ABCDEFGHIJKLMNOPQRSTUVWXYZAAABACADAE
1
PriorityTICalt_IDTmagSTRADECSec_yr_1Sec_yr_2Sec_yr_3Obs_strategyDAO/other notesphot_notesspec_notesBK-numABE-numAP_comKELT_E_IDKELT_W_ID
2
45904500HD_2532149.03B1.5:V:nn93.06915720.086053BK-018ABE-187cbeKELT_N04_lc_000848_V01_east_raw.KELT_N04_lc_033762_V01_west_raw.
3
44938364HD_2517268.562B1V:e91.72653819.034461BK-037ABE-A34cbeKELT_N04_lc_014453_V01_east_raw.KELT_N04_lc_040876_V01_west_raw.
4
450276053V338_Car8.22B9e168.468-58.6084610-11BK-806KELT_S38_lc_007089_V01_east_raw.KELT_S38_lc_007012_V01_west_raw.
5
45116246IGR_J06074+220511.349B0.5Ve91.86088622.096608ABE-A32hmxbKELT_N04_lc_008315_V01_east_raw.KELT_N04_lc_106882_V01_west_raw.
6
45173995TYC_1326-1188-110.412A292.0508321.949611ABE-171cbeKELT_N04_lc_019402_V01_east_raw.KELT_N04_lc_030584_V01_west_raw.
7
45904358HD_25321510.505none93.05778320.000967BK-033ABE-188cbeKELT_N04_lc_009945_V01_east_raw.KELT_N04_lc_032652_V01_west_raw.
8
20413239V731_Tau6.01B2.5Ve85.8312523.20439BK-066NULLKELT_N04_lc_119172_V01_west_raw.
9
247589847BD+13_97610.281A086.40504813.1891856ABE-083cbeKELT_S05_lc_022708_V01_east_raw.KELT_S05_lc_023836_V01_west_raw.
10
19935717TYC_1310-2084-110.338B884.92704322.257774ABE-154cbeKELT_N04_lc_006428_V01_east_raw.KELT_N04_lc_055803_V01_west_raw.
11
429944492V963_Ori7.72B2IIpe94.8203620.57995BK-042KELT_N04_lc_015364_V01_east_raw.KELT_N04_lc_012743_V01_west_raw.
12
46022938IV_Vir9.228symB[e]214.142916-21.76390711ABE-P25bpeKELT_S25_lc_009125_V01_east_raw.KELT_S25_lc_008015_V01_west_raw.
13
19621526HD_2453108.67B2IIInnpe84.0959121.18653BK-014KELT_N04_lc_000384_V01_east_raw.KELT_N04_lc_015670_V01_west_raw.
14
18442894HD_301238.11B8e71.3944919.32833BK-002KELT_N03_lc_009488_V01_east_raw.KELT_N03_lc_058807_V01_west_raw.
15
64333488AS_1508.706symB[e]111.344866-3.597447ABE-P24bpeKELT_J06_lc_008264_V01_east_raw.KELT_J06_lc_007923_V01_west_raw.
16
79823872HD_1512429.58B5IIIe252.00703-40.3536BK-877KELT_S36_lc_008942_V01_east_raw.KELT_S36_lc_006129_V01_west_raw.
17
12725034del_Sco2.384B0.2IVe240.083375-22.62170556
18
191168285_Cnc6.02046B9.5Vne120.376208316.45531111
19
719704573zet_Tau4.6218B2IVe84.4112083321.14254444Will be observed in TESS cycle 4, s43, 44, 45, 2021-Sep-16 -- 2021-Sep-16Observations between Sept. 11 2020 - March 11 2021 will be valuable, since the BRITE space photometer is observing this star during that time.Being observed by BRITE satellite September 11th, 2020 - March 11th, 2021
20
27141005105_Tau5.58788B2Ve76.98121.704825
21
19701113V1162_Tau8.83B5ne84.4091723.14748BK-028KELT_N04_lc_006743_V01_east_raw.KELT_N04_lc_082111_V01_west_raw.
