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Dawson, KS;Kneib, J-P;Percival, WJ;Alam, S;Albareti, FD;Anderson, SF;Armengaud, E;Aubourg, E;Bailey, S;Bautista, JE;Berlind, AA;Bershady, MA;Beutler, F;Bizyaev, D;Blanton, MR;Blomqvist, M;Bolton, AS;Boyy, J;Brandt, WN;Brinkmann, J;Brownstein, JR;Burtin, E;Busca, NG;Cai, Z;Chuang, C-H;Clerc, N;Comparat, J;Cope, F;Croft, RAC;Cruz-Gonzalez, I;da Costa, LN;Cousinou, M-C;Darling, J;de la Macorra, A;de la Torre, S;Delubac, T;des Bourboux, HDM;Dwelly, T;Ealet, A;Eisenstein, DJ;Eracleous, M;Escoffier, S;Fan, X;Finoguenov, A;Font-Ribera, A;Frinchaboy, P;Gaulme, P;Georgakakis, A;Green, P;Guo, H;Guy, J;Ho, S;Holder, D;Huehnerhoff, J;Hutchinson, T;Jing, Y;Jullo, E;Kamble, V;Kinemuchi, K;Kirkby, D;Kitaura, F-S;Klaene, MA;Laher, RR;Lang, D;Laurent, P;Le Goff, J-M;Li, C;Liang, Y;Lima, M;Lin, Q;Lin, W;Lin, Y-T;Long, DC;Lundgren, B;MacDonald, N;Maia, MAG;Malanushenko, E;Malanushenko, V;Mariappan, V;McBride, CK;McGreer, ID;Menard, B;Merloni, A;Meza, A;Montero-Dorta, AD;Muna, D;Myers, AD;Nandra, K;Naugle, T;Newman, JA;Noterdaeme, P;Nugent, P;Ogando, N;Olmstead, MD;Oravetz, A;Oravetz, DJ;Padmanabhan, N;Palanque-Delabrouille, N;Pan, K;Parejko, JK;Paris, I;Peacock, JA;Petitjean, P;Pieri, MM;Pisani, A;Prada, F;Prakash, A;Raichoor, A;Reid, B;Rich, J;Ridl, J;Rodriguez-Torres, S;Rosell, AC;Ross, AJ;Rossi, G;Ruan, J;Salvato, M;Sayres, C;Schneider, DP;Schlegel, DJ;Seljak, U;Seo, H-J;Sesar, B;Shandera, S;Shu, Y;Slosar, A;Sobreira, F;Streblyanska, A;Suzuki, N;Taylor, D;Tao, C;Tinker, JL;Tojeiro, R;Vargas-Magana, M;Wang, Y;Weaver, BA;Weinberg, DH;White, M;Wood-Vasey, WM;Yeche, C;Zhai, Z;Zhao, C;Zhao, G-B;Zheng, Z;Zhu, GB;Zou, H
Blanton, MR;Bershady, MA;Abolfathi, B;Albareti, FD;Allende Prieto, C;Almeida, A;Alonso-Garcia, J;Anders, F;Anderson, SF;Andrews, B;Aquino-Ortiz, E;Aragon-Salamanca, A;Argudo-Fernandez, M;Armengaud, E;Aubourg, E;Avila-Reese, V;Badenes, C;Bailey, S;Barger, KA;Barrera-Ballesteros, J;Bartosz, C;Bates, D;Baumgarten, F;Bautista, J;Beaton, R;Beers, TC;Belfiore, F;Bender, CF;Berlind, AA;Bernardi, M;Beutler, F;Bird, JC;Bizyaev, D;Blanc, GA;Blomqvist, M;Bolton, AS;Boquien, M;Borissova, J;Van den Bosch, R;Bovy, J;Brandt, WN;Brinkmann, J;Brownstein, JR;Bundy, K;Burgasser, AJ;Burtin, E;Busca, NG;Cappellari, M;Delgado Carigi, ML;Carlberg, JK;Rosell, AC;Carrera, R;Chanover, NJ;Cherinka, B;Cheung, E;Maqueo Chew, YG;Chiappini, C;Choi, PD;Chojnowski, D;Chuang, C-H;Chung, H;Cirolini, RF;Clerc, N;Cohen, RE;Comparat, J;da Costa, L;Cousinou, M-C;Covey, K;Crane, JD;Croft, RAC;Cruz-Gonzalez, I;Garrido Cuadra, D;Cunha, K;Damke, GJ;Darling, J;Davies, R;Dawson, K;de la Macorra, A;Dell'Agli, F;De Lee, N;Delubac, T;Di Mille, F;Diamond-Stanic, A;Cano-Diaz, M;Donor, J;Jose