Data Wrangling with Pandas III#

We will begin soon! Until then, feel free to use the chat to socialize, and enjoy the music!

Image by Hands off my tags! Michael Gaida from Pixabay.

Outline#

In this Class we will talk about:

Mid-Course Feedback
Useful packages: random and numpy
Aggregation and Grouping in Pandas
Additional Notes

Mid-Course Feedback#

Here is the mid-course feedback survey that I am hoping you can fill out during class.

Useful packages: Numpy and Random#

Generating Random numbers using the random package
Using numpy

import random
import numpy as np

# Generate a random integer (!) between a and b (here a=0, b=50)

random.randint(a=0, b=50)

# Generate a random number (int) (!) between a and b (here a=0, b=50) in steps. For e.g., an "even number"

random.randrange(0, 50, step=2) + 1

# Generate a random number (!) between a and b (here a=0, b=50) in "step". Can use tricks to divide.

random.randrange(0, 100, step=1) / 10

6.7

# for loop to generate 10 random numbers

for i in range(10):
    print(random.randrange(5, 50))

# for loop to generate 10 random numbers
# and store into a list

rints = []
for i in range(10):
    rints.append(random.randrange(5, 50))

rints

[26, 49, 48, 49, 27, 14, 15, 24, 27, 9]

# list comprehension to generate 10 random numbers

[random.randrange(5, 50) for i in range(10)]

[35, 28, 41, 18, 35, 12, 27, 41, 11, 29]

# list comprehension to generate 10 random numbers
# and store into a list

rints2 = [random.randrange(5, 50) for i in range(10)]
rints2

[8, 24, 5, 15, 6, 7, 21, 35, 23, 49]

np.arange(5, 50)

array([ 5,  6,  7,  8,  9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21,
       22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34, 35, 36, 37, 38,
       39, 40, 41, 42, 43, 44, 45, 46, 47, 48, 49])

rints3 = np.arange(5, 50)

random.choice(rints3)

# another way
for i in range(10):
    print(random.choice(rints3))

Seeds#

What if you want the same random number every time? (Trust me, it’s useful!)

You can set the seed.

# Setting a seed to a specific number
random.seed(3.1415)

random.randint(0, 500)

Numpy#

# Generate 10 random floats (!) between 0 and 1
# Yes, numpy also has a random number generator

np.random.rand(10)

array([0.57235174, 0.61121143, 0.11754961, 0.09369188, 0.57572205,
       0.57786272, 0.1121864 , 0.51405043, 0.5149087 , 0.08766438])

# store that into a variable

r = np.random.rand(10)

# Check the type:

type(r)

numpy.ndarray

What is a numpy array?#

Let’s find out!

Click here

# but numpy is a lot more useful, it is the primary tool used for scientific computing!

Aggregation and Grouping#

Attribution#

This notebook contains an excerpt from the Python Data Science Handbook by Jake VanderPlas; the content is available on GitHub.

The text is released under the CC-BY-NC-ND license, and code is released under the MIT license. If you find this content useful, please consider supporting the work by buying the book!

An essential piece of analysis of large data is efficient summarization: computing aggregations like sum(), mean(), median(), min(), and max(), in which a single number gives insight into the nature of a potentially large dataset. In this section, we’ll explore aggregations in Pandas, from simple operations akin to what we’ve seen on NumPy arrays, to more sophisticated operations based on the concept of a groupby.

For convenience, we’ll use the same display magic function that we’ve seen in previous sections:

import numpy as np
import pandas as pd


class display(object):
    """Display HTML representation of multiple objects"""

    template = """<div style="float: left; padding: 10px;">
    <p style='font-family:"Courier New", Courier, monospace'>{0}</p>{1}
    </div>"""

    def __init__(self, *args):
        self.args = args

    def _repr_html_(self):
        return "\n".join(
            self.template.format(a, eval(a)._repr_html_()) for a in self.args
        )

    def __repr__(self):
        return "\n\n".join(a + "\n" + repr(eval(a)) for a in self.args)

Simple Aggregation in Pandas#

import pandas as pd

df = pd.DataFrame({"A": np.random.rand(5), "B": np.random.rand(5)})
df

	A	B
0	0.086238	0.197296
1	0.604400	0.307045
2	0.197429	0.402477
3	0.908598	0.611019
4	0.224398	0.773432

np.mean([0.734562, 0.723762, 0.075712, 0.683636, 0.878895])

