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Searching for codes credited to 'Smith, M.'

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Found 4 codes.

[ascl:2511.004] HyperGal: Supernovae extraction and classification
Lezmy, J.; Copin, Y.; Rigault, M.; Smith, M.; Neill, J. D.
HyperGal models fully chromatic scenes by using pre-transient photometric images to generate a hyperspectral representation of a host galaxy. It applies the CIGALE SED fitter (ascl:1111.004) as a physically motivated spectral interpolator to construct the galaxy model. The galaxy model, complemented by a point source and a diffuse background component, is projected onto the SEDm spectro-spatial observation space and adjusted to observations.
[ascl:2405.001] SPEDAS: Space Physics Environment Data Analysis System
Angelopoulos, V.; Cruce, P.; Drozdov, A.; Grimes, E. W.; Hatzigeorgiu, N.; King, D. A.; Larson, D.; Lewis, J. W.; McTiernan, J. M.; Roberts, D. A.; Russell, C. L.; Hori, T.; Kasahara, Y.; Kumamoto, A.; Matsuoka, A.; Miyashita, Y.; Miyoshi, Y.; Shinohara, I.; Teramoto, M.; Faden, J. B.; Halford, A. J.; McCarthy, M.; Millan, R. M.; Sample, J. G.; Smith, D. M.; Woodger, L. A.; Masson, A.; Narock, A. A.; Asamura, K.; Chang, T. F.; Chiang, C. Y.; Kazama, Y.; Keika, K.; Matsuda, S.; Segawa, T.; Seki, K.; Shoji, M.; Tam, S. W. Y.; Umemura, N.; Wang, B. J.; Wang, S. Y.; Redmon, R.; Rodriguez, J. V.; Singer, H. J.; Vandegriff, J.; Abe, S.; Nose, M.; Shinbori, A.; Tanaka, Y. M.; UeNo, S.; Andersson, L.; Dunn, P.; Fowler, C.; Halekas, J. S.; Hara, T.; Harada, Y.; Lee, C. O.; Lillis, R.; Mitchell, D. L.; Argall, M. R.; Bromund, K.; Burch, J. L.; Cohen, I. J.; Galloy, M.; Giles, B.; Jaynes, A. N.; Le Contel, O.; Oka, M.; Phan, T. D.; Walsh, B. M.; Westlake, J.; Wilder, F. D.; Bale, S. D.; Livi, R.; Pulupa, M.; Whittlesey, P.; DeWolfe, A.; Harter, B.; Lucas, E.; Auster, U.; Bonnell, J. W.; Cully, C. M.; Donovan, E.; Ergun, R. E.; Frey, H. U.; Jackel, B.; Keiling, A.; Korth, H.; McFadden, J. P.; Nishimura, Y.; Plaschke, F.; Robert, P.; Turner, D. L.; Weygand, J. M.; Candey, R. M.; Johnson, R. C.; Kovalick, T.; Liu, M. H.; McGuire, R. E.; Breneman, A.; Kersten, K.; Schroeder, P.
The SPEDAS (Space Physics Environment Data Analysis Software) framework supports multi-mission data ingestion, analysis and visualization for the Space Physics community. It standardizes the retrieval of data from distributed repositories, the scientific processing with a powerful set of legacy routines, the quick visualization with full output control and the graph creation for use in papers and presentations. SPEDAS includes a GUI for ease of use by novice users, works on multiple platforms, and though based on IDL, can be used with or without an IDL license. The framework supports plugin modules for multiple projects such as THEMIS, MMS, and WIND, and provides interfaces for software modules developed by the individual teams of those missions. A Python implementation of the framework, PySPEDAS (ascl:2405.005), is also available.
[ascl:2312.034] pycheops: Light curve analysis for ESA CHEOPS data
Maxted, P. F. L.; Ehrenreich, D.; Wilson, T. G.; Alibert, Y.; Cameron, A. Collier; Hoyer, S.; Sousa, S. G.; Olofsson, G.; Bekkelien, A.; Deline, A.; Delrez, L.; Bonfanti, A.; Borsato, L.; Alonso, R.; Anglada Escudé, G.; Barrado, D.; Barros, S. C. C.; Baumjohann, W.; Beck, M.; Beck, T.; Benz, W.; Billot, N.; Biondi, F.; Bonfils, X.; Brandeker, A.; Broeg, C.; Bárczy, T.; Cabrera, J.; Charnoz, S.; Corral Van Damme, C.; Csizmadia, Sz; Davies, M. B.; Deleuil, M.; Demangeon, O. D. S.; Demory, B. -O.; Erikson, A.; Florén, H. G.; Fortier, A.; Fossati, L.; Fridlund, M.; Futyan, D.; Gandolfi, D.; Gillon, M.; Guedel, M.; Guterman, P.; Heng, K.; Isaak, K. G.; Kiss, L.; Laskar, J.; Lecavelier des Etangs, A.; Lendl, M.; Lovis, C.; Magrin, D.; Nascimbeni, V.; Ottensamer, R.; Pagano, I.; Pallé, E.; Peter, G.; Piotto, G.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Reimers, C.; Ribas, I.; Salmon, S.; Santos, N. C.; Scandariato, G.; Simon, A. E.; Smith, A. M. S.; Steller, M.; Swayne, M. I.; Szabó, Gy M.; Ségransan, D.; Thomas, N.; Udry, S.; Van Grootel, V.; Walton, N. A.
pycheops analyzes CHEOPS light curve data. The models in the package can also be applied to other types of data. pycheops includes a "cook book" and examples; in addition, it provides a command-line tool that aids in the preparation of observing requests for CHEOPS observers.
[ascl:2202.013] PSLS: PLATO Solar-like Light-curve Simulator
Samadi, R.; Deru, A.; Reese, D.; Marchiori, V.; Grolleau, E.; Green, J. J.; Pertenais, M.; Lebreton, Y.; Deheuvels, S.; Mosser, B.; Belkacem, K.; Börner, A.; Smith, A. M. S.
PSLS simulates solar-like oscillators representative of PLATO targets. It includes planetary transits, stochastically-excited oscillations, granulation and activity background components, as well as instrumental systematic errors and random noises representative for PLATO.