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 | HESS J0632+057 | 98.2448 | 5.8057 | 97.576095 | 5.844008 | 98.600145 | -17.389477 | 205.66080027 | -1.43890266 | 289.9631 | 54941.5631944444 | 2009-04-20 13:31:00 | 54944.1542708333 | 2009-04-23 03:42:09 | 404027010 | 100.0343 | 100 | 100.0343 | 100.0343 | 0 | 100.0343 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 82.3918 | 82.3918 | 223.8419 | 6 | PROCESSED | 57546.2406481482 | 2016-06-07 05:46:32 | 55336 | 2010-05-20 00:00:00 | 54966.5323958333 | 2009-05-15 12:46:39 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040102 | We propose a coordinate observation of HESS J0632+057 with Suzaku and VLA. This source is recently discovered as a fourth gamma-ray binary with HESS and XMM-Newton, and our results obtained in Suzaku AO-3 also confirmed a gradual variety of X-ray intensity, possibly associated with the binary period. With a combined observation with VLA, we will for the first time obtain a "real-time" variety from both of image and spectrum of this interesting source. | GALACTIC POINT SOURCES | 4 | A | MOTOHIDE KOKUBUN | JAP | 4 | AO4 | SIMULTANEOUS OBSERVATION OF HESS J0632+057 WITH SUZAKU AND VLA | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404027010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404027010'
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