WIYN OPEN CLUSTER STUDY. LXII. COMPARISON OF ISOCHRONE SYSTEMS USING DEEP MULTI-BAND PHOTOMETRY OF M35

By Ben Thompson, P. Frinchaboy, K. Kinemuchi, A. Sarajedini, R. Cohen. 2014

23 citations recorded by the source corpus.

The current generation of stellar isochrone models exhibits non-negligible discrepancies due to variations in the input physics. The success of each model is determined by how well it fits the observations, and this paper aims to disentangle contributions from the various physical inputs. New deep, wide-field optical and near-infrared photometry (UBVRIJHKS) of the cluster M35 is presented, against which several isochrone systems are compared: Padova, PARSEC, Dartmouth, and Y2. Two different atmosphere models are applied to each isochrone: ATLAS9 and BT-Settl. For any isochrone set and atmosphere model, observed data are accurately reproduced for all stars more massive than 0.7 M☉. For stars less massive than 0.7 M☉, Padova and PARSEC isochrones consistently produce higher temperatures than observed. Dartmouth and Y2 isochrones with BT-Settl atmospheres reproduce optical data accurately; however, they appear too blue in IR colors. It is speculated that molecular contributions to stellar spectra in the near-infrared may not be fully explored, and that future study may reconcile these differences.

Subfields: Astronomy and Astrophysics, Instrumentation

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Timothy Morton
2. J. Johnson
3. A. Mann
4. Daniel Foreman-Mackey
5. David W. Hogg
6. D. Latham
7. B. Montet
8. B. Bowler

In Instrumentation

1. Timothy Morton
2. Daniel Foreman-Mackey
3. J. Johnson
4. A. Mann
5. David W. Hogg
6. B. Bowler
7. D. Latham
8. B. Montet

Citations in the corpus

• STELLAR AND PLANETARY PROPERTIES OF K2 CAMPAIGN 1 CANDIDATES AND VALIDATION OF 17 PLANETS, INCLUDING A PLANET RECEIVING EARTH-LIKE INSOLATION (2015, background): “…h e A stro ph y sica l Jo u rn a l, 809:25 (15pp), 2015 A ugust 10 M o n tet et a l. reliance on BT-Settl atmospheres, which are based on incomplete molecular line lists and have been shown to predict near-IR colors that are too blue (Thompson et al. 2014).”