Sample TESS target pixel file stack and aperture (TIC 261136679 shown here).
The TESS mission successfully launched on 18 April 2018 and began science operations on 25 July 2018. Observations of science Sector 1 were performed from 25 July to 22 August, during which pixel data from nearly 16,000 objects were collected at two-minute cadence. These data were sent to the Science Processing Operations Center (SPOC) at NASA Ames for calibration, reduction, cotrending, and transit detection. The potential planet signatures, in the form of Threshold Crossing Events (TCEs), were reviewed by the TESS Science Office to identify targets for imaging and spectroscopic follow-up. A total of 44 high-quality planet candidates in Sector 1 were initially selected from the two-minute cadence data for follow-up observations by the TESS Follow-Up Program (TFOP). Additional deliveries of alerts are provided as more Sectors and multi-Sector searches are conducted by the team. In the table below, the target pixel files, extracted light curves, and data validation reports for planet candidates identified as TESS Data Alerts are made available for download.
The release notes describing these products can be downloaded via the Data Release Notes link at the top of this page. You can refer to the full collection of TESS-DATA-ALERTS data products using the DOI http://dx.doi.org/10.17909/t9-wx1n-aw08 .
The target pixel files (TPFs), extracted light curves, and Data Validation (DV) files are stored as FITS or PDF files, with the following naming convention:
hlsp_tess-data-alerts_tess_phot_<tid>-<s##>[-##]_tess_v1_<exten>
where:
<tid> = TESS Input Catalog (TIC) identifier of the host star
<s##> = the 2-digit, zero-padded sector number the TPF comes from
[-##]; = the 2-digit, zero-padded planet candidate number, only present for the dvs.pdf files
<exten> = "tp.fits" for the target pixel files, "lc.fits" for the extracted light curve files, "dvr.pdf" for the full report PDFs, and "dvs.pdf" for the DV summary PDFs
As an example, here are the full file names for the data products from TIC 52368076, from Sector 1, for the second planet candidate:
hlsp_tess-data-alerts_tess_phot_00052368076-s01-02_tess_v1_dvs.pdf
hlsp_tess-data-alerts_tess_phot_00052368076-s01_tess_v1_dvr.pdf
hlsp_tess-data-alerts_tess_phot_00052368076-s01_tess_v1_lc.fits
hlsp_tess-data-alerts_tess_phot_00052368076-s01_tess_v1_tp.fits
Some targets have additional data validation reports that include information from multiple sectors. In those cases, the files include multiple sector numbers in the dvr.pdf and dvs.pdf files. For example, the "dvs.pdf" files and the "dvr.pdf" file for the target TIC 51912829 that has three planet candidates and include data from both sectors 1 and 2 are named:
hlsp_tess-data-alerts_tess_phot_00051912829-s01s02-01_tess_v1_dvs.pdf
hlsp_tess-data-alerts_tess_phot_00051912829-s01s02-02_tess_v1_dvs.pdf
hlsp_tess-data-alerts_tess_phot_00051912829-s01s02-03_tess_v1_dvs.pdf
hlsp_tess-data-alerts_tess_phot_00051912829-s01s02_tess_v1_dvr.pdf
In addition to the TPF and DV files, a .csv table containing information on the TOI's released as part of the TESS data alerts HLSP is also included in the table below. The .csv columns are:
TIC ID, TOI ID, Disposition, RA (deg.), Dec. (deg.), TESS mag, TESS mag uncertainty, Primary Transit Epoch (T0) (BJD - 2457000.), T0 Uncertainty, Orbital Period (days), Orbital Period Uncertainty, Primary Transit Duration (hours), Primary Transit Duration Uncertainty
Note that the names of files released as part of the Data Alerts HLSP do not follow the same naming convention as TESS data products in the full public release. Except where and if noted, the Data Alerts files are produced by the TESS mission pipeline. The format and structure of those products are identical to the ones to be released in the first TESS data release.
The data products are available for download through the table below. A bundle of all data products for all targets is available for download at the top of the table. Note that the exoplanet parameters are from the Sector 1 information when an exoplanet candidate is present in both Sector 1 and Sector 2. Rows containing data products that analyze multiple sectors of data together are denoted by multi-sector strings, e.g., "1-3" for data that span Sectors 1 through 3. But note: the range is the possible minimum and maximum Sectors used, it does not mean data was necessarily used from each Sector in the range in that column or file name. Always consult the information contained with the data validation reports to determine what data was used to generate those reports. Some planet candidates only have sector-combined data validation files, in those situations, the individual sector DV table cells will be empty, and the corresponding sector-combined DV files should be the primary reference for data validation information.
Note: Some TOI's were identified from the Full Frame Images using an MIT "Quick Look Pipeline" (QLP). These do not have 2-minute cadence products at the time they were announced, and are identifed as such with "FFI" and "FFI-QLP" in the table below. Download the Full Frame Images from the mission data products for these targets using MAST interfaces like TESSCut, the Portal, Astroquery, or bulk downloads. For a summary of how to search for and retrieve TESS data products, see the Data Search Summary page of the TESS Archive Manual.
TOI Target Information (Download .csv File ) | Bundle Of All Files (Download .tar.gz File ~9 GB)
TIC ID
TOI ID
RA (deg.)
Dec. (deg.)
Period (days)
Epoch (TJD)
Sectors
TP File
LC File
DV File
Comment
1129033
398.01
37.155148
-7.060682
1.36003
1412.34503
 
4
FFI
FFI
FFI-QLP
WASP-77b
2758565
287.01
356.283124
-17.449174
3.78192
1356.03117
 
2
FFI
FFI
FFI-QLP
synchronized with stellar rotation
2760710
227.01
356.527700
-16.691200
NaN
1364.102069
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
The second event is not real. single transit (no period).
7624182
412.01
64.311397
-38.844151
1.10801
1411.822
 
4,5
FFI
FFI
FFI-QLP
need to check 7624180 with follow-up
8988289
316.01
354.759305
-9.882061
13.32379
1365.98759
 
2
FFI
FFI
FFI-QLP
V-shaped
9006668
238.01
349.231362
-18.606628
1.272419
1354.669184
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
centroid offset not significant.
9032368
373.01
355.901887
-11.269515
1.632
1355.67942
 
2
FFI
FFI
FFI-QLP
target is likely 9032367 (still possible to be a planet);
9033144
367.01
349.606182
-19.823931
4.71452
1354.29153
 
