ALCDEF Home

ALCDEF Defined Constant Keywords

NameValues
{CCNI-ATLAS-1}J. L. Tonry
[tonry@hawaii.edu] Institute for Astronomy, Univ. Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822
{CCNI-KLINGLESMITH-1}D. A. Klinglesmith
[dklinglesmith@mro.nmt.edu] 1215 Vista Dr., Socorro, NM 87801
{CCNI-PILCHER-1}F. Pilcher
[fpilcher35@gmail.com] 4438 Organ Mesa Loop, Las Cruces, NM 88011 USA
{CCNI-STEPHENS-1}Robert D. Stephens
[rstephens@foxandstephens.com] 11355 Mount Johnson Court, Rancho Cucamonga, CA 91737
{CCNI-WARNER-1}Brian D. Warner
[brian@MinorPlanetObserver.com] 446 Sycamore Ave., Eaton, CO, USA
{CCOM-ATLAS-1}OBSERVERS is list of coauthors for Tonry et al. (2018a)
OBJECTRA/DEC, PAB, and Phase computed from average of converted MJD
The original ATLAS data were light-time corrected MJD.
The MJD were converted to JD with JD = MJD + 2400000.5 + LTCDays
The original light-time correction was POINT. The value given here is
based on SESSIONDATE/SESSIONTIME and internal calculations.
LTCDays used a single iteration of DeltaT = 0.0057755 * Earth Distance
The magnitudes are Johnson V converted from the native FILTER.
See Tonry et al. (2018b) Ap. J. 867, A105 (ATLAS Reference Catalog)
{CCOM-DATETIME-1}The original SessionDate/Time were adjusted to match the average JD of the lightcurve data
{CCOM-EQUIP-1}Telescope and Detector are those most likely used.
The actual telescope was 0.25-0.35 SCT or 0.5-m R-C.
The actual detector was likely a KAF-E CCD chip in FLI/SBIG camera.
{CCOM-ERASMUS-1}Photometry done by N. Erasmus using The Photometry Pipeline (PP) developed by M. Mommert
Some magnitudes were converted to V from R and I, see PUBLICATION for colors
Original RA/Dec PAB/Phase values overwritten during data verification using SessionDate/Time and ObjectNumber/Name
{CCOM-MOLNAR-1}Observations from Kepler spacecraft
Continuous observations for up to 2+ days for each obejct
SESSIONDATE/TIME are for mid-observing run
Magnitudes are USNO R
Original data were BJD; Assumed to be HJD then corrected to JD
Corrections based on orbital elements as of 2017-09-30
Maximum JD error ~12 seconds: raw data to 0.0001 d (8.64 s) + BJD-HJD
{CCOM-POSITIONS-1}The original RA/Dec PAB/Phase values were modified during data import/validation
using SessionDate/Time and ObjectNumber/Name.
{CCOM-SZABO-1}Observations from Kepler spacecraft
Continuous observations for up to 2+ days for each obejct
SESSIONDATE/TIME are for mid-observing run
Magnitudes are USNO R
Original data were BJD; Assumed to be HJD then corrected to JD
Corrections based on orbital elements as of 2017-09-12
Maximum JD error ~12 seconds: raw data to 0.0001 d (8.64 s) + BJD-HJD
{CCOMP-FIX-1}One or more of the following fixes were applied to one or more of the comp stars:
RA, Dec, MagBand, and/or CIBand were missing and set to the object's values.
No magnitude; set to 0.000 to avoid empty value.
{CDET-ATLAS-1}Semiconductor Technology Associates STA-1600 10560x10560x9-micron
{CFAC-STEPHENS-1}Center for Solar System Studies - Trojan Station (Landers, CA)
{CFAC-STEPHENS-2}Goat Mountain Astronomical Research Station (GMARS; Landers, CA)
{CFAC-WARNER-1}Center for Solar System Studies - Palmer Divide Station (Landers, CA)
{CFAC-WARNER-2}Palmer Divide Observatory, Colorado Springs, CO
{COBS-ATLAS-1}Tonry, J.L.; Denneau, L.; Heinze, A.N.; Stalder, B.; Smith, K.W.;
Smartt, S.J.; Stubbs, C.W.; Weiland, H.J.; Rest, A.
{CPUB-ATLAS-1}Tonry et al. (2018a) Pub. Ast. Soc. of the Pacific 130, pp 064505
{CTEL-ATLAS-1}0.5-m f/2 DFM Wright Schmidt