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 | CYG_COCOON2 | 306.1992 | 40.9463 | 305.753337 | 40.782769 | 326.198572 | 57.540222 | 78.99355785 | 1.86268914 | 253.1744 | 56603.8842939815 | 2013-11-07 21:13:23 | 56605.000162037 | 2013-11-09 00:00:14 | 508020010 | 46.4489 | 50 | 46.4489 | 46.4489 | 0 | 46.4489 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 44.6569 | 44.6569 | 96.3739 | 3 | PROCESSED | 57613.2763194444 | 2016-08-13 06:37:54 | 57018 | 2014-12-27 00:00:00 | 56652.6462152778 | 2013-12-26 15:30:33 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 080048 | The long-standing question on the origin of Galactic cosmic-rays (GCRs) is still not settled, and star-forming regions are promising sites for the production of GCRs. We propose deep observations of nearby star-forming region Cygnus X, aiming at GeV gamma-ray excess revealed by Fermi. By utilizing high sensitivity of the Suzaku XIS, particularly for diffuse X-rays, we can identify particle species (electrons or protons) and evaluate the cosmic-ray energy density and spatial distribution in this important object. | GALACTIC DIFFUSE EMISSION | 5 | C | TSUNEFUMI MIZUNO | JAP | 8 | AO8 | SUZAKU INVESTIGATION OF PARTICLE ACCELERATION IN NEARBY STAR-FORMING REGION CYGNUS X | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/508020010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '508020010'
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