2
FFI
FFI
FFI-QLP
likely EB
9100874
307.01
350.578441
-22.677390
6.16425
1357.84005
 
2
FFI
FFI
FFI-QLP
none
9102327
313.01
350.779792
-19.419677
3.2615
1354.54332
 
2
FFI
FFI
FFI-QLP
target star is two stars in Gaia (); check if it is on target;
9725627
239.01
358.408542
-10.118057
4.15701
1356.962278
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
9727392
236.01
358.444723
-10.884944
4.534451
1355.325711
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1700 ppm secondary. Likely EB.
9858404
394.01
48.499528
-8.573568
0.39149
1411.26947
 
4
FFI
FFI
FFI-QLP
v-shaped; some odd-even
12421862
198.01
2.268200
-27.122100
20.427265
1356.375417
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
12423815
234.01
2.568707
-26.282400
2.839249
1356.088115
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
centroid shift is not significant.
12862099
259.01
3.903156
-11.938108
2.423823
1386.578118
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-44
13023378
344.01
347.053599
-28.007883
6.06764
1358.25733
 
2
FFI
FFI
FFI-QLP
none
13023738
360.01
347.084817
-29.590306
8.05577
1354.97828
 
2
FFI
FFI
FFI-QLP
centroid shift in X/Y is due to the star nearby but the signal is on target.
20892672
378.01
1.398970
-19.489429
3.10926
1356.50088
 
2
FFI
FFI
FFI-QLP
2 stars in same pixel with dmag 1
25155310
114.01
63.373890
-69.226789
3.28891
1327.51895
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-126
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
25375553
143.01
328.767654
-22.612566
2.310894
1325.58249
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
27966179
330.01
358.751494
-22.538712
4.27958
1355.6917
 
2
FFI
FFI
FFI-QLP
none
29344935
109.01
313.215480
-25.687338
2.766737
1326.127529
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-14
29781292
282.01
65.238019
-68.102664
56.00327
1337.21241
 
1
tp.fits
lc.fits
|
two transits; a third transit could be an eccentric secondary or single transit of second planet; there are nearby stars (TIC 29781293) and centroid analysis inconclusive
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
29781292
282.02
65.238019
-68.102664
31.323499
1355.735635
 
1
tp.fits
lc.fits
|
could be a secondary of .01 or a single transit detection of a second planet
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
29831208
124.01
66.582618
-67.806508
1.84286
1326.544424
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
known TOI
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
29857954
172.01
316.631883
-26.692620
9.47572
1326.91973
 
1
FFI
FFI
FFI-QLP
Star to NW checked. Transit likely on the target.
29960109
393.01
42.249300
-14.537900
2.49221
1411.66942
 
4
FFI
FFI
FFI-QLP
may be on 29960110
32090583
218.01
58.420270
-68.739532
0.438317
1325.550345
 
1
tp.fits
lc.fits
|
known TOI; host star is m dwarf
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
33911302
341.01
355.844948
-23.997888
1.81383
1355.75117
 
2
FFI
FFI
FFI-QLP
none
35857242
400.01
41.639090
-0.463937
3.6349
1413.31319
 
4
FFI
FFI
FFI-QLP
WASP-138
37749396
260.01
4.773193
-9.964846
13.470018
1392.294408
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
only two transits
38541473
395.01
56.304548
-10.973384
6.06054
1415.51522
 
4
FFI
FFI
FFI-QLP
large; possible EB
38696105
281.01
66.136300
-60.129968
5.566734
1387.482051
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
38846515
106.01
68.959732
-64.027040
2.84938
1326.74502
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-100
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
41865539
335.01
21.322323
-39.947812
1.26092
1354.86627
 
2,3
FFI
FFI
FFI-QLP
odd even unreliable
42054565
280.01
24.168710
-36.413670
10.175948
1393.67584
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
low SNR; possible instrument systematic; source is possibly 42054566 which is 4.24 as away
47316976
288.01
340.307725
-28.032712
NaN
1364.46064
 
2
FFI
FFI
FFI-QLP
single transit
47423120
352.01
342.067496
-24.838607
11.6235
1356.83006
 
2
FFI
FFI
FFI-QLP
The period could be half;
47425697
364.01
342.256131
-24.959275
0.49393
1354.46949
 
2
FFI
FFI
FFI-QLP
a little v-shaped; possible EB
47484268
226.01
342.966400
-24.787500
NaN
1358.500535
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
The second event is not real. Single transit (no period).
47525799
225.01
343.879737
-24.409619
NaN
1355.118503
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
single transit (no period); centroid information is hard to interpret
49687222
254.01
351.705496
-11.725416
20.186539
1360.073308
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
The transit shape looks asymmetric but it is not near known systematics; recommend to confirm signal on target before follow up.
49710555
291.01
352.164383
-10.859566
12.07397
1359.62204
 
2
FFI
FFI
FFI-QLP
possible centroid shift
49899799
416.01
48.854273
-2.175283
7.01152
1413.19546
 
4
FFI
FFI
FFI-QLP
tropical Jupiter
51912829
180.01
14.298400
-67.496272
0.835398
1325.897913
 
1
tp.fits
lc.fits
|
Likely EB
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
52204645
209.01
19.394306
-66.902497
4.379757
1325.883984
 
1
tp.fits
lc.fits
|
The signal is likely on target; the centroid offset seen in SPOC report is likely caused by the nearby giant 9th mag star;which has a peak in periodogram at 8.60 days; and causes the second bright spot seen in difference image
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
52368076
125.01
23.594697
-66.675830
4.653811
1327.432906
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
52368076
125.02
23.594697
-66.675830
9.150607
1334.45669
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
second planet (125.02)
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
52368076
125.03
23.594697
-66.675830
19.981866
1342.851835
 
1
tp.fits
lc.fits
| dvr.pdf
period is likely correct but possibly two independent single transits
2
tp.fits
lc.fits
| dvr.pdf
1-2
dvs.pdf | dvr.pdf
55452495
336.01
70.670414
-64.885194
8.85709
1328.46551
 
1,2,3,4,5
FFI
FFI
FFI-QLP
2x period; hot star; may not be on target
55650590
206.01
73.737190
-62.522369
0.736283
1325.542781
 
1
tp.fits
lc.fits
|
Gaia indicates it is an M dwarf
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
55652896
216.01
73.980231
-63.260063
34.539342
1331.28513
 
1
tp.fits
lc.fits
|
warm Jupiter
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
55652896
216.02
73.980231
-63.260063
17.099142
1325.335632
 
