§ 01Sky tonight
Research targets up tonight
Objects the group has studied that rise above the horizon at Broida Hall during tonight's dark hours, by research theme. Times are Pacific.
Rise and set times are computed in your browser for tonight at Broida Hall.
Exoplanets & instruments
HIP 65426
Multiple star
107 pc
- The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. III. Aperture Masking Interferometric Observations of the Star HIP 65426 at 3.8 μm 2025
- The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. IV. NIRISS Aperture Masking Interferometry Performance and Lessons Learned 2024
- The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 μm 2023
AB Aur
Herbig Ae/Be star
156 pc
HD 143811 AB b
Exoplanet candidate
137 pc
HIP 93398 B
Brown dwarf
HR 2562 B
Brown dwarf
33.9 pc
TWA 7
T Tauri star
34.1 pc
VHS 1256-1257 b
Brown dwarf
22.2 pc
- The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. V. Do Self-consistent Atmospheric Models Represent JWST Spectra? A Showcase with VHS 1256─1257 b 2024
- The JWST Early-release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 μm Spectrum of the Planetary-mass Companion VHS 1256-1257 b 2023
14 Her b
Exoplanet
17.9 pc
β Pictoris
Star
19.6 pc
HD 109573
T Tauri star
70.8 pc
Stars, explosions & transients
SN 2023ixf
Supernova
6.95 Mpc
- Late-time Hubble Space Telescope Ultraviolet Spectra of SN 2023ixf and SN 2024ggi Show Ongoing Interaction with Circumstellar Material 2026
- One Year of SN 2023ixf: Breaking through the Degenerate Parameter Space in Light-curve Models with Pulsating Progenitors 2025
- Spectropolarimetry of SN 2023ixf Reveals Both Circumstellar Material and an Aspherical Helium Core 2025
- +4 more
SN 2017gmr
Supernova
15 Mpc
SN 2021aefx
Supernova
6.61 Mpc
Crab Nebula & Pulsar
Pulsar
2.0 kpc
Remnant of the supernova of 1054. MKID cameras built at UCSB have timed its pulsar's optical pulses photon by photon.
SN 2012Z
Supernova
31.2 Mpc
SN 2017cbv
Supernova
17.8 Mpc
SN 2021yja
Supernova
23 Mpc
Black holes & gravitational waves
Cygnus A
Radio galaxy
261 Mpc
BL Lacertae
BL Lac object
304 Mpc
Centaurus A
Radio galaxy
3.66 Mpc
J1430+2303
Seyfert 2 galaxy
381 Mpc
M 87
Active galaxy
16.5 Mpc
NGC 1068
Seyfert 2 galaxy
14 Mpc
Spectropolarimetry revealed hidden broad lines in its nucleus, the basis of AGN unification.
NGC 3147
Seyfert 2 galaxy
39.3 Mpc
NGC 4151
Seyfert 1 galaxy
15.8 Mpc
NGC 4261
LINER galaxy
32.4 Mpc
Vela Pulsar
Pulsar
287 pc
A young pulsar in the Vela supernova remnant. From interstellar scintillation, Gwinn and colleagues measured its radio emission region at about 500 km across.
