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Smartt, SJChambers, KCSmith, KWHuber, MEYoung, DRCappellaro, EWright, DECoughlin, MSchultz, ASBDenneau, LFlewelling, HHeinze, AMagnier, EAPrimak, NRest, ASherstyuk, AStalder, BStubbs, CWTonry, JWaters, CWillman, MAnderson, JPBaltay, CBotticella, MTCampbell, HDennefeld, MChen, TWDella Valle, MElias-Rosa, NFraser, MInserra, CKankare, EKotak, RKupfer, THarmanen, JGalbany, LGal-Yam, ALe Guillou, LLyman, JDMaguire, KMitra, ANicholl, MOlivares, FRabinowitz, DRazza, ASollerman, JSmith, MTerreran, GValenti, SGibson, BGoggia, T[Pan-STARRS and PESSTO search for an optical counterpart to the LIGO gravitational-wave source GW150914]Pan-STARRS and PESSTO search for an optical counterpart to the LIGO gravitational-wave source GW150914

We present the first results of the High Cadence Transient Survey (HiTS), a survey for which the objective is to detect and follow-up optical transients with characteristic timescales from hours to days, especially the earliest hours of supernova (SN) explosions. HiTS uses the Dark Energy Camera ...


Forster, FMaureira, JCSan Martin, JHamuy, MMartinez, JHuijse, PCabrera, GGalbany, Lde Jaeger, TGonzalez-Gaitan, SAnderson, JPKunkarayakti, HPignata, GBufano, FLittin, JOlivares, FMedina, GSmith, RCVivas, AKEstevez, PAMunoz, RVera, E[THE HIGH CADENCE TRANSIENT SURVEY (HITS). I. SURVEY DESIGN AND SUPERNOVA SHOCK BREAKOUT CONSTRAINTS]THE HIGH CADENCE TRANSIENT SURVEY (HITS). I. SURVEY DESIGN AND SUPERNOVA SHOCK BREAKOUT CONSTRAINTS

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