Astronomy & Astrophysics manuscript no.

2001

Citations in the corpus

• A SYSTEMATIC SEARCH FOR TRANSITING PLANETS IN THE K2 DATA (2015, methodology): “A query to the TRILEGAL (TRIdimensional modeL of thE GALaxy, Girardi et al. 2005) galaxy line-of-sight simulation software reveals that the typical density of field stars along the line of sight to the Campaign 1 field is about 7.8 × 10−4 arcsec−2.”
• LOW FALSE POSITIVE RATE OF KEPLER CANDIDATES ESTIMATED FROM A COMBINATION OF SPITZER AND FOLLOW-UP OBSERVATIONS (2015, methodology): “These authors use the depths from the first 1235 KOIs reported from Borucki et al. (2011) together with generic assumptions and with the stellar population synthesis model TRILEGAL (Girardi et al. 2005) to derive the FPP of all KOIs.”
• THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. X. ULTRAVIOLET TO INFRARED PHOTOMETRY OF 117 MILLION EQUIDISTANT STARS (2014, methodology): “We ran a simulation of the Girardi et al. (2005, 2012) model of the stellar population of the Milky Way at the location of M31.”
• The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans (2022, methodology): “We then add a stellar field, including the known bright stars in the FoV from the GAIA DR2 catalog, plus additional stars fainter than the GAIA limit using TRILEGAL (Girardi et al. 2005, 2012), a populations synthesis code for simulating the stellar photometry of any desired Milky Way stellar field ”
• CHEMICAL CARTOGRAPHY WITH APOGEE: LARGE-SCALE MEAN METALLICITY MAPS OF THE MILKY WAY DISK (2013, methodology): “Distances were tested using a set of simulated observations from TRILEGAL (Girardi et al. 2005), observations of calibration clusters (Mészáros et al. 2013) of known distance, and observations of Kepler giants with asteroseismic parameters (Pinsonneault et al. in prep.) that allow independent…”
• A Framework for Prioritizing the TESS Planetary Candidates Most Amenable to Atmospheric Characterization (2018, methodology): “The Sullivan et al. (2015) catalog is one realization of the TESS planet detection outcomes based on published occurrence rate statistics (Fressin et al. 2013; Dressing & Charbonneau 2015) and a galactic stellar population model (Girardi et al. 2005).”
• Evolution of asymptotic giant branch stars. II. Optical to far-infrared isochrones with improved TP- (2007, methodology): “The new models have been included in the TRILEGAL code (Girardi et al. 2005; Girardi & Marigo 2007b)13 for the simulation of resolved stellar populations in the Milky Waynd in external galaxies, and in the GRASIL code (GRAphite and SILicate; Silva et al. 1998, Panuzzo et al. 2005)14 for computing…”
• CARS: the CFHTLS-Archive-Research Survey - II. Weighing dark matter halos of Lyman-break galaxies at z = 3–5 (2009, methodology): “Furthermore, we simulate the colours of stars in our fields from the TRILEGAL galactic model (Girardi et al. 2005) taking into account the galactic coordinates of our survey fields and the depths of the images (see also Hildebrandt et al. 2007).”
• OBSERVING THE NEXT GALACTIC SUPERNOVA (2013, methodology): “However, if failed SNe associated with red supergiants follow the models of Lovegrove & Woosley (2013) and Piro (2013), it would likely be possible to observe the weak shock breakout and transient associated with such an event occurring within the Galaxy provided that rough positional information is”
• The ACS survey of Galactic globular clusters. XII. Photometric binaries along the main sequence (2011, methodology): “4.1.1 In order to determine field objects contamination in the CMDs of the remaining clusters, we run a program developed by Girardi et al. (2005), which uses a model to predict star numbers in any Galactic field.”
• THE FALSE POSITIVE RATE OF KEPLER AND THE OCCURRENCE OF PLANETS (2013, methodology): “Using the Trilegal model of Girardi et al. (2005) we found that the stellar densities from the latter are approximately 10% smaller, while the distribution of stars in terms of brightness and spectral type is similar (background stars using Trilegal are only 0.47 mag brighter in the R band, and…”
• THE IMPACT OF STELLAR MULTIPLICITY ON PLANETARY SYSTEMS. I. THE RUINOUS INFLUENCE OF CLOSE BINARY COMPANIONS (2016, result): “Our predictions are similar to those from the TRILEGAL survey (Girardi et al. 2005), which also requires a similar rescaling factor.”
• Asteroseismology of red giants from the first four months of Kepler data: Fundamental stellar parameters (2010, methodology): “To do so, we used the synthetic red-giant population for theKepler field of view as presented by Huber et al. (2010) and computed with the stellar synthesis code TRILEGAL (Girardi et al. 2005) in the same way as by Miglio et al. (2009) for one of the CoRoT fields.”
• AN EFFICIENT AUTOMATED VALIDATION PROCEDURE FOR EXOPLANET TRANSIT CANDIDATES (2012, methodology): “TRILEGAL (TRIdimensional modeL of thE GALaxy; Girardi et al. 2005, and used in MJ11) is a tool perfectly suited to this purpose.”
• THE SLOAN DIGITAL SKY SURVEY COADD: 275 deg2 OF DEEP SLOAN DIGITAL SKY SURVEY IMAGING ON STRIPE 82 (2011, methodology): “The models are from Trilegal star count modeling (Girardi et al. 2005, online version v1.”
• The Milky Way’s stellar disk (2013, methodology): “The dissection and subsequent global synthesis of the Disk through MAPs is ultimately an empirical approach that is distinct from synthetic models such as the Besancon model (Robin et al. 2003), Trilegal (Girardi et al. 2005), or the model of Just & Jahreiß (2010), which we do not discuss in detail ”
• ASTEROSEISMOLOGY OF RED GIANTS FROM THE FIRST FOUR MONTHS OF KEPLER DATA: GLOBAL OSCILLATION PARAMETERS FOR 800 STARS (2010, methodology): “To obtain a first qualitative analysis of the observed distributions of the Kepler sample, we calculated a synthetic stellar population the same way as Miglio et al. (2009), using the stellar synthesis code TRILEGAL (Girardi et al. 2005).”
• ASTROMETRIC EXOPLANET DETECTION WITH GAIA (2014, methodology): “TRILEGAL (version 1.6) includes five distinct Galaxy components: the thin and thick disks, the halo, the bulge, and the disk extinction layer (Girardi et al. 2005, Section 3.6).”