0.6193134

np.mean(df["A"].tolist())

0.4042124137337176

df.mean(axis="rows")

A    0.404212
B    0.458254
dtype: float64

By specifying the axis argument, you can instead aggregate within each row:

df.mean(axis="columns")

  0.141767
  0.455722
  0.299953
  0.759808
  0.498915
dtype: float64

Planets Data#

Here we will use the Planets dataset, available via the Seaborn package (see Visualization With Seaborn). It gives information on planets that astronomers have discovered around other stars (known as extrasolar planets or exoplanets for short). It can be downloaded with a simple Seaborn command:

import seaborn as sns  # `conda install -c conda-forge seaborn` in your terminal

planets = sns.load_dataset("planets")
planets

	method	number	orbital_period	mass	distance	year
0	Radial Velocity	1	269.300000	7.10	77.40	2006
1	Radial Velocity	1	874.774000	2.21	56.95	2008
2	Radial Velocity	1	763.000000	2.60	19.84	2011
3	Radial Velocity	1	326.030000	19.40	110.62	2007
4	Radial Velocity	1	516.220000	10.50	119.47	2009
...	...	...	...	...	...	...
1030	Transit	1	3.941507	NaN	172.00	2006
1031	Transit	1	2.615864	NaN	148.00	2007
1032	Transit	1	3.191524	NaN	174.00	2007
1033	Transit	1	4.125083	NaN	293.00	2008
1034	Transit	1	4.187757	NaN	260.00	2008

1035 rows × 6 columns

planets.head()

	method	number	orbital_period	mass	distance	year
0	Radial Velocity	1	269.300	7.10	77.40	2006
1	Radial Velocity	1	874.774	2.21	56.95	2008
2	Radial Velocity	1	763.000	2.60	19.84	2011
3	Radial Velocity	1	326.030	19.40	110.62	2007
4	Radial Velocity	1	516.220	10.50	119.47	2009

This has some details on the 1,000+ extrasolar planets discovered up to 2014.

Pandas Series and DataFrames include all of the common aggregates mentioned in Aggregations: Min, Max, and Everything In Between; in addition, there is a convenience method describe() that computes several common aggregates for each column and returns the result. Let’s use this on the Planets data, for now dropping rows with missing values:

planets.dropna()

	method	number	orbital_period	mass	distance	year
0	Radial Velocity	1	269.30000	7.100	77.40	2006
1	Radial Velocity	1	874.77400	2.210	56.95	2008
2	Radial Velocity	1	763.00000	2.600	19.84	2011
3	Radial Velocity	1	326.03000	19.400	110.62	2007
4	Radial Velocity	1	516.22000	10.500	119.47	2009
...	...	...	...	...	...	...
640	Radial Velocity	1	111.70000	2.100	14.90	2009
641	Radial Velocity	1	5.05050	1.068	44.46	2013
642	Radial Velocity	1	311.28800	1.940	17.24	1999
649	Transit	1	2.70339	1.470	178.00	2013
784	Radial Velocity	3	580.00000	0.947	135.00	2012

498 rows × 6 columns

planets.dropna().describe()

	number	orbital_period	mass	distance	year
count	498.00000	498.000000	498.000000	498.000000	498.000000
mean	1.73494	835.778671	2.509320	52.068213	2007.377510
std	1.17572	1469.128259	3.636274	46.596041	4.167284
min	1.00000	1.328300	0.003600	1.350000	1989.000000
25%	1.00000	38.272250	0.212500	24.497500	2005.000000
50%	1.00000	357.000000	1.245000	39.940000	2009.000000
75%	2.00000	999.600000	2.867500	59.332500	2011.000000
max	6.00000	17337.500000	25.000000	354.000000	2014.000000

This can be a useful way to begin understanding the overall properties of a dataset. For example, we see in the year column that although exoplanets were discovered as far back as 1989, half of all known expolanets were not discovered until 2009 or after. This is largely thanks to the Kepler mission, which is a space-based telescope specifically designed for finding eclipsing planets around other stars.

The following table summarizes some other built-in Pandas aggregations:

Aggregation	Description
`count()`	Total number of items
`first()`, `last()`	First and last item
`mean()`, `median()`	Mean and median
`min()`, `max()`	Minimum and maximum
`std()`, `var()`	Standard deviation and variance
`mad()`	Mean absolute deviation
`prod()`	Product of all items
`sum()`	Sum of all items

These are all methods of DataFrame and Series objects.

