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 | ASO0304 | 213.3355 | -62.0808 | 212.410984 | -61.846899 | 236.335934 | -45.096122 | 312.3597658 | -0.71761471 | 280.2937 | 55036.9044907407 | 2009-07-24 21:42:28 | 55038.1453935185 | 2009-07-26 03:29:22 | 504054010 | 44.2485 | 40 | 44.2485 | 44.2485 | 0 | 44.2485 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 41.0839 | 41.0839 | 107.2018 | 1 | PROCESSED | 57547.9369791667 | 2016-06-08 22:29:15 | 55415 | 2010-08-07 00:00:00 | 55048.3203819444 | 2009-08-05 07:41:21 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040112 | We propose Suzaku observations of the fields of four Fermi-LAT sources on the Galactic plane. With the improved Fermi-LAT locations, we expect to identify the X-ray counterparts based on their morphologies and spectra, and categorize them into classes of known GeV gamma-ray sources (pulsars and AGNs) and VHE gamma-ray sources (SNRs, PWNe and colliding wind binaries), and possibly find a new class of objects. With these studies we hope to understand the population and emission mechanism of high energy sources in the Galaxy. | GALACTIC DIFFUSE EMISSION | 5 | A | NOBUYUKI KAWAI | JAP | 4 | AO4 | UNIDENTIFIED FERMI-LAT GAMMA-RAY SOURCES ON THE GALACTIC PLANE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504054010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '504054010'
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