These limits are from ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\overline{\mathit q}}}$, ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit q}^{*}}$ X, or ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}$ X and depend on transition magnetic couplings between ${{\mathit q}}$ and ${{\mathit q}^{*}}$. Assumptions about ${{\mathit q}^{*}}$ decay mode are given in the footnotes and comments.

VALUE (GeV) CL% DOCUMENT ID TECN  COMMENT $\bf{ > 6700}$ OUR LIMIT $\text{none 1800 - 2500}$ 95 1 TUMASYAN 2023 AF CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit b}}{{\mathit g}}$ $\text{none 1000 - 6000}$ 95 2 TUMASYAN 2023 BC CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \gamma}}$ $\text{none 1000 - 2200}$ 95 3 TUMASYAN 2023 BC CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit b}}{{\mathit \gamma}}$ $\bf{\text{none 2000 - 6700}}$ 95 4 AAD 2020 T ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $\text{none 1250 - 3200}$ 95 4 AAD 2020 T ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit b}}{{\mathit g}}$ , ${{\mathit b}}{{\mathit \gamma}}$ , ${{\mathit b}}{{\mathit Z}}$ , ${{\mathit t}}{{\mathit W}}$ $\text{none 1800 - 6300}$ 95 5 SIRUNYAN 2020 AI CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $\text{none 1500 - 2600}$ 95 6 AABOUD 2018 AB ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit b}}{{\mathit g}}$ $\text{none 1500 - 5300}$ 95 7 AABOUD 2018 BA ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \gamma}}$ $\text{none 1000 - 5500}$ 95 8 SIRUNYAN 2018 AG CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \gamma}}$ $\text{none 1000 - 1800}$ 95 9 SIRUNYAN 2018 AG CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit b}}{{\mathit \gamma}}$ $\text{none 600 - 6000}$ 95 10 SIRUNYAN 2018 BO CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}$ ${{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $\text{none 1200 - 5000}$ 95 11 SIRUNYAN 2018 P CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit W}}$ $\text{none 1200 - 4700}$ 95 11 SIRUNYAN 2018 P CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit Z}}$ $> 6000$ 95 12 AABOUD 2017 AK ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ • • We do not use the following data for averages, fits, limits, etc. • • $\text{none 700 - 3000}$ 95 13 TUMASYAN 2022 O CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit t}}{{\mathit W}}$ $> 2600$ 95 14 SIRUNYAN 2021 AG CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit t}}{{\mathit W}}$ $\text{none 600 - 5400}$ 95 15 KHACHATRYAN 2017 W CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $\text{none 1100 - 2100}$ 95 16 AABOUD 2016 ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit b}}{{\mathit g}}$ $> 1500$ 95 17 AAD 2016 AH ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit t}}{{\mathit W}}$ $> 4400$ 95 18 AAD 2016 AI ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \gamma}}$ 19 AAD 2016 AV ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$, ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit W}}{{\mathit b}}$ $> 5200$ 95 20 AAD 2016 S ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $> 1390$ 95 21 KHACHATRYAN 2016 I CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit b}^{*}}{{\mathit X}}$ , ${{\mathit b}^{*}}$ $\rightarrow$ ${{\mathit t}}{{\mathit W}}$ $> 5000$ 95 22 KHACHATRYAN 2016 K CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $\text{none 500 - 1600}$ 95 23 KHACHATRYAN 2016 L CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $> 4060$ 95 24 AAD 2015 V ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $> 3500$ 95 25 KHACHATRYAN 2015 V CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit g}}$ $> 3500$ 95 26 AAD 2014 A ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \gamma}}$ $> 3200$ 95 27 KHACHATRYAN 2014 CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit W}}$ $> 2900$ 95 28 KHACHATRYAN 2014 CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit Z}}$ $\text{none 700 - 3500}$ 95 29 KHACHATRYAN 2014 J CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \gamma}}$ $> 2380$ 95 30 CHATRCHYAN 2013 AJ CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit W}}$ $> 2150$ 95 31 CHATRCHYAN 2013 AJ CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit q}^{*}}{{\mathit X}}$ , ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit q}}{{\mathit Z}}$ 1  TUMASYAN 2023AF limit quoted above assumes ${{\mathit b}}$ ${{\mathit g}}$ $\rightarrow$ ${{\mathit b}^{*}}$ production. The limit becomes ${\mathit m}_{{{\mathit b}^{*}}}$ $>$ 4$~$TeV if contact interaction is included in the ${{\mathit b}^{*}}$ production cross section. See their Fig. 5 for limits on $\sigma \cdot{}B$. 2  TUMASYAN 2023BC search for excited light flavor quark ${{\mathit q}^{*}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. $\mathit f$ = 1.0 is assumed. 3  TUMASYAN 2023BC search for excited ${{\mathit b}}$ quark ${{\mathit b}^{*}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. $b^*$ production via gauge interactions and $\mathit f$ = 1.0 are assumed. The limit becomes $m_{b^*}>3.8$TeV if contact interaction is included in the $b^*$ production cross section. 4  AAD 2020T search for resonances decaying into dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. Assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. 