To go deeper into the data, however, simple aggregates are often not enough. The next level of data summarization is the groupby operation, which allows you to quickly and efficiently compute aggregates on subsets of data.

GroupBy: Split, Apply, Combine#

Simple aggregations can give you a flavor of your dataset, but often we would prefer to aggregate conditionally on some label or index: this is implemented in the so-called groupby operation. The name “group by” comes from a command in the SQL database language, but it is perhaps more illuminative to think of it in the terms first coined by Hadley Wickham of Rstats fame: split, apply, combine.

Split, apply, combine#

A canonical example of this split-apply-combine operation, where the “apply” is a summation aggregation, is illustrated in this figure:

figure source in Appendix

This makes clear what the groupby accomplishes:

The split step involves breaking up and grouping a DataFrame depending on the value of the specified key.
The apply step involves computing some function, usually an aggregate, transformation, or filtering, within the individual groups.
The combine step merges the results of these operations into an output array.

While this could certainly be done manually using some combination of the masking, aggregation, and merging commands covered earlier, an important realization is that the intermediate splits do not need to be explicitly instantiated. Rather, the GroupBy can (often) do this in a single pass over the data, updating the sum, mean, count, min, or other aggregate for each group along the way. The power of the GroupBy is that it abstracts away these steps: the user need not think about how the computation is done under the hood, but rather thinks about the operation as a whole.

As a concrete example, let’s take a look at using Pandas for the computation shown in this diagram. We’ll start by creating the input DataFrame:

df = pd.DataFrame(
    {"key": ["A", "B", "C", "A", "B", "C"], "data": range(6)}, columns=["key", "data"]
)
df

	key	data
0	A	0
1	B	1
2	C	2
3	A	3
4	B	4
5	C	5

The most basic split-apply-combine operation can be computed with the groupby() method of DataFrames, passing the name of the desired key column:

df.groupby("key")

<pandas.core.groupby.generic.DataFrameGroupBy object at 0x7f905a1aa4d0>

Notice that what is returned is not a set of DataFrames, but a DataFrameGroupBy object. This object is where the magic is: you can think of it as a special view of the DataFrame, which is poised to dig into the groups but does no actual computation until the aggregation is applied. This “lazy evaluation” approach means that common aggregates can be implemented very efficiently in a way that is almost transparent to the user.

To produce a result, we can apply an aggregate to this DataFrameGroupBy object, which will perform the appropriate apply/combine steps to produce the desired result:

df.groupby("key").sum().reset_index()

	key	data
0	A	3
1	B	5
2	C	7

The sum() method is just one possibility here; you can apply virtually any common Pandas or NumPy aggregation function, as well as virtually any valid DataFrame operation, as we will see in the following discussion.

The GroupBy object#

The GroupBy object is a very flexible abstraction. In many ways, you can simply treat it as if it’s a collection of DataFrames, and it does the difficult things under the hood. Let’s see some examples using the Planets data.

Perhaps the most important operations made available by a GroupBy are aggregate, filter, transform, and apply. We’ll discuss each of these more fully in “Aggregate, Filter, Transform, Apply”, but before that let’s introduce some of the other functionality that can be used with the basic GroupBy operation.

Column indexing#

The GroupBy object supports column indexing in the same way as the DataFrame, and returns a modified GroupBy object. For example:

planets

	method	number	orbital_period	mass	distance	year
0	Radial Velocity	1	269.300000	7.10	77.40	2006
1	Radial Velocity	1	874.774000	2.21	56.95	2008
2	Radial Velocity	1	763.000000	2.60	19.84	2011
3	Radial Velocity	1	326.030000	19.40	110.62	2007
4	Radial Velocity	1	516.220000	10.50	119.47	2009
...	...	...	...	...	...	...
1030	Transit	1	3.941507	NaN	172.00	2006
1031	Transit	1	2.615864	NaN	148.00	2007
1032	Transit	1	3.191524	NaN	174.00	2007
1033	Transit	1	4.125083	NaN	293.00	2008
1034	Transit	1	4.187757	NaN	260.00	2008

1035 rows × 6 columns

planets.groupby("method")

<pandas.core.groupby.generic.DataFrameGroupBy object at 0x7f901ccf0220>

planets.groupby("method")["orbital_period"]

<pandas.core.groupby.generic.SeriesGroupBy object at 0x7f901ccf0ac0>

Here we’ve selected a particular Series group from the original DataFrame group by reference to its column name. As with the GroupBy object, no computation is done until we call some aggregate on the object:

planets.groupby("method")["orbital_period"].median()

method
Astrometry                         631.180000
Eclipse Timing Variations         4343.500000
Imaging                          27500.000000
Microlensing                      3300.000000
Orbital Brightness Modulation        0.342887
Pulsar Timing                       66.541900
Pulsation Timing Variations       1170.000000
Radial Velocity                    360.200000
Transit                              5.714932
Transit Timing Variations           57.011000
Name: orbital_period, dtype: float64

This gives an idea of the general scale of orbital periods (in days) that each method is sensitive to.

