- Timestamp:
- Nov 26, 2012, 11:47:14 AM (14 years ago)
- Location:
- trunk/ppTranslate/documentation/ICD
- Files:
-
- 7 added
- 1 edited
-
PSDC-940-005.tex (modified) (12 diffs)
-
figures/basics.xfig (added)
-
figures/exposure_ota.eps (added)
-
figures/exposure_ota.fig (added)
-
figures/ext_theta.eps (added)
-
figures/ext_theta.fig (added)
-
figures/ipp_workflow.eps (added)
-
figures/ipp_workflow.fig (added)
Legend:
- Unmodified
- Added
- Removed
-
trunk/ppTranslate/documentation/ICD/PSDC-940-005.tex
r34509 r34695 2 2 \documentclass[panstarrs,spec]{panstarrs} 3 3 \usepackage{nonfloat} 4 5 \newcommand{\sccomment}[1]{% 6 \textcolor{green}{SC: #1}} 4 \usepackage{caption} 5 7 6 \newcommand{\outformatversion}{% 8 7 \texttt{PS1\_DV3}} … … 12 11 \subtitle{Pan-STARRS IPP-MOPS ICD for PS-1} 13 12 \shorttitle{IPP-MOPS ICD} 14 \author{ Eugene Magnier, Larry Denneau, Jr., Robert Jedicke}13 \author{\parbox{3in}{Serge Chastel; Larry Denneau, Jr.; Denver Green; Robert Jedicke; Eugene Magnier}} 15 14 \audience{Pan-STARRS PMO} 16 15 \group{Pan-STARRS IPP \& MOPS} … … 26 25 \RevisionsStart 27 26 % version Date Description 28 03 & 2012 Oct 04 & \texttt{PS1\_DV3}: Fitted trails, new parameters\\ 29 \hline 30 02 & 2011 Apr 19 & Synchronization with "ICD Lite" wiki page \\ 31 \hline 32 01 & 2010 Oct 27 & New CMF Parameters \\ 33 \hline 34 00 & 2006 Mar 01 & Initial version \\ \hline 27 04 & 2012 Nov 20 & Answers to DG comments/questions \\ 28 \hline 29 03 & 2012 Oct 04 & \texttt{PS1\_DV3}: Fitted trails, new parameters\\ 30 \hline 31 02 & 2011 Apr 19 & Synchronization with "ICD Lite" wiki page \\ 32 \hline 33 01 & 2010 Oct 27 & New CMF Parameters \\ 34 \hline 35 00 & 2006 Mar 01 & Initial version \\ \hline 35 36 \RevisionsEnd 36 37 … … 116 117 \DocumentsEnd 117 118 119 \subsection{Acronyms} 120 121 \begin{table} 122 \small 123 \caption{Acronyms used in this document\label{table-acronyms}} 124 \begin{tabular}{ll} 125 \hline 126 {\bf Acronym} & {\bf Definition} \\ 127 \hline 128 ADU & Analog to Digital Units (counts in an image) \\ 129 ICRS & International Celestial Reference System \\ 130 IPP & Pan-STARRS Image Processing Pipeline \\ 131 FPA & Focal Plane Array \\ 132 MOPS & Pan-STARRS Moving Object Processing System \\ 133 MPC & Center for Astrophysics Minor Planet Center \\ 134 TTI & Transient-Time Interval (about 60 minutes) \\ 135 \hline 136 \end{tabular} 137 \end{table} 138 118 139 \section{Interface Overview} 119 140 … … 144 165 145 166 This document discusses the software interface between IPP and MOPS. 146 IPP must send transient detection descriptions to the MOPS; MOPS 147 must be able to query the IPP regarding whether a particular (RA, 148 Dec) pair could have been detected in a particular focal plane array (FPA). This document 149 defines the data to be transferred between IPP and MOPS and the 150 mechanisms to be used for that interchange. These interfaces are 151 identified as \#005 in Figure~\ref{fig:overview}. The Interfaces167 IPP must send transient detection descriptions to the MOPS; MOPS must 168 be able to query the IPP regarding whether a particular (RA, Dec) pair 169 could have been detected in a particular focal plane array (FPA). 170 This document defines the data to be transferred between IPP and MOPS 171 and the mechanisms to be used for that interchange. These interfaces 172 are identified as \#005 in Figure~\ref{fig:overview}. The Interfaces 152 173 addressed by this document are marked in the table. 153 174 … … 235 256 Though efforts have been made to avoid this from occurring, where 236 257 header keyword names are longer than the usual 8 character maximum, 237 the HIERARCH convention will be used. 258 the HIERARCH convention will be used (see the NASA webpages: 259 \htmladdnormallink{Registered FITS 260 Convention}{http://fits.gsfc.nasa.gov/registry/hierarch_keyword.html} 261 and \htmladdnormallink{4.12.4 HIERARCH Convention for Extended Keyword 262 Names}{http://heasarc.nasa.gov/docs/software/fitsio/c/f_user/node28.html}). 238 263 239 264 \subsection{IPP-MOPS Exchange} … … 241 266 MOPS requires from the IPP a stream of transient detections and their 242 267 FPA metadata obtained from processing of difference images acquired by 243 the PS-1 camera. IPP is additionally required by MOPS to be able to 244 indicate whether a set of detections (with RA, Dec, flux, length, 245 orientation, etc.) on a previously acquired FPA was detectable by the 246 PS-1 telescope. 268 the PS-1 camera. 269 270 IPP is additionally required by MOPS to be able to indicate whether a 271 set of detections (with RA, Dec, flux, length, orientation, etc.) on a 272 previously acquired FPA was detectable by the PS-1 telescope. This 273 functionality is provided through the detectability server. 247 274 248 275 \subsubsection{Conventions} … … 305 332 306 333 \begin{itemize} 307 \item{EXTNAME} - Giving a unique name for the metadata table. Such a 308 name shall contain only the characters a-z, and ``\_''. 