5  SIRUNYAN 2020AI search for resonances decaying into dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. Assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. 6  AABOUD 2018AB assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit b}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit b}^{*}}$ production and decay amplitudes. 7  AABOUD 2018BA search for first-generation excited quarks (${{\mathit u}^{*}}$ and ${{\mathit d}^{*}}$) with degenerate mass, assuming ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. 8  SIRUNYAN 2018AG search for first-generation excited quarks (${{\mathit u}^{*}}$ and ${{\mathit d}^{*}}$) with degenerate mass, assuming ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. 9  SIRUNYAN 2018AG search for excited ${{\mathit b}}$ quark assuming ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. 10  SIRUNYAN 2018BO assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. 11  SIRUNYAN 2018P use the hadronic decay of ${{\mathit W}}$ or ${{\mathit Z}}$, assuming ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$= ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$= 1. 12  AABOUD 2017AK assume $\Lambda $ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. Only the decay of ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit g}}{{\mathit u}}$ and ${{\mathit q}^{*}}$ $\rightarrow$ ${{\mathit g}}{{\mathit d}}$ is simulated as the benchmark signals in the analysis. 13  TUMASYAN 2022O search for ${{\mathit b}^{*}}$ decaying to ${{\mathit t}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above assumes ${{\mathit \kappa}_{{{L}}}^{b}}$ = ${{\mathit g}_{{{L}}}}$ = 1, ${{\mathit \kappa}_{{{R}}}^{b}}$ = ${{\mathit g}_{{{R}}}}$ = 0. The limit becomes ${\mathit m}_{{{\mathit b}^{*}}}$ $>$ 3.0 TeV ($>$3.2 TeV) if we assume ${{\mathit \kappa}_{{{L}}}^{b}}$ = ${{\mathit g}_{{{L}}}}$ = 0, ${{\mathit \kappa}_{{{R}}}^{b}}$ = ${{\mathit g}_{{{R}}}}$ = 1 (${{\mathit \kappa}_{{{L}}}^{b}}$ = ${{\mathit g}_{{{L}}}}$ = 1, ${{\mathit \kappa}_{{{R}}}^{b}}$ = ${{\mathit g}_{{{R}}}}$ = 1). See their Fig. 3 for limits on $\sigma \cdot{}B$. 14  SIRUNYAN 2021AG search for ${{\mathit b}^{*}}$ decaying to ${{\mathit t}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The limit quoted above assumes ${{\mathit \kappa}_{{{L}}}^{b}}$ = ${{\mathit g}_{{{L}}}}$ = 1, ${{\mathit \kappa}_{{{R}}}^{b}}$ = ${{\mathit g}_{{{R}}}}$ = 0. The limit becomes ${\mathit m}_{{{\mathit b}^{*}}}$ $>$ 2.8 TeV ($>$ 3.1 TeV) if we assume ${{\mathit \kappa}_{{{L}}}^{b}}$ = ${{\mathit g}_{{{L}}}}$ = 0, ${{\mathit \kappa}_{{{R}}}^{b}}$ = ${{\mathit g}_{{{R}}}}$ = 1 (${{\mathit \kappa}_{{{L}}}^{b}}$ = ${{\mathit g}_{{{L}}}}$ = ${{\mathit \kappa}_{{{R}}}^{b}}$ = ${{\mathit g}_{{{R}}}}$ = 1). See their Fig. 5 for limits on $\sigma \cdot{}B$. 15  KHACHATRYAN 2017W assume $\Lambda $ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. 16  AABOUD 2016 assume $\Lambda $ = ${\mathit m}_{{{\mathit b}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in the ${{\mathit b}^{*}}$ production and decay amplitudes. 17  AAD 2016AH search for ${{\mathit b}^{*}}$ decaying to ${{\mathit t}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. ${{\mathit f}_{{{g}}}}$ = ${{\mathit f}_{{{L}}}}$ = ${{\mathit f}_{{{R}}}}$ = 1 are assumed. See their Fig. 12b for limits on $\sigma \cdot{}\mathit B$. 18  AAD 2016AI assume $\Lambda $ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. 19  AAD 2016AV search for single production of vector-like quarks decaying to ${{\mathit W}}{{\mathit b}}$ in ${{\mathit p}}{{\mathit p}}$ collisions. See their Fig. 8 for the limits on couplings and mixings. 20  AAD 2016S assume $\Lambda $ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. 21  KHACHATRYAN 2016I search for ${{\mathit b}^{*}}$ decaying to ${{\mathit t}}{{\mathit W}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. ${{\mathit \kappa}_{{{L}}}^{b}}$ = ${{\mathit g}_{{{L}}}}$ = 1, ${{\mathit \kappa}_{{{R}}}^{b}}$ = ${{\mathit g}_{{{R}}}}$ = 0 are assumed. See their Fig. 8 for limits on $\sigma \cdot{}\mathit B$. 22  KHACHATRYAN 2016K assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$= 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. 23  KHACHATRYAN 2016L search for resonances decaying to dijets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV using the data scouting technique which increases the sensitivity to the low mass resonances. 24  AAD 2015V assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. 25  KHACHATRYAN 2015V assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. The contact interactions are not included in ${{\mathit q}^{*}}$ production and decay amplitudes. 26  AAD 2014A assume ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = 1. 27  KHACHATRYAN 2014 use the hadronic decay of ${{\mathit W}}$, assuming ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}={{\mathit f}}={{\mathit f}^{\,'}}$ = 1. 28  KHACHATRYAN 2014 use the hadronic decay of ${{\mathit Z}}$, assuming ${{\mathit \Lambda}}$ = ${\mathit m}_{{{\mathit q}^{*}}}$, ${{\mathit f}_{{{s}}}}={{\mathit f}}={{\mathit f}^{\,'}}$ = 1. 29  KHACHATRYAN 2014J assume ${{\mathit f}_{{{s}}}}$ = ${{\mathit f}}$ = ${{\mathit f}^{\,'}}$ = ${{\mathit \Lambda}}$ $/$ ${\mathit m}_{{{\mathit q}^{*}}}$. 30  CHATRCHYAN 2013AJ use the hadronic decay of ${{\mathit W}}$. 31  CHATRCHYAN 2013AJ use the hadronic decay of ${{\mathit Z}}$.

References