571-025584 VSX match with Delta Cepheid V0371 Gem. K0 spectral class.
573-025534 Possibly multi-periodic
572-024259 Object is spinning too quickly to be a rotator. Likely a giant pulsating star experiencing short-lived multi-mode p-mode oscillations, and perhaps Mira-like variability
572-024468 Rapid rotational or ellipsoidal variable
571-024998 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
572-024629 PDM1
571-024302 We report a period that is half that of the PISCES analysis, however, this is in agreement with both the Libralato and Nardiello results.
572-024283 PDM1
573-024756 Possibly multi-periodic
571-024411 May be multi-periodic. Likely a giant pulsating star experiencing short-lived multi-mode p-mode oscillations, and perhaps Mira-like variability
573-025434 LS2
570-024572 LS2
572-025394 Reddened background hot dwarf star. May be misclassified depending on reddening.
572-025131 PDM1
572-024517 Possibly multi-periodic
572-024803 PDM1
572-025307 Rotational or ellipsoidal variable. Our period is twice the period of the Libralato result.
573-025064 PDM1
572-025114 PDM4
572-024449 PDM1
571-025221 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
573-025414 PDM1
572-024558 Selected period is in good agreement with Libralato, but is half that of Nardiello.
573-024986 Period is slightly less than Meibom analysis, but is in agreement with Libralato result.
572-025244 Gaia-derived luminosity and temperature indicate that this may be a delta scuti variable in M35
573-025238 LS Period 2. Reddened background hot dwarf star. SPB or Gamma Dor (if a reddened A-star).
573-024815 PDM1
571-025101 Likely a rotational variable
571-024404 PDM2
571-024416 We report a period that is half that of the PISCES analysis, however, this is in agreement with the Nardiello result.
571-024847 G star. PM from Gaia DR2 rules out cluster membership
573-024914 This field source is very low in luminosity log(L)=-0.5
572-024790 PDM4
571-025477 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
572-025268 Possibly multi-periodic
571-024817 Our period assignment agrees well with Nardiello, but is half that of Libralato.
573-025412 We report a period that is twice that of Libralato, which agrees well with Meibom.
571-024682 Astroseismology target. Oscillating giant star. Ambiguous blend.
572-025073 PDM1. Common two maxima per cycle spot modulation signal.
573-024729 PDM4. Period chosen after looking at the period-mass relation. Period is twice that of Libralato result, but is in agreement with Meibom.
573-025060 PDM1.
572-024593 PDM1
572-024950 Either rotational or ellipsoidal variable.
573-025446 PDM1
574-024533 Gaia match with 3426303911211046528. Distance indicates it is a RG star.
573-025488 Possibly multi-periodic
571-025553 Rotational Variable with BLS2
573-025452 Marginal signal.
572-024728 Possibly multi-periodic
573-025483 PDM1
572-024900 LS2
573-025241 Rapid rotational or ellipsoidal variable. Likely rotational variable, but could be RR Lyrae (if distant HB star), or contact binary (minima/maxima seem too sharp for that).
572-024969 Rapid rotational or ellipsoidal variable
571-024640 Rapid rotational or ellipsoidal variable. Thickness of phase-folded LC suggests multi-periodic pulsator.
571-025443 PDM1
571-025108 PDM2
571-025327 Rotational Variable. Likely FK Comae Berenices-type.
571-024225 Possibly multi-periodic
571-025203 Likely rotational variable, but depends on where star falls in HR diagram (could also be gamma dor or Type II cepheid, i.e. BL Her in this case given P)
571-025170 Rapid rotational or ellipsoidal variable. We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
573-024853 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
572-024445 Period is half that of the Meibom analysis, but is in agreement with Libralato result.
572-025117 PDM1
571-025060 Rapid rotational or ellipsoidal variable
571-025301 PDM3
572-024762 Rapid rotational or ellipsoidal variable
571-025148 Rapid rotational or ellipsoidal variable. Thickness of phase-folded LC suggests multi-periodic pulsator.
571-025486 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
573-024871 PDM1
572-025162 Rapid rotational or ellipsoidal variable
572-025180 Our period assignment agrees well with Nardiello, but is half that of Libralato.
573-025519 Rapid rotational or ellipsoidal variable
571-025281 Rapid rotational or ellipsoidal variable
572-024692 PDM1. Period is double that of the Meibom analysis, but is in agreement with Libralato result.
573-025518 Rapid rotational or ellipsoidal variable. We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
572-025169 PDM1
573-025589 PDM3. Period chosen after looking at the period-mass relation. Period is twice that of Libralato result, but is in agreement with Meibom.
573-025590 LS1 or PDM1
572-024990 PDM1. Rotational variable K dwarf. We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
572-024206 Rapid rotational or ellipsoidal variable
571-025690 Rotational or ellipsoidal variable.