Galaxies & the gas around them
COSMOS field
Survey field
- The NIRISS PASSAGE Spectroscopic Redshift Catalog in COSMOS 2026
- Large-scale Structure in COSMOS-Web: Tracing Galaxy Evolution in the Cosmic Web up to z ∼ 7 with the Largest JWST Survey 2026
- Expanding the High-z Supernova Frontier: "Wide-area" JWST Discoveries from the First 2 yr of COSMOS-Web 2026
- +14 more
A1835
Galaxy cluster
z = 0.25
- Star Formation Histories and Stellar Dynamics in the Central Galaxies of RX J0820.9+0752, A1835, and PKS 0745−191 2026
- Velocity Structure Correlations between the Nebular, Molecular, and Atmospheric Gases in the Cores of Four Cool Core Clusters 2025
- Complex Kinematics of Nebular Gas in Active Galaxies Centered in Cooling X-Ray Atmospheres 2024
PKS 0745-191
Radio galaxy
z = 0.10
- Star Formation Histories and Stellar Dynamics in the Central Galaxies of RX J0820.9+0752, A1835, and PKS 0745−191 2026
- Velocity Structure Correlations between the Nebular, Molecular, and Atmospheric Gases in the Cores of Four Cool Core Clusters 2025
- Complex Kinematics of Nebular Gas in Active Galaxies Centered in Cooling X-Ray Atmospheres 2024
RX J0820.9+0752
Galaxy cluster
z = 0.11
- Star Formation Histories and Stellar Dynamics in the Central Galaxies of RX J0820.9+0752, A1835, and PKS 0745−191 2026
- Velocity Structure Correlations between the Nebular, Molecular, and Atmospheric Gases in the Cores of Four Cool Core Clusters 2025
- Complex Kinematics of Nebular Gas in Active Galaxies Centered in Cooling X-Ray Atmospheres 2024
ACO 262
Galaxy cluster
71.8 Mpc
J1044+0353
Emission-line galaxy
57.6 Mpc
SBS 0335-052 E
Active galaxy
60 Mpc
CGCG 007-025
Seyfert 1 galaxy
20.5 Mpc
M 82
Active galaxy
3.53 Mpc
UNCOVER DR2 46803
Emission-line galaxy
z = 4.46
Cosmic dawn
QSO J0305-3150
Quasar
z = 6.61
- A Quasar-anchored Protocluster at z = 6.6 in the ASPIRE Survey. II. An Environmental Analysis of Galaxy Properties in an Overdense Structure 2025
- A Quasar-anchored Protocluster at z = 6.6 in the ASPIRE Survey. I. Properties of [O III] Emitters in a 10 Mpc Overdensity Structure 2025
- A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Impact of Galaxies on the Circumgalactic Medium Metal Enrichment at z > 6 Using the JWST and VLT 2024
- +2 more
QSO J1007+2115
Quasar
z = 7.51
ULAS J1342+0928
Quasar
z = 7.54
- First constraints on the local ionization topology in front of two quasars at z ∼ 7.5 2026
- Possible Contamination of the Intergalactic Medium Damping Wing in ULAS J1342+0928 by Proximate Damped Lyα Absorption 2025
- IGM damping wing constraints on reionization from covariance reconstruction of two z ≳ 7 QSOs 2022
- +1 more
J0252-0503
Quasar
z = 7.00
QSO J0910-0414
Quasar
z = 6.64
J0100+2802
Quasar
z = 6.33
PSO J158.6937-14.4210
Quasar
z = 6.05
QSO J0313-1806
Quasar
z = 7.64
QSO J1120+0641
Quasar
z = 7.09
QSO J1129+1846
Quasar
z = 6.82
Experimental cosmology
Proxima Centauri
Star
1.3 pc
Gravitational wave events 22 events, 4 drawn on the sky
Most events have no point position, only a region of the sky that holds the source with 90% probability. Regions of 300 deg² or less are drawn on the sky above; the GW button shows or hides them.
Binary black hole merger
GW151216
Binary black hole merger
GW151226
- 90% region
- 950 deg²
- Distance
- z = 0.10
Map: GWTC-2.1 (GWOSC)
Binary black hole merger
GW170104
- 90% region
- 1,000 deg²
- Distance
- z = 0.22
Map: GWTC-2.1 (GWOSC)
Binary black hole merger
GW170121
Binary black hole merger
GW170202
Binary black hole merger
GW170304
Binary black hole merger
GW170403
Binary black hole merger
GW170425
Binary black hole merger
GW170727
Binary black hole merger
GW170814
- 90% region
- 92 deg²
- Distance
- z = 0.13
Map: GWTC-2.1 skymap (GWOSC)
Binary neutron star merger
GW170817
- 90% region
- 16 deg²
- Distance
- dL = 40 Mpc
Map: GWTC-1 skymap (GWOSC)
Binary neutron star merger
GW190425
- 90% region
- 8,700 deg²
- Distance
- dL = 150 Mpc
