Couplings of ${{\mathit W}^{\,'}}$ to quarks and leptons are taken to be identical with those of ${{\mathit W}}$. The following limits are obtained from ${{\mathit p}}{{\overline{\mathit p}}}$ or ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit W}^{\,'}}$ X with ${{\mathit W}^{\,'}}$ decaying to the mode indicated in the comments. New decay channels ($\mathit e.g.$, ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$) are assumed to be suppressed. The most recent preliminary results can be found in the “${{\mathit W}^{\,'}}$-boson searches” review above.

VALUE (GeV) CL% DOCUMENT ID TECN  COMMENT $\bf{ > 6000}$ OUR LIMIT $\text{none 500 - 5000}$ 95 1 AAD 2024 T ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \nu}}$ $\text{none 2000 - 4300}$ 95 2 HAYRAPETYAN 2024 X CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $>2500$ 95 3 AAD 2023 AH ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 500 - 4600}$ 95 4 AAD 2023 CC ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $> 1200$ 95 5 AAD 2023 L ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit X}}$ $\text{none 400 - 3300}$ 95 6 AAD 2023 O ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $>4400$ 95 7 TUMASYAN 2023 AP CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $>4000$ 95 8 TUMASYAN 2023 AP CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 600 - 4800}$ 95 9 TUMASYAN 2023 AW CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \nu}}$ $> 5700$ 95 10 TUMASYAN 2022 AC CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ , ${{\mathit \mu}}{{\mathit \nu}}$ $> 3900$ 95 11 TUMASYAN 2022 D CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $> 4000$ 95 11 TUMASYAN 2022 D CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 1000 - 4000}$ 95 12 TUMASYAN 2022 J CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 500 - 2000}$ 95 13 TUMASYAN 2022 R CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 1000 - 3400}$ 95 14 SIRUNYAN 2021 Y CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $> 3200$ 95 15 AAD 2020 AJ ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $> 4300$ 95 16 AAD 2020 AT ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 1100 - 4000}$ 95 17 AAD 2020 T ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 1800 - 3600}$ 95 18 SIRUNYAN 2020 AI CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 1200 - 3800}$ 95 19 SIRUNYAN 2020 Q CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 500 - 3250}$ 95 20 AABOUD 2019 E ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\bf{> 6000}$ 95 21 AAD 2019 C ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ , ${{\mathit \mu}}{{\mathit \nu}}$ $\text{none 1300 - 3600}$ 95 22 AAD 2019 D ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 400 - 4000}$ 95 23 SIRUNYAN 2019 AY CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \nu}}$ $> 4300$ 95 24 SIRUNYAN 2019 CP CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$, ${{\mathit W}}{{\mathit H}}$, ${{\mathit \ell}}{{\mathit \nu}}$ $> 2600$ 95 25 SIRUNYAN 2019 I CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 1000 - 3000}$ 95 26 AABOUD 2018 AF ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 500 - 2820}$ 95 27 AABOUD 2018 AI ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 300 - 3000}$ 95 28 AABOUD 2018 AK ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 800 - 3200}$ 95 29 AABOUD 2018 AL ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $> 5100$ 95 30 AABOUD 2018 BG ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ , ${{\mathit \mu}}{{\mathit \nu}}$ $\text{none 250 - 2460}$ 95 31 AABOUD 2018 CH ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 1200 - 3300}$ 95 32 AABOUD 2018 F ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 500 - 3700}$ 95 33 AABOUD 2018 K ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \nu}}$ $\text{none 1000 - 3600}$ 95 34 SIRUNYAN 2018 CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 1000 - 3050}$ 95 35 SIRUNYAN 2018 AX CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 400 - 5200}$ 95 36 SIRUNYAN 2018 AZ CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ , ${{\mathit \mu}}{{\mathit \nu}}$ $\text{none 1000 - 3400}$ 95 37 SIRUNYAN 2018 BK CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 600 - 3300}$ 95 38 SIRUNYAN 2018 BO CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 800 - 2330}$ 95 39 SIRUNYAN 2018 DJ CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $> 2800$ 95 40 SIRUNYAN 2018 ED CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 1200 - 3200, 3300 - 3600}$ 95 41 SIRUNYAN 2018 P CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $>3600$ 95 42 AABOUD 2017 AK ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 1100 - 2500}$ 95 43 AABOUD 2017 AO ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $> 2220$ 95 44 AABOUD 2017 B ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $> 2300$ 95 45 KHACHATRYAN 2017 J CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}_{{{\tau}}}}$ ${{\mathit \tau}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \tau}}{{\mathit j}}{{\mathit j}}$ $\text{none 600 - 2700}$ 95 46 KHACHATRYAN 2017 W CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $> 4100$ 95 47 KHACHATRYAN 2017 Z CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ , ${{\mathit \mu}}{{\mathit \nu}}$ $> 2200$ 95 48 SIRUNYAN 2017 A CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $>2300$ 95 49 SIRUNYAN 2017 AK CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ , ${{\mathit W}}{{\mathit H}}$ $> 2900$ 95 50 SIRUNYAN 2017 H CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit N}}$ $> 2600$ 95 51 SIRUNYAN 2017 I CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $>2450$ 95 52 SIRUNYAN 2017 R CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 2780 - 3150}$ 95 52 SIRUNYAN 2017 R CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $> 2600$ 95 53 AABOUD 2016 AE ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $> 4070$ 95 54 AABOUD 2016 V ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$, ${{\mathit \mu}}{{\mathit \nu}}$ $>1810$ 95 55 AAD 2016 R ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $>2600$ 95 56 AAD 2016 S ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $> 2150$ 95 57 KHACHATRYAN 2016 AO CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 1000 - 1600}$ 95 58 KHACHATRYAN 2016 AP CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 800 - 1500}$ 95 59 KHACHATRYAN 2016 BD CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\mathit \ell}}{{\mathit \nu}}$ $\text{none 1500 - 2600}$ 95 60 KHACHATRYAN 2016 K CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 500 - 1600}$ 95 61 KHACHATRYAN 2016 L CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 300 - 2700}$ 95 62 KHACHATRYAN 2016 O CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \nu}}$ $\text{none 400 - 1590}$ 95 63 AAD 2015 AU ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 1500 - 1760}$ 95 64 AAD 2015 AV ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 300 - 1490}$ 95 65 AAD 2015 AZ ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 1300 - 1500}$ 95 66 AAD 2015 CP ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 500 - 1920}$ 95 67 AAD 2015 R ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 800 - 2450}$ 95 68 AAD 2015 V ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $> 1470$ 95 69 KHACHATRYAN 2015 C CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $>3710$ 95 70 KHACHATRYAN 2015 T CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$, ${{\mathit \mu}}{{\mathit \nu}}$ $\text{none 1000 - 3010}$ 95 71 KHACHATRYAN 2014 O CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit j}}{{\mathit j}}$ • • We do not use the following data for averages, fits, limits, etc. • • $> 4400$ 95 72 AAD 2024 AE ATLS $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$ 73 AAD 2024 CM ATLS Dark ${{\mathit \rho}_{{{D}}}^{\pm}}$ 74 HAYRAPETYAN 2024 AV CMS ${{\mathit X}}$ $\rightarrow$ ${{\mathit W}}{{\mathit \gamma}}$ 75 AAD 2023 BF ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}}$ 76 AAD 2023 CG ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit j}}{{\mathit j}}$ 77 AAD 2023 CK ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit X}}{{\mathit H}}$ 78 AAD 2023 U ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit \gamma}}$ 79 TUMASYAN 2022 CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit R}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}{{\mathit W}}$ 80 TUMASYAN 2022 AL CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit B}}$ , ${{\mathit b}}{{\mathit T}}$ 81 TUMASYAN 2022 B CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit \gamma}}$ 82 TUMASYAN 2022 I CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit R}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}{{\mathit W}}$ 83 TUMASYAN 2022 P CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit j}}{{\mathit j}}$ 84 AAD 2020 AD ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit J}}{{\mathit J}}$ 85 AAD 2020 W ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}}$ 86 AABOUD 2019 B ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit j}}{{\mathit j}}$ 87 AABOUD 2019 BB ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit j}}{{\mathit \ell}}{{\mathit \ell}}$ 88 SIRUNYAN 2019 V CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit B}}{{\mathit t}}$ , ${{\mathit T}}{{\mathit b}}$ 89 AABOUD 2018 AA ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit \gamma}}$ 90 AABOUD 2018 AD ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit H}}{{\mathit X}}$ $> 4500$ 95 91 AABOUD 2018 CJ ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$, ${{\mathit W}}{{\mathit H}}$, ${{\mathit \ell}}{{\mathit \nu}}$ $\text{none 900 - 4400}$ 95 92 SIRUNYAN 2018 CV CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit j}}{{\mathit j}}$ 93 KHACHATRYAN 2017 U CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ 94 AAD 2015 BB ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$ $\text{none 300 - 880}$ 95 95 AALTONEN 2015 C CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 1200 - 1900 and 2000 - 2200}$ 95 96 KHACHATRYAN 2015 V CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $>3240$ 95 AAD 2014 AI ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$, ${{\mathit \mu}}{{\mathit \nu}}$ 97 AAD 2014 AT ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit \gamma}}$ $\text{none 200 - 1520}$ 95 98 AAD 2014 S ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 1000 - 1700}$ 95 99 KHACHATRYAN 2014 CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ 100 KHACHATRYAN 2014 A CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 500 - 950}$ 95 101 AAD 2013 AO ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 1100 - 1680}$ 95 AAD 2013 D ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 1000 - 1920}$ 95 CHATRCHYAN 2013 A CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ 102 CHATRCHYAN 2013 AJ CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $> 2900$ 95 103 CHATRCHYAN 2013 AQ CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$, ${{\mathit \mu}}{{\mathit \nu}}$ $\text{none 800 - 1510}$ 95 104 CHATRCHYAN 2013 E CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 700 - 940}$ 95 105 CHATRCHYAN 2013 U CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 700 - 1130}$ 95 106 AAD 2012 AV ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 200 - 760}$ 95 107 AAD 2012 BB ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ 108 AAD 2012 CK ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\overline{\mathit t}}}{{\mathit q}}$ $> 2550$ 95 109 AAD 2012 CR ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$, ${{\mathit \mu}}{{\mathit \nu}}$ 110 AAD 2012 M ATLS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit j}}{{\mathit j}}$ 111 AALTONEN 2012 N CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\overline{\mathit t}}}{{\mathit q}}$ $\text{none 200 - 1143}$ 95 107 CHATRCHYAN 2012 AF CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ 112 CHATRCHYAN 2012 AR CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\overline{\mathit t}}}{{\mathit q}}$ 113 CHATRCHYAN 2012 BG CMS ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \ell}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit j}}{{\mathit j}}$ $> 1120$ 95 AALTONEN 2011 C CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ $\text{none 180 - 690}$ 95 114 ABAZOV 2011 H D0 ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 600 - 863}$ 95 115 ABAZOV 2011 L D0 ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 285 - 516}$ 95 116 AALTONEN 2010 N CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $\text{none 280 - 840}$ 95 117 AALTONEN 2009 AC CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $> 1000$ 95 ABAZOV 2008 C D0 ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ $\text{none 300 - 800}$ 95 ABAZOV 2004 C D0 ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $\text{none 225 - 536}$ 95 118 ACOSTA 2003 B CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ $\text{none 200 - 480}$ 95 119 AFFOLDER 2002 C CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ $>786$ 95 120 AFFOLDER 2001 I CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$, ${{\mathit \mu}}{{\mathit \nu}}$ $\text{none 300 - 420}$ 95 121 ABE 1997 G CDF ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ $>720$ 95 122 ABACHI 1996 C D0 ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ $>610$ 95 123 ABACHI 1995 E D0 ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$, ${{\mathit \tau}}{{\mathit \nu}}$ $\text{none 260 - 600}$ 95 124 RIZZO 1993 RVUE ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ 1  AAD 2024T limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ =1 3 TeV. Bosonic decays of ${{\mathit W}^{\,'}}$ and ${{\mathit W}}−{{\mathit W}^{\,'}}$ interference are neglected. See their Fig. 7a for limits on $\sigma \cdot{}B$. 