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 | G22.0+0.0 | 277.823 | -9.7151 | 277.134886 | -9.751345 | 277.921132 | 13.510599 | 22.00005623 | 0.00370699 | 89.3658 | 55302.6023842593 | 2010-04-16 14:27:26 | 55303.7272222222 | 2010-04-17 17:27:12 | 505025010 | 50.5294 | 50 | 50.5294 | 50.5294 | 0 | 50.5294 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 44.6208 | 44.6208 | 97.1598 | 0 | PROCESSED | 57551.270775463 | 2016-06-12 06:29:55 | 55737 | 2011-06-25 00:00:00 | 55375.7533101852 | 2010-06-28 18:04:46 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050009 | ASCA galactic plane survey discovered many extended X-ray sources on the galactic plane. They have hard X-ray spectra with significant low energy absorption. However, due to poor photon statistics, we could not conclude whether they are thermal emission or non-thermal emission. We propose observations of the extended X-ray sources with Suzaku. Precise measurements of the X-ray structure and spectrum with the Suzaku XIS will reveal their nature. | GALACTIC DIFFUSE EMISSION | 5 | B | SHIGEO YAMAUCHI | JAP | 5 | AO5 | SUZAKU OBSERVATIONS OF EXTENDED SOURCES DISCOVERED WITH ASCA | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505025010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505025010'
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