309 \item{CMFVERSION} - A string specifying the version of the table 310 description file for this table. 334 \item{EXTNAME} - A \emph{string} giving a unique name for the metadata 335 table. Such a name shall contain only the characters a-z, A-Z, and 336 ``\_''. 337 \item{CMFVERSION} - A \emph{string} specifying the version of the 338 table description file for this table. 311 339 \end{itemize} 312 340 … … 389 417 exposure. 390 418 391 In addition to the required BINTABLE extension header keywords392 described above, the FITS header shall include the keywords shown in393 table \ref{trans-keywords}. The subsequent FITS table, with EXTNAME394 of \code{MOPS_TRANSIENT_DETECTIONS}, shall include columns whose395 definitions are listed in table \ref{trans-table}.396 397 419 {\centering% 398 \tabcaption{IPP-MOPS Transient Detection Keywords\label{trans-keywords}} 399 \begin{longtable}{|lcp{0.5in}p{3in}|} 400 \hline \hline {\bf FITS Keyword} 401 & \parbox{0.5in}{\textbf{Version}} 402 & {\bf Precision} & {\bf Description}\\ 403 \hline \hline 404 \multicolumn{4}{|l|}{\null\hspace{10mm}\textbf{Version Information}}\\ 405 \hline 406 SWSOURCE & 1+ & string & source of software (e.g., "60eb6cdc-a59c-4636-a4e0-dba66a9721fd")\\ 407 \hline 408 SWVERSN & 1+ & string & version of software (e.g., "trunk/ppMops@24658")\\ 409 \hline 410 HIERARCH\_CMFVERSION & 2+ & char(7) & PS1\_DV1 or PS1\_DV2 or PS1\_DV3 \\ 411 \hline 412 \multicolumn{4}{|l|}{\null\hspace{10mm}\textbf{Provenance Information}}\\ 413 \hline 414 EXP\_NAME & 1+ & string & Exposure name (e.g., "o1234g5678")\\ 415 \hline 416 EXP\_ID & 1+ & S64 & Exposure identifier \\ 417 \hline 418 CHIP\_ID & 1+ & S64 & Chip stage identifier \\ 419 \hline 420 CAM\_ID & 1+ & S64 & Camera stage identifier \\ 421 \hline 422 FAKE\_ID & 1+ & S64 & Fake stage identifier \\ 423 \hline 424 WARP\_ID & 1+ & S64 & Warp stage identifier \\ 425 \hline 426 DIFF\_ID & 1+ & S64 & Diff stage \\ 427 \hline 428 DIFF\_POS & 1+ & boolean & Sense of subtraction; T for forward, F for backward\\ 429 \hline 430 \multicolumn{4}{|l|}{\null\hspace{10mm}\textbf{Exposure Details}}\\ 431 \hline MJD-OBS & 0+ 432 & F64 & midpoint time of the exposure as a MJD and day fraction \\ 433 \hline 434 RA & 0+ 435 & {\tiny HH:MM:SS.SSS} & field center RA at exposure midpoint, string \\ 436 \hline 437 DEC & 0+ & 438 {\tiny sDD:MM:SS}& (s is + or -) field center declination at exposure midpoint, string \\ 439 \hline 440 EXPTIME & 0+ 441 & F64 & exposure time in seconds \\ 442 \hline 443 ROTANGLE & 0+ 444 & F64 & image rotation of the y-axis in degrees, from local N toward E \\ 445 \hline 446 FILTER & 0+ & char(3) & effective filter used for the exposure, 447 one of g, r, i, z, y, B, V, w 448 appended with '.00000'\\ 449 \hline 450 AIRMASS & 0+ & F64 451 & airmass at exposure midpoint \\ 452 \hline 453 OBSCODE & 0+ & char(5) & MPC three-character observatory code \\ 454 \hline 455 TEL\_ALT & 0+ & F64 & telescope altitude at exposure midpoint, in degrees \\ 456 \hline 457 TEL\_AZ & 0+ & F64 & telescope azimuth at exposure midpoint, in degrees \\ 458 \hline 459 SEEING & 1+ & F32 & Measured seeing at diff stage, arcsec \\ 460 \hline 461 MAGZP & 1+ & F32 & Magnitude zero point \\ 462 \hline 463 MAGZPERR & 1+ & F32 & Error in magnitude zero point \\ 464 \hline 465 ASTRORMS & 1+ & F32 & RMS of astrometric fit, arcsec \\ 466 \hline 467 COMMENT & 3+ & String & Comment associated to the exposure\\ 468 \hline 469 OBS\_MODE & 3+ & String & Observation mode (e.g. MD, 3PI...)\\ 470 \hline 471 DIFFTYPE & 3+ & String & Difference type: WW (Warp-Warp Difference), WS (Warp-Stack Difference)\\ 472 \hline 473 SKY & 3+ & F64 & Exposure average sky background \\ 474 \hline 475 SHUTOUTC & 3+ & String & Camera exposure shutter open (UTC) \\ 476 \hline 420 \tabcaption{IPP-MOPS Data Types Definition\label{table-datatypes}} 421 \begin{longtable}{|cp{5in}|} 422 \hline 423 \textbf{Alias} & \textbf{Description} \\ 424 \texttt{bool} & (Not a FITS type) An enumerated type defining a Boolean 425 value, either \texttt{true} or \texttt{false}\\ 426 \texttt{char($n$)} & (Not a FITS type) A sequence of exactly $n$ bytes that 427 can be interpreted 428 as a sequence of ASCII characters\\ 429 \texttt{HH:MM:SS.sss} & (Not a FITS type) a \texttt{char(12)} encoding 430 a time or an angle: (1) the hours \texttt{HH} are encoded with two 431 decimal figures; (2) a separator \texttt{:} between the hours and 432 the minutes; (3) the minutes \texttt{MM} are encoded with two 433 decimal figures; (4) a separator \texttt{:} between the minutes 434 and the seconds; (5) the seconds \texttt{SS} are encoded with two 435 decimal figures; (6) a separator \texttt{.