2  HAYRAPETYAN 2024X search for right-handed ${{\mathit W}^{\,'}}$ decaying to ${{\mathit t}}{{\mathit b}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 7 for limits on $\sigma \cdot{}B$. 3  AAD 2023AH search for resonances produced through Drell-Yan and vector-boson-fusion processes in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 7 and Fig. 8 for limits on $\sigma \cdot{}B$. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3 produced mainly via Drell-Yan. 4  AAD 2023CC search for resonances decaying to ${{\mathit t}}{{\mathit b}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for right-handed ${{\mathit W}^{\,'}}$ assuming a ${{\mathit W}^{\,'}}$ coupling equal to the SM ${{\mathit W}}$ coupling. The limit becomes ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 4200 GeV for left-handed ${{\mathit W}^{\,'}}$. See their Figs. 12 and 13 for limits on $\sigma \cdot{}B$. 5  AAD 2023L perform a generic search for resonances with events containing a ${{\mathit Z}}$ decaying into ${{\mathit e}^{+}}{{\mathit e}^{-}}$ or ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Figs. 6, 7, 8 for model independent limits on $\sigma \cdot{}B$ for Gaussian-shaped resonances. The limit above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ decaying to ${{\mathit W}}{{\mathit Z}}$ with ${{\mathit g}_{{{V}}}}$ = 3 as well as with ${{\mathit g}_{{{V}}}}$ = 1. 6  AAD 2023O search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2950 GeV for ${{\mathit g}_{{{V}}}}$ = 1. 7  TUMASYAN 2023AP search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 4.8 TeV assuming ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ = ${{\mathit M}}_{{{\mathit Z}^{\,'}}}$ and combining ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$, ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$, ${{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}$, ${{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit H}}$ channels. 8  TUMASYAN 2023AP search for resonances decaying to ${{\mathit W}}{{\mathit H}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 4.8 TeV assuming ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ = ${{\mathit M}}_{{{\mathit Z}^{\,'}}}$ and combining ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$, ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}$, ${{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}$, ${{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit H}}$ channels. 9  TUMASYAN 2023AW search for SSM ${{\mathit W}^{\,'}}$ resonance decaying to ${{\mathit \tau}}{{\mathit \nu}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}}-{{\mathit W}^{\,'}}$ intereference and bosonic decays of ${{\mathit W}^{\,'}}$ are not included. See their Fig. 6 for limits on $\sigma \cdot{}B$. 10  TUMASYAN 2022AC search for ${{\mathit W}^{\,'}}$ with SM-like couplings in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The diboson decays of ${{\mathit W}^{\,'}}$ are assumed to be suppressed. See their Fig. 5 for limits on $\sigma \cdot{}B$. 11  TUMASYAN 2022D search for resonances produced through Drell-Yan and vector-boson-fusion processes in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 8 for limits on $\sigma \cdot{}B$. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3 produced mainly via Drell-Yan. 12  TUMASYAN 2022J search for resonances produced through Drell-Yan and vector-boson-fusion processes in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3, produced mainly via Drell-Yan. See their Fig. 9 for limits on $\sigma \cdot{}B$. 13  TUMASYAN 2022R search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ produced mainly via Drell-Yan. See their Fig. 8 for limits on $\sigma \cdot{}B$. 14  SIRUNYAN 2021Y search for resonances decaying to ${{\mathit t}}{{\mathit b}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 2 for limits on ${{\mathit \sigma}}\cdot{}$ B(${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$). 15  AAD 2020AJ search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes M$_{{{\mathit W}^{\,'}}}$ $>$ 2900 GeV for ${{\mathit g}_{{{V}}}}$ = 1. See their Fig. 6 for limits on $\sigma \cdot{}B$. 16  AAD 2020AT search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 3900 GeV for ${{\mathit g}_{{{V}}}}$ = 1. See their Fig. 13 for limits on $\sigma \cdot{}B$. 17  AAD 2020T search for ${{\mathit W}^{\,'}}$ with SM-like couplings in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 4(c) for limits on the product of the cross section, acceptance, and branching fraction. 18  SIRUNYAN 2020AI limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. 19  SIRUNYAN 2020Q search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. 20  AABOUD 2019E search for right-handed ${{\mathit W}^{\,'}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 8 for limit on on $\sigma \cdot{}\mathit B$. 21  AAD 2019C search for ${{\mathit W}^{\,'}}$ with SM-like couplings in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. Bosonic decays and ${{\mathit W}}−{{\mathit W}^{\,'}}$ interference are neglected. The limits on ${{\mathit e}}$ and ${{\mathit \mu}}$ separately are 6.0 and 5.1 TeV respectively. See their Fig. 2 for limits on $\sigma \cdot{}B$. 22  AAD 2019D search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3400 GeV for ${{\mathit g}_{{{V}}}}$ = 1. If we assume $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$, the limit increases $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3800 GeV and $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3500 GeV for ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit g}_{{{V}}}}$ = 1, respectively. See their Fig. 9 for limits on $\sigma \cdot{}B$. 