1
tp.fits
lc.fits
|
another warm Jupiter in the system
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
| dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
62483237
139.01
336.402307
-34.909623
11.058421
1334.896388
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Level 1 candidate
63898957
261.01
15.217632
-24.423907
3.361391
1387.285571
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
ambiguous period
63898957
261.02
15.217632
-24.423907
13.039359
1389.727185
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
ambiguous period; many transits; need photometry to constrain period
66356824
315.01
12.076306
-32.119339
1.77662
1355.60958
 
2,3
FFI
FFI
FFI-QLP
none
66413476
325.01
13.876994
-33.512212
4.36924
1357.72126
 
2,3
FFI
FFI
FFI-QLP
There might be some odd even difference.
66497310
343.01
356.045314
-18.889502
1.75649
1355.52155
 
2
FFI
FFI
FFI-QLP
none
69838258
339.01
337.921602
-21.945681
6.73069
1354.57336
 
2
FFI
FFI
FFI-QLP
difference image not conclusive
70440470
126.01
339.489337
-35.153982
3.035381
1326.731043
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
70513361
262.01
32.533514
-31.069860
11.146909
1389.839926
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
ambiguous period
70785910
348.01
1.583606
-30.336272
0.49486
1354.36474
 
2
FFI
FFI
FFI-QLP
V-shaped;
70797900
224.01
1.977400
-29.979000
NaN
1365.843681
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
V-shaped; single transit; likely EB.
76923707
181.01
352.171955
-34.491371
4.532037
1358.118127
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
76989773
182.01
353.294594
-35.463618
1.769141
1355.082723
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
v-shaped; two stars in PSF
77031413
368.01
354.170142
-34.611816
1.38665
1355.1953
 
2
FFI
FFI
FFI-QLP
two stars in the same pixel;
77031414
241.01
354.168219
-34.611234
1.386653
1355.195771
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
target could also be 77031413.
77044471
228.01
358.558713
-30.012999
2.686063
1356.102509
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-16
79395355
164.01
320.054165
-51.309907
7.31898
1328.33733
 
1
FFI
FFI
FFI-QLP
Potential blend with 79395356 to NE
80432617
359.01
11.673080
-42.361801
5.48403
1360.67423
 
2
FFI
FFI
FFI-QLP
two events (near 1360 and 1377); wrong period?
80439101
340.01
11.747296
-44.369938
7.42229
1361.05759
 
2
FFI
FFI
FFI-QLP
V-shaped; likely EB; period could be twice the reported.
89020549
132.01
338.399420
-43.436628
2.109307
1326.903983
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Possible centroid shift toward faint star to the SE
92226327
256.01
11.247108
-15.271294
24.73712
1389.285282
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
LHS-1140b
92226327
256.02
11.247108
-15.271294
3.778378
1389.293276
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
LHS-1140c
92352620
107.01
313.783108
-34.135572
3.950054
1328.29934
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-94A (planet host)
92359850
387.01
52.225563
-19.979760
4.15493
1411.50406
 
4
FFI
FFI
FFI-QLP
should check 92359852 with follow-up photometry
97409519
113.01
332.714323
-30.749674
3.372877
1327.053085
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-124
99493790
162.01
317.639656
-23.305696
7.76686
1332.98188
 
1
FFI
FFI
FFI-QLP
100014359
380.01
23.280468
-47.882043
0.50459
1354.38198
 
2,3
FFI
FFI
FFI-QLP
none
100097716
354.01
24.047739
-42.303771
2.99995
1354.37712
 
2,3
FFI
FFI
FFI-QLP
Two stars in the same pixel
100099031
353.01
24.272345
-46.945312
1.29866
1355.02081
 
2,3
FFI
FFI
FFI-QLP
big;
100100827
185.01
24.354314
-45.677896
0.941449
1354.458014
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-18b
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
100990000
411.01
54.819851
-42.762575
9.57219
1386.18895
 
3,4
FFI
FFI
FFI-QLP
101948569
240.01
14.754696
-44.160832
19.472408
1360.113171
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
102030574
305.01
15.844683
-44.705807
9.94962
1364.10083
 
2
FFI
FFI
FFI-QLP
likely EB;
114749636
306.01
359.191553
-22.153163
4.59971
1357.67041
 
2
FFI
FFI
FFI-QLP
none
115242351
297.01
6.176856
-36.114396
5.67116
1358.77289
 
2
FFI
FFI
FFI-QLP
none
116156517
338.01
7.709303
-40.573434
5.36732
1357.37358
 
2
FFI
FFI
FFI-QLP
none
118327533
346.01
10.344500
-37.343003
8.28154
1354.79225
 
2
FFI
FFI
FFI-QLP
the period is twice as reported; V-shaped.
118327550
244.01
10.570615
-36.718138
7.395586
1357.365444
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Stellar radius is likely to be smaller because Teff is low. Gaia shows it is a high proper motion star with big parallax.
118586896
365.01
10.922291
-38.043195
12.10588
1365.97342
 
2
FFI
FFI
FFI-QLP
likely EB; V-shaped
120585579
242.01
4.451491
-38.110851
6.340315
1357.778211
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
The detected secondary could have a wrong depth estimation because of the low points near 1380.
120610833
229.01
5.237503
-35.998265
3.126068
1354.773398
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
V-shaped.
120896927
402.01
36.868245
-27.635184
4.75649
1387.67761
 
3,4
FFI
FFI
FFI-QLP
there may be a second planet at the period of 9.698 found by SPOC
120916706
263.01
37.108100
-25.097400
0.556737
1386.172349
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
122612091
264.01
41.040001
-30.169041
2.21685
1385.61513
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-72b
122613513
279.01
41.188507
-32.210889
11.489788
1388.368911
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
129637892
155.01
321.114974
-37.850144
5.43636
1326.74444
 
1
FFI
FFI
FFI-QLP
139285736
377.01
348.039807
-45.017154
1.55028
1326.05107
 
1,2
FFI
FFI
FFI-QLP
possible centroid offset;
139285832
332.01
348.058743
-44.876365
0.77707
1325.80984
 
1,2
FFI
FFI
FFI-QLP
none
139357541
328.01
349.487672
-43.925560
4.47894
1355.80666
 
1,2
FFI
FFI
FFI-QLP
V-shaped
140068425
140.01
330.301574
-49.060026
2.28139
1327.399305
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
140691463
157.01
73.701279
-76.680516
2.08457
1326.54604
 