} between the seconds 436 and the milli(arc)seconds; (7) 437 the milli(arc)seconds \texttt{ss} are encoded with three decimal figures; \\ 438 \texttt{sDD:MM:SS} & (Not a FITS type) a \texttt{char(9)} encoding an 439 angle. (1) \texttt{s} is either the \texttt{+} or \texttt{-} sign; 440 (2) \texttt{DD} is the number of degrees encoded with two decimal 441 figures; (3) a separator \texttt{:} between the degrees and the 442 minutes; (4) the minutes \texttt{MM} are encoded with two decimal 443 figures; (5) a separator \texttt{:} between the minutes and the 444 seconds; (6) the 445 seconds \texttt{SS} are encoded with two decimal figures;\\ 446 \texttt{enum} & (Not a FITS type) a \texttt{string} having a fixed number of 447 different values. The explicit set of values shall be expressed in 448 this ICD.\\ 449 \texttt{F32} & (FITS type) IEEE 32-bit single precision floating point real numbers \\ 450 \texttt{F64} & (FITS type) IEEE 64-bit double precision floating point real numbers \\ 451 \texttt{S16} & (FITS type) 16-bit signed integer \\ 452 \texttt{S32} & (FITS type) 32-bit signed integer \\ 453 \texttt{S64} & (FITS type) 64-bit signed integer \\ 454 \texttt{string} & (Not a FITS type) Sequence of bytes of arbitrary length 455 usually interpreted as a sequence of ASCII characters \\ 456 \texttt{U16} & (FITS type) 16-bit unsigned integer \\ 457 \texttt{U32} & (FITS type) 32-bit unsigned integer \\ 477 458 \hline 478 459 \end{longtable} 479 460 } 480 461 481 {\centering 482 \tabcaption{IPP-MOPS Transient Detection Table Columns\label{trans-table}} 483 \begin{longtable}{|lclp{3.5in}|} 462 In addition to the required BINTABLE extension header keywords 463 described above (TODO: Where? What?), the FITS header shall include the 464 keywords shown in tables relative to versioning 465 \ref{table-keywords-versioning}, data provenance 466 \ref{table-keywords-provenance}, and exposure 467 \ref{table-keywords-exposure}. The subsequent FITS table, with EXTNAME 468 of \code{MOPS_TRANSIENT_DETECTIONS}, shall include columns whose 469 definitions are listed in table \ref{table-detections} and, when trail 470 fitting has been succesfully performed, \ref{table-detections-ext}. 471 472 \begin{center} 473 \begin{longtable}{|lcp{0.5in}p{3in}|} 474 \caption{IPP-MOPS Transient Detection Keywords:\\ Version Information}\label{table-keywords-versioning}\\ 475 \hline\hline 476 \multicolumn{4}{|l|}{\null\hspace*{1in}\textbf{Version Information}}\\ 477 \hline\hline 478 {\bf FITS Keyword} 479 & \parbox{0.5in}{\textbf{Version}} 480 & {\bf Precision} 481 & {\bf Description} \\ 482 \hline 483 SWSOURCE & 1+ & \texttt{string} & source of software (e.g., "60eb6cdc-a59c-4636-a4e0-dba66a9721fd") \\ 484 \hline 485 SWVERSN & 1+ & \texttt{string} & version of software (e.g., "trunk/ppMops@24658") \\ 486 \hline 487 HIERARCH CMFVERSION & 2+ & \texttt{enum} & \texttt{PS1\_DV3} \\ 488 \hline\hline 489 \end{longtable} 490 \end{center} 491 492 \begin{center} 493 \begin{longtable}{|lcp{0.5in}p{3in}|} 494 \caption{IPP-MOPS Transient Detection Keywords:\\ Provenance Information}\label{table-keywords-provenance}\\ 495 \hline\hline 496 \multicolumn{4}{|l|}{\null\hspace{10mm}\textbf{Provenance Information}}\\ 484 497 \hline \hline 485 {\bf Column} & \textbf{Version} & {\bf Precision} & {\bf Description} \\ 486 \hline 487 RA & 1+ & F64 & detection center coordinates in degrees\\ 488 \hline 489 RA\_ERR & 1+ & F64 & error in the detection center, in degrees \\ 490 \hline 491 DEC & 1+ & F64 & detection center coordinates in degrees \\ 492 \hline 493 DEC\_ERR & 1+ & F64 & error in the detection center, in degrees \\ 494 \hline 495 MAG & 1+ & F32 & Magnitude \\ 496 \hline 497 MAG\_ERR & 1+ & F32 & Magnitude error \\ 498 \hline 499 PSF\_CHI2 & 1+ & F32 & $\chi^2$ of PSF fit \\ 500 \hline 501 PSF\_DOF & 1+ & S32 & Degrees of freedom of PSF fit \\ 502 \hline 503 CR\_SIGNIFICANCE & 1+ & F32 & Significance of Cosmic Ray \\ 504 \hline 505 EXT\_SIGNIFICANCE & 1+ & F32 & Significance of extendedness \\ 506 \hline 507 PSF\_MAJOR & 1+ & F32 & PSF major axis (pixels) \\ 508 \hline 509 PSF\_MINOR & 1+ & F32 & PSF minor axis (pixels) \\ 510 \hline 511 PSF\_THETA & 1+ & F32 & PSF position angle (deg on chip) \\ 512 \hline 513 PSF\_QUALITY & 1+ & F32 & PSF quality factor \\ 514 \hline 515 PSF\_NPIX & 1+ & S32 & Number of pixels in PSF \\ 516 \hline 517 MOMENTS\_XX & 1+ & F32 & xx moment \\ 518 \hline 519 MOMENTS\_XY & 1+ & F32 & xy moment \\ 520 \hline 521 MOMENTS\_YY & 1+ & F32 & yy moment \\ 522 \hline 523 N\_POS & 1+ & S32 & Number of positive pixels \\ 524 \hline 525 F\_POS & 1+ & F32 & Fraction of positive pixels \\ 526 \hline 527 RATIO\_BAD & 1+ & F32 & Ratio of positive pixels to negative \\ 528 \hline 529 RATIO\_MASK & 1+ & F32 & Ratio of positive pixels to masked \\ 530 \hline 531 RATIO\_ALL & 1+ & F32 & Ratio of positive pixels to all \\ 532 \hline 533 FLAGS & 1+ & U32 & Detection bit flags\footnote{See \htmladdnormallink{http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/PSPSFlags\#StackDetectionFull.infoFlagsFLAGS232FLAGS}{http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/PSPSFlags\#StackDetectionFull.infoFlagsFLAGS232FLAGS} for the meaning of each bit}\\ 534 \hline 535 DIFF\_SKYFILE\_ID & 1+ & S64 & Identifier for diff skyfile. A 536 diff\_id (for Warp-Warp difference) or a stack\_id 537 (for Warp-Stack difference) \\ 538 \hline 539 IPP\_IDET & 2+ & U32 & IPP detection identifier index \\ 540 \hline 541 PSF\_INST\_FLUX & 2+ & F32 & PSF fit instrumental magnitude \\ 542 \hline 543 PSF\_INST\_FLUX\_SIG & 2+ & F32 & Sigma of PSF instrumental magnitude \\ 544 \hline 545 AP\_MAG & 2+ & F32 & magnitude in standard aperture \\ 546 \hline 547 AP\_MAG\_RAW & 2+ & F32 & magnitude in real aperture \\ 548 \hline 549 AP\_MAG\_RADIUS & 2+ & F32 & radius used for aperture mags \\ 550 \hline 551 AP\_FLUX & 2+ & F32 & instrumental flux in standard aperture \\ 552 \hline 553 AP\_FLUX\_SIG & 2+ & F32 & aperture flux error \\ 554 \hline 555 PEAK\_FLUX\_AS\_MAG & 2+ & F32 & Peak flux expressed as magnitude \\ 556 \hline 557 CAL\_PSF\_MAG & 2+ & F32 & PSF Magnitude using supplied calibration \\ 558 \hline 559 CAL\_PSF\_MAG\_SIG & 2+ & F32 & measured scatter of zero point calibration \\ 560 \hline 561 SKY & 2+ & F32 & Sky level \\ 562 \hline 563 SKY\_SIGMA & 2+ & F32 & Sigma of sky level \\ 564 \hline 565 PSF\_QF\_PERFECT & 2+ & F32 & PSF coverage/quality factor (poor) \\ 566 \hline 567 MOMENTS\_R1 & 2+ & F32 & first radial moment \\ 568 \hline 569 MOMENTS\_RH & 2+ & F32 & half radial moment \\ 570 \hline 571 KRON\_FLUX & 2+ & F32 & Kron Flux (in 2.5 R1) \\ 572 \hline 573 KRON\_FLUX\_ERR & 2+ & F32 & Kron Flux Error \\ 574 \hline 575 KRON\_FLUX\_INNER & 2+ & F32 & Kron Flux (in 1.0 R1) \\ 576 \hline 577 KRON\_FLUX\_OUTER & 2+ & F32 & Kron Flux (in 4.0 R1) \\ 578 \hline 579 DIFF\_R\_P & 2+ & F32 & distance to positive match source \\ 580 \hline 581 DIFF\_SN\_P & 2+ & F32 & signal-to-noise of pos match src \\ 582 \hline 583 DIFF\_R\_M & 2+ & F32 & distance to negative match source \\ 584 \hline 585 DIFF\_SN\_M & 2+ & F32 & signal-to-noise of neg match src \\ 498 {\bf FITS Keyword} 499 & \parbox{0.5in}{\textbf{Version}} 500 & {\bf Precision} 501 & {\bf Description} \\ 502 \hline 503 EXP\_NAME & 1+ & \texttt{string} & Exposure name (e.g., "o1234g5678")\\ 504 \hline 505 EXP\_ID & 1+ & \texttt{S64} & Exposure identifier \\ 506 \hline 507 CHIP\_ID & 1+ & \texttt{S64} & Chip stage identifier \\ 508 \hline 509 CAM\_ID & 1+ & \texttt{S64} & Camera stage identifier \\ 510 \hline 511 FAKE\_ID & 1+ & \texttt{S64} & Fake stage identifier \\ 512 \hline 513 WARP\_ID & 1+ & \texttt{S64} & Warp stage identifier \\ 514 \hline 515 DIFF\_ID & 1+ & \texttt{S64} & Diff stage \\ 516 \hline 517 DIFF\_POS & 1+ & \texttt{bool} & Sense of subtraction; \texttt{true} for forward, 518 \texttt{false} for backward\\ 519 \hline 520 \end{longtable} 521 \end{center} 522 523 \begin{center} 524 \begin{longtable}{|lcp{0.5in}p{3in}c|} 525 \caption{IPP-MOPS Transient Detection Keywords:\\ Exposure Details}\label{table-keywords-exposure}\\ 526 \hline \hline 527 \multicolumn{5}{|l|}{\null\hspace{10mm}\textbf{Exposure Details}}\\ 528 \hline \hline {\bf FITS Keyword} 529 & \parbox{0.5in}{\textbf{Version}} & {\bf Precision} & {\bf 530 Description} 531 & \textbf{Units}\\ 532 \hline MJD-OBS & 0+ & \texttt{F64} & midpoint time of the exposure 533 as a MJD and day fraction 534 & N/A\\ 535 \hline RA & 0+ & {\tiny \texttt{HH:MM:SS.SSS}} 536 & Field center RA at exposure midpoint & N/A \\ 537 \hline DEC & 0+ & {\tiny \texttt{sDD:MM:SS}} & 538 (s is + or -) Field center declination at exposure midpoint & N/A \\ 539 \hline EXPTIME & 0+ & \texttt{F64} 540 & Exposure time & seconds \\ 541 \hline ROTANGLE & 0+ & \texttt{F64} 542 & Image rotation of the y-axis from local N toward E & degrees \\ 543 \hline FILTER & 0+ & \texttt{char(7)} & Effective filter used for 544 the exposure, one of \texttt{g}, \texttt{r}, \texttt{i}, 545 \texttt{z}, \texttt{y}, \texttt{B}, 546 \texttt{V}, \texttt{w} appended with '.00000' & N/A \\ 547 \hline AIRMASS & 0+ & \texttt{F64} 548 & Airmass at exposure midpoint & N/A\\ 549 \hline OBSCODE & 0+ & char(5) & 550 MPC 3-character observatory code (F51 for PS1) & N/A \\ 551 \hline TEL\_ALT & 0+ & \texttt{F64} & 552 Telescope altitude at exposure midpoint & degrees \\ 553 \hline TEL\_AZ & 0+ & \texttt{F64} 554 & Telescope azimuth at exposure midpoint & degrees \\ 555 \hline SEEING & 1+ & \texttt{F32} & 556 Measured seeing at diff stage & arcsec \\ 557 \hline MAGZP & 1+ & \texttt{F32} & 558 Magnitude zero point & N/A \\ 559 \hline MAGZPERR & 1+ & \texttt{F32} & 560 Error in magnitude zero point & N/A \\ 561 \hline ASTRORMS & 1+ & \texttt{F32} & 562 RMS of astrometric fit & arcsec \\ 563 \hline CMMTOBS & 3+ & \texttt{string} & 564 Comment associated to the exposure & N/A\\ 565 \hline OBS\_MODE & 3+ & \texttt{enum} & Observation modes list: 566 3PI, CNP, ESS, M31, MD, MSS, OSS, PI, STD (Note: The exposures 567 having the following PS1 observation modes are not used by MOPS: 568 CAL, PR201108, SAS2, SS, STS, STS2A, STS2B) & N/A\\ 569 \hline DIFFTYPE & 3+ & \texttt{enum} & 570 Difference type: \texttt{WW} (Warp-Warp