23  SIRUNYAN 2019AY limits shown for ${{\mathit W}^{\,'}}$ with SM-like coupling using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}}−{{\mathit W}^{\,'}}$ interference and bosonic decays of ${{\mathit W}^{\,'}}$ are not included. See their Fig. 5 for limits on $\sigma \cdot{}\mathit B$. Limits in the context of a nonuniversal gauge interaction are shown in Fig. 7. Model independent limits on ${{\mathit \sigma}}{{\mathit B}}{{\mathit A}}{{\mathit \epsilon}}$ can be seen in Fig. 8. 24  SIRUNYAN 2019CP present a statistical combinations of searches for ${{\mathit W}^{\,'}}$ decaying to pairs of bosons or leptons in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. If we assume ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ = ${{\mathit M}}_{{{\mathit Z}^{\,'}}}$, the limit becomes ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 4500 GeV for ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 5000 GeV for ${{\mathit g}_{{{V}}}}$ = 1. See their Figs. 2 and 3 for limits on $\sigma \cdot{}B$. 25  SIRUNYAN 2019I search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2800 GeV if we assume $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$. 26  AABOUD 2018AF give the limit above for right-handed ${{\mathit W}^{\,'}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. These limits also exclude ${{\mathit W}}$ bosons with left-handed couplings with masses below 2.9 TeV, at the 95$\%$ confidence level. ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}_{{{R}}}}$ is assumed to be forbidden. See their Fig.5 for limits on $\sigma \cdot{}{{\mathit B}}$ for both cases of left- and right-handed ${{\mathit W}^{\,'}}$. 27  AABOUD 2018AI search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2670 GeV for ${{\mathit g}_{{{V}}}}$ = 1. If we assume $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$, the limit increases $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2930 GeV and $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2800 GeV for ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit g}_{{{V}}}}$ = 1, respectively. See their Fig. 5 for limits on $\sigma \cdot{}\mathit B$. 28  AABOUD 2018AK search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2800 GeV for ${{\mathit g}_{{{V}}}}$ = 1. 29  AABOUD 2018AL search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2900 GeV for ${{\mathit g}_{{{V}}}}$ = 1. 30  AABOUD 2018BG limit is for ${{\mathit W}^{\,'}}$ with SM-like couplings using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. Bosonic decays of ${{\mathit W}^{\,'}}$ and ${{\mathit W}}−{{\mathit W}^{\,'}}$ interference are neglected. See Fig. 2 for limits on $\sigma \cdot{}{{\mathit B}}$. 31  AABOUD 2018CH search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2260 GeV for ${{\mathit g}_{{{V}}}}$ = 1. 32  AABOUD 2018F search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3000 GeV for ${{\mathit g}_{{{V}}}}$ = 1. If we assume $\mathit M_{{{\mathit Z}^{\,'}}}$ = $\mathit M_{{{\mathit W}^{\,'}}}$, the limit increases $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3500 GeV and $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3100 GeV for ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit g}_{{{V}}}}$ = 1, respectively. See their Fig.5 for limits on $\sigma \cdot{}{{\mathit B}}$. 33  AABOUD 2018K limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}}−{{\mathit W}^{\,'}}$ interference and bosonic decays of ${{\mathit W}^{\,'}}$ are not included. See their Fig. 4 for limit on $\sigma \cdot{}{{\mathit B}}$. 34  SIRUNYAN 2018 limit is for right-handed ${{\mathit W}^{\,'}}$ using $pp$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}_{{{R}}}}$ decay is assumed to be forbidden. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3.4 TeV if $\mathit M_{{{\mathit \nu}_{{{R}}}}}{}\ll$ $\mathit M_{{{\mathit W}^{\,'}}}$. See their Fig. 5 for exclusion limits on ${{\mathit W}^{\,'}}$ models having both left- and right-handed couplings. 35  SIRUNYAN 2018AX search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. See their Fig.6 for limits on $\sigma \cdot{}$B. 36  SIRUNYAN 2018AZ limit is derived for ${{\mathit W}^{\,'}}$ with SM-like coupling using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. No interference with SM ${{\mathit W}}$ process is considered. The bosonic decays are assumed to be negligible. See their Fig.6 for limits on $\sigma \cdot{}B$. 37  SIRUNYAN 2018BK search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes M$_{{{\mathit W}^{\,'}}}>$ 3100 GeV for ${{\mathit g}_{{{V}}}}$ = 1. 38  SIRUNYAN 2018BO limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. 39  SIRUNYAN 2018DJ search for resonances decaying to $WZ$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2270 GeV for ${{\mathit g}_{{{V}}}}$ = 1. 40  SIRUNYAN 2018ED search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit above is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. If we assume $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$, the limit increases $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2900 GeV and $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2800 GeV for ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit g}_{{{V}}}}$ = 1, respectively. 41  SIRUNYAN 2018P give this limit for a heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. If they assume $\mathit M_{{{\mathit Z}^{\,'}}}$ = $\mathit M_{{{\mathit W}^{\,'}}}$, the limit increases to $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 3800 GeV. 42  AABOUD 2017AK search for a new resonance decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit above is for a ${{\mathit W}^{\,'}}$ boson having axial-vector SM couplings and decaying to quarks with 75$\%$ branching fraction. 43  AABOUD 2017AO search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for a ${{\mathit W}^{\,'}}$ in the heavy-vector-triplet model with ${{\mathit g}_{{{V}}}}$ = 3. See their Fig.4 for limits on $\sigma \cdot{}{{\mathit B}}$. 44  AABOUD 2017B search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ (${{\mathit H}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit c}}{{\overline{\mathit c}}}$; ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$) in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 1750 GeV for ${{\mathit g}_{{{V}}}}$ = 1. If we assume ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ = ${{\mathit M}}_{{{\mathit Z}^{\,'}}}$, the limit increases ${{\mathit M}}_{{{\mathit W}^{\,'}}}>$ 2310 GeV and ${{\mathit M}}_{{{\mathit W}^{\,'}}}>$ 1730 GeV for ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit g}_{{{V}}}}$ = 1, respectively. See their Fig.3 for limits on ${{\mathit \sigma}}\cdot{}{{\mathit B}}$. 