IR Observations to Probe Dust Formation in the Remarkably Nearby Stripped-Envelope Supernova 2023dbc | Melissa Shahbandeh | MIRI NIRSpec |
4.4 | 2 |
4522 | Dust Our Luck – Measuring Molecule and Dust Formation in M101’s Hydrogen-rich SN 2023ixf | Chris Ashall | MIRI NIRSpec |
2.4 | 1 |
4446 | SN H0pe: Independent Measurement of H0 by the Time Delay of a Multiply-imaged Supernova | Brenda Frye | NIRCam NIRSpec |
10.5 | 1 |
4445 | Revealing the nature of the exceptional GRB 230307A: nearby nucleosynthesis or a primordial explosion? | Andrew Levan | NIRCam NIRSpec |
4.7 | 1 |
4436 | Near- and Mid-IR Observations to Probe Dust Formation in the Remarkably Nearby Stripped-Envelope Supernova 2023dbc | Melissa Shahbandeh | MIRI NIRSpec |
1.8 | 1 |
The late time spectrum of a kilonova in the exceptionally bright GRB 230307A | Andrew Levan | NIRCam NIRSpec |
4.9 | 1 | |
The impact of smaller accretion bursts on the planet-forming material in the disk of a young eruptive star | Peter Abraham | MIRI | 2.2 | 1 | |
4426 | An unprecedented spatially resolved analysis of the brightest galaxy at z>10 in GOODS-N | Roberto Maiolino | NIRSpec | 17.7 | 1 |
2787 | A sensitive search for rings and small moons in the Martian system using JWST | Geronimo Villanueva | NIRCam | 5.7 | 1 |
2784 | Late Time Observations of GRB 221009A: The First Search for r-Process Nucleosynthesis in a Collapsar | Peter Blanchard | NIRCam NIRSpec |
11.2 | 1 |
2783 | MIRI LRS follow up on SO2 detection in WASP-39b | Diana Powell | MIRI | 10.7 | 1 |
2782 |
Heavy element formation in the brightest gamma-ray burst of all time |
Andrew Levan |
MIRI NIRSpec |
2.2 | 1 |
2767 | Imaging and Spectroscopy of Three Highly Magnified Images of a Supernova at z=1.5 | Patrick Kelly | NIRCam NIRSpec |
10.3 | 1 |
2756 | Imaging and Spectroscopic Follow-up of a Supernova at Redshift z=3.47 | Wenlei Chen | NIRCam NIRSpec |
9.4 |
1 |
2754 | Unique Constraints on Early Dust Growth in Core-Collapse Supernovae | Justin Pierel | MIRI | 5.6 | 1 |
2750 |
Spectroscopic follow-up of ultra-high-z candidates in CEERS: Characterizing true z > 12 galaxies and z~4-7 interlopers in preparation for JWST Cycle 2 |
Pablo Arrabal Haro | NIRSpec | 8.0 | 1 |
The Volatile Content of Oort Cloud Comet C/2014 UN271 | Bryce Bolin | NIRSpec |
4.4 |
1 | |
JWST Cycle 1 Outreach Campaign |
Klaus Pontoppidan |
MIRI NIRCam |
45.4 |
1 |
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The NASA James Webb Space Telescope, developed in partnership with ESA and CSA, is operated by AURA’s Space Telescope Science Institute.