1,2,3,4,5
FFI
FFI
FFI-QLP
141608198
210.01
88.960448
-73.984659
9.010138
1329.821358
 
1
tp.fits
lc.fits
|
Gaia indicates this is a M dwarf. There is another star in the same aperture; SG1 needed.
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
144065872
105.01
337.457199
-48.003087
2.184659
1326.50599
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-95
144276942
361.01
353.904034
-44.808807
1.53533
1354.57959
 
2
FFI
FFI
FFI-QLP
none
144301052
301.01
354.297494
-42.010266
3.74317
1356.92824
 
2
FFI
FFI
FFI-QLP
none
144301273
376.01
354.445491
-42.966404
2.75161
1355.44295
 
2
FFI
FFI
FFI-QLP
none
144336525
326.01
356.114886
-46.866585
0.24733
1354.25954
 
2
FFI
FFI
FFI-QLP
really short period.
144440290
222.01
359.161519
-44.719088
NaN
1376.544
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
single transit (no period)
145750719
303.01
341.364029
-14.991761
3.56133
1357.55952
 
2
FFI
FFI
FFI-QLP
none
147203645
166.01
323.195894
-44.017794
5.06187
1326.38424
 
1
FFI
FFI
FFI-QLP
149010208
243.01
3.394055
-31.334372
3.437004
1356.619165
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Gaia radius is 1.8 Rsun. Planet radius is big.
149603524
102.01
87.139956
-63.988427
4.4121
1326.07657
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-62
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
149990841
167.01
90.662314
-64.819485
4.45339
1328.03406
 
1,2,4,5
FFI
FFI
FFI-QLP
150030205
286.01
90.983643
-60.666326
4.511412
1327.82102
 
1
tp.fits
lc.fits
|
likely marginal
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
150098860
220.01
91.799884
-61.996896
10.696823
1335.900564
 
1
tp.fits
lc.fits
|
slight grazing
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
152476657
415.01
62.616051
-45.898221
3.61194
1411.72779
 
4,5
FFI
FFI
FFI-QLP
WASP-120
153065527
406.01
49.262400
-42.242400
13.17363
1388.56658
 
3,4
FFI
FFI
FFI-QLP
154618248
245.01
345.778770
-33.500373
8.773772
1361.546719
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
"The target is two stars separated by <1""; TICOffset and OOTOffset not significant; no other star at the location of the centroid shift indicating signal likely on target"
155986102
337.01
7.329948
-50.140124
6.87168
1360.61731
 
2
FFI
FFI
FFI-QLP
The period is twice as reported; there appear to be a second event in the data.
155995204
384.01
7.658508
-52.049388
9.30734
1357.58381
 
2
FFI
FFI
FFI-QLP
big;
156002449
324.01
8.481881
-50.729261
5.2852
1357.7274
 
2
FFI
FFI
FFI-QLP
Big;
156016136
371.01
8.923843
-50.316982
3.4805
1357.43733
 
2
FFI
FFI
FFI-QLP
none
156075294
299.01
10.594603
-48.293550
5.72144
1354.69581
 
2
FFI
FFI
FFI-QLP
none
158623531
246.01
24.168162
-50.659178
7.872846
1355.732521
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-105
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
159951311
265.01
49.562227
-41.302145
5.92479
1387.5705
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-139
160074939
230.01
346.319044
-36.945536
13.340145
1366.329788
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
The transit signal maybe caused by scattered light.
160148385
247.01
1.046353
-47.360626
3.425239
1354.319952
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-96
164767175
266.01
26.209635
-18.400947
10.767807
1393.078739
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
period ambiguous for .01 and .02; unclear which transits are attributed to which candidates; will not be observed again in nominal mission
164767175
266.02
26.209635
-18.400947
6.19132
1392.104974
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
period ambiguous for .01 and .02; unclear which transits are attributed to which candidates; will not be observed again in nominal mission
166697854
300.01
35.737327
-53.070244
2.75753
1354.42965
 
2,3
FFI
FFI
FFI-QLP
two stars in the same pixel; Gaia radius of 166697854 is 1.6 Rsun; second star is 4 as away and dmag 4
166739520
190.01
36.775436
-50.284518
10.020817
1357.571578
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-117
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
166833457
404.01
58.428804
-34.328198
2.96273
1413.16667
 
4
FFI
FFI
FFI-QLP
WASP-98
166836920
267.01
39.897688
-50.008005
5.75244
1387.960271
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-99
167415965
214.01
99.460653
-70.932628
18.55378
1336.68217
 
1
tp.fits
lc.fits
|
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
167418898
383.01
99.609505
-67.656173
10.98042
1335.77232
 
1,2,3,4,5
FFI
FFI
FFI-QLP
could be on 167418903
167754523
409.01
104.181690
-60.686970
1.69992
1326.31473
 
1,2,3,4,5
FFI
FFI
FFI-QLP
centroid offset on 167754526
169765334
329.01
351.320880
-15.634658
5.7018
1354.94883
 
2
FFI
FFI
FFI-QLP
none
170634116
413.01
66.370903
-30.600444
3.66242
1412.89287
 
4,5
FFI
FFI
FFI-QLP
WASP-79
175476629
321.01
350.977728
-38.225709
1.14057
1354.27156
 
2
FFI
FFI
FFI-QLP
"There is some centroid offset
175477257
310.01
351.105838
-36.975983
4.26938
1356.58788
 
2
FFI
FFI
FFI-QLP
none
175482273
369.01
351.229222
-38.160736
5.46349
1354.34549
 
2
FFI
FFI
FFI-QLP
PC (star radius 1.70); Simbad says it's a known double. Gaia did not have a second star at the same coordinate.
176778112
408.01
47.827948
-35.628053
1.33919
1411.5384
 
3,4
FFI
FFI
FFI-QLP
176957796
137.01
101.297297
-66.238034
4.819018
1327.369003
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
3
tp.fits
lc.fits
|
176984236
405.01
101.909386
-66.328353
1.75617
1326.54565
 
1,2,3,4,5
FFI
FFI
FFI-QLP
possible EB on 176984248; small possible secondary eclipse
178155732
396.01
42.984364
-30.814529
3.5873
1384.08418
 
3,4
FFI
FFI
FFI-QLP
possible TASC candidate
178284730
418.01
60.385614
-20.451086
2.23595
1412.69841
 
4,5
FFI
FFI
FFI-QLP
WASP-140
179317684
163.01
79.768168
-71.895588
4.23163
1328.87975
 
1,2,3,4,5
FFI
FFI
FFI-QLP
179985715
249.01
14.080413
-38.948683
6.613147
1359.540377
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
centroid offset not significant.
180145006
312.01
14.523299
-37.942514
3.54148
1357.54535
 