22
429900163EM*_MWC_8009.68Be94.7206521.31726BK-013KELT_N04_lc_000144_V01_east_raw.KELT_N04_lc_034866_V01_west_raw.
23
429863539HD_437038.072B1IV:p?94.66435623.007929BK-020ABE-A07cbeKELT_N04_lc_001510_V01_east_raw.KELT_N04_lc_040913_V01_west_raw.
24
429602037BD+22_11478.038B990.67104222.046737ABE-169cbeKELT_N04_lc_021668_V01_east_raw.KELT_N04_lc_080037_V01_west_raw.
25
237544639V742_Mon6.77B2IIIe102.940655.08437BK-415KELT_S05_lc_000496_V01_east_raw.KELT_S05_lc_000410_V01_west_raw.
26
25256180V728_Mon7.41B1.5IVe98.18017-7.508996BK-429KELT_S05_lc_001167_V01_east_raw.KELT_S05_lc_001120_V01_west_raw.
27
269845286HD_2501638.87B1.5Vnpe90.0483719.19264BK-017KELT_N04_lc_000757_V01_east_raw.KELT_N04_lc_056383_V01_west_raw.
28
27043894BD+22_8256.866B8.5V76.67057522.510803ABE-054cbeKELT_N04_lc_031803_V01_east_raw.KELT_N04_lc_135414_V01_west_raw.
29
29277573HD_381918.527B1:V:ne:86.23432421.460669BK-029ABE-A05cbeKELT_N04_lc_006758_V01_east_raw.KELT_N04_lc_075611_V01_west_raw.
30
294553294CQ_Cir8.83B1Ve222.70942-60.286211BK-884KELT_S37_lc_007838_V01_east_raw.KELT_S37_lc_008098_V01_west_raw.
31
316279926WRAY_15-111910.6Be203.44179-63.5346611BK-941KELT_S37_lc_107707_V01_east_raw.KELT_S37_lc_123482_V01_west_raw.
32
317666530HD_1180947.91B8Vne204.08741-63.1456611BK-672KELT_S38_lc_004775_V01_east_raw.NULL
33
319854805HD_473598.6B0IVe99.603764.880966BK-435KELT_S05_lc_003811_V01_east_raw.KELT_S05_lc_003411_V01_west_raw.
34
337498268HD_2415709.75B5ne78.224821.96727BK-039KELT_N04_lc_014988_V01_east_raw.KELT_N04_lc_040975_V01_west_raw.
35
220238856BD+09_13159.919O/B299.631529.4200676ABE-274cbeNULLKELT_S05_lc_013974_V01_west_raw.
36
341262262AS_2148.674B3254.075061-40.680225ABE-419cbeKELT_S36_lc_006245_V01_east_raw.NULL
37
389576843HD_16999910.55B8Vne277.52718-52.2045413BK-167KELT_S36_lc_036402_V01_east_raw.KELT_S36_lc_032075_V01_west_raw.
38
401635731V1012_Cen8.8B3Vne220.02282-59.9313411-12BK-775KELT_S37_lc_005000_V01_east_raw.KELT_S37_lc_005645_V01_west_raw.
39
408757239V716_Cen6.09B5Ve213.41585-54.6256611BK-610KELT_S37_lc_000167_V01_east_raw.KELT_S37_lc_000204_V01_west_raw.
40
413350702HD_1250157.22B7Vne214.71238-58.68644BK-639KELT_S37_lc_000649_V01_east_raw.KELT_S37_lc_000725_V01_west_raw.
41
429433216HD_2502897.66B2IIIe90.2744523.33899BK-060KELT_N04_lc_056897_V01_east_raw.KELT_N04_lc_140482_V01_west_raw.
42
429501634HR_21166.368B8V90.42340322.401022ABE-170cbenoneKELT_N04_lc_037205_V01_east_raw.
