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.
observation_id
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
exposure
awarded_exposure
resolve_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner5_ra
corner5_dec
corner6_ra
corner6_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner5_ra_b1950
corner5_dec_b1950
corner6_ra_b1950
corner6_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner5_ecliptic_lon
corner5_ecliptic_lat
corner6_ecliptic_lon
corner6_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
corner5_galactic_lon
corner5_galactic_lat
corner6_galactic_lon
corner6_galactic_lat
resolve_adr_mode
resolve_thr_name
resolve_shp_date
1 201109010 WR140 305.11785 43.85413 304.69581 43.69484 327.37156 60.49126 80.93046 4.17613 189.85852 60687.62921 2025-01-12 15:06:04 60689.45560 2025-01-14 10:56:04 80.792 65.000 80.792 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 313430 11310 PROCESSED 2025-01-21 12:02:55 2026-01-22 00:00:00 2025-01-22 12:02:55 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000012182 Cosmic dust is a primary building block of the Earth, and its formation is a fundamental question. The massive colliding wind binary system, WR140, produces massive dust near periastron of its 7.9-year-long orbit. During the dust emission rise in previous binary cycles, the CIII line excess enhanced, and the X-ray emission declined oppositely, suggesting strong cooling of the WWC plasma produced a condition for dust formation. The star experiences another periastron passage on November 22nd, 2024. We propose 3 XRISM observations around that time to study the location and motion of the WWC plasma using the Fe XXV emission line. We also expect to detect the fluorescent Fe line, which strongly constrains the distance of the WWC apex from the stellar surface. STELLAR CORONAE, WINDS, AND YOUNG STARS 2 A KENJI HAMAGUCHI USA 1 NOR DYNAMICS OF THE EXPLOSIVE DUST FORMATION NEAR PERIASTRON IN WR140 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201109010/ Quick Look 305.14537 43.82589 305.15767 43.8766 305.09925 43.88385 305.09729 43.87547 305.08573 43.87697 305.07541 43.83474 304.72304 43.66648 304.7357 43.71714 304.67749 43.72463 304.67547 43.71625 304.66395 43.7178 304.65334 43.67561 327.38061 60.45702 327.44437 60.4978 327.37549 60.52381 327.36503 60.51704 327.35146 60.52224 327.29825 60.48829 80.9183 4.1438 80.96529 4.16509 80.94749 4.20396 80.93975 4.2004 80.93628 4.20813 80.8971 4.19048 HELIUM A75A 2021-12-13 00:00:00

Used SQL

SELECT * FROM xrism_resolve_data WHERE observation_id = '201109010'

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