573-024894 PDM1
573-025035 LS2
571-025063 Rotational or ellipsoidal variable.
571-024874 PDM4 is in agreement with periodicity derived by both Libralato and Meibom.
571-024625 We report a period that is half that of the PISCES analysis, however, this is in agreement with the Libralato result.
572-023825 VSX match with HN Gem -- No period listed in VSX for this source
572-024427 Period agrees with Libralato and Nardiello, but is in disagreement with Meibom.
571-024932 PDM1
573-025240 LS2. Rapid rotational or ellipsoidal variable. Thickness of phase-folded LC suggests multi-periodic pulsator.
573-024983 Rapid rotational or ellipsoidal variable.
571-024734 Period is slightly less than Meibom analysis, but is in agreement with Libralato result.
572-024814 We report a period that is twice that of Libralato, but agrees with Nardiello.
571-025692 PDM1
571-025540 PDM1
573-025250 Rapid rotational or ellipsoidal variable
571-025158 PDM1
571-024652 We report a period that is half that of the PISCES analysis, however, this is in agreement with the Libralato result.
572-025011 Marginal signal. Ambiguous whether period is from GLS1 or BLS1.
572-025000 Reddened background hot dwarf star. Could be an SPB (GLS1) or an ellipsoidal variable (PDM3).
573-024695 Rapid rotational or ellipsoidal variable
571-024216 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the PISCES result.
572-025314 Possibly multi-periodic
572-024876 Either LS1 or BLS2
571-024426 PDM3 is in agreement with PISCES analysis.
572-025192 LS2
573-024854 BLS1
573-025549 PDM1. Period chosen after looking at the period-mass relation. Period is twice that of Libralato result, but is in agreement with Meibom and Nardiello.
572-024976 We report a period that is twice that of Libralato, which agrees with Nardiello and Meibom./Users/msoares/Dropbox/K20/Data_Files/FullComments.txt
571-025680 Rapid rotational or ellipsoidal variable
573-025500 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
571-024857 PDM1
572-024939 Either rotational or ellipsoidal variable.
572-024785 PDM1
571-024848 PDM1
571-024855 Rapid rotational or ellipsoidal variable
572-024359 LS2
571-024914 PDM1
571-024433 EB with BLS2. Inferred stellar density too low (0.047 gm/cm^3) for this to be a planet system in NGC 2158 given Rp/R* ~ 0.1. Period is twice that of Libralato but agrees with Nardiello.
571-024320 EB with OOT ellipsoidal variability. Wiggles imply spot modulation.
571-025426 Semi-detached EB with BLS2. Meibom, Nardiello, and Libralato measured half this period, but we see the secondary quite nicely with the period reported.
571-024873 Strong OOTV. Likely EB with BLS3. Our period is twice that of the period derived by Nardiello and Libralato.
572-024695 EB with OOTV. Both Libralato and Meibom report P=1.35 days, however, we upon close inspection of our LC we observe a secondary eclipse at P=2.7 days -- this agrees with Nardiello derived period.
571-024971 Gaia DR2 parallax rules out M35 membership.
571-025495 Either EB or ellipsoidal variable with BLS2. Gaia DR2 parallax rules out M35 membership. Both Libralato and Meibom report P=0.158 days, however, we upon close inspection of our LC we deem P=0.316 days, which agrees with Nardiello.
571-024330 Likely EB with BLS3.
571-024688 Possible OOTV. BLS2 is in agreement with PISCES.
571-024709 PDM2. Contact Eclipsing Binary (W Uma). Both Libralato and Meibom report P=0.18 days, however, we upon close inspection of our LC we deem P=0.36 days.
571-024827 EB with BLS 3.
571-025548 EB with ellipsoidal variation. Strong OOTV.
572-024507 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
572-025069 EB with ellipsoidal variation.
572-024307 EB with BLS2
570-025055 526 cadences for this TPF source far from super stamp center. 0.246 d signal arises from thruster firing. Gaia parallax indicates distance of 597 to 722 pc. Unlikely cluster member. Gmag=14.75
573-025574 EB with BLS2. Agrees with period of Nardiello, but is twice that of Libralato.
571-024279 EB with BLS2
570-024652 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
573-025333 Possibly an EB with BLS2?
573-025613 Detached EB with BLS2
571-024604 Single eclipsing EB with OOT ellipsoidal variability.We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
571-025474 Eccentric EB. Curious apparent dip between primary and secondary eclipse. Eccentricity is high for such short period.
571-024645 Density points to early K dwarf or late G dwarf. Some evidence that it may be a blended EB.
570-024492 Eccentric EB. 534 cadences for this TPF source far from super stamp center. 0.246 d signal arises from thruster firing
571-024950 Period is larger than Meibom analysis, but is in agreement with Libralato result.