Iteration over groups#

The GroupBy object supports direct iteration over the groups, returning each group as a Series or DataFrame:

for (method, group) in planets.groupby("method"):
    print(f"{method:30s} shape={group.shape}")

Astrometry                     shape=(2, 6)
Eclipse Timing Variations      shape=(9, 6)
Imaging                        shape=(38, 6)
Microlensing                   shape=(23, 6)
Orbital Brightness Modulation  shape=(3, 6)
Pulsar Timing                  shape=(5, 6)
Pulsation Timing Variations    shape=(1, 6)
Radial Velocity                shape=(553, 6)
Transit                        shape=(397, 6)
Transit Timing Variations      shape=(4, 6)

This can be useful for doing certain things manually, though it is often much faster to use the built-in apply functionality, which we will discuss momentarily.

Dispatch methods#

Through some Python class magic, any method not explicitly implemented by the GroupBy object will be passed through and called on the groups, whether they are DataFrame or Series objects. For example, you can use the describe() method of DataFrames to perform a set of aggregations that describe each group in the data:

planets.groupby("method")["year"].describe().unstack()

       method                       
count  Astrometry                          2.0
       Eclipse Timing Variations           9.0
       Imaging                            38.0
       Microlensing                       23.0
       Orbital Brightness Modulation       3.0
                                         ...  
max    Pulsar Timing                    2011.0
       Pulsation Timing Variations      2007.0
       Radial Velocity                  2014.0
       Transit                          2014.0
       Transit Timing Variations        2014.0
Length: 80, dtype: float64

Looking at this table helps us to better understand the data: for example, the vast majority of planets have been discovered by the Radial Velocity and Transit methods, though the latter only became common (due to new, more accurate telescopes) in the last decade. The newest methods seem to be Transit Timing Variation and Orbital Brightness Modulation, which were not used to discover a new planet until 2011.

This is just one example of the utility of dispatch methods. Notice that they are applied to each individual group, and the results are then combined within GroupBy and returned. Again, any valid DataFrame/Series method can be used on the corresponding GroupBy object, which allows for some very flexible and powerful operations!

Aggregate, filter, transform, apply#

The preceding discussion focused on aggregation for the combine operation, but there are more options available. In particular, GroupBy objects have aggregate(), filter(), transform(), and apply() methods that efficiently implement a variety of useful operations before combining the grouped data.

For the purpose of the following subsections, we’ll use this DataFrame:

rng = np.random.RandomState(0)
df = pd.DataFrame(
    {
        "key": ["A", "B", "C", "A", "B", "C"],
        "data1": range(6),
        "data2": rng.randint(0, 10, 6),
    },
    columns=["key", "data1", "data2"],
)
df

	key	data1	data2
0	A	0	5
1	B	1	0
2	C	2	3
3	A	3	3
4	B	4	7
5	C	5	9

Aggregation#

We’re now familiar with GroupBy aggregations with sum(), median(), and the like, but the aggregate() method allows for even more flexibility. It can take a string, a function, or a list thereof, and compute all the aggregates at once. Here is a quick example combining all these:

df.groupby("key").aggregate(["min", np.median, max])

	data1			data2
	min	median	max	min	median	max
key
A	0	1.5	3	3	4.0	5
B	1	2.5	4	0	3.5	7
C	2	3.5	5	3	6.0	9

Another useful pattern is to pass a dictionary mapping column names to operations to be applied on that column:

df.groupby("key").aggregate({"data1": "min", "data2": "max"})

	data1	data2
key
A	0	5
B	1	7
C	2	9

Filtering#

A filtering operation allows you to drop data based on the group properties. For example, we might want to keep all groups in which the standard deviation is larger than some critical value:

def filter_func(x):
    return x["data2"].std() > 4


display("df", "df.groupby('key').std()", "df.groupby('key').filter(filter_func)")

	key	data1	data2
0	A	0	5
1	B	1	0
2	C	2	3
3	A	3	3
4	B	4	7
5	C	5	9

df.groupby('key').std()

	data1	data2
key
A	2.12132	1.414214
B	2.12132	4.949747
C	2.12132	4.242641

df.groupby('key').filter(filter_func)

	key	data1	data2
1	B	1	0
2	C	2	3
4	B	4	7
5	C	5	9

The filter function should return a Boolean value specifying whether the group passes the filtering. Here because group A does not have a standard deviation greater than 4, it is dropped from the result.