45  KHACHATRYAN 2017J search for right-handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \tau}}$ and hypothetical heavy neutrino ${{\mathit N}_{{{\tau}}}}$, with ${{\mathit N}_{{{\tau}}}}$ decaying into ${{\mathit \tau}}{{\mathit j}}{{\mathit j}}$. The quoted limit is for $\mathit M_{{{\mathit N}_{{{\tau}}}}}$ = $\mathit M_{{{\mathit W}_{{{R}}}}}$/2. The limit becomes $\mathit M_{{{\mathit W}_{{{R}}}}}$ $>$ 2350 GeV (1630 GeV) for $\mathit M_{{{\mathit W}_{{{R}}}}}/\mathit M_{{{\mathit N}_{{{\tau}}}}}$ = 0.8 (0.2). See their Fig. 4 for excluded regions in the $\mathit M_{{{\mathit W}_{{{R}}}}}−\mathit M_{{{\mathit N}_{{{\tau}}}}}$ plane. 46  KHACHATRYAN 2017W search for resonances decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. 47  KHACHATRYAN 2017Z limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The bosonic decays of ${{\mathit W}^{\,'}}$ and the interference with SM ${{\mathit W}}$ process are neglected. 48  SIRUNYAN 2017A search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ with ${{\mathit W}}$ ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}}$, ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit q}}{{\overline{\mathit q}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2000 GeV for ${{\mathit g}_{{{V}}}}$ = 1. If we assume $\mathit M_{{{\mathit Z}^{\,'}}}$ = $\mathit M_{{{\mathit W}^{\,'}}}$, the limit increases $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2400 GeV and $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2300 GeV for ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit g}_{{{V}}}}$ = 1, respectively. See their Fig.6 for limits on $\sigma \cdot{}\mathit B$. 49  SIRUNYAN 2017AK search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ or ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 and 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2300 GeV for ${{\mathit g}_{{{V}}}}$ = 1. If we assume $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$, the limit increases $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2400 GeV for both ${{\mathit g}_{{{V}}}}$ = 3 and ${{\mathit g}_{{{V}}}}$ = 1. See their Fig.1 and 2 for limits on ${{\mathit \sigma}}\cdot{}{{\mathit B}}$. 50  SIRUNYAN 2017H search for right-handed ${{\mathit W}^{\,'}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}^{\,'}}$ is assumed to decay into ${{\mathit \tau}}$ and a heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying to ${{\mathit \tau}}{{\mathit q}}{{\overline{\mathit q}}}$. The limit above assumes M$_{N}$ = M$_{{{\mathit W}^{\,'}}}$/2. 51  SIRUNYAN 2017I limit is for a right-handed ${{\mathit W}^{\,'}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit becomes ${{\mathit M}}_{{{\mathit W}^{\,'}}}$ $>$ 2400 GeV for ${{\mathit M}}_{{{\mathit \nu}_{{{R}}}}}{}\ll$ ${{\mathit M}}_{{{\mathit W}^{\,'}}}$. 52  SIRUNYAN 2017R search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. Mass regions $\mathit M_{{{\mathit W}^{\,'}}}$ $<$ 2370 GeV and 2870 $<$ $\mathit M_{{{\mathit W}^{\,'}}}$ $<$ 2970 GeV are excluded for ${{\mathit g}_{{{V}}}}$ = 1. If we assume $\mathit M_{{{\mathit Z}^{\,'}}}$ = $\mathit M_{{{\mathit W}^{\,'}}}$, the excluded mass regions are 1000 $<$ $\mathit M_{{{\mathit W}^{\,'}}}$ $<$ 2500 GeV and 2760 $<$ $\mathit M_{{{\mathit W}^{\,'}}}$ $<$ 3300 GeV for ${{\mathit g}_{{{V}}}}$ = 3; 1000 $<$ $\mathit M_{{{\mathit W}^{\,'}}}$ $<$ 2430 GeV and 2810 $<$ $\mathit M_{{{\mathit W}^{\,'}}}$ $<$ 3130 GeV for ${{\mathit g}_{{{V}}}}$ = 1. See their Fig.5 for limits on ${{\mathit \sigma}}\cdot{}{{\mathit B}}$. 53  AABOUD 2016AE search for resonances decaying to ${{\mathit V}}{{\mathit V}}$ (${{\mathit V}}$ = ${{\mathit W}}$ or ${{\mathit Z}}$) in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. Results from ${{\mathit \nu}}{{\mathit \nu}}{{\mathit q}}{{\mathit q}}$, ${{\mathit \nu}}{{\mathit \ell}}{{\mathit q}}{{\mathit q}}$, ${{\mathit \ell}}{{\mathit \ell}}{{\mathit q}}{{\mathit q}}$ and ${{\mathit q}}{{\mathit q}}{{\mathit q}}{{\mathit q}}$ final states are combined. The quoted limit is for a heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3 and $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$. 54  AABOUD 2016V limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The bosonic decays of ${{\mathit W}^{\,'}}$ and the interference with SM ${{\mathit W}}$ process are neglected. 55  AAD 2016R search for ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}^{\,'}}{{\mathit \ell}^{\,'}}$, ${{\mathit \ell}}{{\mathit \ell}}{{\mathit q}}{{\overline{\mathit q}}}$, ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}}$, and all hadronic channels are combined. The quoted limit assumes ${{\mathit g}}_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/{{\mathit g}}_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = (${{\mathit M}_{{{W}}}}/{{\mathit M}}_{{{\mathit W}^{\,'}}}){}^{2}$. 56  AAD 2016S search for a new resonance decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for a ${{\mathit W}^{\,'}}$ having SM-like couplings to quarks. 57  KHACHATRYAN 2016AO limit is for a SM-like right-handed using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The quoted limit combines ${{\mathit t}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\mathit b}}$ and ${{\mathit t}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit b}}$ events. 58  KHACHATRYAN 2016AP search for a resonance decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. Both ${{\mathit H}}$ and ${{\mathit W}}$ are assumed to decay to fat jets. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. 59  KHACHATRYAN 2016BD search for resonance decaying to ${{\mathit H}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The quoted limit is for heavy-vector-triplet (HVT) ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. The HVT model ${\mathit m}_{{{\mathit W}^{\,'}}}$ = ${\mathit m}_{{{\mathit Z}^{\,'}}}$ $>$ 1.8 TeV is also obtained by combining ${{\mathit W}^{\,'}}/{{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit H}}/{{\mathit Z}}$ ${{\mathit H}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit b}}{{\mathit b}}$, ${{\mathit q}}{{\mathit q}}{{\mathit \tau}}{{\mathit \tau}}$, ${{\mathit q}}{{\mathit q}}{{\mathit b}}{{\mathit b}}$, and ${{\mathit q}}{{\mathit q}}{{\mathit q}}{{\mathit q}}{{\mathit q}}{{\mathit q}}$ channels. 