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
1 SN 1978K 49.5382 -66.5402 49.387343 -66.721221 341.369857 -74.185234 283.41338803 -44.62366671 13.2585 56804.2369097222 2014-05-27 05:41:09 56806.5279398148 2014-05-29 12:40:14 709023010 107.3136 100 107.3216 107.3216 0 107.3136 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57615.1724074074 2016-08-15 04:08:16 57234 2015-07-31 00:00:00 56866.7205092593 2014-07-28 17:17:32 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 094341 SN 1978K is a remarkable Type IIn supernova that remains bright at X-ray through radio wavelengths 35 years after its explosion. Our ongoing multiwavelength observations probe the dense medium that was ejected by the progenitor star, possibly a Luminous Blue Variable. While the radio flux dropped steadily, the X-ray and UV/optical fluxes remained surprisingly constant for a decade. However, our most recent XMM observation in 2013 June reveals a significant fading compared to the 2006 Oct Suzaku observation. Here we request a 100 ksec observation to study the spectral evolution during the decay. This will serve as a pathfinder for younger Type IIn supernovae. As secondary science, we will obtain data on the ULXs X-1 and X-2, and the other luminous sources in NGC 1313. EXTRAGALACTIC COMPACT SOURCES 7 B IAN SMITH SHOGO KOBAYASHI USJ 9 AO9 STUDYING THE LATE-TIME DECAY OF SN 1978K XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/709023010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '709023010'

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