Transformation#

While aggregation must return a reduced version of the data, transformation can return some transformed version of the full data to recombine. For such a transformation, the output is the same shape as the input. A common example is to center the data by subtracting the group-wise mean:

df.groupby("key").transform(lambda x: x - x.mean())

	data1	data2
0	-1.5	1.0
1	-1.5	-3.5
2	-1.5	-3.0
3	1.5	-1.0
4	1.5	3.5
5	1.5	3.0

The apply() method#

The apply() method lets you apply an arbitrary function to the group results. The function should take a DataFrame, and return either a Pandas object (e.g., DataFrame, Series) or a scalar; the combine operation will be tailored to the type of output returned.

For example, here is an apply() that normalizes the first column by the sum of the second:

def norm_by_data2(x):
    # x is a DataFrame of group values
    x["data1"] /= x["data2"].sum()  # "y/= something" is equivalent to "y = y/something"
    return x


display("df", "df.groupby('key').apply(norm_by_data2)")

<string>:1: FutureWarning: Not prepending group keys to the result index of transform-like apply. In the future, the group keys will be included in the index, regardless of whether the applied function returns a like-indexed object.
To preserve the previous behavior, use

	>>> .groupby(..., group_keys=False)

To adopt the future behavior and silence this warning, use 

	>>> .groupby(..., group_keys=True)
<string>:1: FutureWarning: Not prepending group keys to the result index of transform-like apply. In the future, the group keys will be included in the index, regardless of whether the applied function returns a like-indexed object.
To preserve the previous behavior, use

	>>> .groupby(..., group_keys=False)

To adopt the future behavior and silence this warning, use 

	>>> .groupby(..., group_keys=True)

	key	data1	data2
0	A	0	5
1	B	1	0
2	C	2	3
3	A	3	3
4	B	4	7
5	C	5	9

df.groupby('key').apply(norm_by_data2)

	key	data1	data2
0	A	0.000000	5
1	B	0.142857	0
2	C	0.166667	3
3	A	0.375000	3
4	B	0.571429	7
5	C	0.416667	9

apply() within a GroupBy is quite flexible: the only criterion is that the function takes a DataFrame and returns a Pandas object or scalar; what you do in the middle is up to you!

There is LOTS more to explore!#

Below are some additional notes that show the (additional) power of combining many of the operations we’ve discussed up to this point when looking at realistic datasets. We can gain a thorough understanding of when and how planets have been discovered over the past several decades!

I would suggest digging into these few lines of code, and evaluating the individual steps to make sure you understand exactly what they are doing to the result. It’s certainly a somewhat complicated example, but understanding these pieces will give you the means to similarly explore your own data.

That’s it!

Have a good weekend!

Additional Notes#

Specifying the split key#

In the simple examples presented before, we split the DataFrame on a single column name. This is just one of many options by which the groups can be defined, and we’ll go through some other options for group specification here.

A list, array, series, or index providing the grouping keys#

The key can be any series or list with a length matching that of the DataFrame. For example:

L = [0, 1, 0, 1, 2, 0]
display("df", "df.groupby(L).sum()")

<string>:1: FutureWarning: The default value of numeric_only in DataFrameGroupBy.sum is deprecated. In a future version, numeric_only will default to False. Either specify numeric_only or select only columns which should be valid for the function.
<string>:1: FutureWarning: The default value of numeric_only in DataFrameGroupBy.sum is deprecated. In a future version, numeric_only will default to False. Either specify numeric_only or select only columns which should be valid for the function.