43
211750828HD_1532228.58B1IIe255.11954-49.2541512BK-750KELT_S36_lc_003721_V01_east_raw.KELT_S36_lc_003749_V01_west_raw.
44
173381049HD_591978.02B6Ve111.74772-41.629097-8BK-194KELT_S34_lc_002333_V01_east_raw.KELT_S34_lc_002186_V01_west_raw.
45
46943830nu_Gem4.1499B6IIIe97.2407916720.21213611
46
238513140HD_25085410.95B5e90.8957522.3274BK-051KELT_N04_lc_034843_V01_east_raw.KELT_N04_lc_056899_V01_west_raw.
47
220531502V1040_Sco5.43216B2Ve238.48275-23.97809722
48
2028981731eps_Cap4.70159B3Vpe324.270125-19.46601389
49
465735344GG_Car7.696B[e]_or_SG163.9954792-60.3926207810-11B[e]_Chile
50
11411724StHA_527.616B1.5V85.409923-2.2590136ABE-A42cbeKELT_S05_lc_000674_V01_east_raw.KELT_S05_lc_000777_V01_west_raw.
51
437790952120_Tau5.46365B2IVe83.3817916718.54023056
52
425224332bet_CMi2.992B8Ve111.78766678.2893166677
53
375232307lam_Pav4.3731B2Ve283.0542917-62.1875916713
54
19191310251_Oph4.76064A0Ve262.8539583-23.96264167
55
9281047621ome_Ori4.56749B2IIIe84.796458334.1214666676Being observed by BRITE satellite until March 11 2020. 2021-01-16 and 2021-02-10 show roughtly constant Ha profile, symmetric, E/C~1.9. He 6678 has strong and narrow emission wings that are very well-defined.Extremely simple LC, with one main frequency near 1.05 c/d, and a weak harmonic. The main frequency seems variable in amplitude, so it might be an unresolved pair.
56
464643264
CCDM_J19106-6003AB
7.524B9II/III287.658847-60.0457827ABE-254cbeKELT_S27_lc_000266_V01_east_raw.KELT_S27_lc_000400_V01_west_raw.
57
61566852HD_1792539.87B7Ve288.43412-42.413391327BK-166KELT_S27_lc_007130_V01_east_raw.KELT_S27_lc_007197_V01_west_raw.
58
181454187LHA_115-S_1812.8638B[e]_or_SG13.5397565-72.6953588127-28B[e]_Chile
59
304055856LHA_115-S_6511.1642B[e]_or_SG26.01613041-74.680500331-2-1327-28B[e]_Chile
60
180617038LHA_115-S_612.8687B[e]_or_SG11.72928962-73.14281653127-28B[e]_Chile
61
260640910mu_Pic5.8061B9Ve97.99295833-58.753836111-2-3-4-5-6-8-9-10-11-12-1327-28-29-30-31-32-33-34-35-36-37One NRES obs. from Jan 17. Should get another... Virtually no changes at all by April 22 (~100 d later). Kind of remarkable how stable this is. No need for a third spectrum
62
55295028HD_335999.21B2Vpe76.80385-61.805121-2-3-4-5-6-7-8-9-10-11-12-1327-28-29-30-31-32-33-34-35-36-37Monitor at low cadence to see how the disk does or does not develop. Basically no changes by April 22. No need for further spectra.FIDEOSInteresting behavior in TESS year 1. We see disk build-up, and then subsequent dissipation, with much higher amplitude oscillations during build-up. Shell star.BK-144KELT_S20_lc_002751_V01_east_raw.KELT_S20_lc_002753_V01_west_raw.
