REFERENCES

If you use RaveSpan (or a part of it) and publish your results, please cite:

• Mass and p-factor of the type II Cepheid OGLE-LMC-T2CEP-098 in a binary system
  Pilecki, B., Gieren, W., Smolec, S., et al., 2017, ApJ, 842, 110
  arxiv:1704.07782 - ADS:2017ApJ...842..110P

You can also consider citing some of the following papers as examples of the use of the code:

• The Dynamical Mass and Evolutionary Status of the Type II Cepheid in the Eclipsing Binary System OGLE-LMC-T2CEP-211 with a Double-ring Disk
  Pilecki, B., Dervişoğlu, A., Gieren W., et al., 2018, ApJ, 868, 30
  arxiv:1810.06524 - ADS:2018ApJ...868...30P
• The Araucaria Project: High-precision Cepheid astrophysics from the analysis of variables in double-lined eclipsing binaries
  Pilecki, B., Gieren W., Pietrzyński, G., et al., 2018, ApJ, 862, 43
  arxiv:1806.01391 - ADS:2018ApJ...862...43P
• The Araucaria Project: The FO Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-2532
  Pilecki, B., Graczyk, D., Gieren W., et al., 2015, ApJ, 806, 29
  arxiv:1504.04611 - ADS:2015ApJ...806...29P
• Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227
  Pilecki, B., Graczyk, D., Pietrzyński, G., et al., 2013, MNRAS, 436, 953
  arXiv:1308.5023 - ADS:2013MNRAS.436..953P

If you use the provided template spectra library ('slib_coelho05.tgz') , please also cite the following paper:

• A library of high resolution synthetic stellar spectra from 300 nm to 1.8 μm with solar and α-enhanced composition
  Coelho, P., Barbuy, B., Meléndez, J., et al., 2005, A&A, 443, 735
  ADS:2005A&A...443..735C - specmodels.iag.usp.br

Full example of a citation:

"Radial velocities are measured using the [Broadening Function] method implemented in the RaveSpan code written by B. Pilecki (see Appendix in Pilecki et al. 2017b) with template spectra taken from the synthetic spectra library of Coelho et al. (2005). [Preliminary] Orbital solutions are obtained using the same program. [The examples of the application of the RaveSpan code can be found in Pilecki et al. (2013 and/or 2015 and/or 2018).]"