571-025549 Thickness of phase-folded LC suggests multi-periodic pulsator. If you fit and subtracted sine curve at domi   t P, and then ran another periodogram, you'd probably see another significant, unrelated P show up. Discrete Fourier transform could show full forest of modes in this light curve. PDM for multi-periodic pulsator is hard to interpret. It may also be that TFA filtering is distorting LC of this high amplitude variable.
571-025061 Possibly multi-periodic
572-024470 PDM1
572-024796 PDM1
572-024398 Possible VSX match with DScuti V0392
573-025379 Shallow transit around a K-dwarf. Promising transit. Transit density and photometry suggest a ~0.76 M_sun star located at 560 pc distance, and the planet radius would be ~3.4 R_earth, or just a mini-Neptune. Was placed in Keck follow-up proposal. Gaia parallax suggests 690-740 pc in distance. Gmag=15.6. Gaia match 3426297073623137024.
570-024339 Gaia DR2 indicates that this is a GDor star of spectral class F. Gaia ID 3426162791474814848.
572-024591 PDM1
573-025110 LS2
571-024767 May be multi-periodic
570-024366 May be multi-periodic
571-024819 We report a period that is half that of Libralato, but agrees with Nardiello.
573-025427 Eccentric EB
571-024775 EB with BLS2.
573-024845 Blend with HAT-264-0152329. EB with large OOTV.
573-024844 Blend with HAT-264-0070077. EB given the 0.06 mag deep transits and J-K = 0.397. Large ellipsoidal out of eclipse variation.
571-024524 May show combined variability of two stars
572-025138 Eccentric EB
571-024365 EB with secondary seen at P=3.77 days. Our period is twice the period derived by Libralato.
571-024353 EB with BLS2
571-024774 EB with BLS2
571-024838 LS2
573-024971 Possibly multi-periodic
573-024948 Our period assignment agrees well with Meibom, but is half that of Libralato.
571-025496 Gaia match with 3425509892015303040 (Gmag=14.9). Parallax and parallax error indicate d~6 pc and T~6800 K. F type star. We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
571-024521 Possibly multi-periodic
571-025371 LS2
571-024851 LS1. Agrees well with Libralato results, but not Meibom.
571-024670 We report a period that is half that of the PISCES analysis, however, this is in agreement with the Libralato result.
572-024743 In Gaia DR2 as 3426270754063847552. Teff suggests class A star. Proper motion rules out cluster membership.
571-024945 Possibly multi-periodic
572-024471 LS1 or PDM1
570-025184 Possibly multi-periodic
571-024788 Likely rotational variable, due to asymmetry. Possibly multi-periodic.
571-024892 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
571-024617 We report a period that is half that of the PISCES analysis, however, this is in agreement with the Libralato result.
572-024298 We report a period that is half that of the Nardiello analysis, however, this is in rough agreement with the Libralato and PISCES result.
570-024772 VSX match with DScuti+GDor Blend HD 252154
572-024596 LS1 or PDM2. Suggestive spot evolution or multi-periodic variation.
571-024231 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
570-024167 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
571-024532 PDM1
572-024479 May be hybrid DScuti + gamma dor pulsator (A or early F MS star at red edge of the instability strip which simultaneously has p mode oscillations (P~0.04 day signal, though may be sampling alias of 1.6 day signal) and g-mode oscillations (p > 1 day signals). Alternatively, 1.6 day signal might be low frequency sampling alias of some high frequency DScuti oscillation, or this could be some rotation signal.
572-024898 We report a period that is half that of the Nardiello analysis, however, this is in agreement with the Libralato result.
571-024985 May be some ellipsoidal variation in PDM1 (less in BLS1). May be EB. 0.3 from NGC 2158 cluster center. Gaia source 3426255086023032576. Unreliable parallax (large error). Distance is > 3.7 kpc. Gmag=15.6.
571-025326 LS1 or PDM1. Catalog photometry should not be trusted. Likely a giant pulsating star experiencing short-lived multi-mode p-mode oscillations, and perhaps Mira-like variability
573-025354 May be multi-periodic. Rapid rotational or ellipsoidal variable. Thickness of phase-folded LC suggests multi-periodic pulsator. Likely a giant pulsating star experiencing short-lived multi-mode p-mode oscillations, and perhaps Mira-like variability
572-025230 Could be a very rapidly rotating star (near break-up rotation rate for sun-like star), an ellipsoidal variable with 2x the measured period, or some other type of rapidly oscillating star. With reddening, appears to be an A star.
572-024315 Possibly multi-periodic
572-024928 PDM2
573-025547 May be multi-periodic
571-024397 May be multi-periodic
571-024450 LS2
570-024363 May be multi-periodic
572-024875 Likely rotational variable, due to asymmetry. Possibly multi-periodic.
573-024728 Period is half that of the Meibom analysis, but is in agreement with Libralato result.
571-025180 Our period of 0.0676 days is in agreement with Libralato, but is much lower than the Meibom result of 0.382 days.