60  KHACHATRYAN 2016K search for resonances decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. 61  KHACHATRYAN 2016L search for resonances decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV with the data scouting technique, increasing the sensitivity to the low mass resonances. 62  KHACHATRYAN 2016O limit is for ${{\mathit W}^{\,'}}$ having universal couplings. Interferences with the SM amplitudes are assumed to be absent. 63  AAD 2015AU search for ${{\mathit W}^{\,'}}$ decaying into the ${{\mathit W}}{{\mathit Z}}$ final state with ${{\mathit W}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}^{\,'}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{W}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. 64  AAD 2015AV limit is for a SM like right-handed ${{\mathit W}^{\,'}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$ decay is assumed to be forbidden. 65  AAD 2015AZ search for ${{\mathit W}^{\,'}}$ decaying into the ${{\mathit W}}{{\mathit Z}}$ final state with ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{{{\mathit W}}}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. 66  AAD 2015CP search for ${{\mathit W}^{\,'}}$ decaying into the ${{\mathit W}}{{\mathit Z}}$ final state with ${{\mathit W}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{{{\mathit W}}}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. 67  AAD 2015R limit is for a SM like right-handed ${{\mathit W}^{\,'}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$ decay is assumed to be forbidden. 68  AAD 2015V search for new resonance decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. 69  KHACHATRYAN 2015C search for ${{\mathit W}^{\,'}}$ decaying via ${{\mathit W}}{{\mathit Z}}$ to fully leptonic final states using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=8 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = $\mathit M_{W}$ $\mathit M_{Z}/\mathit M{}^{2}_{{{\mathit W}^{\,'}}}$. 70  KHACHATRYAN 2015T limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling which interferes the SM ${{\mathit W}}$ boson constructively using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. For ${{\mathit W}^{\,'}}$ without interference, the limit becomes $>$ 3280 GeV. 71  KHACHATRYAN 2014O search for right-handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying into ${{\mathit \ell}}{{\mathit j}}$ ${{\mathit j}}$. The quoted limit is for ${{\mathit M}}_{{{\mathit \nu}_{{{eR}}}}}$ = ${{\mathit M}}_{{{\mathit \nu}}_{{{\mathit \mu}} {{\mathit R}}}}$ = ${{\mathit M}}_{{{\mathit W}_{{{R}}}}}$/2. See their Fig. 3 and Fig. 5 for excluded regions in the ${{\mathit M}}_{{{\mathit W}_{{{R}}}}}−{{\mathit M}}_{{{\mathit \nu}}}$ plane. 72  AAD 2024AE search for resonances decaying to ${{\mathit q}}{{\mathit q}}$, ${{\mathit t}}{{\mathit t}}$, ${{\mathit t}}{{\mathit b}}$, ${{\mathit V}}{{\mathit V}}$, ${{\mathit V}}{{\mathit H}}$, ${{\mathit \ell}}{{\mathit \ell}}$, ${{\mathit \ell}}{{\mathit \tau}}$, ${{\mathit \tau}}{{\mathit \nu}}$, ${{\mathit \tau}}{{\mathit \tau}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit is for heavy-vector-triplet ${{\mathit W}^{\,'}}$ with ${{\mathit g}_{{{V}}}}$ = 3. $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$ is assumed. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 5.8 TeV for ${{\mathit g}_{{{V}}}}$ = 1. 73  AAD 2024CM search for pair productions of dark pions ${{\mathit \pi}_{{{D}}}^{\pm}}{{\mathit \pi}_{{{D}}}^{0}}$ in ${{\mathit t}}{{\mathit t}}{{\mathit b}}{{\mathit b}}$ events of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit \pi}_{{{D}}}^{\pm}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}$ and ${{\mathit \pi}_{{{D}}}^{0}}$ $\rightarrow$ ${{\mathit t}}{{\mathit t}}$ decays are assumed. The production cross section is computed in a model with dark ${{\mathit \rho}_{{{D}}}^{\pm}}$ assuming dark isospin symmetry ${\mathit m}_{{{\mathit \rho}_{{{D}}}^{\pm}}}$ = ${\mathit m}_{{{\mathit \rho}_{{{D}}}^{0}}}$, ${\mathit m}_{{{\mathit \pi}_{{{D}}}^{\pm}}}$ = ${\mathit m}_{{{\mathit \pi}_{{{D}}}^{0}}}$. See their Fig. 12 for limits on the production cross sections. 74  HAYRAPETYAN 2024AV search for a spin-0 particle ${{\mathit X}}$ decaying to ${{\mathit W}}{{\mathit \gamma}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 8 for limits on $\sigma \cdot{}B$. 75  AAD 2023BF search for ${{\mathit W}^{\,'}}$ decaying to ${{\mathit W}}{{\mathit Z}^{\,'}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The mass difference between ${{\mathit W}^{\,'}}$ and ${{\mathit Z}^{\,'}}$ is assumed to be 250 GeV. See their Fig. 9(a) for limits on $\sigma \cdot{}B$ as a function of $\mathit M_{{{\mathit W}^{\,'}}}$. 76  AAD 2023CG search for right-handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying into ${{\mathit \ell}}{{\mathit j}}{{\mathit j}}$. See their Fig. 9 for limits in ${\mathit m}_{{{\mathit N}}}-{\mathit m}_{{{\mathit W}_{{{R}}}}}$ plane. 77  AAD 2023CK search for a new resonance decaying to ${{\mathit H}}{{\mathit X}}$ (${{\mathit H}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit X}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}^{\,'}}$) in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 12 for limits on $\sigma \cdot{}B$. 78  AAD 2023U search for a narrow charged vector boson decaying to ${{\mathit W}}{{\mathit \gamma}}$. See their Fig. 8(d) for the exclusion limit in ${\mathit m}_{{{\mathit W}^{\,'}}}−\sigma \cdot{}B$ plane. 79  TUMASYAN 2022 search for KK excited ${{\mathit W}}$ decaying in cascade to three ${{\mathit W}}$ via a scalar radion ${{\mathit R}}$. See their Fig. 4 for limits in $\mathit M_{{{\mathit W}^{\,'}}}−{{\mathit M}_{{{R}}}}$ plane. 80  TUMASYAN 2022AL search for resonances decaying to ${{\mathit t}}{{\mathit B}}$ or ${{\mathit b}}{{\mathit T}}$ with vector-like quarks ${{\mathit B}}$ (${{\mathit T}}$) subsequently decaying to ${{\mathit b}}{{\mathit H}}$ or ${{\mathit b}}{{\mathit Z}}$ (${{\mathit t}}{{\mathit H}}$ or ${{\mathit t}}{{\mathit Z}}$). See their Fig. 7 for limits on $\sigma \cdot{}B$. 81  TUMASYAN 2022B search for a narrow charged vector boson decaying to ${{\mathit W}}{{\mathit \gamma}}$. See their Fig. 5 for limits on $\sigma \cdot{}B$. 82  TUMASYAN 2022I search for KK excited ${{\mathit W}}$ decaying in cascade to three ${{\mathit W}}$ via a scalar radion ${{\mathit R}}$. See their Fig. 10 for limits in $\mathit M_{{{\mathit W}^{\,'}}}−{{\mathit M}_{{{R}}}}$ plane. 