2,3
FFI
FFI
FFI-QLP
none
180285396
292.01
14.713941
-36.688350
10.3698
1363.14401
 
2,3
FFI
FFI
FFI-QLP
V-shaped3
183120439
169.01
16.778300
-75.198873
2.25596
1327.43797
 
1
FFI
FFI
FFI-QLP
183532609
191.01
359.900305
-35.031390
8.159165
1358.920239
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-8
183537452
192.01
357.879533
-39.906726
3.922743
1356.414736
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-29
183593642
355.01
17.888013
-36.709111
1.03742
1355.08121
 
2,3
FFI
FFI
FFI-QLP
potential odd/even difference
183675732
374.01
358.227493
-41.700497
5.4823
1356.62212
 
2
FFI
FFI
FFI-QLP
none
183979262
183.01
21.649233
-72.749038
3.430776
1326.104287
 
1
tp.fits
lc.fits
|
700 ppm secondary; likely EB; possibly synchronized with rotation
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
183985250
193.01
358.667547
-37.628020
0.792072
1354.214863
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Tdur is short for Rstar
184240683
250.01
359.348992
-41.277150
1.628393
1355.508203
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-5
188570092
294.01
339.026294
-16.999954
7.32829
1358.78126
 
2
FFI
FFI
FFI-QLP
none
188593930
320.01
345.522736
-16.359925
1.46503
1354.27607
 
2
FFI
FFI
FFI-QLP
none
198077394
322.01
63.825187
-56.253756
3.99076
1355.68563
 
2,3,4,5
FFI
FFI
FFI-QLP
not synchronized; no GAIA radius
199731190
350.01
21.292013
-47.262926
2.51276
1355.90325
 
2,3
FFI
FFI
FFI-QLP
none
200723869
257.01
47.516558
-50.832418
18.37073
1385.77602
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
First event is a partial transit
201233610
290.01
359.516537
-49.300804
NaN
1360.59149
 
2
FFI
FFI
FFI-QLP
single event; really big
201248411
129.01
0.187097
-54.830506
0.980981
1354.552404
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
TOI 129.01
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
201292545
289.01
2.900495
-56.599656
NaN
1326.64586
 
1,2
FFI
FFI
FFI-QLP
single event; no period
201793781
248.01
34.683547
-54.859771
5.991198
1354.835774
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
known TOI
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
204317710
255.01
346.075057
-21.271946
2.812077
1355.983448
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-32
204376737
231.01
348.157236
-22.673953
3.361021
1357.394512
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-6
206352378
318.01
355.015478
-53.039028
3.74649
1327.33174
 
1,2
FFI
FFI
FFI-QLP
V-shaped; need to check if it is on target.
206466531
410.01
56.815204
-52.985150
1.42748
1384.6552
 
3,4
FFI
FFI
FFI-QLP
206609630
212.01
22.551000
-59.583200
0.335269
1325.491317
 
1
tp.fits
lc.fits
|
Possible M dwarf; Gaia give this source duplication flag; no radius/parallax available
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
206669860
327.01
343.633006
-34.502741
10.06378
1362.96027
 
2
FFI
FFI
FFI-QLP
two events; odd even?
206686292
298.01
344.060677
-34.361099
1.32901
1354.35602
 
2
FFI
FFI
FFI-QLP
synchronized?
207081058
121.01
331.867232
-41.815456
14.775056
1336.139719
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Warm Jupiter candidate with a possible secondary
207084429
381.01
22.756615
-51.215438
4.89388
1356.07033
 
2,3
FFI
FFI
FFI-QLP
the target may be on the neighbor on the north (Rstar 1.3; dmag=6).
207141131
179.01
44.262259
-56.192071
4.137394
1354.588395
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
known TOI
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
211438925
194.01
5.160559
-23.935731
4.899379
1356.565648
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-20
219253008
268.01
65.915985
-53.850952
5.06671
1385.12523
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
GAIA visual binary with 2as separation and equal mass
219338557
133.01
354.395739
-58.954636
8.1952
1327.291396
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
219379012
397.01
76.833821
-48.115925
1.54683
1412.48913
 
4,5
FFI
FFI
FFI-QLP
close companion star 219379014
219388773
399.01
77.047581
-50.858766
1.57111
1412.39194
 
4,5
FFI
FFI
FFI-QLP
220016044
357.01
32.321768
-48.484745
0.93985
1354.34394
 
2,3
FFI
FFI
FFI-QLP
weak signal
220396259
379.01
68.891565
-56.138684
0.91693
1354.7083
 
2,3,4,5
FFI
FFI
FFI-QLP
needs follow-up to confirm whether is on target
220435095
147.01
73.641400
-57.513557
3.42316
1326.61107
 
1,2,3,4,5
FFI
FFI
FFI-QLP
220459976
285.01
74.697149
-56.394049
32.332528
1361.663925
 
2
tp.fits
lc.fits
|
possible single transit
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
220479565
269.01
75.846109
-54.177194
3.69799
1385.54129
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
220518305
156.01
41.467255
-64.320724
14.14893
1336.13203
 
1,3
FFI
FFI
FFI-QLP
Warm Jupiter candidate with a period of about 14 days
224225541
251.01
353.061818
-37.255890
4.937712
1357.305816
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
centroid shift not significant.
224245334
333.01
353.357466
-41.171509
3.79069
1355.55844
 
2
FFI
FFI
FFI-QLP
none
224271611
347.01
354.489847
-36.571572
4.0394
1355.18601
 
2
FFI
FFI
FFI-QLP
none
228381868
351.01
357.580534
-17.077572
3.46583
1356.67382
 
2
FFI
FFI
FFI-QLP
star is evolved
228507250
309.01
358.039584
-15.800830
6.15864
1360.01144
 
2
FFI
FFI
FFI-QLP
none
229091748
382.01
3.797690
-46.272415
0.4568
1354.59152
 
2
FFI
FFI
FFI-QLP
none
229111835
302.01
17.480755
-52.239441
6.70145
1356.68237
 
2
FFI
FFI
FFI-QLP
none
230982885
195.01
24.604344
-55.772082
2.072761
1355.490416
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-97
231081369
153.01
68.073647
-66.916366
7.63227
1329.84791
 
