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Table B.1

Abundances of ammonia in comets from ground-based observations.

UT date (yyyy/mm/dd.d) rh (au) (%) Comet Typea Name Reference
Radio data (λ ~cm)b

1996 03 24 1.07 0.44 ± 0.17 LPC C/1996 B2 (Hyakutake) Wootten et al. (1996a,b); Palmer et al. (1996), (A. Wootten & B. Butler, pers. comm.)c
1997 03 30 0.92 0.66 ± 0.13 LPC C/1995 O1 (Hale-Bopp) Bird et al. (1997)d
1997 04 20 0.98 1.8 ± 0.9 LPC C/1995 O1 (Hale-Bopp) Hirota et al. (1999)
1997 05 22 1.27 0.14 ± 0.05 LPC C/1995 O1 (Hale-Bopp) Butler et al. (2002),

(A. Wootten & B. Butler, pers. comm.)e

2020 07 24.8 0.67 < 0.29 LPC C/2020 F3 (NEOWISE) This paper

Radio data (λ = 0.52 mm)

2004 04 29.8 1.00 0.50 ± 0.09 DNC C/2001 Q4 (NEAT) Biver et al. (2007)
2004 05 25.9 0.93 0.33 ± 0.08 DNC C/2002 T7 (LINEAR) Biver et al. (2007)
2010 07 19.1 1.43 0.46 ± 0.04 JFC 10P/Tempel2 Biver et al. (2012)
2010 10 30.6 1.06 0.45 ± 0.04 JFC 103P/Hartley2 Unpublished results from Herschel (N. Biver, pers. comm.)
2011 08 14.0 1.03 0.80 ± 0.03 JFC 45P/Honda-Mrkos-Pajdušáková idem
2011 10 08.9 1.86 0.20 ± 0.03 DNC C/2009 P1 (Garradd) idem

Infrared data

2007 12 23 1.16 0.72 ± 0.38 HTC 8P/Tuttle Lippi et al. (2021)
2007 10 29 2.45 0.82 ± 0.52 JFC 17P/Holmes idem
2005 07 04 1.51 1.14 ± 0.72 JFC 9P/Tempel 1 idem
2010 07 26 1.44 1.12 ± 0.24 JFC 10P/Tempel2 idem
2010 10 30 1.07 0.64 ± 0.06 JFC 103P/Hartley2 idem
1999 08 19 1.07 0.56 ± 0.15 LPC C/1999 H1 (Lee) idem
2005 01 19 1.21 0.24 ± 0.01 LPC C/2004 Q2 (Machholz) idem
2009 02 01 1.26 0.27 ± 0.16 DNC C/2007 N3 (Lulin) idem
2008 07 09 0.89 0.76 ± 0.14 DNC C/2007 W1 (Boattini) idem
2012 01 09 1.57 1.03 ± 0.81 DNC C/2009 P1 (Garradd) idem
2013 06 20 1.74 0.58 ± 0.23 LPC C/2012 F6 (Lemmon) idem
2013 10 25 1.32 1.48 ± 0.28 LPC C/2013 R1 (Lovejoy) idem
2008 08 11 1.35 0.52 ± 0.15 JFC 6P/d’Arrest Dello Russo et al. (2016)
2005 07 04 1.51 0.9 ± 0.3 JFC 9P/Tempel 1 idem
2010 07 26 1.44 0.83 ± 0.2 JFC 10P/Tempel2 idem
2010 02 23 1.60 0.6 ± 0.3 JFC 81P/Wild 2 idem
2010 10 30 1.07 0.66 ± 0.06 JFC 103P/Hartley2 idem
1999 08 21 1.08 0.70 ± 0.22 LPC C/1999 H1 (Lee) idem
2005 01 25 1.21 0.31 ± 0.03 LPC C/2004 Q2 (Machholz) idem
2007 01 28 0.55 1.5 ± 0.3 DNC C/2006 P1 (McNaught) idem
2009 02 15 1.35 0.24 ± 0.05 DNC C/2007 N3 (Lulin) idem
2008 07 10 0.90 1.74 ± 0.17 DNC C/2007 W1 (Boattini) idem
2011 10 13 1.83 0.48 ± 0.13 DNC C/2009 P1 (Garradd) idem
2013 06 20 1.74 0.61 ± 0.21 LPC C/2012 F6 (Lemmon) idem
2013 11 07.6 0.84 < 0.93 DNC C/2012 S1 (ISON) DiSanti et al. (2016)
2013 11 19.8 0.46 3.58 ± 0.33 DNC C/2012 S1 (ISON) idem
2013 11 23.0 0.34 3.22 ± 0.70 DNC C/2012 S1 (ISON) idem
2013 11 07 1.16 0.10 ± 0.02 LPC C/2013 R1 (Lovejoy) Dello Russo et al. (2016)
2014 02 03 1.29 0.64 ± 0.06 LPC C/2014 Q2 (Lovejoy) Dello Russo et al. (2022)
2017 01 08 0.56 0.64 ± 0.24 JFC 45P/Honda-Mrkos-Pajdušáková DiSanti et al. (2017)
2017 02 16 1.05 0.83 ± 0.67 JFC 45P/Honda-Mrkos-Pajdušáková Dello Russo et al. (2020)
2017 03 25 0.53 0.61 ± 0.04 ETC 2P/Encke Roth et al. (2018)
2014 09 05 0.78 0.75 ± 0.10 DNC C/2013 V5 (Oukaimeden) DiSanti et al. (2018)
2017 04 04 0.66 1.86 ± 0.36 LPC C/2017 E4 (Lovejoy) Faggi et al. (2018)
2018 12 17 1.06 0.66 ± 0.20 JFC 46P/Wirtanen Bonev et al. (2021)
2018 12 21 1.06 0.50 ± 0.06 JFC 46P/Wirtanen Khan et al. (2021)
2020 07 31.1 0.81 0.73 ± 0.10 LPC C/2020 F3 (NEOWISE) Faggi et al. (2021)
2020 08 06.3 0.94 0.92 ± 0.19 LPC C/2020 F3 (NEOWISE) idem

Notes.(a) ETC = Encke-Type Comet, JFC = Jupiter-Family Comet, LPC = Long-Period Comets originating from the Oort Cloud, DNC = Dynamically New Oort Cloud Comet, HTC = Halley-Type Comet. (b) For other tentative detections and non-detections in further comets, see also Altenhoff et al. (1983); Bird et al. (1987); Churchwell et al. (1976); Bird et al. (2002); Hatchell et al. (2005). (c) mol s−1 from the tabulated references and mol s−1 from Mumma et al. (1996). (d) mol s−1 from Bird et al. (1997) and mol s−1, which is the best-possible estimate for the dates of NH3 observations based on SOHO/SWAN measurements of Combi (2002), NRT data analysis of Colom et al. (1999), and near-ultraviolet OH observations of Harris et al. (2002). (e) mol s−1 from the tabulated references and mol s−1 Combi et al. (2000).

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