Image Details

Choose export citation format:

The Gray Needle: Large Grains in the HD 15115 Debris Disk from LBT/PISCES/Ks and LBTI/LMIRcam/L′ Adaptive Optics Imaging

  • Authors: Timothy J. Rodigas, Philip M. Hinz, Jarron Leisenring, Vidhya Vaitheeswaran, Andrew J. Skemer, Michael Skrutskie, Kate Y. L. Su, Vanessa Bailey, Glenn Schneider, Laird Close, Filippo Mannucci, Simone Esposito, Carmelo Arcidiacono, Enrico Pinna, Javier Argomedo, Guido Agapito, Daniel Apai, Giuseppe Bono, Kostantina Boutsia, Runa Briguglio, Guido Brusa, Lorenzo Busoni, Giovanni Cresci, Thayne Currie, Silvano Desidera, Josh Eisner, Renato Falomo, Luca Fini, Kate Follette, Adriano Fontana, Peter Garnavich, Raffaele Gratton, Richard Green, Juan Carlos Guerra, J. M. Hill, William F. Hoffmann, Terry J. Jones, Megan Krejny, Craig Kulesa, Jared Males, Elena Masciadri, Dino Mesa, Don McCarthy, Michael Meyer, Doug Miller, Matthew J. Nelson, Alfio Puglisi, Fernando Quiros-Pacheco, Armando Riccardi, Eleonora Sani, Paolo Stefanini, Vincenzo Testa, John Wilson, Charles E. Woodward, and Marco Xompero

Rodigas et al. 2012 The Astrophysical Journal 752 57.

  • Provider: AAS Journals

Caption: Figure 6.

(a) Final image at L′, in units of σ, computed with an aggressive LOCI reduction. See the text for methodology. The white dot marks the location of the star and the size of a resolution element at L′. No high S/N point sources are detected. (b) 5σ sensitivity curve for our L′ data, computed by inserting artificial planets into the raw data and running our aggressive LOCI reduction. We reach a background limit of ~17.8 mag, and a contrast of ~9.5 mag at ~0 farcs6. The horizontal dashed lines represent the magnitudes of 10 Myr old and 10 Gyr old planets, from the Baraffe et al. (2003) COND mass–luminosity models. We rule out planets more massive than ~3 M J if the star is young and 30 M J if the star is old.

Other Images in This Article

Show More

Copyright and Terms & Conditions