1,2,3,4,5
FFI
FFI
FFI-QLP
231663901
101.01
318.736981
-55.871780
1.430401
1326.008874
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-46
231670397
104.01
319.949611
-58.148876
4.087445
1327.673462
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-73
231702397
122.01
332.947000
-58.945100
5.077677
1329.121491
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Small star with a small planet candidate
231912935
215.01
7.318019
-63.790619
26.296721
1334.391185
 
1
tp.fits
lc.fits
|
A weak detection.
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
233964642
334.01
36.498808
-63.647560
17.91563
1325.44586
 
1,2,3
FFI
FFI
FFI-QLP
v-shaped; source is possibly 233964643
234345288
213.01
38.886663
-71.624147
23.516847
1343.336546
 
1
tp.fits
lc.fits
|
Be aware one of the signals is on the edge.
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
234519192
196.01
14.551711
-64.761619
1.163088
1354.30751
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
v-shaped
234523599
127.01
15.551099
-61.756001
3.795609
1325.650197
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
234994474
134.01
350.031300
-60.065200
1.401461
1326.033176
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Level 1 candidate
235037761
131.01
353.826767
-64.561769
6.240662
1326.068952
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
V shaped
237924601
252.01
57.553578
-63.053777
1.002192
1354.720066
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
known TOI
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
238059180
386.01
104.138389
-53.545486
5.112
1356.21389
 
2
FFI
FFI
FFI-QLP
v-shaped; two stars about 1as separation in same pixel
238176110
116.01
357.845260
-70.152863
2.798594
1326.689274
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-91
244161191
278.01
4.883100
-5.911300
0.298746
1386.106592
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
possible dipper; not a planet candidate; Rstar may be larger than stated
250386181
390.01
30.114395
-4.985569
1.47043
1412.37337
 
4
FFI
FFI
FFI-QLP
nearby star is 6 mag fainter
251848941
178.01
7.301250
-30.453734
6.558054
1360.242325
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
251848941
178.02
7.301250
-30.453734
10.354252
1354.55219
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
similar period to candidate 3
251848941
178.03
7.301250
-30.453734
9.955936
1362.953314
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
similar period to candidate 2 and may be wrong; only two transits
251852984
323.01
8.202822
-32.059327
2.77422
1355.57459
 
2
FFI
FFI
FFI-QLP
none
251855940
370.01
8.659667
-32.166524
4.04655
1354.28979
 
2
FFI
FFI
FFI-QLP
none
251878904
366.01
9.691992
-34.214912
1.70429
1354.48285
 
2
FFI
FFI
FFI-QLP
too faint
253917293
160.01
337.500659
-31.924254
4.608
1327.37627
 
1
FFI
FFI
FFI-QLP
Source is star to the WSW (253917292).
257567854
403.01
52.818043
-23.819696
3.53272
1411.90242
 
4
FFI
FFI
FFI-QLP
WASP-22
259377017
270.01
68.415400
-51.956200
5.660209
1389.502678
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
possibly half or same period as .02
259377017
270.02
68.415400
-51.956200
11.379126
1389.678659
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
period possibly half because of gap in data
259377017
270.03
68.415400
-51.956200
3.359857
1387.092173
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
259511357
271.01
70.775334
-50.219614
2.47603
1384.70394
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
259701242
401.01
74.466266
-53.817906
2.4861
1384.17554
 
3,4,5
FFI
FFI
FFI-QLP
may be on 259701232
259962054
203.01
43.018800
-67.687600
51.953234
1327.729066
 
1
tp.fits
lc.fits
|
M dwarf; first transit is on/near momentum dump; the transit duration is a bit long for the reported period;
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
260043723
217.01
91.608606
-58.953644
3.13879
1327.066685
 
1
tp.fits
lc.fits
|
possible centroid shift
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
260271203
207.01
94.218078
-58.229816
5.64939
1330.09558
 
1
tp.fits
lc.fits
|
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
260304296
187.01
94.615669
-57.013569
0.512589
1325.778915
 
1
tp.fits
lc.fits
|
v-shaped; very likely EB
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
260609205
219.01
97.453901
-57.254837
4.461939
1328.754344
 
1
tp.fits
lc.fits
|
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
260985861
149.01
76.635855
-80.768181
3.34024
1327.40226
 
1
FFI
FFI
FFI-QLP
Source is apparently 260985864- which may be a planet depending on host star size.
261136679
144.01
84.291198
-80.469143
6.266571
1325.503694
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Π Mensae
262530407
177.01
20.439100
-46.714400
2.853133
1356.153
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
known TOI
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
262530780
363.01
20.547259
-44.861946
8.22393
1361.87743
 
2,3
FFI
FFI
FFI-QLP
none
262530873
304.01
20.494044
-44.416756
2.24172
1356.28606
 
2,3
FFI
FFI
FFI-QLP
Likely EB; Big but flat bottomed.
262531275
331.01
20.419310
-42.481733
2.48421
1356.00813
 
2,3
FFI
FFI
FFI-QLP
possible centroid offset; the fainter star to the north has a smaller radius than the target.
263003176
130.01
12.541184
-83.743964
14.339928
1336.559583
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Centroid shift is almost a pixel away but there is no corresponding star in that position. There are two nearby stars Gmag=13 close to the NW and Gmag=18 to the SE. If the transit signal is on target it is a small planet around a bright star.
265612438
145.01
333.174746
-55.978763
5.12944
1327.04953
 
1
FFI
FFI
FFI-QLP
Some confusion about whether source is this star or the close pair of equal brightness stars to the NE (260985864)- but difference image seems to indicate source is more likely to be this star.
266980320
118.01
349.556843
-56.903885
6.036061
1329.199631
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
267263253
135.01
7.328937
-76.304075
4.126904
1325.783759
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
268766053
272.01
31.909198
-20.661837
3.30968
1386.231709
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-53
270341214
173.01
33.458316
-80.582809
NaN
1333.41089
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Single-transit planet candidate, identified in report as having a 14.2-day period. The transit parameters provided with this TOI (and not those in the DV report) are the correct ones.
271893367
150.01
112.965695
-73.606125
5.85758
1326.27838
 
1,2,3,4,5
FFI
FFI
FFI-QLP
271900960
389.01
112.941801
-75.527428
13.45913
1330.37074
 
1,2,3,4,5
FFI
FFI
FFI-QLP
272086159
176.01
115.003400
-72.207700
16.15427
1363.04625
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
277103955
284.01
84.254370
-66.791439
1.30926
1326.41347
 
1
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
277683130
138.01
328.926194
-61.673286
6.198041
1328.058635
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
278683844
119.01
99.237983
-58.015237
5.541738
1327.614054
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
119.01
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
278683844
119.02
99.237983
-58.015237
10.694535
1328.037451
 
