Latest Images

Top panel: multiband light curves of SN 2017ens...

SN 2017ens: The Metamorphosis of a Lumi...

Top panel: multiband light curves of SN 2017ens. Note the discontinuous abscissa. Middle...

The Astrophysical Journal Letters 867 2 L31

Spectroscopic evolution of SN 2017ens. The righ...

SN 2017ens: The Metamorphosis of a Lumi...

Spectroscopic evolution of SN 2017ens. The right panels show the velocity of the Hα, Hβ,...

The Astrophysical Journal Letters 867 2 L31

Top panel: comparison between SN 2017ens and ot...

SN 2017ens: The Metamorphosis of a Lumi...

Top panel: comparison between SN 2017ens and other SNe at three selected epochs. Middle ...

The Astrophysical Journal Letters 867 2 L31

VLT/X-Shooter spectra of SN 2017ens at +190 day...

SN 2017ens: The Metamorphosis of a Lumi...

VLT/X-Shooter spectra of SN 2017ens at +190 day. Top panel: UVB and optical (VIS) parts....

The Astrophysical Journal Letters 867 2 L31

Small subset of the real-life diagnostic data u...

Applying Deep Learning to Fast Radio Bu...

Small subset of the real-life diagnostic data used in the LOTAAS survey with LOFAR (Coen...

The Astronomical Journal 156 6 256

Schematic diagram of a perceptron (top) and a c...

Applying Deep Learning to Fast Radio Bu...

Schematic diagram of a perceptron (top) and a collection of perceptrons combined to form...

The Astronomical Journal 156 6 256

Example of our CNN architecture for the frequen...

Applying Deep Learning to Fast Radio Bu...

Example of our CNN architecture for the frequency–time array of a dedispersed FRB. The i...

The Astronomical Journal 156 6 256

Hierarchical hybrid neural network built from c...

Applying Deep Learning to Fast Radio Bu...

Hierarchical hybrid neural network built from concatenating multiple nets after their fe...

The Astronomical Journal 156 6 256

Four examples of simulated FRBs injected into r...

Applying Deep Learning to Fast Radio Bu...

Four examples of simulated FRBs injected into real data from the CHIME Pathfinder survey...

The Astronomical Journal 156 6 256

Statistics of missed FRBs as a function of S/N ...

Applying Deep Learning to Fast Radio Bu...

Statistics of missed FRBs as a function of S/N from the CHIME Pathfinder. The histogram ...

The Astronomical Journal 156 6 256

Comparison of performance metrics between the f...

Applying Deep Learning to Fast Radio Bu...

Comparison of performance metrics between the four input data products using a subset of...

The Astronomical Journal 156 6 256

Ability of a model trained on simulated bursts ...

Applying Deep Learning to Fast Radio Bu...

Ability of a model trained on simulated bursts to correctly identify Galactic pulsars. O...

The Astronomical Journal 156 6 256

Classification and training time as a function ...

Applying Deep Learning to Fast Radio Bu...

Classification and training time as a function of the number of dynamic spectra candidat...

The Astronomical Journal 156 6 256

Layout of the 39 compound beams that can maxima...

Applying Deep Learning to Fast Radio Bu...

Layout of the 39 compound beams that can maximally be formed at full bandwidth. This pat...

The Astronomical Journal 156 6 256

Black circles and error bars indicate the previ...

Limits on Clouds and Hazes for the TRAP...

Black circles and error bars indicate the previous HST/WFC3 observations (de Wit et al. ...

The Astronomical Journal 156 6 252

Black circles and error bars are from the HST o...

Limits on Clouds and Hazes for the TRAP...

Black circles and error bars are from the HST observations (de Wit et al. 2018) in all p...

The Astronomical Journal 156 6 252

Line strength as a function of metallicity for ...

Limits on Clouds and Hazes for the TRAP...

Line strength as a function of metallicity for TRAPPIST-1 d, e, f, and g (labeled). We d...

The Astronomical Journal 156 6 252

Top: Comparisons of the confirmed Kepler planet...

Simulating the M–R Relation from APF Fo...

Top: Comparisons of the confirmed Kepler planets from Q1 to Q16 (Mullally et al. 2015) i...

The Astronomical Journal 156 6 255

Top: The true and estimated mass values for eac...

Simulating the M–R Relation from APF Fo...

Top: The true and estimated mass values for each of the TESS simulation planets orbiting...

The Astronomical Journal 156 6 255

(A) Effective temperature (Teff) versus apparen...

Simulating the M–R Relation from APF Fo...

(A) Effective temperature (Teff) versus apparent V magnitude for the stars in the TESS s...

The Astronomical Journal 156 6 255

Histogram of the K/2 values (in light red) and ...

Simulating the M–R Relation from APF Fo...

Histogram of the K/2 values (in light red) and resulting desired precision values set fo...

The Astronomical Journal 156 6 255

Top: Schematic RV phase curve of two planets or...

Simulating the M–R Relation from APF Fo...

Top: Schematic RV phase curve of two planets orbiting a star: a massive long-period plan...

The Astronomical Journal 156 6 255

Phase coverage based on every observation taken...

Simulating the M–R Relation from APF Fo...

Phase coverage based on every observation taken across all 10 trials for each prioritiza...

The Astronomical Journal 156 6 255

Results from one 36-month trial of simulated ob...

Simulating the M–R Relation from APF Fo...

Results from one 36-month trial of simulated observing on the APF using each of the four...

The Astronomical Journal 156 6 255

Power-law fits to the decrease in σK as a funct...

Simulating the M–R Relation from APF Fo...

Power-law fits to the decrease in σK as a function of the number of RV data points (mode...

The Astronomical Journal 156 6 255

SEARCH TERM(S)

AUTHOR

PUBLICATIONS

  • 493978
  • 99454
  • 62671
  • 45477
  • 2224
  • 598
  • 563
  • 217
  • 197
  • 128
  • 111
  • 46
  • 23
  • 22
  • 10

YEAR RANGE:

1942
2018

CONTENT TYPE

ADVANCED

ANNOUNCEMENTS

Take the AstroExplorer for a spin!

Be sure to try the search and sorting features, which were added based on user feedback; browse and find the links to videos and interactive figures in our Journal articles; find AAS Research Notes; or notice that new publishers have begun adding their figures to the AIE. Get in touch to hear more!