Making the most of big qualitative datasets: a living systematic review of analysis methods by Chandrasekar, A, Clark, SE, Martin, S, Vanderslott, S, Flores, EC, Aceituno, D, Barnett, P, Vindrola-Padros, C, Vera San Juan, N

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). VII. A Tomographic View of Far-infrared and Radio Polarimetric Observations through MHD Simulations of Galaxies by Martin-Alvarez, S, Lopez-Rodriguez, E, Dacunha, T, Clark, SE, Borlaff, AS, Beck, R, Rodríguez Montero, F, Jung, SL, Devriendt, J, Slyz, A, Roman-Duval, JC, Ntormousi, E, Tahani, M, Subramanian, K, Dale, DA, Marcum, PM, Tassis, K, del Moral-Castro, I, Tram, LN, Jarvis, MJ

The Atacama Cosmology Telescope: a measurement of the cosmic microwave background power spectra at 98 and 150 GHz by Choi, SK, Hasselfield, M, Ho, S-PP, Koopman, B, Lungu, M, Abitbol, MH, Addison, GE, Ade, PAR, Aiola, S, Amiri, M, Amodeo, S, Angile, E, Austermann, JE, Baildon, T, Battaglia, N, Beall, JA, Bean, R, Becker, DT, Bond, JR, Bruno, SM, Calabrese, E, Calafut, V, Campusano, LE, Carrero, F, Chesmore, GE, Cho, H-M, Clark, SE, Cothard, NF, Crichton, D, Crowley, KT, Darwish, O, Datta, R, Denison, EV, Devlin, MJ, Duell, CJ, Duff, SM, Duivenvoorden, AJ, Dunkley, J, Dünner, R, Essinger-Hileman, T, Fankhanel, M, Ferraro, S, Fox, AE, Fuzia, B, Gallardo, PA, Gluscevic, V, Golec, JE, Grace, E, Et al.

The Atacama Cosmology Telescope: DR4 maps and cosmological parameters by Aiola, S, Calabrese, E, Maurin, L, Naess, S, Schmitt, BL, Abitbol, MH, Addison, GE, Ade, PAR, Alonso, D, Amiri, M, Amodeo, S, Angile, E, Austermann, JE, Baildon, T, Battaglia, N, Beall, JA, Bean, R, Becker, DT, Bond, JR, Bruno, SM, Calafut, V, Campusano, LE, Carrero, F, Chesmore, GE, Cho, H-M, Choi, SK, Clark, SE, Cothard, NF, Crichton, D, Crowley, KT, Darwish, O, Datta, R, Denison, EV, Devlin, MJ, Duell, CJ, Duff, SM, Duivenvoorden, AJ, Dunkley, J, Dünner, R, Essinger-Hileman, T, Fankhanel, M, Ferraro, S, Fox, AE, Fuzia, B, Gallardo, PA, Gluscevic, V, Golec, JE, Grace, E, Gralla, M, Guan, Y