	key	data1	data2
0	A	0	5
1	B	1	0
2	C	2	3
3	A	3	3
4	B	4	7
5	C	5	9

df.groupby(L).sum()

	data1	data2
0	7	17
1	4	3
2	4	7

Of course, this means there’s another, more verbose way of accomplishing the df.groupby('key') from before:

display("df", "df.groupby(df['key']).sum()")

	key	data1	data2
0	A	0	5
1	B	1	0
2	C	2	3
3	A	3	3
4	B	4	7
5	C	5	9

df.groupby(df['key']).sum()

	data1	data2
key
A	3	8
B	5	7
C	7	12

A dictionary or series mapping index to group#

Another method is to provide a dictionary that maps index values to the group keys:

df2 = df.set_index("key")
mapping = {"A": "vowel", "B": "consonant", "C": "consonant"}
display("df2", "df2.groupby(mapping).sum()")

df2

	data1	data2
key
A	0	5
B	1	0
C	2	3
A	3	3
B	4	7
C	5	9

df2.groupby(mapping).sum()

	data1	data2
key
consonant	12	19
vowel	3	8

Any Python function#

Similar to mapping, you can pass any Python function that will input the index value and output the group:

display("df2", "df2.groupby(str.lower).mean()")

df2

	data1	data2
key
A	0	5
B	1	0
C	2	3
A	3	3
B	4	7
C	5	9

df2.groupby(str.lower).mean()

	data1	data2
key
a	1.5	4.0
b	2.5	3.5
c	3.5	6.0

A list of valid keys#

Further, any of the preceding key choices can be combined to group on a multi-index:

df2.groupby([str.lower, mapping]).mean()

		data1	data2
key	key
a	vowel	1.5	4.0
b	consonant	2.5	3.5
c	consonant	3.5	6.0

Grouping example#

As an example of this, in a couple lines of Python code we can put all these together and count discovered planets by method and by decade:

planets

	method	number	orbital_period	mass	distance	year
0	Radial Velocity	1	269.300000	7.10	77.40	2006
1	Radial Velocity	1	874.774000	2.21	56.95	2008
2	Radial Velocity	1	763.000000	2.60	19.84	2011
3	Radial Velocity	1	326.030000	19.40	110.62	2007
4	Radial Velocity	1	516.220000	10.50	119.47	2009
...	...	...	...	...	...	...
1030	Transit	1	3.941507	NaN	172.00	2006
1031	Transit	1	2.615864	NaN	148.00	2007
1032	Transit	1	3.191524	NaN	174.00	2007
1033	Transit	1	4.125083	NaN	293.00	2008
1034	Transit	1	4.187757	NaN	260.00	2008

1035 rows × 6 columns

decade = 10 * (planets["year"] // 10)
decade

     2000
     2000
     2010
     2000
     2000
        ... 
  2000
  2000
  2000
  2000
  2000
Name: year, Length: 1035, dtype: int64

decade = decade.astype(str) + "s"
decade

     2000s
     2000s
     2010s
     2000s
     2000s
        ...  
  2000s
  2000s
  2000s
  2000s
  2000s
Name: year, Length: 1035, dtype: object

decade.name = "decade"

planets.groupby(["method", decade])["number"].sum().unstack().fillna(0)

decade	1980s	1990s	2000s	2010s
method
Astrometry	0.0	0.0	0.0	2.0
Eclipse Timing Variations	0.0	0.0	5.0	10.0
Imaging	0.0	0.0	29.0	21.0
Microlensing	0.0	0.0	12.0	15.0
Orbital Brightness Modulation	0.0	0.0	0.0	5.0
Pulsar Timing	0.0	9.0	1.0	1.0
Pulsation Timing Variations	0.0	0.0	1.0	0.0
Radial Velocity	1.0	52.0	475.0	424.0
Transit	0.0	0.0	64.0	712.0
Transit Timing Variations	0.0	0.0	0.0	9.0

COSC 301

Data Wrangling with Pandas III

Contents

Data Wrangling with Pandas III#

Outline#

Mid-Course Feedback#

Useful packages: Numpy and Random#

Seeds#

Numpy#

What is a numpy array?#

Aggregation and Grouping#

Attribution#

Simple Aggregation in Pandas#

Planets Data#

GroupBy: Split, Apply, Combine#

Split, apply, combine#

The GroupBy object#

Column indexing#

Iteration over groups#

Dispatch methods#

Aggregate, filter, transform, apply#

Aggregation#

Filtering#

Transformation#

The apply() method#

There is LOTS more to explore!#

Additional Notes#

Specifying the split key#

A list, array, series, or index providing the grouping keys#

A dictionary or series mapping index to group#

Any Python function#

A list of valid keys#

Grouping example#