- Las Cumbres Observatory Gravitational-wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy 2026
- The Gravity Collective: A Comprehensive Analysis of the Electromagnetic Search for the Binary Neutron Star Merger GW190425 2025
- The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: A Case Study on GW190425 2021
Map: GWTC-2.1 (GWOSC)
Neutron star–black hole merger
GW190426_152155
- 90% region
- 1,385 deg²
- Distance
- dL = 370 Mpc
Map: GWTC-2 skymap (GWOSC)
Binary black hole merger
GW190521
- 90% region
- 1,000 deg²
- Distance
- z = 0.56
Map: GWTC-2.1 (GWOSC)
Binary black hole merger
GW190711_030756
- Distance
- z = 0.40
Binary black hole merger
GW190728_064510
- 90% region
- 400 deg²
- Distance
- z = 0.18
Map: GWTC-2.1 (GWOSC)
Neutron star–black hole merger
GW190814
- 90% region
- 22 deg²
- Distance
- dL = 230 Mpc
- Las Cumbres Observatory Gravitational-wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy 2026
- SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO/Virgo Event GW190814 2022
- The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814 2021
Map: GWTC-2.1 skymap (GWOSC)
Binary black hole merger
GW190909_114149
- 90% region
- 3,958 deg²
- Distance
- z = 0.62
Map: GWTC-2 skymap (GWOSC)
Binary black hole merger
GW191216_213338
- 90% region
- 910 deg²
- Distance
- dL = 340 Mpc
Map: GWTC-3 (GWOSC)
Binary black hole merger
GW200114_020818
Binary black hole merger
GW200129
- 90% region
- 80 deg²
- Distance
- z = 0.18
Map: GWTC-3 skymap (GWOSC)
Binary black hole merger
GW231123
- 90% region
- 1,664 deg²
- Distance
- z = 0.40
Map: GWTC-4.1 skymap (GWOSC)
None of the research targets rise above the horizon during tonight's dark hours.
Below the horizon all night
- COSMOS field
- SN 2023ixf
- QSO J0305-3150
- QSO J1007+2115
- ULAS J1342+0928
- A1835
- HIP 65426
- J0252-0503
- PKS 0745-191
- RX J0820.9+0752
- AB Aur
- ACO 262
- Cygnus A
- HD 143811 AB b
- HIP 93398 B
- HR 2562 B
- J1044+0353
- QSO J0910-0414
- SBS 0335-052 E
- SN 2017gmr
- SN 2021aefx
- TWA 7
- VHS 1256-1257 b
- 14 Her b
- β Pictoris
- BL Lacertae
- Centaurus A
- CGCG 007-025
- Crab Nebula & Pulsar
- HD 109573
- J0100+2802
- J1430+2303
- M 82
- M 87
- NGC 1068
- NGC 3147
- NGC 4151
- NGC 4261
- Proxima Centauri
- PSO J158.6937-14.4210
- QSO J0313-1806
- QSO J1120+0641
- QSO J1129+1846
- SN 2012Z
- SN 2017cbv
- SN 2021yja
- UNCOVER DR2 46803
- Vela Pulsar
§ 02Notes
How the sky is drawn
- The view
- You look south from Broida Hall, with the center of the view 30° above the horizon. Drag the sky, or use the arrow keys, to turn between east and west. The view is 76° to 120° wide, depending on your screen.
- Projection
- The sky is drawn in stereographic projection. Circles on the sky stay circles on the screen, so constellations keep their shapes, and the scale grows toward the edges.
- Positions
- Astronomy Engine computes the Sun, Moon and planets in your browser for the time shown. Star positions are precessed from J2000 to that date, and refraction lifts objects near the horizon. The Sun and Moon are drawn three times their real size, so the Moon's phase can be read.
- Stars
- Stars to magnitude 6, constellation lines and the outline of the Milky Way come from d3-celestial. Star colors follow the B−V color index. Stars fade near the horizon, by 0.2 magnitudes per airmass, and in twilight and moonlight.
- Horizon
- The Channel Islands sit on the sea horizon at their real azimuths, with their heights drawn three times too tall so they can be seen. The mainland coast runs along either side.
- Time
- Tonight sets the clock to 30 minutes after astronomical twilight ends. The slider runs from noon to noon, Pacific time, and Play turns the sky at one hour per second. Add
?t=and an ISO time to the address to fix the time. - Targets
- Gold reticles mark objects the group has studied. The ones with the most papers carry labels. Hover over or focus a reticle to name the others, and select it for its papers.