Difference), \texttt{WS} (Warp-Stack Difference) & N/A\\ 571 \hline SKY & 3+ & \texttt{F64} & 572 Exposure average sky background & counts/pixel \\ 573 \hline SHUTOUTC & 3+ & \texttt{string} & 574 Camera exposure shutter open (UTC) & N/A \\ 575 \hline \hline 576 \end{longtable} 577 \end{center} 578 579 \begin{center} 580 \begin{longtable}{|lclp{3.5in}c|} 581 \caption{IPP-MOPS Transient Detection Table Columns:\\ Detection Details}\label{table-detections}\\ 582 \hline \hline 583 \multicolumn{5}{|l|}{\null\hspace{10mm}\textbf{Detection Details}}\\ 584 \hline \hline 585 {\bf Column} & \textbf{Version} & {\bf Precision} & {\bf Description} & \textbf{Units}\\ 586 \hline 587 RA & 1+ & F64 & Detection center coordinates & degrees\\ 588 \hline 589 RA\_ERR & 1+ & F64 & Error in the detection center & degrees \\ 590 \hline 591 DEC & 1+ & F64 & Detection center coordinates & degrees \\ 592 \hline 593 DEC\_ERR & 1+ & F64 & Error in the detection center & degrees \\ 594 \hline 595 MAG & 1+ & F32 & Filter magnitude & N/A \\ 596 \hline 597 MAG\_ERR & 1+ & F32 & Filter magnitude error & N/A \\ 598 \hline 599 PSF\_CHI2 & 1+ & F32 & $\chi^2$ of PSF fit & N/A \\ 600 \hline 601 PSF\_DOF & 1+ & S32 & Degrees of freedom of PSF fit & N/A \\ 602 \hline 603 CR\_SIGNIFICANCE & 1+ & F32 & Significance of cosmic ray (source: \emph{src/psphot/psphotSourceSize.c}) & N/A \\ 604 \hline 605 EXT\_SIGNIFICANCE & 1+ & F32 & Significance of extendedness (source: \emph{src/psphot/psphotSourceSize.c}) & N/A \\ 606 \hline 607 PSF\_MAJOR & 1+ & F32 & PSF major axis & pixels \\ 608 \hline 609 PSF\_MINOR & 1+ & F32 & PSF minor axis & pixels \\ 610 \hline 611 PSF\_THETA & 1+ & F32 & PSF position angle on chip & degrees \\ 612 \hline 613 PSF\_QUALITY & 1+ & F32 & PSF quality factor & N/A \\ 614 \hline 615 PSF\_NPIX & 1+ & S32 & Number of pixels in PSF & N/A \\ 616 \hline 617 MOMENTS\_XX & 1+ & F32 & xx moment & N/A \\ 618 \hline 619 MOMENTS\_XY & 1+ & F32 & xy moment & N/A \\ 620 \hline 621 MOMENTS\_YY & 1+ & F32 & yy moment & N/A \\ 622 \hline 623 N\_POS & 1+ & S32 & Number of positive pixels & N/A \\ 624 \hline 625 F\_POS & 1+ & F32 & Fraction of positive pixels & N/A \\ 626 \hline 627 RATIO\_BAD & 1+ & F32 & Ratio of positive pixels to negative & N/A \\ 628 \hline 629 RATIO\_MASK & 1+ & F32 & Ratio of positive pixels to masked & N/A \\ 630 \hline 631 RATIO\_ALL & 1+ & F32 & Ratio of positive pixels to all & N/A \\ 632 \hline 633 FLAGS & 1+ & U32 & Detection bit flags\footnote{See \htmladdnormallink{http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/PSPSFlags\#StackDetectionFull.infoFlagsFLAGS232FLAGS}{http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/PSPSFlags\#StackDetectionFull.infoFlagsFLAGS232FLAGS} for the meaning of each bit}. The PM\_SOURCE\_MODE\_EXTENDED\_FIT flag (at position 0x00800000) is set when the Trail Fitting is attempted. It does not mean that the Trail Fitting is successful. \\ 634 \hline DIFF\_SKYFILE\_ID & 1+ & S64 & Identifier for diff 635 skyfile. Either a diff\_id (for Warp-Warp difference) or a 636 stack\_id 637 (for Warp-Stack difference) & N/A \\ 638 \hline 639 IPP\_IDET & 2+ & U32 & IPP detection identifier index & N/A \\ 640 \hline 641 PSF\_INST\_FLUX & 2+ & F32 & PSF fit instrumental magnitude & N/A \\ 642 \hline 643 PSF\_INST\_FLUX\_SIG & 2+ & F32 & Sigma of PSF instrumental magnitude & N/A \\ 644 \hline 645 AP\_MAG & 2+ & F32 & magnitude in standard aperture (i.e. 25 pixels radius) & N/A \\ 646 \hline 647 AP\_MAG\_RAW & 2+ & F32 & magnitude in real aperture & N/A \\ 648 \hline 649 AP\_MAG\_RADIUS & 2+ & F32 & radius used for aperture mags & pixels \\ 650 \hline 651 AP\_FLUX & 2+ & F32 & instrumental flux in standard aperture & ADU \\ 652 \hline 653 AP\_FLUX\_SIG & 2+ & F32 & aperture flux error & N/A \\ 654 \hline 655 PEAK\_FLUX\_AS\_MAG & 2+ & F32 & Peak flux expressed as magnitude & N/A \\ 656 \hline 657 CAL\_PSF\_MAG & 2+ & F32 & PSF Magnitude using supplied calibration & N/A \\ 658 \hline 659 CAL\_PSF\_MAG\_SIG & 2+ & F32 & Measured standard-deviation of zero point calibration & N/A \\ 660 \hline 661 SKY & 2+ & F32 & Sky level & counts/pixel \\ 662 \hline 663 SKY\_SIGMA & 2+ & F32 & Sigma of sky level & counts/pixel\\ 664 \hline PSF\_QF\_PERFECT & 2+ & F32 & PSF coverage/quality factor 665 (poor): PSF value weighted by unmasked pixels 666 (source: psmodules/src/objects/pmSourcePhotometry.c) & N/A \\ 667 \hline 668 MOMENTS\_R1 & 2+ & F32 & first radial moment & N/A \\ 669 \hline 670 MOMENTS\_RH & 2+ & F32 & half radial moment & N/A \\ 671 \hline 672 KRON\_FLUX & 2+ & F32 & Kron Flux (that is, flux in 2.5 $\times$ first radial moment) & N/A \\ 673 \hline 674 KRON\_FLUX\_ERR & 2+ & F32 & Kron Flux Error & N/A \\ 675 \hline 676 KRON\_FLUX\_INNER & 2+ & F32 & Inner Kron Flux (that is, flux in 1.0 $\times$ first radial moment) & N/A \\ 677 \hline 678 KRON\_FLUX\_OUTER & 2+ & F32 & Outer Kron Flux (that is, flux in 4.0 $\times$ first radial moment) & N/A \\ 679 \hline 680 DIFF\_R\_P & 2+ & F32 & distance from detection to positive matching source & pixels \\ 681 \hline 682 DIFF\_SN\_P & 2+ & F32 & signal-to-noise of pos match src & N/A \\ 683 \hline 684 DIFF\_R\_M & 2+ & F32 & distance from detectionto negative match source & pixels \\ 685 \hline 686 DIFF\_SN\_M & 2+ & F32 & signal-to-noise of neg match src & N/A \\ 586 687 \hline 587 688 FLAGS2 & 2+ & U32 & psphot analysis flags (group 2)\footnote{See \htmladdnormallink{http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/PSPSFlags\#StackDetectionFull.infoFlagsFLAGS232FLAGS}{http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/PSPSFlags\#StackDetectionFull.infoFlagsFLAGS232FLAGS} for the meaning of each bit}\\ 588 689 \hline 589 N\_FRAMES & 2+ & U16 & Number of frames overlapping source center \\690 N\_FRAMES & 2+ & U16 & Number of exposures overlapping source center \\ 590 691 \hline 591 692 PADDING & 2+ & S16 & padding \\ 592 \hline 593 \multicolumn{4}{|c|}{\textbf{Extended (trail fitting) parameters}}\\ 594 \multicolumn{4}{|c|}{Values like \texttt{NaN} mean that the extended parameters are undefined for the detection}\\ 595 \hline 596 X\_EXT & 2+ & F32 & Extended model X coordinate \\ 597 \hline 598 Y\_EXT & 2+ & F32 & Extended model Y coordinate \\ 599 \hline 600 X\_EXT\_SIG & 2+ & F32 & Sigma in extended model X coordinate \\ 601 \hline 602 Y\_EXT\_SIG & 2+ & F32 & Sigma in extended model Y coordinate \\ 603 \hline 604 EXT\_INST\_MAG & 2+ & F32 & Extended fit instrumental magnitude \\ 605 \hline 606 EXT\_INST\_SIG\_MAG & 2+ & F32 & Sigma of extended fit instrumental magnitude \\ 607 \hline 608 NPARAMS & 2+ & F32 & Number of model parameters \\ 609 \hline 610 EXT\_WIDTH\_MAJ & 2+ & F32 & EXT width (major axis), length for trail \\ 611 \hline 612 EXT\_WIDTH\_MIN & 2+ & F32 & EXT width (minor axis), sigma for trail \\ 613 \hline 614 EXT\_THETA & 2+ & F32 & EXT orientation angle\\ 615 \hline 616 EXT\_WIDTH\_MAJ\_ERR & 2+ & F32 & EXT width error (major axis)\\ 617 \hline 618 EXT\_WIDTH\_MIN\_ERR & 2+ & F32 & EXT width error (minor axis)\\ 619 \hline 620 EXT\_THETA\_ERR & 2+ & F32 & EXT orientation angle (error)\\ 621 \hline 622 RA\_EXT & 3+ & F32 & Fitted centroid RA \\ 623 \hline 624 RA\_EXT\_SIGMA & 3+ & F32 & Fitted RA sigma \\ 625 \hline 626 DEC\_EXT & 3+ & F32 & Fitted centroid DEC \\ 627 \hline 628 DEC\_EXT\_SIGMA & 3+ & F32 & Fitted DEC sigma \\ 629 \hline 630 POSANG\_EXT & 3+ & F32 & Fitted position angle \\ 631 \hline 632 PLTSCALE\_EXT & 3+ & F32 & Plate scale at centroid \\ 633 \hline 634 EXT\_FLUX & 3+ & F32 & Fitted flux \\ 635 \hline 636 EXT\_CAL\_MAG & 3+ & F32 & Calibrated magnitude \\ 637 \hline 638 EXT\_MAG\_SIG & 3+ & F32 & Sigma of calibrated magnitude \\ 639 \hline 640 EXT\_CHISQ & 3+ & F32 & $\chi^2$ of fit \\ 641 \hline 642 EXT\_NDOF & 3+ & S32 & Fit degrees of freedom \\ 643 \hline 693 \hline \hline 644 694 \end{longtable} 645 } 695 \end{center} 696 697 \begin{center} 698 \begin{longtable}{|lclp{3.5in}c|} 699 \caption{IPP-MOPS Transient Detection Table Columns:\\ Extended (Trail Fitting) Details}\label{table-detections-ext}\\ 700 \hline \hline 701 \multicolumn{5}{|c|}{\textbf{Extended (trail fitting) parameters}}\\ 702 \multicolumn{5}{|c|}{Values like \texttt{NaN} mean that the extended parameters are undefined for the detection}\\ 703 \hline 704 X\_EXT & 2+ & F32 & 705 Extended model X coordinate & pixels\\ 706 \hline 707 Y\_EXT & 2+ & F32 & 708 Extended model Y coordinate & pixels \\ 709 \hline 710 X\_EXT\_SIG & 2+ & F32 & 711 Sigma in extended model X coordinate & pixels \\ 712 \hline 713 Y\_EXT\_SIG & 2+ & F32 & 714 Sigma in extended model Y coordinate & pixels \\ 715 \hline 716 EXT\_INST\_MAG & 2+ & F32 & 717 Extended fit instrumental magnitude & N/A \\ 718 \hline 719 EXT\_INST\_SIG\_MAG & 2+ & F32 & 720 Sigma of extended fit instrumental magnitude & N/A \\ 721 \hline 722 NPARAMS & 2+ & S32 & 723 Number of model parameters (TODO: Reference to PV paper for details) & N/A \\ 724 \hline 725 EXT\_WIDTH\_MAJ & 2+ & F32 & % The name is weird but it's because of normalization 726 Length of trail & pixels \\ % in the IPP: Check if MOPS want to change it 727 \hline 728 EXT\_WIDTH\_MIN & 2+ & F32 & % The name is weird but it's because of normalization 729 Sigma of trail & pixels \\ % in the IPP: Check if MOPS want to change it 730 \hline 731 EXT\_THETA & 2+ & F32 & EXT orientation angle & radians \\ 732 \hline 733 EXT\_WIDTH\_MAJ\_ERR & 2+ & F32 & EXT width error (major axis) & pixels \\ 734 \hline 735 EXT\_WIDTH\_MIN\_ERR & 2+ & F32 & EXT width error (minor axis) & pixels \\ 736 \hline 737 EXT\_THETA\_ERR & 2+ & F32 & EXT orientation angle (error) & radians \\ 738 \hline 739 RA\_EXT & 3+ & F32 & Fitted centroid RA & degrees \\ 740 \hline 741 RA\_EXT\_SIGMA & 3+ & F32 & Fitted RA sigma & degrees? \\ 742 \hline 743 DEC\_EXT & 3+ & F32 & Fitted centroid DEC & degrees \\ 744 \hline 745 DEC\_EXT\_SIGMA & 3+ & F32 & Fitted DEC sigma & degrees? \\ 746 \hline 747 POSANG\_EXT & 