83  TUMASYAN 2022P search for right handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisiions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying to ${{\mathit \ell}}{{\mathit j}}{{\mathit j}}$. See their Fig. 7 for excluded regions in ${{\mathit M}}_{{{\mathit W}_{{{R}}}}}−{{\mathit M}_{{{N}}}}$ plane. 84  AAD 2020AD search for a narrow resonance decaying to a pair of large-radius-jets ${{\mathit J}_{{{1}}}}$ and ${{\mathit J}_{{{2}}}}$ employing a machine-learning procedure. See their Fig. 3 for limits on $\sigma \cdot{}B$ depending on assumptions about invariant masses for ${{\mathit J}_{{{1}}}}$, ${{\mathit J}_{{{2}}}}$, and ${{\mathit J}_{{{1}}}}{{\mathit J}_{{{2}}}}$. 85  AAD 2020W search for ${{\mathit W}^{\,'}}$ decaying to ${{\mathit W}}{{\mathit Z}^{\,'}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 5(b) for limits on $\sigma \cdot{}B$ as a function of ${\mathit m}_{{{\mathit Z}^{\,'}}}$. The ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}^{\,'}}$ branching fraction was chosen to be 0.5 and the mass difference between the ${{\mathit W}^{\,'}}$ and ${{\mathit Z}^{\,'}}$ was set to 250 GeV. 86  AABOUD 2019B search for right-handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying to ${{\mathit \ell}}{{\mathit j}}{{\mathit j}}$. See their Figs. 7 and 8 for excluded regions in $\mathit M_{{{\mathit W}_{{{R}}}}}$ $−$ ${{\mathit M}_{{{N}}}}$ plane. 87  AABOUD 2019BB search for right handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and a boosted hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying to ${{\mathit \ell}}$ and a large radius jet ${{\mathit j}}$ = ${{\mathit q}}{{\overline{\mathit q}}}$. See their Fig. 7 for excluded regions in ${{\mathit M}}_{{{\mathit W}_{{{R}}}}}−{{\mathit M}_{{{N}}}}$ plane. 88  SIRUNYAN 2019V search for a new resonance decaying to a top quark and a heavy vector-like bottom partner ${{\mathit B}}$ decaying to ${{\mathit H}}{{\mathit b}}$ (or a bottom quark and a heavy vector-like top partner ${{\mathit T}}$ decaying to ${{\mathit H}}{{\mathit t}}$) in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Fig. 8 for limits on ${{\mathit \sigma}}\cdot{}{{\mathit B}}$. 89  AABOUD 2018AA search for a narrow charged vector boson decaying to ${{\mathit W}}{{\mathit \gamma}}$. See their Fig. 9 for the exclusion limit in M$_{{{\mathit W}^{\,'}}}$ $−$ $\sigma $B plane. 90  AABOUD 2018AD search for resonances decaying to ${{\mathit H}}{{\mathit X}}$ (${{\mathit H}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit X}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}^{\,'}}$) in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. See their Figs. $3 - 5$ for limits on $\sigma \cdot{}$B. 91  AABOUD 2018CJ search for heavy-vector-triplet ${{\mathit W}^{\,'}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above is for model with ${{\mathit g}_{{{V}}}}$ = 3 assuming $\mathit M_{{{\mathit W}^{\,'}}}$ = $\mathit M_{{{\mathit Z}^{\,'}}}$. The limit becomes $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 5500 GeV for model with ${{\mathit g}_{{{V}}}}$ = 1. 92  SIRUNYAN 2018CV search for right-handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying to ${{\mathit \ell}}{{\mathit j}}{{\mathit j}}$. The quoted limit is for ${{\mathit M}_{{{N}}}}$ = ${{\mathit M}}_{{{\mathit W}_{{{R}}}}}$/2. See their Fig. 6 for excluded regions in the ${{\mathit M}}_{{{\mathit W}_{{{R}}}}}−{{\mathit M}_{{{N}}}}$ plane. 93  KHACHATRYAN 2017U search for resonances decaying to ${{\mathit H}}{{\mathit W}}$ (${{\mathit H}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$; ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$) in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit on the heavy-vector-triplet model is $\mathit M_{{{\mathit Z}^{\,'}}}$ = $\mathit M_{{{\mathit W}^{\,'}}}$ $>$ 2 TeV for ${{\mathit g}_{{{V}}}}$ = 3, in which constraints from the ${{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit H}}{{\mathit Z}}$ (${{\mathit H}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$; ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$, ${{\mathit \nu}}{{\overline{\mathit \nu}}}$) are combined. See their Fig.3 and Fig.4 for limits on $\sigma \cdot{}\mathit B$. 94  AAD 2015BB search for ${{\mathit W}^{\,'}}$ decaying into ${{\mathit W}}{{\mathit H}}$ with ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit H}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$. See their Fig. 4 for the exclusion limits in the heavy vector triplet benchmark model parameter space. 95  AALTONEN 2015C limit is for a SM-like right-handed ${{\mathit W}^{\,'}}$ assuming ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$ decays are forbidden, using ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.96 TeV. See their Fig. 3 for limit on $\mathit g_{{{\mathit W}^{\,'}}}/\mathit g_{{{\mathit W}}}$. 96  KHACHATRYAN 2015V search new resonance decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. 97  AAD 2014AT search for a narrow charged vector boson decaying to ${{\mathit W}}{{\mathit \gamma}}$. See their Fig. 3a for the exclusion limit in ${\mathit m}_{{{\mathit W}^{\,'}}}−\sigma \mathit B$ plane. 98  AAD 2014S search for ${{\mathit W}^{\,'}}$ decaying into the ${{\mathit W}}{{\mathit Z}}$ final state with ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=8 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{{{\mathit W}}}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. 99  KHACHATRYAN 2014 search for ${{\mathit W}^{\,'}}$ decaying into ${{\mathit W}}{{\mathit Z}}$ final state with ${{\mathit W}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=8 TeV. The quoted limit assumes ${{\mathit g}}_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/{{\mathit g}}_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = (${{\mathit M}_{{{W}}}}/{{\mathit M}}_{{{\mathit W}^{\,'}}}){}^{2}$. 100  KHACHATRYAN 2014A search for ${{\mathit W}^{\,'}}$ decaying into the ${{\mathit W}}{{\mathit Z}}$ final state with ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$, or ${{\mathit W}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}$. ${{\mathit p}}{{\mathit p}}$ collisions data at $\sqrt {s }$=8 TeV are used for the search. See their Fig. 13 for the exclusion limit on the number of events in the mass$−$width plane. 101  AAD 2013AO search for ${{\mathit W}^{\,'}}$ decaying into the ${{\mathit W}}{{\mathit Z}}$ final state with ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit Z}}$ $\rightarrow$ 2 ${{\mathit j}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=7 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{{{\mathit W}}}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. 