Table A.1: Observing Log for the NEP spectra. Scan numbers are from Gioia et al. (2003).

Scan	Date	RA	Dec	Spectral type	ti (s)	S/N
		(h m s)
*20	2004 Jun. 28	17 52 44.8	+67 00 20	G8	5400	70
260	2004 Jun. 01	17 58 28.3	+67 26 08	G2	2400	50
330	2004 Jun. 02	17 59 23.6	+66 02 55	G9	1800	70
370	2004 May 25	18 00 02.2	+66 45 53	F8	2400	90
*1420	2004 Mar. 08	17 19 28.8	+65 22 29	K0	3600	60
*1441	2004 Jan. 31	17 20 05.6	+62 06 22	G2	1200	100
1470	2004 Mar. 09	17 20 26.7	+67 03 37	G8	1800	80
1500	2004 Apr. 07	17 21 10.9	+69 48 02	G2	600	200
1511	2004 Feb. 03	17 21 42.5	+62 00 32	K4	3600	60
1580	2004 Apr. 07	17 24 00.4	+69 40 30	K2	3600	50
*1600	2004 Mar. 08	17 24 26.8	+64 12 23	G2	1800	50
1601	2004 Mar. 09	17 24 38.8	+64 40 51	G0	1800	80
1690	2004 Mar. 09	17 26 45.4	+69 37 53	G2	2400	60
1800	2004 May 06	17 29 39.4	+68 47 38	F5	1200	110
1840	2004 May 25	17 30 19.9	+69 55 27	G0	1800	90
1960	2004 Apr. 07	17 33 16.9	+67 12 08	F2	600	170
2050	2004 Mar. 09	17 36 14.1	+65 02 27	K0	2400	70
2100	2004 May 06	17 36 26.6	+68 20 37	M3	600	170
2210	2004 Jun. 02	17 39 16.1	+70 20 09	F8	1200	80
2250	2004 Mar. 08	17 39 56.1	+65 00 04	K0	2400	200
2360	2004 Jun. 01	17 42 26.5	+69 07 58	F8	1200	120
2400	2004 Mar. 09	17 43 01.6	+66 06 46	G2	1800	90
2470	2004 Jun. 02	17 43 51.7	+70 31 39	F3	1800	40
2480	2004 Jun. 01	17 44 00.6	+70 15 27	K0	2400	50
*2970	2004 Jan. 31	17 49 03.9	+62 47 48	F2	600	290
*3080	2004 Jun. 28	17 50 25.3	+70 45 36	K2.5	1800	90
3220	2004 Jun. 01	17 52 56.0	+66 25 10	K0	600	150
3560	2004 Jun. 28	17 57 03.7	+68 49 14	G8	1800	110
3610	2004 May 06	17 58 01.4	+64 09 34	K4	2700	70
3690	2004 May 06	17 58 48.0	+63 50 39	A2	1200	120
3710	2004 Jun. 30	17 59 13.8	+64 08 33	F2	1200	200
*4090	2004 Jun. 28	18 05 30.5	+69 45 17	G2	2400	50
4100	2004 May 25	18 05 30.3	+62 19 03	K0	1200	150
4130	2004 Jun. 02	18 05 44.8	+65 51 58	F5	1200	80
4180	2004 May 25	18 06 41.0	+64 13 18	K0	600	440
4380	2004 Jun. 01	18 08 45.4	+62 56 37	G5	1200	120
4470	2004 Jun. 29	18 09 55.8	+69 40 39	K3	1200	160
4530	2004 Jun. 29	18 10 49.9	+70 16 09	G9	4800	80
4780	2004 Jun. 29	18 13 48.6	+68 31 32	K2	2400	80
4810	2004 Jun. 03	18 13 51.4	+64 23 57	F5	180	300
*4931	2004 Jun. 28	18 16 21.2	+65 29 39	K8	1200	170
4970	2004 Jun. 03	18 16 49.7	+65 04 26	K2	2400	60
5060	2004 Jun. 29	18 18 31.9	+70 42 17	G5	1800	90
5220	2004 Jun. 03	18 20 19.2	+65 19 19	F8	600	120
*5320	2004 Jun. 28	18 21 46.8	+63 57 10	K0	1800	90
5510	2004 Jun. 03	18 25 09.0	+64 50 21	K0	600	260
5520	2004 Jun. 03	18 25 32.9	+62 34 15	K4	2400	60
5950	2004 Jun. 30	18 32 29.5	+68 36 52	G0	600	190
6030	2004 Jun. 29	18 33 47.8	+65 13 33	K3	1200	150
6051	2004 Jun. 29	18 34 33.6	+69 31 45	K5	3600	50
6160	2004 Jun. 30	18 36 13.5	+65 29 15	F0	300	230
6163	2004 Jun. 29	18 36 22.8	+66 54 54	G3	600	180
6350	2004 Jun. 29	18 39 25.4	+69 02 54	M3	2400	60
6400	2004 Jun. 29	18 40 44.4	+70 38 47	K2	1200	70
6410	2004 Jun. 30	18 40 56.6	+62 44 54	K0	300	300
6510	2004 Jun. 29	18 43 12.6	+69 55 54	F0	1200	80

* We lack the thorium-argon lamp exposures for the nights in which these stars were acquired. They were wavelength calibrated using lamp exposures of the nearest night.