3+ & F32 & Fitted position angle & degrees \\ 748 \hline 749 PLTSCALE\_EXT & 3+ & F32 & Plate scale at centroid & arcsec/pixel \\ 750 \hline 751 EXT\_FLUX & 3+ & F32 & Fitted flux & ADU \\ 752 \hline 753 EXT\_CAL\_MAG & 3+ & F32 & Calibrated magnitude & N/A \\ 754 \hline 755 EXT\_MAG\_SIG & 3+ & F32 & Sigma of calibrated magnitude & N/A \\ 756 \hline 757 EXT\_CHISQ & 3+ & F32 & $\chi^2$ of fit & N/A \\ 758 \hline 759 EXT\_NDOF & 3+ & S32 & Fit degrees of freedom & N/A \\ 760 \hline 761 \end{longtable} 762 \end{center} 646 763 647 764 \subsection{MOPS Detectability Query} … … 764 881 765 882 \pagebreak 883 884 \section{Changes} 885 886 \subsection{Changes in PS1\_DV3 from PS1\_DV2} 887 888 \subsubsection{New Keywords} 889 890 \paragraph{Per Exposure (in FITS header)} 891 \begin{itemize} 892 \item CMMTOBS 893 \item OBS\_MODE 894 \item DIFFTYPE 895 \item SKY 896 \item SHUTOUTC 897 \end{itemize} 898 899 \paragraph{Per Detection (in FITS extension)} 900 \begin{itemize} 901 \item RA\_EXT 902 \item RA\_EXT\_SIGMA 903 \item DEC\_EXT 904 \item DEC\_EXT\_SIGMA 905 \item POSANG\_EXT 906 \item PLTSCALE\_EXT 907 \item EXT\_FLUX 908 \item EXT\_CAL\_MAG 909 \item EXT\_MAG\_SIG 910 \item EXT\_CHISQ 911 \item EXT\_NDOF 912 \end{itemize} 913 914 \subsubsection{Removed Keywords} 915 916 None 917 918 \subsubsection{Datatypes} 919 \begin{itemize} 920 \item NPARAMS is now a S32 and no more a F32. 921 \end{itemize} 922 923 \subsubsection{Known Bugs and Associated Fix} 924 925 \begin{itemize} 926 \item None 927 \end{itemize} 928 929 \newpage 930 766 931 \appendix 767 932 768 \section{Appendix} 933 \section{The IPP Data Workflow} 934 935 The objective of this section is to provide some details about the IPP 936 Workflow. It is intentionnally MOPS oriented in the sense that some 937 details have been voluntarily omitted. 938 939 \begin{minipage}{0.65\linewidth} 940 The IPP receives "exposures" from the telescope. An "exposure" is an 941 image of 60 OTAs (see figure~\ref{fig-exposure-otas}) taken by the 942 GPC1 camera and its associated metadata. All science exposures 943 (which are interesting MOPS) are processed in the IPP according to 944 the following stages. 945 946 The first stage is the CHIP stage. Detrending and objects detections 947 are performed on each OTA at this stage. 948 949 The second stage is the CAMERA stage. Calibration and astrometry are 950 performed on the exposure at this stage. 951 952 The third stage is the WARP stage\footnote{For simplicity and since 953 nothing is performed in this stage, the FAKE stage has been 954 ommitted.}. The image pixels are warped to fit a predefined sky 955 tessellation (it is actually a covering). Cells of the tessellation 956 are called \emph{skycells} and each pixel in a skycell has a size of 957 $0.25" \times 0.25"$. The skycell is oriented so that increasing X 958 (wrt Y) pixel coordinate corresponds to a move toward the West (wrt 959 North). 960 961 The fourth stage is the DIFF stage. The difference between two 962 skycells having the same spatial coordinates but being distant in 963 time (by less than the TTI) is computed. To avoid deconvolution, 964 the image difference can be performed in bothways When the newer 965 image is diffed with the older image, the difference image is called 966 the \emph{positive} image. When the older image is diffed with the 967 newer image, the difference image is called the \emph{negative} 968 image. 969 970 Another stage is executed in parallel of the fourth stage: the STACK 971 stage. Its products (the stacks, that is, "average" observations in 972 a skycell) can be used in the DIFF stage to compute WARP-STACK 973 differences (e.g for MD observations). STACK-WARP are not computed 974 (so far). 975 976 The fifth and last stage is the PPMOPS stage. The exposure is 977 rebuilt from the differences obtained in each skycell of the DIFF 978 stage. For detections falling in areas covered by two or more 979 skycells, the data of the detection being the nearest to a skycell 980 center are taken. 981 \end{minipage}\hfill\begin{minipage}{0.3\linewidth} 982 \begin{center} 983 \includegraphics[width=\linewidth]{figures/ipp_workflow.eps} 984 \captionof{figure}{Caption for figure} 985 \label{fig-ipp-workflow} 986 \end{center} 987 \end{minipage} 988 989 \begin{center} 990 \includegraphics[width=4in]{figures/exposure_ota.eps} 991 \captionof{figure}{Exposure / OTA TODO + Move somewhere else} 992 \label{fig-exposure-otas} 993 \end{center} 994 995 \newpage 996 \section{Obsolete Stuff?