1
tp.fits
lc.fits
| dvr.pdf
119.02
2
tp.fits
lc.fits
| dvr.pdf
3
tp.fits
lc.fits
| dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
278866211
189.01
100.807855
-55.244540
2.194097
1327.357534
 
1
tp.fits
lc.fits
|
8th mag star nearby; v-shaped; likely on target
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
279251651
419.01
104.155300
-59.183300
0.40387
1354.46663
 
1,2,3,4,5
FFI
FFI
FFI-QLP
Rstar 0.55; may be on 279251647
279740441
273.01
51.504634
-64.548553
0.741859
1386.095087
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
still can be a planet on 279740439
1-3
dvs.pdf | dvr.pdf
279741379
186.01
51.746760
-63.499154
NaN
1350.3
 
1
tp.fits
lc.fits
|
known TOI; single transit; no period; associated report shows a second TCE at 7.78 days
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
280095254
235.01
46.196133
-73.396554
20.180235
1357.283631
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
V-shaped. Radius Teff and logg not consistent with each other; recommend follow-up to check stellar parameters. The period could be half of the current value. Gaia has excess astrometric noise.
280097543
375.01
47.150091
-77.383278
9.44859
1329.29739
 
1,2
FFI
FFI
FFI-QLP
needs follow-up to confirm stellar parameters
280830734
188.01
44.555164
-70.760917
1.162031
1325.777845
 
1
tp.fits
lc.fits
|
V-shaped; variable slightly evolved star
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
281459670
110.01
5.618692
-59.942551
3.174305
1328.040464
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-30
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
281541555
115.01
6.702439
-56.316124
4.742745
1329.90069
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-46
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
281575427
205.01
7.975187
-56.965111
4.251801
1326.336481
 
1
tp.fits
lc.fits
|
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
281710229
308.01
11.484669
-55.922574
8.30985
1360.88042
 
2
FFI
FFI
FFI-QLP
v-shaped;
281781375
204.01
12.975211
-59.343014
43.828624
1328.032557
 
1
tp.fits
lc.fits
|
Only two events; first event is on/near momentum dump.
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
281979481
274.01
130.504849
-75.801512
0.542248
1386.381414
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
needs follow-up to check if signal is on-target
289793076
108.01
316.961466
-26.096660
3.043839
1328.084864
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-13
290131778
123.01
319.699400
-26.616077
3.308754
1325.375658
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HD 202772
300293197
211.01
110.279641
-68.578384
6.563939
1329.255719
 
1
tp.fits
lc.fits
|
known TOI
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
300810086
385.01
116.814028
-69.030700
0.66797
1326.06183
 
1,2,3,4,5
FFI
FFI
FFI-QLP
maybe not on target
300871545
184.01
117.657590
-70.533607
4.817028
1327.376627
 
1
tp.fits
lc.fits
|
1000 ppm secondary; likely EB
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
305048087
237.01
353.242700
-29.415100
5.433729
1355.24981
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
low MES.
305048116
362.01
353.238144
-28.319746
7.11679
1357.85959
 
2
FFI
FFI
FFI-QLP
the super bright star to the southwest is TIC 304698788; does not have a signal.
307210830
175.01
124.531900
-68.313000
3.690613
1356.203764
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
307210830
175.02
124.531900
-68.313000
7.451113
1355.2864
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
307210830
175.03
124.531900
-68.313000
2.253014
1354.906208
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
308208458
345.01
5.696952
-34.392090
11.22917
1362.15706
 
2
FFI
FFI
FFI-QLP
possible odd even;
309257814
171.01
124.269511
-63.213478
1.23855
1326.40275
 
1,4
FFI
FFI
FFI-QLP
309792357
199.01
80.105474
-59.895662
NaN
1361.02496
 
1
tp.fits
lc.fits
|
known TOI; single transit; no period
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
314865962
208.01
53.281311
-72.744226
22.434498
1335.985928
 
1
tp.fits
lc.fits
|
Last transit is near a momentum dump so period/depth might be affected. The other two are fine.
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
316769613
314.01
354.668235
-32.860621
10.18242
1355.59503
 
2
FFI
FFI
FFI-QLP
none
316937670
221.01
356.490400
-56.344700
0.62425
1325.342966
 
1
tp.fits
lc.fits
|
M dwarf; low MES USP.
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
321982642
358.01
3.060934
-47.355409
9.105
1356.32633
 
2
FFI
FFI
FFI-QLP
odd/even not reliable
322063810
253.01
14.317859
-51.584652
3.515816
1355.612876
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
There is another star in the same pixel. Centroid offset is not significant.
322307342
117.01
15.005896
-58.904780
3.5855
1328.4809
 
1,2
FFI
FFI
FFI-QLP
HATS-68
325680697
414.01
36.853348
-12.038913
1.82487
1411.51868
 
4
FFI
FFI
FFI-QLP
three stars in central pixel; possible EB
326453034
223.01
339.677665
-25.631723
14.445918
1355.95751
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Low significance; not enough information from centroid plot to determine if object is on target. Gaia indicates R*=2.7. Transit duration seems short for a giant. Period is similar to the spacecraft period but transit events are not near known scattered light events so they could be real.
327952677
295.01
359.091748
-13.271651
3.39656
1356.40432
 
2
FFI
FFI
FFI-QLP
none
328350926
392.01
46.931654
+0.861311
0.84907
1411.599
 
4
FFI
FFI
FFI-QLP
same pixel as 328350925 and 328350924
336732616
103.01
312.457438
-24.428796
3.547854
1327.25256
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-3
339733013
417.01
110.852026
-58.696747
5.62145
1328.3763
 
1,2,3,4,5
FFI
FFI
FFI-QLP
may be on 339733023
348770361
161.01
46.686080
-82.316422
2.76898
1325.70292
 
1
FFI
FFI
FFI-QLP
Unknown stellar (and candidate) radius. Possible small centroid shift to NW.
349518800
407.01
111.211769
-62.092491
2.16555
1326.66101
 
1,3,4,5
FFI
FFI
FFI-QLP
possible EB; check 349518801 with photometric follow-up
350445771
258.01
85.467440
-56.740516
3.190394
1326.800815
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
possible secondary
1-3
dvs.pdf | dvr.pdf
350618622
201.01
87.401712
-54.910734
NaN
1376.05
 