Downes, J;Drory, N;des Bourboux, HDM;Duckworth, CJ;Dwelly, T;Dyer, J;Ebelke, G;Eigenbrot, AD;Eisenstein, DJ;Emsellem, E;Eracleous, M;Escoffier, S;Evans, ML;Fan, X;Fernandez-Alvar, E;Fernandez-Trincado, JG;Feuillet, DK;Finoguenov, A;Fleming, SW;Font-Ribera, A;Fredrickson, A;Freischlad, G;Frinchaboy, PM;Fuentes, CE;Galbany, L;Garcia-Dias, R;Garcia-Hernandez, DA;Gaulme, P;Geisler, D;Gelfand, JD;Gil-Marin, H;Gillespie, BA;Goddard, D;Gonzalez-Perez, V;Grabowski, K;Green, PJ;Grier, CJ;Gunn, JE;Guo, H;Guy, J;Hagen, A;Hahn, C;Hall, M;Harding, P;Hasselquist, S;Hawley, SL;Hearty, F;Gonzalez Hernandez, JI;Ho, S;Hogg, DW;Holley-Bockelmann, K;Holtzman, JA;Holzer, PH;Huehnerhoff, J;Hutchinson, TA;Hwang, HS;Ibarra-Medel, HJ;Ilha, GDS;Ivans, II;Ivory, K;Jackson, K;Jensen, TW;Johnson, JA;Jones, A;Jonsson, H;Jullo, E;Kamble, V;Kinemuchi, K;Kirkby, D;Kitaura, F-S;Klaene, M;Knapp, GR;Kneib, J-P;Kollmeier, JA;Lacerna, I;Lane, RR;Lang, D;Law, DR;Lazarz, D;Lee, Y;Le Goff, J-M;Liang, F-H;Li, C;Li, H;Lian, J;Lima, M;Lin, L;Lin, Y-T;de Lis, SB;Liu, C;de Icaza Lizaola, MAC;Long, D;Lucatello, S;Lundgren, B;MacDonald, NK;Machado, AD;MacLeod, CL;Mahadevan, S;Geimba Maia, MA;Maiolino, R;Majewski, SR;Malanushenko, E;Malanushenko, V;Manchado, A;Mao, S;Maraston, C;Marques-Chaves, R;Masseron, T;Masters, KL;McBride, CK;McDermid, RM;McGrath, B;McGreer, ID;Medina Pena, N;Melendez, M;Merloni, A;Merrifield, MR;Meszaros, S;Meza, A;Minchev, I;Minniti, D;Miyaji, T;More, S;Mulchaey, J;Muller-Sanchez, F;Muna, D;Munoz, RR;Myers, AD;Nair, P;Nandra, K;do Nascimento, JC;Negrete, A;Ness, M;Newman, JA;Nichol, RC;Nidever, DL;Nitschelm, C;Ntelis, P;O'Connell, JE;Oelkers, RJ;Oravetz, A;Oravetz, D;Pace, Z;Padilla, N;Palanque-Delabrouille, N;Alonso Palicio, P;Pan, K;Parejko, JK;Parikh, T;Paris, I;Park, C;Patten, AY;Peirani, S;Pellejero-Ibanez, M;Penny, S;Percival, WJ;Perez-Fournon, I;Petitjean, P;Pieri, MM;Pinsonneault, M;Pisani, A;Poleski, R;Prada, F;Prakash, A;de Andrade Queiroz, AB;Raddick, MJ;Raichoor, A;Rembold, SB;Richstein, H;Riffel, RA;Riffel, R;Rix, H-W;Robin, AC;Rockosi, CM;Rodriguez-Torres, S;Roman-Lopes, A;Roman-Zuniga, C;Rosado, M;Ross, AJ;Rossi, G;Ruan, J;Ruggeri, R;Rykoff, ES;Salazar-Albornoz, S;Salvato, M;Sanchez, AG;Aguado, DS;Sanchez-Gallego, JR;Santana, FA;Santiago, BX;Sayres, C;Schiavon, RP;Schimoia, JDS;Schlafly, EF;Schlegel, DJ;Schneider, DP;Schultheis, M;Schuster, WJ;Schwope, A;Seo, H-J;Shao, Z;Shen, S;Shetrone, M;Shull, M;Simon, JD;Skinner, D;Skrutskie, MF;Slosar, A;Smith, VV;Sobeck, JS;Sobreira, F;Somers, G;Souto, D;Stark, DV;Stassun, K;Stauffer, F;Steinmetz, M;Storchi-Bergmann, T;Streblyanska, A;Stringfellow, GS;Suarez, G;Sun, J;Suzuki, N;Szigeti, L;Taghizadeh-Popp, M;Tang, B;Tao, C;Tayar, J;Tembe, M;Teske, J;Thakar, AR;Thomas, D;Thompson, BA;Tinker, JL;Tissera, P;Tojeiro, R;Hernandez