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
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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