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 | AM HERCULES | 274.126 | 49.8084 | 273.81383 | 49.78911 | 279.176537 | 73.11739 | 77.81082077 | 25.81903319 | 234.8814 | 54768.8590162037 | 2008-10-29 20:36:59 | 54771.3043287037 | 2008-11-01 07:18:14 | 403007010 | 108.4965 | 100 | 108.5045 | 108.5045 | 0 | 108.4965 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 94.4671 | 94.4671 | 211.2577 | 3 | PROCESSED | 57544.3392476852 | 2016-06-05 08:08:31 | 55156 | 2009-11-21 00:00:00 | 54788.4722222222 | 2008-11-18 11:20:00 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030021 | We propose the observation of the proto-type magnetic catacrysmic variables, AM Hercules, to search for possible hard X-ray tail on the thermal emission with Suzaku. To reduce the systematics of the estimation of the GSO background in the analyses, we propose the additional observation of blank sky near the object. | GALACTIC POINT SOURCES | 4 | C | YUKIKATSU TERADA | JAP | 3 | AO3 | NON THERMAL EMISSION FROM THE POLAR AM HERCULES | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403007010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403007010'
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