Searching for codes credited to 'Myers, Adam D.'
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[ascl:1302.016]
XDQSO: Photometic quasar probabilities and redshifts
Bovy, Jo;
Hennawi, Joseph F.;
Hogg, David W.;
Myers, Adam D.;
Kirkpatrick, Jessica A.;
Schlegel, David J.;
Ross, Nicholas P.;
Sheldon, Erin S.;
McGreer, Ian D.;
Schneider, Donald P.;
Weaver, Benjamin A.
XDQSO, written in IDL, calculates photometric quasar probabilities to mimick SDSS-III’s BOSS quasar target selection or photometric redshifts for quasars, whether in three redshift ranges (z < 2.2; 2.2 leq z leq 3.5; z > 3.5) or arbitrary redshift ranges.
[ascl:2106.018]
picca: Package for Igm Cosmological-Correlations Analyses
du Mas des Bourboux, Hélion;
Rich, James;
Font-Ribera, Andreu;
de Sainte Agathe, Victoria;
Farr, James;
Etourneau, Thomas;
Le Goff, Jean-Marc;
Cuceu, Andrei;
Balland, Christophe;
Bautista, Julian E.;
Blomqvist, Michael;
Brinkmann, Jonathan;
Brownstein, Joel R.;
Chabanier, Solène;
Chaussidon, Edmond;
Dawson, Kyle;
González-Morales, Alma X.;
Guy, Julien;
Lyke, Brad W.;
de la Macorra, Axel;
Mueller, Eva-Maria;
Myers, Adam D.;
Nitschelm, Christian;
Muñoz Gutiérrez, Andrea;
Palanque-Delabrouille, Nathalie;
Parker, James;
Percival, Will J.;
Pérez-Ràfols, Ignasi;
Petitjean, Patrick;
Pieri, Matthew M.;
Ravoux, Corentin;
Rossi, Graziano;
Schneider, Donald P.;
Seo, Hee-Jong;
Slosar, Anže;
Stermer, Julianna;
Vivek, M.;
Yèche, Christophe;
Youles, Samantha
picca fits continua of forests, computes correlation functions (1D and 3D) and power-spectra (1D), computes covariance matrices, and fits models for the correlation functions. This set of tools is used for the analysis of the Lyman-alpha forest sample from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) and the Dark Energy Spectroscopic Instrument (DESI).
[ascl:2301.025]
desitarget: Selecting DESI targets from photometric catalogs
Myers, Adam D.;
Moustakas, John;
Bailey, Stephen;
Weaver, Benjamin A.;
Cooper, Andrew P.;
Forero-Romero, Jaime E.;
Abolfathi, Bela;
Alexander, David M.;
Brooks, David;
Chaussidon, Edmond;
Chuang, Chia-Hsun;
Dawson, Kyle;
Dey, Arjun;
Dey, Biprateep;
Dhungana, Govinda;
Doel, Peter;
Fanning, Kevin;
Gaztañaga, Enrique;
A Gontcho, Satya Gontcho;
Gonzalez-Morales, Alma X.;
Hahn, ChangHoon;
Herrera-Alcantar, Hiram K.;
Honscheid, Klaus;
Ishak, Mustapha;
Karim, Tanveer;
Kirkby, David;
Kisner, Theodore;
Koposov, Sergey E.;
Kremin, Anthony;
Lan, Ting-Wen;
Landriau, Martin;
Lang, Dustin;
Levi, Michael E.;
Magneville, Christophe;
Napolitano, Lucas;
Martini, Paul;
Meisner, Aaron;
Newman, Jeffrey A.;
Palanque-Delabrouille, Nathalie;
Percival, Will;
Poppett, Claire;
Prada, Francisco;
Raichoor, Anand;
Ross, Ashley J.;
Schlafly, Edward F.;
Schlegel, David;
Schubnell, Michael;
Tan, Ting;
Tarle, Gregory;
Wilson, Michael J.;
Yèche, Christophe;
Zhou, Rongpu;
Zhou, Zhimin;
Zou, Hu
desitarget selects targets for spectroscopic follow-up by Dark Energy Spectroscopic Instrument (DESI). The pipeline uses bitmasks to record that a specific source has been selected by a particular targeting algorithm, setting bit-values in output data files in a number of different columns that indicate whether a particular target meets specific selection criteria. desitarget also outputs a unique TARGETID that allows each target to be tracked throughout the DESI survey. This TARGETID encodes information about each DESI target, such as the catalog the target was selected from, whether a target is a sky location or part of a random catalog, and whether a target is part of a secondary program.