Here some tests with SDS1104X-E
Of course all tests are with single individual scope and without any kind of hardware modifications. Hardware is just out from factory box. Only difference is explained in this thread Reply
#785
In all test image pairs both have exactly same signal source and signal pathway to scope input BNC. All scope settings equal (these settings which have some effect in this context)
I will reserve some next msg for further test results so that they stay together. This is because I show them delayed.

Picture 1.
This is made using
500MSa/s (250MHz f
Nyquist).
Input: Sweep from 5MHz to 250MHz, generator (HP8642B) output level 4dBm
Note 100MHz model BW shape near 250MHz, reason unknown...
ETA: For clarify this image. It seems that I have forget important information from image (it was all clear when there was just talking about mod, but if later some people look it out from original context it may look strange.
This Image 1. top half is SDS1204X-E (SDS1104X-E mod)
Bottom half is original SDS1104X-E "out from box".

Picture 1.1
"fold back" aliases due to input over 250MHz f
Nyquist but under 2f
NyquistThis is made using
500MSa/s (250MHz f
Nyquist).
Input: Sweep from
250MHz to 500MHz, generator (HP8642B) output level 4dBm
Note: FFT 0-250MHz show now input signal alias. Remember that now when sweep freguency goes up, signal in FFT display goes down. Example input 251MHz alias is 249MHz in FFT and 499MHz frequency input alias is now 1MHz in FFT. Middle point 125MHz is from 375MHz input. Just reverse (fold back from 250MHz f
Nyquist) Think you mirror horizontally this image 1.1 after picture 1. and both together is as sweep from 5MHz - 500MHz. (image 1 start from 5MHz due to reasons with HP8642B)
--Note1 for mod 200 with 1GSa/s this BW shape (think FFT horizontally mirrored and 250 - 500MHz. Of course just same as in FFT also normal scope time domain show this alias.
--Note2 for original 100MHz model with 1GSa/s, this is very different and it continue nearly same attenuation from 250 to 500MHz
--Note3 for both scope screen in image 1.1. Trigger event freq counter (right top corner) show Alias frequency. Of course because this scope have full digital side trigger system and of course it trig to alias - it can not know it is alias instead of direct true input signal. I have removed counter display because during sweep it is always late and it might cause confusion. 
Picture 1.2
Here is combination of some FFT - Sweeps using SDS1104X-E Original.
From previous images you can self look and think same kind of combine with SDS1104X-E (mod200)
Note specially original 100MHz BW shape when samplerate is 500MSa/s. It is near same as (mod200) exept this dip what have 250MHz center. But, 1GSa/s is very different (because.... and so on... all know that if example 100MHz signal in digital side is alias from 400MHz (if 500MSa/s) input or just original 100MHz input signal - digital side can not know it at all. This need also know when use scope what have example some strongly advertised user adjustable DSP filters what may in some cases produce total mess what nice looking product brochure do not tell you. Of course normal user know these potential traps due to education and experience and knows how to identify a potential problem situation and knows how to avoid problems)

Picture 1.3
This is SDS1104X-E mod200
This image can compare with picture 1.2 about SDS1104X-E original.
With 1GSa/s FFT is useable up to 500MHz but of course user need understand and know signal attenuation and front end limits.
Note that FFT noise floor is far down out from screen bottom. Because 5dB div scale and here interested signal top (BW shape)

Picture 1.4
SDS1104X-E mod200
Just example: 303.303 MHz signal, input level ~ -4dBm
As can see displayed noise floor top is under -80dBm (with this setting, including 50mV/div) and our 303MHz signal is around -10dBm (input level around -4dBm (attenuated roughly 6dB))
If look image 1.3 it can easy estimate what is situation if signal is example 490MHz with this same input level.
Yellow (persistence) is noise floor without trace averaging and white with average 16 traces.
Of course scope input have 50ohm termination and oscilloscope set for 50ohm external load. This Ext load value can set from 1ohm to 1Mohm.
Also compare to Reply #808 test image. Make your own conclusions or guesses. I can - but I do not want - speculate what is this or what it looks like at this point until more data.

Picture 2.
Oscilloscope set for
1GSa/s 1ns/div, Sin(x)/x (later Sinc) on. Display mode vectors and color grade on (reason was better visibility in some other tests for better visibility and then it was on also here without reason)
Signal source Tek 284 pulse generator.
(~70ns rise time in specifications but of course it is not true here with this kind of reactive load)
As can see in image with 1GSa/s these scopes works just as 100MHz and 200MHz scope work. No bad aliasing visible (if it exist it can see as corners wobbling with this kind of signals).
100MHz model no any visible aliasing but with 200MHz model there can see small amount corners wobbling (mode of aliasing). Note that input signal have l
ot of high frequency harmonics what goes really far over 500MHz f
Nyquist. Think user with probes. It is very hard to get these aliasing frequencies in to scope with normal probes when studying conventional circuits in practice. Of course if you make or own fast edge pulser you can... just remember, you can not use these scopes for analyze them and if pulse do not have enough wide real flat top you can not analyze scope with these.
But now, just keep it mind that this tests is with 1GSa/s what is available only if one or two channels are in use simultaneously. If three or four channels are in use, maximum is 500MSa/s per channel.
Just one thumb rule. When 500MSa/s in use do not input sinewaves what are more than just bit over 200MHz or pulse/square etc's where exist well under 2ns rise/fall times. Of course you can but then really need to know how to look for results so that aliasing do not fool you. Do not fall in to trap of alias.

Picture 3.
Oscilloscope set for
500MSa/s 1ns/div, Sinc on. Display mode vectors and color grade on.
Signal source Tek 284 pulse generator (as picture 2.).
As can see 500MSa/s is not enough specially for 200MHz BW with this kind of very fast rising signal when there is not brick wall type analog BW filter in front end before ADC what is only possible place. Digital side it can not do. Even if whoever is dreaming or believe fairy tales.
(later I will show how it looks like using different input signal risetimes what are more normal for use with this kind of oscilloscopes. ) With 200MHz model there can see lot of aliasing due to tiny attenuation over f
Nyquist. Input signal have
lot of high frequency harmonics what also have high level and what goes really far over 250MHz f
Nyquist.
100MHz model rejects these high frequency components more and so aliasing is not at all so heavy.
It is bit stupid to drive these scopes with this kind of signal except for show limits of this kind of scopes. It is good that user understand these things and know his equipment for avoid mistakes when he think what is this machine showing. These things are natural and normal, all match with practice and theory. These are not at all bugs. Only way to avoid these are higher samplerates and or more expensive analog side filters. Of course mostly in practice there come other things what rejects frequencies (rise times) before oscilloscope input BNC.
Remember, 500MSa/s is not good for 1.75ns rise time square/rectangle type input signals but still ok for 200MHz sine wave signals. Only exception is if oscilloscope have reallly "hard-core" bit over 200MHz brick wall filter. But then also you can not see 1.75nsa risetime on the screen what ever fast risetime flat top pulse you input. Fundamentals stay...
Of course it is nice if manufacturer implement more and better analog side filters and even better if user can select these. But there do not exist free lounges.
If you need analyze signals and measure real risetimes with good accuracy, remember "five times" rule.
If you need measure example 2ns risetime signals risetimes etc and you need measure quite accurately (~2%) these 2ns risetimes you need oscilloscope + probe what have 0.4ns or more fast risetime.