@@ -82,9 +82,8 @@ calendar dates/times and Julian Dates, refer to UTC for ephemerides queries, TDB
8282for element queries and vector queries. By default, ``epochs=None ``, which uses
8383the current date and time.
8484
85- ``id_type `` controls how `Horizons resolves the ``id ``
86- <https://ssd.jpl.nasa.gov/horizons/manual.html#select>_` to match a Solar System
87- body:
85+ ``id_type `` controls how `Horizons resolves the 'id' <https://ssd.jpl.nasa.gov/horizons/manual.html#select >`_
86+ to match a Solar System body:
8887
8988+--------------------+------------------------------------------------------------------------------------------------------------------------------------------+
9089| ``id_type `` | Query behavior |
@@ -329,8 +328,8 @@ As we have seen before, we can display a truncated version of table
329328.. code-block :: python
330329
331330 >> > print (eph)
332- targetname datetime_str ... PABLon PABLat
333- -- - -- - ... deg deg
331+ targetname datetime_str ... PABLon PABLat
332+ -- - -- - ... deg deg
334333 -------------------------- ---------------- - ... -------- --------
335334 3552 Don Quixote (1983 SA ) 2010 - Jan- 01 00 :00 ... 8.0371 18.9349
336335 3552 Don Quixote (1983 SA ) 2011 - Jan- 01 00 :00 ... 85.4082 34.5611
@@ -354,6 +353,7 @@ Columns
354353-------
355354
356355We can get at list of all the columns in this table with:
356+
357357.. code-block :: python
358358
359359 >> > print (eph.columns)
@@ -362,12 +362,11 @@ We can get at list of all the columns in this table with:
362362 We can address each column individually by indexing it using its name as
363363provided in this list. For instance, we can get all RAs for Don Quixote by using
364364
365-
366365.. code-block :: python
367366
368367 >> > print (eph[' RA' ])
369- RA
370- deg
368+ RA
369+ deg
371370 -------- -
372371 345.50204
373372 78.77158
@@ -385,9 +384,10 @@ This column is formatted like the entire table; it has a column name and a unit.
385384We can select several columns at a time, for instance RA and DEC for each epoch
386385
387386.. code-block :: python
387+
388388 >> > print (eph[' datetime_str' , ' RA' , ' DEC' ])
389- datetime_str RA DEC
390- -- - deg deg
389+ datetime_str RA DEC
390+ -- - deg deg
391391 ---------------- - -------- - --------
392392 2010 - Jan- 01 00 :00 345.50204 13.43621
393393 2011 - Jan- 01 00 :00 78.77158 61.48831
@@ -409,7 +409,7 @@ in quadrature:
409409
410410 >> > import numpy as np
411411 >> > print (np.sqrt(eph[' RA_rate' ]** 2 + eph[' DEC_rate' ]** 2 ))
412- dRA* cosD
412+ dRA* cosD
413413 ------------------
414414 86.18728612153883
415415 26.337249029653798
@@ -437,7 +437,7 @@ h`` - arcseconds per hour:
437437.. code-block :: python
438438
439439 >> > print (eph[' RA_rate' ])
440- RA_rate
440+ RA_rate
441441 arcsec / h
442442 ----------
443443 72.35438
@@ -459,8 +459,8 @@ same dimensions. For instance, we can turn ``RA_rate`` into ``arcsec / s``:
459459
460460 >> > eph[' RA_rate' ].convert_unit_to(' arcsec/s' )
461461 >> > print (eph[' RA_rate' ])
462- RA_rate
463- arcsec / s
462+ RA_rate
463+ arcsec / s
464464 ----------------------
465465 0.02009843888888889
466466 - 0.0066177499999999995
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