DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | M101 | 210.8841 | 54.3679 | 210.442342 | 54.607302 | 174.405989 | 59.838606 | 101.97854462 | 59.72940376 | 150.2959 | 54062.5790625 | 2006-11-23 13:53:51 | 54064.7182175926 | 2006-11-25 17:14:14 | 801063010 | 98.8522 | 100 | 98.8762 | 98.8522 | 0 | 98.8762 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 89.6125 | 89.6125 | 184.802 | 2 | PROCESSED | 57536.2145486111 | 2016-05-28 05:08:57 | 54455 | 2007-12-21 00:00:00 | 54088.707650463 | 2006-12-19 16:59:01 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011402 | We wish to obtain a Suzaku spectrum of the diffuse X-ray emission in a typical galactic disk. The spectral resolution obtainable with Chandra/XMM does not allow the decomposition of the spectrum into more than two thermal components. The higher spectral resolution, better soft response, and lower instrumental background of Suzaku will allow the decomposition into at least three thermal components, and will place constraints on the number of thermal components and the distribution of temperatures and emission measures. The more refined fitting allowed by Suzaku spectra will allow a greater understanding of the sources of the X-ray emission. Given the Suzaku spatial resolution and detector size, M101 is the best observable example of a "typical" galactic disk. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | K. KUNTZ | USA | 1 | AO1 | SOFT DIFFUSE X-RAY EMISSION FROM M101 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801063010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801063010'
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