Toledo, H;de la Torre, S;Tremonti, C;Troup, NW;Valenzuela, O;Martinez Valpuesta, I;Vargas-Gonzalez, J;Vargas-Magana, M;Alberto Vazquez, J;Villanova, S;Vivek, M;Vogt, N;Wake, D;Walterbos, R;Wang, Y;Weaver, BA;Weijmans, A-M;Weinberg, DH;Westfall, KB;Whelan, DG;Wild, V;Wilson, J;Wood-Vasey, WM;Wylezalek, D;Xiao, T;Yan, R;Yang, M;Ybarra, JE;Yeche, C;Zakamska, N;Zamora, O;Zarrouk, P;Zasowski, G;Zhang, K;Zhao, G-B;Zheng, Z;Zheng, Z;Zhou, X;Zhou, Z-M;Zhu, GB;Zoccali, M;Zou, H
We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high re...
Abolfathi, B;Aguado, DS;Aguilar, G;Prieto, CA;Almeida, A;Ananna, TT;Anders, F;Anderson, SF;Andrews, BH;Anguiano, B;Aragon-Salamanca, A;Argudo-Fernandez, M;Armengaud, E;Ata, M;Aubourg, E;Avila-Reese, V;Badenes, C;Bailey, S;Barger, KA;Barrera-Ballesteros, J;Bartosz, C;Bates, D;Baumgarten, F;Bautista, J;Beaton, R;Beers, TC;Belfiore, F;Bender, CF;Bernardi, M;Bershady, MA;Beutler, F;Bird, JC;Bizyaev, D;Blanc, GA;Blanton, MR;Blomqvist, M;Bolton, AS;Boquien, M;Borissova, J;Bovy, J;Diaz, CAB;Brandt, WN;Brinkmann, J;Brownstein, JR;Bundy, K;Burgasser, AJ;Burtin, E;Busca, NG;Canas, CI;Cano-Diaz, M;Cappellari, M;Carrera, R;Casey, AR;Chen, Y;Cherinka, B;Chiappini, C;Choi, PD;Chojnowski, D;Chuang, C-H;Chung, H;Clerc, N;Cohen, RE;Comparat, J;Nascimento, JCD;Costa, LD;Cousinou, M-C;Covey, K;Crane, JD;Cruz-Gonzalez, I;Cunha, K;Damke, GJ;Darling, J;Jr, JWD;Dawson, K;Queiroz, ABDA;Lizaola, MACDI;Macorra, ADL;Torre, SDL;Lee, ND;Agathe, VDS;Machado, AD;Dell'Agli, F;Delubac, T;Diamond-Stanic, AM;Donor, J;Downes, JJ;Drory, N;Bourboux, HDMD;Duckworth, CJ;Dwelly, T;Dyer, J;Ebelke, G;Eigenbrot, AD;Eisenstein, DJ;Elsworth, YP;Emsellem, E;Eracleous, M;Escoffier, S;Fan, X;Alvar, EF;Fernandez-Trincado, JG;Cirolini, RF;Feuillet, D;Fleming, SW;Font-Ribera, A;Freischlad, G;Frinchaboy, P;Chew, YGM;Galbany, L;Perez, AEG;Garcia-Dias, R;Garcia-Hernandez, DA;Gaulme, P;Gelfand, J;Gil-Marin, H;Gillespie, BA;Goddard, D;Gonzalez-Perez, V;Grabowski, K;Green, PJ;Grier, CJ;Gueguen, A;Guo, H;Guy, J;Hagen, A;Harding, P;Hasselquist, S;Hawley, S;Hearty, F;Hekker, S;Hernandez, J;Toledo, HH;Hogg, DW;Holley-Bockelmann, K;Holtzman, J;Hou, J;Hsieh, B-C;Hunt, JAS;Hutchinson, TA;Hwang, HS;Angel, CEJ;Johnson, JA;Jones, A;Jonsson, H;Jullo, E;Khan, FS;Kinemuchi, K;Kirkby, D;IV, CCK;Kitaura, F-S;Knapp, GR;Kneib, J-P;Kollmeier, JA;Lacerna, I;Lane, RR;Lang, D;Law, DR;Goff, J-ML;Lee, Y-B;Li, H;Lian, J;Liang, Y;Lin, L;Long, D;Lucatello, S;Lundgren, B;Mackereth, JT;MacLeod, CL;Mahadevan, S;Maia, MA-G;Majewski, S;Manchado, A;Maraston, C;Mariappan, V;Marques-Chaves, R;Masseron, T;Masters, KL;McDermid, RM;McGreer, ID;Melendez, M;Meneses-Goytia, S;Merloni, A;Merrifield, MR;Meszaros, S;Meza, A;Minchev, I;Minniti, D;Mueller, E-M;Muller-Sanchez, F;Muna, D;Myers, AD;Nair, P;Nandra, K;Ness, M;Newman, JA;Nichol, RC;Nidever, DL;Nitschelm, C;Noterdaeme, P;O'Connell, J;Oelkers, RJ;Oravetz, A;Oravetz, D;Ortiz, EA;Osorio, Y;Pace, Z;Padilla, N;Palanque-Delabrouille, N;Palicio, PA;Pan, H-A;Pan, K;Parikh, T;Paris, I;Park, C;Peirani, S;Pellejero-Ibanez, M;Penny, S;Percival, WJ;Perez-Fournon, I;Petitjean, P;Pieri, MM;Pinsonneault, M;Pisani, A;Prada, F;Prakash, A;Raddick, MJ;Raichoor, A;Rembold, SB;Richstein, H;Riffel, RA;Riffel, R;Rix, H-W;Robin, AC;Torres, SR;Roman-Zuniga, C;Ross, AJ;Rossi, G;Ruan, J;Ruggeri, R;Ruiz, J;Salvato, M;Sanchez, AG;Sanchez, SF;Almeida, JS;Sanchez-Gallego, JR;Santiago, BX;Schiavon, RP;Schimoia, JS;Schlafly, E;Schlegel, D;Schneider, DP;Schuster, WJ;Schwope, A;Seo, H-J;Serenelli, A;Shen, S;Shen, Y;Shetrone, M;Shull, M;Aguirre, VS;Simon, JD;Skrutskie, M;Slosar, A;Smethurst, R;Smith, V;Sobeck, J;Somers, G;Souter, BJ;Souto, D;Spindler, A;Stark, DV;Stassun, K;Steinmetz, M;Stello, D;Storchi-Bergmann, T;Streblyanska, A;Stringfellow, G;Suarez, G;Sun, J;Szigeti, L;Taghizadeh-Popp, M;Talbot, MS;Tang, B;Tao, C;Tayar, J;Tembe, M;Thomas, D;Tissera, P;Tojeiro, R;Tremonti, C;Troup, NW;Valenzuela, O;Bosch, RVD;Vargas-Gonzalez, J;Vargas-Magana, M;Vazquez, JA;Villanova, S;Vogt, N;Wake, D;Wang, Y;Weaver, BA;Weijmans, A-M;Westfall, KB;Whelan, DG;Wilcots, E;Wild, V;Williams, RA;Wilson, J;Wood-Vasey, WM;Wylezalek, D;Xiao, T;Yan, R;Yang, M;Ybarra, JE;Yeche, C;Zakamska, N;Zamora, O;Zarrouk, P;Zasowski, G;Zhang, K;Zhao, C;Zhao, G-B;Zheng, Z;Zhou, Z-M;Zhu, G;Zinn, JC;Zou, H
The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) has been in operation since July 2014. This paper describes the second data release from this phase, and the fourteenth from SDSS overall (making this, Data Release Fourteen or DR14). Th...
We present improved methodology for including covariance matrices in the error budget of Baryon Oscillation Spectroscopic Survey (BOSS) galaxy clustering measurements, revisiting Data Release 9 (DR9) analyses, and describing a method that is used in ...
Extraction of the Baryon Acoustic Oscillations (BAO) to per cent level accuracy is challenging and demands an understanding of many potential systematics to an accuracy well below 1 per cent, in order to ensure that they do not combine significantly ...
We present the distance measurement to z = 0.32 using the eleventh data release (DR) of the Sloan Digital Sky Survey-III Baryon Acoustic Oscillation Survey (BOSS). We use 313 780 galaxies of the low-redshift (LOWZ) sample over 7341 square degrees to ...
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references updated; 26 pages, 15 figures. Submitted to MNRAS