1
tp.fits
lc.fits
|
Single transit (no period)
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
350743714
165.01
88.885933
-57.290593
7.76178
1388.296648
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
known brown dwarf; discovered by WASP; one of transits is in gap
355509914
202.01
15.524836
-59.087778
1.738316
1326.115925
 
1
tp.fits
lc.fits
|
The OOT centroid is wrong; The signal is on target.
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
355636844
146.01
358.301495
-56.013040
6.29632
1330.55618
 
1,2
FFI
FFI
FFI-QLP
Signal coming from a faint star to the SE. At least for the brighter of those it could be a planet.
355637190
293.01
358.154472
-54.468865
0.80546
1326.22108
 
1,2
FFI
FFI
FFI-QLP
V-shaped;
355703913
111.01
0.774485
-62.469342
2.106098
1326.106369
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
HATS-34
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
369336146
356.01
6.069980
-37.222073
5.77014
1358.03764
 
2
FFI
FFI
FFI-QLP
none
369457671
168.01
311.643495
-37.904371
2.31257
1326.49996
 
1
FFI
FFI
FFI-QLP
373844472
275.01
81.516837
-67.233034
0.919476
1326.061419
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
v-shaped; likely EB
1-3
dvs.pdf | dvr.pdf
382188882
276.01
81.352974
-55.019917
4.800523
1387.759868
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
likely EB
382302241
151.01
83.348955
-58.745231
1.59783
1326.04926
 
1,2,3,4
FFI
FFI
FFI-QLP
Large with possible synchronization
382391899
391.01
43.688073
-10.898080
1.95512
1411.0936
 
4
FFI
FFI
FFI-QLP
WASP-50
382463648
296.01
353.104835
-45.909528
12.62733
1355.52978
 
2
FFI
FFI
FFI-QLP
The period could be either 12.635 or 25.27
382474101
349.01
12.274293
-52.046527
2.65221
1354.56049
 
2
FFI
FFI
FFI-QLP
400 ppm secondary; synchronized
382626661
283.01
118.569575
-65.441521
17.61744
1333.47461
 
1
tp.fits
lc.fits
|
two stars in center pixel
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
|
1-3
dvs.pdf | dvr.pdf
388104525
112.01
55.933440
-65.193856
2.499802
1327.409511
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-119
2
tp.fits
lc.fits
|
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
389525208
154.01
313.261485
-38.594870
6.74709
1329.35996
 
1
FFI
FFI
FFI-QLP
389753172
319.01
351.290954
-47.945505
0.71356
1325.89923
 
1,2
FFI
FFI
FFI-QLP
There is a potential odd even;
391949880
128.01
79.522476
-80.964663
4.940663
1328.129344
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
"There is a nearby (2"") comoving dMag~2.5 star. If the signal originates from either the target star or nearby star it could still be a small planet."
393940766
148.01
338.320677
-38.159717
4.8661
1327.33133
 
1
FFI
FFI
FFI-QLP
Planet candidate around 393940766 to the NW.
394137592
120.01
4.446408
-66.358985
11.535076
1332.082805
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
394657039
159.01
51.781947
-78.549812
3.76276
1328.63687
 
1,2
FFI
FFI
FFI-QLP
394698182
170.01
54.988393
-83.088557
3.7118
1325.51317
 
1
FFI
FFI
FFI-QLP
402026209
232.01
353.562839
-42.061409
1.338231
1355.184519
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
WASP-4
402319411
317.01
353.539987
-14.859942
3.3262
1355.09217
 
2
FFI
FFI
FFI-QLP
none
403136413
158.01
333.578639
-55.379022
2.51266
1326.37811
 
1
FFI
FFI
FFI-QLP
403224672
141.01
338.984609
-59.864489
1.007908
1325.538528
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
403287048
152.01
332.357821
-62.333998
7.00776
1327.92337
 
1
FFI
FFI
FFI-QLP
410153553
136.01
340.492100
-69.169000
0.46291
1325.72603
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
LHS 3844
410214986
200.01
354.914556
-69.195787
8.1375
1332.309957
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
The transit was detected with a bunch of false signals due to detrending; But the two transits near epoch 1332.3098 and 1340.4473 looks reasonable;
415969574
342.01
342.170291
-18.520457
10.45776
1362.57199
 
2
FFI
FFI
FFI-QLP
two transits; no gaia radius
415969908
233.01
343.710000
-18.911800
11.665865
1365.263091
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
422655579
388.01
29.263334
+0.758835
2.90326
1413.14271
 
4
FFI
FFI
FFI-QLP
WASP-71
425934411
142.01
4.605790
-62.847886
0.853319
1325.489793
 
1
tp.fits
lc.fits
dvs.pdf | dvr.pdf
Gaia stellar radii 0.69 Rsun.
2
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
425997655
174.01
55.459877
-62.767049
17.668189
1342.994583
 
1
tp.fits
lc.fits
|
known TOI; follow-up in progress
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
425997655
174.02
55.459877
-62.767049
29.797713
1340.303729
 
1
tp.fits
lc.fits
|
known TOI; followup in progress
2
tp.fits
lc.fits
| dvr.pdf
3
tp.fits
lc.fits
|
1-2
dvs.pdf | dvr.pdf
1-3
dvs.pdf | dvr.pdf
425997655
174.03
55.459877
-62.767049
12.166894
1335.733561
 
1
tp.fits
lc.fits
|
known TOI; marginal PC
2
tp.fits
lc.fits
| dvr.pdf
3
tp.fits
lc.fits
|
1-2
| dvr.pdf
1-3
dvs.pdf | dvr.pdf
425997655
174.04
55.459877
-62.767049
3.976337
1326.029824
 
1
tp.fits
lc.fits
|
known TOI; marginal PC
2
tp.fits
lc.fits
| dvr.pdf
3
tp.fits
lc.fits
|
1-2
| dvr.pdf
1-3
dvs.pdf | dvr.pdf
434105231
311.01
354.335560
-13.455698
0.79632
1354.99864
 
2
FFI
FFI
FFI-QLP
maybe EB; V-shaped; some odd-even
439456714
277.01
19.077200
-20.952200
3.994244
1389.02917
 
3
tp.fits
lc.fits
dvs.pdf | dvr.pdf
check that 439456712 is not the target
441075486
372.01
359.759017
-15.612006
1.12026
1354.76663
 
2
FFI
FFI
FFI-QLP
likely EB; V-shaped;
441462736
197.01
353.033649
-21.801397
14.279001
1357.013115
 
2
tp.fits
lc.fits
dvs.pdf | dvr.pdf
evolved star
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