} 997 998 TODO (SC): The following stuff seems obsolete. Tell me if I can remove it. 769 999 770 1000 \subsection{IPP to MOPS} … … 797 1027 \hline 798 1028 Detectability Query & \code{MOPS_DETECTABILITY_QUERY} & table of detectability query tuples (RA, Dec, FPA) \\ 799 \end{tabular}800 \end{center}801 \end{table}802 803 \subsection{Acronyms}804 805 \begin{table}[htbp]806 \begin{center}807 \small808 \caption{Acronyms used in this document\label{table-acronyms}}809 \begin{tabular}{ll}810 \hline811 \hline812 {\bf Acronym} & {\bf Definition} \\813 \hline814 MOPS & Pan-STARRS Moving Object Processing System \\815 IPP & Pan-STARRS Image Processing Pipeline \\816 FPA & Focal plane array \\817 MPC & Center for Astrophysics Minor Planet Center \\818 \hline819 1029 \end{tabular} 820 1030 \end{center} … … 841 1051 \end{itemize} 842 1052 843 \subsection{Example}844 \label{sec-example}845 846 \begin{verbatim}847 XTENSION= 'BINTABLE' / binary table extension848 BITPIX = 8 / 8-bit bytes849 NAXIS = 2 / 2-dimensional binary table850 NAXIS1 = 120 / width of table in bytes851 NAXIS2 = 42032 / number of rows in table852 PCOUNT = 0 / size of special data area853 GCOUNT = 1 / one data group (required keyword)854 TFIELDS = 25 / number of fields in each row855 TTYPE1 = 'RA ' / label for field 1856 TFORM1 = '1D ' / data format of field: 8-byte DOUBLE857 TTYPE2 = 'RA_ERR ' / label for field 2858 TFORM2 = '1D ' / data format of field: 8-byte DOUBLE859 TTYPE3 = 'DEC ' / label for field 3860 TFORM3 = '1D ' / data format of field: 8-byte DOUBLE861 TTYPE4 = 'DEC_ERR ' / label for field 4862 TFORM4 = '1D ' / data format of field: 8-byte DOUBLE863 TTYPE5 = 'MAG ' / label for field 5864 TFORM5 = '1E ' / data format of field: 4-byte REAL865 TTYPE6 = 'MAG_ERR ' / label for field 6866 TFORM6 = '1E ' / data format of field: 4-byte REAL867 TTYPE7 = 'PSF_CHI2' / label for field 7868 TFORM7 = '1E ' / data format of field: 4-byte REAL869 TTYPE8 = 'PSF_DOF ' / label for field 8870 TFORM8 = '1J ' / data format of field: 4-byte INTEGER871 TTYPE9 = 'CR_SIGNIFICANCE' / label for field 9872 TFORM9 = '1E ' / data format of field: 4-byte REAL873 TTYPE10 = 'EXT_SIGNIFICANCE' / label for field 10874 TFORM10 = '1E ' / data format of field: 4-byte REAL875 TTYPE11 = 'PSF_MAJOR' / label for field 11876 TFORM11 = '1E ' / data format of field: 4-byte REAL877 TTYPE12 = 'PSF_MINOR' / label for field 12878 TFORM12 = '1E ' / data format of field: 4-byte REAL879 TTYPE13 = 'PSF_THETA' / label for field 13880 TFORM13 = '1E ' / data format of field: 4-byte REAL881 TTYPE14 = 'PSF_QUALITY' / label for field 14882 TFORM14 = '1E ' / data format of field: 4-byte REAL883 TTYPE15 = 'PSF_NPIX' / label for field 15884 TFORM15 = '1J ' / data format of field: 4-byte INTEGER885 TTYPE16 = 'MOMENTS_XX' / label for field 16886 TFORM16 = '1E ' / data format of field: 4-byte REAL887 TTYPE17 = 'MOMENTS_XY' / label for field 17888 TFORM17 = '1E ' / data format of field: 4-byte REAL889 TTYPE18 = 'MOMENTS_YY' / label for field 18890 TFORM18 = '1E ' / data format of field: 4-byte REAL891 TTYPE19 = 'N_POS ' / label for field 19892 TFORM19 = '1J ' / data format of field: 4-byte INTEGER893 TTYPE20 = 'F_POS ' / label for field 20894 TFORM20 = '1E ' / data format of field: 4-byte REAL895 TTYPE21 = 'RATIO_BAD' / label for field 21896 TFORM21 = '1E ' / data format of field: 4-byte REAL897 TTYPE22 = 'RATIO_MASK' / label for field 22898 TFORM22 = '1E ' / data format of field: 4-byte REAL899 TTYPE23 = 'RATIO_ALL' / label for field 23900 TFORM23 = '1E ' / data format of field: 4-byte REAL901 TTYPE24 = 'FLAGS ' / label for field 24902 TFORM24 = '1J ' / data format of field: 4-byte INTEGER903 TZERO24 = 2147483648 / offset for unsigned integers904 TSCAL24 = 1 / data are not scaled905 TTYPE25 = 'DIFF_SKYFILE_ID' / label for field 25906 TFORM25 = '1K ' / data format of field: 8-byte INTEGER907 SWSOURCE= '60eb6cdc-a59c-4636-a4e0-dba66a9721fd' / Software source908 SWVERSN = 'branches/pap_mops/ppMops@25227' / Software version909 HISTORY ppMops at 2009-09-02T03:48:46.695783910 HISTORY psLib version: branches/pap_mops/psLib@25227911 HISTORY psLib source: 60eb6cdc-a59c-4636-a4e0-dba66a9721fd912 HISTORY ppMops version: branches/pap_mops/ppMops@25227913 HISTORY ppMops source: 60eb6cdc-a59c-4636-a4e0-dba66a9721fd914 EXP_NAME= 'o4995g0129o' / Exposure name915 EXP_ID = 77164 / Exposure identifier916 CHIP_ID = 24019 / Chip stage identifier917 CAM_ID = 17726 / Cam stage identifier918 FAKE_ID = 10227 / Fake stage identifier919 WARP_ID = 8842 / Warp stage identifier920 DIFF_ID = 19219 / Diff stage identifier921 DIFF_POS= F / Positive subtraction?922 MJD-OBS = 54995.4740598313 / MJD of exposure midpoint923 RA = '18:25:01.988' / Right Ascension of boresight924 DEC = '-17:20:40.069' / Declination of boresight925 TEL_ALT = 51.951873 / Telescope altitude926 TEL_AZ = 179.483883 / Telescope azimuth927 EXPTIME = 38. / Exposure time (sec)928 ROTANGLE= 333.1039 / Rotator position angle929 FILTER = 'r.00000 ' / Filter name930 AIRMASS = 1.269 / Airmass of exposure931 OBSCODE = 'F51 ' / IAU Observatory code932 SEEING = 1.678401 / Mean seeing933 MAGZP = 28.65226 / Magnitude zero point934 MAGZPERR= 0.353063 / Error in magnitude zero point935 ASTRORMS= 0.3111496 / RMS of astrometric fit936 EXTNAME = 'MOPS_TRANSIENT_DETECTIONS'937 \end{verbatim}938 939 940 1053 \end{document} 941 1054
Note:
See TracChangeset
for help on using the changeset viewer.