63
30322368LHA_120-S_7310.3537B[e]_or_SG74.19616509-69.840213081-2-3-4-5-6-7-8-9-10-11-12-1327-28-29-30-31-32-33-34-35-36-37Definitely shows some longer-term (tens of days) trends in the 2 sectors of 2-min TESS data. Need to get all sectors from cycle 1B[e]_Chile
64
404851658LHA_120-S_13410.8757B[e]_or_SG85.05552557-69.379576811-2-3-4-5-6-8-9-10-11-12-1327-28-29-30-31-32-33-34-35-36-37B[e]_Chile
65
373848027LHA_120-S_3512.8192B[e]_or_SG81.8243462-66.368228971-2-3-4-5-7-8-9-10-11-12-1327-28-29-30-31-32-33-34-35-37-38B[e]_Chile
66
425083216HD_2697237.7019B[e]_or_SG83.10401996-67.698225381-2-3-4-6-7-8-9-10-11-12-1327-28-29-30-31-32-33-34-36-37-38B[e]_Chile
67
277022967LHA_120-S_1248.8053B[e]_or_SG83.81930487-69.677344351-2-3-4-5-6-7-8-9-10-11-12-1327-28-29-30-31-32-33-35-36-37-38B[e]_Chile
68
277172980LHA_120-S_12710.6563B[e]_or_SG84.10772412-69.382163691-2-3-5-6-7-8-9-10-11-12-1327-28-29-30-31-32-33-35-36-37-38Attempting NRES obs for this supergiant with the B[e] programB[e]_Chile
69
277173642LHA_120-S_12810.8939B[e]_or_SG84.1820595-69.496513721-2-3-4-5-6-7-8-9-10-11-12-1327-28-29-30-31-32-33-35-36-37-38B[e]_Chile
70
30315586LHA_120-S_1212.2074B[e]_or_SG74.4032518-67.793716181-3-4-5-6-7-8-9-10-11-1327-28-29-30-31-33-34-35-36-37-38B[e]_Chile
71
279430029HD_530487.95B6Vne105.0433-56.9071-2-3-4-5-6-7-8-9-10-11-12-1327-28-29-30-32-33-34-35-36-37-38BK-145KELT_S21_lc_000990_V01_east_raw.KELT_S21_lc_000944_V01_west_raw.
72
729730410LHA_120-S_11119.7458B[e]_or_SG82.07512105-69.138052492-3-4-5-6-7-8-9-10-12-1327-28-29-30-32-33-34-35-36-37-38B[e]_Chile
73
40717307LHA_120-S_2210.6288B[e]_or_SG78.47082504-67.448523591-3-4-5-6-7-8-9-10-11-1327-28-30-31-33-34-35-36-37-38-39B[e]_Chile
74
358467471HD_656636.66B8Ve119.06572-61.099491-4-7-8-9-10-1127-28-31-34-35-36-37FIDEOS2 very clear, typical, weak signals in the normal regime of g1 and g2. Possibly some mild amplitude variation, but not much.Kind of weak, stable disk in 3 BeSS spectra 2014 - 2016, Ha E/C=1.6BK-176NULLKELT_S34_lc_000525_V01_west_raw.
75
179305185LHA_120-S_967.4155B[e]_or_SG79.55982187-69.250318931-2-3-4-5-6-7-8-9-10-11-12-1327-29-30-31-32-33-34-35-36-37-39B[e]_Chile
76
364398342V374_Car5.9346B2IVnpe119.710625-60.824461111-4-7-8-9-10-1127-31-34-35-36-37Scheduled 1 NRES obs. Mar 02 2021. Symmetric double-peaked Ha 2.75 continuum. Definite LPVs in He by March 18, and slight increase in HaFIDEOSTypical freq. groups with obvious enhancement of g2 during flicker events.
77
372913367V373_Car8.91Be119.44136-60.826321-4-7-8-9-10-1127-31-34-35-36-37BK-195KELT_S34_lc_002447_V01_east_raw.KELT_S34_lc_002607_V01_west_raw.
78
341040849HD_648317.7B8Vne118.09283-59.493134-7-8-9-1027-34-35-36-37BK-183KELT_S34_lc_001349_V01_east_raw.KELT_S34_lc_001565_V01_west_raw.