102  CHATRCHYAN 2013AJ search for resonances decaying to ${{\mathit W}}{{\mathit Z}}$ pair, using the hadronic decay modes of ${{\mathit W}}$ and ${{\mathit Z}}$, in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=7 TeV. See their Fig. 7 for the limit on the cross section. 103  CHATRCHYAN 2013AQ limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling which interferes with the SM ${{\mathit W}}$ boson using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=7 TeV. 104  CHATRCHYAN 2013E limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling which intereferes with the SM ${{\mathit W}}$ boson using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=7 TeV. For ${{\mathit W}^{\,'}}$ with right-handed coupling, the bound becomes $>$1850 GeV ($>$1910 GeV) if ${{\mathit W}^{\,'}}$ decays to both leptons and quarks (only to quarks). If both left- and right-handed couplings are present, the limit becomes $>$1640 GeV. 105  CHATRCHYAN 2013U search for ${{\mathit W}^{\,'}}$ decaying to the ${{\mathit W}}{{\mathit Z}}$ final state, with ${{\mathit W}}$ decaying into jets, in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=7 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{{{\mathit W}}}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. 106  The AAD 2012AV quoted limit is for a SM-like right-handed ${{\mathit W}^{\,'}}$ using ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=7 TeV. ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$ decay is assumed to be forbidden. 107  AAD 2012BB use ${{\mathit p}}{{\mathit p}}$ collisions data at $\sqrt {s }$=7 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{{{\mathit W}}}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. 108  AAD 2012CK search for ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit t}}{{\mathit W}^{\,'}}$, ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\overline{\mathit t}}}{{\mathit q}}$ events in ${{\mathit p}}{{\mathit p}}$ collisions. See their Fig. 5 for the limit on $\sigma \cdot{}$B. 109  AAD 2012CR use ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$=7 TeV. 110  AAD 2012M search for right-handed ${{\mathit W}_{{{R}}}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying into ${{\mathit \ell}}{{\mathit j}}{{\mathit j}}$. See their Fig. 4 for the limit in the ${\mathit m}_{{{\mathit N}}}−{\mathit m}_{{{\mathit W}^{\,'}}}$ plane. 111  AALTONEN 2012N search for ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit t}}{{\mathit W}^{\,'}}$, ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\overline{\mathit t}}}{{\mathit d}}$ events in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions. See their Fig. 3 for the limit on $\sigma \cdot{}$B. 112  CHATRCHYAN 2012AR search for ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit t}}{{\mathit W}^{\,'}}$, ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\overline{\mathit t}}}{{\mathit d}}$ events in ${{\mathit p}}{{\mathit p}}$ collisions. See their Fig. 2 for the limit on $\sigma \cdot{}$B. 113  CHATRCHYAN 2012BG search for right-handed ${{\mathit W}_{{{R}}}}$ in collisions $\sqrt {s }$ = 7 TeV. ${{\mathit W}_{{{R}}}}$ is assumed to decay into ${{\mathit \ell}}$ and hypothetical heavy neutrino ${{\mathit N}}$, with ${{\mathit N}}$ decaying into ${{\mathit \ell}}{{\mathit j}}{{\mathit j}}$. See their Fig. 3 for the limit in the ${\mathit m}_{{{\mathit N}}}−{\mathit m}_{{{\mathit W}^{\,'}}}$ plane. 114  ABAZOV 2011H use data from ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.96 TeV. The quoted limit is obtained assuming ${{\mathit W}^{\,'}}{{\mathit W}}{{\mathit Z}}$ coupling strength is the same as the ordinary ${{\mathit W}}{{\mathit W}}{{\mathit Z}}$ coupling strength in the Standard Model. 115  ABAZOV 2011L limit is for ${{\mathit W}^{\,'}}$ with SM-like coupling which interferes with the SM ${{\mathit W}}$ boson, using ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.96 TeV. For ${{\mathit W}^{\,'}}$ with right-handed coupling, the bound becomes $>$885 GeV ($>$890 GeV) if ${{\mathit W}^{\,'}}$ decays to both leptons and quarks (only to quarks). If both left- and right-handed couplings present, the limit becomes $>$916 GeV. 116  AALTONEN 2010N use ${{\mathit p}}{{\overline{\mathit p}}}$ collision data at $\sqrt {s }$=1.96 TeV. The quoted limit assumes $\mathit g_{{{\mathit W}^{\,'}} {{\mathit W}} {{\mathit Z}}}/\mathit g_{{{\mathit W}} {{\mathit W}} {{\mathit Z}}}$ = ($\mathit M_{{{\mathit W}}}/\mathit M_{{{\mathit W}^{\,'}}}){}^{2}$. See their Fig.$~$4 for limits in mass-coupling plane. 117  AALTONEN 2009AC search for new particle decaying to dijets using ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.96 TeV. 118  The ACOSTA 2003B quoted limit is for $\mathit M_{{{\mathit W}^{\,'}}}{}\gg\mathit M_{{{\mathit \nu}_{{{R}}}}}$, using ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.8 TeV. For $\mathit M_{{{\mathit W}^{\,'}}}<\mathit M_{{{\mathit \nu}_{{{R}}}}}$, $\mathit M_{{{\mathit W}^{\,'}}}$ between 225 and 566 GeV is excluded. 119  The quoted limit is obtained assuming ${{\mathit W}^{\,'}}{{\mathit W}}{{\mathit Z}}$ coupling strength is the same as the ordinary ${{\mathit W}}{{\mathit W}}{{\mathit Z}}$ coupling strength in the Standard Model, using ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.8 TeV. See their Fig.$~$2 for the limits on the production cross sections as a function of the ${{\mathit W}^{\,'}}$ width. 120  AFFOLDER 2001I combine a new bound on ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}$ of 754 GeV, using ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.8 TeV, with the bound of ABE 2000 on ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit \mu}}{{\mathit \nu}}$ to obtain quoted bound. 121  ABE 1997G search for new particle decaying to dijets using ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.8 TeV. 122  For bounds on ${{\mathit W}_{{{R}}}}$ with nonzero right-handed mass, see Fig.$~$5 from ABACHI 1996C. 123  ABACHI 1995E assume that the decay ${{\mathit W}^{\,'}}$ $\rightarrow$ ${{\mathit W}}{{\mathit Z}}$ is suppressed and that the neutrino from ${{\mathit W}^{\,'}}$ decay is stable and has a mass significantly less ${\mathit m}_{{{\mathit W}^{\,'}}}$. 124  RIZZO 1993 analyses CDF limit on possible two-jet resonances. The limit is sensitive to the inclusion of the assumed ${{\mathit K}}$ factor.

References