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- A. Milani, M. E. Sansaturio, G. Tommei, O. Arratia
- 2004

When the astrometric data for an asteroid are insufficient, the orbit solving the least squares problem can be weakly determined or even not computable. Then it is advantageous for most applications to sample the confidence region (where the orbit could be found without contradicting the observations) with multiple solutions, a finite set of Virtual… (More)

- A. Milani, G. F. Gronchi, Z. Knežević, M. E. Sansaturio, J. Kubica

In the next generation surveys, the discovery of moving objects can be successful only if an observation strategy and the identification/orbit determination procedure are appropriate for the diverse apparent motions of the target sub-populations. The observations must accurately measure the displacement over a short interval of time; observations believed… (More)

Most asteroid discoveries consist of a few astrometric observations over a short time span, and in many cases the amount of information is not enough to compute a full orbit according to the least squares principle. We investigate whether such a Very Short Arc may nonetheless contain significant orbit information, with predictive value, e.g., allowing to… (More)

- Andrea Milani
- 1998

When an asteroid is lost, the observers need to know the portion of the celestial sphere where it could be recovered at a given time. This region is an image of the region, in the space of orbital elements, where the orbit is compatible with the previous observations. The map between these two regions is nonlinear, therefore the classical linear… (More)

The opportunistic pathogen Pseudomonas aeruginosa can establish life-long chronic infections in the airways of cystic fibrosis (CF) patients. Persistent lifestyle is established with P. aeruginosa patho-adaptive variants, which are clonal with the initially-acquired strains. Several reports indicated that P. aeruginosa adapts by loss-of-function mutations… (More)

- G. F. Gronchi, A. Milani
- 1998

Semianalytical averaging is used to compute secular perturbations on the orbits of asteroids and comets; the method is applicable even for planet-crossing orbits. We prove that for every value of the asteroid/comet semimajor axis, and for an arbitrary number of perturbing planets, there is a stable region of orbits free from node crossings; it corresponds… (More)

- Jeremy Kubica, Larry Denneau, Tommy Grav, James Heasley, Robert Jedicke, Joseph Masiero +4 others
- 2006

The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) under development at the University of Hawaii's Institute for Astronomy is creating the first fully automated end-to-end Moving Object Processing System (MOPS) in the world. It will be capable of identifying detections of moving objects in our solar system and linking those detections… (More)

- Andrea Milani, Steven R. Chesley, Maria Eugenia Sansaturio, Fabrizio Bernardi, Giovanni B. Valsecchi, Oscar Arratia
- 2009

The potentially hazardous asteroid (101955) 1999 RQ 36 has a possibility of colliding with the Earth in the latter half of the 22nd century, well beyond the traditional 100-year time horizon for routine impact monitoring. The probabilities accumulate to a total impact probability of approximately 10 −3 , with a pair of closely related routes to impact in… (More)

The manipulation of the immune system through the administration of a vaccine to direct an effective and long-lasting immune response against breast cancer (BC) cells is an attractive strategy. Vaccines would have several theoretical advantages over standard therapies, including low toxicities, high specificity, and long-lasting efficacy due to the… (More)

- G. F. Gronchi, A. Milani, Giovanni F. Gronchi, Linda Dimare, Andrea Milani
- 2009

We investigate a method to compute a finite set of preliminary orbits for solar system bodies using the first integrals of the Kepler problem. This method is thought for the applications to the modern sets of astrometric observations, where often the information contained in the observations allows only to compute, by interpolation , two angular positions… (More)