79
2028220823eta_PsA5.63734B8Ve330.2092917-28.45373889128
80
355653322eps_Tuc4.5689B8Ve359.9790833-65.57713333128
81
47296054eps_PsA4.25765B8Ve340.1639167-27.04361667228
82
53992511UU_PsA6.13289B4IVne331.1532083-26.82236111128
83
281741629BG_Phe10.75B5e12.25548-56.09704228-29BK-142KELT_S18_lc_004929_V01_east_raw.KELT_S18_lc_005277_V01_west_raw.
84
404850274HD_2699539.2671B[e]_or_SG85.05069622-69.668014691-2-3-4-5-6-8-9-10-11-12-1328-29-30-31-32-33-34-35-36-38-39B[e]_Chile
85
308748912HD_684236.38B6Ve122.1027-63.800771-4-8-9-10-1128-31-34-35-36-37-38Unremarkable TESS LC.BK-168KELT_S34_lc_000220_V01_east_raw.KELT_S34_lc_000271_V01_west_raw.
86
4393978942_Cet4.5914B9IVne0.9349583333-17.33599167229
87
224244458bet_Scl4.4997B9.5IVmnpe353.24275-37.81826667229
88
7207176480HD_198188.8B9.5Vne47.10865-59.373732-329-30Spectra to monitor Halpha is interesting. This star has chromospheric activity and flares. Not a classical Be star though.BK-143KELT_S19_lc_001874_V01_east_raw.KELT_S19_lc_001931_V01_west_raw.
89
139472176HD_148508.58B8Ve35.75218-29.61945330BK-704KELT_S30_lc_000977_V01_east_raw.KELT_S30_lc_001023_V01_west_raw.
90
14088298HD_334538.1B8Vne77.11026-40.912435-631-32BK-146KELT_S21_lc_001300_V01_east_raw.KELT_S21_lc_001337_V01_west_raw.
91
388935225MWC_6759.448HAeB[e]84.105975-6.716029632ABE-P16bpeKELT_S05_lc_006421_V01_east_raw.KELT_S05_lc_007300_V01_west_raw.
92
323348984HD_373307.566B5III84.4727250.968581632BK-420ABE-248cbeKELT_S05_lc_000558_V01_east_raw.KELT_S05_lc_000670_V01_west_raw.
93
411933674TYC_1283-1360-111.147none79.48512615.32254432ABE-173shellKELT_S05_lc_038477_V01_east_raw.KELT_S05_lc_039260_V01_west_raw.
94
427451587HD_371498.14B8Ve84.07428-1.63536632BK-428KELT_S05_lc_001553_V01_east_raw.KELT_S05_lc_001969_V01_west_raw.
95
427396133HD_371157.173B7.5V83.975354-5.628421632BK-417ABE-181cbeKELT_S05_lc_000410_V01_east_raw.KELT_S05_lc_000466_V01_west_raw.
96
427400331HD_2906629.63A0Vpe83.98129-0.77756632BK-448KELT_S05_lc_010461_V01_east_raw.KELT_S05_lc_010261_V01_west_raw.
97
011286209sig_Ori_E6.768B2IV-Vp84.69666-2.594594632Not a Be star. Magnetic rapid rotatorABE-236sigorienannone
98
571132174228_Eri5.48451B2Vne67.278875-13.04836667532In TESS s32, interesting dissipation phase, followed by a short flicker where groups are enhanced after the rising phase.Possible flickers in TESS year 1. Good to monitor for mass ejections.Double-peaked E/C~4 Ha emission, symmetric Hb, and an extremely sharp red edge to O I. Mild V/R variability in Ha and Hb. Possibly some activity in He 6678
99
5617972056_Eri6.0504B2Ve71.02216667-8.503566667532
100
264631173V1372_Ori7.514B2Vne82.2019152.164707632BK-418ABE-A41cbeKELT_S05_lc_000676_V01_east_raw.KELT_S05_lc_000783_V01_west_raw.